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On January 2nd, 1959, with|the space age barely a year old, the Soviet Union|launched Lunik - "little moon". It was sent to plant|a Soviet pennant on the moon. Within hours of the launch,|it became clear that Lunik was going|to miss its target. As the Soviet scientists|watched their tiny probe sail out to join the planets in an endless journey|around the sun, an inspired thought|occurred to them. They renamed their spacecraft|Mechta - "The Dream". (Music: The Planets|by Gustav Holst) In 1926, when this recording of|Holst's Planets suite was made, there were thought|to be eight planets. Then, in 1929, a young man arrived|at an observatory in Flagstaff, Arizona,|to start the search for a ninth. At that time, little|was known about the planets. Closest to the sun lies Mercury, a tiny world of iron and rock,|barely discernible in the glare. Then Venus,|perhaps a second Earth, hidden beneath|a blanket of cloud. Then Earth. And beyond us, Mars,|the Red Planet. It has seasons, polar caps, and the possibility of life. Far beyond these rocky worlds|are the distant giants. Jupiter, over 1,000 times|bigger than the Earth, and Saturn, with its distinctive|and dramatic rings. The two remaining planets are 15 times the size|of the Earth, yet are so distant that they appear|as the faintest of stars. Uranus - an aquamarine mystery. And finally, Neptune, a world that moved|unevenly across the sky. This irregular movement suggested the presence|of a more distant planet, whose gravitational tug might be|toying with Neptune's orbit - Planet X. 'February 18th, 1930. 'Clyde Tombaugh,|sitting in an office 'very near to where we are now, 'looking at the photographs he|had taken of the night sky...' With his eye at the eyepiece of|the blink comparator back there. 'And he had been|searching on the plates 'that were centred on a star 'in the constellation|of Gemini, the Twins.' He had started that morning. He had moved slowly across, click, click, seeing one image, then the other,|keeping on moving back. 'All these images were|negative, all the stars. 'And anything else would be|black on a white background. 'At 4pm, he crossed|the plate's centre. 'He passed the area|where the guide star was. 'The star Delta Geminorum -' big, big bright star. He moved a little bit more,|a little bit more, 'and then he saw a very faint,|a very faint black dot.' Then he blinked to the other one|on the other plate, 'and he saw it appear|here and there.' On his plates,|taken several days apart, Tombaugh noticed that|a point of light had moved. He knew instantly this was|what he was looking for. It was an historic moment. 'He took the walk|from the comparator room, 'all the way down|to the director's office, 'and he stopped, did his tie|and combed his hair a little, 'and said "I wanted to appear|a little nonchalant about this." 'Then he stepped|into the office... (Clears throat) "Dr Slipher? I have|found your Planet X." Planet X was soon named Pluto. It marks the end|of the solar system. A tiny world of ice,|smaller than our moon, now known to have|its own satellite, Charon. But Pluto patrols the outer edge|of the solar system, in the distant realm of giants. Worlds of swirling water,|like the azure Neptune, and Uranus, which|mysteriously orbits the sun spinning on its back. Pluto lies way beyond|the gargantuan worlds, the gas planets|that have no landscapes: Saturn, with wind reaching thousands|of kilometres per hour, and Jupiter,|that has an Earth-sized storm that has lasted for centuries. The closest worlds to the sun are small islands|of rock and iron. Mars, with its faint atmosphere|of carbon dioxide, and Venus, smothered|in clouds of sulphuric acid. Then there is Mercury, boiling in sunlight,|and freezing at night. Nine different worlds, with|seemingly little in common, save that they orbit|a single sun and are bound together|by its gravity. And then there is the Earth. A small planet in the measure|of the solar system. It has a thin atmosphere|that clings to a rocky surface. But the Earth is different.|It is special. It has life. What process could create such|a variety of different worlds? Hal Levison is at the forefront|of a branch of astrophysics that is still struggling|with the mystery of how the planets formed. 'It's amazing,' when you consider that all planets in the solar system: the Earth and the rocky planets, the cores of the giant planets,|Jupiter and Saturn, and the majority|of the outer planets, Uranus, Neptune and Pluto, formed from material that is|very fine pieces of dust, much finer than the dust|I'm holding in my hand. About the consistency or size of particles of dust|in cigarette smoke. I was an astrophysicist, interested in an obscure type|of galaxy, when five years ago I got the bug|of trying to understand how material like this can form|the planets we see today. By the 18th century, astronomers|had discovered that galaxies are filled with drifting clouds|of gas called nebulae. Perhaps these clouds were the|raw materials of the planets. Two men, the philosopher|Immanuel Kant and the mathematician|Simon de Laplace, looked at the uniform direction of the orbits|of the planets in the sky. They suggested the planets|were a relic of a cloud of dust and gas that circled|the sun during its formation. In a single process,|they concluded, the solar system was born. The idea was elegant,|and quite brilliant, but the complex details|of their theory lay centuries in the future. Its proof had to wait for|the arrival of the space age. September 1944.