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Last night we spoke to the last man on the moon. Tonight we are heading | :00:11. | :00:20. | |
to the centre of our galaxy. I am Brian Cox, he is Dara O'Briain, and | :00:20. | :00:30. | |
:00:30. | :00:55. | ||
Welcome back to Jodrell Bank for the second night of Stargazing Live. | :00:56. | :00:59. | |
Yesterday, we concentrated on the moon, which is a bit unfair because | :00:59. | :01:03. | |
it did not rise for a couple of hours after we went off air. We | :01:03. | :01:07. | |
were relying on people staying up late or getting up early, and | :01:07. | :01:12. | |
people sent us a number of photographs. This is a beautiful | :01:12. | :01:21. | |
picture of the Moon which was taken by James West. We have another one, | :01:21. | :01:30. | |
it taken by James Dyson. I am fond of this picture. It is a beautiful | :01:30. | :01:36. | |
picture of a cluster of young stars which were formed together. Most | :01:36. | :01:40. | |
people can see about six or seven of them with the naked eye but you | :01:40. | :01:45. | |
can see tens of them through a telescope. That transient. It will | :01:45. | :01:49. | |
drift apart and will not be a cluster anymore. We have had the | :01:49. | :01:54. | |
most incredible response so far. A lot of you have contacted us about | :01:54. | :01:58. | |
Captain Cerna. Some of you wanted to know why the Stars and Stripes | :01:58. | :02:01. | |
flag looked like it was flapping in the wind when there is no | :02:01. | :02:05. | |
atmosphere in the -- on the moon. It sounds like a conspiracy | :02:05. | :02:09. | |
question. The answer is there is a piece of metal in it because they | :02:09. | :02:13. | |
would knew it would flatten if there was no atmosphere. If you | :02:13. | :02:18. | |
think we did not land on the moon, turn over to ITV, I did not -- I do | :02:18. | :02:25. | |
not want to! You can keep questions coming into us, or you can tweet us. | :02:25. | :02:30. | |
You can join the online chatroom, Talk Stargazing, at | :02:30. | :02:35. | |
bbc.co.uk/stargazing. To see what is in the skies over Macclesfield | :02:35. | :02:39. | |
tonight, are there to mark and friends, and a very special guest | :02:39. | :02:44. | |
astronomer. Good evening, I am joined not only | :02:44. | :02:48. | |
by a veritable army of astronomers from the Liverpool and Macclesfield | :02:48. | :02:51. | |
astronomy society, how are you doing? They sound like they're | :02:51. | :02:56. | |
having some fun. They have joined us for our special star party at | :02:56. | :03:00. | |
Jodrell Bank. You can find out details of the events around the | :03:01. | :03:06. | |
country near where you are, at our website, bbc.co.uk/stargazing. | :03:06. | :03:12. | |
Standing relatively close to this new telescope is Impressionist and | :03:12. | :03:21. | |
space, Jon Culshaw. Well come. What is it about astronomy? I remember | :03:21. | :03:25. | |
receiving a book by Patrick Moore when I was nine and I read it to | :03:25. | :03:31. | |
cover to cover, and I was hooked. Any time there was a -- the Moon | :03:31. | :03:36. | |
was out, I could not resist having a look. Do you use these binoculars | :03:36. | :03:43. | |
often? Yes. I have not got a stand for them yet. You do need at quite | :03:43. | :03:49. | |
an impressive stand. The sky is looking incredibly Claire so come | :03:49. | :03:56. | |
back to us later on. -- incredibly clear. | :03:56. | :03:59. | |
Ironically, the thing we are going to talk about is not actually | :03:59. | :04:04. | |
visible. We are going to talk about black holes. The truth is that from | :04:04. | :04:10. | |
a physicist's perspective, we do not really understand them. Here is | :04:10. | :04:15. | |
an introduction to the enigmatic inhabitants of the cosmos. | :04:15. | :04:18. | |
Black holes are some of the strangest, most mysterious and | :04:18. | :04:24. | |
destructive things that exist in the universe. There is one here. | :04:24. | :04:29. | |
And there is probably another one here. But you can't see them. And | :04:29. | :04:34. | |
they can't be photographed. So we have to use computer graphics to | :04:34. | :04:38. | |
try to explain what they are and how they are formed. Black holes | :04:38. | :04:43. | |
are cosmic bodies with such immense gravity, nothing can escape them. | :04:43. | :04:51. | |
For their lives to start, a star has to die. Stars are effectively | :04:51. | :04:56. | |
huge nuclear reactors, fuelled by hydrogen. At the end of their lives, | :04:56. | :05:03. | |
when the fuel runs out, they dive. When this happens, stars the size | :05:03. | :05:09. | |
of our sun with the, to become much smaller bodies, known as white | :05:10. | :05:18. | |
dwarfs. When bigger stars die, they destroy themselves in explosions | :05:18. | :05:23. | |
known as supernovas. If the explosion is 30 times the mass of | :05:23. | :05:28. | |
the Sun, black holes can be formed. As the outer layers of the star | :05:28. | :05:32. | |
blow off into space, the core of the Star, which can be as big as a | :05:32. | :05:36. | |
planet, is crushed down to almost nothing. The whole process can | :05:36. | :05:41. | |
taste -- tastes -- take less than a second. What is left is an object | :05:41. | :05:45. | |
that has the same mass as the core of the star, but is packed into a | :05:45. | :05:50. | |
much less -- much smaller space. Despite being significantly smaller, | :05:50. | :05:55. | |
it still exerts the same gravitational pull. This incredibly | :05:55. | :05:59. | |
powerful entity, which is small but massive at the same time, is what | :05:59. | :06:04. | |
we have come to know as a black hole. From the moment of their | :06:04. | :06:10. | |
creation, some black holes begin firing out great jets of radiation. | :06:10. | :06:14. | |
The immense gravitational pull from the holes means that anything that | :06:14. | :06:19. | |
strays too close to them is powerless to escape. Even a nearby | :06:19. | :06:23. | |
star would be torn apart, the matter from its surface being | :06:23. | :06:29. | |
pulled into orbit around the hole. That poll from the black hole is so | :06:29. | :06:34. | |
strong that eventually, it is eventually -- it is impossible to | :06:34. | :06:40. | |
escape -- that poll. This terrifying point of no return is | :06:40. | :06:45. | |
known as the event horizon. Everything in its path is sucked in, | :06:45. | :06:48. | |
and the more -- the more it swallows, the bigger the black hole | :06:48. | :06:52. | |
becomes. Beyond the event horizon, not even light can travel fast | :06:52. | :06:55. | |
enough to escape. That is why you can't see them, and how they get | :06:56. | :07:02. | |
their name. They are quite literally black holes in space. If, | :07:02. | :07:07. | |
by some miracle, you were to survive the tidal forces at the | :07:07. | :07:11. | |
Event Horizon and fell into a black hole, you would be ripped apart. | :07:11. | :07:17. | |
But nobody knows how long that would take. | :07:17. | :07:21. | |
We are going to go to the age of physics and also the heart of our | :07:21. | :07:25. | |
Garroch -- galaxy. It is a journey we should start right here. Let's | :07:25. | :07:29. | |
take a look at where we are in our galaxy. This is the Milky Way, | :07:29. | :07:32. | |
taken from outside it, so it is a taken from outside it, so it is a | :07:32. | :07:37. | |
graphic. That is the location of earth. We had this as a question | :07:37. | :07:41. | |
from Gary in Belfast, how do we know where the earth is and how can | :07:41. | :07:46. | |
