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Space Exploration

100 chapters on rockets, missions and the people who flew them

The book edition of The Visual Encyclopaedia of Space Exploration: how we leave the planet, from the first gunpowder rockets and the space race to Apollo, the planetary robots, the stations, the new commercial space age and the road to Mars, with real numbers and how we know. 100 chapters in 10 parts, a detailed plate for every chapter.

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Preface

How to read this one.

The book edition of The Visual Encyclopaedia of Space Exploration: how we leave the planet, from the first gunpowder rockets and the space race to Apollo, the planetary robots, the stations, the new commercial space age and the road to Mars, with real numbers and how we know. 100 chapters in 10 parts, a detailed plate for every chapter.

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Volume
Encyclopaedia No. 13
Chapters
100
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Complete

Contents

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100 chapters.

Encyclopaedia No. 13 · Ch 01 / 100

Fire Arrows and Gunpowder Rockets

Space Exploration — 100 chapters on rockets, missions and the people who flew them

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The first rocket was an arrow that did not need a bow. Chinese alchemists had written down a recipe for gunpowder by 1044, in the military manual Wujing Zongyao , and within two centuries someone had tied a bamboo tube of it to an arrow shaft and let the burning powder do the pushing. Chronicles of the Mongol siege of Kaifeng in 1232 describe fire lances and thunder-crash bombs; historians debate exactly when the fire arrow became a true rocket, propelled by its own exhaust rather than merely carrying flame, but by the fourteenth century Chinese, Arab and Indian armies were launching them in volleys from racks.

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The weapon came of age in southern India. The armies of Hyder Ali and his son Tipu Sultan, rulers of Mysore, fielded rockets with iron cases rather than paper or bamboo: a tube around 200 millimetres long and 40 to 50 millimetres across, strapped to a bamboo guide stick up to a metre long, with a range of a kilometre or two. Iron held higher pressure than cardboard, so the rockets flew further and hit harder. British accounts put Tipu's rocket corps at several thousand men, and at Pollilur in 1780 a volley reportedly set off an East India Company ammunition cart and helped rout the column. After Srirangapatna fell in 1799, captured Mysorean rockets were shipped to the Royal Arsenal at Woolwich.

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Congreve rockets entered British service in 1806. The 32-pounder version weighed about 14.5 kilograms and could reach roughly 2.7 kilometres, further than most field guns of the day, and the Royal Navy fired around 300 of them into Copenhagen during the bombardment of September 1807, when the city burned for three days. Seven years later, on the night of 13 to 14 September 1814, the rocket ship HMS Erebus fired Congreves at Fort McHenry in Baltimore harbour. Francis Scott Key watched from a truce ship and wrote of "the rockets' red glare"; the line became the American national anthem. The fort held, which tells you something: the rockets were terrifying and wildly inaccurate.

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That inaccuracy is why the gunpowder rocket stalled for a century. A stick-stabilised rocket wobbles, its powder burns unevenly, and a side wind sends it anywhere. William Hale's spin-stabilised design of 1844, which vented exhaust through angled holes to make the rocket rotate like a rifle bullet, helped, but by the 1860s rifled artillery was hitting targets at longer ranges with far greater precision, and rocket troops were quietly disbanded. The deeper limit was chemical: black powder gives a specific impulse of only around 80 seconds, a quarter of what a modern liquid engine delivers, so no gunpowder rocket could ever carry much, or go high.

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The gunpowder rocket proved the principle, then spent a hundred years as a signal flare and a line-thrower for lifeboats. It took a new fuel, and a few obsessive dreamers, to make it a vehicle.

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Imagining the Voyage

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Long before anyone could leave the planet, people were writing the trip reports. Lucian of Samosata, a Syrian-Greek satirist of the second century, sent a ship to the Moon on a whirlwind in his True History and found the King of the Moon at war with the King of the Sun over the colonisation of the Morning Star; he introduced it by promising that every word was a lie. Fourteen centuries later Johannes Kepler wrote the Somnium , a dream in which a demon carries a traveller to the Moon during an eclipse. Kepler, who had just worked out the laws of planetary motion, used it to describe how the heavens would look from the Moon, with the Earth hanging motionless in the sky and turning once a day. Published in 1634, four years after his death, it counts as the first science fiction built on real astronomy.

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The seventeenth century added the vehicles. Francis Godwin's The Man in the Moone (1638) used a flock of trained geese; Cyrano de Bergerac, in a satire published in 1657, tried bottles of dew warmed by the sun and then, almost in passing, a frame hung with firecrackers that lit in stages. It was a joke, and also literature's first rocket to space.

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Then came Jules Verne, who did his sums. In From the Earth to the Moon (1865) the Baltimore Gun Club casts a 274-metre cannon, the Columbiad , in the ground of central Florida and fires an aluminium projectile carrying three men towards the Moon. Verne chose Florida for its nearness to the equator; he computed an initial speed of around 11 kilometres per second, close to the true escape velocity; and in the sequel the capsule splashes down in the Pacific to be recovered by an American warship, the USS Susquehanna . A century later Apollo launched three men from Florida in an aluminium-alloy capsule at just under 11 kilometres per second and brought them home to a Pacific splashdown beside an aircraft carrier. Apollo 11's command module Columbia took its name partly from Verne's gun.

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H. G. Wells took the other route in The First Men in the Moon (1901), with a gravity-shielding substance called Cavorite and a Moon full of insect-like Selenites, and Georges Méliès turned the two books into A Trip to the Moon in 1902, fourteen minutes of painted sets ending with a capsule in the Man in the Moon's eye. Wells, not Verne, caught the next generation: Robert Goddard read The War of the Worlds as a teenager, and Hermann Oberth read Verne at eleven and spent his life checking the arithmetic.

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The pattern matters because it kept repeating. Konstantin Tsiolkovsky wrote space novels alongside his equations; Wernher von Braun wrote a Mars novel in 1949; Arthur C. Clarke proposed the communications satellite in a magazine in 1945. Fiction did not just predict spaceflight, it recruited the people who would build it.

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Tsiolkovsky and the Rocket Equation

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Konstantin Tsiolkovsky lost most of his hearing to scarlet fever at ten, was turned away from school, and taught himself physics in Moscow's libraries, eating black bread so that he could afford books. From 1892 he taught arithmetic and geometry in Kaluga, a provincial town 150 kilometres south-west of Moscow, and in a workshop at home he worked out, on paper, how to leave the Earth. His notebook dates the key result to 10 May 1897. In 1903 the journal Nauchnoye Obozreniye published his paper Exploration of Outer Space by Means of Reaction Devices , and almost nobody read it.

Paragraph 1 of 4 · Encyclopaedia No. 13 · Ch 03 / 100

What he had found is now called the rocket equation : the change in velocity a rocket can achieve equals its exhaust velocity multiplied by the natural logarithm of its starting mass divided by its final mass. Written out, Δv = ve ln(m0/m1). It follows directly from Newton's laws, and a British mathematician, William Moore, had derived a version of it in 1810 for Congreve rockets, but Tsiolkovsky was the first to point it at space and to see what it implied.

Paragraph 2 of 4 · Encyclopaedia No. 13 · Ch 03 / 100

The logarithm is the cruel part. Orbital speed is about 7.8 kilometres per second, and gravity and air drag during the climb add another 1.5 or so, so a rocket needs around 9.4 kilometres per second of Δv. A kerosene engine exhausts at roughly 3 kilometres per second. Divide, take the exponential, and the starting mass must be 23 times the final mass: 96 per cent of the vehicle on the pad has to be propellant, leaving 4 per cent for tanks, engines, structure and payload. No one can build a tank that light. Tsiolkovsky's answers, in 1903, were the two that still apply. Use the fastest exhaust you can, which is why he proposed burning liquid hydrogen with liquid oxygen, a pairing not flown until 1963. And throw away the empty tanks as you go. His 1929 paper on rocket trains described stages that burn in turn and fall away, so that each later stage starts the equation afresh with a…

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He also drew the pressurised cabin, the airlock, the spacesuit, the closed-loop greenhouse and the orbital station, and wrote science fiction, On the Moon in 1893 and Beyond the Planet Earth in 1920, to carry the ideas to readers who would never open a physics journal. In a letter of 1911 he wrote the line that every space agency has quoted since: the Earth is the cradle of humanity, but one cannot live in the cradle forever. He died in Kaluga in September 1935. Sputnik launched twenty-two years later, in the centenary year of his birth, on a staged rocket designed by engineers who had grown up on his pamphlets.

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The equation has not changed. Every launch vehicle flying today, from Soyuz to Starship, is an argument with that logarithm, and staging is the only answer anyone has found.

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Goddard's Liquid Fuel

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On 16 March 1926, in a snowy cabbage field on his aunt Effie's farm at Auburn, Massachusetts, Robert Goddard lit a rocket fuelled by petrol and liquid oxygen. It burned for 2.5 seconds, climbed 12.5 metres, and landed 56 metres away in the frozen field, at an average speed of about 96 kilometres per hour. Four people watched: Goddard, his wife Esther with a cine camera that ran out of film, his assistant Henry Sachs and a Clark University colleague, Percy Roope. It was the first flight of a liquid-propellant rocket , and it looked like nothing: a three-metre frame of thin pipes with a small engine at the top and the tanks below. Goddard thought an engine above the tanks would make it stable, like pulling a cart; it does not, as he soon found. The date, the figures and the photograph of Goddard beside the frame come from his own meticulous diary.

Paragraph 1 of 4 · Encyclopaedia No. 13 · Ch 04 / 100

Goddard, a physics professor at Clark University in Worcester, had been chasing this since a day in 1899 when, aged seventeen and sitting in a cherry tree, he imagined a device that could rise to Mars. He patented the liquid-fuelled and multi-stage rocket in 1914, and his 1919 Smithsonian paper, A Method of Reaching Extreme Altitudes , mentioned in a footnote that a rocket could carry flash powder to the Moon. The New York Times ran an editorial on 13 January 1920 jeering that he lacked "the knowledge ladled out daily in high schools", since everyone knew a rocket needed air to push against. Newton's third law says otherwise. The paper printed a correction on 17 July 1969, while Apollo 11 was on its way to the Moon.

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The ridicule, and a ban on further launches in Massachusetts, made him secretive. Charles Lindbergh took an interest, and from 1930 the Guggenheim family funded Goddard to move to Roswell, New Mexico, where in a decade of quiet work he solved most of the problems of the modern rocket: gyroscopic steering with movable vanes in the exhaust, turbopumps, regenerative cooling of the combustion chamber, gimballed thrust. In March 1935 one of his rockets passed the speed of sound, and in 1937 another reached around 2.7 kilometres. He filed or was granted 214 patents, many of them posthumously through Esther, and they cover almost every part of a V-2 or a Saturn V.

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Yet his influence on the people who built those machines was small, because he published so little. The German engineers at Peenemünde worked from Oberth's book and their own tests; when they later saw his patents, Wernher von Braun said Goddard had been ahead of them all. Goddard died in August 1945, three months after the last V-2 fell.

Paragraph 4 of 4 · Encyclopaedia No. 13 · Ch 04 / 100

NASA's Goddard Space Flight Center in Maryland carries his name. The cabbage field is now a golf course with a small stone marker, which is roughly the attention he received in his lifetime.

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Oberth and the Rocket Societies

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The rocket entered the 1920s as a book. Hermann Oberth, a Transylvanian Saxon who had read Verne at eleven, submitted a dissertation on rockets to Heidelberg in 1922 and had it rejected; he published it himself in 1923 as Die Rakete zu den Planetenräumen , The Rocket into Planetary Space , 92 dense pages proving that a liquid-fuelled rocket could leave the Earth, carry people and survive the trip. It sold out, and it did something the earlier pioneers had not managed: it created a readership, which within a decade had organised itself into clubs on three continents, and the clubs were firing rockets.

Paragraph 1 of 4 · Encyclopaedia No. 13 · Ch 05 / 100

The German Verein für Raumschiffahrt , the Society for Space Travel, was founded in Breslau in July 1927 and by 1930 had a home: the Raketenflugplatz, a disused ammunition dump in Berlin-Reinickendorf, leased by Rudolf Nebel. Klaus Riedel built the engines, Willy Ley wrote the publicity, and a nineteen-year-old engineering student named Wernher von Braun turned up to help. Their Mirak and Repulsor rockets, little more than a motor and a pair of tanks, reached a kilometre or so; by 1932 the society counted 87 flights and 270 static firings. Johannes Winkler, the VfR's first president, had flown Europe's first liquid-fuelled rocket, the HW-1, near Dessau on 14 March 1931. Then the German Army came calling, the club dissolved in 1934, and von Braun went to work for it.

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Oberth himself had spent 1929 as scientific adviser on Lang's Frau im Mond , which showed a two-stage rocket, acceleration couches and weightlessness aboard, and he promised the studio a real rocket for the premiere. He was injured in a test and the rocket never flew, but the film reached audiences the book could not. In New York, the science fiction editor David Lasser and the journalist G. Edward Pendray founded the American Interplanetary Society on 4 April 1930; their second rocket flew from Staten Island on 14 May 1933 to about 75 metres before its oxygen tank burst. In Moscow, the Group for the Study of Reactive Motion, GIRD, formed in 1931 around Friedrich Zander, Mikhail Tikhonravov and a 24-year-old aircraft designer, Sergei Korolev. Their GIRD-09, burning gelled petrol with liquid oxygen, rose about 400 metres over Nakhabino on 17 August 1933, the first Soviet liquid rocket;…

Paragraph 3 of 4 · Encyclopaedia No. 13 · Ch 05 / 100

The pattern repeats across the four cities: a book, a club, a field, a crude rocket, then the state. The amateurs proved liquid rockets were real and trained the people who would industrialise them. Oberth lived to ninety-five, long enough to watch Apollo 11 launch beside his former student von Braun.

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Every launch count since has begun with Fritz Lang's number ten.

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Encyclopaedia No. 13 · Ch 06 / 100

The V-2

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At 15:58 on 3 October 1942 an A-4 rocket rose from Test Stand VII at Peenemünde, on the Baltic island of Usedom, climbed to 84.5 kilometres and fell into the sea 190 kilometres away. Two earlier attempts that summer had failed; this one worked, and Walter Dornberger, the Army officer in charge, told his engineers that evening that they had opened the door to space travel. The machine he was describing is the one history calls the V-2 , for Vergeltungswaffe , the "vengeance weapon", a name the propaganda ministry attached in 1944.

Paragraph 1 of 4 · Encyclopaedia No. 13 · Ch 06 / 100

It was 14 metres tall, 1.65 metres across and weighed 12.5 tonnes fuelled, of which 8.8 tonnes were propellant: a 75 per cent ethanol-water mix and liquid oxygen, fed by a turbopump driven on steam from hydrogen peroxide. The engine produced about 25 tonnes of thrust, 245 kilonewtons, for roughly 65 seconds, by which time the missile was travelling at around 1,600 metres per second, four and a half times the speed of sound. Three gyroscopes sensed its attitude; graphite vanes in the exhaust and small rudders on the four fins steered it; an accelerometer or a radio beam cut the engine at the planned speed. The warhead carried 738 kilograms of amatol. On an operational shot the trajectory peaked near 88 kilometres and the whole flight to a target 320 kilometres away took about five minutes, arriving at supersonic speed with no warning. Every one of these figures is in the Peenemünde test…

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The programme's leaders were Dornberger and Wernher von Braun, technical director at thirty. After the RAF bombed Peenemünde in August 1943, production moved underground to the Mittelwerk , tunnels in the Kohnstein hill near Nordhausen, where prisoners of the Mittelbau-Dora concentration camp assembled the missiles in cold, dust and hunger. About 6,000 V-2s were built. Historians estimate that around 20,000 prisoners died at Dora and its sub-camps, more than the roughly 9,000 people the V-2 killed at its targets, and the figures are not disputed: more people died building the V-2 than were killed by it.

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The attacks began on 8 September 1944, on Paris in the morning and on Chiswick in west London at 18:43, where three people died in Staveley Road. Of around 3,170 rockets launched in anger, Antwerp received about 1,600 and London about 1,350, including a single hit on a Woolworths in New Cross that killed 168 shoppers. About a third of all launches failed. The last fell on 27 March 1945. As a weapon it was a strategic failure, costing Germany more than it cost the Allies; as a machine it was the ancestor of every ballistic missile and space launcher built in the next fifteen years, by both superpowers.

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The V-2 is where spaceflight's two stories meet, the engineering and the moral ledger, and neither can be told without the other.

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Paperclip and the Soviet Harvest

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The V-2 did not end in 1945; it was divided. In the final weeks of the war the American, British and Soviet armies raced for the Mittelwerk, its missiles and the people who understood them, and the shares each took set the pace of the next decade. On 2 May 1945 Wernher von Braun's younger brother Magnus cycled down a Bavarian road to find an American private and surrender the team; von Braun had already chosen his captor, moving some 500 engineers and 14 tonnes of documents south ahead of the Red Army. The US Army reached the Mittelwerk tunnels near Nordhausen on 11 April, and before handing the area to the Soviet zone on 1 June its Special Mission V-2 hauled out around 100 missiles' worth of parts in 341 railway wagons.

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Operation Paperclip , the programme that brought German scientists to the United States, took 118 members of the rocket team to Fort Bliss, Texas, in late 1945, von Braun among the first seven to arrive. At the White Sands Proving Ground in New Mexico they reassembled V-2s for American crews; the first launch, on 16 April 1946, failed, the second, on 10 May, reached 112 kilometres. On 24 October 1946 a V-2 carrying a 35-millimetre cine camera climbed to 105 kilometres and brought back the first photographs of Earth from space, grainy frames showing the curve of the planet. Sixty-seven V-2s flew from White Sands by 1952, carrying instruments and, twice, monkeys.

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Britain, with no budget for a missile programme, ran Operation Backfire instead: at Cuxhaven in October 1945, German crews under British supervision launched three V-2s into the North Sea so that the procedure could be filmed and documented. The Soviet Union, arriving at an emptied Mittelwerk, assembled what it could with the Germans who had stayed, including Helmut Gröttrup, head of the V-2's guidance group. On the night of 22 October 1946, in Operation Osoaviakhim, Soviet security troops roused around 2,200 German specialists and their families and put them on trains east. Gröttrup's group spent six years on an island in Lake Seliger, consulted but kept from the real work. Sergei Korolev's own team launched its first German-built V-2 from the new range at Kapustin Yar on 18 October 1947, flew the Soviet-built copy, the R-1 , on 10 October 1948, and stretched it into the R-2 with…

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The accounting is lopsided but not simple. The Americans got the leaders and the paperwork; the Soviets got the factory, the production engineers and a decade of hard practice, and were first to orbit anyway. Both nations' rockets of the 1950s, Redstone and R-5 alike, were V-2s that had grown up.

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Half a captured missile programme, it turned out, was enough to start a space race.

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How a Rocket Works

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A rocket is a machine for throwing mass out of the back as fast as possible. Newton's third law does the rest: every kilogram of hot gas flung backwards pushes the vehicle forwards with equal force, in air or in vacuum, and the vacuum is in fact better, since there is no atmosphere pressing on the nozzle exit. Thrust is the mass flow rate multiplied by the exhaust velocity. The Saturn V's first stage burned about 13 tonnes of propellant every second and threw it out at around 2.6 kilometres per second, roughly 34 meganewtons, enough to lift 2,900 tonnes at 1.2 times its weight.

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The second number that matters is specific impulse , the exhaust velocity divided by the strength of gravity, measured in seconds: how many seconds one kilogram of propellant can produce one kilogram of thrust. It is set by the chemistry. Solids, as in the Shuttle's boosters, give about 240 seconds and enormous thrust; kerosene and liquid oxygen, as in the F-1, about 300 in vacuum; hypergolic fuels that ignite on contact, used by Proton and most spacecraft thrusters, a little more; methane and oxygen in SpaceX's Raptor around 350; liquid hydrogen and oxygen in the Space Shuttle's RS-25 about 452, the best any chemical engine achieves, at the cost of a fuel so light that its tanks are vast.

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Getting the propellants into the chamber is the hard part. A chamber runs at 70 bar in the F-1 and over 250 bar in the Russian RD-180, so the turbopumps, turbines spun by hot gas, must push harder than that: the F-1's delivered 41 megawatts, as much as a large ship's engines. Where the hot gas comes from defines the engine cycle. A gas-generator engine, like the F-1 or the Merlin, burns a little propellant in a separate combustor and dumps the exhaust overboard, simple and slightly wasteful. A staged-combustion engine, like the RS-25 or the RD-180, sends that exhaust into the main chamber to be burned again, gaining efficiency and complexity. Raptor runs full-flow staged combustion, with every gram of propellant passing through a turbine first.

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The nozzle turns pressure into speed. Gas reaches Mach 1 at the narrow throat and keeps accelerating as the bell widens, leaving at Mach 3 or more; a vacuum engine has a bigger bell because there is no air to push the plume back in. All of this fights losses: low orbit needs 7.8 kilometres per second of speed but around 9.4 of total Δv, the difference eaten by gravity during the climb, air drag and steering, which is why rockets tilt over as early as they dare.

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The F-1 gave 6.77 meganewtons at sea level, the RD-180 3.83, the RS-25 1.86, a Raptor 3 about 2.75; today's heaviest rockets simply fit more of them. Each is a controlled explosion held steady for minutes, and that they work at all is the quiet miracle of the business.

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Encyclopaedia No. 13 · Ch 09 / 100

Getting into Orbit

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An orbit is a fall that keeps missing. Isaac Newton drew the picture in the 1680s: a cannon on a high mountain fires faster and faster, each ball landing further away, until one goes so fast that the ground curves away as quickly as it drops, and it comes round to hit the gunner from behind. Nothing is holding a satellite up. The International Space Station, 400 kilometres above the Earth, is falling the whole time; it simply moves sideways at 7.7 kilometres per second, and the planet curves out of its way. The weightlessness aboard is the weightlessness of a lift whose cable has snapped.

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Height is cheap and speed is dear. Reaching 100 kilometres, the Kármán line that the records body uses as the edge of space, takes about 1.4 kilometres per second straight up; orbit takes 7.8 sideways, and that speed is 95 per cent of the energy. That is why a rocket climbs only briefly before tilting over in a gravity turn , trading altitude for velocity as soon as the thick air is behind it.

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That rotational bonus explains the map. Kourou in French Guiana, Cape Canaveral at 28 degrees, Sriharikota at 13, Wenchang at 19: launch sites hug the equator and fire east over water. Russia's Baikonur, at 46 degrees in Kazakhstan, gets only 320 metres per second from the spin, and Plesetsk, at 63 degrees, about 210, and the ISS orbits at 51.6 degrees because that is the lowest inclination Baikonur can reach without dropping spent stages on China.

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The orbit chosen depends on the job. Low Earth orbit, below 2,000 kilometres, is for stations and most satellites; sun-synchronous orbit, a near-polar track at around 700 kilometres passing each place at the same local time, is for Earth observation; geostationary orbit, 35,786 kilometres up over the equator, is where a satellite's 24-hour period matches the Earth's spin and it hangs over one spot. The Soviet Molniya orbit, a 12-hour ellipse tilted at 63.4 degrees, lingers over the Arctic, which geostationary satellites cannot see. Reaching it is a two-step: the launcher puts the satellite into a long transfer ellipse and at its far end the satellite's own motor rounds it off, the Hohmann transfer Walter Hohmann worked out in 1925, costing about 2.4 kilometres per second more.

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What goes up comes down, slowly. Even at 400 kilometres there is enough air to drag the ISS down by about 2 kilometres a month, so it is reboosted a few times a year; Sputnik lasted 92 days, Skylab fell on Western Australia in 1979 and Mir was steered into the Pacific in 2001. Above about 1,000 kilometres a satellite will stay for centuries, which is the beginning of the space-junk problem. Orbit is not a place but a speed, and every launch is an argument about how to buy it cheaply.

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Encyclopaedia No. 13 · Ch 10 / 100

Korolev and von Braun

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The space race was run by two engineers who never met and could not have been introduced. One was a name the whole world knew: Wernher von Braun, baron, television presenter, father of the Saturn V. The other was a state secret. Until the day after he died in January 1966, Soviet newspapers called Sergei Korolev only the Chief Designer , and when the Nobel committee asked whom to honour for Sputnik, Nikita Khrushchev replied that the achievement belonged to the whole Soviet people.

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Korolev, born in Zhytomyr in 1907, was an aircraft designer who led GIRD's first liquid-rocket flight in 1933. In June 1938, during Stalin's purges, he was arrested on fabricated charges, beaten until his jaw broke, and sentenced to ten years. He spent the winter of 1939 to 1940 in the Maldyak gold mine in Kolyma, where scurvy took most of his teeth and nearly his life; his mother's letters and the aircraft designer Andrei Tupolev got him moved to a prison design bureau, a sharashka , where he worked under guard until 1944. Sent to Germany in 1945 to study the V-2, he built from the R-1 copy the R-5, the first Soviet nuclear missile, and then the R-7 , the 280-tonne, 32-engine rocket that flew on 21 August 1957, launched Sputnik six weeks later and Gagarin in 1961, and whose descendants still carry crews to the station. He ran the programme on charm, intimidation and a heart weakened…

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Von Braun, born in Wirsitz in 1912, joined the Nazi Party in 1937 and the SS in 1940, rising to major; the records show he visited the Mittelwerk and knew the prisoners' conditions. He said afterwards that he could have done nothing; historians judge that he chose not to try. A brief Gestapo arrest in 1944, for talking about spaceflight rather than weapons, and his surrender to the Americans let him be recast. In the United States he built the Redstone, the Jupiter and the Juno I that orbited Explorer 1 on 31 January 1958, after the Navy's Vanguard had exploded on television. He sold space to the public through Collier's and three Disney television films from 1955, the first of which, Man in Space , drew around 40 million viewers. From Huntsville, Alabama, he led the Saturn V and watched it fly thirteen times without failure.

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Each knew of the other and saw the race as a duel: Korolev's engineers studied the Saturn plans in the open American literature; von Braun lobbied Washington after Sputnik by pointing at a rival he could not name. Korolev's death left the Soviet Moon rocket in weaker hands; von Braun left NASA in 1972 when the Saturn line was cancelled, and died in 1977.

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The race was between two men as much as two systems, and the one who won it is still the harder to judge.

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Encyclopaedia No. 13 · Ch 11 / 100

Sputnik

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On the evening of 4 October 1957, from a launch pad at Tyuratam in the Kazakh steppe that the world would come to call Baikonur, a converted intercontinental missile lifted a polished aluminium sphere into orbit. Sputnik 1 weighed 83.6 kilograms, measured 58 centimetres across and trailed four whip antennas between 2.4 and 2.9 metres long. Inside were two radio transmitters and a battery pack that took up most of the mass. It circled the Earth every 96 minutes on an orbit that dipped to 215 kilometres and rose to 939, and it did almost nothing except beep.

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The beeps were the point. Transmitting on 20.005 and 40.002 megahertz, frequencies chosen so that any radio amateur could tune in, the satellite announced itself to anyone who cared to listen, and the pulses carried a crude message about pressure and temperature inside the sphere. Within a day the BBC and American stations were broadcasting the sound. Jodrell Bank in Cheshire tracked the object by radar, and observers with binoculars reported the satellite passing overhead at dawn and dusk. The batteries lasted three weeks; the transmitters fell silent on 26 October, and the sphere burned up on re-entry on 4 January 1958 after about 1,440 orbits.

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The satellite was a stand-in. Sergei Korolev's design bureau had been building a heavier scientific payload for the International Geophysical Year, the eighteen-month programme of coordinated research that began in July 1957, but it was running late, and Korolev, hearing that the Americans might fly first, ordered a prosteishiy sputnik , a "simplest satellite", built in a few months by Mikhail Tikhonravov's team. The real achievement was the R-7 Semyorka beneath it: a 280-tonne missile with four strap-on boosters and twenty main combustion chambers, designed to carry a hydrogen bomb across the Atlantic. A rocket that could put 84 kilograms in orbit could, Washington understood at once, put a warhead on any city on Earth.

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That is why a beeping ball became a crisis. American newspapers called it a technological Pearl Harbor; Eisenhower, who knew from U-2 reconnaissance that the Soviet missile force was still tiny, tried to calm things and was accused of complacency. Within a year Congress had created NASA, the Advanced Research Projects Agency and the National Defense Education Act, which poured money into science teaching. Nikita Khrushchev saw the reaction and demanded a second one for the fortieth anniversary of the Revolution. Sputnik 2 flew on 3 November 1957, weighing 508 kilograms and carrying the dog Laika, who died of overheating within hours, a fact the Soviet Union did not admit until 2002.

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The name of the chief designer stayed secret until his death in 1966, and the launch site stayed secret rather longer. The satellite itself was a sphere of almost nothing. What it carried into the sky was proof that the rocket worked, and from that night the race had a starting gun.

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Encyclopaedia No. 13 · Ch 12 / 100

Explorer 1 and the Van Allen Belts

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America's answer to Sputnik was broadcast live, and it rose about a metre. On 6 December 1957 the Navy's Vanguard TV-3 lost thrust two seconds after ignition, settled back onto its pad at Cape Canaveral and exploded; its grapefruit-sized satellite was thrown clear and lay beeping in the scrub. The newspapers called it Flopnik and Kaputnik. The humiliation unlocked a rocket the Army had been forbidden to use: Wernher von Braun's Jupiter-C, a Redstone missile with clustered solid upper stages, which his team at Huntsville had quietly kept ready since 1956.

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Renamed Juno I , it launched on the night of 31 January 1958, with the Jet Propulsion Laboratory in Pasadena supplying the upper stages and the satellite. Explorer 1 was a pencil of a spacecraft, 2.03 metres long and 14 kilograms including the spent fourth stage, on an orbit from 358 to 2,550 kilometres. Because the Cape could not track it directly, the team waited in Washington for the first pass over California; the signal came at 1.30 in the morning, eight minutes late, and William Pickering of JPL, James Van Allen of the University of Iowa and von Braun held a model over their heads for the photographers.

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Van Allen's instrument was a single Geiger counter. It behaved oddly: at low altitude it clicked away at the expected rate, and at high altitude it went silent. His student Carl McIlwain showed in the laboratory that the tube was not seeing nothing but far too much, saturated by radiation thousands of times above the predicted level. Explorer 3, launched on 26 March with a tape recorder to capture whole orbits, confirmed it, and on 1 May 1958 Van Allen announced that the Earth sits inside doughnut-shaped belts of charged particles held by its magnetic field. The Van Allen belts were the first discovery of the space age: an inner belt of protons from about 1,000 to 6,000 kilometres and a broader outer belt of electrons out to 60,000 kilometres, which every crewed mission since has crossed quickly or avoided.

