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What a week we have had a Jodrell Bank. When we went hunting, we never | :00:10. | :00:15. | |
thought we would see this. The glorious colours of the Northern | :00:16. | :00:22. | |
lights. Or the extraordinary event of the sun bursting particles the | :00:23. | :00:28. | |
waters. All along you have been searching the galaxies and you have | :00:29. | :00:31. | |
made a remarkable discoveries, and you've had a glimpse of event that | :00:32. | :00:37. | |
happened 11 million years ago. I am Brian Cox, he is Dara O'Briain, and | :00:38. | :00:39. | |
this is Stargazing Live. Welcome back to Stargazing Live. | :00:40. | :01:10. | |
Let's get straight onto the most exciting news of the series - an | :01:11. | :01:14. | |
amazing discovery made by you over the last three nights. We asked you | :01:15. | :01:17. | |
to search for hidden galaxies. And not only have you been successful | :01:18. | :01:21. | |
but what you've discovered is of genuine scientific importance. So | :01:22. | :01:24. | |
much so that some of the biggest telescopes around the world, | :01:25. | :01:27. | |
including this one, have dropped everything to focus on what you've | :01:28. | :01:34. | |
found. This is why it is pointing in this direction, it is tracking one | :01:35. | :01:40. | |
of the things you found because it is so interesting. Here to tell us | :01:41. | :01:46. | |
more is Chris Lintott. What did our viewers need to do? We asked people | :01:47. | :01:53. | |
to look for gravitational lenses, the light where it has been bent by | :01:54. | :01:58. | |
more nearby galaxies, and that bending of light means we see | :01:59. | :02:01. | |
further into the past and we see distant galaxies we would not be | :02:02. | :02:07. | |
able to see. You said you were hoping to get 500,000 hits by | :02:08. | :02:13. | |
Thursday. We broke that easily, so now we are at 6.5 million | :02:14. | :02:22. | |
classification is made by 50,000 Stargazing Live viewers. Such a big | :02:23. | :02:29. | |
response that the professional community have got involved. It's | :02:30. | :02:32. | |
not only the Lovell we have taken over. It's not just the quantity or | :02:33. | :02:38. | |
the classifications, it's they found wonderful things. We have more 50 | :02:39. | :02:43. | |
candidate gravitational lenses, and we've used some of the biggest | :02:44. | :02:48. | |
telescopes in the world. A genuinely global initiative. Let's go over to | :02:49. | :02:53. | |
the UK, because how many telescopes there? We have used the Lovell | :02:54. | :03:00. | |
telescope, and even as far away as Cambridge to track one of the | :03:01. | :03:07. | |
candidates. Six radio telescopes working in congruence. One of the | :03:08. | :03:10. | |
more interesting targets is is there. Over the course of the | :03:11. | :03:18. | |
evening, excitement gathered, and other people in America join this. | :03:19. | :03:24. | |
We got data in America, archive data, from West Virginia, the | :03:25. | :03:30. | |
greenback telescope. We called our friends in Hawaii because we wanted | :03:31. | :03:34. | |
to get optical and infrared data must be called the biggest telescope | :03:35. | :03:41. | |
in the world. It is Hawaii but you are 13,000 feet in the mind him. The | :03:42. | :03:45. | |
dome was frozen shut. They hacked away at the icicles chorus. The | :03:46. | :03:49. | |
director of the Institute have away so we could get the data -- for us. | :03:50. | :03:56. | |
We don't recommend you do this at home, but we were late in the bar | :03:57. | :04:00. | |
last night, and we rang up the Greenback telescope. I also saw you | :04:01. | :04:10. | |
ringing Chile. We called the Canary Islands, but it was snowing, but we | :04:11. | :04:14. | |
still call them. They have been trained on one target in particular, | :04:15. | :04:19. | |
and we will talk about that later. It's all because of the effort of | :04:20. | :04:26. | |
Stargazing Live view is that we've done it. We are contributing to the | :04:27. | :04:30. | |
sum total of human knowledge rather than the usual television thing. | :04:31. | :04:40. | |
This is real star. Real science. We have also been getting astounding | :04:41. | :04:43. | |
images sent over in the last couple of days. Look at this one. The moon, | :04:44. | :04:50. | |
but a beautiful photograph by Julian Cooper from the Black Country. Also | :04:51. | :04:57. | |
beautiful photos of this sunspot group. Again, this is the thing that | :04:58. | :05:02. | |
gives us the possibility of Aurora Borealis tonight. We gave a | :05:03. | :05:08. | |
prediction of the time that the burst of energy might arrive. That | :05:09. | :05:12. | |
might not have been exactly right and we might still be waiting. It is | :05:13. | :05:17. | |
ongoing. We have space observatories up there and we think it might | :05:18. | :05:22. | |
arrive now. I want to show you a couple more. This is a bit of a | :05:23. | :05:28. | |
cheat. We talk about amateur imagery is -- images, but this is a | :05:29. | :05:32. | |
beautiful picture from Reykjavik, in Iceland. Just a few moments ago in | :05:33. | :05:39. | |
Norway, Liz Bonnin took to the skies to see if any of the recent activity | :05:40. | :05:43. | |
on the sun is producing any Aurora yet. How is it looking, Liz? Welcome | :05:44. | :05:54. | |
back to a world first, Aurora hunting. We are crammed into a | :05:55. | :05:58. | |
plane, and the equipment is working nicely. Pete Lawrence is with us on | :05:59. | :06:01. | |
the flight, so let's take a look outside the window. In the last ten | :06:02. | :06:07. | |
minutes, this beautiful site revealed itself. A lot of structure | :06:08. | :06:11. | |
and beautiful curls at the bottom of it. Very bright tonight, isn't it? | :06:12. | :06:17. | |
Very nice. Lots of structure. It's been changing as we have watched out | :06:18. | :06:22. | |
of the window, lots of vertical rays. Am I wishful thinking, or can | :06:23. | :06:29. | |
I see some red and brown? I can see some red at the right. That is a | :06:30. | :06:35. | |
first, and we're excited about it. Let's talk about the forecasting we | :06:36. | :06:40. | |
had last night. Has the corona hit the earth? What has changed between | :06:41. | :06:46. | |
last night and now? It hasn't hit us. It's hard to forecast the | :06:47. | :06:50. | |
arrival, and it got slow down as it headed from the sun towards us. It | :06:51. | :06:55. | |
could arrive anywhere between now and 4am. It could still affect this | :06:56. | :07:01. | |
beautiful light display we see tonight? Absolutely. That is the | :07:02. | :07:07. | |
