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Over 100,000 of you have been working hard scouring an unexplored | :00:11. | :00:14. | |
area of Mars. Your efforts have paid off. You have made an | :00:14. | :00:18. | |
incredible discovery on the surface of the Red Planet. We will be | :00:18. | :00:21. | |
revealing all tonight. I'm Brian Cox. He is Dara O Briain. This is | :00:21. | :00:31. | |
:00:31. | :00:56. | ||
Welcome back to a very foggy Jodrell Bank Observatory. So foggy | :00:56. | :01:03. | |
we can hardly see the big dish. Not a great night for stargazing. It is | :01:03. | :01:07. | |
the third and final night of this year's Stargazing Live. Thank you | :01:07. | :01:10. | |
for your questions. We have some remarkable viewer photographs that | :01:10. | :01:17. | |
I want to show you. This is the Orion Nebula. We saw it on the | :01:17. | :01:27. | |
:01:27. | :01:28. | ||
first night. This is a picture - it is taken with a 4.5 inch reflector. | :01:28. | :01:36. | |
26 30-second exposures. This was taken last night. This one, | :01:36. | :01:45. | |
California Nebula. Is it because it's the shape of California? | :01:45. | :01:54. | |
It was taken on the 9th. This one is the jewel in the crown in many | :01:54. | :02:04. | |
ways. It may not look like it. It's - we now know - a comet. It was | :02:04. | :02:14. | |
:02:14. | :02:18. | ||
discovered, or the photograph was taken by Nick Howes in the States. | :02:18. | :02:25. | |
On Monday night, the stargazers at the school - this is now a comet. | :02:25. | :02:29. | |
That is a genuine discovery. As we mentioned, we have made some | :02:29. | :02:33. | |
interesting discoveries on the surface of Mars. Chris Lintott will | :02:33. | :02:37. | |
be back later in the programme to reveal all. There is much more to | :02:38. | :02:41. | |
stargazing than these TV shows. There are over 500 events taking | :02:41. | :02:45. | |
place up-and-down the country for you to get some hands-on with | :02:45. | :02:49. | |
astronomy. I have some pictures. I want to show you what everybody has | :02:49. | :02:55. | |
been doing. Here is one. This is the Canterbury Star Party. 1,200 | :02:55. | :03:01. | |
guests turned up to Canterbury on Tuesday 8th. This is them showing | :03:01. | :03:09. | |
how to make rockets with a vitamin tablet. This is the Eden Project. | :03:09. | :03:19. | |
:03:19. | :03:20. | ||
1,500 guests on 8th January. Finally, this one - that is nice. | :03:20. | :03:25. | |
Where was that? Birmingham. This is people from Birmingham University | :03:25. | :03:31. | |
explaining how gravity works. One last picture. This one was sent in | :03:31. | :03:38. | |
by Private Eye. There is Dara O Briain looking very handsome and | :03:38. | :03:43. | |
Buzz Lightyear! To find an event near you, go to | :03:43. | :03:50. | |
bbc.co.uk/stargazing. We will be going to see how Mark got on with | :03:50. | :03:56. | |
the Herschel Telescope. Among his many claims to fame, Herschel | :03:56. | :04:01. | |
coined the term "asteroid". It means star-like in Greek. In five | :04:01. | :04:07. | |
weeks' time an asteroid 45 metres wide is going to pass between us | :04:07. | :04:11. | |
and the Moon, coming closer to Earth than some of our satellites. | :04:11. | :04:21. | |
:04:21. | :04:22. | ||
In March, the comet Panstarrs will streak by in the sky followed by | :04:22. | :04:32. | |
:04:32. | :04:43. | ||
Ison. This was taken on 9th. Ison will pass very close to the Sun. If | :04:43. | :04:50. | |
it survives that encounter with the Sun, it could break up, it will | :04:50. | :04:58. | |
sweep out in January 2014 - it could be one of those comets that | :04:58. | :05:05. | |
you see in a tapestry! Fantastic. We are going to pass through the | :05:05. | :05:10. | |
tail of that later in March. It may give us a meteor shower. Fantastic. | :05:10. | :05:13. | |
We have had lots of questions. "What is the difference between | :05:13. | :05:19. | |
asteroids, comets and meteors?" We have to keep on explaining this. | :05:19. | :05:26. | |
Comets are large dirty snowballs. Yes. They are icy with some rock | :05:26. | :05:29. | |
mixed in. They come from distant regions of the Solar System. We | :05:29. | :05:36. | |
will see that later on in regions called the Kuiper belt and the Oort | :05:36. | :05:42. | |
Cloud. The comets are spectacular. We have some fantastic footage. | :05:42. | :05:48. | |
This is a beautiful shot from the International Space Station. Looks | :05:48. | :05:54. | |
like some kind of computer graphic. That is Comet Lovejoy. Lovejoy was | :05:54. | :05:58. | |
discovered in December 2011 by Terry Lovejoy in Australia. Here it | :05:58. | :06:02. | |
is passing behind the Sun. Remarkable piece of footage. Here | :06:02. | :06:12. | |
is another video. This is from the Solar Observatory. The thing about | :06:12. | :06:16. | |
comets - you tend to think of them streaking along. The tail is blown | :06:16. | :06:21. | |
by the solar wind. The Sun is heating the comet up. You are | :06:21. | :06:26. | |
getting gas and dust erupting. it is moving away from the Sun, it | :06:26. | :06:32. | |
follows its own tail? Yes. Asteroids are more like rocky | :06:32. | :06:38. | |
fragments of planets. Yes, this is the first asteroid we encountered | :06:38. | :06:43. | |
in space. This is not a video. This is Eros. It's about 34 kilometres | :06:43. | :06:48. | |
long, which is about the size of the thing that - if it hit us, it | :06:48. | :06:52. | |
would be the size that killed all the dinosaurs. It doesn't cross the | :06:53. | :06:58. | |
Earth's orbit at the moment. It crosses Mars' orbit, though. | :06:58. | :07:05. | |
Because it continually crosses the orbit of Mars, it could be | :07:05. | :07:11. | |
perturbed by Mars. We landed on the surface of that asteroid. When we | :07:11. | :07:16. | |
talk about meteors and meteoroids, they interact with our atmosphere. | :07:16. | :07:26. | |
:07:26. | :07:28. | ||
Meteors are when they burn up. Meteor showers. What are they? | :07:28. | :07:33. | |
is a meteor shower in December. The reason for that is that they were | :07:33. | :07:38. | |
created by a comet. They are the remains of the tail of a comet. | :07:38. | :07:45. | |
you think about what a comet does. It orbits the Sun. So they leave an | :07:46. | :07:49. | |
ellipse of debris and that will sit there in orbit around the Sun in | :07:49. | :07:53. | |
the place where the comet tracks around. The Earth passes through it | :07:53. | :07:57. | |
at the same point in its orbit every year. And that is why you | :07:57. | :08:00. | |
always see them coming from the same place. That is how meteor | :08:00. | :08:10. | |
:08:10. | :08:11. | ||
showers are named. So one of the things we want to | :08:11. | :08:16. | |
talk about is the big asteroid coming our way very soon. It is | :08:16. | :08:20. | |
called Asteroid 2012 DA14. On Friday February 15th it will pass... | :08:20. | :08:28. | |
Here it is. That is how close it is going to come! These are our | :08:28. | :08:32. | |
satellites. The green blobs are the satellites. It will come well | :08:32. | :08:37. | |