|London was under siege. Mysterious weapons|were raining down from the sky. Hitler's vengeance weapon|threw people into confusion. Nothing had prepared them|for a supersonic missile that took just six minutes|to travel from mainland Europe. The technology behind these|missiles was highly advanced. It had been developed|by a brilliant young engineer called Wernher von Braun. Von Braun's rocket|was called the V-2. Designed to save the war for|the Nazis, eventually it became the foundation|of our journey to the planets. When Germany fell, American troops headed|straight for the V-2 factories. Before the dust|had settled in Europe, von Braun and his team|of engineers found themselves working|for the United States Army. In the deserts of New Mexico,|the captured rocket parts were reassembled|by German and US engineers. The modified V-2s soon flew|beyond the range of cameras. Engineers fixed|astronomical telescopes to anti-aircraft gun mounts. The system|was designed by Clyde Tombaugh, the discoverer of Pluto,|and his films still survive. The Americans destroyed|the German rocket factories to keep von Braun's secrets|from the advancing Red Army. But when they arrived, the Soviets found enough|to take back to Moscow. The man given the task of|piecing together the rockets was Sergei Pavlovich Korolev, and Boris Chertok|was his right-hand man. While their brief|was to develop rockets which could reach America, Korolev's eyes were firmly|fixed on the planets. But it was the Americans|who made all the early running. By the end of the decade,|they were strapping film cameras to rockets, and sending them|high above the atmosphere. The cameras had to endure an|18-mile plummet back to Earth. Miraculously, some survived, and astronomers got their|first glimpse of the only planet they couldn't see|with their telescopes. For the first time, we could|see the curvature of the Earth. The arcing horizon|was a humbling reminder that we were living on a|gigantic ball of rock and iron. How such a world could have|grown from a cloud of dust seemed more baffling than ever. George Wetherill|has dedicated his career George Wetherill|has dedicated his career to the question|of planet formation. When he started, the science|was dominated by one man. No great scientist|ever devoted his life to understanding this problem. It was sort of a hobby, something they did on the side. And I think the first person to|really devote his life to this was a Russian scientist|named Victor Safronov, who started|working on these problems shortly after World War II. And he tried to identify what|all the scientific problems are that you need to understand|and need to solve, in order to understand|the grand problem of the formation|of the solar system. And to this day, his lists|of problems are essentially the same problems|that we're working on today. Victor Safronov|revisited the 200-year-old idea that the planets formed|from a disc of gas and dust. He set about structuring|this complex process into comparatively|simple stages. The first stage|is still not fully understood. Remember, we're starting off|with very fine pieces of dust, and the process|of how you get from that to something the size of|a boulder, or even a mountain, is actually|not very well understood. The party line of what most|people think actually happened, was that you had|this disc of dust. Dust settled into the mid plain|of this protoplanetary nebula. 'And you got what's called|gravitational instability 'that formed big clumps, 'things maybe the size|of 100 metres in diameter.' Safronov's second stage|was less complex. It was called accretion. He calculated that in|a remarkably quick time, the clumps|would gather together, building the embryos of planets. As they grew, a new force|became significant - gravity. 'An amazing thing happens that|Victor Safronov discovered.' That is, as these things|start to grow, the bigger something gets,|the more it can eat. So you end up|with this runaway situation, where the bigger guys|are getting bigger still, and it's sort of a race|to eat up the little guys. And so you start off|with an un-countable number of objects|the size of mountains. And you end up with maybe 100, in the inner part|of the solar system, objects the size of the Moon,|going up to the size of Mars. Competing worlds|sucked in the surrounding debris until there was simply|no more to be had. In the inner solar system, where|there are now four planets, there were once|upwards of 100. How that army of worlds became|just four was still a puzzle. But Victor Safronov had a hunch that the process|would leave those planets spattered|with the scars of impact. Was this what we could|see on the moon? Unknown to the West, Safronov|had taken a giant stride towards a theory|of planet formation. Perhaps, somewhere|in the solar system, there might be a planet bearing|the hallmarks of his theory. In 1957, the Americans announced that they were preparing|to enter the space age. They were about to launch the world's first|artificial satellite. In the Soviet Union,|Korolev acted immediately. 