beauty of space weather. The aurora changing all tonight. I will leave | :07:08. | :07:10. | |
you with that beautiful image, a sight for sore eyes. See you in a | :07:11. | :07:17. | |
bit. Seeing different colours within the Aurora, as we have. You can see | :07:18. | :07:23. | |
the red on the right, but if that is the immediate, who knows what will | :07:24. | :07:26. | |
happen? There have been special Stargazing Live parties taking place | :07:27. | :07:32. | |
up and down the country, and there is one in Egham, in Sussex. A | :07:33. | :07:41. | |
wonderful evening at Royal Holloway University. Thousands of excuse you | :07:42. | :07:46. | |
asked it -- enthusiastic stargazers, are you having a good time? What has | :07:47. | :07:53. | |
that been the best thing so far? I think it was the DIY. What do you | :07:54. | :08:00. | |
look forward to seeing next? Tourists in space. That is the thing | :08:01. | :08:06. | |
about this, they're so many things going on. There is the option also | :08:07. | :08:10. | |
to see yourself in infrared, and there is an army of astronomers and | :08:11. | :08:14. | |
telescopes to look at the sky. We've even set up a field of astronomers | :08:15. | :08:19. | |
away from the light so we can take some wonderful views of what the | :08:20. | :08:23. | |
clear sky has to offer. And I will also show you how you can find | :08:24. | :08:29. | |
galaxies through your own telescope and how to navigate through the | :08:30. | :08:34. | |
stars. Back to the studio. Lots of young faces in the studio. Those | :08:35. | :08:40. | |
youngsters seem to be the new co-hosts, and I know how you feel | :08:41. | :08:43. | |
about this out region getting involved. Getting kids excited about | :08:44. | :08:50. | |
astronomy leads to so many other things, entrepreneurialism, careers | :08:51. | :08:53. | |
in science. I remember when I was about three years old watching the | :08:54. | :08:59. | |
Clangers. And we are yet to find them! The great thing about them was | :09:00. | :09:07. | |
the row of kids about seven or eight years old, and that is what | :09:08. | :09:10. | |
astronomy did for me, and I went into physics and I caught the bug. | :09:11. | :09:14. | |
Your career has been mainly based on space hardware, mainly the James | :09:15. | :09:21. | |
Webb telescope, a tremendous telescope. It is amazing. It will | :09:22. | :09:28. | |
travel 1.5 kilometres away from Earth and then deploy, which looks | :09:29. | :09:32. | |
challenging, but what comes out is a heat shield visit and infrared | :09:33. | :09:37. | |
telescope and the biggest source of heat nearby the son, so it hides | :09:38. | :09:42. | |
behind the earth and it protects it from some of the sun and it has | :09:43. | :09:47. | |
Earth radiation. This is the heat shield, then? It's about the size of | :09:48. | :09:53. | |
a telescope. It's going to be launched in about 2018, hopefully. | :09:54. | :09:59. | |
We see the golden mirror, so what is the difference between that and the | :10:00. | :10:03. | |
Hubble telescope? The Hubble telescope was mainly optical, but | :10:04. | :10:10. | |
the James Webb is infrared, so it gets orange and red and the rest is | :10:11. | :10:15. | |
infrared. But why? We have pictures of the Milky Way, so what is it that | :10:16. | :10:23. | |
the James Webb gives us? It was called a next-generation space | :10:24. | :10:29. | |
telescope. Mind you, it is coming from a long way. We can see the | :10:30. | :10:35. | |
Milky Way galaxy, but here you can see the patches of dust, and of | :10:36. | :10:38. | |
course a visible light, optical light, which doesn't past -- passed | :10:39. | :10:44. | |
through it. But with the infrared you can see what is behind. An | :10:45. | :10:49. | |
interesting look at the centre of the galaxy, the black hole obscured | :10:50. | :10:56. | |
by the dust. What I find fascinating is that when people think of | :10:57. | :10:58. | |
telescopes they think of visible light, but we have an amazing piece | :10:59. | :11:03. | |
of equipment, a radio telescope, and the James Webb is infrared. We take | :11:04. | :11:08. | |
parts of the Informatics spectrum and get a broader picture of what is | :11:09. | :11:13. | |
out there. This will be coming back to earth and we will see later. | :11:14. | :11:19. | |
There is a huge question about the Milky Way that spin around for | :11:20. | :11:24. | |
hundreds of years, but Simon Taylor of Runcorn has sent things in over | :11:25. | :11:27. | |
the last two years, and asked, if we've never been outside the Milky | :11:28. | :11:31. | |
Way, how do we know what it has been looking like? Let's find out. On a | :11:32. | :11:39. | |
clear, moonlit night you can see a milky glow across the night. The | :11:40. | :11:45. | |
Romans called it a milky road, and when Galileo pointed his telescope | :11:46. | :11:49. | |
at it, he discovered that this haze of light was in fact made up of | :11:50. | :11:57. | |
distant stars. When we look out into the night sky, we see the stars and | :11:58. | :12:03. | |
the glowing gas and dust which are bound together by gravity and make | :12:04. | :12:07. | |
the galaxy, which we call the Milky Way. But because we are in it, it's | :12:08. | :12:12. | |
very hard to work out what the shape of the galaxy actually is. One of | :12:13. | :12:21. | |
the first attempts to map the galaxy was from astronomer William Herschel | :12:22. | :12:28. | |
in 1785. What needed was to assume that all of the stars we can see the | :12:29. | :12:34. | |
sky are roughly of the same brightness and it uniformly | :12:35. | :12:37. | |
distributed. By doing that, he came up with a map, which is the shape of | :12:38. | :12:46. | |
the known universe of the time. Now, this is not accurate, the many | :12:47. | :12:51. | |
reasons. But one of them is that there are many stars in the Milky | :12:52. | :12:54. | |
Way galaxy that cannot be seen from Earth because they are obscured by | :12:55. | :13:04. | |
dust. No one appreciated the children -- true extent of the Milky | :13:05. | :13:07. | |
Way until tools were developed to help them peer through the dust. In | :13:08. | :13:20. | |
1955, the Stargazing Live -- Lovell telescope was built at Jodrell bank, | :13:21. | :13:23. | |
and it did not look at Starlight, but was designed to capture radio | :13:24. | :13:32. | |
waves. While visible light is easily blocked by dust, radio waves | :13:33. | :13:35. | |
emanating from the furthest reaches of our galaxy can pass through. | :13:36. | :13:44. | |
Clive Dickinson is an astronomer who choose into these electromagnetic | :13:45. | :13:47. | |