we know what it looks like? There is something like between 200 and | :07:46. | :07:52. | |
400 billion stars in the Milky Way. It from there, you can't see it all, | :07:52. | :08:02. | |
:08:02. | :08:03. | ||
we use telescopes like the Lovell, radio astronomy. Looking at the | :08:03. | :08:09. | |
radio emission, you can see how bright the universe is. Also, by | :08:09. | :08:14. | |
looking at how that shifts, you can see how fast it is moving. So you | :08:14. | :08:17. | |
can work out precisely the structure and speed of rotation of | :08:17. | :08:22. | |
our galaxy. When we look into the sky, every star we see is part of | :08:22. | :08:25. | |
the Milky Way. Everything you can see with the naked eye apart from | :08:25. | :08:31. | |
one thing. We have a life picture of that one thing. This is from | :08:31. | :08:37. | |
Macclesfield now. Where are we? This is a picture of the Andromeda | :08:37. | :08:41. | |
galaxy. This is the nearest neighbouring galaxy, about 2 | :08:41. | :08:44. | |
million light years away. There is something like a trillion stars in | :08:44. | :08:51. | |
that galaxy. That is a live picture now of Andromeda. The Galaxy is | :08:51. | :08:55. | |
basically a collection of stars? They are. That is the nearest | :08:55. | :09:00. | |
neighbour, so there are two of them. This is one of the most famous | :09:00. | :09:03. | |
pictures in astronomy. It is a picture of the piece of sky you | :09:03. | :09:08. | |
would cover, if you took a five pence piece and held it about 25 | :09:08. | :09:13. | |
metres away, cover a little piece of sky. It was a piece of sky that | :09:13. | :09:18. | |
is anti from the surface of the Earth as far as we could tell, but | :09:18. | :09:21. | |
the Hubble take -- telescope took this picture and it is far from | :09:21. | :09:27. | |
empty. There are over 10,000 galaxies in this image, the most | :09:27. | :09:33. | |
distant his 13 billion light years away. If you extend that over the | :09:33. | :09:40. | |
entire sky, there are around 350 billion galaxies. Although we can | :09:40. | :09:44. | |
see the Andromeda galaxy in the night sky, that is pretty much the | :09:44. | :09:47. | |
only visible to the naked eye in this hemisphere, but there is | :09:47. | :09:57. | |
plenty more visible in the southern Welcome to the southern African | :09:57. | :10:01. | |
large telescope in the middle of the Karoo desert. The weather has | :10:01. | :10:04. | |
been rubbish again, but it looks like it might be clearing up, which | :10:04. | :10:13. | |
is why the SALT telescope is moving into position. There are two | :10:13. | :10:18. | |
galaxies visible to the naked eye, closer than Andromeda. A couple of | :10:18. | :10:22. | |
nights ago I went galaxy gazing with budding astronomers from the | :10:22. | :10:25. | |
nearby town. In the middle of the Karoo desert, | :10:26. | :10:30. | |
about 200 miles north-east of Cape Town, lies the tiny town of | :10:30. | :10:34. | |
Sutherland. Before the South African astronomical observatory | :10:34. | :10:37. | |
relocated here in the mid-70s, this was just a small farming community | :10:37. | :10:45. | |
with a few hundred people. But now, Sutherland is home to one of the | :10:45. | :10:50. | |
largest telescopes in the world, and that has made it something of a | :10:50. | :10:54. | |
tourist destination. Astronomers are also keen that the whole | :10:54. | :10:59. | |
community understands just what a special star-gazing spot this is. | :10:59. | :11:07. | |
Anthony runs the Observer drew's outreach programme. -- the | :11:07. | :11:12. | |
observatory's outreach programme. Why are they flying kites? You have | :11:12. | :11:16. | |
to look up, it is a way of exposing them to the night sky. As the stars | :11:16. | :11:21. | |
come out, they will change their attention... To what is happening. | :11:21. | :11:25. | |
Sometimes before a lucky, we get a shooting star, and somebody will | :11:25. | :11:30. | |
ask, what just happened? One of the astronomers down here, at David | :11:30. | :11:37. | |
Gilbank, will be talking to the kids about galaxies later on. | :11:37. | :11:42. | |
good way to describe a galaxy is as a city of stars. Our Milky Way is | :11:42. | :11:46. | |
all the stars that belong to the Star City. If we can see our galaxy | :11:46. | :11:50. | |
from the outside, we would see something that looks like the East | :11:50. | :11:55. | |
shape of a dinner plate. We live about two-thirds of the way out | :11:55. | :11:59. | |
from the centre. When we look at the night sky, we are actually | :11:59. | :12:02. | |
looking into the thickest part of the stars, as if we are looking | :12:02. | :12:07. | |
through the edge of the plate. many stars are in the Milky Way? | :12:07. | :12:13. | |
good question. They are about 100 billion within our own galaxy. | :12:13. | :12:17. | |
is the closest galaxy to our own Milky Way? The nearest galaxy is | :12:17. | :12:23. | |
called the Andromeda galaxy, but there are lots of much that smaller | :12:23. | :12:27. | |
galaxies in between. -- the mirrors that is the same size. This misty | :12:27. | :12:33. | |
patch looks like a small version of the Milky Way. | :12:33. | :12:39. | |
This is called the Large Magellanic Cloud. This is the satellite galaxy | :12:39. | :12:44. | |
of the Milky Way. The Large Magellanic Cloud is the satellite | :12:44. | :12:48. | |
galaxy of the Milky Way that orbits around us. What you are looking at | :12:48. | :12:53. | |
through the telescope, it looks like a bright patch, this is called | :12:53. | :12:59. | |
the tarantula nebula. It looks like little legs of the Spider. It is a | :12:59. | :13:05. | |
cloud of gas in which stars are being born. You can see there are | :13:05. | :13:10. | |
new starts by looking around, we can see bright blue luminous stars. | :13:10. | :13:15. | |
Why are the new stars blue? If you think about the taps on the sink, | :13:15. | :13:21. | |
blue is cold, bread is hot, it is the opposite in astronomy. -- red | :13:21. | :13:25. | |
is hot. Imagine taking a piece of iron into a fire, it will start of | :13:25. | :13:29. | |
glowing red hot, that is the coolest you can get. If you heat it | :13:29. | :13:33. | |
further, it will glow white hot. If you could eat it furthered without | :13:33. | :13:39. | |
the metal Motty, it would be blew hot. Blue is the hottest iPod star | :13:39. | :13:49. | |
:13:49. | :13:53. | ||
-- without the metal nothing. Back These very bright stars do not live | :13:53. | :13:57. | |
very long. If you see these hot blue stars in the galaxy, you know | :13:57. | :14:02. | |
they have been put there recently. If there is no new star formation | :14:02. | :14:07. | |
going on, you will only see these older stars, which will appear red. | :14:07. | :14:12. | |
They are red because they are older? That is right. What stops | :14:12. | :14:16. | |
star formation in galaxy? To form stars we need these nebula, these | :14:16. | :14:21. | |
clouds of gas. We know something must be removing the gas and | :14:21. | :14:23. | |
preventing it from forming stars, but we don't know what that is, | :14:23. | :14:31. | |
this is one of the things I am trying to answer in the work I am | :14:31. | :14:35. | |
doing with SALT. There is also a Small Magellanic | :14:35. | :14:41. | |
Cloud in the southern hemisphere. In fact, SALT altered its viewing | :14:41. | :14:46. | |
window in order to observe it in its entirety. It has about a 10th | :14:46. | :14:49. | |