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The political machinery moved as fast as the science. The Advanced Research Projects Agency was set up in February 1958 to stop the services fighting over rockets, and on 29 July Eisenhower signed the National Aeronautics and Space Act, turning the old aeronautics committee NACA into a civilian agency, NASA , which opened for business on 1 October with 8,000 staff. Reconnaissance, the thing the White House really wanted from space, went to a secret programme called Corona, which failed thirteen times before recovering its first film capsule from orbit in August 1960.

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Explorer 1 transmitted until 23 May 1958 and re-entered in 1970. In four months the United States had gone from a fireball on the pad to a discovery about the planet, and had built the institution that would carry the next twelve years.

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Encyclopaedia No. 13 · Ch 13 / 100

Luna: First to the Moon

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For a decade the Moon belonged to a series of Soviet robots. Luna 1 , launched on 2 January 1959, was meant to hit the surface and instead missed by about 6,000 kilometres, which made it the first object to escape the Earth's gravity; on the way it released a cloud of sodium vapour visible from the ground, and its ion traps made the first direct measurement of the solar wind. Luna 2 did not miss. On 13 September 1959 it struck the surface near the crater Autolycus at over 3 kilometres a second, the first human-made object on another world, carrying steel pennants stamped with the hammer and sickle. Two days later Khrushchev presented Eisenhower with a copy at the White House.

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Luna 3 was cleverer still. Launched on 4 October 1959, it looped behind the Moon and on 7 October photographed the far side, which no human had ever seen. The spacecraft developed the film on board, scanned it with a light beam and radioed the pictures to Earth as a television signal. The images were murky, but they showed a hemisphere with far fewer dark plains than the near side, and Soviet astronomers named what they saw, including the Sea of Moscow and the crater Tsiolkovsky.

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Landing took longer. Twelve attempts failed before Luna 9 touched down in the Ocean of Storms on 3 February 1966, a 99-kilogram egg-shaped capsule that was thrown clear at the last moment and bounced to rest, opened four petals and raised its antennas. Its panorama proved that the surface would bear weight, settling a real worry that a lander might sink into dust. The pictures were first published not in Moscow but in Manchester: Bernard Lovell's team at Jodrell Bank recorded the signal, recognised the format as that of a standard newspaper fax machine, borrowed one from the Daily Express and printed the Moon's surface before the Soviet press release. Luna 10 followed on 3 April 1966 as the first spacecraft to orbit another world.

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After Apollo 11, the programme turned to robotic sample return. Luna 16 landed in the Sea of Fertility on 20 September 1970, drilled 35 centimetres, sealed 101 grams of soil in a capsule and fired it home. Two months later Luna 17 delivered Lunokhod 1 , a 756-kilogram eight-wheeled rover steered from a control room near Simferopol with a five-second round-trip delay; it worked for eleven months and drove 10.5 kilometres. Lunokhod 2 covered 39 kilometres in 1973, and Luna 24 brought back the last Soviet sample in 1976, making 326 grams in all.

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Each first was announced with fanfare and each failure went unmentioned, so the programme looked unstoppable. In truth it was a chain of narrow wins, and the firsts it collected, flyby, impact, far side, soft landing, orbit, robotic return and rover, were exactly the steps a human landing would need.

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Encyclopaedia No. 13 · Ch 14 / 100

Yuri Gagarin

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At 09.07 Moscow time on 12 April 1961 a Vostok-K rocket, another descendant of the R-7, left the same Baikonur pad as Sputnik. In the spherical capsule on top sat a 27-year-old senior lieutenant of the Soviet air force, Yuri Alekseyevich Gagarin, call sign Kedr, "Cedar". As the engines lit he said "Poyekhali!", "Let's go!", a phrase that has done duty in Russian ever since. Vostok 1 completed one orbit of the Earth in 108 minutes and he was on the ground before most of the planet had finished breakfast.

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Gagarin was a passenger in a machine that flew itself. The 4.7-tonne spacecraft had two parts: a sphere 2.3 metres across holding the cosmonaut, and an instrument module with the retro-rocket. Soviet doctors did not know whether a human could think clearly in weightlessness, so the controls were locked and the key, a three-digit code, sealed in an envelope to be opened only in an emergency; several of his superiors told him the code anyway. The orbit came out higher than planned, 169 by 327 kilometres, because the upper stage shut down late, which would have left him stranded for over a week had the retro-rocket failed. It did not. Over Africa it fired for 42 seconds, but the instrument module failed to separate cleanly and the two parts tumbled together, joined by a cable bundle, until the heat of re-entry burned it through.

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Then came the part the Soviet Union did not mention for years. At 7 kilometres the hatch blew and Gagarin's seat fired him out of the capsule, and he came down under his own parachute near the village of Smelovka, close to Engels on the Volga, where a farmer's wife and her granddaughter asked whether he had come from space. The capsule landed separately. Because the rules of the Fédération Aéronautique Internationale required a pilot to land inside his craft for a record to count, the official account said he had, and the ejection was only admitted later.

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He had been born on 9 March 1934 in the village of Klushino, west of Moscow, the son of a carpenter, had lived under German occupation, trained as a foundry worker and learned to fly at the Saratov aero club. Promoted to major during the flight, he toured the world for two years, charmed the Queen and the crowds of Manchester, and was never allowed to fly in space again. He died on 27 March 1968 when the MiG-15 trainer he was flying with Vladimir Seryogin crashed near Kirzhach; the cause is still debated, with wake turbulence from another aircraft the leading explanation.

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Six Vostoks flew between 1961 and 1963. The first carried a man who did almost nothing on board, because nobody yet knew what a man could do; what he proved, in 108 minutes, was that a human being could go round the world and come back smiling.

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Encyclopaedia No. 13 · Ch 15 / 100

The Mercury Seven

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On 9 April 1959 NASA introduced seven men to the press in Washington and the reporters applauded, which had not been in the plan. The Mercury Seven , Scott Carpenter, Gordon Cooper, John Glenn, Gus Grissom, Wally Schirra, Alan Shepard and Deke Slayton, had been sifted from 508 military test pilots by rules of brutal simplicity: under 40, under 5 feet 11 inches so as to fit the capsule, a degree, 1,500 hours in jets, and a week of tests at the Lovelace Clinic in Albuquerque that included enemas and ice water in the ear. A contract with Life magazine for their family stories made them the most famous people in America before any had left the ground.

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The machine was a cone 1.9 metres across the base and 1.35 tonnes, built by McDonnell in St Louis, with the pilot lying on his back facing a periscope and, after the pilots insisted, a window. Two rockets lifted it: the Army's Redstone , with 350 kilonewtons of thrust, enough for a fifteen-minute lob into space and back, and the Air Force's Atlas , a thin-skinned missile that stood up only when pressurised and delivered the 1,600 kilonewtons needed for orbit. Before any pilot flew, chimpanzees did. Ham flew a suborbital hop on 31 January 1961 and pulled his levers for banana pellets throughout; Enos rode two orbits in November.

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Alan Shepard flew Freedom 7 on 5 May 1961, three weeks after Gagarin, 187 kilometres up and 487 kilometres downrange in 15 minutes and 22 seconds. Gus Grissom's Liberty Bell 7 in July ended with the hatch blowing early and the capsule sinking in 5,000 metres of Atlantic; it was raised in 1999. Then, on 20 February 1962, John Glenn rode the Atlas for three orbits in Friendship 7 . At first light he reported "fireflies" around the capsule, which turned out to be frost shaken loose from the hull, and a faulty sensor suggested his heat shield had come loose, so Mercury Control told him to keep the retro-rocket pack strapped over it; he watched chunks of it burn past the window on the way down.

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Carpenter overshot his landing by 400 kilometres in May 1962, Schirra flew a textbook six orbits in October, and Gordon Cooper closed the programme in May 1963 with 22 orbits and 34 hours in Faith 7 , flying the re-entry by hand after the electrics failed. Slayton, grounded by an irregular heartbeat, ran the astronaut office for a decade and finally flew in 1975. The worldwide tracking network built for Mercury, from Bermuda to Zanzibar and Western Australia, became the nervous system of every programme after it.

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Six flights, 53 hours in space, no one lost. Mercury did not catch the Russians, but it taught NASA how to put a person on top of a missile and get him back, and that lesson was the one everything else was built on.

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Encyclopaedia No. 13 · Ch 16 / 100

We Choose to Go to the Moon

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Six weeks after Gagarin's flight and five after the Bay of Pigs, John F. Kennedy stood before a joint session of Congress on 25 May 1961 and asked for something extravagant. "I believe that this nation should commit itself to achieving the goal, before this decade is out, of landing a man on the Moon and returning him safely to the Earth." The applause was polite. Alan Shepard had flown twenty days earlier; the United States had fifteen minutes of human spaceflight to its name, and the president had just promised a round trip of 770,000 kilometres by 1970.

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He had not chosen the Moon out of romance. On 20 April, the day after the Cuban landing collapsed, Kennedy sent Vice-President Lyndon Johnson a memo asking whether there was "a space programme which promises dramatic results in which we could win". Johnson, Wernher von Braun and the new NASA administrator James Webb answered that the Soviets would win any race to a space station or a lunar flyby, because their rockets were bigger, but that a landing needed a rocket neither side had, which made it a fair contest. The Moon was picked precisely because it was far enough away to reset the clock.

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The famous speech came later, at Rice University in Houston on 12 September 1962, in punishing Texas heat. "We choose to go to the Moon in this decade and do the other things, not because they are easy, but because they are hard." Houston had been chosen a year earlier for the new Manned Spacecraft Center , and the speech was partly a thank-you to a city filling up with engineers. What the public never heard was a recording made in the White House two months later, on 21 November 1962, in which Kennedy told Webb that beating the Russians to the Moon was the only point: "otherwise we shouldn't be spending this kind of money, because I'm not that interested in space."

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The money was the programme. NASA's budget rose from under half a per cent of federal spending in 1960 to a peak of 4.4 per cent in 1966, when the agency employed 36,000 people directly and about 400,000 more through contractors and universities: Saturn stages in Alabama and Louisiana, capsules in California, computers at MIT. Polls through the decade mostly found that a majority of Americans thought the Moon was not worth the cost. Kennedy himself wobbled; in September 1963 he proposed to the United Nations a joint expedition with the Soviet Union, and was shot two months later, which made the deadline a memorial nobody could cancel.

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The decision was political, the motive was Cold War prestige, and the deadline was arbitrary. It also worked, which is the part that has puzzled every administration since: a clear goal, a fixed date and four per cent of the budget turned out to be a formula that nothing has repeated.

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Encyclopaedia No. 13 · Ch 17 / 100

Valentina Tereshkova

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On 16 June 1963 a 26-year-old former textile worker from Yaroslavl became the first woman in space, and for the next nineteen years she was the only one. Valentina Tereshkova flew Vostok 6 for 48 orbits and 70 hours and 50 minutes, nearly three days, longer than all six Mercury astronauts put together. Her call sign was Chaika, "Seagull", and the flight was the second half of a double act: Valery Bykovsky had launched in Vostok 5 two days earlier and would stay up for five days, a record for a solo flight that still stands. The two capsules came within about five kilometres of each other.

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She had been chosen for the one thing the Vostok needed of its pilot, the ability to jump. Vostok cosmonauts ejected at 7 kilometres and landed by parachute, and Tereshkova, who had joined the Yaroslavl air sports club in 1959 while working at the Krasny Perekop cotton mill, was an accomplished amateur parachutist with well over a hundred jumps. Five women were selected in secret in February 1962, trained alongside the men and were commissioned as air force lieutenants. Korolev picked Tereshkova partly for her flying, partly for her biography: a worker, a Komsomol member, the daughter of a tractor driver killed in the Finnish war.

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The flight was uncomfortable and nearly dangerous. She was sick, found the food inedible and the suit chafing, and on the first day noticed that the automatic orientation system had been set to raise the orbit rather than lower it for re-entry, an error that Korolev's engineers confirmed and corrected by uplinking new settings. She kept the discovery quiet for thirty years at his request. On 19 June she ejected and landed near Baevo in the Altai, bruised her nose on her helmet and handed out her space food to the villagers who found her. Five months later she married the cosmonaut Andriyan Nikolayev; their daughter Elena, born in 1964, was the first child of two people who had both flown in space.

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America had women who could have flown and chose not to. In 1960 and 1961 the physician William Randolph Lovelace, who had tested the Mercury Seven, put 19 experienced female pilots through the same examinations, and 13 passed, among them Jerrie Cobb, who had 10,000 hours in the air. The Navy cancelled the next phase of testing, and in July 1962 a congressional subcommittee heard John Glenn explain that the order of things was that "men go off and fight the wars and fly the airplanes". The Mercury 13 , as they were later called, never flew. Svetlana Savitskaya became the second woman in space in August 1982 and Sally Ride the first American in June 1983.

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Her flight was a propaganda triumph the Soviet Union declined to follow up; the women's group was disbanded in 1969. What it proved was never in doubt among the engineers: the body in the seat did not care who it belonged to.

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The First Spacewalk

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The first human to float free of a spacecraft nearly did not get back in. On 18 March 1965 Alexei Leonov, co-pilot of Voskhod 2 , crawled through an inflatable fabric airlock called Volga , a tube 2.5 metres long and 1.2 metres across that had been folded against the hull at launch, opened the outer hatch and pushed himself out on a 5.35-metre tether 475 kilometres above the Earth. He spent 12 minutes and 9 seconds outside, tumbling slowly, filmed by a camera on the airlock rim and by a second one on his thigh that he could not reach to operate.

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Then the suit took over. The Berkut was a soft pressure suit inflated to 0.4 atmospheres, and in vacuum it ballooned until his fingers slipped out of the gloves and his feet out of the boots; he could not bend enough to fit through the hatch. Without telling the ground, he opened a valve and bled the pressure down to 0.27 atmospheres, below the safe limit, and squeezed in head first, which meant turning round inside a tube only slightly wider than he was. His body temperature rose nearly two degrees and the suit filled with sweat to the knees. Had he passed out, his commander Pavel Belyayev would have had to cut the airlock loose and come home alone.

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The flight had more in store. The automatic re-entry system failed, and Belyayev flew the first manual re-entry of the Soviet programme, overshooting by 386 kilometres into the snowbound forest near Perm. The crew spent two nights in the capsule at around minus 25 degrees Celsius, before a rescue party on skis reached them; a helicopter lifted them out on 21 March. Voskhod itself was a Vostok with the ejection seat removed to make room: Voskhod 1, in October 1964, had carried three men, Komarov, Feoktistov and Yegorov, in shirtsleeves because there was no room for suits, a stunt timed to beat Gemini's first two-man flight.

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The American reply came eleven weeks later. On 3 June 1965 Ed White opened the hatch of Gemini 4 and spent about 20 minutes outside, moving with a hand-held gun that squirted compressed oxygen, his helmet visor gold-plated against the sun, his tether 7.6 metres long and fitted with an oxygen line. The gun ran out in three minutes, and James McDivitt, in the left seat, took the photographs that made the spacewalk look serene. Getting White back in was the hard part: the hatch latch jammed and he reported that closing it was "the saddest moment of my life".

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Both men came home. Between them they had shown that a human could work outside a spacecraft, and that doing anything useful there, let alone building a station, would need handholds, training and a suit that did not fight its wearer. That took the rest of the decade to learn.

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Gemini: Learning to Rendezvous

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Apollo needed four things that nobody had done: find another spacecraft in orbit and dock with it, stay up for the two weeks a lunar round trip would take, work outside for hours, and come down where you meant to. Project Gemini bought all four in ten crewed flights between March 1965 and November 1966, on a two-seat capsule of 3.8 tonnes launched by the Air Force's Titan II missile, 1,900 kilonewtons of thrust burning hypergolic propellants that ignite on contact. Gemini had ejection seats instead of an escape tower, the first fuel cells flown in space, an onboard computer and sixteen manoeuvring thrusters, which made it the first spacecraft a pilot could really fly.

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Rendezvous is not intuitive. Speed up to catch something ahead of you and you climb to a higher, slower orbit and fall behind; the trick is to drop lower and faster, then rise to meet the target. The man who had worked out the mathematics was Buzz Aldrin, whose MIT doctorate on the subject earned him the nickname Dr Rendezvous. In December 1965 Frank Borman and Jim Lovell flew Gemini 7 for 14 days, a record that stood until 1970, and on 15 December Wally Schirra and Tom Stafford in Gemini 6A rose to meet them, closing to 30 centimetres and flying in formation for more than five hours, proving the orbital mechanics worked exactly as the equations said.

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Docking came next and nearly ended in disaster. On 16 March 1966 Neil Armstrong and David Scott in Gemini 8 joined an unmanned Agena target vehicle, the first docking in history, and twenty-seven minutes later the combined craft began to roll. They undocked, assuming the Agena was at fault, and the spin got worse, reaching one revolution a second as a stuck thruster, number 8, kept firing. On the edge of blacking out, Armstrong shut down the manoeuvring system, steadied the capsule with the re-entry thrusters and brought it down early in the Pacific. The calm he showed that day was a large part of why he commanded Apollo 11.

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Gemini 9 found its target's shroud jammed half open, which Stafford called an "angry alligator", and Gene Cernan's spacewalk ended with his visor fogged and his pulse at 180 after he exhausted himself fighting the suit. Gemini 11 used its Agena's engine to reach 1,369 kilometres, a record for Earth orbit that still stands. The lesson of the exhausted spacewalkers was learned on the last flight: Aldrin, on Gemini 12 in November 1966, trained underwater in a swimming pool, and with handholds, foot restraints and tethers fitted to the capsule he worked outside for five and a half hours across three excursions without strain.

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Twenty months, ten crews, every objective met. When Apollo's crews later docked with the lunar module and took their spacewalks on the Moon, they were spending skills that Gemini had earned.

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The Soviet Moon Rocket

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The Soviet answer to the Saturn V was taller, heavier at the base and had thirty engines where the American rocket had five, and it never once reached orbit. The N1 stood 105 metres on its pad at Site 110, Baikonur, and weighed 2,750 tonnes fuelled. Its first stage, Block A, was a truncated cone 17 metres across with thirty NK-15 engines arranged in two rings, producing 45 meganewtons of thrust, the most of any rocket until Starship. Above it sat Block B with eight engines, Block V with four, then the two stages of the lunar complex and at the top the LOK orbiter and a single-seat LK lander, to put 95 tonnes into low orbit and one cosmonaut on the Moon.

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Thirty engines was not a choice but a quarrel. Valentin Glushko, the country's great engine designer, refused to build the large kerosene-and-oxygen engines Sergei Korolev wanted, insisting on hypergolic propellants Korolev considered poison. Korolev turned instead to Nikolai Kuznetsov, a builder of aircraft turbines who had never made a rocket engine; his NK-15 was excellent but small, so thirty were needed, policed by a computer called KORD that shut down a failing engine and its opposite number. There was no test stand big enough to fire the whole stage, so the first time all thirty engines ran together was at launch. Korolev died on the operating table on 14 January 1966, and his deputy Vasily Mishin inherited the programme with less money than Apollo and three rival bureaux.

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The four launches were four explosions. On 21 February 1969 a fire in the engine bay caused KORD to shut everything down at 69 seconds. On 3 July 1969, thirteen days before Apollo 11, a pump failure cut 29 of 30 engines just above the pad, and the rocket fell back onto Site 110 with 2,300 tonnes of propellant, destroying the pad in one of the largest non-nuclear explosions ever recorded and damaging its twin. On 26 June 1971 the third vehicle rolled uncontrollably and broke up at 51 seconds. On 23 November 1972 the fourth flew for 107 seconds, nearly to first-stage burnout, before a pump exploded. A fifth, with improved NK-33 engines, was ready in 1974 when Glushko replaced Mishin and cancelled the programme; the remaining rockets were cut up, and the Soviet Union denied for fifteen years that it had ever raced for the Moon.

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In September 1968 Zond 5 , a stripped Soyuz, flew round the Moon and back with two tortoises, flies and seeds aboard; Zond 6 in November depressurised and crashed. Had either worked cleanly, two cosmonauts might have beaten Apollo 8 round the Moon that December. The LK lander was tested in Earth orbit three times in 1970 and 1971 and worked.

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The programme stayed secret until 1989. The Soviet Union lost the Moon not for want of engineers but for want of a single boss, a single budget and a test stand.

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The Saturn V

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Stand it on a football pitch and the Saturn V would overhang both goals: 110.6 metres tall, 10.1 metres across at the base, and 2,970 tonnes at the moment the hold-down arms let go. Almost all of that mass was propellant. The first stage, the S-IC, carried 2,100 tonnes of kerosene and liquid oxygen and burned through it in two and a half minutes, feeding five F-1 engines that between them produced 34 meganewtons of thrust, each one drinking about 2.6 tonnes of propellant a second. By the time the stage fell away the rocket was 67 kilometres up and travelling at 2.7 kilometres a second.

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Above it sat two stages that burned liquid hydrogen, a fuel so light and so cold that it had defeated engineers for a decade. The S-II used five J-2 engines for six minutes; the S-IVB used a single J-2, first to finish the climb to orbit and then, after a coast of up to three hours, to restart and push the spacecraft towards the Moon at 10.8 kilometres a second. Between the S-IVB and the Apollo spacecraft rode the Instrument Unit, a ring built by IBM that held the guidance computer and flew the whole stack. A Saturn V could place about 120 tonnes in low orbit or send 45 tonnes to the Moon, a record no rocket equalled for half a century.

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How do we know it worked? Thirteen launched between 9 November 1967 and 14 May 1973 and none lost its payload, a record documented in the Marshall Space Flight Center's flight evaluation reports. Wernher von Braun's team at Marshall in Huntsville ran the design; Boeing built the S-IC at Michoud in New Orleans, North American the S-II in California, Douglas the S-IVB, Rocketdyne the engines. The boldest decision came from George Mueller, NASA's head of manned spaceflight, who in 1963 overruled the cautious German stage-by-stage tradition and ordered all-up testing : fly the complete vehicle, live, the first time.

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The first flight, Apollo 4, was flawless, and the sound at the press site shook ceiling tiles loose over Walter Cronkite's head. The second, Apollo 6 in April 1968, was not. A longitudinal oscillation called pogo shook the first stage, two J-2s on the S-II failed and the S-IVB would not restart. The fixes, helium-filled cavities in the propellant lines to damp the oscillation and redesigned fuel-line bellows on the J-2, were made in months, and NASA judged the rocket safe enough to send Apollo 8 to the Moon on only its third launch.

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Three complete vehicles survive on their sides in Florida, Texas and Alabama, because the last three Moon landings were cancelled and the rockets built to fly them were never used. The Saturn V was retired at the height of its powers, which is why it has had so long to become a legend.

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Lunar Orbit Rendezvous

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Before anyone could build a Moon rocket, NASA had to decide what shape the journey would take, and in 1961 there were three answers on the table. Direct ascent was the version from the films: one enormous rocket, called Nova, flies to the Moon, lands tail-first on the surface and flies home again. Earth-orbit rendezvous assembled a Moon ship from two or more Saturn launches in orbit around Earth, then flew the whole thing down and back. Both put a vehicle the height of a church spire on the lunar surface and asked the crew to land it backwards, looking at the sky.

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The third answer came from a Langley engineer named John Houbolt , building on work by his colleague William Michael and, unknown to any of them, on an idea the Ukrainian theorist Yuri Kondratyuk had published in 1929. Lunar-orbit rendezvous sent one Saturn V, but split the spacecraft in two at the Moon. A command and service module stayed in lunar orbit; a small, light lander went down and came back up with only what it needed. Nothing that was not required for the landing was carried to the surface, and nothing that was not required for the return was lifted off it. Houbolt's arithmetic said this cut the mass launched from Earth roughly in half.

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The idea was deeply unpopular. The Space Task Group dismissed it, and Houbolt broke the chain of command in November 1961 with a nine-page letter to NASA's associate administrator Robert Seamans that began, "Somewhat as a voice in the wilderness". The objection was obvious: it required two spacecraft to find each other and dock 380,000 kilometres from home, with no possibility of rescue if they failed. The persuading took months. In June 1962, after a day of briefings at Marshall, Wernher von Braun stood up and surprised his own engineers by backing lunar-orbit rendezvous, saying his team now agreed it offered the best chance of success within the decade. NASA announced the choice on 11 July 1962, Kennedy's science adviser Jerome Wiesner fought it through the autumn, and in November the contract for the lander went to Grumman.

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The decision defined everything that followed: the two-part spacecraft, the docking tunnel, the lonely third crew member circling the Moon, the whole choreography of Apollo. It also defined the risks. Every landing mission depended on a rendezvous above the far side, out of contact with Earth, and on an ascent engine that had no backup. The Soviet lunar plan reached the same conclusion: the N1-L3 design used a single cosmonaut lander and a separate orbital ship, with the lone cosmonaut transferring by spacewalk.

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Rendezvous worked every time it was tried. The mode that the engineers had called too risky turned out to be the only one that could have met the deadline, and the Moon was reached because one stubborn man kept writing letters.

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The Apollo 1 Fire

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On the afternoon of 27 January 1967, three astronauts were strapped into a command module on top of an unfuelled Saturn IB at Pad 34, rehearsing the countdown. It was called a plugs-out test, and nobody had rated it hazardous. Gus Grissom , Ed White and Roger Chaffee had been inside for more than five hours, held up by a sour smell in the oxygen supply and by a communications system so poor that Grissom asked how they were going to get to the Moon if they could not talk between two or three buildings. At 6.31 in the evening a voice on the loop said there was a fire in the cockpit. Seventeen seconds later the transmissions stopped.

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The cabin had been sealed and pressurised with pure oxygen at 16.7 pounds per square inch, two pounds above the air outside, the standard practice since Mercury. At that pressure pure oxygen turns ordinary materials into fuel. The review board, chaired by Langley's director Floyd Thompson , never found the exact spark, but it found plenty of candidates: chafed wiring under Grissom's couch, a leaking coolant line carrying flammable ethylene glycol, and generous amounts of Velcro, nylon netting and foam that the crew had added for convenience. The hatch opened inwards, in three pieces, and even a well-drilled crew needed ninety seconds to remove it. The pressure of the fire sealed it shut and then split the cabin wall.

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The board's report, delivered in April 1967, was blunt about the spacecraft and about the agency. The Block I command module had more than a hundred engineering changes pending, poor workmanship, and no plan for fire on the pad. North American Aviation, the contractor, was overhauled; so was NASA's oversight. The next crewed version, the Block II , used a 60/40 mix of oxygen and nitrogen on the pad, a single hatch that opened outwards in a few seconds, stainless-steel coolant pipes, fire-resistant Beta-cloth suits, and wiring wrapped and routed under rules written in the fire's aftermath. Twenty months passed before Apollo 7 flew in October 1968, and the delay, in a programme racing a decade's deadline, is why the Moon was reached with five months to spare rather than two years.

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The Soviet programme had already lost a cosmonaut the same way. In March 1961 Valentin Bondarenko , at 24 the youngest of the first group, died in a pressure chamber filled with oxygen when a cloth touched a hotplate; the accident was kept secret until 1986, so the lesson that might have saved three Americans stayed in a Moscow file.

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Flight director Gene Kranz told his controllers the following Monday that they had been neither tough enough nor competent enough, and that the two words would be written on every blackboard in Mission Control. Pad 34 still stands at the Cape, concrete and empty, with the words "Abandon in place" stencilled on the legs.

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Mission Control

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The room most people picture when they think of Apollo is not at the Cape but 1,500 kilometres west, on the second floor of Building 30 at the Manned Spacecraft Center in Houston. The Mission Operations Control Room , the MOCR, ran its first flight in June 1965 and every Apollo mission after it. Four tiered rows of grey consoles faced a wall of maps and data, and the point of it was a single idea that Chris Kraft had worked out during Mercury: the spacecraft was too complex for a pilot to manage alone, so a team on the ground, with more information than the crew, would make the decisions, and one person, the flight director , would have the final word.

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The rows had names. The front row, closest to the screens, was called the Trench: Booster, who watched the Saturn; Retro, who planned the way home; FIDO, the flight dynamics officer who tracked the trajectory; and Guido, who watched the onboard computer. Behind them sat the systems controllers: EECOM for the command module's power and life support, GNC for its guidance, TELMU and Control for the lunar module. The third row held the flight director, the flight surgeon and CAPCOM , always an astronaut, the only person who normally spoke to the crew. Each console had a back room of specialists on its own voice loop, so the room stood on a pyramid of hundreds. Flight directors took team colours: Kraft's Red, Gene Kranz's White, Glynn Lunney's Black, Cliff Charlesworth's Green.

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The method was procedure. Thousands of flight rules were written in advance so that a decision taken in two seconds had been argued for weeks. Before any critical moment the flight director polled the room, position by position, and any "no go" stopped the clock. The controllers were young; their average age during Apollo 11 was around 26. The room could not see the spacecraft at all without the Manned Space Flight Network : three 26-metre dishes spaced around the world at Goldstone in California, Honeysuckle Creek near Canberra and Fresnedillas near Madrid, so that one was always facing the Moon, with Australia's 64-metre Parkes radio telescope added to relay the television from the Apollo 11 landing.

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The Soviet Union worked the same problem with a different shape. Its lunar and interplanetary flights were run from the Yevpatoria deep-space centre in Crimea, and in 1973 a new Flight Control Centre opened at Kaliningrad near Moscow, now Korolyov, in time for the joint Apollo-Soyuz flight. There the State Commission and the chief designer carried the weight that Houston gave to a single engineer at a console.

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The MOCR was restored to its 1969 appearance in 2019, down to the ashtrays and the rotary telephones. What it preserves is less a room than a way of thinking, in which authority goes to whoever has the best data, and everyone has agreed, in writing, what to do before it goes wrong.

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Apollo 8: Earthrise

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In August 1968 the lunar module was months behind schedule, and NASA faced a Christmas with nothing to fly. George Low, the Apollo spacecraft manager, proposed something that had not been in any plan: send the next command module to the Moon without a lander. The CIA's reports that a Soviet Zond spacecraft might carry a cosmonaut round the Moon before the year's end made the gamble easier to accept, and Zond 5 did fly round the Moon in September with a cargo of tortoises. On 21 December 1968 Frank Borman , Jim Lovell and Bill Anders became the first crew to ride a Saturn V, and two hours and fifty minutes later the third stage relit for the translunar injection burn, the first time human beings had left Earth's orbit.

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The flight was a list of firsts, recorded in the mission transcript and the trajectory logs. The crew were the first to see the whole Earth as a disc, the first to be captured by another world's gravity, and the first to see the far side of the Moon with their own eyes. Apollo 8 entered lunar orbit on Christmas Eve after a four-minute engine burn behind the Moon, out of contact with Houston, and made ten orbits in twenty hours at around 110 kilometres above the surface. Borman spent much of the outbound coast ill, which was reported to Earth on a delayed tape rather than the live loop.