'For Korolev,|it was the beginning 'of the race with Americans.' And he wanted to be first, ahead of the Americans, like all of us. And I think he wanted to do this maybe 100 times|more than any others. 'Then he called my father|and told him, '"I want to launch|this first satellite.' "Let's do this before the|Americans, as soon as we can." It would be a huge gamble, but finally Khrushchev|agreed to let him try. Now Korolev had to convince his|engineers they could do it too. On October 4th, 1957, while the Americans were still|finalising their plans, Sputnik was launched. (Beeping) (Beeping) (Beeping) 40 years on, Korolev's achievement|is still celebrated in Russia. 'That evening,|he was very proud, 'he realised|it was a great achievement.' And next day, he understood the|reaction of the outside world was much stronger|than it was in our country, and the feeling was much|stronger than even his feeling, specially in the United States. Korolev's rockets|had opened the door to space. The planets were beckoning. Bruce Murray is a veteran|of the US space programme. When his career started, the planets seemed|a very long way away. He still remembers|the first time he saw Mars through a telescope. And it just blew me away. I was so taken with the fact that here was a real object, it was three-dimensional,|or seemed to be. 'It was colourful, glowed,|and really drove home to me' there's a place out there,|a real place, not just something|I studied in school somewhere. As a young man, Bruce Murray|was taken under the wing of physicist Bob Leighton,|who had developed a way to make time-lapsed films|of the planets. The images were extraordinary|because they could show the planet rotating, you could|time-lapse it, take one frame, wait a minute, take another|frame, and make a time-lapse. And it brought to everybody|the image of Mars that the most dedicated|astronomers only infer, because they have to|remember all those frames. And he did it for fun. Leighton's films|brought the planets to life. For the first time, astronomers could see|one of the moons of Jupiter orbiting its giant parent. 'The outer planets, 'the ones that are|huge masses of gas, 'in the case|of Jupiter and Saturn, 'you could actually|see some beautiful structure.' The first thing,|as in the inner solar system, is diversity - "My Lord,|everything is different." But Mars,|the Earth's smaller cousin, was always|the most tantalising. Leighton could see|mysterious dark patches rotating with the planet. But what would a close encounter|with the surface reveal? In 1964, the American|probe Mariner 4 set off to send back the first|pictures from another planet. 'Bob Leighton was charged|with bringing back the images.' ..and blue clouds, oh, yes... 'He asked Bruce Murray|to join him.' 'I was dragged or sucked along,|however you want to look at it,' into this wonderful experience, of becoming the first|experimenters to look at Mars through a close-up camera. 'This is|Mariner Control Center at JPL. 'The spacecraft is 134.217|million miles from Earth 'and 50,142 miles from Mars.' After a journey of eight months, Mariner 4 was homing|in on its target. 'The first picture will|cover an area of approximately '176 miles square on|the sunlit bit of the planet.' I wish I was as sure as he is! 'About four minutes from now,|we should be able to determine 'the camera shutter is operating 'and that|the recorder is running.' The anticipation|of not just the scientists, but the public and news media,|was incredible, because Mars was thought to have|life, and in the popular mind, maybe it had Martians,|as far as we were concerned. Mariner 4 was a fly-by. It would get only one chance|at the pictures. '..the scan position for 5605|is 323. Congratulations.' 323! Exactly where|they wanted her! 10,000 miles from the surface, Mariner 4's cameras|whirred into life. These signals came back - if you|think of one picture element, one sample of light - the rate|at which these came in from Mars was one of these per second. - Hey! Here we go.|- There she goes. That's data! And so it took three weeks for|our 20 pictures to come back. Give me Bruce Murray's|phone number. Where the devil are|the Mars picture interpreters? Yeah, data's coming in, boy.|What are you doing in bed? There we go. We got some pictures. The planet was not|what they had expected. There was no sign|of life here. No vegetation. Just picture after picture|of a dull, flat landscape. It wasn't until frame 12 that the first features|became visible. 'What we could see|were these huge craters. '300 kilometres, 200-mile|craters across, on Mars.' Impact craters - and that meant that Mars|was preserving a signature from its earliest times,|3 or 4 billion years ago. So we had a major conclusion,|stunning everybody, from these|very few pictures we got. When the news filtered|through to the Soviet Union, one man wasn't as surprised|as his Western rivals. Craters were exactly|what Victor Safronov expected. Soon, Safronov's ideas were|being discussed in the West, where superior technology|allowed George Wetherill to take|the accretion theory further. 