of the stars of the large cloud, and it is more elongated and the | :14:49. | :14:53. | |
large one, but we look at it head on from Earth. The magellanic | :14:53. | :14:57. | |
clouds are part of this local group of galaxies, what is the local | :14:57. | :15:01. | |
group? It is the name we give to the collection of nearby galaxies | :15:01. | :15:05. | |
bound together by gravity. It consists of three big galaxies | :15:05. | :15:08. | |
including the Milky Way and Andromeda, and debris several dozen | :15:08. | :15:13. | |
smaller galaxies. -- may be several dozen. You have been attempting to | :15:13. | :15:16. | |
find out how many galaxies there are in the universe, you have | :15:16. | :15:26. | |
:15:26. | :15:27. | ||
looked at 3% of the sky, what have We are mainly looking for galaxy | :15:27. | :15:34. | |
clusters and we have found 38,000, which amounts to 3 million galaxies | :15:34. | :15:38. | |
in one tiny speck of the sky. Galaxies are everywhere you look. | :15:38. | :15:41. | |
They are distributed across the universe in a cosmic web of | :15:41. | :15:44. | |
filaments and astronomers are only just beginning to understand what | :15:44. | :15:50. | |
that might look like. Join me later when I find out how galaxies growth. | :15:50. | :15:54. | |
Apparently the Milky Way is in for a bumpy ride. | :15:54. | :16:02. | |
Here is a positive message for those people needing more exercise. | :16:02. | :16:07. | |
You cannot be at rest. We travel around the sun but also around the | :16:07. | :16:14. | |
Milky Way. Of course we travel round the Sun every year. But the | :16:14. | :16:18. | |
sun is one of 200 billion stars in the Milky Way galaxy. Our whole | :16:18. | :16:22. | |
solar system is travelling around the galactic centre. We think it | :16:22. | :16:27. | |
takes about 225 million years to make one orbit. If you think about | :16:27. | :16:30. | |
that, that means that since this formation of the solar system we | :16:30. | :16:35. | |
have made 20 orbits, which is 20 galactic years, if you like. The | :16:35. | :16:39. | |
most remarkable thing about that is if you think that humans have been | :16:39. | :16:44. | |
around for a long time, we have been around for 11 thousandth of a | :16:44. | :16:52. | |
single galactic year, which is like a afternoon. We will get an | :16:52. | :16:56. | |
explanation of how that formation happens but first let's go into the | :16:56. | :17:06. | |
:17:06. | :17:09. | ||
field. This guy's a miraculously clear for us. -- the sky is run | :17:09. | :17:15. | |
Cristie Kerr for us and we have found the Andromeda galaxy. For you | :17:15. | :17:25. | |
:17:25. | :17:27. | ||
are not mood to astronomy. -- you are not new to astronomy. That is | :17:27. | :17:31. | |
right. A bit of cloud has gone across and it can be quite helpful | :17:31. | :17:37. | |
if it takes away some of the glare. But not too much. Oh exactly. | :17:37. | :17:42. | |
was the first time that you have seen galaxies? The first time I saw | :17:42. | :17:46. | |
Andromeda was in the 80s. I think my favourite view of our galaxy, | :17:46. | :17:52. | |
the Milky Way, was in Kenya a few years ago. Far away from any kind | :17:52. | :17:58. | |
of light pollution. We have a wonderful, polished sky tonight so | :17:58. | :18:03. | |
we can make out the stars. It is beautiful. It seems that two thirds | :18:03. | :18:07. | |
of Western Europe cannot see our galaxy because of light pollution. | :18:07. | :18:11. | |
That is basically excess and intrusive light that Brighton's the | :18:11. | :18:21. | |
:18:21. | :18:22. | ||
night sky. On your screens is Europe, and it looks spectacular | :18:22. | :18:26. | |
but that is basically the glare from streetlights, offices and | :18:26. | :18:30. | |
houses. The effects of excess lighting are plentiful. It affects | :18:30. | :18:34. | |
the environment, wasting vast amounts of money, and it can | :18:34. | :18:38. | |
disturb wildlife. It can even affect your own body clock. More | :18:39. | :18:48. | |
:18:49. | :18:49. | ||
crucially it is disastrous for I have come to the Royal | :18:49. | :18:52. | |
Observatory in Greenwich, one of my favourite places and a real | :18:52. | :18:59. | |
landmark of British astronomy. I am here to meet a group of stargazers | :18:59. | :19:05. | |
who all live nearby in London. I want to know about their experience | :19:05. | :19:09. | |
of astronomy in the city and find out how they are affected by light | :19:09. | :19:14. | |
pollution. So what is it that you find frustrating about light | :19:14. | :19:18. | |
pollution? It is just the glowing in the sky that prevents me from | :19:19. | :19:23. | |
seeing what I want to see. Especially when I am with my | :19:23. | :19:28. | |
children. I see the images in books and on television and they always | :19:28. | :19:32. | |
ask why they cannot see things like that. Clearly the answer is light | :19:32. | :19:37. | |
pollution. It is constant, really. Your eyes never adapt fully to the | :19:38. | :19:41. | |
night sky. Security lights at debating where animals in gardens, | :19:41. | :19:50. | |
constantly flashing. -- activating by animals. Some of the brighter | :19:50. | :19:54. | |
stars we cannot even say because of the constant orange glowing that is | :19:54. | :20:00. | |
there all the time. When Greenwich Observatory was first founded in | :20:00. | :20:05. | |
the 1600's, it was a long way outside the centre of London. Now | :20:05. | :20:10. | |
it looks straight out over the city. And all of these lights from the | :20:11. | :20:16. | |
Millennium Dome to the individual street lights have blocked the sky | :20:16. | :20:24. | |
it from view. As London astronomers, these people rarely get to | :20:24. | :20:28. | |
experience proper darkness. I am taking them somewhere to experience | :20:28. | :20:32. | |
stars without the glowing. I am taking you to a proper dark sky. | :20:32. | :20:36. | |
What would you like to see? naked eye view of the Andromeda | :20:36. | :20:41. | |
galaxy which people say is possible. That would make my day. I am | :20:41. | :20:45. | |
longing to see the Milky Way. I just love seeing it in photographs | :20:45. | :20:49. | |
because it is beautiful. Just to see that with my own eyes would be | :20:49. | :20:55. | |
a dream, really. How about yourself? I am dying to see a | :20:55. | :21:00. | |
galaxy, any galaxy will do! Just to see it with my own eyes, in real | :21:00. | :21:08. | |
time, something that is so far away, that would be amazing. So to fulfil | :21:08. | :21:14. | |
the wishes of the city astronomers, we are leaving the bright lights | :21:14. | :21:20. | |
behind and heading somewhere really, really dark. Now we have come all | :21:20. | :21:24. | |
the way from London. We have diligently kept our heads down. | :21:24. | :21:34. | |
:21:34. | :21:35. | ||
Three, two, one. Take a look. How is that? Beautiful. Amazing. There | :21:35. | :21:44. | |
is just so much to see. Just so many stars. It is overwhelming and | :21:44. | :21:53. | |
disorientating. Beautiful. This is the stone circle in the Cotswolds. | :21:53. | :21:58. | |
It is so dark here that we have to use a special light intensifying | :21:58. | :22:01. | |
camera that is thousands of times more sensitive than any normal | :22:01. | :22:09. | |
camera. Can I tell you away for just a moment? I know it looks | :22:09. | :22:13. | |
impressive. I know you want to make the most of it but we have got a | :22:13. | :22:19. | |
challenge for you. You have to work for this. If I use my laser pointer, | :22:19. | :22:25. | |