waves from our Milky Way. -- choosing. -- tunes in. Obviously | :13:48. | :14:00. | |
there are lots of stars in the galaxy, but when you look with the | :14:01. | :14:04. | |
radio waves you get a different picture. You can still see the | :14:05. | :14:07. | |
galactic plane, but you can also see completely different things, and | :14:08. | :14:10. | |
different objects and different structures. What is revealed is that | :14:11. | :14:17. | |
the space between the stars is far from empty. It is filled with gas, | :14:18. | :14:23. | |
mostly hydrogen. And because radio telescopes can detect waves emitted | :14:24. | :14:28. | |
by the hydrogen gas, they can be deduced to work out the shape of the | :14:29. | :14:34. | |
Milky Way. This is a map of the hydrogen gas in our galaxy that was | :14:35. | :14:39. | |
first made in the 1950s, and the hydrogen follows the distribution of | :14:40. | :14:42. | |
stars in the galaxy. By measuring the velocity of that gas, and the | :14:43. | :14:50. | |
brightness in any direction, you can deduce that the Milky Way is, in | :14:51. | :15:04. | |
fact, a giant spiral of stars. But astronomers are now mapping more | :15:05. | :15:09. | |
than hydrogen. These brands in new views of our galaxy show other | :15:10. | :15:12. | |
components in our Milky Way, including the dust that obscure | :15:13. | :15:20. | |
would their view 200 years ago. By combining these results, we are | :15:21. | :15:24. | |
finally beginning to build a picture of what the Milky Way looks like. A | :15:25. | :15:29. | |
disc of hundreds of billions of stars, gas and dust, swirling around | :15:30. | :15:36. | |
a central bar into the most beautiful spiral galaxy. | :15:37. | :15:44. | |
We know enough now to take an educated guess at what the Milky Way | :15:45. | :15:52. | |
looks like. About 27 light-years from the centre. But the most | :15:53. | :15:56. | |
distinctive features of the spiral arms. They are the focus about one | :15:57. | :16:02. | |
of the big debates about the Milky Way. How many arms are there and | :16:03. | :16:09. | |
what pattern do they form? That is one thing the team here at Jodrell | :16:10. | :16:14. | |
Bank have been studying. Professor Tim O'Brien is here. You have one of | :16:15. | :16:21. | |
your telescopes scanning? The severed meter telescope has been | :16:22. | :16:25. | |
scanning through the Milky Way and I have a live signal from it now. What | :16:26. | :16:30. | |
you are seeing in this spectrum which is updated in real-time, the | :16:31. | :16:34. | |
peaks in the middle are from hydrogen atoms in the spiral arms of | :16:35. | :16:40. | |
the Milky Way. There is a peak along the side which is a second arm. It | :16:41. | :16:46. | |
indicates a cloud of hydrogen gas as we look through the disc of the | :16:47. | :16:50. | |
Milky Way. Each produces a peak in this spectrum. We just talked about | :16:51. | :16:56. | |
the infrared, this is the 21 centimetre? Yes, it is the same | :16:57. | :17:02. | |
thing Maggie mentioned, there is dust and it makes it difficult to | :17:03. | :17:09. | |
see through it. What is this image? It is a scan we did earlier. You see | :17:10. | :17:16. | |
these patterns, each of these spikes is a spiral arm. I can see three | :17:17. | :17:25. | |
arms for example. It seems to reveal it into arms and three arms? It is | :17:26. | :17:30. | |
difficult to see the structure of the Milky Way from inside. We were | :17:31. | :17:36. | |
aware of four of them, and then there was a paper that said there | :17:37. | :17:42. | |
were just two, now they reckon there are four of them again. This | :17:43. | :17:48. | |
telescope, we have taken over. It is not looking it's beautiful self. But | :17:49. | :17:51. | |
it is pointing at an interesting object? But beside the moon, there | :17:52. | :17:58. | |
was an object discovered by our view was the other day that is billions | :17:59. | :18:03. | |
of light years away. We will be showing you that later. It is not | :18:04. | :18:06. | |
the only galaxy you can see from Earth. Mark Thompson can show you | :18:07. | :18:12. | |
how to see our closest galactic neighbours. | :18:13. | :18:20. | |
We have wonderful clear skies. The party and come local astronomers. I | :18:21. | :18:35. | |
want to show you this wonderful moon. We are here to spot as many | :18:36. | :18:43. | |
galaxies as we can. We shot this video in Norfolk a few days ago that | :18:44. | :18:51. | |
the Andrew Meda galaxy. Jamie, what can you say? I can see a bit of a | :18:52. | :19:02. | |
blur. If you look to one side, you can use a technique called averted | :19:03. | :19:10. | |
vision. Have another look. Is that better? Can you see the spiral | :19:11. | :19:16. | |
nature of the galaxy? Yes. It is wonderful, you are looking back in | :19:17. | :19:25. | |
time, 2.5 million years. It is a weird concept. You can see it with | :19:26. | :19:32. | |
binoculars and you can see it in the south-west at this time of year. I | :19:33. | :19:37. | |
will leave you to enjoy that. There are a couple of other galaxies you | :19:38. | :19:42. | |
can see tonight. We had some footage we took about half an hour ago | :19:43. | :19:52. | |
called M81 if we look through the Hubble telescope, it looks | :19:53. | :19:57. | |
spectacular. It is visible just above the plough at this time of | :19:58. | :20:01. | |
night. If you want to bind the details you have two June into my | :20:02. | :20:09. | |
Starcast. This is a view of M82 sometimes you can see the two | :20:10. | :20:16. | |
galaxies through one telescope will stop with the big Hubble telescope, | :20:17. | :20:22. | |
we get some wonderful views, sharing the turbulent nature in that galaxy | :20:23. | :20:25. | |
where loads of new, young stars are starting to form. That is all we can | :20:26. | :20:30. | |
see for tonight. If it is clear where you are, get outside and see | :20:31. | :20:36. | |
how many galaxies you can spot. You can find information on our website. | :20:37. | :20:46. | |
Now back to Brian and Dara O'Brian. We are about to explore a galaxy in | :20:47. | :20:53. | |
more details. There is a new mission underway set to revolutionise our | :20:54. | :20:58. | |
knowledge of the Milky Way. The chief K scientist behind this is | :20:59. | :21:06. | |
Professor Gerry Gilmore. We spoke to Caroline about the nerve wracking | :21:07. | :21:14. | |
nature of space exploration. What did you feel? I was there. It is an | :21:15. | :21:25. | |
interesting experience. There was perceptible relief when it opened up | :21:26. | :21:30. | |
and it was working. It is not just the money it is the 20 years of work | :21:31. | :21:36. | |