within the orbit of the station. will pass on 15th February. This is | :08:37. | :08:41. | |
going to be more pressurised Valentine's Day so do something | :08:41. | :08:50. | |
good on the 14th February! It will miss us by a mile! How can we be so | :08:50. | :08:58. | |
sure that this trajectory is so right? Liz Bonnin is standing by | :08:58. | :09:03. | |
for us at the Goldstone Observatory. Welcome to Goldstone in the Mojave | :09:03. | :09:13. | |
Desert. This is the Mars Antenna, part of NASA's Deep Space Network. | :09:13. | :09:18. | |
Now, I'm inside the base of the antenna and presently, it's | :09:18. | :09:27. | |
tracking the New Horizon's Mission to Pluto. Marina, you are one of | :09:27. | :09:31. | |
the scientists that does that work. How does tracking an asteroid work? | :09:31. | :09:36. | |
It is simple. You point it to the asteroid and you bounce on some | :09:36. | :09:43. | |
mike waves. This allows you to get its location very precisely -- | :09:43. | :09:48. | |
microwaves. This allows you to get its location very precisely. | :09:48. | :09:54. | |
were tracking Apophis last night. Scientists thought it was going to | :09:54. | :09:59. | |
hit us. What is the latest? Well, we have been tracking it since late | :09:59. | :10:02. | |
December and what you are seeing here are the images from this | :10:02. | :10:07. | |
morning. Is that Apophis? What you are looking at, this is a 300 metre | :10:07. | :10:12. | |
diameter object that is 14.5 million kilometres away and we have | :10:13. | :10:16. | |
the detection. Radar data that we have collected have completely | :10:16. | :10:22. | |
excluded any chance of impact. We are safe. That is good news. | :10:22. | :10:29. | |
Furthermore, we can now precisely predict its trajectory decades into | :10:29. | :10:36. | |
the future. Fantastic work. As well as tracking, you get a good | :10:36. | :10:40. | |
resolution from these orbits. This is Toutatis. This is a prime | :10:40. | :10:47. | |
example of what radar can do. This is 4.6 kilometre-long asteroid. It | :10:47. | :10:55. | |
was 7.5 million kilometres away from Earth. We are getting | :10:55. | :10:59. | |
resolution to resolve surface boulders. Wonderful technology. | :10:59. | :11:02. | |
Scientists are also getting a better idea of the composition of | :11:02. | :11:06. | |
asteroids with their latest work. What is clear is that there are | :11:06. | :11:11. | |
many more different types than previously thought. Amy Mainzer, | :11:11. | :11:19. | |
another NASA scientist, taught me how to make my own. | :11:19. | :11:27. | |
We have asteroids that are solid lumps of metal. Take some of this | :11:27. | :11:34. | |
dirt and spoon it in. Step one - all asteroid also have some type of | :11:34. | :11:39. | |
dirt? That's right. You have silicon in here, all kinds of | :11:39. | :11:44. | |
heavier elements and that's going to be the basic constituent of most | :11:44. | :11:50. | |
asteroids. We will pour some of that water in and make a big mess. | :11:50. | :11:55. | |
One theory about why there's so much water on Earth is that some | :11:55. | :11:59. | |
arrived here aboard comets and asteroids. That's not the only | :11:59. | :12:09. | |
:12:09. | :12:14. | ||
familiar substance found in them. Let's take some of this molasses. | :12:14. | :12:20. | |
How much? That's pretty good. This one is carbon-rich! Now we need a | :12:20. | :12:23. | |
squirt of another ingredient that has been found in the remains of | :12:23. | :12:32. | |
asteroids that have landed on Earth, ammonia. Then we add our final | :12:32. | :12:38. | |
ingredient - dry ice. At minus 78 centigrade, it will mimic the | :12:38. | :12:43. | |
freezing conditions of the Solar System. Sprinkle that in there. We | :12:43. | :12:50. | |
will freeze it up good. Let's take a look and see what we have ended | :12:50. | :12:59. | |
up with. Amazing! That is what we got. In true asteroid-style, it is | :12:59. | :13:03. | |
beautifully irregular. It is not completely round. Oh my goodness! | :13:03. | :13:09. | |
This asteroid is a very particular kind, a randomly active main belt | :13:09. | :13:14. | |
object. A Rambo, would you believe?! It is special. We have | :13:14. | :13:19. | |
discovered in the last ten years or so this very unusual class of | :13:19. | :13:23. | |
asteroid that becomes active. Active in what way? These things | :13:23. | :13:27. | |
exhibit huge clouds of gas and dust coming off the surface. What | :13:27. | :13:32. | |
happens is when the Sun hits the objects, we use this bright lamp to | :13:32. | :13:37. | |
represent the Sun, what we think happens is that a smaller asteroid | :13:37. | :13:43. | |
may strike the surface and scrape off some of this dirty outer layer | :13:43. | :13:48. | |
and it may expose some of the ice. Look at that jet coming out from a | :13:48. | :13:51. | |
tiny little hole and you can't see any of the ice exposed? That's | :13:51. | :13:54. | |
right. This is a really good example of what we think happens. | :13:54. | :13:58. | |
If we were orbiting the Sun, this object would have a big tail around | :13:58. | :14:04. | |
it. And a big halo following it. Almost two years ago, the Hubble | :14:04. | :14:07. | |
Space Telescope photographed a Rambo which grew a tail when it was | :14:07. | :14:13. | |
heated by the Sun and just there is its X-shaped impact scar. Closer to | :14:13. | :14:18. | |
home, what is the worst that could happen to the Rambo we have made? | :14:18. | :14:24. | |
This is a good sized lump of rock. How can this really cause that much | :14:24. | :14:28. | |
damage? Well, something this small obviously can't. If something were | :14:28. | :14:32. | |
the size of a building, like 30 or 40 metres in diameter, it would be | :14:32. | :14:36. | |
large enough to make it through the Earth's atmosphere. Now you have | :14:36. | :14:41. | |
something that can cause a great deal of damage because if it is | :14:41. | :14:45. | |
travelling at 10 kilometres a second or more, it packs an | :14:45. | :14:53. | |
enormous punch. Amy has now joined us at Goldstone. You use Space | :14:53. | :14:58. | |
Telescopes to find out potentially dangerous asteroids. Tell me about | :14:58. | :15:02. | |
the project? It's a Space Telescope that used infrared light to | :15:02. | :15:07. | |
discover and track near Earth asteroids. Infrared is heat. We are | :15:07. | :15:11. | |
sensing heat. It gives us an idea of the size of the object. We can | :15:11. | :15:13. | |
tell the difference between something that is really large but | :15:13. | :15:18. | |
dark, like a piece of coal, or something that is much smaller, but | :15:18. | :15:21. | |
highly reflective. OK. Getting the size is important for understanding | :15:21. | :15:30. | |
We sampled some of the population and used it to look at what is out | :15:30. | :15:35. | |
there. What have you come up with? For objects that are larger than a | :15:35. | :15:39. | |
kilometre, like the dinosaur killing object, 90% of these have | :15:39. | :15:44. | |
been found. What about the other 10%? We don't know where they are | :15:44. | :15:48. | |