can you see the consolation of Pegasus? The winged horse. It is | :22:25. | :22:30. | |
the square that we are interested in. I am guessing that you can pick | :22:30. | :22:34. | |
out those stars back in London, just about. You challenge is to | :22:35. | :22:41. | |
count how many you can see within the Square of Pegasus. Really? | :22:41. | :22:45. | |
I can't normally count any inside it. So from London you can't see | :22:45. | :22:55. | |
:22:55. | :22:56. | ||
any? 1, two, three... 10. Nine. There leaven. I have got 12. | :22:56. | :23:02. | |
have 12. I have one that might be a discrepancy because it is on the | :23:02. | :23:09. | |
line. Borderline! Let's say that it is. You can see 12 stars within the | :23:09. | :23:13. | |
Square of Pegasus. That is a fantastic measure of how dark the | :23:13. | :23:19. | |
sky is. To see 12 is incredible. And zero in London. It makes you | :23:19. | :23:24. | |
realise the beauty of what you get. I have a treat for you. If we take | :23:24. | :23:33. | |
the top corner stark of the Square of Pegasus, -- corner star, and we | :23:33. | :23:37. | |
hop further to the North, there is one there and a faint one there. | :23:37. | :23:43. | |
You can make out that fuzzy blob just there. That is the Andromeda | :23:43. | :23:50. | |
galaxy. Mind-blowing, isn't it? Truly amazing. We have seen some | :23:50. | :23:53. | |
pretty incredible things are so far but the crowning glory, the thing I | :23:53. | :23:56. | |
am pretty sure you could not normally see from your houses in | :23:56. | :24:01. | |
London, is that overhead, running all the way from the horizon over | :24:01. | :24:10. | |
there. The Milky Way. Fantastic. That is actually the combined light | :24:10. | :24:15. | |
from all the stars in our galaxy. As you can see, there are thousands | :24:15. | :24:19. | |
and thousands of them. Even our specialist cameras are not | :24:19. | :24:24. | |
sensitive enough to pick up the Milky Way. But here it is in all | :24:24. | :24:33. | |
its glory. It was taken on a long exposure from exactly where we are | :24:33. | :24:38. | |
standing. It is incredible. takes a moment to take it all in. | :24:38. | :24:43. | |
So overwhelming. I have seen it in pictures. All this time, there it | :24:43. | :24:49. | |
is. I am awestruck because I have never seen so many stars in such | :24:49. | :24:57. | |
clarity. It is just awesome. It really is. My have just never seen | :24:57. | :25:03. | |
it before. -- I have just never seen it before. It goes to show | :25:03. | :25:10. | |
that the beauty of the night sky is taken from us by pollution. | :25:10. | :25:14. | |
It is incredible how much more you can see in the correct conditions. | :25:14. | :25:18. | |
Dark Sky Discovery is a network of groups that puts together of dark | :25:18. | :25:22. | |
areas in the country near you. don't have to be in the middle of | :25:22. | :25:28. | |
nowhere. We have some images of some of the areas. This one, for | :25:28. | :25:37. | |
example, is a science centre in Winchester in Hampshire. That | :25:38. | :25:41. | |
stunning picture was taken from there. Then we have this | :25:41. | :25:45. | |
observatory in Northumberland. Again a beautiful scene of the | :25:45. | :25:53. | |
North Star with the start trials rotating around it. -- star trails. | :25:53. | :26:00. | |
Actually we are the ones rotating. And this one near London. And now | :26:00. | :26:07. | |
this car-park on the Isle of Skye. The sun is very active at the | :26:07. | :26:13. | |
moment. If you are in the North of the UK, you can see quite a lot. | :26:13. | :26:21. | |
All of the information is on our website, as always. You will find | :26:21. | :26:30. | |
details of how to find an area of darkness. It just needs to be far | :26:30. | :26:33. | |
away from light pollution and with a clear horizon. Light pollution is | :26:33. | :26:37. | |
not just from office blocks. We are all guilty of it because even the | :26:37. | :26:42. | |
smallest communities create a lot of light. Tomorrow we are going to | :26:42. | :26:46. | |
ask a small town to switch off all of their lives simultaneously on | :26:46. | :26:51. | |
air. Here is the low-down on what we are trying to pull off. This | :26:51. | :26:54. | |
rural town may not be the kind of place you would associate with | :26:54. | :27:00. | |
light pollution. Only 1600 people live here and it is near to an area | :27:00. | :27:04. | |
of Exmoor which has the darkest skies in Britain. That is precisely | :27:04. | :27:09. | |
why we have chosen this town for the challenge. Even a town this | :27:09. | :27:14. | |
small generates a lot of excess light. As the sun sets, the lights | :27:14. | :27:19. | |
go up and a familiar orange glow descends on Dulverton. We should be | :27:19. | :27:23. | |
able to see the Milky Way from here, but like 90% of the UK, we can't. | :27:23. | :27:28. | |
We decided to give every single person the challenge of turning off | :27:28. | :27:32. | |
every single light. Last week we cent mark down there to help to | :27:32. | :27:42. | |
:27:42. | :27:43. | ||
make it happen. With 40 shops and cafes, three pubs, a sports ground | :27:43. | :27:48. | |
and all those houses, there was plenty to do. There are literally | :27:48. | :27:52. | |
thousands of lives here and it will take some serious powers of | :27:52. | :27:56. | |
persuasion to get everybody on board. There are also some | :27:56. | :28:00. | |
technical hurdles. As it turns out, most of the street lights are | :28:00. | :28:03. | |
controlled individually by automatic light sensors, so there | :28:03. | :28:07. | |
is no big button that we can use to turn them all off. This challenge | :28:07. | :28:11. | |
will not be easy but if it works, it will really bring this community | :28:11. | :28:17. | |
together. We might even get to see the night sky as nature intended. | :28:17. | :28:21. | |
The last couple of weeks, Mark has been trying to spread the word | :28:21. | :28:26. | |
among the inhabitants of Dulverton. How is that going? It has been a | :28:26. | :28:29. | |
challenge, I will say that, but the people in Dulverton seem to be | :28:29. | :28:35. | |
getting on board with it. I have had posters, fly is a letter boxes, | :28:35. | :28:43. | |
and even shops putting up special displays, including a space cake. - | :28:43. | :28:50. | |
- flyers in letterboxes. They probably think you are weird. What | :28:50. | :28:55. | |
is the chance of success? We have to rely on everybody. Not just the | :28:55. | :28:58. | |
council, the shops, but on everyone doing their thing. Until tomorrow | :28:58. | :29:04. | |
night, we just don't know. Mark will be going down to Somerset to | :29:04. | :29:09. | |
persuade the town before coming live from doll that in itself for | :29:09. | :29:13. | |
the big switch off tomorrow night. If you are from there, he is | :29:13. | :29:18. | |
legitimate! It is not just a massive burglary heist. Don't take | :29:18. | :29:24. | |
him out of town! Aside from the amazing array of planets, stars and | :29:24. | :29:29. | |
galaxies, occasionally things crop up that do not make sense. Look at | :29:29. | :29:34. | |
his picture. If you think it is a UFO, you should have already turned | :29:34. | :29:43. | |
over to Celebrity Big Brother! Having said that, why she is -- my | :29:43. | :29:48. | |
machine is not working. It is not too bad. Apart from the faeces that | :29:48. | :29:58. | |
the seagull is dropping behind him. That is the giveaway. UFOs | :29:58. | :30:03. | |