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On the fourth orbit the spacecraft was rolling to a new attitude when the Earth appeared above the lunar horizon. Borman saw it first and took a black-and-white frame; Anders called for colour film, and Lovell's "Hey, don't take that, it's not scheduled" is on the transcript as a joke. Anders's photograph, frame AS8-14-2383, became Earthrise : a blue and white half-planet above a grey, lifeless edge, taken by a man who had gone to photograph the Moon. That evening, in the most watched television broadcast to that date, the three men read the first ten verses of Genesis, and Borman signed off with "good night, good luck, a Merry Christmas and God bless all of you, all of you on the good Earth".

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The way home began with the engine burn that had to work: the service propulsion system fired behind the Moon on Christmas morning, and when the spacecraft emerged Lovell told Houston, "Please be informed there is a Santa Claus". Re-entry on 27 December, at 11 kilometres a second, was the fastest any human had ever travelled. Among the thousands of telegrams waiting for Borman was one from a stranger that read simply, "You saved 1968".

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The photograph did more than the mission. Earthrise is credited with helping to launch the modern environmental movement, and the first Earth Day followed sixteen months later. Three men went to look at the Moon and came back having discovered the Earth.

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The Lunar Module

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The lunar module was the first true spacecraft: a vehicle that never had to fly in air and so made no concessions to it. There was no nose cone, no smooth skin, no symmetry: two boxes of equipment bolted together, four splayed legs and two triangular windows that gave it the look of an insect. Grumman built it at Bethpage on Long Island under the engineer Tom Kelly , from a contract signed in November 1962, and the first flight-ready article arrived six years later, a delay that reshaped the whole Apollo schedule.

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It was two spacecraft stacked. The descent stage , an octagonal box 4.2 metres across, carried the landing legs, the scientific equipment and a throttleable engine built by TRW that could run anywhere between about ten and sixty per cent of its 45-kilonewton maximum, the first throttleable rocket engine to fly in space. The ascent stage above it held the crew cabin, the computer, the radars and a smaller fixed-thrust engine of 16 kilonewtons that had to work once, with no backup, or two men stayed on the Moon. Fully fuelled, the Apollo 11 lander weighed 15.1 tonnes, of which more than ten tonnes was propellant, and the later versions with a rover aboard reached 16.4 tonnes.

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Weight ruled everything. Grumman's engineers chemically milled the structure, shrank the windows and removed the seats altogether: the crew stood, held by cables and harnesses, which also let them see the ground through smaller windows. In places the pressure skin of the cabin was aluminium 0.3 millimetres thick, which a dropped screwdriver could puncture, and the outer thermal blankets of gold-coloured Kapton and foil could be dented with a finger. Built for a sixth of Earth's gravity, it could never have landed on Earth, so it could never be fully tested.

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The flight record shows how carefully it was introduced. Apollo 5 flew an uncrewed lander in Earth orbit in January 1968. Apollo 9's Spider in March 1969 was flown by James McDivitt and Rusty Schweickart up to 180 kilometres from the command module and back, the first time a crew had put their lives in a vehicle that could not return to Earth. In May, Apollo 10's Snoopy descended to within 15 kilometres of the surface in a full dress rehearsal, then jettisoned its ascent stage into orbit around the Sun. Two months later Eagle landed with fuel for about twenty-five seconds, by the controller's call, and in April 1970 Aquarius kept the Apollo 13 crew alive for four days as a lifeboat, a job its designers had thought about but never planned for.

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Six landers reached the surface, six descent stages still stand on it, and most of the ascent stages were crashed into the Moon on purpose to ring the seismometers. The lunar module was an ugly, fragile, brilliant machine, and it is the only crewed spacecraft in history that never once failed its crew.

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Apollo 11

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Apollo 11 lifted off from Pad 39A at 13:32 UTC on 16 July 1969 with Neil Armstrong , Buzz Aldrin and Michael Collins aboard, watched by around a million people on the Florida beaches. Three days later the stack was in lunar orbit, and on the afternoon of 20 July the lunar module Eagle undocked from Columbia , leaving Collins to circle alone, out of radio contact for forty-eight minutes of every two-hour orbit while he passed behind the Moon.

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The descent is preserved minute by minute in the air-to-ground transcript and the guidance computer's own logs. Five minutes in, the computer flashed a 1202 alarm , then a 1201: its memory was overloaded by data from a rendezvous radar that a checklist had left switched on. At the guidance console a 26-year-old controller, Steve Bales, with Jack Garman in the back room, judged within seconds that the computer was coping and called "Go". Nearer the ground Armstrong saw that the automatic target was a crater the size of a football field, West crater, surrounded by boulders, and took manual control to fly past it. The controller's calls of "sixty seconds" and "thirty seconds" of fuel remaining are on the tape; the engine stopped at 20:17 UTC with roughly twenty-five seconds left, by the gauge, and Armstrong's first words were "Houston, Tranquility Base here. The Eagle has landed."

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Six and a half hours later, at 02:56 UTC on 21 July, Armstrong stepped off the footpad. Aldrin followed nineteen minutes later and described the view as "magnificent desolation". The moonwalk lasted two hours and thirty-one minutes. They set up a seismometer and a laser reflector, planted a flag, collected 21.5 kilograms of rock and soil, and took a telephone call from President Nixon. An estimated 600 million people watched the grainy television pictures, relayed through Honeysuckle Creek and Parkes in Australia. The same week, the uncrewed Soviet probe Luna 15, sent to grab a soil sample and return it before the Americans, crashed into the Sea of Crises.

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Back inside, Aldrin found that a backpack had snapped off the circuit breaker that armed the ascent engine. He pushed it back in with a felt-tip pen the next morning, and Eagle lifted off at 17:54 UTC, blowing the flag over as it went. A speech drafted for the President in case they were stranded stayed in a drawer. Columbia splashed down in the Pacific on 24 July, and the crew spent the next three weeks in quarantine, first in a converted caravan on the carrier Hornet , in case the Moon had germs.

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Eight days, three men, one landing. The flag they planted was knocked flat, the seismometer fell silent within weeks, and the retroreflector is still returning laser pulses. The Moon had been a place to point at for all of human history. On 20 July 1969 it became a place where people had been.

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Apollo 13

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Fifty-six hours into the flight, 330,000 kilometres from Earth, Jack Swigert flipped a switch to stir the oxygen tanks in the service module, a routine request from Houston. There was a bang, and Apollo 13 's master alarm came on. Swigert's "OK, Houston, we've had a problem here" and Jim Lovell's repeat of it are on the tape, as is Lovell's report a few minutes later that he could see something venting into space. Oxygen tank 2 had exploded, tank 1 was leaking, and the fuel cells that made the command module's electricity and water were dying with them.

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The Cortright review board traced a chain of small decisions. In 1965 the tank's heater thermostats had been specified for 28 volts, and when the ground equipment at the Cape was upgraded to 65 volts nobody changed them. The tank had been dropped five centimetres during handling in 1968 and its drain line damaged, so before launch technicians emptied it by running the heaters for eight hours, welding the thermostat contacts shut and cooking the insulation off the wiring inside.

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What followed is the finest hour of Mission Control . Gene Kranz's White Team handed the main room to Glynn Lunney and became a tiger team working the problem offline. The command module Odyssey was shut down to save its re-entry batteries, and the three men moved into the lunar module Aquarius , designed to keep two people alive for two days, now asked to keep three alive for four. Its descent engine fired for thirty seconds to restore a free-return trajectory , and for four and a half minutes after rounding the Moon to speed the journey home. The lander's carbon-dioxide scrubbers were round and the command module's spares were square; a team under Ed Smylie designed an adaptor from a plastic bag, a hose, tape and the cover of the flight plan, and Swigert built it from instructions read up by voice. The cabin fell to 3 degrees Celsius and water was rationed to a few hundred…

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The last problem was powering up a frozen command module from nothing, a procedure that had never been written. Ken Mattingly, bumped from the crew three days before launch because he had been exposed to German measles, spent days in the simulator with controller John Aaron working out a sequence that would not blow the batteries. It worked. Odyssey splashed down near Samoa on 17 April, after a radio blackout that ran longer than expected, and Lovell later called the mission a successful failure.

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The film made Kranz's line "failure is not an option" famous; he never said it during the flight, and later adopted it as a book title. What the records show is a room of people in their twenties and thirties who had rehearsed disaster for years. The Moon was not reached. Everyone came home, and that is the point of the story.

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Science on the Moon

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Apollo 11 proved the landing; the five missions that followed turned the Moon into a field site. Apollo 12 showed what precision could do. On 19 November 1969 Pete Conrad and Alan Bean set Intrepid down 163 metres from Surveyor 3 , a robot that had landed two and a half years earlier, walked over to it and cut off its camera and scoop to see what thirty-one months on the lunar surface had done to them. They also carried the first ALSEP , the Apollo Lunar Surface Experiments Package, a nuclear-powered station that ran for years after the crew had gone. Its seismometer recorded the lander's ascent stage being crashed back into the Moon and the ground ringing for nearly an hour.

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The five ALSEP stations, switched off in September 1977 only to save money, revealed a world with a small core, a thick cold crust and quakes triggered by tides. The laser retroreflectors left by Apollo 11, 14 and 15, and by the Soviet Lunokhod rovers, are still used: a pulse from Earth takes two and a half seconds to return, and the measurements show the Moon drifting away by 3.8 centimetres a year.

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The last three missions carried a battery-powered rover, and the explorers' radius jumped from a few hundred metres to several kilometres. On Apollo 15 , in 1971, Dave Scott and Jim Irwin drove to the edge of Hadley Rille, a lava channel 300 metres deep, and picked up sample 15415, a chunk of white anorthosite about four billion years old that the press called the Genesis Rock. Before leaving, Scott dropped a hammer and a falcon feather together on live television. Apollo 16 went to the Descartes highlands in April 1972 expecting volcanic rock and found impact breccias, overturning the leading theory of the site in an afternoon. Apollo 17 , in December 1972, carried the only professional geologist to walk on the Moon, Harrison Schmitt, who spotted orange soil at Shorty crater: tiny beads of volcanic glass 3.6 billion years old, sprayed from a fire fountain.

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Between them the six crews brought home 382 kilograms in 2,196 samples, and the three Soviet Luna robots added about 300 grams. The rocks settled old questions: the highlands were the frozen crust of a global magma ocean, the dark seas were basalt floods, and the Moon's chemistry matched the Earth's so closely that it must have been born from the Earth in a giant collision. Later laboratories found water locked in the glass beads, and in 2022 NASA opened an Apollo 17 sample that had been sealed for fifty years so that better machines could read it.

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China's Chang'e 5 and 6 have since returned nearly four kilograms more, including the first far-side rocks, but the Apollo collection remains the foundation. Every date in the history of the inner Solar System is counted, somewhere down the chain, from a rock that an astronaut picked up with a pair of tongs.

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After Apollo: Skylab and Soyuz-Apollo

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The last three landings were cancelled before the second one had flown: Apollo 20 in January 1970, Apollo 18 and 19 that September, their Saturn Vs already built. What remained went into two final projects: a laboratory the size of a house, and a handshake.

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Skylab was a Saturn V third stage with the fuel tank turned into living space: a cylinder 6.6 metres across with two decks, a wardroom, sleeping cubicles, a shower and a telescope mount, 77 tonnes in all, launched on 14 May 1973 on the last Saturn V to fly. Sixty-three seconds into the climb the micrometeoroid shield tore off, taking one of the two main solar wings with it and jamming the other. The station reached orbit with half its power and no sun shade, and the cabin climbed past 50 degrees Celsius. Eleven days later Pete Conrad, Joe Kerwin and Paul Weitz arrived, pushed a folding parasol out through a small airlock, and on 7 June Conrad and Kerwin went outside with cable cutters to free the stuck wing. The station was saved by a spacewalk, as Hubble would be in 1993.

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Three crews lived aboard for 28, 59 and 84 days, the last of them, Gerald Carr, Ed Gibson and Bill Pogue, setting an American duration record that stood until 1995. The Apollo Telescope Mount returned more than 150,000 images of the Sun in X-rays and ultraviolet and discovered the coronal holes from which the solar wind pours. The third crew, overscheduled, took an unplanned day off on 28 December 1973; the story that they went on strike grew in the telling, and Carr spent years correcting it. Skylab was abandoned in February 1974, awaiting a Shuttle boost that came too late, and on 11 July 1979 it fell across the Indian Ocean and Western Australia.

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The Apollo-Soyuz Test Project grew from the détente of 1972, when Nixon and Kosygin signed an agreement on a joint mission. Each side had to learn the other's language, docking hardware and air: Soyuz breathed nitrogen and oxygen at sea-level pressure, Apollo pure oxygen at a third of it, so a docking module served as an airlock between them. Soyuz 19, with Alexei Leonov and Valeri Kubasov, launched from Baikonur on 15 July 1975; Apollo followed seven hours later with Tom Stafford, Vance Brand and Deke Slayton, the last of the Mercury Seven to fly, thirteen years after being grounded for a heart murmur. They docked on 17 July, and three hours later Stafford and Leonov shook hands through the open hatch.

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It was the last flight of an Apollo spacecraft and the last American crewed launch for nearly six years. The two programmes that had raced each other to the Moon ended with their crews sharing a meal in orbit, and two decades later a descendant of its androgynous docking port joined the Shuttle to Mir.

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Mariner: The First Flybys

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The first spacecraft to reach another planet was the second one built. Mariner 1 left Cape Canaveral on 22 July 1962 and was destroyed by the range safety officer 293 seconds later, after its Atlas wandered off course. Its twin, Mariner 2 , 203 kilograms, built at the Jet Propulsion Laboratory in Pasadena, launched on 27 August and flew past Venus on 14 December 1962 at a distance of 34,773 kilometres. Its microwave radiometer scanned the planet's disc and found the edges cooler than the centre, which meant the heat was coming from the ground, not the cloud tops: a surface above 400 °C. On the way out, Marcia Neugebauer and Conway Snyder's plasma instrument measured the solar wind blowing continuously for the first time.

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Mars came next. Mariner 4 , 260 kilograms, launched on 28 November 1964 and passed Mars on 15 July 1965 at 9,846 kilometres, taking 21 complete pictures and part of a 22nd on a tape recorder. Each frame was 200 by 200 pixels in 64 shades of grey, and the radio link ran at 8⅓ bits per second, so a single picture took about eight hours to reach Earth. Engineers too impatient to wait for the computer pinned the first strips of numbers to a wall and coloured them in by hand with pastels. The pictures showed craters, a dead, Moon-like surface under an atmosphere that radio tracking put at under one per cent of Earth's. Lowell's canals died that week.

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Mariner 8 fell into the Atlantic in May 1971, so Mariner 9 , launched on 30 May, went to Mars alone and entered orbit on 14 November 1971, the first spacecraft to orbit another planet, thirteen days ahead of the Soviet Mars 2 . It arrived in the middle of a global dust storm that hid the entire surface. JPL simply waited. When the dust settled in January the cameras found a volcano 22 kilometres high, later named Olympus Mons, a canyon system 4,000 kilometres long now called Valles Marineris after the spacecraft, and channels that looked carved by water. It returned 7,329 pictures and mapped 85 per cent of the planet.

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Mariner 10 was the cleverest. Giuseppe Colombo of Padua pointed out in 1970 that if the spacecraft's orbit were tuned to exactly twice Mercury's period, it could meet the planet again and again. Launched on 3 November 1973, it swung past Venus on 5 February 1974, the first use of one planet's gravity to reach another, and flew by Mercury three times, on 29 March 1974, 21 September 1974 and 16 March 1975, mapping 45 per cent of a cratered world that, to everyone's surprise, had a magnetic field.

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Flyby, orbit and gravity assist: the three tools of planetary exploration were all worked out by ten spacecraft of which three were lost. Every mission in this part of the book is a Mariner by descent.

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The Venera Landings

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Venus is the easier planet to reach and the harder one to survive. Its surface sits under 92 bar of carbon dioxide, the pressure found 900 metres down in the sea, at 465 °C, hot enough to melt lead, beneath clouds of sulphuric acid. Nobody knew that in 1967. Venera 4 , a 383-kilogram Soviet capsule, parachuted into the atmosphere on 18 October 1967 and transmitted for 93 minutes as its readings climbed past 262 °C and the pressure gauge ran off its scale at 18 atmospheres; it was crushed around 25 kilometres up. The American Mariner 5 flew past a day later and its radio signal, bent by the atmosphere, confirmed that the ground lay far deeper and hotter than anyone had designed for.

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So the Lavochkin bureau under Georgy Babakin built a spacecraft for 180 atmospheres. Venera 7 carried a titanium pressure sphere, pre-chilled before entry, and landed on 15 December 1970. Its parachute tore, it hit at 17 metres per second and toppled, and the signal seemed to die. Weeks later engineers re-examining the tapes found 23 minutes of transmission at one per cent of normal strength: 475 °C and about 92 atmospheres, the first data ever sent from the surface of another planet. Venera 8 survived 50 minutes in July 1972 and found daylight bright enough for photographs.

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The photographs came in October 1975. Venera 9 and 10 were 1,560-kilogram descent craft with a disc aerobrake, a crushable landing ring and a sphere a metre across, each with an orbiter overhead to relay the signal. On 22 October 1975 Venera 9 sent the first picture from another planet's surface, a 180-degree panorama of flat, sharp-edged rocks; it lasted 53 minutes. The lens caps on Venera 11 and 12 in 1978 refused to come off. Venera 13 , landing on 1 March 1982, sent the first colour panoramas, drilled into the soil and analysed a sample by X-ray fluorescence, and survived 127 minutes at 457 °C and 89 bar, still the record for any machine on Venus. Venera 14 managed 57 minutes four days later.

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Everything was timed in minutes, because the heat always won: the instruments sat in the titanium sphere beside a pre-chilled heat sink, the cameras looked out through quartz windows, and the drill and spectrometer had to finish before the electronics cooked. In June 1985 the two Vega craft, on their way to Halley's Comet, dropped landers and two balloons that floated for about 46 hours in the cloud deck 54 kilometres up, tracked by twenty radio telescopes round the world, the only aircraft ever to fly on another planet.

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The Soviet Union never managed a working Mars lander, but it owned Venus: all ten successful landings, between 1970 and 1985. Nothing has touched the surface since, and the landers planned for the 2030s will be built with Venera's numbers in front of them.

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Viking on Mars

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On 20 July 1976, seven years to the day after Apollo 11, Viking 1 came down on Chryse Planitia and sent back a picture of its own footpad resting on red gravel. It was meant to land on 4 July, the American bicentennial, but orbiter pictures showed the chosen site strewn with boulders and the team spent two weeks hunting for somewhere flatter. Viking 2 landed on 3 September in Utopia Planitia, on the other side of the planet. Each lander weighed about 600 kilograms, ran on two radioisotope generators, and came down on three legs under eighteen small rocket nozzles that spread the exhaust so it would not scour the soil the mission had come to test.

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Viking was built to ask whether there was life on Mars, and carried three biology experiments in a box the size of a microwave oven. The Gas Exchange experiment fed a sample nutrient broth and watched for gases; the Pyrolytic Release experiment offered radioactive carbon dioxide and looked for it fixed into organic matter; and Gilbert Levin's Labeled Release experiment dripped radioactive nutrient onto soil and listened for labelled gas coming off. Labeled Release gave a strong positive at both sites, and when the control sample was heated to 160 °C first the response vanished, exactly as it would for living things. But the gas chromatograph mass spectrometer, which looked directly for organic molecules, found none at all, not even the few that meteorites deliver. Most scientists concluded that the soil was chemically reactive, oxidised by ultraviolet light, and that chemistry, not…

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The argument reopened in 2008, when NASA's Phoenix lander found perchlorate salts in the Martian soil. Perchlorate heated in a spectrometer oven destroys organic molecules, so Viking may have cooked the evidence it was looking for; a 2010 reanalysis found traces of chlorinated organics had been there all along, and Curiosity has since found organics in Gale Crater. Viking's are still the only life-detection experiments run on another planet, and still ambiguous.

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The two orbiters mapped the planet in 52,000 images and on 25 July 1976 photographed a mesa in Cydonia that, with the sun low and a dropout pixel in the right place, resembled a face. NASA released it as a curiosity, the tabloids adopted it, and Mars Global Surveyor's camera in 1998 and 2001 showed an ordinary eroded hill. The landers reported weather for years. Viking 2 fell silent in April 1980; Viking 1, renamed the Thomas Mutch Memorial Station after the leader of its imaging team, worked until 11 November 1982, six years and four months after landing.

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Every lander since has stood on Viking's shoulders. Its question, whether Martian soil has ever been alive, is still open, and is why Perseverance's sample tubes are waiting to come home.

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Pioneer and the Plaque

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Nobody knew whether a spacecraft could cross the asteroid belt. Pioneer 10 , a 258-kilogram spinning craft run by NASA's Ames Research Center, launched on 2 March 1972 on an Atlas-Centaur at a record 51,800 kilometres per hour, passed the Moon in eleven hours and entered the belt in July. Engineers had put the odds of a fatal collision as high as one in ten; its detectors registered a sprinkling of dust and in February 1973 it came out the other side. On 3 December 1973 it passed 132,000 kilometres above Jupiter's cloud tops, took the first close pictures and absorbed a radiation dose a thousand times what would kill a person; instruments glitched, false commands fired, and it survived. Pioneer 11 followed on 5 April 1973, flew within 42,800 kilometres of Jupiter on 2 December 1974, used its gravity to climb across the solar system, and on 1 September 1979 became the first spacecraft…

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Both carried a message. The science writer Eric Burgess suggested it; Carl Sagan and Frank Drake designed it in three weeks; Linda Salzman Sagan drew it. The Pioneer plaque is a gold-anodised aluminium plate, 15 by 23 centimetres, bolted to the antenna struts. It shows hydrogen's spin-flip transition as a unit of length and time, a map of fourteen pulsars locating the Sun in the galaxy, the solar system with the spacecraft's path, and a man and a woman standing in front of the craft to give their scale. The nudity drew letters to newspapers; the pulsar map drew the remark that it was a very good way to tell strangers where we live.

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Pioneer 10 kept going. Its four plutonium generators, 155 watts at launch, faded year by year, and its last faint signal arrived on 23 January 2003 from 12.2 billion kilometres, eighty times the Earth's distance from the Sun. Pioneer 11 was last heard in 1995. Tracking had shown both craft slowing slightly more than gravity could explain, by under a billionth of a metre per second squared. The Pioneer anomaly was debated for twenty years as a possible flaw in gravity, until in 2012 Slava Turyshev and colleagues rebuilt the spacecraft from old drawings and showed that heat from the generators and electronics, radiating unevenly off the back of the dish, produced exactly the push observed.

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The name was reused closer to home. In 1978 Pioneer Venus sent an orbiter whose radar mapped 93 per cent of Venus's surface through its clouds, and a bus that released four probes into the atmosphere on 9 December 1978. None was built to survive landing; the one that came down on the day side transmitted from the surface for 67 minutes anyway.

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The Pioneers were scouts, cheap and tough, sent to see whether the road was passable. It was, and the Voyagers were already built to take it.

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The Voyager Grand Tour

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In 1965 Gary Flandro, a summer student at JPL, noticed that in the late 1970s Jupiter, Saturn, Uranus and Neptune would line up so that a spacecraft could use each planet's gravity to reach the next, cutting a thirty-year journey to twelve. The alignment comes round every 175 years or so. NASA could not afford the full Grand Tour it proposed, so it built two cheaper craft and aimed only the second at the outer two planets. Voyager 2 launched first, on 20 August 1977; Voyager 1 , on a faster route, left on 5 September. Each weighed 825 kilograms, carried a 3.7-metre dish, eleven instruments and three plutonium generators.

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Voyager 1 reached Jupiter on 5 March 1979. Four days later a navigation engineer, Linda Morabito, overexposed a picture of the moon Io to find background stars and saw a cloud rising 270 kilometres off its edge: a volcano in eruption, the first seen beyond Earth. Both craft found rings round Jupiter, lightning in its clouds and an ice shell cracked like a windscreen on Europa. At Saturn, on 12 November 1980, Voyager 1 was sent close to Titan, the one moon with a thick atmosphere, a choice that threw it up out of the plane of the planets and ended its tour. Voyager 2 took the long road: Saturn on 25 August 1981, Uranus on 24 January 1986 and Neptune on 25 August 1989, finding geysers on the moon Triton. It remains the only spacecraft to have visited either planet.

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Each carries a Golden Record , a gold-plated copper disc with a stylus and pictorial instructions on its cover, assembled by a committee under Carl Sagan: 115 images, greetings in 55 languages, whale song, a kiss, and ninety minutes of music from Bach to Chuck Berry. On 14 February 1990, at Sagan's urging, Voyager 1 turned its camera back from six billion kilometres and took the Pale Blue Dot , the Earth less than a pixel wide in a ray of scattered sunlight. The cameras were then switched off to save power.

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On 25 August 2012 Voyager 1 crossed the heliopause, where the solar wind gives way to interstellar gas; its plasma wave instrument heard the change in density. Voyager 2 followed on 5 November 2018. Both still transmit, Voyager 1 from more than 160 times the Earth's distance from the Sun, its signal taking nearly a day to arrive. The generators lose about four watts a year, so JPL has been switching instruments off one by one through the 2020s; in 2024 a failed memory chip was worked round by rewriting code on a computer forty-six years old and twenty-four billion kilometres away.

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NASA took a once-in-175-years chance with two spacecraft built in five years. Neither will ever reach another star, but both will outlast the Earth, carrying the record of what we sounded like.

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Galileo and Juno at Jupiter

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Galileo left Earth in the cargo bay of the shuttle Atlantis on 18 October 1989, with no upper stage powerful enough to throw it straight at Jupiter. So it went the long way: past Venus in February 1990 and past Earth twice, in December 1990 and December 1992, and photographed the asteroids Gaspra and Ida on the way. In April 1991 the 4.8-metre high-gain antenna was commanded to open like an umbrella and three of its eighteen ribs stuck, probably because lubricant had worn off during years of lorry journeys while the mission waited out the Challenger grounding. Every trick failed, and the mission would have to be flown through an emergency low-gain antenna at about ten bits per second.

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JPL rewrote the spacecraft: new compression software, the tape recorder as a buffer and three Deep Space Network dishes combined raised the link to around 160 bits per second, enough for perhaps seventy per cent of the planned science. In July 1994 the crippled craft watched the fragments of Comet Shoemaker-Levy 9 strike Jupiter's far side, the only direct view of the impacts. On 7 December 1995 the 339-kilogram probe, released five months earlier, hit the cloud tops at 47 kilometres per second, braked at 228 g, and transmitted for 58 minutes as it sank 160 kilometres, reporting winds of 720 kilometres per hour and far less water than expected: it had fallen into a dry spot. The orbiter arrived the same evening.

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Over 34 orbits Margaret Kivelson's magnetometer found that Europa bends Jupiter's magnetic field as a conducting shell would, which meant a global ocean of salty water beneath the ice, and that Ganymede has a field of its own. On 21 September 2003, its fuel nearly gone, Galileo was steered into Jupiter at 48 kilometres per second so that it could never crash on Europa and contaminate the ocean it had found.

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Juno is its opposite: solar-powered where Galileo carried plutonium, with three nine-metre wings giving about 500 watts at Jupiter; its instruments in a titanium vault a centimetre thick; and flying over the poles, dipping within 4,200 kilometres of the cloud tops each orbit before retreating far out of the radiation belts. Launched on 5 August 2011, it arrived on 4 July 2016. A worry over helium valves kept it on a 53-day orbit instead of the planned 14. Its microwave radiometer found the Great Red Spot reaching some 300 kilometres down and the winds 3,000 kilometres; its gravity data showed a core that is fuzzy rather than solid. Extended, it added flybys of Ganymede in 2021, Europa in 2022 and Io in December 2023 and February 2024, within 1,500 kilometres of the most volcanic body in the solar system.

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Galileo found the ocean; Juno measured the planet that heats it. Europa Clipper, launched in October 2024, is on its way to the ice to look for a way in.

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Cassini-Huygens at Saturn

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Cassini-Huygens was the largest interplanetary spacecraft ever launched by the West: 5.7 tonnes at lift-off on a Titan IVB on 15 October 1997, more than half of it propellant, with a 4-metre dish supplied by the Italian Space Agency, twelve instruments on the NASA orbiter and six more on ESA's Huygens probe. No rocket could throw that at Saturn, so it borrowed speed from Venus twice, in April 1998 and June 1999, from Earth in August 1999 and from Jupiter in December 2000, and fired its engine for 96 minutes on 1 July 2004 to slip into orbit through a gap in the rings.

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Huygens separated on Christmas Day 2004 and on 14 January 2005 entered the atmosphere of Titan, the moon under an orange haze. It descended for two hours and 27 minutes under three parachutes, its cameras clearing the haze at 30 kilometres to reveal river channels running into a dark shoreline, and landed at 4.5 metres per second on a damp plain of ice pebbles with the consistency, its penetrometer reported, of crème brûlée. It transmitted for 72 minutes from the ground while the Green Bank and Parkes radio telescopes listened to its faint carrier directly; one of its two radio channels was lost because a command to switch on a receiver had never been sent, and half the pictures went with it.

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Cassini stayed thirteen years and 294 orbits. Its radar, peering through Titan's haze on 127 flybys, found seas of liquid methane and ethane near the north pole, the only open liquid known beyond Earth. In 2005 its magnetometer noticed Saturn's field draped round the small moon Enceladus, and the cameras then saw why: geysers of water ice jetting from four warm fractures at the south pole, feeding Saturn's E ring. The dust analyser tasted salt in the grains, and in 2015 the mass spectrometer flew through the plume at 49 kilometres altitude and found molecular hydrogen, a sign of hot rock reacting with seawater on the floor of a global ocean. In the rings it photographed the propeller-shaped wakes of embedded moonlets and waves raised by passing moons; over the north pole it mapped a hexagonal jet stream 30,000 kilometres across.

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The mission ran on 33 kilograms of plutonium-238, and in 2017 the fuel for steering ran short. Rather than risk a crash on Enceladus or Titan, the team flew 22 Grand Finale orbits through the 2,000-kilometre gap between the planet and its innermost ring, weighing the rings and sounding Saturn's interior, and on 15 September 2017 sent Cassini into the atmosphere, antenna tilted to keep transmitting until its signal ended at 11:55 Universal Time.

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Cassini turned Saturn from a picture into a place with weather, seasons and an ocean moon that may be habitable. The next craft, NASA's Dragonfly , is a rotorcraft due to fly across Titan's dunes in the 2030s.