yet. There's another piece of not so good news which is that for | :15:48. | :15:53. | |
objects larger than 100 metres, we've only discovered 25% of those. | :15:53. | :16:00. | |
They can cause great damage. Absolutely. You need to continue | :16:00. | :16:04. | |
this surveying work. We have a lot more work to do. What happens if a | :16:04. | :16:11. | |
big one is coming at us? Ideally we will find an object 20 to 30 years | :16:11. | :16:18. | |
before it will happen. If we have time like that, we can design | :16:18. | :16:21. | |
strategies that would use explosives to push the asteroid | :16:21. | :16:26. | |
aside or break it into pieces or maybe even devised technology to | :16:26. | :16:31. | |
target out the way. How? A either gravitationally or attaching solar | :16:31. | :16:37. | |
sails. Astonishing. Thank you. Come back to us when we talk about | :16:37. | :16:44. | |
emissions and more about asteroids and comets. Standing by it on our | :16:44. | :16:48. | |
live block is Don. He is head of NASA's near earth objects | :16:48. | :16:55. | |
department. He will be informed if an asteroid is heading our way for | :16:55. | :16:59. | |
a start -- he will have to inform the President. He can take your | :16:59. | :17:03. | |
questions at bbc.co.uk/stargazing. A lot of people are asking where | :17:03. | :17:08. | |
these objects originate from. We have a model for you. All of the | :17:08. | :17:15. | |
asteroids we ever encountered... Everything comes from three places. | :17:15. | :17:19. | |
We have an animation that shows just the asteroid belt ter, between | :17:19. | :17:25. | |
Mars and Jupiter and it is the Mars and Jupiter and it is the | :17:25. | :17:27. | |
green area. Every point is a map position of an asteroid. This is | :17:27. | :17:34. | |
what it looks like. It is a bit of a mess, which is why we get impact. | :17:34. | :17:38. | |
The asteroid belt is packed with Rocky objects, including this one. | :17:38. | :17:44. | |
This is called Vesta. I have an image of it. It is quite a big rock. | :17:45. | :17:51. | |
It is about 350 kilometres in diameter. The remarkable thing | :17:52. | :17:59. | |
about Vester is I have a piece of it here. This came from there. The | :17:59. | :18:05. | |
mystery will be revealed later. It mystery will be revealed later. It | :18:05. | :18:11. | |
is beautiful. This is the Kuiper belt. Faces a region of IAC, rocky | :18:11. | :18:18. | |
object. This is where Pluto lives. It was demoted because it turn | :18:18. | :18:22. | |
Celtic is one week -- one of many objects of a large size in the | :18:22. | :18:29. | |
Kuiper belt. We are on our way to Pluto at the moment. This is a | :18:29. | :18:35. | |
picture of a spacecraft on its way. It left in January 2006. When it | :18:35. | :18:39. | |
left Pluto was a planet. When it got to about there, Pluto was | :18:39. | :18:45. | |
demoted, but by that time it was too late to stop. It makes no | :18:45. | :18:46. | |
too late to stop. It makes no difference to the mission. These | :18:46. | :18:51. | |
are the best images we have of Pluto now. They are from the Hubble | :18:51. | :18:56. | |
Space Telescope. It is extremely cold. We don't know a lot about | :18:56. | :19:03. | |
Pluto other than these images. is ice. For is an ice, about -200 | :19:03. | :19:10. | |
Celsius. Finally you step into this region, the far reaches of the | :19:10. | :19:15. | |
solar system, the Kuiper belt. This is a picture of the Oort cloud, a | :19:15. | :19:22. | |
spherical cloud. This is a disc of the solar system? Yes. This is more | :19:22. | :19:27. | |
spherical. It is a vast collection of large and small lumps of ice and | :19:27. | :19:33. | |
rock. It stretches out about a light year, we think. A quarter of | :19:33. | :19:37. | |
the way to the nearest star. Nearly all of the Committee's wheezy come | :19:37. | :19:43. | |
from either the Kuiper belt or the Oort cloud. -- comets we see. | :19:43. | :19:47. | |
wanted to work out what things were in danger of hitting. We need to | :19:47. | :19:51. | |
know where the Earth is at any time. How do we were kicked out? The | :19:51. | :19:53. | |
How do we were kicked out? The answer lies in the southern | :19:53. | :20:02. | |
hemisphere's guy. -- southern- hemisphere sky. This is an iconic | :20:02. | :20:07. | |
constellation. It even features on the Australian national flag. It | :20:07. | :20:11. | |
was by interpreting patterns have stars in the sky that we began to | :20:11. | :20:18. | |
make sense of our cosmic surroundings. On Earth, it is easy | :20:18. | :20:22. | |
for me to work out my position relative to the object I can say. I | :20:22. | :20:26. | |
can understand my place in this world. If you're an astronomer, you | :20:26. | :20:30. | |
have a problem because all you can see on little points of light in | :20:30. | :20:35. | |
the sky and for the early astronomers, they knew nothing more | :20:35. | :20:39. | |
than that. To make progress, people began to make maps of the night sky | :20:39. | :20:46. | |
end as much detail as possible. He this is an early start shot of the | :20:46. | :20:53. | |
southern sky from 1801. It is a two dimensional representation of the | :20:53. | :20:58. | |
position of the stars. This is the Southern Cross. When you follow | :20:58. | :21:05. | |
what you get to the bright southern star. 200 years ago, the way these | :21:05. | :21:12. | |
maps were made meant their accuracy was limited. When he made this map, | :21:12. | :21:16. | |
he did it by hand. He looked at this guy and transcribed the | :21:16. | :21:21. | |
positions of the stars on to this piece of paper. A huge opportunity | :21:21. | :21:27. | |
for human error in that process. But in the late 19th century, a new | :21:27. | :21:33. | |
technique allowed astronomers to achieve real precision. Photography. | :21:33. | :21:37. | |
If you have a photograph, a plate and a telescope, the marks on a | :21:37. | :21:42. | |
plate are not made by the human hand, they are made by photons of | :21:42. | :21:47. | |
light that have travelled from the stars themselves, hundreds or even | :21:47. | :21:54. | |
thousands of light-years to register their position on the map. | :21:54. | :21:59. | |
By fitting a camera to a telescope, the accurate positions of thousands | :21:59. | :22:03. | |
of stars could be recorded in a single exposure. Something | :22:03. | :22:10. | |
astronomers hoped would help them determine our place in the universe. | :22:10. | :22:15. | |
In 1887, a decision was taken to map the position of every star that | :22:15. | :22:20. | |
can be seen in this guide with high precision. That was a project that | :22:20. | :22:30. | |
:22:30. | :22:32. | ||
An incredible commitment, like building a cathedral. Much of the | :22:33. | :22:38. | |
southern sky was mapped here, at Sydney Observatory, and this is one | :22:38. | :22:42. | |
of the photographic plate that was used Clinton's -- to construct the | :22:42. | :22:46. | |
used Clinton's -- to construct the Astra graphic catalogue. An | :22:46. | :22:52. | |