generally do not drop faeces. How come so many people are seeing | :30:03. | :30:13. | |
:30:13. | :30:15. | ||
There are some things that just seemed to belong in Hollywood movie. | :30:15. | :30:23. | |
And not on roads in Wiltshire. But this is a surprising statistic. One | :30:23. | :30:26. | |
in five people in Britain are convinced that aliens have visited | :30:26. | :30:36. | |
:30:36. | :30:43. | ||
In fact, the government took sightings of UFOs sufficiently | :30:43. | :30:48. | |
seriously that until 2009, the MoD had a department investigating them. | :30:48. | :30:53. | |
Over 11,000 cases were examined by MoD staff. David Clark has been | :30:53. | :30:59. | |
studying them, and he wins a prize for best job title of the show. | :30:59. | :31:05. | |
have got reports from police officers, coastguards, military air | :31:05. | :31:09. | |
crew. And some quite silly reports from people who have seen things | :31:09. | :31:15. | |
whilst leaving the pub and that kind of thing. A couple of sighting | :31:15. | :31:21. | |
stand out. In 1996, a strange light was spotted in the sky above | :31:21. | :31:26. | |
Skegness in Lincolnshire. It was made all the more credible by the | :31:26. | :31:29. | |
fact that the key witnesses in this case were police officers. In the | :31:30. | :31:34. | |
end, one of the police officers went on to the top of the police | :31:34. | :31:38. | |
headquarters in Boston and started making a film. The police alerted | :31:38. | :31:42. | |
the RAF, who saw an odd blip on their radar which stayed there for | :31:42. | :31:48. | |
hours. The UFO caused such a step, the newspapers had a field day. | :31:48. | :31:52. | |
Another strange case was that of Alex Bird, who took this photograph | :31:52. | :31:57. | |
in Sheffield. It was examined by intelligence officers, there was a | :31:57. | :32:01. | |
full report produced. Quite something for a 14-year-old lad in | :32:01. | :32:07. | |
the 1960s. By an eerie coincidence, Alex was privy to another UFO | :32:07. | :32:10. | |
sighting when he took this photograph, more than 40 years | :32:10. | :32:15. | |
later, of Retford Town Hall in Nottinghamshire. When he got home, | :32:15. | :32:19. | |
he was looking at the negatives and he could not believe it, on one of | :32:19. | :32:23. | |
the images, there is a classic flying saucer, by the side of the | :32:23. | :32:28. | |
town hall. It is clear that many perfectly normal members of the | :32:28. | :32:32. | |
public are spotting UFOs all over the place, but not everybody is | :32:32. | :32:35. | |
convinced they have everything -- anything to do with aliens visiting | :32:35. | :32:39. | |
Earth. There are many things we don't fully understand about the | :32:39. | :32:43. | |
atmosphere. Just because you don't know what something is, doesn't | :32:43. | :32:49. | |
mean it is a flying saucer, or an alien spacecraft. It may simply be | :32:49. | :32:54. | |
something we don't understand. to expect aliens to even reach | :32:54. | :33:01. | |
Earth is asking quite a lot. Most people have very little idea of the | :33:01. | :33:05. | |
enormous distances between the stars. We are talking like Cheers. | :33:05. | :33:10. | |
At our current rocket speed, it would take tens of thousands of | :33:10. | :33:16. | |
years for our own spacecraft to go outside of our solar system and | :33:16. | :33:19. | |
reach another star system. We have no reason to believe there would be | :33:19. | :33:27. | |
any other civilisation with many, many light years of Earth. If we | :33:28. | :33:37. | |
are not seeing aliens, what are we seeing? In the case of the Boston, | :33:37. | :33:41. | |
it is rather embarrassing. They consulted the Greenwich Observatory | :33:41. | :33:45. | |
and their opinion was from the directions and times, what the | :33:45. | :33:49. | |
police had not -- observed was the bright planet, Venus, which was | :33:49. | :33:53. | |
really prominent in the sky at the time. This is quite a common | :33:53. | :33:59. | |
mistake. Venus is known as the Queen of the LSO's -- de UFOs, | :33:59. | :34:06. | |
because it is often mistaken for something mysterious. It was | :34:06. | :34:11. | |
concluded that Alex Birch's UFOs were most likely ice crystals, and | :34:11. | :34:17. | |
the one in Red that was most likely caused by a more Strood drop it on | :34:17. | :34:21. | |
his camera lens -- Moorish Je drop it. Some are also as a result of | :34:21. | :34:28. | |
the latest military hide where. Their forces are often | :34:28. | :34:33. | |
experimenting with new technologies and they can be 10 or 20 years | :34:33. | :34:39. | |
ahead of what you see on the news. I favour it was this one by NASA, | :34:39. | :34:43. | |
launched in 1961 -- my favourite. It was a vast spherical metal | :34:43. | :34:50. | |
balloon which was launched into the upper atmosphere, used to bounce | :34:50. | :34:55. | |
communications from one part of the world to another. For decades, the | :34:55. | :34:58. | |
military have been flying exotic objects around the site, and they | :34:58. | :35:05. | |
are still doing it. By the 1980s, much of the US Air Force's | :35:05. | :35:09. | |
technological research was going into stealth aircraft, and the | :35:09. | :35:14. | |
enormous Stealth bomber. By the time the Stealth aircraft had been | :35:14. | :35:18. | |
publicly revealed, it is probably no coincidence that the general | :35:18. | :35:22. | |
trend in UFO sightings was moving away from the circular disc, | :35:22. | :35:29. | |
towards something that was more triangular in shape. And a lot of | :35:29. | :35:32. | |
UFO reports are down to people simply not knowing what is in the | :35:32. | :35:37. | |
night sky. Satellites for example. There is a group of satellites, | :35:37. | :35:41. | |
they are communication satellites in very high orbits. Most of the | :35:41. | :35:45. | |
time you don't see them but often - - every so often they catch the | :35:45. | :35:49. | |
light of the Sun for 10 or 15 seconds. Anyone looking at that, | :35:49. | :35:52. | |
seeing it get brighter, might think it is something coming straight | :35:52. | :35:57. | |
towards them, and then as it faded they might think it had turned | :35:57. | :36:00. | |
around and whizzed away, but it is the satellite going across the sky | :36:00. | :36:06. | |
and catching the light of the Sun for 10 or 15 seconds. Satellites, | :36:06. | :36:10. | |
water drops, planets, secret military planes, that is that | :36:10. | :36:16. | |
settled, then, hey? No matter how many cases you explain, people will | :36:16. | :36:20. | |
always be seen something new and asking for an explanation. I don't | :36:20. | :36:28. | |
think UFOs will ever really die. We may mention more about UFOs and | :36:28. | :36:32. | |
aliens tomorrow. An apology on behalf of my colleague, Celebrity | :36:32. | :36:36. | |
Big Brother does not start until nine. He is not the professor of | :36:36. | :36:40. | |
everything! Liz Bonnin got an amazing view of the closest port | :36:40. | :36:43. | |
galaxy to earth and now she has moved to a larger telescope to get | :36:44. | :36:47. | |
a more detailed look -- closest dwarf galaxy. | :36:47. | :36:52. | |
We are in the control room of SALT with ape Peter who we met last | :36:52. | :36:58. | |
night. -- with Petri Vaisanen. Tell us what that SALT image is there. | :36:58. | :37:02. | |
We were looking at this contracting colliding galaxy about 400 million | :37:02. | :37:06. | |
light years away. It is a major galaxy, smaller than the Milky Way | :37:06. | :37:10. | |