'I'd called it|the planetesimal problem.' That says there's a lot|of objects, small planets, moving around the sun in orbits. What you want to understand|is how they accumulate together to form large planets. Wetherill's computers uncovered a terrifying period|of planet formation. 'What you find if you do|the problem with the computer' is that, as they grow, they|start to perturb one another into orbits which cross|the orbit of another planet. Soon, the neat orbits|of Safronov's army of planets became fatally disrupted. As they started|tugging each other off course, the solar system|was brimming with loose cannon. World-shattering collisions|were inevitable. 'George realised that|it was like a wild frat party.' All hell breaks loose|in the inner solar system. Stuff either hits the sun|or gets thrown out to Jupiter, and out of the solar system. It's a very violent,|happening party. If Wetherill was right, during this period,|the inner solar system must have been strewn|with planetary debris. The four surviving planets|would have had to endure a final stage|of intense bombardment. In 1973, George Wetherill|got the chance to test his work. Mariner 10|was on its way to Mercury. 78 million kilometres|from Earth, beyond the scope of the most powerful telescopes, the surface of this planet|was a total mystery. 'A few months|before the Mercury mission,' I was in a meeting|where people discussed what we might find on Mercury,|to get thinking about Mercury. A very distinguished|planetary astronomer in answer to a question,|proclaimed that Mercury would have|no craters, or few. The curious thing is|that the craters on Mars were also a surprise|to most planetary astronomers. After a journey|that took in a fly-by of Venus, by February, Mariner 10|was nearing its target. 'Subsequently,|I was invited to JPL' and sat in a little room|above mission control and saw the pictures coming in. 'The first pictures of Mercury|showed just a fuzzy ball.' You could imagine seeing|craters, but then it got closer. Soon, it started|to look like the Moon. Mercury was the most cratered|planet in the solar system. One impact was so great that it left|shock waves set in stone on the other side of the planet. It was proof of the final stage|of the accretion theory. I was just thrilled by this.|I knew they were there, but actually seeing them,|that I'd been thinking about all these years,|and now here they are. It made me very excited. And all these military|men around kept saying, "Isn't that beautiful? It's|just like a 52 drop in 'Nam." Here, then,|are the inner planets. The survivors|of a life-or-death struggle. Mercury, Venus and Mars. Each bearing|the scars of creation. But what of the Earth? Surely our planet could not|have survived unscathed? In the field, Hal Levison gets|a real sense of the violence that rained down on the planets,|including our own. This hole in the ground|was made in a matter of seconds. Despite being an awesome sight, 'something that tells us the|solar system is still active 'and that things are still|running into each other,' 'It's a relatively insignificant|hole in the ground. 50,000 years ago, a 50-metre|fragment of a world blown apart billions of years earlier|careered into the Earth in what is now Arizona. Here is evidence of|the final stages of accretion. But what of the worlds|that dwarf the inner planets? How does the accretion theory|account for the gassy giants that rule the distant regions|of the solar system? We have different planets|as we get farther from the sun, because as you get farther from|the sun, the temperatures drop. About four times more distant|from the sun than the Earth is, we hit a point where water would|condense and become a solid. With water turning to ice, the|amount of material available to form the outer planets|was far greater. Jupiter and Saturn grew so large|that they started sucking in the primordial gases|from the original dust cloud, swelling them to hundreds|of times the mass of the Earth. This region had many more worlds|than exist today. Their orbits|were also disrupted. We can find no traces of impacts|in their gassy atmospheres, but evidence can be seen|in their rotation. It is believed that a world|the size of the Earth collided with Uranus. Today, Uranus still rolls|around the sun on its back. When did these planet-building|impacts come to an end? 'I've found a lot of comets. 'I've helped|discover 21 of them.' There is nothing like the night we found the Shoemaker-Levy 9. We had no idea how important|that discovery was going to be. 'It made page 23|in the London Times, 'that Carolyn and Jean Shoemaker|and I discovered this comet.' Interest increased|several months later, when it was announced|that Shoemaker-Levy 9 was on a collision course|with Jupiter. This was not page 23 of the|London Times, it was page 1. It was a different story. Shoemaker-Levy 9 was going|to show us what it's all about. In all civilisation, since Galileo first looked|through a telescope, in 1609, and since he first|looked at Jupiter, in 1610, this is the first time we've|seen a comet strike a planet. July 16th, 1994. Impact day. And every available telescope|is trained on Jupiter. Look! Oh, my God! Look at that! 