exposure, just over six hours, and you can see very faint black dots | :22:52. | :22:59. | |
on the plate. Each one of these black dots is a star and the | :22:59. | :23:03. | |
positions were measured and transcribed into here. The Astra | :23:03. | :23:13. | |
:23:13. | :23:13. | ||
graphic catalogue. This is 1893, John Reid 20th. Documenting the | :23:13. | :23:21. | |
positions of the stars in this photograph. What we have here is a | :23:21. | :23:24. | |
perfect representation of the positions of the stars in the sky | :23:24. | :23:34. | |
:23:34. | :23:35. | ||
from Sydney on January 20th, 1893. 750,000 stars were recorded at | :23:35. | :23:39. | |
Sydney Observatory and the results were combined with surveys made at | :23:39. | :23:43. | |
19 other observatories around the world, creating a single, huge | :23:43. | :23:49. | |
catalogue of the stars across both hemispheres. For the very first | :23:49. | :23:54. | |
time, astronomers had an accurate record of our position relative to | :23:54. | :23:59. | |
4.5 million stars. That has helped us to make another intriguing | :23:59. | :24:05. | |
characteristic of the stars with great precision. In the 1990s, | :24:05. | :24:10. | |
these measurements were repeated, this time by a satellite the | :24:10. | :24:16. | |
European Space Agency Bill. What was found was that for at least | :24:16. | :24:22. | |
some of the stars, their positions had changed an appreciable amount. | :24:22. | :24:29. | |
For his slow drift is unique to each star and because it takes | :24:29. | :24:33. | |
years to become apparent, comparing recent satellite data with this | :24:33. | :24:37. | |
catalogue has given us the most accurate ever record of this | :24:37. | :24:45. | |
phenomenon. He the reason for this movement is that all of the stars | :24:45. | :24:49. | |
in the Milky Way are a orbiting around the centre of the galaxy, | :24:49. | :24:58. | |
but each at its own particular speed. Today, even deeper in the | :24:58. | :25:04. | |
universe, it is not just stars fat have their own unique motion. -- of | :25:04. | :25:11. | |
that have. By looking out beyond the stars in the Milky Way, we | :25:11. | :25:15. | |
found that all the galaxies in the universe on moving relative to each | :25:15. | :25:21. | |
other as well. We are part of a group loan -- known as a local | :25:21. | :25:24. | |
group. 43 galaxies bound together in the same way the stars are bound | :25:25. | :25:30. | |
together in the Milky Way. That group itself is moving roughly in | :25:30. | :25:37. | |
that direction to something called the Super cluster, a group of 5,000 | :25:37. | :25:42. | |
galaxies or more, about half a billion light years in that | :25:42. | :25:48. | |
direction. And we are travelling towards this enormous cluster of | :25:48. | :25:54. | |
galaxies that is over 500 -- at over 500 kilometres per second. | :25:54. | :25:58. | |
What we discovered over hundreds of years of astronomy, making | :25:58. | :26:02. | |
precision measurements of the sky, is that everything in the universe | :26:02. | :26:08. | |
is moving relative to everything else. We've learned that the stars | :26:08. | :26:13. | |
and galaxies are all taking part in a vast cosmic doused which we -- | :26:13. | :26:23. | |
:26:23. | :26:26. | ||
dance which we can now plot with We have all of these objects in an | :26:26. | :26:31. | |
Orbit around the sun. Why are some of them suddenly lurching out on | :26:31. | :26:36. | |
these crazy journeys? The answer, as with every answer, lies with | :26:36. | :26:41. | |
mathematics. We've got Tim O'Brien to explain. The mathematics of | :26:41. | :26:47. | |
this? You remember that all these objects orbiting around the Sun a | :26:47. | :26:52. | |
doing it under Newton's law of gravity. It turns out that there's | :26:52. | :26:57. | |
only four possible shapes of orbits they can have. They are really -- | :26:57. | :27:01. | |
the really neat bit of mascot those shapes are defined by slices | :27:01. | :27:08. | |
through a core. Depending on what angle you slice through, you get a | :27:08. | :27:12. | |
circular Orbit, and elliptical Orbit, a Parabolica or Orbit or a | :27:12. | :27:18. | |
hyperbolical bit. Fees are in her elliptical orbits, some of them a | :27:18. | :27:23. | |
more secular. But in general, everything... They go round and | :27:23. | :27:30. | |
back. A most common or bits of the elliptical and hyperbolic her. | :27:30. | :27:35. | |
Hyperbolic Orbit is open. If something gets bumped into a | :27:35. | :27:38. | |
hyperbolic Orbit, that will go around the same place as before, | :27:38. | :27:43. | |
but it will shoot off. Yes, and it never comes back. It goes out into | :27:43. | :27:49. | |
interstellar space. The difference is essentially to do with energy | :27:49. | :27:53. | |
and angular momentum. Let's say we are in the Kuiper belt and | :27:53. | :27:59. | |
something has a gravitational interaction. It interacts with lets | :27:59. | :28:06. | |
a Pluto. It will change the energy of that object. It will change the | :28:06. | :28:09. | |
Orbit because these shapes are defined partly by the energy. One | :28:09. | :28:14. | |
of these things can be perturbed spirit begins a journey into the | :28:14. | :28:21. | |
inner solar system. Halley's Comet, which came from the Oort cloud, | :28:21. | :28:26. | |
that comes in. It is still an ellipse. It is. A period of 76 | :28:27. | :28:31. | |
years, it comes back every 76 years. It could have jumped from a | :28:31. | :28:37. | |
circular Orbit into an elliptical Orbit. Because of an interaction. | :28:37. | :28:45. | |
The Oort cloud is interesting because it is so far out. Many of | :28:45. | :28:50. | |
the perturbations come from passing stars. They are very weakly bound. | :28:50. | :28:58. | |
The false drops away. -- force. bombed sit by passing and Zenit | :28:58. | :29:02. | |
heads off on a new journey. These hyperbolical orbits are interesting. | :29:02. | :29:06. | |
You don't see them coming because they come in and they have such an | :29:06. | :29:11. | |
Orbit that they go round once and disappear. Something perturb them | :29:11. | :29:20. | |
and dumps them. It is gone and we Bonevacia him again! Maybe some | :29:20. | :29:26. | |
time he will pass you. Let's find out if there are clear skies where | :29:26. | :29:36. | |
:29:36. | :29:37. | ||
you are tonight. Let's go to Susan We are up against it this evening | :29:37. | :29:41. | |
thanks to a lot of cloud piling into the UK. To the east of the UK, | :29:41. | :29:45. | |
we have had a weather front that has hung around for much of the day | :29:45. | :29:49. | |
today. So that will obscure the skies here. Further west, another | :29:49. | :29:52. | |
front that's fizzling out. We will lose the rain but the cloud is | :29:52. | :29:57. | |
going to stick around. Between the two, a few clearer spells across | :29:57. | :30:01. | |
the North West and for Northern Scotland. My top picks for the | :30:01. | :30:11. | |
:30:11. | :30:12. | ||
clearest skies - it will be in the west. And give it a couple of hours | :30:12. | :30:16. | |