but bigger than the magellanic clouds. How do galaxies get that | :37:10. | :37:17. | |
big? They grow by accumulating smaller galaxies around them, | :37:17. | :37:20. | |
eating up other galaxies. The bigger the galaxy, the faster it | :37:20. | :37:24. | |
will grow. Little galaxies are coming up to bigger ones but bigger | :37:24. | :37:31. | |
ones interact and merge. This is of colliding galaxies? That is right. | :37:31. | :37:36. | |
They are two major galaxies, and a small reward in interaction and | :37:36. | :37:41. | |
basically a collision. -- smaller one. The individual stars did | :37:42. | :37:45. | |
actually collide, they are too far apart from each other, they are | :37:45. | :37:49. | |
very small -- don't actually collide. The gas and dusts collides | :37:49. | :37:53. | |
and when that compresses, new stars are born. The more violent the | :37:53. | :37:59. | |
interaction is, the more spectacular starburst you get. | :37:59. | :38:05. | |
is a beautiful image but you are interested in more? Yes, we take | :38:05. | :38:10. | |
spectra and from that a lot of the science comes. We can measure | :38:10. | :38:13. | |
masses and their star formation history is, and try to piece | :38:13. | :38:17. | |
together where they came from, where they went, how they changed. | :38:17. | :38:23. | |
Fascinating, thank you very much. Another SALT astronomer is Steve | :38:23. | :38:27. | |
Crawford. I believe the Milky Way is on a collision course with | :38:27. | :38:31. | |
Andromeda, is that right? That is true. They are expected to merge | :38:31. | :38:35. | |
together in about four and a half billion years. Not too soon, what | :38:35. | :38:42. | |
is going to happen? If we look at the simulation, we can see the two | :38:42. | :38:45. | |
spiral galaxies merging together for top they are literally going to | :38:45. | :38:50. | |
pass through each other? What is going to happen to our solar system | :38:50. | :38:57. | |
and Planet Earth? It depends on where in the Milky Way It -- where | :38:57. | :39:00. | |
in the solar system the Milky Way is, it could be floating out into | :39:00. | :39:07. | |
deep space. What will the resulting galaxy look like? They will form | :39:07. | :39:11. | |
together to make a new elliptical galaxy. What are we going to call | :39:11. | :39:19. | |
it? Milkdromeda? What do you reckon? I might go with Andromeda's | :39:19. | :39:24. | |
milkshake! It is a really good name! I don't think we have to | :39:24. | :39:28. | |
worry about it quite yet. Coming up tomorrow, or we are going to go | :39:28. | :39:33. | |
right across the plateau to check out this, it is called Superwasp, | :39:33. | :39:37. | |
super wide angle search for planets. It has found 75 exo planets and is | :39:37. | :39:41. | |
looking for more as we speak. I will be finding out how that works | :39:41. | :39:46. | |
tomorrow. See you then. Thank you. We will also find out | :39:46. | :39:52. | |
how our search for a planet has gone. Let's go back to see how Mark | :39:52. | :39:57. | |
and the observers are getting on. John has had a great time but he | :39:57. | :40:03. | |
has had to head back into the studio. The skies are still clear | :40:03. | :40:06. | |
for the second night running, which is remarkable. The guys have been | :40:06. | :40:10. | |
taking some beautiful images and joining me is Steve from the Mac | :40:10. | :40:16. | |
has filled astronomers society, he has taken a beautiful image -- the | :40:16. | :40:24. | |
Macclesfield. It is an assembly of 109 of the 110 Messier 83 objects | :40:24. | :40:29. | |
because one of them is never visible from my back garden. As the | :40:29. | :40:32. | |
seasons have rolled by, I have made a conscious effort to try to | :40:32. | :40:36. | |
capture the more obscure ones in a digital camera, attached to a | :40:36. | :40:41. | |
telescope. Whilst my sky conditions are orange and challenging, overall | :40:41. | :40:44. | |
I am plight -- quite pleased with the result. From the back garden, | :40:44. | :40:49. | |
it is incredible. Stay tuned for Back To Earth, where I have a guide | :40:49. | :40:54. | |
to find what -- to show what you can find in the night sky. But with | :40:54. | :41:04. | |
Thank you, the cleverness of the skies has been a real treat but | :41:04. | :41:09. | |
things are different tonight -- clear theirs. Thicker cloud has | :41:09. | :41:16. | |
spread in. ICloud dulling the sky in one or two spots, you will have | :41:16. | :41:22. | |
to get out quickly -- high cloud, dulling the sky. We are going to | :41:22. | :41:27. | |
see those cloud layers spread southwards and eastwards, bringing | :41:27. | :41:30. | |
mist and rain for the most part. By the end of the night, before the | :41:30. | :41:35. | |
sun gets up, you might get clear skies into the north-west of | :41:35. | :41:39. | |
Scotland. It is a case of getting out early if you can for tonight. | :41:40. | :41:43. | |
Tomorrow we split the country into two. Southern parts of England and | :41:43. | :41:47. | |
Wales, a lot of cloud with outbreaks of rain. North Wales, | :41:47. | :41:57. | |
:41:57. | :42:05. | ||
Midlands, East Anglia, you might One of the biggest questions is how | :42:05. | :42:09. | |
the Milky Way was formed. We asked Oxford University to do something | :42:09. | :42:13. | |
they have never done on this scale before, to run a computer | :42:13. | :42:16. | |
simulation to show how it started from the beginning of time from the | :42:16. | :42:21. | |
Big Bang, how our galaxy formed. Fiat to show us the result is Dr | :42:21. | :42:25. | |
Andrew Pontzen, this is not a simple task -- here to showers were | :42:25. | :42:31. | |
that it is not. We started with programming a computer with simple | :42:31. | :42:38. | |
physics. We then set up the computer with what we think the | :42:38. | :42:42. | |
universe look like near the big bang. So you say the basic laws and | :42:42. | :42:49. | |
you press go? That is basically it. So the earlier slide we can see in | :42:49. | :42:57. | |
years after the Big Bang. Yes, it had tiny ripples in it which we | :42:57. | :43:02. | |
think came from quantum processes at the start. This is the beginning | :43:02. | :43:12. | |
:43:12. | :43:13. | ||
Talk us through what we are seeing now. You are seeing the matter that | :43:13. | :43:16. | |
started out being quite uniformly spread out, it is starting to clump. | :43:17. | :43:20. | |
As well as the whole universe expanding, it is forming comes out | :43:20. | :43:26. | |
of what was originally quite smooth. What is the green? I have coloured | :43:26. | :43:29. | |
it green because it is dark matter so normally would not be able to | :43:29. | :43:35. | |
see it at all. But we can pick out anything in the virtual universe. | :43:35. | :43:40. | |
We have picked it out in green. have frozen 1.7 billion years after | :43:40. | :43:45. | |
the Big Bang. Dark matter, we should talk about that a bid. The | :43:45. | :43:50. | |
universe is dominated by staff that is not this. Yes, something like | :43:50. | :43:54. | |
four fifths of the stuff, we think, is not like the stuff that you and | :43:54. | :44:00. | |
I are made out of. We can infer its presence, we are fairly certain how | :44:00. | :44:04. | |
much there is. We can measure it through the cosmic microwave | :44:04. | :44:10. | |
background. What we are seeing is the visible matter. That is right. | :44:11. | :44:15. | |
We have switched and the faint blue stuff is gas, the white stuff is | :44:15. | :44:20. | |