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Mars Rovers

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The first wheels on Mars were the size of a microwave oven. Sojourner , 10.6 kilograms under a solar panel the size of a tea tray, rolled off the Pathfinder lander on 5 July 1997, a day after it bounced to a stop on Ares Vallis inside a cluster of airbags. Designed for seven days, it ran for 83 and covered about 100 metres, while a new thing called the World Wide Web served its pictures to a public that had not seen Mars close up since Viking. The airbags were reused in January 2004 for Spirit and Opportunity , 185-kilogram twins built for 90 days. Spirit lasted six years and found silica from ancient hot springs before bogging down in 2009; Opportunity found rock laid down by water, drove 45.16 kilometres, more than any other vehicle on another world, and fell silent in a global dust storm in June 2018 after 14 and a half years.

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Curiosity , 899 kilograms with a plutonium generator instead of solar panels, was too heavy for airbags, so on 6 August 2012 it was lowered on cables from a hovering rocket platform, the sky crane, into Gale Crater. It drilled rock, found organic molecules and a lake bed that had been habitable for millions of years, and began climbing the five-kilometre mound of Mount Sharp, where it is still working. Perseverance , its 1,025-kilogram near-twin, landed in Jezero Crater on 18 February 2021 with a different job: to drill cores from an ancient river delta and seal them in titanium tubes for return to Earth. By 2025 it had filled most of its 43 tubes and left ten in a depot at Three Forks as insurance.

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Strapped to its belly was Ingenuity , a 1.8-kilogram helicopter with rotors at 2,400 revolutions per minute to grip air one per cent as dense as Earth's. Meant for five test flights, it made 72 between 19 April 2021 and 18 January 2024, scouting routes until a rotor blade broke on landing. China's Zhurong , a 240-kilogram solar rover, landed in Utopia Planitia on 14 May 2021, drove about two kilometres, found signs of ancient water in the dunes, and hibernated in May 2022 as winter dust coated its panels; it never woke.

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A command takes between four and 24 minutes to arrive, so planners send a day's instructions each morning and rovers drive themselves between waypoints with stereo cameras, perhaps 100 metres a day. The samples are the unfinished business: the Mars Sample Return plan, a NASA lander with ESA's return orbiter, slipped to a return in the 2040s and was sent back for redesign in 2024; its future is uncertain, and the tubes wait on the crater floor.

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Six rovers have driven about 150 kilometres in 28 years. The next, ESA's Rosalind Franklin , is to drill two metres down, deeper than any rover has gone, to look for life where the radiation does not reach.

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New Horizons and Pluto

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New Horizons left Earth on 19 January 2006 faster than any spacecraft before it: 16.26 kilometres per second, on an Atlas V with an extra solid stage, so that it passed the Moon's orbit in nine hours. Seven months later, on 24 August 2006, the International Astronomical Union voted that its destination was no longer a planet. The spacecraft, a 478-kilogram grand piano with a 2.1-metre dish and seven instruments, had been seventeen years in the campaigning: Alan Stern and a group of young scientists calling themselves the Pluto Underground had pushed for a mission since 1989, two designs were cancelled, and in 2001 NASA chose this one, built at the Johns Hopkins Applied Physics Laboratory for a fraction of Cassini's cost.

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On 28 February 2007 it passed Jupiter at 2.3 million kilometres, gaining four kilometres per second from its gravity, then settled into the long cruise, hibernating for about two thirds of the eight years that followed and waking once a year for a check-up, so that a small team could fly it on a single plutonium generator. It woke for good on 6 December 2014. Ten days before the encounter the main computer overloaded and the craft dropped into safe mode; the team at APL rebuilt the command sequence in three days.

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The flyby came on 14 July 2015, 12,500 kilometres above a world 2,377 kilometres across, at 13.8 kilometres per second, 4.8 billion kilometres from Earth with a radio delay of four and a half hours. The craft could not point its dish and its cameras at the same time, so it worked blind all day and phoned home that evening. Pluto turned out to have a heart: Sputnik Planitia , a 1,000-kilometre basin of nitrogen ice churning in slow convection cells, uncratered because the surface renews itself; mountains of water ice 3.5 kilometres high; a blue haze of a dozen layers; and a moon, Charon, with a dark red cap and canyons longer than the Grand Canyon. The 6.25 gigabytes of data took until October 2016 to trickle home at a kilobit a second.

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NASA then pointed it at a body found by Hubble only in 2014. On 1 January 2019 New Horizons flew within 3,500 kilometres of Arrokoth , a 36-kilometre snowman of two lobes gently fused, 6.6 billion kilometres from the Sun, the most distant and most primitive object ever visited: a leftover of the solar system's first days, untouched by heat since. The spacecraft still travels at about 14 kilometres per second, measuring the dust and gas of the outer solar system, and expects to cross the termination shock, where the solar wind stalls, before the decade is out.

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Pluto was reclassified while its first visitor was on the way, and the visit showed why the argument hardly matters: it is a small world with ice volcanoes, weather and a heart.

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Bringing Pieces Home

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A picture of a rock tells you what it looks like. A grain of it in a laboratory tells you how old it is, where it formed and what water has touched it, with instruments that would never fit on a spacecraft. That is why agencies spend a decade to bring back a few grams. The first modern attempt went badly: Genesis spent two years beyond the Moon catching solar wind on wafers of sapphire and silicon, and on 8 September 2004 its capsule hit the Utah desert at 300 kilometres per hour because an accelerometer had been fitted upside down and the parachute never fired. Scientists picked through the shattered wafers for years and still showed that the Sun's oxygen differs from the Earth's.

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Stardust did better. It flew through the tail of Comet Wild 2 on 2 January 2004 at 236 kilometres, catching dust in aerogel, a glass foam, and its capsule landed in Utah on 15 January 2006 at 12.9 kilometres per second, the fastest re-entry of any human-made object. The grains held minerals that could only have formed near the Sun, which meant the early solar system had stirred its ingredients from the inside out, and in 2009 the amino acid glycine.

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Japan's Hayabusa , launched in 2003 to the 535-metre asteroid Itokawa, lost two reaction wheels, leaked fuel, lost contact for weeks and failed to fire its sampling projectile, but it touched down twice, and when its capsule landed at Woomera on 13 June 2010 about 1,500 grains had come along anyway. Hayabusa2 did everything its parent could not: it fired a copper slug into the asteroid Ryugu to make a crater, landed twice, and on 6 December 2020 delivered 5.4 grams, which turned out to contain 20 amino acids and uracil, a building block of RNA. NASA's OSIRIS-REx reached the asteroid Bennu, touched it for six seconds on 20 October 2020, nearly sinking into loose rubble, then dropped 121.6 grams in Utah on 24 September 2023, the largest asteroid sample ever, rich in carbon, water-bearing clays and the salts of an evaporated brine.

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China has brought back the Moon. Chang'e 5 collected 1,731 grams from Oceanus Procellarum in December 2020, the first lunar samples since Luna 24 in 1976, and dated its basalts at two billion years, a billion younger than any Apollo rock: the Moon stayed volcanic far longer than thought. Chang'e 6 landed in the Apollo basin on the far side in June 2024, working through a relay satellite, and on 25 June returned 1,935 grams, the first material from the half of the Moon we never see.

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Mars is the sample still missing. Perseverance's tubes are sealed, but the plan to fetch them was sent back for redesign in 2024, and China has announced its own Tianwen-3 return for the early 2030s. The world that most needs a laboratory may be the last to get one.

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Weightlessness and the Body

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A body in orbit is not beyond gravity. The International Space Station, 400 kilometres up, feels about 90 per cent of the pull we feel on the ground; it simply falls round the Earth fast enough never to land, and everything inside falls with it. The effect is free fall , and the body treats it as a permanent handstand. Within hours, roughly two litres of blood and tissue fluid that gravity normally holds in the legs migrate upwards. Faces puff, legs thin into what crews call "bird legs", the sinuses block, and the sense of smell dulls, which is one reason astronauts ask for hot sauce.

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The slower changes are the dangerous ones. Weight-bearing bone, in the hips, spine and heels, loses about 1 to 1.5 per cent of its mineral density per month, a rate ten times that of an elderly person on Earth, and the calcium leaving the skeleton raises the risk of kidney stones. Muscle shrinks too: without exercise, calf and thigh muscles can lose a fifth of their mass on a six-month flight. The countermeasure is sweat. Each crew member is scheduled around two hours of exercise a day, on the ARED resistive machine, which uses vacuum cylinders to mimic up to 270 kilograms of barbell, on the T2 treadmill, where bungee cords hold the runner to the belt, and on a cycle ergometer with no seat.

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The eyes were a surprise. From around 2005, flight surgeons noticed that returning astronauts' eyeballs had flattened at the back, their optic discs swollen and their eyesight shifted, in some cases permanently. The condition is now called spaceflight-associated neuro-ocular syndrome , SANS, and it affects about two-thirds of long-duration crew; the leading suspect is the headward fluid shift pressing on the brain and the optic nerve. The immune system also drifts, with dormant viruses such as herpes and shingles reactivating in saliva samples.

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How we know all this comes from flight medicine done on the crews themselves. The sharpest study was NASA's Twins Study: Scott Kelly spent 340 days aboard the station from March 2015, while his identical twin Mark stayed on the ground as a control, and ten laboratories compared the pair. Scott's telomeres lengthened in flight and snapped back on landing, his gut bacteria shifted, and some gene expression changed, most of it returning to normal within six months. The endurance record is Soviet: Valeri Polyakov spent 437 days aboard Mir in 1994 and 1995, and walked, unaided, from his capsule to a chair to prove that a Mars crew could stand up on arrival. In June 2024 Oleg Kononenko became the first person to pass 1,000 cumulative days in space.

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None of this has yet stopped anyone flying. It has, instead, defined the problem for Mars: a journey of six to nine months each way, with no treadmill waiting at the far end. The body adapts to orbit remarkably well. The question is how much of Earth it needs to bring along.

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The Spacesuit

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A spacesuit is a spacecraft shaped like a person. It must hold pressure against vacuum, supply oxygen, scrub carbon dioxide, carry away the heat of a working body, stop micrometeoroids and 120-degree sunlight, and still bend at the fingers. The first ones barely did. Mercury's silver suits were modified Navy Mark IV pressure suits from B.F. Goodrich, meant as a backup if the cabin leaked; they were never pressurised in flight. Yuri Gagarin's SK-1 was the same idea in orange, built by the Zvezda plant outside Moscow, which still makes Russia's suits today.

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The Moon demanded a suit a man could walk in. The Apollo A7L , sewn by ILC Dover in Delaware, a company better known for Playtex bras, had a pressure bladder and restraint layer inside a thermal micrometeoroid garment of around twenty layers of Mylar, Kapton, Beta cloth and Teflon fabric. Under it the astronaut wore a liquid-cooling garment threaded with tubing that carried chilled water across the skin, and on his back the PLSS , a 38-kilogram life-support pack good for seven or eight hours. Seamstresses worked to a tolerance of a sixty-fourth of an inch, and every seam was X-rayed. The suit operated at 3.7 psi of pure oxygen, a quarter of sea-level pressure, which is why it could flex at all.

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The two suits in use today are old designs kept young. NASA's Extravehicular Mobility Unit, the EMU , first flew on the Shuttle in April 1983 and still services the International Space Station; with its backpack it weighs about 145 kilograms on Earth, and runs at 4.3 psi, low enough that crews must breathe pure oxygen for hours beforehand to purge nitrogen from the blood, or risk the bends. The Russian Orlan , in service since Salyut 6 in 1977, takes the other approach: the whole backpack is a hinged door, the cosmonaut climbs in through the back in about five minutes, and the suit runs at a higher 5.8 psi with a shorter pre-breathe. An Orlan is serviced in orbit and never comes home.

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Gloves remain the hardest problem. Pressurised fabric fights every grip, and a six-hour spacewalk is a six-hour squeeze of a tennis ball; fingernail loss, from the nail bed pressing against the glove, is common enough to have its own entry in the medical literature. The EMU's age shows too. A spacewalk on 24 June 2024 was abandoned minutes after the hatch opened when water leaked from Tracy Dyson's suit umbilical, and NASA's own inspector general has warned that the fleet cannot last indefinitely. Replacements are coming from industry: Axiom's AxEMU for the Artemis lunar landings, and SpaceX's slimmer EVA suit, which four Polaris Dawn crew wore when they opened their hatch to space on 12 September 2024.

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Every suit is a negotiation between pressure and movement, protection and weight. Sixty years on, the handshake inside the glove is still the thing engineers cannot quite perfect.

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Eating, Washing and the Toilet

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Yuri Gagarin's lunch on 12 April 1961 came from aluminium tubes: meat purée and chocolate sauce, squeezed into the mouth to prove that a human could swallow in free fall. Doctors had genuinely wondered. By Gemini the Americans had freeze-dried food and gelatin-coated bite-sized cubes, which crews disliked so much that John Young smuggled a corned-beef sandwich from a Cocoa Beach delicatessen aboard Gemini 3 on 23 March 1965. He took two bites, crumbs floated off, and the sandwich was put away; Congress held a hearing about it. Apollo added hot water and the spoon-bowl pouch, and Skylab in 1973 had a freezer, a dining table and the only shower ever flown by NASA, a collapsible cylinder that took hours to use and dry.

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Today the International Space Station runs on a menu of around 200 items, most of them thermostabilised pouches or freeze-dried packs rehydrated at the galley in the Unity module, where a food warmer and a potable water dispenser sit beside a table the crew strap their feet beneath. Bread is banned because of crumbs; tortillas replaced it in the Shuttle era and have never left. Salt and pepper come as liquids. Fresh fruit and vegetables arrive on each cargo ship, a Progress, a Dragon or a Cygnus, and disappear within days. Every crew member gets bonus containers of personal choice, and nations supply their own: Russian borscht, Japanese ramen, French pâté for ESA astronauts.

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Water is the real engineering. Lifting a litre to orbit is so expensive that the station recycles almost all of it. The Water Recovery System in Tranquility distils urine in a spinning drum, polishes the result through filters and a catalytic reactor, and blends it with condensate scavenged from the cabin air, including sweat and breath. In 2023, with a new brine processor squeezing the last water from the urine distiller's residue, NASA reported recovering about 98 per cent of the water aboard. The crew joke that today's coffee is tomorrow's coffee is literally true.

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The toilet is the question everyone asks. The Russian ASU in Zvezda and the American Universal Waste Management System , delivered in October 2020, both work on airflow rather than gravity: a fan draws urine into a hose with a personal funnel and solids into a bag inside a canister, where it is compacted and sealed. Urine goes to the recovery system; solid waste is stowed, loaded into a departing cargo ship and burns up with it over the Pacific. Crew train on the ground with a camera-equipped positioning trainer. Washing is wipes, rinseless shampoo and a damp towel, because water does not run in free fall; it clings to the skin in a sheet.

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Every mission plan to Mars begins with the same arithmetic: a crew of four needs about 30 kilograms of food, water and oxygen a day, and nothing can be sent after them. The station is where that arithmetic has been learned, one recycled litre at a time.

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Sleep, Time and Mind

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The International Space Station crosses from night into day every 45 minutes, sixteen sunrises in every 24 hours, so the Sun is useless as a clock. The station runs instead on Coordinated Universal Time , Greenwich time, chosen in the 1990s as a compromise between Houston and Moscow. The crew wake around 06:00, hold a morning conference with the control centres, work through a timeline planned to five-minute blocks, exercise for two hours, and are scheduled to sleep from 21:30. They rarely get the eight and a half hours the plan allows; six is typical, and sleeping pills are the most used drug in orbit.

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Sleep itself needs a cabin. Each crew member has a phone-box-sized crew quarters , four in the Harmony node and two in the Russian Zvezda module, with a temporary seventh in Columbus, with a sleeping bag strapped to the wall, a laptop, a fan, earplugs and a door that shuts out the 60-decibel hum of pumps and fans. Without a pillow or a mattress the body curls into a neutral posture, arms floating in front of the chest. Since 2016 the station's fluorescent tubes have been replaced by LED panels that shift from blue-white in the morning to a dim amber before bed, a deliberate attempt to steer the circadian clock that the windows cannot.

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Crews have been studied for the strain of confinement long before they leave the ground. In Moscow, six volunteers spent 520 days sealed inside the Mars-500 mock spacecraft from June 2010 to November 2011, with a simulated Mars landing in the middle, and the main finding was how much their sleep and activity drifted apart. On the slopes of Mauna Loa in Hawaii, HI-SEAS crews lived in a dome for up to a year; at Concordia station on the Antarctic plateau, ESA studies a dozen winter-over staff who cannot leave for nine months at 3,200 metres and minus 80 degrees. The pattern that emerges is that the quarrels are rarely between crew members and usually between the crew and the ground.

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That is the real story behind the famous Skylab "mutiny". On 28 December 1973 the Skylab 4 crew of Gerald Carr, Edward Gibson and William Pogue, overworked since launch, took an unscheduled day off and then negotiated a lighter timeline with Houston. There was no strike and no radio silence by design; the legend grew in the retelling. Modern support is deliberate: weekly private video calls with family, a psychologist's conference every fortnight, care packages on each cargo ship, music, films and a small artificial Christmas tree that has been aboard for years. Frank White named the other side of the experience in 1987, the overview effect : the shift many astronauts describe on seeing the whole Earth, thin-skinned and without borders.

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Sleep, time and temper are not soft problems; a tired, irritable crew is a safety risk as real as a leaking seal. For Mars, with a 20-minute radio delay and no care packages, the mind may be the hardest system to keep in balance.

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Radiation

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Space is not empty; it is full of fast particles. Three kinds matter to a crew. Galactic cosmic rays are atomic nuclei flung from supernovae at close to the speed of light, a thin, steady drizzle that no practical shielding stops, and the heavy ones, iron nuclei among them, tear through cells like cannonballs. Solar particle events are the opposite: rare, violent floods of protons from a solar flare or coronal mass ejection, lasting hours to days, which good shielding can block. And around the Earth lie the Van Allen belts , two doughnuts of trapped particles found by Explorer 1 in 1958, an inner belt of protons from about 1,000 kilometres up and an outer belt of electrons out beyond 13,000.

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The International Space Station sits beneath the belts at about 400 kilometres, and the Earth's magnetic field deflects much of what comes in. Even so, a crew member absorbs roughly 0.5 to 1 millisievert a day, as much in a day as most people on Earth receive in several months, and a six-month tour adds up to between 80 and 160 millisieverts, the equivalent of thousands of chest X-rays. Most of it arrives over the South Atlantic Anomaly , a region off Brazil where the inner belt dips low because the Earth's magnetic field is offset from its centre; crews there sometimes see flashes of light as particles cross the retina, a phenomenon first reported by Buzz Aldrin on Apollo 11.

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Beyond the magnetic field the numbers climb. The Curiosity rover carried a Radiation Assessment Detector on its 2012 cruise to Mars and recorded about 1.8 millisieverts a day in transit; Cary Zeitlin's team at the Southwest Research Institute worked that out as roughly 0.66 sieverts for a round trip with the current rockets, more than NASA's entire career limit, which in 2021 was set at 600 millisieverts for every astronaut regardless of age or sex. Apollo was lucky as well as brief. Between 4 and 7 August 1972, in the four months between Apollo 16 and Apollo 17, the Sun produced one of the most intense proton storms ever recorded. Calculations since suggest that a crew in a suit on the lunar surface would have received a dose high enough to cause acute radiation sickness, and possibly death.

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Shielding is a trade in mass. Hydrogen-rich materials are best, because light nuclei absorb energy without spraying secondary particles the way aluminium does, so designers favour water tanks, food stores and polyethylene panels placed around sleeping areas. The ISS crew quarters are lined with polyethylene bricks. On NASA's Orion capsule the crew would answer a storm warning by building a shelter from stowage bags in the centre of the cabin and waiting it out. Mars habitats will probably be buried under a metre or more of regolith.

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Radiation is the one hazard of spaceflight that engineering cannot yet remove, only measure and dilute. Every plan for Mars is, in the end, a plan to get there fast and hide well.

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Training to Fly

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The odds of becoming an astronaut are worse than those of winning a seat in most parliaments. When NASA opened applications in 2016 it received 18,300, a record, and in June 2017 chose twelve. ESA's 2021 call drew 22,500 applicants from across Europe and in November 2022 named seventeen: five career astronauts, eleven reservists and one candidate with a physical disability, the British surgeon John McFall, cleared in 2025 for a long-duration flight. China picked its first fourteen fighter pilots from 1,500 in 1996. The requirements have softened from the test-pilot era to a science or engineering degree, good health and a temperament that can be locked in a tin with strangers.

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A new NASA candidate, an ASCAN , spends two years on the basics before being assigned to anything: jet flying in T-38 trainers, systems classes on every module of the International Space Station, robotics on the Canadian arm simulator, wilderness and water survival, and, because the Soyuz and the station's Russian segment demand it, Russian. Only after assignment to a crew does mission-specific training begin, and that takes another two to three years. The "vomit comet" flies parabolas that give 25 seconds of weightlessness at a time; NASA's KC-135 retired in 2004, and ESA uses an Airbus A310 flown from Bordeaux.

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The cathedral of this training is the Neutral Buoyancy Laboratory at the Sonny Carter Training Facility in Houston: a pool 62 metres long, 31 wide and 12 deep, holding 62 million litres of water, with full-scale mock-ups of station modules and truss sections lying on its floor. A suited astronaut is weighted until they neither sink nor float, and spends six or seven hours at a time rehearsing a spacewalk under the eyes of four safety divers, a test director and television cameras, at a ratio of about ten hours in the pool for every hour outside the station. Russia's Hydrolab at Star City, the Gagarin Cosmonaut Training Centre outside Moscow, does the same job with a 12-metre tank; the centre also owns the TsF-18 centrifuge, with an 18-metre arm, and has trained every cosmonaut since 1960.

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Survival training is where the stories come from. Soyuz crews practise a winter landing in a forest near Moscow, two days on the capsule's survival kit, building a shelter from parachute fabric; they practise sea survival in the Black Sea, stripping off Sokol suits inside a bobbing capsule at 40 degrees. ESA sends candidates underground on CAVES, a week in the Sardinian karst, and NASA has sent crews to live ten days in the Aquarius habitat 19 metres below the Florida Keys on NEEMO missions since 2001. The point is to learn how a person behaves when tired, cold and wrong.

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From selection to first launch typically takes five years or more; some candidates wait a decade. Nobody flies untrained, and nobody flies alone: by the time the hatch closes, the crew has rehearsed every ordinary minute and most of the extraordinary ones.

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Launch and Re-entry

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The two most dangerous half hours of any space mission are the first and the last. On a Soyuz launch from Baikonur the crew lie on their backs in moulded seats, knees up, as the rocket builds to a peak of about four g at the end of the first stage; the whole climb to orbit takes under nine minutes, at the end of which a small toy on a string in front of the commander floats free. Above them for the first two minutes sits the launch escape system , a solid-fuel tower that can yank the descent module clear of a failing rocket. On 26 September 1983 the Soyuz T-10a booster caught fire on the pad, and controllers fired the escape tower by radio command two seconds before the rocket exploded; Vladimir Titov and Gennady Strekalov endured around 15 g and landed four kilometres away, bruised. On 11 October 2018 a strap-on booster failed to separate cleanly from Soyuz MS-10 at 119 seconds, and…

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Coming home means losing 28,000 kilometres per hour of speed, and the atmosphere does almost all the work. After a deorbit burn the Soyuz separates into three parts, and only the bell-shaped descent module, with its ablative heat shield , survives. The shield chars and flakes away on purpose, carrying heat with it, while the plasma around the capsule reaches around 1,600 degrees and blocks radio for several minutes. A capsule with its centre of mass offset from its axis can be flown through this, rolling to steer and spreading the deceleration to about four g; lose that control and the fall becomes ballistic , shorter and steeper, at eight g or more. Soyuz TMA-11 made such a descent in 2008, and Soyuz 18a's crew of 1975, after a staging failure, hit a peak above 20 g and came to rest on a mountainside in the Altai, their capsule held by a tree.

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The last kilometres are national styles. A Soyuz lands on the grassland of Kazakhstan under a single 1,000-square-metre parachute, and at about 80 centimetres above the ground six solid rockets in the base fire for a jolt that crews compare to a car crash; recovery helicopters are usually there within minutes to lift the crew out. The Space Shuttle glided to a runway at 346 kilometres per hour, with no second chance. Dragon and Orion return to the water: Dragon under four main chutes into the sea off Florida or California, and Orion, after a skipping entry on Artemis I in December 2022, into the Pacific off Baja California, where a Navy ship winches it aboard.

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How we know the numbers is the flight recorder in each descent module and the crew's own debrief. Every landing is studied as closely as every launch, because nearly seventy years on, the sum of the two is still where most of the risk lives.

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Emergencies in Orbit

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Space stations have three nightmares, and crews drill for all of them: fire, loss of pressure and toxic air. The first great lesson came from the worst one. On 30 June 1971 the crew of Soyuz 11 , Georgy Dobrovolsky, Vladislav Volkov and Viktor Patsayev, returning from three weeks aboard Salyut 1, died when a pressure-equalisation valve jolted open as their modules separated at 168 kilometres. The cabin emptied in under a minute. They wore no pressure suits, because three men in suits would not fit, and the capsule landed itself perfectly. Since then every Soyuz crew has worn the Sokol suit for launch and landing; the ship flew with two cosmonauts until a 1980 redesign seated three in suits.

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Mir in 1997 taught the rest of the list in four months. On 23 February a lithium-perchlorate oxygen candle, the kind the station burned to top up its air, ignited in the Kvant-1 module and spat a blowtorch flame for around 14 minutes while smoke filled the station; the six aboard, including the American physician Jerry Linenger, fought it with extinguishers while it blocked the way to one of the two escape Soyuz. On 25 June a Progress cargo ship, flown by hand by Vasily Tsibliyev with a television camera and a faulty range estimate, struck the Spektr module and holed it. Aleksandr Lazutkin and the NASA astronaut Michael Foale cut the cables running through the hatch and sealed Spektr before the station lost all its air, at the price of a third of its power.

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The station era's emergencies have been quieter and stranger. On 16 July 2013 Luca Parmitano's helmet began to fill with water 44 minutes into a spacewalk, from a clogged fan-pump separator in his suit; blinded, with water in his ears and nose, he felt his way back along the tether to the airlock. NASA's mishap board found the same suit had leaked a week earlier and the sign had been misread. In August 2018 a slow leak traced to a two-millimetre drill hole in the orbital module of Soyuz MS-09 , made on the ground, was sealed in orbit with gauze and epoxy. On 14 December 2022 a micrometeoroid or debris strike punctured the coolant loop of Soyuz MS-22, and a fountain of coolant sprayed into space on live camera; Roscosmos launched a replacement, MS-23, empty, in February 2023, and the crew flew home on it in September after 371 days.

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Behind all of these lies rehearsal. Every ISS crew runs regular emergency drills, racing to the nearest spacecraft with oxygen masks on, closing hatches in order and finding the fire ports in rack panels. Each lifeboat seat is assigned, and ammonia, the coolant in the station's external loops, is the toxic case the drills fear most.

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Nobody has died in space since 1971, and nobody has died aboard a station at all. That record was not luck; it was drilled, module by module, from the lessons of those who did not come back.

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Science in Microgravity

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The International Space Station was sold as a laboratory, and for its first decade the lab was mostly being built. Since 2011 it has hosted well over 3,000 investigations from more than a hundred countries, and the honest audit is more interesting than the brochure. The physics case is the clearest. Remove gravity and buoyancy, sedimentation and convection vanish with it, so fluids, flames and crystals behave as the equations say they should. In the Combustion Integrated Rack in the Destiny module, the FLEX experiments burned droplets of heptane and found, in 2012, that after the visible flame went out the droplet kept burning invisibly as a cool flame at around 500 degrees, a chemistry that engine designers had suspected but never seen cleanly. Capillary-flow experiments rewrote how spacecraft fuel tanks are designed.

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Biology is where the hype has been loudest and the results most mixed. Protein crystals grown in orbit, without the convection currents that disorder them on Earth, can come out larger and more regular, and some have fed drug design, including a reformulated cancer antibody from Merck that now needs an injection rather than a drip. Tissue chips, thumb-sized devices lined with living human cells, have shown muscle and bone ageing in weeks, a model for disease that no clinic can run. In August 2016 Kate Rubins used a MinION the size of a chocolate bar to sequence DNA in orbit for the first time, which means a future crew could identify an infection on the way to Mars. The Twins Study of Scott and Mark Kelly belongs here too, as does the Veggie garden: red romaine lettuce eaten by the crew on 10 August 2015, and a zinnia that flowered in January 2016 after Scott Kelly disobeyed the…

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Some of the station's best science simply points outward. Bolted to the main truss since May 2011, the seven-tonne Alpha Magnetic Spectrometer has recorded more than 200 billion cosmic-ray particles, measuring the antimatter and positron fractions that might betray dark matter. The Cold Atom Lab , installed in Destiny in 2018, chills clouds of rubidium and potassium atoms to within a ten-billionth of a degree of absolute zero and made the first Bose-Einstein condensates in orbit, which last far longer when they do not fall out of their trap. Europe's Columbus module, launched in February 2008, carries the Biolab, a fluid-science laboratory and an electromagnetic levitator for molten metals; Japan's Kibo , completed in 2009, is the largest module and the only one with its own airlock and exposed balcony, where small satellites are released by a robot arm.

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The verdict after a quarter century is modest and real: the ISS has been a superb physics bench, a fair biology lab and a decisive test bed for keeping humans alive. The Nobel-grade discovery may never come. The habit of doing careful science 400 kilometres up is already here.

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Coming Home

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A long-duration crew does not step out of the capsule; they are lifted. Within minutes of a Soyuz thumping down on the Kazakh steppe, recovery teams haul each crew member through the hatch and sit them in a folding chair with a blanket, where they grin, hold a fruit, and try not to be sick. The inner ear's balance organs, idle for six months, now report every head movement as a lurch; blood pools in the legs again and the heart, which has shrunk slightly in orbit, struggles to push it uphill, so standing up risks fainting. Crews describe their arms feeling like lead. Russian crews are flown to Star City, American ones to Houston, and all begin the next morning with a medical team and a tilt table.

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Rehabilitation is a programme, not a rest. NASA's post-flight reconditioning runs two hours a day for 45 days, beginning with walking and balance drills on the landing day and building to running and weights, and the flight surgeons measure everything against the pre-flight baseline. Most systems recover on a schedule: balance within days, blood volume within a fortnight, muscle within a month or two. Bone is the exception. A 2022 study of 17 astronauts led by Leigh Gabel at the University of Calgary found that a year after landing the shin bone had recovered only part of its lost density, and for those who had flown six months or longer the net loss resembled a decade of ageing; the exercise in orbit helped, but it did not close the gap.