and Northern Ireland will be looking almost crystal clear. | :30:16. | :30:23. | |
More information as ever on the BBC More information as ever on the BBC | :30:23. | :30:27. | |
Weather website. Thanks. Mark Thompson has been | :30:27. | :30:32. | |
building a modern interpretation of William Herschel's 20-foot | :30:32. | :30:42. | |
:30:42. | :30:47. | ||
telescope. Anyway, in a tribute to his work, | :30:47. | :30:52. | |
Mark has been trying to re-create that telescope. | :30:52. | :30:56. | |
Over the past three weeks, I have been working with the local | :30:56. | :31:00. | |
community in Derby and a crack team of experts. We have had to make | :31:00. | :31:06. | |
changes to Herschel's plans to keep everyone safe, but we have remained | :31:06. | :31:11. | |
true to his principles. So far, we have built the supporting structure. | :31:11. | :31:16. | |
Big, isn't it? Now we have the small matter of making the | :31:16. | :31:25. | |
telescope. In Herschel's Telescope, right at the bottom of the tube was | :31:25. | :31:29. | |
a piece of polished metal to reflect the light from the stars. | :31:29. | :31:33. | |
It was shaped and positioned to focus the light towards the top of | :31:33. | :31:37. | |
the tube and here, Herschel would have stood on this viewing platform | :31:37. | :31:41. | |
and looked down the barrel through an eye-piece. This is our telescope | :31:41. | :31:45. | |
tube. We will put a mirror up this far end. So light comes down the | :31:45. | :31:50. | |
tube, hits the mirror, bounces back up the tube and then all the way up | :31:50. | :31:54. | |
to the top into this special adjustment we have made. We have | :31:54. | :31:57. | |
had to cut some of the tube out where the eye-piece is going to go | :31:57. | :32:00. | |
and hopefully, we will see some stunning views of the sky through | :32:00. | :32:05. | |
it? Want me to push? Not too much! Now we need to get it up into the | :32:05. | :32:15. | |
:32:15. | :32:16. | ||
cradle. Chris Hill is on hand to supervise. That will do. That's it. | :32:16. | :32:23. | |
It is finally starting to look like a telescope. Inside the university | :32:23. | :32:28. | |
workshop, Chris is putting the final touches to the mount for the | :32:28. | :32:34. | |
mirror. An instrumentation expert is here with the missing piece. | :32:34. | :32:40. | |
It's arrived! We are using a modern glass mirror in our telescope. | :32:40. | :32:44. | |
Herschel would have used a piece of metal and that would have easily | :32:44. | :32:49. | |
tarnished. Even though he polished it for hours, it still wouldn't | :32:49. | :32:56. | |
have been very reflective. Herschel would have been blown away by this. | :32:57. | :33:00. | |
Yes, this would have been his Christmases! The mount has a set of | :33:00. | :33:06. | |
screws on the back, so that the angle can be adjusted. Now, we can | :33:06. | :33:10. | |
align the mirror. So the light from the stars is reflected through the | :33:10. | :33:16. | |
eye-piece. Shall we put it in then? Let's try it. The time has come. | :33:16. | :33:24. | |
Yeah. You got the screws? Back a bit. There! The first step is to | :33:24. | :33:28. | |
cover the opening with a large sheet of paper. For the next bit, | :33:28. | :33:32. | |
Herschel would have probably used a candle but we are going to use a | :33:32. | :33:38. | |
laser pointer. The light travels through a small hole in the paper, | :33:38. | :33:42. | |
down the tube and hits the mirror at the bottom. It is reflected back | :33:42. | :33:47. | |
at an angle to hit the paper again. I need to guide Chris to adjust the | :33:47. | :33:52. | |
mirror. Until the reflected laser light moves into position where the | :33:52. | :33:56. | |
eye-piece will be. Chris, if you can tilt the bottom towards me so | :33:56. | :34:03. | |
bring that away from you? Got you! Can you see it moving? Yes, keep | :34:03. | :34:09. | |
going. Woah! Spot on! How is that looking? Perfect. Excellent. That | :34:09. | :34:13. | |
is perfect, mate. Well done. This laser beam is simulating star light | :34:13. | :34:17. | |
and it is bouncing back out of the tube which is where I need to look. | :34:17. | :34:23. | |
If I spray this, you can see where the beam is coming out the tube. It | :34:23. | :34:30. | |
shows that we are ready for some clear skies! | :34:30. | :34:35. | |
After all that work, the time has come to reveal the telescope. Let's | :34:35. | :34:40. | |
cross live to Mark at the University of Derby. | :34:40. | :34:50. | |
There is a fantastic atmosphere. We have our own Herschel quintet. We | :34:50. | :34:55. | |
have the children from the school here. CHEERING We have also got the | :34:55. | :35:03. | |
members of the Derby Astronomical Society. Hello, guys. Now it's | :35:03. | :35:09. | |
taken us five weeks and hundreds of man hour. It weighs in at just | :35:09. | :35:15. | |
under half a tonne. It is Stargazing Live's Herschel | :35:15. | :35:20. | |
Telescope. CHEERING Now, it is the most amazing piece of kit. It has a | :35:20. | :35:24. | |
crank to turn the whole telescope. The whole structure moves around so | :35:24. | :35:28. | |
that you can access any part of the sky that you want to. It is the | :35:28. | :35:32. | |
most amazing piece of kit. Hopefully, we might get a chance to | :35:32. | :35:37. | |
look through the telescope. With me is Professor Alan Chapman. Alan, | :35:38. | :35:42. | |
what do you make of it? It is absolutely remarkable. It is a | :35:42. | :35:46. | |
tremendous realisation of Herschel's Telescope, using | :35:46. | :35:50. | |
scaffolding and modern equipment. I have never seen anything like it | :35:50. | :35:54. | |
before. Me neither! Even to the chaps pushing it around. Herschel | :35:54. | :35:59. | |
probably used sailors! We have used the same tube dimensions, the same | :35:59. | :36:04. | |
mirror diameter. We only had a drawing to work from. It took him a | :36:04. | :36:13. | |
year. We did it in five weeks. That is incredible? To him it was | :36:13. | :36:16. | |
entirely experimental and a brilliant piece of inspired | :36:16. | :36:25. | |
engineering. Herschel was a skilled worker with his hands. He employed | :36:25. | :36:32. | |
carpenters to do the heavy work for him. Yet, Herschel was a skilled | :36:32. | :36:37. | |
musician. A string player, a keyboard player and I think all of | :36:37. | :36:41. | |
those skills were necessary to the manipulation and adjustment of that | :36:41. | :36:47. | |
instrument. I will have to stop you there. Thanks to the guys from the | :36:47. | :36:51. | |
Derby Rugby Team. I'm really looking forward to looking through | :36:51. | :36:54. | |
the telescope. It is still cloudy here. It is foggy in Derby. With a | :36:54. | :36:58. | |
bit of luck, it may clear up. Do come back to us later on tonight | :36:58. | :37:03. | |
and we will see if we can re-create the images that Herschel saw. | :37:03. | :37:08. | |
Hopefully we will. We have been talking about asteroids and comets. | :37:08. | :37:12. | |
Of course, we will be struck by large objects from space. It's | :37:12. | :37:15. | |