stars. If he did not run this would be dark matter in the simulation, | :44:20. | :44:24. | |
would it work -- you did not? you would not see this. There would | :44:24. | :44:29. | |
not be a big enough gravitational pull. We need the dark matter to | :44:29. | :44:36. | |
create the galaxies. Yes. We can roll the clock on again. I think we | :44:36. | :44:40. | |
keep it frozen for a moment. We are zooming in. The blobs might have | :44:40. | :44:47. | |
looked like single stars, they are many galaxies, they have up to 100 | :44:47. | :44:53. | |
million stars in their -- meanie galaxies. We can see that all of | :44:53. | :44:58. | |
these are surrounded, we call them halos of dark matter. We have these | :44:58. | :45:06. | |
irregular shaped things that have already formed, the real matter is | :45:06. | :45:16. | |
:45:16. | :45:17. | ||
Yes, when we see what happens next, the dark matter controls it. The | :45:17. | :45:21. | |
little galaxies all merged together. What is notable about this process | :45:21. | :45:26. | |
is that it carries ongoing. It is not just that a few little galaxies | :45:26. | :45:31. | |
come together and that is a galaxy, it carries on happening. This is | :45:31. | :45:35. | |
the history of our galaxy through time. We started as a small clump, | :45:35. | :45:38. | |
then we mashed with other ones, spinning around to create larger | :45:38. | :45:48. | |
galleries. -- galaxies. Yes. And if we skip to the present day, we can | :45:48. | :45:51. | |
see enormous spiral galaxy and fly in to see what it looks like from | :45:51. | :45:59. | |
inside. This is a simulation of the creation of the universe. You have | :45:59. | :46:02. | |
put in some basic physics, basic data about the distribution of dark | :46:03. | :46:07. | |
matter and you have pressed go. You sit there and this galaxy emerges, | :46:07. | :46:11. | |
looking like the Milky Way. This is a picture of the real Milky Way, | :46:11. | :46:15. | |
and if we cross fade them, you can see how similar it is. It is a | :46:15. | :46:18. | |
testament to the power of what we know from basic physics that we can | :46:18. | :46:24. | |
do this. That is the simulated Milky Way and that is the real one. | :46:24. | :46:29. | |
Are we leaving anything out of this model? Yes, there are certainly | :46:29. | :46:32. | |
things that we do not fully understand at the moment. We have | :46:32. | :46:37. | |
black holes in there. We don't really understand fully what we are | :46:37. | :46:41. | |
doing with those black holes. are one of the big unknowns in the | :46:41. | :46:46. | |
galaxy formation. That is because nobody has ever seen one. How do we | :46:46. | :46:51. | |
know for sure that they definitely exist? | :46:51. | :46:54. | |
Ask any physicist about black holes and they will tell you that they | :46:54. | :47:04. | |
:47:04. | :47:04. | ||
exist. But I could say there is the Unicorn in these would lens, and | :47:04. | :47:09. | |
you would rightly say that there is not because you cannot see it. -- | :47:09. | :47:14. | |
this woodland. I could say that it is there but it is invisible and | :47:14. | :47:17. | |
you would probably think I was daft at best. But what is the difference | :47:17. | :47:22. | |
between my imaginary Unicorn and a black hole? But goals by definition | :47:22. | :47:28. | |
are invisible. You cannot see them so how do we know they exist? -- | :47:28. | :47:32. | |
black holes are by definition invisible. The first clue that | :47:32. | :47:36. | |
black holes are real came from here, in the Cambridgeshire countryside. | :47:36. | :47:42. | |
It was in the 1950s. While the rest of the country was this thing into | :47:42. | :47:46. | |
wireless radio at home, out here they were listing into a different | :47:46. | :47:56. | |
:47:56. | :47:57. | ||
radio signal. Radio signals from outer space. This is the mallard | :47:57. | :48:01. | |
Radio Observatory. Back in the 1950s some of the first radio | :48:01. | :48:05. | |
telescopes in the world were built here. When they turned them to the | :48:05. | :48:15. | |
:48:15. | :48:29. | ||
Nobody could work out what it was and what it was coming from. | :48:29. | :48:33. | |
Imagine that this thought is a beam of radio waves. Telescopes in the | :48:33. | :48:37. | |
1950s could detect radio sources in the sky. They could tell roughly | :48:37. | :48:41. | |
where the beams were coming from. Somewhere over there. But they | :48:41. | :48:46. | |
could not tell precisely. Then an of astronomer at the very clever | :48:46. | :48:53. | |
idea indeed. -- had a very clever idea indeed. He knew that on 25th | :48:53. | :48:58. | |
August, 1962, the Moon would be in the same patch of sky as the radio | :48:58. | :49:04. | |
source. So he watched and he waited and he saw that as the moon | :49:04. | :49:09. | |
travelled across the sky, it went in between the Earth and the radio | :49:09. | :49:15. | |
source, and carted off. Then as it continued its journey across the | :49:15. | :49:22. | |
sky, the radio source reappeared. By measuring precisely when the | :49:22. | :49:28. | |
been disappeared and appeared, the astronomer was able to pinpoint | :49:28. | :49:34. | |
precisely the source of the beam. It was tracked to what looked like | :49:34. | :49:38. | |
a faint star in the constellation Virgo. One tiny dots of light among | :49:38. | :49:44. | |
the millions of others in the sky. This is an image of that piece of | :49:44. | :49:51. | |
sky. That point of light just there is the source of the radio signal. | :49:51. | :49:55. | |
Pretty much every point of light that you can see in this image is a | :49:55. | :50:01. | |
star inside our galaxy, inside the Milky Way. But this point of light, | :50:01. | :50:07. | |
the origin of that radio signal, is 3 billion light years away. And yet | :50:07. | :50:15. | |
it can still be seen. No star could shine that brightly. So what could | :50:15. | :50:21. | |
that possibly be? The astronomers called it acquired the stellar | :50:21. | :50:31. | |
:50:31. | :50:33. | ||
object, quasar for short. -- Scientists could only think of one | :50:33. | :50:36. | |
way that stars could appear that bright, and that is if they were | :50:36. | :50:40. | |
falling into a black hole. Stars falling into a black hole would be | :50:40. | :50:43. | |
completely ripped apart. Gas and dust would be torn from their | :50:43. | :50:51. | |
services as they spiral inwards at tremendous speeds. They would in it | :50:51. | :50:54. | |
so much radiation that it could be seen right across the universe and | :50:54. | :50:59. | |
that would mean we could detect it on earth. -- they would emit | :50:59. | :51:02. | |
radiation. The astronomers in Cambridge realised that the quasar | :51:02. | :51:08. | |
that they were seeing was actually a black hole, a giant black hole, | :51:08. | :51:15. | |
and the light and radio waves were coming from entire stars having | :51:15. | :51:17. | |
light and dust ripped off them and spiralling to destruction inside | :51:17. | :51:25. | |
the black hole. Over 100,000 quasars have now been discovered. | :51:25. | :51:30. | |
All are thought to be super massive black holes, actively feeding on | :51:30. | :51:35. | |
stars. And all of them are found in exactly the same place, right in | :51:35. | :51:40. | |
the centre of galaxies. So does that mean there is a black hole at | :51:40. | :51:45. | |
the centre of every galaxy? Our galaxy, the Milky Way, could not | :51:45. | :51:49. | |
have a quasar like the one discovered in Cambridge because we | :51:49. | :51:54. | |