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The long stays give the clearest readings. Scott Kelly's 340 days in 2015 and 2016 ended with swollen legs, rashes where fabric touched skin and a fever, but within six months more than 90 per cent of the gene-expression changes measured against his twin had returned to baseline. Frank Rubio went up in September 2022 for six months and came down a year later, after the Soyuz MS-22 coolant leak stranded his crew, with 371 days, the American single-flight record; he walked within days but said it took months to feel normal. Peggy Whitson, flying again in 2025 at 65, holds the American cumulative record at nearly 700 days. Barry Wilmore and Sunita Williams, who had launched in June 2024 for a planned eight-day test of Boeing's Starliner, came home on a SpaceX Crew Dragon on 18 March 2025 after 286 days, and walked within a day.

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What all this means for Mars is sobering and useful. A crew will arrive after six to nine months of free fall and must stand, walk and work on a planet with a third of Earth's gravity, with no recovery team in folding chairs. Polyakov's walk from the capsule in 1995 was the first demonstration that this is possible, and every long stay since has refined the dose. Home, it turns out, is a place the body has to relearn.

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Salyut and Almaz

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The first space station was not American and it was not comfortable. Salyut 1 , launched on a Proton rocket from Baikonur on 19 April 1971, was a stepped cylinder about 15.8 metres long, 18.4 tonnes, with roughly 90 cubic metres of living space, one docking port at the front and a Soyuz propulsion block at the back. It was the Soviet answer to Apollo: having lost the Moon, they would be first to live in orbit.

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Its first crew became its tragedy. Soyuz 10 docked in April 1971 but could not open the hatch. Soyuz 11, with Georgi Dobrovolsky, Vladislav Volkov and Viktor Patsayev, entered on 7 June and stayed a record 23 days. On 30 June, as their descent module separated for re-entry, a pressure-equalisation valve jolted open and the cabin vented to space in under two minutes. The crew wore no pressure suits; there was no room. Recovery teams found the three men dead in their seats. Every Soviet and Russian crew since has worn the Sokol suit for launch and landing.

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Behind the civil name hid a second programme. Vladimir Chelomei's Almaz ("diamond") stations were military reconnaissance platforms with a large camera and a film-return capsule, flown under the Salyut label to disguise them: Salyut 2, which failed in 1973, Salyut 3 in 1974 and Salyut 5 in 1976. Salyut 3 carried a 23-millimetre aircraft cannon, aimed by turning the whole station. On 24 January 1975, with no crew aboard and shortly before it was deorbited, the gun was test-fired by remote command, the only time a weapon has been fired from a crewed spacecraft.

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The civil line matured with Salyut 6 , launched in September 1977, and Salyut 7 in April 1982. Each had two docking ports, so a long-stay crew could receive visitors and, from January 1978, the uncrewed Progress freighter, which brought fuel, air, water and food and then burned up full of rubbish; its descendants still fly to the International Space Station. Salyut 6 hosted sixteen crews and, under the Interkosmos programme, the first spacefarers from neither superpower: Vladimír Remek of Czechoslovakia in March 1978, then Poland's Mirosław Hermaszewski, East Germany's Sigmund Jähn, Vietnam's Phạm Tuân, Cuba's Arnaldo Tamayo Méndez and others. France's Jean-Loup Chrétien and India's Rakesh Sharma followed on Salyut 7, where the stay record reached 237 days in 1984. The record sits in the logs of TsUP, the control centre outside Moscow.

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Salyut 7's finest hour came after it died. In February 1985 the empty station's electrics failed and it fell silent, drifting and freezing. In June, Vladimir Dzhanibekov and Viktor Savinykh flew Soyuz T-13 to it, docked by hand with a laser rangefinder, and found the cabin dark, freezing and furred with frost. In fur hats, they recharged the batteries from Soyuz, thawed the water tanks and had the station alive within a week. The Salyuts taught everything the later stations knew: docking modules together, robot resupply, months in a tin can, and what it costs to get it wrong.

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The Space Shuttle

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On 12 April 1981, twenty years to the day after Gagarin, John Young and Bob Crippen rode Columbia off Pad 39A on the first flight of a vehicle nobody had flown before, not even uncrewed. The Space Shuttle was three things bolted together: a delta-winged orbiter the size of a DC-9 airliner, 37 metres long with a 24-metre wingspan; a 47-metre external tank holding about 720 tonnes of liquid hydrogen and oxygen; and two solid rocket boosters , each 45 metres tall and giving around 12 million newtons of thrust. At lift-off the stack weighed about 2,000 tonnes, and the boosters supplied most of the push for the first two minutes before splashing down under parachutes to be reused.

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The orbiter's three RS-25 engines, fed from the tank, ran for eight and a half minutes at a nominal "104 per cent" of their original rating, a label kept after the engines were uprated and never renamed. The tank was discarded to burn up; the orbiter carried up to about 24 tonnes in a payload bay 18 metres long and 4.6 metres wide, and could bring cargo home. Re-entry at Mach 25 was survived by about 24,000 silica tiles, each individually shaped and numbered, with reinforced carbon-carbon panels on the nose and wing leading edges, where the heat reached around 1,600 degrees Celsius. Landing was a 350-kilometre-an-hour glide with no engines and no second chance.

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The record is in NASA's mission archive: 135 flights by five orbiters, Columbia , Challenger , Discovery , Atlantis and Endeavour , carrying 355 individuals from 16 countries. The Shuttle launched and then fixed the Hubble Space Telescope, repaired Solar Max in 1984 in the first on-orbit satellite service, caught the stranded Intelsat VI in 1992 with three astronauts holding it by hand, flew Europe's Spacelab laboratory from 1983 with Germany's Ulf Merbold aboard, docked nine times with Mir and delivered most of the International Space Station. Canada's robotic arm, flying from the second mission in November 1981, made much of that possible.

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The promise was different from the product. In 1972 the Shuttle was sold as routine, airline-like access to orbit, with dozens of flights a year and turnarounds measured in weeks. The busiest year, 1985, saw nine launches; a typical turnaround took months, and the tiles and engines needed inspection after every flight. The Air Force's demand for a large cross-range gave the orbiter its big wings and much of its weight. And two of the five orbiters were lost with their crews, fourteen people in all.

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Atlantis rolled to a stop at Kennedy at dawn on 21 July 2011, the 135th and final landing, after thirty years that no later vehicle has matched for versatility and none has wished to copy. The capsules that replaced it are simpler, cheaper and safer. The Shuttle remains the only machine that ever carried people, built a station and brought a satellite home in the same hold.

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Challenger

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At 11:38 on the morning of 28 January 1986, Challenger lifted off from Kennedy Space Center into air just above freezing, the coldest launch in Shuttle history. Seventy-three seconds later, about 14 kilometres up, it broke apart. Aboard were Dick Scobee, Michael Smith, Ellison Onizuka, Judith Resnik, Ronald McNair, Gregory Jarvis and Christa McAuliffe , a teacher from New Hampshire chosen from 11,000 applicants for the Teacher in Space project. Schools across America were watching.

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The cause was known before the flight. Each solid rocket booster was built in segments, and the joints between them were sealed by two rubber O-rings that had to flex into place in the first fraction of a second of ignition; cold rubber is stiff. On the evening of 27 January, with temperatures forecast to fall well below freezing overnight, engineers at the booster maker Morton Thiokol, among them Roger Boisjoly and Arnie Thompson, argued in a teleconference with NASA that the launch should wait until the joints had warmed to at least 12 degrees Celsius, the coldest they had ever flown, on a flight that had already shown scorching. NASA managers pushed back; Thiokol's executives went off the line, overruled their engineers and signed off the launch. The right booster's aft joint was at about minus 2 degrees at lift-off.

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Film from the pad cameras told the rest. At 0.68 seconds, puffs of black smoke left that joint as the O-rings failed to seal; slag from the burning propellant plugged the gap for a while. At 58 seconds, after the strongest wind shear of any Shuttle flight, a flame appeared at the joint. It burned through the strut holding the booster to the external tank; the booster swung, struck the tank, the hydrogen tank failed and aerodynamic forces tore the vehicle apart at nearly twice the speed of sound. It did not explode in the usual sense: the fireball was propellant burning in the open. The crew cabin stayed intact and fell for two minutes and forty-five seconds into the Atlantic.

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The Rogers Commission , with Neil Armstrong and Sally Ride among its members, reported in June 1986 that the joint was flawed and that NASA and Thiokol had known for years, accepting each scorched O-ring because the last one had not killed anyone. The sociologist Diane Vaughan later called the habit "normalisation of deviance". Feynman's own appendix ended: "For a successful technology, reality must take precedence over public relations, for nature cannot be fooled."

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The fleet was grounded for 32 months while the joints were redesigned with a third O-ring, a capture lip and heaters, the crew got pressure suits and a bail-out pole, and commercial satellites left the Shuttle for good; Discovery flew again on 29 September 1988. Barbara Morgan, McAuliffe's backup, reached orbit in 2007. Challenger is taught in every engineering school as the case where the data were in the room and the launch went ahead anyway.

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Mir

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Mir means peace, and also world, and also the old Russian word for a village community; the station lived up to all three. Its core module, a 20-tonne Salyut descendant with a six-port docking node at the front, was launched by Proton on 20 February 1986, three weeks after Challenger . Over the next decade the Soviet Union, and then Russia, bolted on Kvant-1 (1987, astrophysics), Kvant-2 (1989, an airlock and a shower), Kristall (1990, materials furnaces and two ports for a shuttle that would be Buran and turned out to be Atlantis ), Spektr (1995) and Priroda (1996), plus a docking module delivered by the Americans. The finished station massed about 130 tonnes and sprawled over 30 metres, the first spacecraft assembled in orbit from pieces launched years apart.

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Life aboard was long. Mir was permanently crewed from 1989 to 1999, and in all it hosted more than a hundred people from a dozen countries, including Britain's Helen Sharman in 1991 and Japan's Toyohiro Akiyama, a journalist whose television network paid for his seat. Sergei Krikalev launched a Soviet citizen in May 1991 and landed a Russian one in March 1992, his stay doubled by the collapse of the country that sent him. Valeri Polyakov's 437 days in 1994 and 1995 remain the longest single spaceflight.

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The Cold War ended in Mir's docking node. Under the Shuttle-Mir programme, Atlantis docked on 29 June 1995, forming for five days the largest spacecraft ever flown, about 225 tonnes; nine Shuttle dockings followed and seven NASA astronauts lived aboard for months, Shannon Lucid for 188 days. The Americans learned long-duration operations from the Russians; the Russians received hard currency that kept their programme alive.

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1997 nearly ended it. On 23 February a lithium-perchlorate oxygen canister in Kvant-1 caught fire and burned like a blowtorch for about fourteen minutes while six people, including NASA's Jerry Linenger, put on masks and considered which Soyuz to flee in. On 25 June a Progress freighter, being flown in by hand on a television link during a docking test, struck Spektr and punctured it; Aleksandr Lazutkin cut cables and sealed the hatch as the pressure fell, and Michael Foale, Vasili Tsibliyev and Lazutkin lived on with Spektr's solar arrays, nearly half the station's power, cut off for good. The accounts are in the crew's debriefs and in Linenger's and Foale's own books.

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By then the station was tired: mould on the walls, condensation behind panels, computers that crashed and left it tumbling. On 23 March 2001 a final Progress fired its engines and Mir came down over the South Pacific near Fiji, 86,331 orbits after launch, in a shower of fragments watched from the beaches. It had shown how to build a home in orbit piece by piece, and how to keep it alive when the pieces failed.

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Columbia

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Columbia , the oldest orbiter, launched on 16 January 2003 on STS-107, a sixteen-day science mission with a laboratory module in its bay and a crew of seven: Rick Husband, William McCool, Michael Anderson, David Brown, Kalpana Chawla, Laurel Clark and Ilan Ramon, Israel's first astronaut. Eighty-two seconds after lift-off a piece of insulating foam about the size of a briefcase broke from the external tank's left bipod ramp and struck the leading edge of the left wing at roughly 240 metres per second. The launch cameras caught it. Nobody aboard felt it.

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Foam had fallen off the tank on most flights without bringing an orbiter down, so the strike was logged as a maintenance concern rather than a threat. Engineers in the Debris Assessment Team asked three times for military telescopes or satellites to photograph the wing; the Mission Management Team, which did not consider the strike a safety-of-flight issue, declined. On day two an Air Force radar had tracked a small object drifting away from the orbiter, later judged to be part of the wing's reinforced carbon-carbon panel; nobody connected it at the time. The crew was told of the strike in an email and reassured.

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On 1 February Columbia began re-entry over the Pacific at 8:44 Eastern time. From 8:53, as it crossed California at Mach 23, sensors in the left wing began to fail one by one, then the left landing-gear tyre pressures, then the hydraulic lines; superheated gas was pouring through a hole in panel 8 and melting the wing from inside. At 8:59:32 Mission Control lost contact at about 61 kilometres over Texas, and the orbiter broke apart at eighteen times the speed of sound. Some 84,000 pieces were later recovered across Texas and Louisiana by 25,000 searchers, among them a videotape of the cabin in the early minutes of entry.

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The Columbia Accident Investigation Board , chaired by Admiral Harold Gehman, reported in August 2003. On 7 July its engineers had fired a foam block from a nitrogen gun at a real wing panel and blown a hole 40 centimetres across, settling the physical cause. The organisational one was familiar: schedule pressure, a management chain that silenced engineers, and a culture that had learned to accept foam strikes as normal, "echoes of Challenger" in the board's words. The report recommended that the Shuttle be recertified or retired by 2010.

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Discovery returned to flight on 26 July 2005 under Eileen Collins, with the tank redesigned, a 15-metre inspection boom, a back-flip under the International Space Station so its crew could photograph the belly, and a second orbiter standing by for rescue. The tank still shed foam, and the fleet was grounded again for a year. In January 2004 the White House had already decided: finish the station, then retire the Shuttle. Columbia's seven changed what came next for everyone who followed.

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Building the ISS

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The International Space Station began as two spacecraft from opposite sides of the Cold War meeting 400 kilometres up. Zarya , a 19-tonne Russian-built module paid for by NASA, rode a Proton out of Baikonur on 20 November 1998. Two weeks later Endeavour brought the American node Unity , and on 6 December the crew of STS-88 pulled the two together with the Shuttle's robotic arm and bolted them with a hundred-odd cable connections over three spacewalks. For eighteen months the pair circled empty while Russia finished Zvezda , the service module with the living quarters, life support and engines, launched in July 2000. Its pressure hull had been built in the mid-1980s as the core of the never-flown Mir-2.

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Expedition 1, Bill Shepherd, Yuri Gidzenko and Sergei Krikalev, arrived by Soyuz on 2 November 2000 and kept a ship's log in the naval style; the station has not been empty since. The design they were building was the 1993 merger of Reagan's Space Station Freedom with Mir-2, under a partnership of fifteen nations: the United States, Russia, Canada, Japan and eleven members of the European Space Agency. Each paid in kind. Italy built the American nodes Harmony and Tranquility and the seven-windowed Cupola in exchange for research time; Canada built the 17.6-metre Canadarm2 and the two-armed robot Dextre ; Japan built Kibo, the largest laboratory; Europe built Columbus.

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The order was a puzzle in logistics. The American laboratory Destiny came in February 2001, Canadarm2 in April, the airlock Quest in July; the first truss segment and the first giant solar wing had gone up in late 2000. Then Columbia was lost, and for two and a half years only Soyuz and Progress flew, with the crew cut to two to save supplies. Assembly resumed in 2005. Harmony arrived in 2007, Columbus on 7 February 2008, Kibo in three deliveries in 2008 and 2009, Tranquility and the Cupola in February 2010. The flight-by-flight record is NASA's assembly sequence, revised dozens of times.

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The finished structure, declared complete in 2011 after the last Shuttle deliveries, is about 420 tonnes, 109 metres from one end of the truss to the other and 73 metres along the line of modules, with eight solar wings covering some 2,500 square metres and a pressurised volume of about 900 cubic metres, roughly a Boeing 747. It took more than 40 assembly flights and around 160 spacewalks, the most concentrated spacewalking in history. Russia's Nauka laboratory joined late, in July 2021, and new roll-out solar arrays have been added since.

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The station is the largest thing humans have built in space and the most expensive single object ever made, and it exists because the Shuttle could carry the pieces and because former enemies agreed to depend on one another's hardware. Its successors, planned to be commercial, will be smaller. None will be built the way this one was.

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Life Aboard the ISS Today

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The International Space Station circles the Earth about 400 kilometres up at 27,600 kilometres an hour, once every 93 minutes, so its crew of seven sees roughly sixteen sunrises a day and lives on Greenwich time, a compromise between Houston and Moscow. It has been inhabited without a break since 2 November 2000, by more than 280 people from more than twenty countries. The day runs by a timeline sent up from the ground: about six and a half hours of science and maintenance, two hours of exercise to hold off bone and muscle loss, meals from pouches, and a sleeping bag strapped to a wall in a phone-booth-sized cabin.

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Keeping seven people alive is plumbing. Oxygen is split from water by electrolysis; the carbon dioxide they breathe out is scrubbed and, in a Sabatier reactor, turned back into water; urine and cabin humidity are distilled and filtered until, since 2023, about 98 per cent of the water aboard is recycled. The rest arrives by freighter. Russia's Progress has flown since 1978; SpaceX's cargo Dragon , from 2012, is the only one that brings experiments back down; Northrop Grumman's Cygnus burns up full of rubbish; Japan's HTV-X, successor to the Kounotori, made its first delivery in late 2025. Crews ride Soyuz MS or Crew Dragon. Boeing's Starliner reached the station in June 2024 but came home empty after thruster faults, leaving Butch Wilmore and Suni Williams aboard for 286 days instead of eight; they returned on a Dragon in March 2025.

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The station must also be flown. Thin air at that altitude drags it down by a kilometre or two a month, so a Progress or Zvezda's engines reboost it several times a year. When tracked debris threatens, controllers nudge the orbit: about forty avoidance manoeuvres since 1999, and sometimes a crew sheltering in their return craft. Since 2019 a tunnel at the back of Zvezda has leaked air through fine cracks; by 2024 the rate had reached more than a kilogram a day, the hatch is kept shut, and NASA's inspector general listed it as a top risk.

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Four control rooms share the shift: Houston for the American segment, the TsUP outside Moscow for the Russian one, Munich's Columbus Control Centre and Tsukuba for Kibo, with Canada's robotics team near Montreal flying the arm. How we know all this is the daily status report NASA has published for every day of every expedition, and the audited inspector-general reports that count the leaks and the spares.

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The end is scheduled. The partners have committed to operate the station to 2030, and in 2024 NASA chose SpaceX to build a deorbit vehicle, a heavily modified Dragon with 46 thrusters, to steer 420 tonnes into the South Pacific around 2031. Until then it remains what it has been for a quarter of a century: the one address in the universe that is never unoccupied.

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Tiangong

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China was never invited aboard the International Space Station. In 2011 the United States Congress passed the Wolf Amendment, barring NASA from bilateral cooperation with China, so China built its own. Tiangong , "heavenly palace", is the only other crewed station in orbit, and the first ever built by a single country alone.

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It was approached in steps. Tiangong-1 , an 8.5-tonne test laboratory, launched in September 2011 and received the uncrewed Shenzhou 8, then Shenzhou 9 in June 2012 with Liu Yang, China's first woman in space, and Shenzhou 10 in 2013, from which Wang Yaping gave a physics lesson to 60 million schoolchildren. It fell back uncontrolled into the South Pacific in 2018. Tiangong-2 followed in 2016 and tested refuelling by the first Tianzhou cargo ship in 2017. Then came the real thing: the Tianhe core module, 22.5 tonnes and 16.6 metres long, launched from Wenchang on a Long March 5B on 29 April 2021. Its twenty-tonne core stage fell back uncontrolled ten days later into the Indian Ocean, as it did after both laboratory launches, drawing protests from NASA and debris over Borneo.

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Wentian docked in July 2022 and Mengtian in October, each about 23 tonnes, each swung from the forward port to a side port by a robotic arm to make a T about 55 metres across. Tianhe holds the crew quarters, the controls and the main 10-metre arm, which can inch along the hull hand over hand; Wentian carries life-science racks, a second airlock for spacewalks and a smaller arm; Mengtian carries materials and physics racks and a cargo airlock that pushes small satellites out. The complex masses about 100 tonnes, a fifth of the ISS, with 110 cubic metres of living space for three, and flies at around 390 kilometres inclined 41.5 degrees. Its orbit is held by four Hall-effect electric thrusters, the first on any crewed station.

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Crews of three have rotated every six months since Shenzhou 12 in June 2021, overlapping for a week at handover. Shenzhou 13 brought Wang Yaping back for China's first spacewalk by a woman; by 2025 the station had hosted its tenth resident crew and several hundred experiments, from rice grown seed to seed to a cold atom clock. In November 2025 it also had its first emergency: a return capsule window suspected cracked by debris, a crew sent home in another ship, and an uncrewed Shenzhou launched in a hurry as a replacement lifeboat.

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The station is opening up. The 2-metre Xuntian survey telescope is planned to fly alongside and dock for servicing; a further module with extra ports is planned; and in 2025 China agreed to train Pakistani astronauts, the first foreign guests, with other countries lining up. When the ISS comes down around 2030, Tiangong may for a time be the only permanent human address in space, run by the one nation that was told to stay outside.

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Space Tourists and Private Crews

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The first person to buy a seat into orbit was not an American millionaire but a Japanese television journalist. In December 1990 the Tokyo Broadcasting System paid for Toyohiro Akiyama to spend a week on Mir , broadcasting nightly; Britain's Helen Sharman followed in 1991 on a flight that began as a commercial venture. The pattern was set: a cash-starved Russian programme sold what NASA would not.

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Dennis Tito , a Californian engineer turned investment manager, booked through the broker Space Adventures and launched on Soyuz TM-32 on 28 April 2001 for eight days on the International Space Station, over NASA's loud objections. Six more clients followed on Soyuz through 2009, among them Anousheh Ansari, the first woman to pay her own way, and Charles Simonyi, who went twice. The seats dried up when the Shuttle retired and NASA needed every Soyuz berth; they reopened in December 2021 with the Japanese billionaire Yusaku Maezawa.

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Suborbital tourism arrived in a single fortnight. On 11 July 2021 Richard Branson rode Virgin Galactic's rocket plane VSS Unity to 86 kilometres, above the 80-kilometre line the United States counts as space; on 20 July Jeff Bezos's New Shepard capsule carried four, including 82-year-old Wally Funk, to 107 kilometres, past the 100-kilometre Kármán line that most of the world uses. Each gave a few minutes of weightlessness and a view of the curve of the Earth; New Shepard has since flown dozens of passengers, William Shatner at 90 among them.

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Orbit returned to private hands with Inspiration4 in September 2021: Jared Isaacman chartered a Crew Dragon, filled it with three people who were not professionals, including Hayley Arceneaux, a childhood cancer survivor flying with a prosthesis, and spent three days at 585 kilometres, higher than the station, under a glass cupola. Axiom Space then began selling whole missions to the ISS: Ax-1 in 2022 under the veteran Michael López-Alegría, Ax-2 with the first Saudi woman in orbit, Ax-3 with Turkey's and Sweden's astronauts, and Ax-4 in June 2025, which carried India's Shubhanshu Shukla, Poland's Sławosz Uznański-Wiśniewski and Hungary's Tibor Kapu, each nation's first spacefarer in decades.

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That flight, Polaris Dawn , had two days earlier reached 1,400 kilometres, the farthest from Earth anyone had travelled since Apollo 17, and tested SpaceX's new suit. In April 2025 Fram2 , chartered by a Maltese entrepreneur, Chun Wang, flew the first humans over the poles in a 90-degree orbit, with Germany's Rabea Rogge and a Norwegian film-maker and an Australian polar guide aboard. The records are SpaceX's, Axiom's and NASA's, and the flight surgeons' papers that followed.

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Whether these people are tourists, private astronauts or customers is argued about. The numbers are not: more than a hundred people have now flown as paying or sponsored passengers, and the first crews with no government employee aboard have gone higher than the station, over the poles and out of the hatch. The next step is somewhere for them to stay.

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The Stations to Come

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Around 2030 the International Space Station will be steered into the ocean, and what replaces it exists so far on paper. The partners have agreed to fly to 2030; Russia, which once threatened to leave earlier, has signed on to 2028 and is designing its own station; and NASA plans to stop owning a station and start renting rooms.

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That policy is the Commercial LEO Destinations programme. In 2021 NASA gave early funding to Orbital Reef , led by Blue Origin with Sierra Space's inflatable habitats, and to Starlab , from Voyager and Airbus, a single 8-metre-wide module designed to launch complete on one Starship. Separately, Axiom Space won the right to attach its own modules to the ISS's forward port, the first a power-and-thermal module planned for 2027, to be detached as a free-flying station before the ISS comes down. Vast 's Haven-1, a single 45-cubic-metre module for four visitors on two-week stays, is planned to launch on a Falcon 9 and would be the first commercial station if it flies on time. In 2025 NASA reset the programme's second phase around funded agreements and a minimum of four crew for month-long stays. All the dates are "planned": none of these habitats has yet reached orbit.

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Other nations are not waiting for the market. Roscosmos approved its Russian Orbital Station in 2024, with a first science-and-power module planned around 2027 and a steep 97-degree orbit that would overfly the whole of Russia, something the ISS never does. India's Bharatiya Antariksh Station is to begin with a module planned for 2028 and grow to five modules of about 52 tonnes by 2035, following the first crewed Gaganyaan flights. China plans a further Tiangong module with more docking ports. Beyond Earth orbit the lunar Gateway , a small station in a looping orbit around the Moon with modules from NASA, Europe, Japan, Canada and the United Arab Emirates, had its first elements under construction when, in 2025, the White House proposed cancelling it; its future has been argued since.

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What is lost when the ISS falls is not mainly hardware. It is the only laboratory where experiments have run for a quarter of a century under one roof, the habit of fifteen nations depending on one another's parts, and the unbroken human presence off the planet since November 2000. NASA's auditors have warned of a gap between the station's end and any replacement, during which only Tiangong would be inhabited. What stays is the knowledge: how to recycle 98 per cent of your water, how to live a year in free fall, how to dock a ship built on another continent.

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The stations to come will be smaller, more numerous and privately owned, with agencies as tenants and tourists as guests. Whether they are built in time is the open question of the decade. Humans have had a home in orbit for over fifty years; the next few will decide whether we keep one.

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Telstar and the Satellite Age

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In October 1945 a young RAF radar officer named Arthur C. Clarke published a four-page article in Wireless World called "Extra-Terrestrial Relays". It pointed out that a satellite 35,786 kilometres above the equator would circle the Earth in exactly one day and so appear to hang motionless in the sky; three of them, spaced evenly, could relay radio to the whole planet. He later joked that he should have patented it. The geostationary orbit is still called the Clarke orbit, and most of the television beamed to rooftop dishes today comes down from it.

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The first experiments were humbler. Echo 1, launched on 12 August 1960, was a 30-metre balloon of aluminised plastic film that simply bounced signals back; it carried a recorded message from President Eisenhower and was bright enough to be seen from the ground. Active relay came with Telstar 1 , built by Bell Telephone Laboratories and launched on a Thor-Delta on 10 July 1962. It weighed 77 kilograms, measured 88 centimetres across, and flew an elliptical orbit between about 950 and 5,900 kilometres, so it was in view of both sides of the Atlantic for only around 20 minutes per pass. That evening it carried the first live transatlantic television picture, the flag outside the Andover ground station in Maine, received at Pleumeur-Bodou in Brittany and, after a frantic adjustment, at Goonhilly Downs in Cornwall, where the 26-metre dish "Arthur" still stands. The Tornados' instrumental…

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Low orbits meant short, interrupted sessions. Hughes engineer Harold Rosen's answer was Clarke's orbit in practice: Syncom 2 reached a geosynchronous orbit in July 1963 and Syncom 3, launched on 19 August 1964, became the first truly geostationary satellite, relaying the opening of the Tokyo Olympics to American screens that October. Intelsat I, nicknamed Early Bird, followed on 6 April 1965 with 240 telephone circuits or a single television channel, and commercial transatlantic satellite service began. The Soviet Union, whose territory sits too far north for a good view of the equator, chose instead the highly elliptical Molniya orbit , launched from April 1965, which lingers for hours over the northern hemisphere on each twelve-hour loop.

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Today the Clarke orbit is crowded with several hundred working satellites, each parked in a slot assigned by the International Telecommunication Union. Direct-to-home television, Inmarsat's distress and safety service for ships, and the relays that carry weather images from geostationary observers all live there. Telstar's twenty-minute windows have become a planetary utility, and the orbit a 1945 radar officer sketched in a hobby magazine is now real estate.

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Weather from Above

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On 1 April 1960 a 122-kilogram drum called TIROS-1 rose from Cape Canaveral carrying two television cameras, and within hours meteorologists were looking at something no one had seen before: whole cloud systems, spiral storms and fronts stretching across thousands of kilometres. The satellite worked for only 78 days and returned about 23,000 pictures, many of them of the top of the spacecraft, but the point was made. Weather had been forecast from scattered station reports and balloon soundings; now it could be watched.

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Two families of satellite grew from that start. Polar orbiters pass over the poles about 850 kilometres up, crossing each point on Earth twice a day and seeing everything, including the empty oceans where storms are born. Nimbus 3 in 1969 carried the first infrared sounder, measuring temperature through the depth of the atmosphere rather than just photographing its top. Today NOAA's JPSS satellites, Europe's MetOp series, China's Fengyun-3 and Russia's Meteor-M share the work. Geostationary satellites, parked 35,786 kilometres above the equator, watch one hemisphere continuously; the spin-scan camera that made this possible was built by Verner Suomi of the University of Wisconsin and flew on ATS-1 in 1966. GOES-1 followed in 1975, Japan's Himawari in 1977 and Europe's Meteosat-1 on 23 November 1977. The latest GOES carries a lightning mapper that counts flashes across the Americas…

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The decisive change came when satellite measurements were fed into numerical models. The European Centre for Medium-Range Weather Forecasts began operational forecasting in 1979 and now assimilates tens of millions of observations a day, well over ninety per cent of them from satellites: temperature and humidity soundings, winds inferred from cloud drift, sea-surface wind speed from the radar scatterometers on MetOp. The result is what meteorologists call a quiet revolution: forecast skill has gained roughly a day per decade, so a modern five-day forecast is about as reliable as a two- or three-day forecast was around 1980. We know this because every forecast is scored against what happened, and the verification archives go back decades.

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Hurricanes show the gain most plainly. In August 1969 satellite pictures of Camille showed a compact, ferocious storm, but its landfall on Mississippi was still a surprise to many. In 2005 Katrina's track and intensity were forecast more than two days ahead, within tens of kilometres of the actual landfall, time enough to empty much of New Orleans. India's cyclone warnings, built on its INSAT satellites, have cut death tolls from the tens of thousands in Odisha in 1999 to dozens in storms of equal strength since.

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A satellite image on the evening news is now so ordinary that we forget it was once a miracle. Behind it stands a global observing system that is one of the few genuinely shared pieces of infrastructure on Earth: no country's forecast works without everyone else's satellites.