happened all through history. It isn't necessarily a bad thing. | :37:15. | :37:19. | |
Without these impacts, our world might not be the place that we know | :37:19. | :37:23. | |
today. If you want to see one of the best | :37:23. | :37:28. | |
preserved meteor impact sites on Earth, you need to travel to the | :37:28. | :37:32. | |
Barringer crater in Arizona. Craters can be found all over the | :37:32. | :37:37. | |
Solar System like this. The battle scars of a long history of impacts. | :37:37. | :37:42. | |
Most are the result of one period, around 3.6 billion years ago, when | :37:42. | :37:47. | |
the whole Solar System was turned upside-down. It was all to do with | :37:47. | :37:52. | |
the combined gravitational force of our two biggest planets, Jupiter | :37:52. | :38:00. | |
and Saturn. We now believe that the giant planets formed much closer to | :38:00. | :38:09. | |
the Sun than they are today. Their orbits drifted hundreds of millions | :38:09. | :38:14. | |
of years until Jupiter and Saturn fell into a regular pattern. Once | :38:14. | :38:19. | |
every cycle the two planets aligned creating a gravitational surge that | :38:19. | :38:29. | |
:38:29. | :38:29. | ||
played havoc with the orbits of all the planets. Neptune was catapulted | :38:29. | :38:35. | |
outwards and smashed into the ring of comets surrounding the Solar | :38:35. | :38:41. | |
of comets surrounding the Solar System with dramatic consequences. | :38:41. | :38:48. | |
For 100 million years, the Solar System turned into a shooting | :38:48. | :38:55. | |
gallery as the comets ploughed through it. Millions of comets were | :38:55. | :39:00. | |
scattered in all directions peppering the planets. It was | :39:00. | :39:09. | |
called the Late Heavy Bombardment. It created many of the craters we | :39:09. | :39:15. | |
see throughout the Solar System today. It left scars all over our | :39:15. | :39:25. | |
:39:25. | :39:25. | ||
Moon. And it had a lasting impact on the Earth as well. The only | :39:25. | :39:29. | |
impact craters we see on Earth today, like this one in Arizona, | :39:29. | :39:34. | |
were made much more recently, but they reveal the scale of these | :39:34. | :39:44. | |
:39:44. | :39:47. | ||
impacts. Today, impacts like this are relatively rare. They will | :39:47. | :39:57. | |
:39:57. | :39:58. | ||
happen again. But during the late Late Heavy Bombardment, the | :39:58. | :40:03. | |
environment was changed radically and dramatically. Those changes | :40:03. | :40:07. | |
weren't necessarily catastrophic. It's now thought that a significant | :40:07. | :40:13. | |
amount of the water in the Earth's oceans was delivered by the impacts | :40:13. | :40:17. | |
of water-rich comets and other objects during the Late Heavy | :40:17. | :40:21. | |
Bombardment. That means that impacts could have played a key | :40:21. | :40:31. | |
:40:31. | :40:33. | ||
role in the development of life on Earth. Before the Late Heavy | :40:33. | :40:42. | |
Bombardment, the Earth was a barren rock. Afterwards, it supported the | :40:42. | :40:47. | |
oceans that would become the Crucible for life. Without the | :40:47. | :40:52. | |
water delivered in the Late Heavy Bombardment life on Earth may never | :40:53. | :40:57. | |
have evolved. All this may have been caused by the violent | :40:57. | :41:07. | |
:41:07. | :41:10. | ||
gravitational pull generated by two Joining us now is Dr Richard | :41:10. | :41:14. | |
Greenwood. We have seen one of your fantastic samples already. | :41:14. | :41:19. | |
talked about Vesta. It is from Australia. It has a special | :41:19. | :41:25. | |
composition that we know matches Vesta. One billion years ago, a | :41:25. | :41:33. | |
meteorite smashed into the southern hemisphere of Vesta. They drifted | :41:33. | :41:38. | |
into the three to one resonance with Jupiter and it is a real | :41:38. | :41:42. | |
conveyer belt. We have ten times as many meteorites coming from Vesta | :41:42. | :41:47. | |
as we have from the Moon, or Mars. That is remarkable. It is to do | :41:47. | :41:52. | |
with this gravitational interaction with Jupiter throwing these things | :41:52. | :41:58. | |
our way. Absolutely. This is iron? That is. If we pick it up, you will | :41:58. | :42:01. | |
see it is three times denser than a rock that you find in your garden. | :42:01. | :42:06. | |
It is pure metal. It is the core of an asteroid that melted. When it | :42:06. | :42:11. | |
melted, the metal sank and formed a core. We used to think these were | :42:11. | :42:16. | |
quite young. That is one of the oldest objects in the Solar System. | :42:16. | :42:23. | |
The reason for that is - at that time, they had a short | :42:23. | :42:27. | |
concentration of Aluminium 26. That would have been formed in a | :42:27. | :42:34. | |
supernova. Yes. It's probably the shockwave from the supernova that | :42:34. | :42:42. | |
triggered the collapse which formed Within two million years, which is | :42:42. | :42:48. | |
a small length of time, it would have gone. These are relatively | :42:48. | :42:53. | |
unstable and made in a supernova explosion? Exactly. Heated the | :42:53. | :43:01. | |
asteroids up. That is why you get the iron sinking? That's right. | :43:01. | :43:11. | |
:43:11. | :43:11. | ||
is not the oldest thing? This fell in Tanzania, it is called Ivuna. | :43:11. | :43:18. | |
That is some of them there. In there, there are diamonds, graphite | :43:18. | :43:26. | |
and they came from some of the stars that pre-dated... This is | :43:26. | :43:33. | |
older than the Solar System? Yes. 4,567 million years. That is older. | :43:33. | :43:37. | |
That is older. The story of the origin of the Solar System is a | :43:37. | :43:41. | |
supernova went off, a shockwave came through this gas and dust, | :43:41. | :43:45. | |
that caused it to collapse and pieces of that shockwave - this is | :43:45. | :43:50. | |
from outside the Solar System? Exactly. And got trapped? Yes. | :43:50. | :43:57. | |
Startling. Technology now allows us to get up close and personal with | :43:57. | :44:01. | |
asteroids and comets whilst they are still in orbit. Let's go back | :44:01. | :44:05. | |
to Liz in the Goldstone Observatory to hear more. Thank you very much. | :44:05. | :44:08. | |
Goldstone and the rest of the Deep Space Network have communicated | :44:08. | :44:12. | |
with some truly remarkable missions getting us very close to asteroids | :44:12. | :44:16. | |
and comets that are speeding through space. Amy, if we can talk | :44:16. | :44:26. | |
:44:26. | :44:28. | ||
about a few of them? Stardust? Stardust Mission flew through the | :44:28. | :44:32. | |
comet and it collected tiny pieces of the comet and it brought them | :44:32. | :44:36. | |
back to Earth. It has given us a new window into the Solar System. | :44:36. | :44:45. | |
None of that material has changed for 4.5 billion years? Exactly. | :44:45. | :44:50. | |
Deep Impact Mission does what it says on the tin? Exactly. It was | :44:50. | :44:56. | |
two spacecraft in one. An impacter spacecraft and an observer. They | :44:56. | :45:01. | |