would see it. It would shine as brightly as the full moon, visible | :51:54. | :51:59. | |
in the daytime. But imagine a black hole that had eaten all the nearby | :51:59. | :52:03. | |
star systems, so there is no gas and dust to spiral own and no | :52:03. | :52:09. | |
radiation to make it bright. So it could still be that there is a | :52:09. | :52:18. | |
super massive black hole at the heart of the Milky Way. One group | :52:18. | :52:22. | |
of scientists spent 16 years painstakingly searching for it. | :52:22. | :52:28. | |
This is what they found. I think this is one of the most remarkable | :52:28. | :52:32. | |
graphics in recent scientific history. It is a picture of the | :52:32. | :52:38. | |
centre of our galaxy and the stars that orbit around it. In a two | :52:38. | :52:42. | |
stars that you can see are orbiting very fast around some central | :52:42. | :52:50. | |
object. They reach speeds of around 11 million mph. When you plot the | :52:50. | :52:54. | |
orbits out precisely, you can calculate the mass of the object | :52:54. | :52:59. | |
that they are orbiting around. It turns out that the mass of that | :52:59. | :53:03. | |
object is 4 million times the mass of the sun. But it is more than | :53:03. | :53:08. | |
that, because you can also work out the maximum size that it can be. In | :53:08. | :53:16. | |
a star get close to that central object, as close as Neptune gets to | :53:16. | :53:21. | |
the sun. We have an object 4 million times the mass of our son, | :53:21. | :53:27. | |
compressed into a space smaller than our solar system. And it is | :53:27. | :53:32. | |
invisible. The only thing that could be is a black hole. The | :53:32. | :53:38. | |
centre of our galaxy. Black holes started out in the imagination of | :53:38. | :53:42. | |
physicists. But we now have evidence to prove that they are | :53:42. | :53:47. | |
real. Not only do black holes exist, but we now suspect that they formed | :53:47. | :53:55. | |
the heart of nearly every galaxy in the universe. Including arrow. -- | :53:55. | :53:59. | |
including our own. Someone up there we know there is a super massive | :53:59. | :54:02. | |
black hole at the centre of our galaxy and the solar system is | :54:02. | :54:06. | |
orbiting around it. Why do we orbit around a black hole? We need to | :54:06. | :54:12. | |
explain how gravity works. This is the theory of relativity and it | :54:12. | :54:17. | |
showed us this. It was the interaction of a planet and how we | :54:17. | :54:21. | |
twisted the space around it. This is traditionally shown by | :54:21. | :54:25. | |
physicists by using spandex. wondered where my trousers had | :54:25. | :54:30. | |
gone! It is a large mass and it twists the space around it. | :54:30. | :54:34. | |
Something going past it is sent off course. Einstein said that things | :54:34. | :54:38. | |
follow a straight line through space and time. Mass is curved | :54:38. | :54:42. | |
space and time, so if you do not know that the space and time is | :54:42. | :54:45. | |
curved and you are travelling through it, then it will look to | :54:45. | :54:49. | |
you that you have curved around the mass. If you enter the density at | :54:49. | :54:52. | |
the right speed, you will be spinning round and round, and that | :54:52. | :54:57. | |
is what an orbit is. You can think of Einstein's gravity as a | :54:57. | :55:05. | |
fictitious force, at the space and time be incurred by massive -- be | :55:05. | :55:11. | |
incurred by massive objects. This is the curve that you get from a | :55:11. | :55:16. | |
black hole. The black hole curves the space so far, that when | :55:16. | :55:20. | |
something approaches bit... This could be a photon, a particle of | :55:20. | :55:24. | |
light. What happens in a black hole is that the photon approaches and | :55:24. | :55:28. | |
it cannot escape when it crosses the boundary, which is called the | :55:28. | :55:33. | |
event horizon. Eyes and's theory predicts that if you get close to | :55:33. | :55:37. | |
the centre of the black hole, which is caused the singularity, | :55:37. | :55:41. | |
infinitely dense, infinitely small, space and time are infinitely | :55:41. | :55:45. | |
curved, and the theory itself breaks down. This is probably the | :55:45. | :55:48. | |
most fascinating thing about black holes on the physicist's | :55:48. | :55:53. | |
perspective. The best theory we have, the theory of relativity, | :55:53. | :55:59. | |
predicts its own demise somewhere down there. Spandex cannot read as | :55:59. | :56:05. | |
much as space can, of course. -- cannot stretch. There is literally | :56:05. | :56:14. | |
no way out for anything. Yes. Tim O'Brien, associate director here, | :56:14. | :56:18. | |
has been telling us that that holes a one of the specialist subjects | :56:19. | :56:28. | |
here. -- black holes of one of the specialist subjects. Yes. This is | :56:28. | :56:35. | |
the Hubble telescope. And some other telescopes. This is a radio | :56:35. | :56:39. | |
image of the sky. We can see through the dust cloud that block | :56:39. | :56:42. | |
our view of the centre of the galaxy. In the middle, that is | :56:42. | :56:52. | |
Sagittarius, the black hole. This is new research, essentially. | :56:52. | :56:58. | |
just last week. The quasar is in the middle and this is the optical | :56:58. | :57:02. | |
view, the black dot in the middle. We can zoom in and look at the | :57:02. | :57:07. | |
radio image. Where the black hole is the bright spot in the middle. | :57:07. | :57:11. | |
The thing that shoots off to the left is a jet of particles we think | :57:11. | :57:17. | |
out from the black hole, almost at the speed of light. -- rushing out | :57:17. | :57:21. | |
from the black hole. The shape of it is like a corkscrew. It is | :57:21. | :57:25. | |
spinning like that. One way in which that might happen would be if | :57:25. | :57:31. | |
this were the result of a merger between two galaxies. When the | :57:31. | :57:35. | |
galaxies merge, the two black holes end up whipping around each other | :57:35. | :57:40. | |
and that causes this. Do they fall into each other over time? Yes. | :57:40. | :57:45. | |
They will. They spiral closer together. They create ripples in | :57:45. | :57:49. | |
space and time, predicted by Einstein. Not yet directly detected | :57:49. | :57:53. | |
but we are working on that with this telescope across Europe. | :57:53. | :57:58. | |
of the most remarkable things about these images, these experiments, is | :57:58. | :58:02. | |
that we are trying to look for a breakdown in relativity. The | :58:02. | :58:06. | |
breakdown in Einstein's theory. For me this is what science is all | :58:06. | :58:11. | |
about. We are trying to test our theory to destruction. We have | :58:11. | :58:16. | |
discussed this for a long time. The show carries on for another half an | :58:16. | :58:21. | |
hour in this very room and you can ask more questions. We need help to | :58:21. | :58:26. | |
fight our own exo-planet. 60,000 of you have taken part so far and the | :58:26. | :58:31. | |
more of you that take part, the more likely it is that we will find | :58:31. | :58:40. | |
one. You can download your star guide from the website. We are | :58:40. | :58:43. | |
going off and now here but we are coming back on in 10 seconds to go | :58:43. | :58:50. | |
and sit over there. -- going off- air. We will be talking about black | :58:50. | :58:55. | |
holes and you can send in your questions for us to answer. Jon | :58:55. | :59:00. |