from the 400 engineers. Tell us about the mission? GAIA is designed | :21:37. | :21:44. | |
to answer the questions you were asking. It is a shield half the size | :21:45. | :21:49. | |
of a tennis court, but it is a big camera and to telescope will stop it | :21:50. | :21:54. | |
is taking a video of the sky for five years and will measure the | :21:55. | :22:01. | |
distance of a billion objects. This is exquisite UK technology. They are | :22:02. | :22:10. | |
cameras? Every one of these things is a bigger version of what you have | :22:11. | :22:16. | |
in your telephone. This is only half of it. You have two touch them | :22:17. | :22:26. | |
carefully. In terms of an eight megapixel camera, what is that? It | :22:27. | :22:34. | |
is a Ilion pixel camera. It is very sensitive, thousands of times more | :22:35. | :22:41. | |
sensitive in terms of dynamic range and quality of anything that has | :22:42. | :22:44. | |
ever been made before. We need that to get that exquisite position GAIA | :22:45. | :22:53. | |
is designed to get. If you put a human hair in space, this thing can | :22:54. | :22:59. | |
see either side of it? From London. GAIA will locate the stars. It is | :23:00. | :23:09. | |
the equivalent of locating a small coin on the moon. Also how they are | :23:10. | :23:19. | |
moving? Yes, we keep doing this for five years and see how it moves. It | :23:20. | :23:25. | |
allows us to measure the distance of the object. We can see where all of | :23:26. | :23:30. | |
these objects are in 3-dimensional. Also how everything is moving. When | :23:31. | :23:36. | |
we walk through space and we can see what is there, and where it really | :23:37. | :23:42. | |
is, but how those things are moving and from that we can deduce the | :23:43. | :23:46. | |
entire formation of the Milky Way and that is what GAIA is. What | :23:47. | :23:52. | |
affect will this have on the industry? GAIA will rewrite the | :23:53. | :24:02. | |
textbooks. People have studied with these giant telescope because they | :24:03. | :24:07. | |
knew it was interesting. We haven't done that for a billion objects | :24:08. | :24:15. | |
before. So GAIA will do it for a billion objects and tell us what | :24:16. | :24:21. | |
looks normal. How did the Milky Way get to be the way it is? We have a | :24:22. | :24:28. | |
video from last year and one of the theories. We know the Andromeda | :24:29. | :24:32. | |
galaxy, one with about a trillion stars is coming towards us quite | :24:33. | :24:39. | |
quickly and is going to hit us. The debate is that it has hit us before? | :24:40. | :24:48. | |
That is one of the questions GAIA is designed to answer. We can | :24:49. | :24:54. | |
understand one, then we have a Rosetta Stone for all of them. To | :24:55. | :24:58. | |
answer that question we need to know not only were the galaxies are now, | :24:59. | :25:05. | |
so GAIA will tell us that, we also need to know how much they weigh. | :25:06. | :25:11. | |
That is the unique thing with GAIA. We can introduce weight, so we know | :25:12. | :25:16. | |
for the first time, not only what we can see, but everything that is | :25:17. | :25:20. | |
there. It is an incredible project. We will be talking to you later. In | :25:21. | :25:27. | |
a moment we will be revealing a new galaxy you have discovered, but last | :25:28. | :25:30. | |
night Brian looked at how we might fuel a starship puckered | :25:31. | :25:37. | |
transporters to the stars as close to the speed of light. What about | :25:38. | :25:40. | |
the astronauts on board? I were to find out what it would feel like. | :25:41. | :25:48. | |
To travel anywhere fast, first you have to accelerate. Apparently this | :25:49. | :25:57. | |
car can go from zero to 60 mph in just six seconds. Acceleration | :25:58. | :26:13. | |
creates the force that pins at you back in your chair whenever you | :26:14. | :26:25. | |
change speed. And in small doses... It is a lot of fun. However, to get | :26:26. | :26:32. | |
to the kind of speeds you need for intergalactic travel, you can have | :26:33. | :26:38. | |
too much of a good thing. So, would my body stand any chance of handling | :26:39. | :26:43. | |
the kind of acceleration needed to reach near lightspeed? To find out, | :26:44. | :26:55. | |
I have come to brook city based in San Antonio in Texas. Hidden inside | :26:56. | :27:00. | |
building 170 is a machine of torture. In it, over 100 astronauts | :27:01. | :27:09. | |
have learned to endure the extreme acceleration of a space shuttle | :27:10. | :27:16. | |
launch. It is a human centrifuge. And today, it is my turn to take a | :27:17. | :27:23. | |
ride. How are you? This man is lead centrifuge technician. Basically I | :27:24. | :27:31. | |
am in a space shuttle launch? Yes, we will go through the same protocol | :27:32. | :27:36. | |
the astronauts go through. The centrifuges is going to spin me ever | :27:37. | :27:40. | |
faster, subjecting me to the crushing force. What can the body | :27:41. | :27:59. | |
take? The G will be pushing on your chest. I won't feel more sure is, I | :28:00. | :28:05. | |
won't feel ill? I hope you don't. Will I feel all of my limbs heavier? | :28:06. | :28:15. | |
Your ear lobes, your eyelids, everything will feel three times | :28:16. | :28:19. | |
heavier. It is heavy enough as it is! Wow! This is amazing. At maximum | :28:20. | :28:34. | |
acceleration, reducing 3G, my body will feel three times heavier than | :28:35. | :28:40. | |
normal. It takes shuttle astronauts seven seconds to reach the speed. | :28:41. | :28:45. | |
Obviously they are trained professionals. Three, two, 1... | :28:46. | :28:56. | |
Liftoff. You are at 2.5 G. This is about as | :28:57. | :29:15. | |
much as the shuttle or anyone on board can take for more than a few | :29:16. | :29:23. | |
seconds. I am beginning to see why. It may not look it, but my arm feels | :29:24. | :29:30. | |
as heavy as a bag of cement. Wave to the camera. That is getting | :29:31. | :29:38. | |
uncomfortable and it would take months to get to lightspeed at this | :29:39. | :29:41. | |
rate. That is not good enough, we need more G. Would you like us to | :29:42. | :29:53. | |
take you 25 G for ten or 15 seconds just to see what it feels like? Go | :29:54. | :30:13. | |
on then. 2.5, three. 4.5 and we are at five, how does it feel? Tough | :30:14. | :30:23. | |
will stop back down now. That is tough. It is amazing. No way you | :30:24. | :30:32. | |
could do anything at five G. Can't even talk. It would not be very | :30:33. | :30:40. | |
flattering. He has been laughing at this all day. It is unflattering. | :30:41. | :30:45. | |