separated when they got close to a comet. The observer watched and | :45:02. | :45:07. | |
allowed us to see the inside of the comet. What have we learned from | :45:07. | :45:10. | |
that material? It was a really surprising result. It turns out | :45:10. | :45:16. | |
that this particular comet was more dust than water-ice. Also, the | :45:16. | :45:26. | |
:45:26. | :45:33. | ||
They have a lot more in common than we thought. And then for Dawn | :45:33. | :45:38. | |
Mission which sent an order to do my to it -- mighty fester. It has | :45:38. | :45:42. | |
been orbiting Vesta and it has returned spectacular images that | :45:42. | :45:46. | |
have allowed us to see the turbulent history that has happened | :45:46. | :45:53. | |
to this asteroid. Two giant impact craters on the South poll of the | :45:53. | :45:58. | |
asteroid and joy and scrapes that I even larger than the Grand Canyon. | :45:58. | :46:04. | |
Thank you for joining us. Dawn is on its way to Ceres, the biggest | :46:04. | :46:09. | |
rock in the asteroid belt, 950 kilometres in diameter and it has | :46:09. | :46:15. | |
been declassified as a dwarf planet. It will reach it in 2015 and will | :46:15. | :46:21. | |
begin its exploration then. That space around our planet is not | :46:21. | :46:24. | |
just filled with natural objects, it is also filled with staff and we | :46:24. | :46:32. | |
put up there. So much stuff that there's a pilot waiting to happen. | :46:32. | :46:36. | |
He in a quiet corner of Hertfordshire is a radar tracking | :46:36. | :46:41. | |
station that is used to monitor the movement of objects 2000 kilometres | :46:41. | :46:45. | |
above the earth. There are lots of things we got up | :46:45. | :46:52. | |
there. 1,000 satellites, nearly 20 telescopes and one space station. | :46:52. | :46:56. | |
But there's also a lot of junk, affectionately known as space | :46:56. | :47:02. | |
debris. So space debris is effectively all of the stuff in | :47:02. | :47:07. | |
space we know longer use or need. It could be dead satellites, did | :47:07. | :47:12. | |
rockets, fragments, pieces of electronic circuits, pieces of | :47:12. | :47:14. | |
paint from the outside of the spacecraft. They are floating | :47:14. | :47:22. | |
around. The Final Frontier is packed with rubbish, litter. | :47:22. | :47:27. | |
There's everything from an astronauts glove, that one stage in | :47:27. | :47:33. | |
Orbit for a month, to particles of you're in, flushed from early space | :47:33. | :47:39. | |
craft. There are bits of rock left by the Apollo missions. Even 32 | :47:39. | :47:46. | |
nuclear reactors that used to power satellites. This shows you a | :47:46. | :47:50. | |
simulation of what we can see in Orbit. It ranges from debris close | :47:50. | :47:57. | |
to the Earth to places where TV satellites up operating. Fees range | :47:57. | :48:01. | |
in size from some things are size of a mobile phone up to a space | :48:01. | :48:05. | |
station. Her these objects mean we are getting tight for space in | :48:05. | :48:10. | |
space. We've realised over many years that although the universe is | :48:10. | :48:15. | |
potentially infinite, the space around the Earth is very finite. | :48:15. | :48:18. | |
But the problem isn't just that it is crowded up there, it is also | :48:18. | :48:25. | |
dangerous. All these objects are hurtling about at over 25,000 | :48:25. | :48:32. | |
kilometres per hour. It is like a cloud of flying pockets. It has a | :48:32. | :48:37. | |
high energy moving at that speed. A pound coin in Orbit around the | :48:37. | :48:41. | |
earth has the same energy as a minibus travelling at 1,000 | :48:41. | :48:46. | |
kilometres an hour. If that hit a spacecraft, it would destroy it. | :48:46. | :48:52. | |
1983, a chip of paint collided with the Space Shuttle. The impact was | :48:52. | :48:59. | |
enough to crack its 1.5 centimetre thick windscreen. In 2009 a US and | :48:59. | :49:04. | |
Russian satellite hit each other. Both were completely destroyed and | :49:04. | :49:11. | |
created up to 1,500 new bits of junk. It can only get worse. In 60 | :49:11. | :49:15. | |
years we've gone from no man-made objects in Orbit to an estimated 35 | :49:15. | :49:22. | |
million. And the worry is that areas of space we rely on to send | :49:22. | :49:25. | |
satellites for navigation, weather forecasting and TV will soon become | :49:25. | :49:33. | |
no-go areas. Currently there's no working answer, but all sorts of | :49:33. | :49:38. | |
plans are being hatched. From sales that would slow an object down so | :49:38. | :49:44. | |
they fell back to earth to giant balloons that would inflate to help | :49:44. | :49:51. | |
put the brakes on. But the UK's largest space company has come up | :49:51. | :50:00. | |
Astrium in Stevenage is better known for building satellites that | :50:00. | :50:07. | |
get sent to space. But engineer Jamie's job is to use his harpoon | :50:07. | :50:13. | |
to drag them back to work. We've got a harpoon we are going to fire. | :50:13. | :50:18. | |
It goes into the barrel inside a protective chamber. I will put some | :50:18. | :50:23. | |
goggles on. For harpoon uses compressed air rather than | :50:23. | :50:29. | |
explosives to fire. It is safer for space. We are ready to fire now. | :50:30. | :50:39. | |
:50:40. | :50:43. | ||
Turn the firing switched on. Sadly At the moment, Jamie is test firing | :50:43. | :50:48. | |
his harpoon into pieces of actual satellite. It's early days, but | :50:48. | :50:52. | |
when complete the harpoons will have a spring loaded barrel and her | :50:52. | :50:59. | |
capers. If the system works, the harpoon will be mounted on a | :50:59. | :51:05. | |
satellite that will Chasetown space junk, harpoon it and tow it back | :51:05. | :51:10. | |
towards earth where we it will burn up socially in the atmosphere. -- | :51:10. | :51:15. | |
safely. This only works with large objects. In Orbit, pig objects are | :51:15. | :51:21. | |
just thousands of small objects waiting to happen. -- big object. | :51:21. | :51:25. | |
Something has to be done and this could be the big thing -- best | :51:25. | :51:31. | |
thing. But until somebody can enforce an intergalactic litter | :51:31. | :51:35. | |
campaign, the research has to continue. | :51:35. | :51:40. | |
This is a vivid demonstration of the problem. This is lent was by | :51:40. | :51:48. | |
the National Space Centre a, a panel from a satellite. That is a | :51:48. | :51:52. | |
great picture with us shuttle underneath. The office was in Orbit | :51:52. | :52:00. | |
for six years. They saw this Goring. These are impact of micro meteors. | :52:00. | :52:06. | |
Invisible to the human eye. They are travelling between 8 and 9 | :52:07. | :52:09. | |
kilometres per second and up to 30 kilometres per second. A tremendous | :52:09. | :52:18. | |
amount of energy. The plasma Burns. If you lift it up, you can see... | :52:18. | :52:25. | |
This is the spacecraft... That is a whole and that is a whole. You can | :52:25. | :52:33. | |
see the Dent. Minuscule pieces of dust. Back over to mark in Dobbie. | :52:33. | :52:38. | |