'It's how the solar system was|built, comets hitting planets. 'Comets first hitting|each other. 'Very slowly, almost an embrace|rather than a collision,' then these objects get bigger|and their gravity gets bigger, the speed gets higher,|and it gets more violent. The teenage solar system|has become dysfunctional. And finally, when does it end? 'What Shoemaker-Levy 9 taught us|is it hasn't happened yet.' Right then,|in the summer of 1994, around Jupiter, there's|a big yellow police fence, that says danger, keep out,|solar system under construction. It's still happening. Jupiter grew a little bit during|the week of July 16, 1994. 'Water was dumped on Jupiter. 'It had more|carbon sulphide down there.' It was as if nature had said, "OK, guys, I'm going|to show you how it works, "and all you have|to do is watch it." Here, then, are the gas giants. Jupiter and Saturn|mark the current limit of the plant builders' theories. Far beyond these gargantuan|worlds lie the ice giants, Uranus and Neptune. But out here, the accretion|theory runs into trouble. 'The formation|of Uranus and Neptune 'are the greatest mysteries|in the solar system,' because everything goes more|slowly at greater distances from the sun, so all|these processes slow down. When we try to run the same|computer programs out there that we did|in the terrestrial planet zone, we don't get planets forming. No matter what we do,|we can't form Uranus and Neptune using these kind of models. 'I can't make|Uranus and Neptune go away.' They're there,|and our models can't make them. So we do indeed|have a long way to go before we really|figure all this out. How these worlds formed|so quickly is a puzzle. Scientists don't know enough|about early conditions this far from the sun. What kinds of worlds|went into the formation of Uranus and Neptune? In 1992, two astronomers|were surveying the space beyond Neptune when they found|a substantial chunk of ice. Since then,|they have found many more. Called the Kuiper Belt,|it is now thought that they are the building blocks|of ice giants that never were. 'The Kuiper Belt is a region|where the small ice mountains 'that we've talked about|started accreting and building 'into larger things. 'To me, that's the region|we need to look at, 'because planet formation|started there,' and it was frozen in at some intermediate state. Understanding that will tell us in detail how accretion started, but what shut it off|is also going to be interesting, and will tell us something|about the process. So to me, the future lies in the|outer part of the solar system. But there is a planet that lies at the inner edge|of the Kuiper Belt. 70 years after its discovery,|the strange, tiny world of Pluto may at last be making sense. 'Pluto was discovered in 1930,' and it was the oddball|of the solar system. Most of the planets are in nice|circular orbits. Not Pluto. Most are set in this plane that|represents the accretion disc. Not Pluto. And it was just an oddball,|it was small and icy, different to anything|else that we knew about. Could this small, icy world|be a survivor of accretion? A world that somehow|escaped being swallowed up by the growing Neptune, or being|hurled out of the solar system? Could Pluto be the missing link in the formation|of the ice giants? 'Turns out Pluto was just|the largest known member 'of this population. 'It went from being|this lonely remote oddball,' to being essentially the|grandfather of a population. And the Kuiper Belt|probably has more objects than any other region|in the solar system. It's the most populous region and yet we didn't know|about it 10 years ago. In the 40 years|since Mechta broke free from the Earth's gravity, we've|sent probes to all the planets. We've sampled|the corrosive clouds of Venus, and recorded planet-wide|thunderstorms on its surface. We've survived|dust storms on Mars, and seen canyons|that could swallow countries. We've mapped|the icy moons of Jupiter, and plunged into its atmosphere. We've skimmed|the rings of Saturn. We've seen active geysers on the most distant and freezing|moon in the solar system. But just as the first|stage of our reconnaissance of the planets draws to a close, we have|a new region to explore. In 1992, Clyde Tombaugh|got a request from NASA - permission to visit his planet. 'Clyde was melted. He melted|when he got that letter. 'He felt that all of his life's|effort and work with Pluto, 'his work at White Sands,|was coming to a head.' He felt that letter|was really a sign that NASA, through their mission to Pluto, was finally acknowledging him|as the man that he really was. Clyde Tombaugh died in 1997. Pluto Express is planned|to launch in 2003. It will take 12 years|to reach its goal. After analysing|Pluto's composition, it will head out in search|of a Kuiper Belt object. Perhaps something in their|cratering record or chemistry will provide the final piece|of the creation jigsaw. Whatever the craft finds,|Pluto's importance in the grand order|of the solar system is assured. It will be a manned mission to|Pluto in a very special sense. It's not going to have|a real living person, but you can bet it's going|to have Clyde's spirit on board on its way to Pluto,|to see what kind of a planet |
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