This famously good-looking man in a centrifuges, this is what he looked | :30:46. | :30:53. | |
at stop that was at seven. You look like an old woman out of correlation | :30:54. | :31:01. | |
Street. Now back to Liz. What is in the sky above you? You | :31:02. | :31:05. | |
have no idea what you have been witnessing. | :31:06. | :31:12. | |
We were giddy, applauding and at one point we were circled by this stuff. | :31:13. | :31:17. | |
The sky is filled with Green. There was a pink border at the bottom. It | :31:18. | :31:22. | |
is changing every second. What have we been looking at? I have lost | :31:23. | :31:27. | |
track of the amount of movements, the red and the pink. It is | :31:28. | :31:33. | |
glorious. It gets confusing doesn't it? You can see how the bands fold | :31:34. | :31:38. | |
upon themselves. They wrap around and you get various struck just. It | :31:39. | :31:46. | |
looked like a cascade of light. We have some footage from a few moments | :31:47. | :31:52. | |
ago. It was a multilayered, multi-structural, if that is the | :31:53. | :32:07. | |
right terminology. I am overwhelmed, it is mind blowing, I never expected | :32:08. | :32:12. | |
to see such beautiful displays. The fantastic thing was it that was | :32:13. | :32:17. | |
moving dynamically. The ripples of light moving through the whole | :32:18. | :32:22. | |
display. People describe the Aurora is a dance across the sky, and we | :32:23. | :32:27. | |
have witnessed it, it is glorious. With regard to the different shapes, | :32:28. | :32:31. | |
are they ever in a certain order or does it happen haphazardly? Those | :32:32. | :32:39. | |
bright bands are characteristic, and what happens is they fold up on | :32:40. | :32:42. | |
themselves and it gives the impression of a curtain hanging in | :32:43. | :32:46. | |
the sky. They can also wrap up into a huge spiral structure and they | :32:47. | :32:51. | |
look amazing. They are enormous, and go up to about 1600 kilometres. We | :32:52. | :32:58. | |
can see it now, it is a little more diffused, but they are vertical, | :32:59. | :33:03. | |
streaking through the colour. What is that? They are bits of the | :33:04. | :33:09. | |
curtain which folds up on themselves. When you look from the | :33:10. | :33:13. | |
side, you look through multiple layers of light, so they look | :33:14. | :33:17. | |
brighter than the rest of the Aurora, and those are called Reyes. | :33:18. | :33:22. | |
I have heard about the crowns as well. What are they? You see the | :33:23. | :33:28. | |
rays going up vertically, but if you're underneath, and you look up, | :33:29. | :33:32. | |
you can see those rays going up several hundred kilometres into the | :33:33. | :33:36. | |
night sky, and via perspective they converge together, that is the | :33:37. | :33:41. | |
Aurora Crown. On the right-hand corner of the screen we can see a | :33:42. | :33:47. | |
new bright bit of green that defuses upwards. It is very much in real | :33:48. | :33:52. | |
time, this is the beauty of the cameras, we can see it as it happens | :33:53. | :33:57. | |
without a need for time-lapse. Guys, we are besides ourselves. As you can | :33:58. | :34:01. | |
imagine from my boys. Please come back to us soon because we will try | :34:02. | :34:07. | |
to get more footage -- as you can imagine from my voice. You can tell | :34:08. | :34:14. | |
that you was quite overwhelmed. It is beautiful. That demonstrates the | :34:15. | :34:20. | |
power of the stars. We think of it giving light and heat, but it is a | :34:21. | :34:24. | |
magnetic field that is influencing particles from the stars and | :34:25. | :34:28. | |
reaching out across 90 billion miles and causing the atmosphere to light | :34:29. | :34:34. | |
up. It is beautiful. You say all that, and I am thinking Mavis Riley, | :34:35. | :34:38. | |
the old woman from Coronation Street. You look like Mavis Riley, I | :34:39. | :34:47. | |
am like Eric pickles. -- Pickles. We have been building up this discovery | :34:48. | :34:53. | |
all night, but it's quite a big one. Let's look at the images that the | :34:54. | :34:57. | |
viewers were the first to find. Six people on the first night saw a | :34:58. | :35:02. | |
close-up of the image, so let's zoom in on the galaxy. This is the | :35:03. | :35:05. | |
infrared image we showed people, and you can see that lens. There were | :35:06. | :35:18. | |
six people on the very first night is spotted this. You are looking at | :35:19. | :35:24. | |
the nearby galaxy, a couple of billion light years away, so nearby | :35:25. | :35:30. | |
in astronomy terms. This red ring, I think it is a ring, that is a | :35:31. | :35:33. | |
distant galaxy and we are seeing that as it was about 11 billion | :35:34. | :35:41. | |
years ago. To be clear, the light from the galaxy, 11 billion light | :35:42. | :35:46. | |
years away. Well, further than that, so it's actually about 40 billion | :35:47. | :35:53. | |
will -- years away. The starters, we are looking back at when the | :35:54. | :35:58. | |
universe was getting going -- for starters. This galaxy is quite big. | :35:59. | :36:02. | |
It's very active, and we know it is forming stars at a rate of about 100 | :36:03. | :36:07. | |
times that of the Milky Way, so about a hundred huge stars every | :36:08. | :36:13. | |
year. The really exciting thing is what happens when we switch to the | :36:14. | :36:17. | |
radio. We will show you the radio image, and the scientists we work | :36:18. | :36:22. | |
with haven't seen it yet and we wanted to share this with all of the | :36:23. | :36:27. | |
collaborators. So this is from a little telescope, five other | :36:28. | :36:31. | |
telescopes. If you are a professional astronomer, this is | :36:32. | :36:36. | |
exciting. This blog here is the result of yesterday evening's | :36:37. | :36:42. | |
observations. -- this blob. It shows is a nice narrow arc, so perfectly | :36:43. | :36:49. | |
convincing as a lens, but there is more radio emission here than we | :36:50. | :36:54. | |
expected. Brighter than we expected. An unusual object, in that sense? We | :36:55. | :37:01. | |
get the Radio 2 ways, from the young stars. We can predict that, but we | :37:02. | :37:06. | |
might also get it from the gas spiralling in and growing a black | :37:07. | :37:09. | |
hole at the centre of the galaxy. We are watching the early stages of the | :37:10. | :37:14. | |
galaxy. It might be young galaxies merging together. This kind of black | :37:15. | :37:21. | |
hole normally means a collision, so these could be proto- galaxies. | :37:22. | :37:27. | |