Last time we saw him he had unveiled our version of Herschel's | :52:38. | :52:44. | |
telescope. Have they observed anything with it? | :52:44. | :52:47. | |
Unfortunately not. It is amazing standing on this platform like | :52:47. | :52:51. | |
Herschel did all those years ago. Herschel did it in the damp English | :52:51. | :52:55. | |
weather. I'm safer than he is because I have harnessed to make | :52:55. | :53:01. | |
sure I don't fall off. There have been times observers have fallen | :53:01. | :53:04. | |
off those platforms. We can't show you any pictures, but it is | :53:04. | :53:08. | |
incredible to think that Herschel spent many years observing the | :53:08. | :53:13. | |
British night sky with the weather to contend with. We did get some | :53:13. | :53:18. | |
clear skies a few nights ago. We managed to record some images of | :53:18. | :53:19. | |
managed to record some images of things in the sky. The first | :53:19. | :53:23. | |
things in the sky. The first picture we got was Jupiter. Moving | :53:23. | :53:28. | |
very gracefully across the screen, caused by the rotation of the Earth. | :53:28. | :53:30. | |
The telescope doesn't have the The telescope doesn't have the | :53:30. | :53:35. | |
drive system so you can't see the object being tracked. A picture of | :53:35. | :53:45. | |
a beautiful Binary Star system in Cygnus. We have the picture of a | :53:45. | :53:52. | |
star cluster inside the Orion nebula. We have a final image of | :53:52. | :53:56. | |
Uranus which Herschel discovered with a slightly smaller telescope. | :53:56. | :54:00. | |
There's a very slight distortion which is caused by the orientation | :54:01. | :54:05. | |
of the optics in a telescope. He will have had to have contended | :54:05. | :54:09. | |
with these poor images. We can't show you anything live tonight, but | :54:09. | :54:13. | |
it is great to follow in Herschel's footsteps. Without greater | :54:13. | :54:16. | |
astronomers like him, we would not have learned as much about the | :54:17. | :54:21. | |
universe as we can see now. It is great that we can leave his | :54:21. | :54:24. | |
telescope to the residents of Derby so hopefully in the years to come | :54:24. | :54:28. | |
they can enjoy the night sky like Herschel did all those years ago. | :54:28. | :54:33. | |
Back to the studio. They are beautiful images and that | :54:33. | :54:37. | |
talent the scope will be in Derby for the next three years. -- | :54:37. | :54:42. | |
telescope. This week you have been doing your own pioneering | :54:42. | :54:47. | |
scientific work thanks to our online experiment. We asked you to | :54:47. | :54:51. | |
study Mars's surface looking for unusual features. I spend a lot of | :54:51. | :54:58. | |
time looking at this guy thinking it is amazing. In this case, the | :54:58. | :55:01. | |
hyperbolic and third -- adjectives are appropriate. This is wonderful | :55:01. | :55:08. | |
and amazing. Real science in two days. More than 100,000 people have | :55:08. | :55:12. | |
helped us explore an area about the size of Holland. It was | :55:13. | :55:18. | |
Switzerland! We are working our way up. We found some great stuff. We | :55:18. | :55:21. | |
were looking at the Antarctic region of Mars and these strange | :55:21. | :55:25. | |
France which we think on from material suddenly erupting | :55:25. | :55:27. | |
material suddenly erupting underneath the surface of Mars. We | :55:27. | :55:31. | |
had this idea that it has to do with ice under the surface that was | :55:31. | :55:38. | |
being heated up. It is the time lapse. Yes. It was a year on Mars | :55:38. | :55:44. | |
has put together by users. At some point in the year, in the Martian | :55:44. | :55:48. | |
spring, these things erupt as the planet heats up? That is what we | :55:48. | :55:53. | |
now know. I can tell you for sure because we only find these around | :55:53. | :55:59. | |
March in the Marshin calendar. They happen close to the equator and | :55:59. | :56:02. | |
then they head closer to the polls and we thought they were rare, but | :56:03. | :56:06. | |
look at this. This whole region of ground would have erupted | :56:06. | :56:14. | |
underneath your feet. Don't go there in the spring! What about | :56:14. | :56:18. | |
this are titters -- artistic impression. We discovered that. Our | :56:18. | :56:22. | |
viewers discovered that is what is happening. We know when and where | :56:22. | :56:25. | |
it happens and we now know it is much more common than we thought. | :56:25. | :56:32. | |
That is because people used pattern recognition skills. More than that. | :56:32. | :56:35. | |
A good scientific experiment always leaves you with more questions. | :56:35. | :56:39. | |
We've no idea what this is. This is a type of terrain I'd never seen | :56:39. | :56:45. | |
before. It has angular features. These moved from year to year. No | :56:45. | :56:49. | |
idea what this is. It is something to do with ice escaping from | :56:50. | :56:53. | |
underneath and going into the Martian atmosphere. People will be | :56:53. | :56:57. | |
working on this the years. Wonderful. We have more time in the | :56:57. | :57:06. | |
show afterwards. I pledged applied to somebody. -- a pint. Tell us | :57:06. | :57:11. | |
what to think that is. The best week, I will buy you another pint. | :57:11. | :57:16. | |
I'm very excited. What is that? other guy is still waiting for his | :57:16. | :57:21. | |
plight. Before we go, just time to say goodbye to Liz and NASA. How | :57:21. | :57:30. | |
has it been? 30 seconds. Thanks. It's been such a privilege to meet | :57:30. | :57:34. | |
all of the people behind so many or inspiring endeavours. What struck | :57:34. | :57:37. | |
inspiring endeavours. What struck me most is how every single mission | :57:37. | :57:41. | |
seems impossible on paper. I'm not sure what impresses any more, for | :57:41. | :57:46. | |
fact they are able to dream up crazy schemes like lowering a road | :57:46. | :57:51. | |
on to Mars using as Guy Cramer and sampling, it as they hurtle through | :57:51. | :57:54. | |
space or the fact they are able to make those ideas a reality. They | :57:54. | :58:00. | |
are always thinking ahead. By the mid- 2020s, there's talk of putting | :58:00. | :58:04. | |
a man on an asteroid, and a few decades after that a man on another | :58:04. | :58:08. | |
planet. It is an exciting time. Sadly, it is time for us to say | :58:08. | :58:15. | |
goodbye to everybody at NASA and you at home. At night from NASA. | :58:15. | :58:22. | |
Thank you for wearing your telescope hat especially! Don't | :58:22. | :58:25. | |
forget there are hundreds of stargazing events happening up and | :58:25. | :58:29. | |
down the country. Details are on the website, bbc.co.uk/stargazing. | :58:29. | :58:36. | |
Don't forget about our Star Guide. We're going to be back in a second, | :58:37. | :58:42. | |
but do you want to wrap up? discoveries on Mars are real | :58:42. | :58:45. | |
scientific discoveries. Chris was telling me there's going to be a | :58:45. | :58:50. | |
paper written. There's a scientific paper written and everybody | :58:50. | :58:53. |