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Landsat and Watching the Land

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On 23 July 1972 a Delta rocket from Vandenberg put the Earth Resources Technology Satellite into a 900-kilometre polar orbit. Renamed Landsat 1 , it carried a television camera system that soon failed and an experimental instrument that did not: the Multispectral Scanner, designed by Virginia Norwood at Hughes, which swept a mirror across a 185-kilometre swath and recorded the ground in four colours, two of them infrared, at about 80 metres per pixel. Plants reflect near-infrared light strongly, so for the first time crops, forests and bare soil could be told apart over whole countries, every 18 days. The record that began that day has never stopped.

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Each generation sharpened the view. Landsat 4 in 1982 introduced the Thematic Mapper with 30-metre pixels and seven bands, the resolution that still defines the series; Landsat 7 in 1999 added a 15-metre panchromatic channel; Landsat 8 in 2013 and Landsat 9, launched on 27 September 2021, carry pushbroom sensors that image the whole planet every eight days between them. Landsat 6 never reached orbit in 1993, and Landsat 5, designed for three years, worked for nearly 29, a record for an Earth-observing satellite. More than ten million scenes sit in the archive at the United States Geological Survey in Sioux Falls, South Dakota.

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For its first 36 years the archive was sold by the scene, and researchers bought a handful. In 2008 the USGS made every image free , and the field changed overnight: downloads rose from a few thousand scenes a year to millions, and scientists began to treat the archive as a time machine rather than a photograph. Matthew Hansen's team at the University of Maryland processed 650,000 scenes to map every forest gain and loss on Earth between 2000 and 2012 at 30-metre resolution. Brazil's space agency INPE had already been using Landsat since 1988 to measure Amazon clearing each year, the fishbone pattern of roads and fields in Rondônia visible from orbit before any inspector reached it.

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The most famous sequence is the Aral Sea. In 1960 it was the fourth-largest lake on Earth; Soviet irrigation canals took the rivers that fed it, and Landsat images from 1977 onwards show the shoreline retreating year by year until, in 2014, the eastern basin was dry for the first time in modern history. Europe joined the long record with Copernicus Sentinel-2A in June 2015 and 2B in 2017, imaging at 10 metres every five days in 13 bands, also free. India's Resourcesat series and the hundreds of small Dove satellites flown by Planet, which photograph the entire land surface daily at about three metres, fill in the gaps.

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A single satellite picture tells you what a place looks like. Fifty-three years of them tell you what it is becoming, and that is a record no nation can now afford to interrupt.

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GPS: Where Everything Is

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Within days of Sputnik's launch in October 1957, two physicists at the Johns Hopkins Applied Physics Laboratory, William Guier and George Weiffenbach, found they could work out the satellite's orbit from the Doppler shift of its beeps. Their boss asked the reverse question: could a known orbit fix an unknown position on the ground? The answer became Transit , operational from 1964, which told Polaris submarines where they were every hour or so. Its limitation, a fix only when a satellite passed overhead, drove the next idea: enough satellites, with clocks good enough, that four would always be in view.

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The Global Positioning System was approved in 1973 under Air Force Colonel Bradford Parkinson, drawing on Roger Easton's timing work at the Naval Research Laboratory and the orbital models of mathematician Gladys West. The first Navstar satellite flew on 22 February 1978, and the constellation was declared fully operational on 17 July 1995: 24 satellites in six planes, 20,200 kilometres up, circling twice a day. Each carries atomic clocks and broadcasts the time and its own position. A receiver notes when each signal arrives; since radio travels about 30 centimetres in a nanosecond, the delay gives the distance. Three distances fix a point, and a fourth satellite corrects the receiver's cheap quartz clock. The signal that reaches the ground is astonishingly faint, comparable to a light bulb seen from 20,000 kilometres.

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Einstein is built into every fix. Moving at 3.9 kilometres a second, the satellite clocks run slow by about 7 microseconds a day; sitting higher in Earth's gravity, they run fast by about 45. The net 38 microseconds a day would, uncorrected, drift positions by about ten kilometres daily, so the clocks are set to tick slightly slow before launch.

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The system was military until a tragedy. On 1 September 1983 a Soviet fighter shot down Korean Air Lines Flight 007, a Boeing 747 that had strayed into Soviet airspace through a navigation error, killing 269 people. President Reagan announced that GPS would be made available to civil aviation. Civil signals were still deliberately blurred to about 100 metres by Selective Availability until President Clinton switched it off at midnight on 1 May 2000; accuracy improved tenfold overnight, and the satnav, the phone map and the ride-hailing app followed. Other powers built their own: Russia's GLONASS, Europe's Galileo, operating since 2016, China's BeiDou, completed in June 2020, plus regional systems in Japan and India. Most phones now listen to all of them.

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The weakness is the faintness. Jamming and spoofing of GPS around the Baltic, the Black Sea and the Middle East have disrupted thousands of flights since 2022, and ships have found themselves apparently parked at inland airports. A free signal from 20,000 kilometres quietly rebuilt the world's logistics, farming, finance and timing; losing it, even briefly, now shows how much rests on it.

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Spy Satellites

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On 19 August 1960 a C-119 transport aircraft over the Pacific near Hawaii flew a trapeze into the parachute lines of a falling gold-plated capsule and reeled it aboard. Inside was a reel of film from Discoverer 14 , the first successful mission of the CIA and Air Force programme code-named Corona . That single bucket covered more of the Soviet Union than all the U-2 spy plane flights put together, at a time when U-2s had become too dangerous: Francis Gary Powers had been shot down over Sverdlovsk in May. For the first time, a country could look inside another from a place no fighter could reach.

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Corona's cameras photographed strips of ground onto 70-millimetre film, which was wound into a re-entry capsule, dropped over the ocean and caught in the air or fished from the sea. Early pictures resolved objects about 8 metres across; by the KH-4B cameras of the late 1960s that had improved to under two metres. Over 145 missions to 1972 the programme returned more than 800,000 images. Its first great result was negative: the "missile gap" that had alarmed Washington turned out not to exist. By September 1961 American analysts counted a few dozen Soviet intercontinental missiles, not the hundreds feared. The Soviet Union answered with Zenit , a reconnaissance camera packed into a Vostok capsule, flying from 1962 under the anonymous Kosmos label and returning its whole camera to Earth; more than 500 were launched before the series ended in 1994.

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Film has one flaw: you must wait for it to fall. The KH-11, first launched on 19 December 1976, carried a charge-coupled device instead and sent its pictures down by radio through relay satellites, so an analyst could see a Soviet shipyard within hours. Its 2.4-metre mirror was the same size as Hubble's, built at the same time by the same industry; in 2012 the National Reconnaissance Office handed NASA two spare telescopes of that class, one of which became the Nancy Grace Roman Space Telescope. The NRO itself, founded in 1961, had its existence officially admitted only in 1992, and Corona's imagery was declassified in February 1995, when historians and geographers found a 1960s baseline for everything from Siberian forests to Middle Eastern archaeology.

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Signals-intelligence satellites listen alongside the cameras, collecting radio traffic from geostationary orbit. And the view is no longer only governmental. In February 2022 commercial images from Maxar showed the world a Russian military convoy more than 60 kilometres long approaching Kyiv, and Planet's and Capella's satellites tracked the war daily; what had once taken a presidential finding could be bought by a newspaper.

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Spy satellites did not end secrecy, but they changed its scale. Nothing larger than a car can be hidden for long, and both the arms-control treaties of the Cold War and the open-source analysts of today rest on that fact.

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Measuring the Planet's Pulse

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The most important climate measurement of the past thirty years is a few millimetres long. TOPEX/Poseidon , launched by NASA and France's CNES on 10 August 1992, bounced radar pulses off the ocean from 1,336 kilometres up and timed the echo to measure the height of the sea surface to within a few centimetres on each pass. Averaged over the globe and over months, the errors shrink and the trend appears. Its successors Jason-1, Jason-2, Jason-3 and Sentinel-6 Michael Freilich have flown the same ground track ever since, and the record is unambiguous: the global sea has risen about ten centimetres since 1993, at roughly 3 millimetres a year on average and more than 4 a year now. Tide gauges had hinted at it for a century; the satellites made it a single global number.

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Where does the water come from? GRACE , a German-American pair launched on 17 March 2002, answered by weighing the planet. The two satellites flew 220 kilometres apart on the same orbit and measured the distance between them to a few microns with a microwave link; when the leading one passed over a mass, Greenland's ice, say, or the Ganges basin aquifer, it was tugged ahead and the gap stretched. Month by month, GRACE and its 2018 successor GRACE-FO have tracked Greenland losing around 270 billion tonnes of ice a year and groundwater vanishing under northern India and California's Central Valley. ICESat-2, launched in September 2018, fires 10,000 green laser pulses a second and times single photons back, mapping ice height to a few centimetres.

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The atmosphere has its monitors too. NASA's Terra, launched in 1999, and Aqua, in 2002, lead a train of satellites crossing the equator in the early afternoon, measuring clouds, aerosols, fires and the radiation budget. OCO-2 , launched on 2 July 2014, maps carbon dioxide to better than one part per million from orbit, showing emissions plumes over cities and the breathing of the forests. SMAP, from 2015, reads soil moisture with a microwave radiometer; its radar failed after three months, which is how we know radar amplifiers are harder than radiometers. Europe's Copernicus Sentinel-1 radar images the ground day and night through cloud, catching subsidence, floods and glacier flow, while ESA's Earth Explorers each ask one question: GOCE mapped gravity, CryoSat-2 measures ice thickness, SMOS reads soil moisture and ocean salt, and EarthCARE, launched in 2024, profiles clouds with lidar…

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Climate science before 1992 argued from scattered thermometers, tide gauges and ice cores. It now argues from a continuous, global, physically calibrated record kept by instruments that no single government controls. Satellites did not create the climate problem, but they are the reason we can state its size to a decimal place.

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Fixing Hubble

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The Hubble Space Telescope left the payload bay of Discovery on 25 April 1990, the day after launch on STS-31, a school-bus-sized cylinder 13.2 metres long and weighing 11 tonnes, with a 2.4-metre primary mirror that had been polished for years. Lyman Spitzer had proposed a telescope above the atmosphere in 1946; Nancy Grace Roman had spent the 1960s and 1970s at NASA persuading astronomers and Congress to pay for it. Within weeks, the first star images came down as fuzzy haloes. The mirror had spherical aberration : its edge was too flat by about 2.2 microns, a fiftieth of the width of a human hair, and it could not bring light to one focus.

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The cause was found quickly and embarrassingly. A review board under Lew Allen reported in November 1990 that a measuring device at the manufacturer, Perkin-Elmer, had been assembled with a spacer out of place by 1.3 millimetres; the mirror had been polished precisely to the wrong shape, and two cruder tests that disagreed had been dismissed. Because the error was so exact, it could be cancelled. Engineer Jim Crocker, studying a folding shower head in a Munich hotel, saw how small corrective mirrors on arms could swing into the light path. COSTAR did that for three instruments, at the cost of the High Speed Photometer, and a new camera, WFPC2, carried its own correction ground into its optics.

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The repair, STS-61 aboard Endeavour , launched on 2 December 1993 after a year of underwater rehearsal. Over five spacewalks, a record at the time, Story Musgrave and Jeffrey Hoffman, Kathryn Thornton and Thomas Akers installed COSTAR and WFPC2, replaced the solar arrays that flexed every time the telescope crossed from night into day, and changed gyroscopes, with Claude Nicollier of ESA operating the robotic arm. The first corrected images in January 1994 were as sharp as the designers had promised, and the mission is still studied as the model for complex orbital servicing.

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Four more missions kept the telescope young. STS-82 in 1997 fitted the STIS spectrograph and NICMOS infrared camera; STS-103 in December 1999 replaced gyroscopes after the fourth of six failed and put Hubble into safe mode; STS-109 in 2002 added the Advanced Camera for Surveys and new arrays; and STS-125 in May 2009, cancelled after the Columbia loss and reinstated in 2006, installed Wide Field Camera 3, new batteries, six fresh gyroscopes, and repaired two instruments never designed to be opened in orbit. COSTAR itself was removed, its work done, and now sits in the Smithsonian.

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More than thirty-five years after launch, Hubble still observes, slower now and lower, its orbit slowly decaying from 600 kilometres towards an eventual re-entry. It is the first great telescope to have been repaired by hand in orbit, and the proof that a flaw in a mirror need not be the end of a machine.

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Unfolding Webb

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At 12:20 Universal Time on Christmas Day 2021 an Ariane 5 lifted off from Kourou in French Guiana carrying the James Webb Space Telescope , folded like origami inside a fairing 5.4 metres wide. The telescope had taken more than twenty years to build, involved more than 10,000 people in 14 countries, and was fourteen years past its original launch date. It was also the most complex deployment ever attempted: engineers counted 344 single-point failures , mechanisms that each had to work or the mission was lost, and none could be reached for repair. Webb was heading for a halo orbit around the second Lagrange point, L2 , 1.5 million kilometres from Earth.

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The unfolding began within half an hour, when the solar array opened as planned. Over the next fortnight a choreography was worked through from the control room at the Space Telescope Science Institute in Baltimore. On the third and fourth days the two pallets holding the sunshield swung down; on day five a tower extended 1.2 metres to separate the cold telescope from the warm spacecraft bus; on New Year's Eve two booms slid out to stretch the sunshield to its full 21 by 14 metres, roughly the size of a tennis court. Then came the step the engineers feared most: on 3 and 4 January 2022, motors drew 90 cables through pulleys to tension five layers of Kapton film, each thinner than a human hair, into separate, vacuum-gapped sheets. On 5 January the secondary mirror swung out on its tripod, and on 7 and 8 January the two wings of the primary mirror folded forward and latched, completing…

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The launch itself turned out to be a gift. Ariane 5 flew so accurately that Webb needed far less of its own propellant than planned for course corrections, and the fuel budget for station-keeping, which limits the mission's life, roughly doubled from ten years to twenty or more. In the shade of the sunshield the mirror cooled to around 40 kelvin, while the mid-infrared instrument was chilled by a cryocooler to 7 kelvin. Over the following three months the 18 segments, each adjustable to nanometres by seven actuators, were nudged until they focused as one; fine phasing was declared complete on 11 March 2022, and the mirror performed better than specification. A micrometeoroid larger than modelled struck segment C3 in May 2022 and left a permanent small error, now compensated by the others, and operators turned the telescope to keep its mirror out of the worst of the oncoming dust.

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Webb's first images were released on 12 July 2022. Every one of the 344 mechanisms had worked. It is the proof that a machine too far away to touch can be built so that it does not need touching.

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Space Junk

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In 1978 Donald Kessler and Burton Cour-Palais of NASA published a paper with a dull title, "Collision frequency of artificial satellites: the creation of a debris belt", and an alarming argument. Once enough objects share a band of orbit, collisions between them will produce fragments faster than the atmosphere drags them down, and the fragments will cause more collisions, a chain reaction that could make low Earth orbit unusable for generations. It is known as the Kessler syndrome . At the time there were a few thousand tracked objects. Today radar networks follow around 40,000 larger than ten centimetres, of which only some 11,000 are working satellites, and the European Space Agency estimates more than a million fragments bigger than a centimetre, each moving at around 7.5 kilometres a second.

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Three events built much of the cloud. On 11 January 2007 China destroyed its own retired weather satellite Fengyun-1C with a ground-launched missile at 865 kilometres, creating more than 3,000 tracked fragments where the air will take centuries to clear them. On 10 February 2009 the working Iridium 33 and the dead Russian Cosmos 2251 collided over Siberia at 789 kilometres, the first accidental collision of two satellites, adding around 2,300 pieces. On 15 November 2021 a Russian missile test shattered Cosmos 1408 at about 480 kilometres, and the crew of the International Space Station spent hours sheltering in their Soyuz and Dragon capsules as the fragments passed. The station has dodged debris dozens of times since 1999. The US Space Force and ESA publish the catalogues, and the Space Shuttle came home with its windows pitted; over the programme about a hundred cockpit panes were…

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Prevention came slowly. Guidelines from 2002 asked operators to remove satellites from low orbit within 25 years of the end of their mission; in September 2022 the US Federal Communications Commission cut that to five years for satellites it licenses. ESA's Zero Debris approach aims to leave nothing behind by 2030. Satellites now carry fuel for a final de-orbit burn or are flown low enough that drag does the work, and upper stages are vented so they cannot explode.

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Removal is harder, and just beginning. Japan's Astroscale launched ADRAS-J in February 2024 and flew it to within 15 metres of a dead H-IIA rocket stage, photographing it to plan a future capture. ESA's ClearSpace-1 is planned to grapple a derelict object with four robotic arms later this decade. China's Shijian-21 towed a dead BeiDou satellite into a graveyard orbit in January 2022, and other militaries noted that a tug able to move a dead satellite can also move a live one.

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Low Earth orbit is a commons with no fence and no sweeper. Kessler's belt has not formed, but every new collision moves it closer, and the clean-up has barely started.

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Megaconstellations

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On 23 May 2019 a Falcon 9 released 60 flat-packed satellites in a line that observers on the ground mistook for a train of lights. They were the first of Starlink , and by 2026 SpaceX had launched more than 8,000 of them, so that a single company operated well over half of all working satellites in orbit. Each is a slab of about 800 kilograms with a solar wing, krypton or argon ion thrusters, and phased-array antennas that steer beams to flat user terminals on the ground. They fly at around 550 kilometres, low enough that the round trip to a user takes about 25 milliseconds, against roughly 600 for a geostationary link, and low enough that a dead satellite falls back within about five years.

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The idea is older than the hardware. Iridium flew 66 satellites for telephone calls in 1998 and went bankrupt within a year; Teledesic planned 840 and built none. What changed was launch: a reusable Falcon 9 lifting 60 at a time, and later Starship's promise of hundreds, made the arithmetic work. OneWeb, rescued by the British government and Bharti in 2020 after its own bankruptcy, completed a 648-satellite network at 1,200 kilometres in 2023 and merged with Eutelsat. Amazon's Kuiper launched its first 27 production satellites on an Atlas V on 28 April 2025 towards a planned 3,236. China has two: the state Guowang, with a filing for about 13,000, and Shanghai's Qianfan, or Thousand Sails, which placed its first 18 in orbit in August 2024 and plans around 14,000. The International Telecommunication Union, which registers frequencies and orbits, has received filings for hundreds of…

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The uses arrived faster than the regulators. Within days of Russia's invasion in February 2022, Starlink terminals were keeping Ukrainian hospitals, government and troops online, the first war in which a private constellation was critical infrastructure; the company's decisions about where service worked showed the power that gave one firm. Direct-to-cell satellites, launched by Starlink from January 2024 and by AST SpaceMobile, now connect ordinary phones in dead zones.

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The cost falls on the sky. Astronomers at the Vera C. Rubin Observatory in Chile, which began surveying in 2025, find satellite streaks across a share of their wide-field exposures, and radio telescopes pick up the constellations' leakage. SpaceX responded with darker coatings, sun visors and attitude changes to keep satellites fainter than seventh magnitude; it now also de-orbits one or two a day as early models wear out. Collision-avoidance manoeuvres run to tens of thousands per half-year across the Starlink fleet.

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A century ago the telephone needed a wire to every house; now a tray of satellites sweeps overhead every few minutes. Whether the low orbits can be shared by half a dozen fleets and several thousand new satellites a year, without becoming the belt Kessler warned of, is the open question of the decade.

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The Human Computers

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Before the computer was a machine it was a job title, and the job was mostly held by women. From 1935 the NACA's Langley laboratory in Virginia hired women with mathematics degrees to reduce wind-tunnel data by hand, working with pencils, slide rules and Friden desk calculators that weighed as much as a typewriter. From 1943 the Black women among them were seated apart in the West Area Computing unit, with separate toilets and a separate table in the canteen. Its supervisor from 1949 was Dorothy Vaughan, the first Black manager at the NACA, who later taught herself and her staff FORTRAN when the IBM machines arrived and the hand-computing pools were disbanded.

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Katherine Johnson joined West Computing in 1953 and was soon borrowed by the Flight Research Division and never returned. In 1960 she co-authored with Ted Skopinski a report on the burnout azimuth needed to put a capsule down at a chosen spot, the first time a woman in her division had her name on a research paper. Before Friendship 7 on 20 February 1962, John Glenn asked that the orbit predicted by the IBM 7090 be checked by hand; Johnson worked through the equations over more than a day, and the numbers agreed. She later calculated the Apollo 11 rendezvous windows and worked on the return trajectory for Apollo 13. Mary Jackson, another West Computer, petitioned the city of Hampton to attend night classes at a whites-only school and in 1958 became NASA's first Black woman engineer.

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The pattern was not unique to Langley. At the Jet Propulsion Laboratory in Pasadena, Macie Roberts built an all-women computing section from the 1940s, insisting that women would be more welcome in a room run by women. Helen Ling, who succeeded her, hired mothers and rehired them after maternity leave. Sue Finley joined in January 1958, days before Explorer 1, and was still at JPL more than sixty years later, tracking spacecraft signals in the Deep Space Network, the longest-serving woman in NASA's history.

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The 2016 film Hidden Figures , from Margot Lee Shetterly's book, got the substance right and compressed the detail. The scene of Johnson running across the campus to a distant toilet belongs to Jackson's experience, not hers; Johnson said she simply used the nearest one. The white boss who smashes the "Colored" sign is a composite and did no such thing. What the film could not compress is the arithmetic: a Mercury orbit solved by hand, and a 101-year-old mathematician who received the Presidential Medal of Freedom in 2015 for it.

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The human computers were made obsolete by the machines they helped to program, which is the way of most engineering. Their legacy is the method: every number that leaves a mission is still checked by a second pair of eyes.

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Margaret Hamilton and the Apollo Software

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In August 1961 NASA gave its first major Apollo contract not to a rocket builder but to the MIT Instrumentation Laboratory in Cambridge, Massachusetts, for a guidance and navigation system that could find its way to the Moon if the ground fell silent. The heart of it was the Apollo Guidance Computer , a 32-kilogram box drawing 55 watts, with 2,048 words of erasable memory and 36,864 words of fixed memory, in 16-bit words. The fixed memory was core rope : the program was literally woven, a wire threaded through a ferrite core for a one and around it for a zero, by women at Raytheon's plant in Waltham working from printed instructions. A change to the software meant reweaving the rope, so the code had to be right months before launch.

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The crew spoke to it through the DSKY , a display and keyboard that took commands as a verb and a noun: Verb 16, Noun 68 showed landing data; Verb 37 selected a program. Behind it was an operating system designed by Hal Laning in which jobs carried priorities and a lower job could be dropped if the computer ran out of time. That design was tested on 20 July 1969, when the landing radar and a rendezvous radar switch set to the wrong mode together asked the computer for about 15 per cent more work than it had. It threw 1202 and 1201 alarms, restarted, kept the guidance job and shed the rest. In Mission Control, 24-year-old Jack Garman had the alarm list on a handwritten card; he told Steve Bales "go", and Bales told Gene Kranz.

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Margaret Hamilton led the Instrumentation Laboratory's software division through those years, having arrived in 1963 as a programmer with a mathematics degree and a young daughter who sometimes played with the simulator. She has said she began calling the work "software engineering" to win it the same respect as hardware; the NATO conference of 1968 made the phrase a discipline. The famous photograph of her beside a stack of listings as tall as she is shows the printouts of the Apollo code, around 145,000 lines across the command module and lunar module programs. Her insistence on error handling was vindicated on Apollo 8, when Jim Lovell accidentally keyed Program 01 and wiped the navigation data, which the ground then rebuilt by uploading.

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The Soviet programme took a different route. Early Soyuz flew with analogue controls, and the first Soviet onboard digital computer, Argon-11S, flew on the circumlunar Zond craft in 1968; the triple-redundant Argon-16 went into Soyuz from 1974 and served for decades. The AGC's descendants are everywhere: fly-by-wire aircraft, the Shuttle's redundant computers, and every system that decides what to drop when it runs out of time.

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Hamilton received the Presidential Medal of Freedom in 2016. The lesson she drew was simple: assume the unexpected, and write for it.

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Flight Directors

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The job did not exist until Christopher Kraft invented it. A Langley flight-test engineer, Kraft was assigned in 1958 to work out how a Mercury flight should be run from the ground, and concluded that someone had to be in charge of the whole thing in real time. He wrote the first flight rules , decisions made in advance so that nobody argued in the moment, and sat as flight director for every Mercury mission. His definition stuck: the flight director may take any action necessary for crew safety and mission success, and the decision is final. Nobody, not the NASA Administrator, can overrule a flight director during a flight.

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The role is a shift. During Apollo 11 four teams rotated, each named by colour: Gene Kranz's White Team took the landing, Glynn Lunney's Black Team the orbital work, Cliff Charlesworth's Green Team the launch and Milton Windler's Maroon Team the long cruise. Kranz wore a white waistcoat sewn by his wife Marta, a new one for each mission. On Apollo 13 it was Lunney's Black Team that took over an hour after the oxygen tank burst and powered up the lunar module as a lifeboat, a shift colleagues still call the finest in the room's history, while Kranz pulled his team off-line to plan the way home. The line "Failure is not an option" was never spoken in 1970; the screenwriters of the 1995 film built it from a conversation with controller Jerry Bostick, and Kranz liked it enough to use it as the title of his memoir.

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A go/no-go poll is how authority is exercised. Before the Apollo 11 descent Kranz called each console in turn, "Retro, FIDO, Guidance, Control, TELCOM, GNC, EECOM, Surgeon", and each answered "Go". Only the CAPCOM , always an astronaut, speaks to the crew: Charlie Duke passed it up as "You're go for landing". The crew never hear the room. The same cadence runs today for an ISS spacewalk or a Dragon docking, with the consoles renamed.

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Moscow built a different hierarchy. At TsUP , the flight control centre in Korolyov that opened for the Apollo-Soyuz flights of 1975, the flight director has usually been a former cosmonaut-engineer: Alexei Yeliseyev ran Salyut and early Soyuz flights, and Vladimir Solovyov, who flew to Salyut 7 and Mir, has directed the Russian segment from Mir's first years to the ISS. The ESA Columbus module answers to Oberpfaffenhofen near Munich, Japan's Kibo to Tsukuba, and China's Tiangong to Beijing, each with its own poll.

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The flight director's power rests on preparation, not rank. Thousands of pages of flight rules, hundreds of simulations in which the training team breaks something on purpose, and a culture in which "I don't know" is an acceptable answer and a guess is not. That is why, when a lunar module computer threw alarms fifty years ago, the right word was ready.

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The Seamstresses and Welders

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At its peak in 1966 the Apollo programme employed around 400,000 people, and only a few dozen of them were astronauts. The rest welded, sewed, wove, wired and polished, mostly for contractors spread across the United States. The Saturn V alone was built in four places: the 10-metre first stage by Boeing at the Michoud Assembly Facility outside New Orleans, the second stage by North American at Seal Beach in California, the third by Douglas at Huntington Beach, and the instrument unit by IBM in Huntsville. The command module came from North American at Downey, the lunar module from Grumman at Bethpage on Long Island.

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The spacesuit shows how much of spaceflight is craft. The A7L suit was made by ILC Dover , the industrial arm of Playtex, which beat Hamilton Standard's hard-suit design in 1965. Its 21 layers of nylon, neoprene, Mylar and Teflon-coated Beta cloth were sewn by seamstresses recruited from the bra and girdle lines, to a tolerance of a sixty-fourth of an inch; a stray pin could puncture a bladder, so pins were banned and every needle counted out and in. Hazel Fellows, who sewed the outer layers, and Eleanor Foraker, who supervised the line, worked shifts that stretched to eighty hours a week before Apollo 11. Each suit was made for one named astronaut, who came to Delaware to be measured.

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At Michoud the first stage's tanks were welded by hand and machine in a building large enough to hold a cathedral, then floated by barge to Mississippi for test firing. At Raytheon in Waltham the computer's program was woven wire by wire, the weavers checking each other's work against the listing. At Northrop Ventura riggers packed the three 25-metre main parachutes by hand; a mis-packed canopy cannot be inspected once stowed, so each rigger signed for his own. At Kennedy Space Center the pad leader Günter Wendt, who had closed the hatch on every Mercury and Gemini crew, ran the white room at the top of the tower and was the last face each Apollo crew saw. The Shuttle later needed 24,000 heat-shield tiles, each a unique shape, glued on by technicians at Palmdale and Kennedy.

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The Soviet programme was the same kind of industry under different names. Soyuz capsules and the R-7 that launched them were built at the Progress plant in Kuibyshev, now Samara; the pressure suits came from Zvezda at Tomilino, where seamstresses still sew the Sokol launch suit by hand. In Toulouse, Bremen, Tsukuba and Bengaluru the rooms look the same: gowned technicians, torque wrenches logged, every stitch and weld on a traveller sheet.

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Spaceflight has never become mass production. Each vehicle is still built by a few thousand people who know its serial number, which is why the industry calls itself, with some pride, a craft.

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The Cosmonaut Corps

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On 7 March 1960 twenty young Air Force pilots, none older than 35 and none taller than 1.75 metres, so that they would fit the Vostok capsule, were enrolled as the Soviet Union's first cosmonaut group . They trained at a secret base in the birch woods north-east of Moscow that became Star City , home of the Cosmonaut Training Centre, named for Yuri Gagarin after his death in 1968. Six were picked out early as the "vanguard": Gagarin, Gherman Titov, Grigori Nelyubov, Andriyan Nikolayev, Pavel Popovich and Valery Bykovsky. Their existence was a state secret; a cosmonaut's name was published only once he had flown.

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Secrecy cut both ways. Nelyubov, third in line after Gagarin and Titov, was dismissed in 1963 after a drunken quarrel with a military patrol and airbrushed from the group photograph; he died under a train in 1966. Valentin Bondarenko, the youngest, died in a pressure-chamber fire in March 1961, three weeks before Gagarin's flight, and his name was not released until 1986. Vladimir Komarov , the most experienced engineer in the group, was killed on 24 April 1967 when the parachute of Soyuz 1 failed to deploy, the first death in flight. In 1962 a women's group of five was recruited from parachutists and pilots; Valentina Tereshkova flew, the other four never did.

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A second kind of cosmonaut arrived with the engineers. Konstantin Feoktistov, who had helped design Vostok, flew on Voskhod 1 in 1964 as the first civilian in space. Georgy Grechko, another designer from Korolev's bureau, made three flights to three Salyut stations between 1975 and 1985. Svetlana Savitskaya, a test pilot and the daughter of an air marshal, became the first woman to walk in space on 25 July 1984, outside Salyut 7 for three hours and 35 minutes. The corps' records are long-duration ones: Anatoly Solovyev made sixteen spacewalks totalling more than 82 hours, Gennady Padalka logged 878 days across five flights, and Oleg Kononenko passed 1,000 cumulative days in June 2024 and finished his fifth mission with 1,111.