Billions of years ago as well, so close to the beginning of the | :37:28. | :37:32. | |
universe. We still have to name it, and we want you to do that as well, | :37:33. | :37:38. | |
so please send suggestions. The only thing is that it needs to have the | :37:39. | :37:43. | |
number nine at the stars. We will give you a decision on that and we | :37:44. | :37:46. | |
will have it by the end of the show. And that will be its name. There | :37:47. | :37:51. | |
will be scientific papers with the name on it, and that's wonderful. To | :37:52. | :37:56. | |
find out what the conditions are like for stargazing outside, here is | :37:57. | :38:03. | |
Helen Willetts. It was not the best weather for getting out Stargazing | :38:04. | :38:07. | |
Live, but I can tell you there are going to be more clear skies | :38:08. | :38:11. | |
tonight. It won't be warm if you head out and about, widespread frost | :38:12. | :38:15. | |
coming and icy patches, and some patchy cloud, but if we are lucky | :38:16. | :38:22. | |
enough to see Aurora Borealis, and talking to my colleagues at the | :38:23. | :38:25. | |
space centre, it could arrive, we might see it in northern England and | :38:26. | :38:28. | |
Northern Ireland, but if we don't see it, plenty more to look at in | :38:29. | :38:32. | |
the sky and we should have plenty of clear skies. Come tomorrow, there | :38:33. | :38:38. | |
will still be cloud across southern and eastern areas, but for many, | :38:39. | :38:42. | |
with the cold light, it could be clear and plenty to see. If you are | :38:43. | :38:48. | |
not lucky enough to see Aurora Borealis, Jupiter is meant to be | :38:49. | :38:51. | |
bright in the sky, and the good news is that into the weekend, Friday and | :38:52. | :38:55. | |
Saturday, it looks clearer, but it will be cold, so wrap up warm. | :38:56. | :39:01. | |
Mark is under the stars in egg, with a huge crowd of other stargazers. | :39:02. | :39:12. | |
Hello, I'm still here. Now, all evening I've been at the Royal | :39:13. | :39:15. | |
Holloway University at one of the biggest star spectaculars in the | :39:16. | :39:19. | |
country - and this is where lots of budding scientists start their | :39:20. | :39:21. | |
astronomy careers. This is where many budding scientists start their | :39:22. | :39:26. | |
careers. And one of the first things any beginner has to is learn their | :39:27. | :39:29. | |
way around the night sky. So I've decided to enlist the help of Royal | :39:30. | :39:32. | |
Holloway's Physics department to bring to life the one constellation | :39:33. | :39:36. | |
everyone should know and I'm also going to use some ingenious BBC | :39:37. | :39:39. | |
software to create a human constellation. There is the gang of | :39:40. | :39:41. | |
students, we have armed them with torches. There you go, guys! With a | :39:42. | :39:44. | |
bit of BBC magic, we will try to create a human constellation. If you | :39:45. | :39:49. | |
look at the sky on any night, you can seek seven bright stars. There | :39:50. | :39:54. | |
they are appearing, and as those stars form, it is a shape we are | :39:55. | :40:01. | |
familiar with, the Plough. It's one we can see at any time of night from | :40:02. | :40:06. | |
the UK. The lines are wobbly, but maybe that is gravitational lenses. | :40:07. | :40:10. | |
You should be able to see this at any time of night, but the itself is | :40:11. | :40:15. | |
Ursa Major. Those are the stars slowly appealing -- appearing, and | :40:16. | :40:21. | |
they are slowly joining up the lines, that is the great Bear, the | :40:22. | :40:26. | |
name of the constellation, where we find MA and M 82. -- M81. I can't | :40:27. | :40:36. | |
quite see a bear, even squinting, but if you look now, you can make | :40:37. | :40:42. | |
the shape of the bear. The important thing about this constellation is | :40:43. | :40:47. | |
that there are two stars at the end of the bowl that point towards | :40:48. | :40:51. | |
Polaris, the North polar Star, and that is the only fixed star in the | :40:52. | :40:58. | |
sky. If you can find the poll by looking at those two points, you can | :40:59. | :41:03. | |
find anything in the night sky -- pole. And that means navigating is | :41:04. | :41:09. | |
easy, as I found, when I took to the seas. I might know my way around the | :41:10. | :41:14. | |
night sky, but I don't know how to use the knowledge down here on | :41:15. | :41:19. | |
Earth. Fortunately, I'm not alone. With me is natural navigation expert | :41:20. | :41:28. | |
Tristan Gooley. Without even knowing where we are starting, we are | :41:29. | :41:32. | |
navigating to Alderney. Tristan, nice to meet you. Alderney is 50 | :41:33. | :41:40. | |
miles from England, and just three miles across, so it will make for a | :41:41. | :41:46. | |
small target as night falls. Before we can think about finding the | :41:47. | :41:49. | |
island, we need to think exactly where the boat is. We are not using | :41:50. | :41:56. | |
GPS, radar, any modern gizmos. I have even had my phone taken of me. | :41:57. | :42:01. | |
With the sun setting, we better make a start. To calculate position on | :42:02. | :42:05. | |
Earth, we need to work out which area of the night sky we are under. | :42:06. | :42:11. | |
And Polaris, the star always due north, is the perfect place to | :42:12. | :42:17. | |
start. If you're standing on the North Pole, the star directly above | :42:18. | :42:22. | |
your head would be Polaris, and if you travel south, that star gets | :42:23. | :42:26. | |
steadily lower and lower, and if you reach the equator, it will be on the | :42:27. | :42:30. | |
horizon. We are halfway between the equator and the North Pole, so we | :42:31. | :42:34. | |
should expect the North Star to be halfway between the horizon and | :42:35. | :42:40. | |
directly above. Tristan uses the sextant to measure Polaris and give | :42:41. | :42:44. | |
us the latitude, how far north or south we are. But what about East or | :42:45. | :42:49. | |
West? That is trickier. Unlike Polaris, all the other stars move | :42:50. | :42:54. | |
around the sky through the night. Tristan sets his sights on Vega, so | :42:55. | :43:02. | |
we can work out how long that -- how far along the path it is. Timing is | :43:03. | :43:09. | |
critical. Now! Like every star, the timing of the path is predicted. | :43:10. | :43:20. | |
That is 59 degrees and 47 minutes. Its position at any moment depends | :43:21. | :43:23. | |
on how far east or west you are, the longitudinal. The time now is for 30 | :43:24. | :43:32. | |
a.m. And 50 seconds. Now we know the longitudinal attitude, we can | :43:33. | :43:35. | |
pinpoint where we are on the map, so we can tell what direction Alderney | :43:36. | :43:42. | |
should be. -- 4.30am. We are about five miles from land, so we can | :43:43. | :43:46. | |
pretty much say it is five miles due south. It is a pretty creepy | :43:47. | :43:52. | |
experience heading into the darkness. I can barely see anything | :43:53. | :43:56. | |
ahead of me. We are having to put our faith completely in the stars. | :43:57. | :44:03. | |
The signpost now is the star due south at this time of night. If we | :44:04. | :44:08. | |
look up, you can see Pegasus. If we look at the bottom left-hand star, | :44:09. | :44:14. | |
that is very close to the North Star, so that's a good one to follow | :44:15. | :44:19. | |
now. We sail into the darkness were a couple of hours and the stars | :44:20. | :44:25. | |
constantly move on, so once again, it's time to realign the sites. | :44:26. | :44:29. | |
Judging by where Polaris is, we properly need to head for the group | :44:30. | :44:38. | |
of stars called Cetus. If we look at that group of stars, and you lower | :44:39. | :44:42. | |
your gaze to the horizon, what do you see? I can see a clump of | :44:43. | :44:47. | |
lights, where I am confident that that is Alderney. Looks good to me. | :44:48. | :44:55. | |
The constellation known as the sea monster is currently south of us, | :44:56. | :44:59. | |
and it is guiding us in. One hour later, out of the inky blackness, we | :45:00. | :45:03. | |
see the shape of Alderney. We have made it. You can see where the Pope | :45:04. | :45:12. | |
kisses the ground. I can feel it coming on. We have travelled well | :45:13. | :45:17. | |
over 50 miles and managed to hit a small target using just the stars to | :45:18. | :45:21. | |
navigate by, but unfortunately, it has turned cloudy, so no way I can | :45:22. | :45:25. | |
enjoy a nice dark skies that Alderney has to offer. I guess it is | :45:26. | :45:38. | |
time for bed. Navigating by the stars seems archaic, but the | :45:39. | :45:43. | |
commander of the space shuttle navigates by the stars as well. | :45:44. | :45:54. | |
Let's play guess the planet. That is Mars. Has the biggest volcano in the | :45:55. | :46:03. | |
solar system. Next one, what do we have there? That is Mercury. No way | :46:04. | :46:09. | |
would we have had pictures like this without messenger being in orbit. | :46:10. | :46:13. | |
What is fascinating is in these permanently shadowed craters, | :46:14. | :46:21. | |
Mercury only presents one place, you can get zones that are so cold, you | :46:22. | :46:27. | |
can get water and ice mixed in with the pebbles. There is water on | :46:28. | :46:35. | |
Mercury, frozen solid. And planet you cannot recognise easily? | :46:36. | :46:46. | |
Neptune. Nobody has ever seen this planet. This has been worked out by | :46:47. | :46:52. | |
a team of scientists at Exeter University. This is remarkable, it | :46:53. | :47:01. | |
is a genuine simulation. A planet we have never seen. This is how they | :47:02. | :47:08. | |
did it. Planets beyond our solar system are | :47:09. | :47:12. | |
very far away and we have little hope of imaging verse surfaces. So | :47:13. | :47:17. | |
finding anything out about what these worlds are like, might seem | :47:18. | :47:22. | |
like an impossible task. But a team of planet hunters at Exeter | :47:23. | :47:27. | |
University are gearing up to do just that. With a new technique that may | :47:28. | :47:31. | |
one day help us identify another habitable Earth. Planets can be | :47:32. | :47:42. | |
detected by the almost imperceptible dip they cause as they pass in front | :47:43. | :47:47. | |
of their staff. And that is all of the scientists have to work with. | :47:48. | :47:52. | |
But with some ingenious methods they are beginning to construct these | :47:53. | :48:03. | |
distant worlds. This stock has been working on one of the current | :48:04. | :48:06. | |
planets. Orbiting around a star 150 light years away. When I started | :48:07. | :48:14. | |
there was only one planet we could study the atmosphere of. This is an | :48:15. | :48:24. | |
image of the host star. David measures precisely how the light | :48:25. | :48:31. | |
from the host star changes as this iris filters it through its | :48:32. | :48:34. | |
atmosphere. Starlight is made up of many different colours. And by | :48:35. | :48:43. | |
analysing the colours that are absorbed by the planet's atmosphere | :48:44. | :48:48. | |
when it passes across the star, David can work out what is in the | :48:49. | :48:53. | |
atmosphere and even how thick it is. Unfortunately, it does not sound | :48:54. | :49:06. | |
very welcoming. It looks quite alien, it is mainly made of hydrogen | :49:07. | :49:16. | |
and helium. They have also detected sodium in the atmosphere and not a | :49:17. | :49:19. | |
place that could support life as we know it. But even if they found | :49:20. | :49:24. | |
oxygen and nitrogen, an earthlike atmosphere, to predict if it could | :49:25. | :49:29. | |
be habitable we have to see how the atmosphere behaves. And that is how | :49:30. | :49:36. | |
David was Makro Collie comes in. We are trying to interpret these | :49:37. | :49:41. | |
observations of these climates. To do this Nathan's team have | :49:42. | :49:47. | |
reconstruct did its atmosphere in the most sophisticated climate | :49:48. | :49:52. | |
prediction model around. The Met Office's model of planet Earth. This | :49:53. | :50:00. | |
brings the planet to life. This is the night side facing away from the | :50:01. | :50:08. | |
start. This is the heart day side, temperatures of a few thousand | :50:09. | :50:13. | |
degrees. And the arrows represent the wind flying past, incredibly | :50:14. | :50:21. | |
fast. With this model we can dive through its atmosphere and it | :50:22. | :50:25. | |
reveals 3000 miles down there are even stormy conditions. Very violent | :50:26. | :50:34. | |
region, and nastier place to be, for a human anyway. Although this might | :50:35. | :50:43. | |
not be the earthlike than it we are looking for, Nathan hopes modelling | :50:44. | :50:48. | |
its atmosphere will help the search. Models like this can make a | :50:49. | :50:51. | |
contribution in trying to find an alert analogue or an alert to win | :50:52. | :50:55. | |
and trying to understand that atmosphere. -- and Earth twin. You | :50:56. | :51:06. | |
can see the behaviour of the fluids? The model predicts there is an | :51:07. | :51:14. | |
equatorial band, so a Jetstream at the equator. Also a couple of | :51:15. | :51:22. | |
storms, that is Jupiter's red spot. This is orbiting around what we call | :51:23. | :51:36. | |