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Today the Air Force, design-bureau and Academy of Sciences groups have been merged into a single Roscosmos corps based at Star City, with a few dozen active members and selections in 2018 and 2021 open to civilians. Cosmonauts still launch from Baikonur in Kazakhstan, still train in the Hydrolab and the centrifuge Gagarin's group used, and still fly on Soyuz, whose design dates from Komarov's death.

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The corps' story is the Soviet century in miniature: brilliance, secrecy, loss and endurance, and the quiet pride of people who stayed in orbit while the map beneath them was redrawn.

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Astronauts of Many Nations

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For the first seventeen years of human spaceflight every traveller was American or Soviet. On 2 March 1978 Vladimír Remek, a Czechoslovak Air Force pilot, lifted off on Soyuz 28 and broke the pattern, the first person in space from a third country. He flew under Interkosmos , a Soviet programme that offered a week aboard Salyut 6 to one citizen of each allied state: Mirosław Hermaszewski of Poland and Sigmund Jähn of East Germany in 1978, then Bulgaria, Hungary, Vietnam, Cuba, Mongolia and Romania. Arnaldo Tamayo Méndez of Cuba, who flew in September 1980, was the first Black person and the first Latin American in space. In 1982 the programme opened to the West with Jean-Loup Chrétien of France, and in April 1984 Rakesh Sharma of India spent a week on Salyut 7, telling Indira Gandhi that from orbit his country looked "better than the whole world", a line from a famous Urdu poem.

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The Shuttle offered the second road. Ulf Merbold of West Germany flew on STS-9 in November 1983 as the first ESA astronaut and the first non-American on a US spacecraft; two months earlier Guion Bluford had become the first African-American in space on STS-8. Marc Garneau of Canada followed in 1984, Mae Jemison became the first Black woman in orbit in September 1992, and Chiaki Mukai, a surgeon, the first Japanese woman in 1994, though the first Japanese citizen in space had been the television journalist Toyohiro Akiyama, who bought a seat to Mir in December 1990. Helen Sharman, a chemist from Sheffield, reached Mir in May 1991 as the first Briton, chosen from 13,000 applicants to a radio advertisement.

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China built its own road. Yang Liwei orbited alone in Shenzhou 5 on 15 October 2003, making China the third nation to launch its own astronaut; its taikonauts have since flown only on Chinese rockets, and Tiangong has hosted no foreigner yet, though a Pakistani astronaut has been announced. After the Shuttle retired, Soyuz seats again carried new flags: Marcos Pontes of Brazil in 2006, Hazzaa AlMansoori of the United Arab Emirates in September 2019, Marina Vasilevskaya of Belarus in 2024. The fourth road is private. Axiom's missions to the ISS carried the first Saudi woman, Rayyanah Barnawi, in 2023, the first Turk in January 2024, and in June 2025 Shubhanshu Shukla, an Indian Air Force pilot, forty-one years after Sharma, as a paying passenger of his government.

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By mid-2026 around 700 people from some 45 countries had reached orbit, most of them still American or Russian. The rest flew because a superpower wanted an ally, a customer or a partner, which is the honest history of who gets to go.

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Whatever the motive, the view is the same, and nearly everyone who has had it has come back saying the same thing: the borders are not visible from there.

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Women in Space

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Valentina Tereshkova's three days in orbit in June 1963 were followed by a silence of nineteen years. The Soviet women's group was disbanded in 1969, and NASA had turned away the thirteen women who passed the Lovelace clinic's astronaut medical tests in 1960 and 1961, on the grounds that astronauts had to be military jet test pilots and women could not be. The silence ended with Svetlana Savitskaya , who flew to Salyut 7 in August 1982 and returned in July 1984 to make the first spacewalk by a woman, three hours and 35 minutes outside the station welding and cutting metal with an electron-beam tool. The timing was not accidental; NASA had announced that Kathryn Sullivan would walk in October.

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Sally Ride , a physicist with a doctorate from Stanford, rode STS-7 into orbit on 18 June 1983, operating the Shuttle's robotic arm. At the press conference beforehand she was asked whether she wept when things went wrong. Sullivan's spacewalk followed in October 1984. Mae Jemison flew in 1992, Chiaki Mukai in 1994, and in February 1995 Eileen Collins , an Air Force test pilot, became the first woman to pilot a spacecraft; in July 1999 she commanded STS-93 and deployed the Chandra X-ray observatory. Her commander's seat, like Ride's arm, had been a matter of rules, not ability: once the rule changed, the queue was already there.

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Endurance and command followed. Peggy Whitson , a biochemist, commanded the ISS in 2007 and again in 2017, became NASA's chief astronaut, and after retiring flew twice more for Axiom as a private commander, her career total passing 675 days, more than any other American. Samantha Cristoforetti of ESA took command of the station in September 2022, the first European woman to do so. Liu Yang became the first Chinese woman in orbit in 2012, and Wang Yaping made China's first female spacewalk on 7 November 2021 from Tiangong. Kalpana Chawla, born in Haryana and killed on Columbia in 2003, was the first woman of Indian origin to fly; Yelena Serova in 2014 was only the fourth Russian woman.

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Koch was assigned to the Artemis II crew, the first people to fly around the Moon since 1972. By 2026 about one space traveller in nine was a woman, a ratio that recent astronaut classes, roughly half female at NASA and ESA, are slowly changing.

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The pattern of sixty years is consistent: women were excluded by rule, admitted when the rule changed, and then did the job, which is the dullest and most convincing argument there is.

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The Scientist-Astronauts

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NASA's first astronauts were test pilots, chosen because Eisenhower wanted people already cleared for secrets and used to risk. The scientists came in two reluctant batches. In June 1965 the agency selected six scientist-astronauts , chosen with the National Academy of Sciences: among them the physician Joe Kerwin, the physicists Owen Garriott and Ed Gibson, and a Harvard geologist named Harrison Schmitt. A second group of eleven followed in August 1967 and promptly nicknamed itself the Excess Eleven, since the lunar programme was shrinking and there were no seats. All of them were sent to Air Force flight school first, because the pilot culture that ran the office did not trust anyone who could not fly a jet.

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Schmitt forced the issue. The scientific community lobbied for a geologist on the Moon, and in 1971 he replaced Joe Engle on the final crew. On Apollo 17 in December 1972 he spotted the orange soil at Shorty crater, volcanic glass beads 3.6 billion years old, the single most discussed sample of the programme. Skylab gave the others their turn: Kerwin on the first crew, Garriott for 59 days on the second, Gibson for 84 on the third, where he studied the Sun through the station's telescope mount. Story Musgrave, a surgeon from the 1967 group, waited sixteen years for his first flight and in December 1993 led the spacewalks that fixed Hubble.

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The Shuttle created the payload specialist , a researcher flown for a single mission to run their own experiment, from Ulf Merbold and Byron Lichtenberg on Spacelab 1 in 1983 onward, and the ISS turned science into a routine. Don Pettit, a chemical engineer, filmed "Saturday Morning Science" on Expedition 6 in 2003, showing water films and spinning tools in free fall. Kate Rubins, a virologist, sequenced DNA in orbit for the first time in August 2016 with a palm-sized MinION. Jessica Watkins, a planetary geologist, spent 170 days aboard in 2022, the first Black woman on a long-duration crew.

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What a station scientist's day looks like is less romantic than the title. A typical ISS schedule gives each crew member about six and a half hours of work, shared between experiments and the maintenance that keeps the station alive, two and a half hours of exercise against bone and muscle loss, and eight and a half hours for sleep. Most experiments are designed by scientists on the ground and executed by the crew, who are technicians of other people's ideas; the station's hundreds of investigations a year depend on that division.

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The tension between the two cultures never fully resolved. It was settled, as such things are, by the schedule: the pilot flies the ship, the scientist runs the rack, and on a good day they are the same person.

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The Cost in Lives

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Spaceflight has killed fewer people than a single bad year on a mountain, but each death was public, investigated and written into the rules. The first were hidden. On 24 October 1960 an R-16 missile exploded on its pad at Baikonur while Marshal Mitrofan Nedelin sat on a chair beside it to show confidence; at least 90 people died, probably more, and the Nedelin catastrophe was officially a plane crash until 1989. On 23 March 1961 the youngest cosmonaut, 24-year-old Valentin Bondarenko, dropped a cotton pad onto a hot plate in an oxygen-rich isolation chamber and died of his burns; the Soviet Union did not admit it until 1986.

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The Americans learned the same lesson about oxygen on 27 January 1967, when a fire in the pure-oxygen cabin of Apollo 1 killed Gus Grissom, Ed White and Roger Chaffee during a ground test. The review board blamed flammable materials, a hatch that opened inward and poor wiring; the cabin was changed to a nitrogen-oxygen mix on the pad and the hatch redesigned. Three months later Vladimir Komarov died when Soyuz 1's parachute failed. On 30 June 1971 Georgy Dobrovolsky, Vladislav Volkov and Viktor Patsayev, returning from the first space station after a record 23 days, were killed when a valve opened at 168 kilometres and the cabin emptied in under a minute; they wore no suits. Since then every Soyuz crew has worn a Sokol pressure suit for launch and landing.

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The Shuttle's two losses, Challenger on 28 January 1986 and Columbia on 1 February 2003, each killed seven and each produced a famous inquiry. The Rogers Commission found that NASA had flown with a known O-ring weakness; Richard Feynman dropped a piece of rubber into iced water on television to show why. The Columbia Accident Investigation Board found a culture that had learned to live with foam strikes, and its report ended the programme by 2011. Ground deaths continued elsewhere: 48 at Plesetsk when a Vostok rocket exploded during fuelling on 18 March 1980, 21 at Brazil's Alcântara launch centre on 22 August 2003 when a VLS-1 ignited on its pad, and villagers near Xichang in 1996 when a Long March fell on their homes. On 31 October 2014 the test pilot Michael Alsbury died when SpaceShipTwo broke up over the Mojave after its feathering tail unlocked too early; the inquiry blamed a…

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Each loss altered the hardware and the habits. Soyuz 11 gave crews their suits. Apollo 1 gave them an outward hatch. Challenger ended the carrying of passengers on experimental vehicles for a generation. Columbia gave every Shuttle an inspection on orbit.

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The modern rule, written in blood, is that a spacecraft must be designed so that no single error, by a person or a part, can kill its crew.

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The Agencies

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A space mission begins as a sentence in a report. In the United States the National Academies convene a Decadal Survey for each field, in which hundreds of scientists rank the questions and the missions that would answer them; NASA then runs competitions in three sizes. Discovery missions are led by a single principal investigator under a strict cost cap, such as Lucy, launched in 2021 to the Trojan asteroids, and Psyche in 2023. New Frontiers missions are larger, including New Horizons, Juno and the Dragonfly rotorcraft planned for Titan. Flagships are chosen directly, like Cassini, the Mars rovers and Europa Clipper, launched on 14 October 2024. A proposal passes through Phase A studies, a down-select, then Phases B, C and D of design, build and test, and a confirmation review that can kill it.

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NASA itself is smaller than its reputation: about 18,000 civil servants across ten centres, with most of the work done by contractors and universities, and a budget that has stayed below half a per cent of federal spending for decades, after a peak near four per cent in 1966. Cancellation is part of the system. The Constellation Moon programme was cancelled in 2010, the VIPER lunar rover in 2024 after it had been built, and Mars Sample Return was sent back for cheaper options in 2024 and 2025.

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The European Space Agency , with 23 member states since Slovenia joined in 2025, works by subscription: a mandatory science programme funded by GDP share, and optional programmes, such as launchers or human spaceflight, that each country joins as it chooses, with France, Germany and Italy the largest contributors. Its launches fly from Kourou in French Guiana, and its missions are picked in Cosmic Vision calls by size class, from the small to the large. JAXA, formed in 2003 from three Japanese institutes, is famous for frugal sample return. China's CNSA, founded in 1993, publishes five-year plans and has executed them with unusual precision, from Chang'e to Tiangong. ISRO, created in 1969, landed Chandrayaan-3 near the lunar south pole on 23 August 2023. The Canadian Space Agency's contribution to every station since 1981 has been a robotic arm, and Canadarm3 is its ticket to the…

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Missions are shared because no one can afford them alone. Webb carries ESA's launch and instruments, Gateway will carry a Canadian arm, a European habitat and a Japanese one, and even a flagship is a treaty in hardware.

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An agency is a machine for turning a question into a budget line and a budget line into a spacecraft, slowly, and with many chances to say no.

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Ariane and Europe's Launchers

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Europe's first rocket was a committee. Europa , built from 1964 by the European Launcher Development Organisation, stacked a British Blue Streak first stage on a French second and a German third, with no single authority over the whole. Of eleven launches from Woomera and Kourou between 1964 and 1971, not one placed a satellite in orbit; the Blue Streak worked every time and the stages above it failed in turn. When the European Space Agency was founded on 30 May 1975, France insisted that the new launcher be run by one prime contractor under one management, and the lesson of Europa became the design rule of Ariane .

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Ariane 1 lifted off from Kourou in French Guiana on 24 December 1979, a 47-metre, 210-tonne rocket burning storable propellants in its first two stages and hydrogen in its third. The site was the point: Kourou sits at 5.2° north, so a launch eastward borrows nearly the full 465 metres per second of the Earth's rotation and a satellite bound for geostationary orbit needs a far smaller plane change than one from Florida or Baikonur. In March 1980 the partners set up Arianespace , the first company to sell launches commercially, and through the 1980s and 1990s it carried roughly half of the world's commercial communications satellites. Ariane 4 flew 116 times between 1988 and 2003 with 113 successes, the workhorse that made the business.

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Ariane 5 began with the most expensive software failure in the industry's history. On 4 June 1996 flight 501 broke apart 37 seconds after lift-off, because its inertial reference system reused Ariane 4 code that converted a 64-bit velocity figure into a 16-bit integer; the faster Ariane 5 overflowed the number, both redundant units shut down in the same instant, and the rocket swung its nozzles hard over. The inquiry report is still taught to software engineers. The rocket recovered to fly 117 times before its last launch on 5 July 2023, lofting Rosetta, four ATV cargo ships, BepiColombo, JUICE and Webb. Beside it the Italian-led solid-fuelled Vega flew small payloads from 2012.

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Then the ground shifted. From about 2014 SpaceX's partly reusable Falcon 9 undercut Ariane 5 on the commercial orders that had paid for Europe's independence. For a year after Ariane 5 retired, with Vega-C grounded after a December 2022 failure and Russian Soyuz withdrawn from Kourou, Europe had no rocket of its own and launched Galileo navigation satellites on Falcon 9. Ariane 6 finally flew on 9 July 2024, a 56-metre rocket with a Vulcain 2.1 core, a restartable Vinci upper stage and two or four P120C solid boosters shared with Vega-C.

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Ariane 6 is not reusable, and Europe knows it; the Prometheus methane engine and the Themis hopper are its answer for the 2030s. What Ariane proved from 1979 remains true: a continent that cannot launch its own satellites is a customer, not a power.

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Russia After the Union

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When the Soviet Union dissolved in December 1991, its space programme woke up in the wrong country. Baikonur , the cosmodrome that had launched Sputnik and Gagarin, lay in newly independent Kazakhstan, and Russia has rented it ever since under a 1994 agreement extended to 2050. Half the industry's factories were in Ukraine, including the makers of the Zenit rocket and the control systems of the Proton. Budgets collapsed; cosmonauts on Mir went unpaid for months, and in 1993 the Russian Space Agency began selling what it had, from Soyuz seats to Proton launches and the hard-won experience of long-duration flight that made the International Space Station possible.

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The selling worked for twenty years. Proton, marketed through International Launch Services from 1995, carried a large share of the world's commercial geostationary satellites; Soyuz rockets launched from Kourou from 2011; and when the Space Shuttle retired in July 2011, the three-seat Soyuz became the only way for any human being to reach the station, a monopoly that lasted until Crew Dragon's first crewed flight in May 2020. The money disguised a thinning workforce and lapsing quality control. On 2 July 2013 a Proton-M carrying three GLONASS navigation satellites flipped over seconds after lift-off and exploded on live television; the inquiry found angular-rate sensors installed upside down, hammered into place against their locating pins.

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The state rebuilt where it could. The Vostochny cosmodrome, begun in 2012 in the Amur region of the Russian Far East to end the dependence on Baikonur, saw its first launch on 28 April 2016 and its first Angara A5 in April 2024, after a decade of construction scandals and embezzlement trials. Roscosmos became a state corporation in 2015. Then the invasion of Ukraine in February 2022 brought sanctions, the loss of Western customers, the withdrawal of Soyuz from Kourou and the suspension of the ExoMars rover partnership; thirty-six OneWeb satellites sat impounded at Baikonur. The flagship Luna 25, Russia's first Moon lander since 1976, launched from Vostochny on 11 August 2023 and crashed eight days later when an orbit-lowering burn ran for 127 seconds instead of 84.

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The station partnership survived, mostly because neither side could run the ISS alone. In July 2021 the long-delayed Nauka module docked and then fired its thrusters uncommanded, rotating the whole station through about 540 degrees before the Russian segment ran out of propellant; the crew were never in danger, NASA said, but Houston declared a spacecraft emergency. Russia has committed to the station until 2028 and plans its own Russian Orbital Station for the years after, while crews still swap seats, cosmonauts riding Dragon and astronauts riding Soyuz.

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Korolev's machine still flies, cheaply and often. What it lacks is what the old firm once had in surplus: money, youth and a next thing to build.

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China Rises

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China's first satellite, Dong Fang Hong 1 , went up from Jiuquan on 24 April 1970 on the first Long March rocket, a 173-kilogram sphere that broadcast the song "The East Is Red" for 28 days, making China the fifth nation to orbit its own spacecraft. The programme's founder was Qian Xuesen, a co-founder of the Jet Propulsion Laboratory, deported from the United States in 1955 on suspicion of communist sympathies. For three decades afterwards China launched satellites steadily and humans not at all.

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That changed on 15 October 2003, when Yang Liwei flew fourteen orbits in 21 hours aboard Shenzhou 5, a craft whose Soyuz lineage is plain but whose systems were Chinese. The lunar programme named for the Moon goddess Chang'e followed a stated sequence, orbit, land, return, and kept to it. Chang'e 1 orbited the Moon in 2007; Chang'e 3 landed in Mare Imbrium on 14 December 2013 with the 140-kilogram Yutu rover, the first soft landing on the Moon since Luna 24 in 1976. Chang'e 4 did what no one had done: on 3 January 2019 it set down in Von Kármán crater on the far side, where the Moon's bulk blocks all radio contact with Earth, talking home through the Queqiao relay satellite parked in a halo orbit around the Earth-Moon L2 point since 2018.

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Then the samples. Chang'e 5 launched on a Long March 5 from Wenchang on 23 November 2020, landed near Mons Rümker in Oceanus Procellarum, drilled and scooped 1,731 grams of two-billion-year-old basalt, lifted off from the surface, docked in lunar orbit with its return craft and dropped a capsule in Inner Mongolia on 16 December, a miniature Apollo flown by robots. Chang'e 6 repeated the feat on the far side, returning 1,935 grams from Apollo crater on 25 June 2024, the only far-side material on Earth. Meanwhile Tianwen-1 reached Mars orbit in February 2021 and on 15 May landed the Zhurong rover in Utopia Planitia, the first nation to orbit, land and rove on its first Mars attempt.

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The hardware behind this is the Long March 5, a 57-metre, 870-tonne rocket with a 5-metre core and four kerosene boosters, launched from the coastal Wenchang site on Hainan Island at 19° north so that spent stages fall into the sea rather than onto villages, as earlier inland launches sometimes did. Tianwen-2 left for the asteroid Kamoʻoalewa in 2025; Tianwen-3, a Mars sample return, is planned for 2028, ahead of NASA's stalled equivalent; and the Mengzhou capsule, Lanyue lander and Long March 10 are being built for a crewed lunar landing before 2030.

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China has reached the Moon's surface four times in eleven years without a failure. Whatever the race to return is, it now has two runners.

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India's Frugal Space Programme

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The Indian space programme began in a church. In 1962 the physicist Vikram Sarabhai chose the fishing village of Thumba, near Thiruvananthapuram on the magnetic equator, for a sounding-rocket range, and the bishop gave up the church of St Mary Magdalene to serve as its first workshop. Rocket parts arrived by bicycle and bullock cart, as the famous photographs show, and the first rocket, an American Nike-Apache, flew on 21 November 1963. Sarabhai's stated purpose was unusual: not prestige but satellites for television, weather and resource mapping in a poor country. The Indian Space Research Organisation was formed in 1969 and launched its first satellite, Aryabhata, on a Soviet rocket in April 1975.

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India's own launcher, the SLV-3, put the 35-kilogram Rohini satellite in orbit on 18 July 1980 under a project director named A. P. J. Abdul Kalam, later President of the republic. The rocket that made ISRO's reputation was the PSLV , first successful in 1994: a four-stage vehicle alternating solid and liquid stages that has flown more than sixty times, and on 15 February 2017 released 104 satellites from one flight, 88 of them Planet's Dove imaging CubeSats, a record that stood until 2021. Its successor LVM3, with two large solid boosters and a cryogenic upper stage, lifts about four tonnes to geostationary transfer orbit and carried OneWeb's satellites when Russia would not.

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The deep-space record is remarkable for a programme spending a small fraction of NASA's budget. Mangalyaan , the Mars Orbiter Mission, launched on a PSLV on 5 November 2013, too small a rocket to go direct, so the 1,337-kilogram craft raised its orbit around Earth six times before departing; it entered Mars orbit on 24 September 2014, making India the first nation to succeed at Mars on its first attempt. Chandrayaan-2's lander crashed in September 2019 during the final braking phase. Its successor Chandrayaan-3 landed on 23 August 2023 at 69° south, nearer the lunar south pole than any craft before it, with a 26-kilogram rover named Pragyan that measured sulphur in the soil; the lander later fired its engines and hopped 40 centimetres, a rehearsal for a future sample return. Aditya-L1 followed in September 2023 to watch the Sun from the L1 point.

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The next step is crew. The Gaganyaan capsule has flown an abort test in October 2023, and a crewed orbital flight is planned for 2027, which would make India the fourth nation to launch its own astronauts. A private sector has appeared under the IN-SPACe regulator of 2020: Skyroot's Vikram-S reached space on 18 November 2022, the first Indian privately built rocket, and Agnikul test-flew a 3D-printed engine in 2024.

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ISRO's style is sequential, patient and cheap, and it ends at places others have not reached. The south pole of the Moon was first touched by the programme that started in a church.

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Japan, Europe and the Others

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Between the superpowers and the start-ups sit the programmes that cannot afford everything and therefore choose well. Japan's JAXA is the clearest case. Hayabusa, launched in 2003, lost two of its four ion engines, a reaction wheel, its fuel and contact with Earth for seven weeks, and still brought the first asteroid dust home to Woomera in June 2010, 1,500 grains from Itokawa. Hayabusa2 did it properly: it fired a copper impactor into Ryugu to expose fresh material, and on 6 December 2020 delivered 5.4 grams that contained amino acids and uracil, a base of RNA. Japan's Kibo is the largest module on the International Space Station, and nine HTV freighters supplied it between 2009 and 2020.

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JAXA also shows how a mid-sized agency recovers from a bad year. Its new H3 rocket failed on its first flight on 7 March 2023 when the second-stage engine did not ignite, taking the ALOS-3 Earth-observation satellite with it; the second flight on 17 February 2024 succeeded. Weeks earlier, on 20 January 2024, the small SLIM lander had touched down 55 metres from its target, inside a 100-metre goal that no previous lander had attempted, using crater-matching cameras. One engine nozzle had fallen off in the final descent and SLIM came to rest on its nose with its solar cells facing west; it woke when the Sun moved round, and survived three lunar nights it was never designed to endure.

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The European Space Agency, twenty-three member states voting on a budget around a quarter of NASA's, picks the missions the giants have skipped. Rosetta spent ten years reaching comet 67P and two years flying beside it. Gaia, launched in 2013, measured the positions and motions of nearly two billion stars, the most-cited data set in modern astronomy. ExoMars shows the cost of partnerships: its Schiaparelli demonstrator crashed in 2016, and the Rosalind Franklin rover, built for a Russian lander and a Russian rocket, was stranded by the 2022 sanctions and is now planned for 2028 on an American launcher.

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The newcomers choose smaller targets and reach them. The United Arab Emirates' Hope orbiter, built with American universities and launched on a Japanese H-IIA, entered Mars orbit on 9 February 2021 to study the planet's weather. South Korea's own Nuri rocket reached orbit on 21 June 2022, and its Danuri probe has circled the Moon since December 2022 carrying NASA's ShadowCam to peer into permanently dark craters. Israel's Beresheet, a privately funded lander the size of a washing machine, crashed on 11 April 2019 when a gyroscope fault cascaded into a main-engine shutdown, the first private attempt on the Moon.

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What the mid-sized programmes do that giants do not is specialise: sample return, precision landing, the comet, the catalogue, the weather of Mars. Exploration is not a two-horse race but a relay, and these are the runners who take the awkward legs.

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SpaceX and the Reusable Rocket

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On 28 September 2008 a small rocket called Falcon 1 reached orbit from Omelek Island in the Kwajalein Atoll on its fourth attempt, after three failures that had used up almost all of the money its founder had put in. Elon Musk had said there was cash for three flights; the fourth was borrowed time. Three months later NASA awarded SpaceX a fixed-price contract to carry cargo to the International Space Station under its Commercial Orbital Transportation Services scheme, the arrangement by which the agency bought a service rather than designing a vehicle, and the company survived.

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Falcon 9 first flew on 4 June 2010: 70 metres tall, 549 tonnes at lift-off, nine Merlin engines burning kerosene and liquid oxygen for 7,600 kilonewtons at sea level, with a single Merlin vacuum engine upstairs. The Dragon capsule berthed at the station on 25 May 2012, the first commercial spacecraft to do so. The idea that made the rocket different was that the first stage, which carries about 60 percent of the vehicle's cost, should come back. Parachute recovery failed; from 2013 the company tried propulsive landing instead, lighting three engines to flip the booster round and slow it, deploying titanium grid fins to steer it through the air, and lighting one engine for a final braking burn onto four unfolding legs.

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The record sets itself out in dates. First landing on solid ground: 21 December 2015 at Cape Canaveral, after the Orbcomm mission. First landing on a drone ship at sea, which a mission to geostationary orbit requires because the booster is moving too fast to return: 8 April 2016. First reflight of a used booster: 30 March 2017, carrying the SES-10 satellite. Two failures punctuate the sequence, a strut that broke in flight in June 2015 and a helium tank that burst on the pad in September 2016. Then the curve bends: by 2024 the company flew 134 Falcon missions in a single year, more than the rest of the world combined, individual boosters passed twenty and then thirty flights, and the fairing halves were being fished from the sea and reused as well.

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On 30 May 2020 Crew Dragon carried Doug Hurley and Bob Behnken to the station from Pad 39A, the first crewed orbital launch from the United States in nine years and the end of the Soyuz monopoly. Commercial Crew, like COTS, was a fixed-price contract in which the company owned the vehicle.

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How much did reuse save? Estimates vary and the company does not publish its accounts, but the published price per kilogram to low orbit fell by about an order of magnitude from the Shuttle era, and the cadence rose faster than the price fell. A reusable booster is a rocket treated like an aircraft: the fuel is cheap, the machine is not, and the trick is to keep the machine.

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Starship

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Starship is the largest and most powerful rocket ever flown and the first designed to be entirely reusable, booster and ship alike. The stack stands about 120 metres on the pad at Starbase near Boca Chica, Texas: a 71-metre Super Heavy booster with 33 Raptor engines burning liquid methane and liquid oxygen for roughly 74 meganewtons of thrust, more than twice the Saturn V, under a 50-metre Starship with six Raptors, three for sea level and three for vacuum. Both are stainless steel, chosen over carbon fibre because it is cheap, weldable and strong when cold and hot. The goal is a hundred tonnes to orbit for the price of the propellant, refilled in space, and eventually Mars.

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The test campaign has been conducted in public. The first integrated flight on 20 April 2023 lifted off from a pad with no flame trench and no water deluge, tore a crater beneath the launch mount, lost several engines and tumbled at 39 kilometres before the self-destruct system, late to act, broke it up. A water-cooled steel plate followed. On 6 June 2024 the fourth flight brought both stages to controlled ocean splashdowns, the ship's flap burning through on camera and still steering. On 13 October 2024 the booster returned to the launch site and was caught in mid-air by the two arms of the launch tower, a manoeuvre that eliminates landing legs and puts the stage back on the mount in minutes.

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Then 2025 showed the other side of iterating in public. The upgraded Block 2 ship was lost on its first three flights in January, March and May, raining debris near the Caribbean, while the boosters were caught twice and one flew again in May, the first reuse of a Super Heavy. The tenth flight on 26 August 2025 finally delivered a clean mission with dummy Starlink satellites deployed and both stages down where intended, and the eleventh in October 2025 repeated it; a larger Block 3 and a second pad are planned to follow.

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Two things are unproven, and the Moon programme depends on both. One is propellant transfer in orbit: a lunar Starship must be refilled by around a dozen tanker flights before it can leave for the Moon, and no ship-to-ship transfer of cryogenic propellant has yet been performed. The other is landing: the version NASA selected in April 2021 as the Artemis III human landing system must descend to the lunar south pole on its own engines, having never landed on anything but Earth. NASA's schedule for that landing has slipped repeatedly and is now described as planned rather than dated.

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Starship has proven that a 5,000-tonne rocket can fly, come back and be caught. It has not yet proven that it can be a spacecraft. Both halves of that sentence matter.

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New Rockets, New Players

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Falcon 9 proved that a private company could build an orbital rocket; a decade later dozens are trying. At the heavy end is New Glenn , Blue Origin's 98-metre two-stage rocket with seven methane-burning BE-4 engines and a 7-metre fairing, the widest in service. Founded by Jeff Bezos in 2000, the company spent a quarter of a century reaching orbit: New Glenn's first flight on 16 January 2025 succeeded but lost its booster during the descent, and on the second flight, on 13 November 2025, the booster landed on the ship Jacklyn in the Atlantic while the upper stage sent NASA's two ESCAPADE probes towards Mars. United Launch Alliance's Vulcan , the successor to Atlas V and Delta IV, first flew on 8 January 2024 using the same BE-4 engines bought from its rival, and was certified for national-security launches in 2025.