a K star. But it is the M stars that are the most common in the galaxy. | :51:37. | :51:42. | |
What these models have shown is that does not preclude the existence of | :51:43. | :51:47. | |
life potentially on these planets. These storms distribute the heat | :51:48. | :51:53. | |
around the planet. So we can add myth about 75% of the stars in the | :51:54. | :51:59. | |
galaxy could support life. But this cannot support life? Know it also | :52:00. | :52:09. | |
has silicon rain, so it rains glace. If you do last 20 years ago, perhaps | :52:10. | :52:16. | |
ten years ago, we did not know about the other solar systems in the | :52:17. | :52:23. | |
galaxy. Now we have over 1000 planets beyond the solar system | :52:24. | :52:29. | |
confirmed. Many of them looking at a planet as it passes across the | :52:30. | :52:34. | |
star. This is an encyclopaedia of the planets passing by. The most | :52:35. | :52:37. | |
interesting than it is, the most interesting candidates are the 12 | :52:38. | :52:42. | |
planets that have been found and are most likely to be second earths. | :52:43. | :52:48. | |
They are in what is called the habitable zone of the staff. We can | :52:49. | :52:56. | |
also tell about the gases within the atmosphere? We can look at the | :52:57. | :53:02. | |
atmosphere to ask questions such as is their oxygen in the atmosphere? | :53:03. | :53:08. | |
Carbon dioxide, so the likes of Venus, it's atmosphere is too dense. | :53:09. | :53:14. | |
But we can look for industrial pollutants in the atmosphere. If you | :53:15. | :53:21. | |
found CFC which are not created naturally. You would know there is | :53:22. | :53:27. | |
industrial civilisation. We're not far away from being able to do that. | :53:28. | :53:36. | |
For the final time, we are crossing over to Liz who has been circling | :53:37. | :53:45. | |
the skies in Norway. We are still admiring the aurora borealis. It has | :53:46. | :53:54. | |
changed quite a lot? Yes, it has actually hit now. I am not landing | :53:55. | :54:02. | |
now. This could burst into a multicoloured ray of light? This is | :54:03. | :54:13. | |
the beginning of it. It is changing by the second. Do Rohrer occur | :54:14. | :54:22. | |
regularly? There is always something there, whether it be a faint glow up | :54:23. | :54:27. | |
to a full-blown display like we are going to get now. As we're looking | :54:28. | :54:32. | |
at this appear, there is the equivalent happening in the South? | :54:33. | :54:42. | |
Yes, in the southern Oval as well. We have been sending our hunters out | :54:43. | :54:50. | |
to get us some pictures. This was captured in Tasmania several hours | :54:51. | :54:57. | |
ago. It is beautiful. Seven hours ago then, that would have been | :54:58. | :55:02. | |
manifesting itself appear, the equivalent of it somewhere in the | :55:03. | :55:07. | |
zone? Yes, the northern zone as well. So many questions from viewers | :55:08. | :55:14. | |
about the nature of this. Someone asking, are they identical in | :55:15. | :55:20. | |
appearance? As one happens up here, the exact same patterns and | :55:21. | :55:26. | |
features, happens down there? If you are standing the same distance, yes | :55:27. | :55:31. | |
that is what would happen. When it comes to them being mirrored image | :55:32. | :55:37. | |
of each others, one is mirroring the other in shape and position? It was | :55:38. | :55:42. | |
thought for a long time that was the case, but in 2002 a couple of NASA | :55:43. | :55:48. | |
spacecraft by chance just imaged both ovals so they were able to | :55:49. | :55:52. | |
compared them. There are subtle differences. When things come from | :55:53. | :55:57. | |
the solar wind it can make both ovals move in opposite directions. | :55:58. | :56:01. | |
On the regions of maximum at liberty in the ovals tilt towards the dawn | :56:02. | :56:07. | |
side of the Earth as well. It is nearly time for us to say goodbye, | :56:08. | :56:13. | |
but it has been glorious. We are still waiting for changes in | :56:14. | :56:17. | |
colours. It has been an ambitious mission over the last three nights | :56:18. | :56:25. | |
and a privilege to observe this. We were lucky when we were on the | :56:26. | :56:29. | |
ground? Extremely lucky, I have known people who waited two weeks | :56:30. | :56:35. | |
and saw nothing at all. There is so much to learn, but somewhere in the | :56:36. | :56:40. | |
not too distant future, not only will we be able to admire this, we | :56:41. | :56:45. | |
will have learned enough to say exactly what is going on at that | :56:46. | :56:50. | |
moment in time. VAT for me is thrilling and it brings home are | :56:51. | :56:54. | |
intrinsic relationship with our start. That is it from us. We will | :56:55. | :56:59. | |
keep rolling until the end of the show. It has been an honour to be | :57:00. | :57:07. | |
part of this live from 30,000 feet. It is good night from northern | :57:08. | :57:14. | |
Norway. I don't know what to say without being hyperbolic. We knew it | :57:15. | :57:21. | |
was a gamble and we knew we could not get nothing. Mark, how are you | :57:22. | :57:32. | |
getting on? We have had a wonderful evening, the | :57:33. | :57:37. | |
unforgettable human constellation. A Milky Way projection the size of a | :57:38. | :57:42. | |
house and there is a simulator somewhere. Not forgetting the | :57:43. | :57:47. | |
wonderful clear skies, we have seen beautiful images are planets and | :57:48. | :57:52. | |
beautiful images of galaxies. These guys are going to be here for some | :57:53. | :57:55. | |
time yet so I am going to join the party. So from me and everyone here, | :57:56. | :58:04. | |
goodbye. Rebecca, some names coming in. Nine Jodrell Scope, I like that. | :58:05. | :58:16. | |
We will be discussing this in a moment. Thank you for all of you who | :58:17. | :58:24. | |
have taken part. What a wonderful way to finish the series. Let's take | :58:25. | :58:30. | |
a last look at those images captured from the Ark ticks circle. It is | :58:31. | :58:36. | |
incredible. Thanks to all of our viewers who have sent in | :58:37. | :58:40. | |
photographs, or just watching at home. The show may be over for | :58:41. | :58:49. | |
another year, joiners in two minutes per K9's space tributes. The first | :58:50. | :58:56. | |
time we made this programme four years ago was to encourage you to | :58:57. | :59:02. | |
look up and go outside. We have described the planets, the space | :59:03. | :59:07. | |
probes orbiting the planets, let your imagination fly and we will see | :59:08. | :59:13. | |
you next year. Also in two minutes as well. | :59:14. | :59:22. |