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The small end is the most crowded. Rocket Lab's Electron , an 18-metre carbon-fibre rocket whose Rutherford engines are 3D-printed and pump their propellants with battery-driven electric motors, first reached orbit on 21 January 2018 from the Mahia peninsula in New Zealand, the first private orbital launch site, and has since flown more than seventy times. Its medium-lift Neutron, with a reusable first stage, is planned to follow from Wallops Island in Virginia. Firefly's Alpha reached orbit in October 2022, and Firefly's Blue Ghost lander touched down in Mare Crisium on 2 March 2025, the first fully successful commercial landing on the Moon. Relativity Space launched Terran 1, 85 percent 3D-printed by mass, in March 2023; it failed at stage separation and was abandoned for the larger Terran R.

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China's commercial sector appeared after a 2014 policy opened launch to private capital. Galactic Energy's Ceres-1 reached orbit in November 2020; LandSpace's Zhuque-2 became the first methane rocket in orbit in July 2023; several firms are flying grasshopper-style hop tests towards reusable boosters. In June 2024 Space Pioneer's Tianlong-3 first stage broke free during a static firing and crashed into hills near Gongyi. Europe's entry came on 30 March 2025, when Isar Aerospace's Spectrum lifted off from Andøya in Norway, the first orbital attempt from the European mainland, flew for about thirty seconds and fell into the sea, which the company called a successful first test.

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Who survives the launch glut? The demand that was supposed to justify dozens of small rockets has largely been absorbed by rideshare on Falcon 9 and by megaconstellations launched on their owners' vehicles. Virgin Orbit went bankrupt in 2023, and the survivors tend to share three features: an anchor customer, usually a government; a vehicle large enough to carry a useful satellite alone; and a plan to reuse the first stage.

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The 1960s had two launch programmes and the 2020s have perhaps forty. Most will fail, as most railways and airlines failed, and the ones that do not will set the terms of the next century's access to orbit.

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The Space Economy

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Ask where the money in space is and the honest answer is: not in rockets. The Space Foundation put the global space economy at around 600 billion dollars in 2024, and by every industry count the bulk of it is satellite services and the ground equipment that uses them, television, broadband, navigation chips in phones and cars, weather and imagery, with government budgets the next largest slice. Launch, the part everyone photographs, is a few percent of the total. The satellites built in the last decade are smaller and far more numerous than those of the 1990s, and that change begins with a box ten centimetres on a side.

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The CubeSat standard was proposed in 1999 by Jordi Puig-Suari of California Polytechnic and Bob Twiggs of Stanford so that students could finish a satellite within a degree course: a 10-centimetre cube weighing no more than 1.33 kilograms, ejected from a standard dispenser any rocket could carry. The first six flew on a Russian Rokot in June 2003. Planet, founded in 2010 by three former NASA engineers, builds Doves, three-unit CubeSats the size of a loaf, launched 88 of them on one Indian PSLV in February 2017 and now images the whole land surface of the Earth every day with a fleet of around two hundred. On 24 January 2021 SpaceX's Transporter-1 rideshare carried 143 satellites on a single Falcon 9, a record, at a price a university could afford.

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The second change was in how governments buy. NASA's Commercial Orbital Transportation Services programme, begun in 2006, paid fixed sums on milestones to SpaceX and Orbital Sciences and let them own the vehicles; a NASA study in 2011 estimated that Falcon 9 had cost a fraction of what the traditional cost-plus model would have. Commercial Crew applied the same logic in 2014 to Dragon and Boeing's Starliner, and the Commercial Lunar Payload Services scheme since 2018 has bought rides to the Moon's surface from Intuitive Machines, whose Odysseus tipped over on landing in February 2024, and Firefly, whose Blue Ghost landed cleanly in March 2025. Fixed prices move the risk of overruns to the contractor, as Boeing's Starliner losses show.

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The winners are concentrated. SpaceX, valued by private investors at hundreds of billions of dollars, earns most of its revenue not from launch but from Starlink, whose subscribers passed five million in early 2025; launch is the delivery van for the broadband business. The casualty list is long: Virgin Orbit filed for bankruptcy in April 2023 months after a failed launch from Cornwall, Astra was taken private after its share price collapsed, and OneWeb was rescued from insolvency in 2020 by the British government and Bharti.

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The space economy is mostly an information economy that happens to run through orbit. The rockets are the roads; the money travels on the signals.

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The Law and Politics of Space

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There is law in orbit, and it was written quickly. The Outer Space Treaty , opened for signature on 27 January 1967 and in force from October, now binds more than 110 states. It says that space is free for exploration by all, that no nation may claim sovereignty over the Moon or any celestial body, that nuclear weapons may not be placed in orbit, that the Moon is for peaceful purposes, that states are responsible for the acts of their companies and citizens in space, and that a launching state is liable for the damage its objects cause. Four further treaties followed: the Rescue Agreement of 1968, the Liability Convention of 1972, the Registration Convention of 1975 and the Moon Agreement of 1979, which would make lunar resources the common heritage of humankind and which no spacefaring power has ratified.

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The Liability Convention was tested once. On 24 January 1978 the Soviet reconnaissance satellite Cosmos 954, powered by a nuclear reactor, re-entered over northern Canada and scattered radioactive fragments across 124,000 square kilometres of the Northwest Territories. Canada's Operation Morning Light recovered the debris, Canada presented a claim, and in 1981 the Soviet Union paid about half of it without admitting fault. It is the only claim ever settled under the convention.

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The gaps in the 1967 treaty are where the politics now lives. It forbids national appropriation but is silent on extraction, so the United States legislated in November 2015 that its citizens may own resources they mine in space, and Luxembourg followed in 2017. In October 2020 NASA and seven partners signed the Artemis Accords , non-binding principles on transparency, heritage sites and resource use that by 2025 had more than fifty signatories; China and Russia, outside it, signed their own agreement in 2021 for an International Lunar Research Station and are gathering a smaller bloc. Between the two sits the Wolf Amendment, a line in a 2011 American spending bill that bars NASA from bilateral cooperation with China without approval from Congress, which is why no Chinese astronaut has visited the International Space Station and why Tiangong exists.

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The treaty bans nuclear weapons in orbit, not weapons in general, and anti-satellite tests have gone ahead: the United States in 1985 and 2008, China in January 2007, creating more than 3,000 trackable fragments that still threaten spacecraft, India in March 2019, and Russia in November 2021, forcing the station crew to shelter in their capsules. In April 2022 the United States declared a unilateral moratorium on destructive direct-ascent tests and a United Nations resolution endorsing it passed with 155 votes. The US Space Force, established in December 2019, is the first new American armed service since 1947.

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Who decides? Formally, the United Nations committee in Vienna, by consensus, which means slowly. In practice, whoever lands first writes the rules by doing, as every frontier has found.

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Artemis: Back to the Moon

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Fifty years after Apollo 17 left the Taurus-Littrow valley, the United States is going back, this time with partners, with commercial landers and with a promise that the next footprints will be left near the lunar south pole. The programme is called Artemis , for Apollo's twin sister, and its heavy lifter is the Space Launch System , a 98-metre rocket that puts out 39 meganewtons at lift-off, about 15 per cent more thrust than a Saturn V. On top sits Orion , a 26-tonne capsule whose service module is built in Bremen by Airbus for ESA, so that Europe supplies the propulsion, power and air for every crew that flies.

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Artemis I proved the stack. It launched from Pad 39B on 16 November 2022, after two scrubs and a hurricane, and flew an uncrewed Orion for 25.5 days. The capsule entered a distant retrograde orbit tens of thousands of kilometres beyond the Moon, reached 432,210 km from Earth, farther than Apollo 13, and came home at 11 km per second to test the heat shield at lunar return speed. It splashed down off Baja California on 11 December 2022. The flight record is public, including the finding that the shield's Avcoat ablator had cracked and shed in unexpected ways, which cost more than a year of analysis before a crew was allowed to ride it.

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Artemis II flew the crew: Reid Wiseman, Victor Glover, Christina Koch and Canada's Jeremy Hansen, the first non-American to leave low Earth orbit. They launched on 1 April 2026, looped around the far side of the Moon on a free-return trajectory and splashed down in the Pacific on 10 April, a ten-day flight and the first by humans beyond Earth orbit since December 1972. Artemis III, planned to follow, is the landing, and it depends on a vehicle NASA does not own: SpaceX's Starship Human Landing System , which must be refuelled in orbit by a string of tanker flights before it can carry two astronauts from Orion down to the surface and back. The Gateway, a small station in lunar orbit, was proposed for cancellation in the 2026 budget request and its future is uncertain.

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Meanwhile the robots have gone first. Under the Commercial Lunar Payload Services scheme, NASA buys rides rather than building landers. Intuitive Machines' Odysseus reached the surface on 22 February 2024, the first American landing since Apollo, then tipped over on a broken leg. Firefly's Blue Ghost landed upright in Mare Crisium on 2 March 2025 and worked through a full lunar day. Each flight maps the terrain, tests the drills and the navigation that a crewed landing will need.

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The target is a ring of ridges near Shackleton crater , where sunlight falls for most of the year and ice may lie in the permanent shadow a few kilometres away. Thirteen candidate regions have been published. Apollo went to the Moon to prove a point; Artemis goes to stay, if the budgets and the tankers hold.

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The Moon Base

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A base on the Moon has been drawn since the 1950s, usually as a dome. The real one, if it is built, will be low, half-buried and placed with a surveyor's care near the south pole, because that is where the two things a base needs happen to be a few kilometres apart: light and water. On the rims of Shackleton and nearby ridges, the Sun circles the horizon and some spots are lit for more than 80 per cent of the year, the so-called peaks of eternal light . In the crater floors below, which have not seen the Sun for two billion years, the temperature sits at about 40 kelvin, cold enough to trap water ice indefinitely.

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The ice is not a guess. On 9 October 2009 NASA's LCROSS steered a spent Centaur stage into Cabeus crater at 2.5 km per second and flew through the plume: the spectrometers found about 5.6 per cent water by mass, plus hydroxyl, carbon monoxide and ammonia. India's Chandrayaan-1 had mapped hydration across the poles the year before, and China's Chang'e 6 brought back the first far-side samples in June 2024. Water means drinking, breathing and, split by electrolysis, rocket propellant. Oxygen can also be cooked out of ordinary regolith, which is 40 per cent oxygen by mass; ESA has demonstrated the molten-salt process in the laboratory.

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Shelter comes from the ground itself. Lunar regolith can be sintered with sunlight or microwaves into bricks, or printed layer by layer over an inflatable; ESA and Foster + Partners printed a 1.5-tonne demonstrator block in 2013. A metre of regolith halves the radiation dose; a lava tube would do far better. The Marius Hills pit, spotted by Japan's Kaguya orbiter in 2009, is about 65 by 90 metres across and opens onto a cavity that radar suggests runs for kilometres.

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Power is the hard constraint. At the equator the night lasts 14 Earth days and the surface falls to around −170 °C; solar panels and batteries alone cannot bridge it. NASA's Fission Surface Power project is designing a 40-kilowatt reactor to run for ten years, and China has said its base will include a nuclear unit. Two plans are now on the table: NASA's Artemis Base Camp , built with ESA, JAXA and Canada around a pressurised rover and a fixed habitat, and the International Lunar Research Station led by China and Russia, which has signed up more than a dozen partners and aims for a robotic phase in the 2030s.

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The far side offers one more prize: a radio-quiet site shielded from Earth's chatter, ideal for listening to the universe's first hydrogen. The Moon base will not be a dome, and it will not be quick. It will be a mine, a power station, a laboratory and a dust-management problem, and whoever learns to live there learns how to live anywhere else.

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Getting to Mars

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Mars is not far by the standards of the solar system, but it is awkwardly placed. Earth laps it every 780 days, and only around those alignments is the cheapest route open: the Hohmann transfer , a half-ellipse that leaves Earth tangentially and arrives at Mars tangentially seven to nine months later. Miss the window, which lasts a few weeks, and you wait 26 months for the next. Every Mars mission since Mariner 4 in 1964 has been timed by this clock, and so will the first crew.

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Leaving is the easy part. Arriving is not. Mars has just enough atmosphere to burn a spacecraft and not enough to slow it, which is why landing there is called the seven minutes of terror . Perseverance hit the top of the atmosphere on 18 February 2021 at 19,500 km per hour, took the heat of entry on a 4.5-metre shield, opened a 21.5-metre parachute at Mach 1.7, dropped the shield, steered by radar and camera to a safe spot, and was lowered on cables from a rocket-powered sky crane that then flew off to crash a safe distance away. All of it was autonomous; the radio delay was eleven minutes. The whole sequence tops out at about one tonne of payload. A crew habitat would weigh twenty to forty times that, and nothing yet flown can put it down.

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The bigger question is how long people must be away. A Hohmann round trip with the shortest wait at Mars, a so-called opposition-class mission, still takes about 18 months and often needs a Venus flyby; the fuel-efficient conjunction-class plan means 500 days on the surface and a total of nearly three years. Over that time Curiosity 's radiation detector, which measured 1.8 millisieverts a day in cruise, implies a dose approaching a sievert, close to a career limit. Robert Zubrin and David Baker's Mars Direct of 1990 attacked the mass problem by sending the return rocket first, empty, to make its own methane and oxygen from Martian air and a cargo of hydrogen, a trick now built into Starship's plan to refuel on the surface.

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Faster engines would help. The NERVA programme ground-tested nuclear thermal rockets in Nevada in the 1960s with roughly twice the efficiency of chemical engines, and DARPA and NASA revived the idea as DRACO in 2023 before ending it in 2025 when the cost no longer matched the benefit. Starship's answer is brute mass: refuel a 100-tonne-payload ship in Earth orbit with a dozen tanker flights, and the arithmetic of a crewed landing changes.

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How we know all this is the record of nine American landings, the Soviet Mars 3 that fell silent 20 seconds after touchdown in 1971, ESA's two lost landers, and China's Zhurong in 2021. Getting to Mars is a solved problem for a tonne of robot. For a hundred tonnes of people, every step but the launch is still a design.

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Living on Mars

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Mars is the most Earth-like place we can reach and still a place that kills in about two minutes without a suit. The average temperature is around −60 °C, the air is 95 per cent carbon dioxide at 0.6 per cent of Earth's sea-level pressure, there is no ozone layer and no global magnetic field, and the soil is laced with perchlorates , salts toxic to the thyroid, which the Phoenix lander measured at about half a per cent in 2008. Living there means making almost everything from what is already there.

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The first factory was the size of a car battery. MOXIE , bolted inside Perseverance , split carbon dioxide into oxygen by solid-oxide electrolysis at 800 °C. Between April 2021 and August 2023 it ran sixteen times and made 122 grams in total, with a peak of 12 grams an hour, roughly what a small dog breathes. Its principal investigator, Michael Hecht of MIT, called it a proof that the chemistry works in Martian dust and cold; a crew-scale plant would need to run several thousand times faster to fill an ascent vehicle's tanks.

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Water is underfoot. NASA's Subsurface Water Ice Mapping project combines radar, neutron and thermal data into charts of ice within a metre of the surface across the mid-latitudes, where Phoenix scraped it up in 2008 and ESA's Mars Express radar has traced it since. Buried ice solves two problems at once, because a habitat dug into it, or covered with two or three metres of regolith, cuts the radiation that an unshielded crew would take at about 0.7 millisieverts a day on the surface, around 250 times the dose on Earth.

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Then there is the mind. NASA's CHAPEA analogue put four volunteers, Kelly Haston, Ross Brockwell, Nathan Jones and Anca Selariu, into a 3D-printed habitat called Mars Dune Alpha at the Johnson Space Center for 378 days, from June 2023 to July 2024, with 22-minute communication delays, rationed food and simulated Marswalks in a sand-filled hall. Russia's Mars-500 had locked six men in a Moscow mock-up for 520 days in 2010 and 2011. Both studies found that food, sleep and the texture of boredom matter as much as the hardware. Closed-loop life support, which the ISS does for about 90 per cent of its water, must approach 100 per cent on Mars.

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Two cautions close the subject. Planetary protection rules, kept by COSPAR, limit where spacecraft may go until we know whether Mars has its own life to protect. And terraforming is not on: Bruce Jakosky and Christopher Edwards showed in 2018 that all the carbon dioxide Mars can be made to release would at best raise its pressure to a few per cent of Earth's. Mars will not be made into a second Earth. People may still live there, indoors, carefully, like submariners who happen to have a view.

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Asteroids: Defence and Mining

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On the morning of 15 February 2013 a rock about 20 metres across came in over the Russian city of Chelyabinsk at 19 km per second, exploded 30 km up with the energy of around 500 kilotons of TNT, and injured some 1,500 people, nearly all cut by glass as they stood at windows to watch the flash. No telescope had seen it coming; it arrived from the direction of the Sun. A century earlier, on 30 June 1908, a larger body flattened 2,000 square kilometres of Siberian forest at Tunguska without leaving a crater. Those two events are the case for planetary defence , and the case has recently gained a test.

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The surveys came first. Catalina, Pan-STARRS and ATLAS have catalogued more than 37,000 near-Earth objects and about 95 per cent of the kilometre-class bodies that could end civilisations; the shortfall is in the 140-metre class that would destroy a region, of which perhaps 40 per cent are known. NASA's NEO Surveyor , an infrared telescope planned for launch in 2027, is designed to find most of the rest from a vantage point where the Sun no longer hides them.

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Then the experiment. On 26 September 2022 NASA's DART spacecraft, 570 kilograms of mostly empty box, struck Dimorphos, the 160-metre moon of the asteroid Didymos, at 6.1 km per second. Ground telescopes timed the pair's eclipses before and after: Dimorphos's orbit around Didymos shortened from 11 hours 55 minutes to 11 hours 22 minutes, 33 minutes, more than 25 times the minimum needed to call the test a success. The ejecta did much of the work, pushing back like a rocket exhaust. Italy's LICIACube photographed the plume, and ESA's Hera , launched in October 2024, is due to arrive in late 2026 to weigh the crater and the body it left.

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Mining has had a harder decade. Planetary Resources and Deep Space Industries raised money in the 2010s on the promise of water and platinum from asteroids, and both were sold off by 2019 without flying a prospector. The legal ground was prepared anyway: the United States in 2015 and Luxembourg in 2017 passed laws granting companies title to resources they extract, a reading of the Outer Space Treaty that other states dispute. A newer company, AstroForge, launched a small probe in February 2025 toward an asteroid flyby and lost contact within days. The science missions have done better: Psyche , launched on 13 October 2023, is cruising on Hall thrusters toward a 220-kilometre metal-rich asteroid, with arrival planned for 2029.

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Whether mining ever pays depends on where the customer is. Platinum carried to Earth would crash its own market; water sold as propellant in orbit might one day be worth the journey. For now the asteroids have earned their keep in the other direction. We have moved one, on purpose, and measured it. No other species has ever been able to say that.

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Ocean Worlds

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The most promising places to look for life in the solar system are not on any surface. They are oceans sealed under kilometres of ice on the moons of Jupiter and Saturn, kept liquid by tidal flexing rather than sunlight. Europa alone is thought to hold about twice the water of all Earth's seas in a layer perhaps 100 km deep. The question that has reorganised planetary science over twenty years is simple: is anything swimming in it?

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The evidence began with Galileo , whose magnetometer in the late 1990s found that Europa and Callisto disturbed Jupiter's field the way a shell of salty, conducting water would. Then Cassini found the leak. In 2005 its cameras caught plumes of ice jetting from cracks near the south pole of Saturn's small moon Enceladus ; in 2008 and again in October 2015, when it flew just 49 km above the surface, its dust analyser and mass spectrometer sampled the spray directly. The grains carried sodium salts, silica nanoparticles and molecular hydrogen, the signature of hot water reacting with rock on a seafloor. Frank Postberg's team published the salts in 2009, Hunter Waite's the hydrogen in 2017. An ocean, warm vents, chemistry that could feed microbes: three of the four ingredients, with only the microbes unaccounted for.

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Now the fleet is on its way. NASA's Europa Clipper , the largest planetary spacecraft the agency has built at about 6,000 kg with solar arrays spanning 30 metres, launched on a Falcon Heavy on 14 October 2024 and is due at Jupiter in April 2030. Rather than orbit Europa inside Jupiter's radiation belts, it will orbit Jupiter and make 49 flybys, some as low as 25 km, carrying ice-penetrating radar, a magnetometer and spectrometers to measure the shell's thickness and sniff any plumes. ESA's JUICE , launched on 14 April 2023, arrives in 2031 and in late 2034 will become the first spacecraft to orbit a moon other than our own, Ganymede, which may hide the largest ocean of all.

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Titan gets a flying machine. Dragonfly , a car-sized rotorcraft with eight rotors and a radioisotope generator, is planned to launch in 2028 and land in 2034 in Saturn's moon's dunes, where the air is four times denser than Earth's and gravity a seventh, hopping tens of kilometres between sites to sample organic sands and the rim of an impact crater where water once pooled.

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Landing on Europa itself, or melting a cryobot through the ice, remains a study rather than a mission, partly because planetary-protection rules demand that nothing earthly reach a liquid ocean; Clipper will end by crashing into Ganymede, not Europa. How we will know, if we ever do, is the same way Cassini knew: a mass spectrometer, a salty grain, a molecule that should not be there. The oceans have waited four billion years. Dragonfly's arrival is pencilled for 2034.

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New Ways to Move

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Every rocket in this book so far has worked by burning something, and chemistry has a ceiling. The best hydrogen-oxygen engine ever flown, the RL10, manages a specific impulse of about 465 seconds, a measure of how much push each kilogram of propellant buys. That number is fixed by the energy in the chemical bonds, and it is why Mars takes seven months and the outer planets take a decade. The alternatives trade thrust for efficiency, and each has now flown.

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The ion engine throws xenon atoms out at 30 km per second using electricity rather than heat. NASA's Deep Space 1 proved it in 1998, running its NSTAR thruster for more than 16,000 hours at a thrust of 92 millinewtons, about the weight of a sheet of paper. Dawn then used three such engines to do what no chemical probe could: orbit Vesta in 2011, leave, and orbit Ceres in 2015, a total velocity change of 11 km per second. Hall thrusters, a Soviet design flown since 1971, now sit on every Starlink satellite and on Psyche , the first deep-space mission to use them. Their specific impulse is 1,500 to 3,000 seconds; their thrust would not lift a coin.

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Japan's IKAROS unfurled a 14-metre square of polyimide film 7.5 micrometres thick on 10 June 2010 and measured the push on its way to Venus, the first spacecraft propelled by sunlight. The Planetary Society's crowdfunded LightSail 2 raised its orbit with a 32-square-metre sail in 2019, and NASA's ACS3 deployed an 80-square-metre sail on composite booms in 2024. The Breakthrough Starshot study takes the idea to its limit: a gram-scale chip on a sail a few metres wide, driven by a 100-gigawatt laser array to 20 per cent of light speed in minutes. Nothing about it breaks physics; everything about it breaks current engineering.

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Heat is the other route. A nuclear thermal rocket passes hydrogen through a reactor and reaches a specific impulse near 900 seconds; the NERVA tests of the 1960s ran for hours in Nevada, and the DARPA–NASA DRACO demonstrator of 2023 was shelved in 2025 before it flew. Deep-space probes meanwhile depend on a quieter nuclear source: radioisotope generators turning the heat of plutonium-238 into electricity, 110 watts for Perseverance from 4.8 kilograms of oxide. The United States stopped making Pu-238 in 1988 and restarted at Oak Ridge in 2015, producing it by the gram, which is why outer-planet missions are rationed.

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One trick remains untried. Aerocapture, braking into orbit in a single pass through a planet's atmosphere, would save tonnes of fuel at Titan or Neptune, and no mission has yet dared it. The rocket equation has not been repealed. We have simply found more ways to argue with it, and the slowest-looking engines are now the ones that go furthest.

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Space Elevators and Other Big Ideas

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In 1895 Konstantin Tsiolkovsky looked at the new Eiffel Tower and imagined one so tall that its top would hang weightless in orbit. In 1960 the Leningrad engineer Yuri Artsutanov turned the tower upside down in a Sunday newspaper article, proposing a cable lowered from a geostationary satellite to the ground. Jerome Pearson worked out the engineering independently in 1975, and Arthur C. Clarke built a novel on it. The space elevator has been the most seductive big idea in spaceflight ever since, because the physics is clean and the material does not exist.

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The geometry is this. A satellite in geostationary orbit at 35,786 km above the equator stays over one spot. Extend a cable down from it to an anchor at sea, and another cable up to a counterweight at around 100,000 km, and the whole structure hangs in balance, pulled down by gravity below the geostationary point and flung out by rotation above it. Climbers would ride the cable on electricity, reaching orbit in days for a fraction of a rocket's energy. The catch is the tension. A cable of uniform cross-section would need a specific strength around 50 gigapascals per unit of steel density; steel manages about one. Carbon nanotubes measure over 100 in the laboratory, but the longest flawless fibres are centimetres long, and the cable needs to be 100,000 km. The Japanese contractor Obayashi published a plan in 2012 for a 96,000-km cable and climbers travelling at 200 km per hour, with a…

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Tethers have actually flown, briefly. On STS-75 in February 1996 the Shuttle Columbia reeled out the Italian-built TSS-1R satellite on a 20-km conducting tether; it generated 3,500 volts and nearly an amp from its motion through Earth's magnetic field before the tether burned through at 19.7 km. The experiment proved both the promise of electrodynamic tethers and their fragility. Rotating skyhooks, long tethers spinning in orbit that would snatch a suborbital vehicle and fling it higher, remain on paper.

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Gerard O'Neill's The High Frontier of 1976 offered a different order of ambition: cylinders 32 km long and 8 km across at the L5 point, spun for gravity and built from lunar rock thrown into space by an electromagnetic mass driver, which his Princeton students demonstrated on a bench. Paul Birch's orbital rings, the launch loop, the StarTram maglev tube and the gun-launch studies of the 1960s HARP project belong to the same family: use infrastructure, not fuel, to pay the cost of climbing out of the well.

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The sorting rule is simple. Physics allows the elevator, the skyhook, the mass driver and the cylinder; none breaks a conservation law. Engineering so far allows a 20-km tether that broke. The gap between those two sentences is where the next century of launch will be decided.

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Interstellar

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The farthest object humans have made is Voyager 1 , launched in 1977 and now about 25 billion kilometres away, roughly 170 times the Earth–Sun distance, still sending data at 160 bits per second. It crossed the heliopause, where the solar wind gives way to interstellar gas, in August 2012 at about 121 astronomical units. It is travelling at 17 km per second. At that speed it would take about 73,000 years to cover the 4.24 light-years to Proxima Centauri , and it is not pointed there; in around 40,000 years it will pass within 1.6 light-years of a dim star in Camelopardalis called Gliese 445. That is interstellar travel with today's engines.

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Serious designs for doing better are older than Apollo. Project Orion , studied by General Atomics from 1958 with Freeman Dyson among its physicists, would have pushed a ship with nuclear bombs exploded behind a pusher plate, a few thousand of them, and could in principle have reached a few per cent of light speed; the 1963 Partial Test Ban Treaty closed it. The British Interplanetary Society's Project Daedalus , published in 1978 after five years of volunteer work, specified a two-stage fusion rocket of 54,000 tonnes, fuelled with helium-3 mined from Jupiter's atmosphere, to reach Barnard's Star at 12 per cent of light speed in about 50 years. It remains the most detailed starship ever designed; nobody has built a fusion engine.

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The modern idea is to go small. Breakthrough Starshot , announced in 2016 by Yuri Milner with Stephen Hawking at his side, proposes a swarm of gram-mass chips on metre-scale sails, each boosted to 20 per cent of light speed in a few minutes by a 100-gigawatt ground laser, reaching Proxima in about 20 years and radioing back images of its planet, Proxima b, found in 2016. Every component is a research problem: the laser, the sail that must not burn, the camera that must survive dust at that speed. A more modest step is the Interstellar Probe studied by the Johns Hopkins Applied Physics Laboratory, a conventional craft that would use a close solar flyby to reach 1,000 astronomical units in about 50 years, seven times further than Voyager.

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The visitors came to us first. On 19 October 2017 Pan-STARRS in Hawaii found 'Oumuamua , an elongated object a few hundred metres long passing through the solar system on a hyperbolic path, the first known interstellar body; the comet 2I/Borisov followed in 2019 and a third, 3I/ATLAS, in 2025. They prove that material crosses between stars routinely. The ethics of a generation ship, whose crew would be born and die aboard without choosing the voyage, are debated more seriously than the propulsion.

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Four point two four light-years is 40 trillion kilometres. Light itself needs four years and three months. Interstellar flight is not forbidden; it is simply the point where the scales of human time and cosmic distance finally refuse to meet, and our oldest spacecraft is still, patiently, making the argument.

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Why Go?

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A hundred chapters in, the question deserves a straight answer. People give five reasons for going to space, and each has a critic worth hearing.

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The first is science , and here the record is strongest. The Apollo samples rewrote the Moon's origin as a giant impact; Venera showed a runaway greenhouse; Cassini found a habitable ocean; the Bennu grains returned by OSIRIS-REx in 2023 carried amino acids and the five nucleobases of DNA and RNA. The critic answers that robots do nearly all of this, more cheaply and without risk, and is largely right. Human spaceflight needs other grounds.

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The second is survival . Stephen Hawking said more than once that humanity should not keep all its eggs in one basket, and the asteroid record shows the basket is occasionally hit. The critic notes that no other world is remotely as hospitable as a damaged Earth, and that a colony of a few hundred would not save a species of eight billion for centuries. Both are true. Planetary defence, which DART proved possible in 2022, may be the version that actually pays.

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The third is the spin-off . First the myths. Tang was sold by General Foods from 1957, Teflon was discovered at DuPont in 1938, and Velcro was patented by a Swiss engineer in the 1950s; NASA used all three and invented none. The genuine list is better than the fake one: the CMOS active-pixel sensor in every phone camera was developed at JPL in the 1990s by Eric Fossum's team to shrink spacecraft cameras; memory foam came from Ames in 1966; the water filters, insulin pumps and fire-resistant fabrics each have a traceable patent. The critic asks whether a direct research grant would have bought the same for less, and nobody can prove it either way.

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The fourth is perspective . Frank White named the overview effect in 1987 after astronauts told him that seeing the whole Earth, thin-skinned and borderless, had changed them. Carl Sagan made the same point with Voyager 1's photograph of 14 February 1990, a pale blue dot smaller than a pixel, taken from six billion kilometres. Against this stands Gil Scott-Heron's "Whitey on the Moon" of 1970, which asked why a rat bit his sister Nell while the money went to the Moon, still the best short argument on the other side. NASA today takes about 0.4 per cent of the US federal budget, a tenth of its 1966 share; European agencies spend proportionally less.

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The fifth reason is that we are the kind of animal that goes, which is not an argument at all, and may be the true one. The next fifty years, soberly: a lunar outpost, crewed Mars flights that slip, oceans under ice sampled by robots, many more satellites and a treaty under strain. Whether it is worth it is not a question the engineers can settle. It is the reader's, and this book has tried only to see that the answer is given with the numbers in hand.

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Roll the dice