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Last night we looked at the supermassive black hole at the | :00:09. | :00:12. | |
centre of our galaxy, tonight we are hunting aliens. | :00:12. | :00:17. | |
We will be revealing, and how incredible is this, how you at home | :00:17. | :00:21. | |
helped us to discover a brand new planet. | :00:21. | :00:24. | |
I'm Brian Cox and this is Dara O'Briain, and this is Stargazing | :00:24. | :00:34. | |
:00:34. | :00:54. | ||
Welcome back to the control room here in Jodrell Bank Observatory | :00:54. | :00:58. | |
for the third and final night of this year's Stargazing live, we are | :00:58. | :01:01. | |
going to be tackling perhaps the biggest question in all of science, | :01:01. | :01:05. | |
are we alone in the universe? are living in a revolutionary | :01:05. | :01:09. | |
period in a search for life beyond earth, we are now able to find | :01:09. | :01:13. | |
planets billions of miles outside our Solar System. They are called | :01:13. | :01:19. | |
exo-planets, so far we have found over 700 of them. Last month | :01:19. | :01:23. | |
scientists announced the discovery of Kepler 22b. A planet quite close, | :01:23. | :01:27. | |
about ten light years away, it is thought to be the closest one we | :01:27. | :01:32. | |
have come across beyond our Solar System. This is an artist | :01:32. | :01:38. | |
impression. It is earth-like with an atmosphere. That is because it | :01:38. | :01:42. | |
probably is earth-like at moss stpeers and could be a strong | :01:42. | :01:47. | |
candidate -- atmosphere, and could be a strong candidate for life. | :01:47. | :01:53. | |
can actually listen to Kepler 22b. Are we there with the co-ordinates, | :01:53. | :02:01. | |
I have to hit "return ", are you sure, there is a genuine note of | :02:01. | :02:06. | |
peril. Bingo, a monkey can do that. That will turn to face directly to | :02:06. | :02:10. | |
Kepler 22b. Later, as it has turned around, we can listen to it. We | :02:10. | :02:13. | |
will tell you about the planet at home you have found. | :02:14. | :02:19. | |
Last night we looked at light pollution, all the artificial light | :02:19. | :02:24. | |
that obscures the stars in the night sky. To tell you the light a | :02:24. | :02:27. | |
smallest place can create, we asked landmarks across the country to | :02:27. | :02:32. | |
turn their lights out. We tried to convince an entire town to switch | :02:32. | :02:37. | |
their lights off live on aifrplt standing by in Dulverton is Mark, - | :02:37. | :02:42. | |
- live on air. Standing by in Dulverton is Mark. What is | :02:42. | :02:46. | |
happening? It is wet here in Dulverton, the | :02:47. | :02:50. | |
atmosphere is electric. It is a small town. I'm here on the high | :02:50. | :02:57. | |
street of Dulverton, a small town with 1600 inhabitant, 800 houses, | :02:57. | :03:01. | |
50 shops, bars and restaurants. We have tried to spread the word to | :03:01. | :03:04. | |
get people to think about their lighting. | :03:04. | :03:06. | |
The weather doesn't look particularly good, does that mean | :03:07. | :03:12. | |
if the lights are out you won't suddenly see the Milky Way in all | :03:12. | :03:18. | |
its glory, you won't see a great show overhead? Not amazing in stars, | :03:18. | :03:22. | |
the clouds are looking stunning. Over the past few weeks we have had | :03:22. | :03:26. | |
teams working in Dulverton to spread the word. In 20 minutes time, | :03:26. | :03:30. | |
when the bells ring, we will find out how successful that message has | :03:30. | :03:38. | |
spread. As this film shows, the message or task was not an easy one. | :03:38. | :03:45. | |
Dulverton has 720 houses, 177 street lights, 40 shops and cafes, | :03:45. | :03:49. | |
three schools, three pubs, and a sports ground. That is a lot of | :03:49. | :03:54. | |
lights. If this is going to work, we will need to get the whole town | :03:54. | :03:58. | |
on board. First things first, we had to meet with the mayor. What do | :03:58. | :04:01. | |
you think will be the biggest challenge for us? Getting out the | :04:01. | :04:05. | |
word to everybody that they should do what we want them to do that is | :04:05. | :04:10. | |
to make the big switch off, the biggest we could ever make. | :04:10. | :04:14. | |
knocked on hundreds of doors, dropped leaflets through | :04:14. | :04:20. | |
letterboxes and spoke to as many residents as we could find. Can you | :04:20. | :04:27. | |
turn that off for us? Hello, what lights do you normally | :04:27. | :04:31. | |
have on? Maybe the upstairs light. Most of the lights, yeah. | :04:31. | :04:36. | |
Thank you very much indeed for your support. Thank you too. | :04:36. | :04:38. | |
I'm exhausted, I have been delivering leaflets all day, but | :04:38. | :04:42. | |
the response, I think, has been pretty positive. I just hope they | :04:42. | :04:47. | |
weren't telling me that to get me off their doorsteps. Dulverton is | :04:47. | :04:51. | |
part of Exmoor National Park, with some of the darkest skies in the UK. | :04:51. | :04:56. | |
Even this relatively small town generates enough life to obliterate | :04:56. | :05:00. | |
the skies with a fuzzy orange glow. Light pollution doesn't just reduce | :05:00. | :05:03. | |
the visibility of stars, light that shines where it isn't needed is a | :05:03. | :05:08. | |
waste of energy and money. We have chosen Dulverton as our switch-off | :05:08. | :05:11. | |
challenge, but there are thousands of towns and cities all over the | :05:11. | :05:15. | |
country that could benefit from a little less light. | :05:15. | :05:19. | |
Only a few days to go. This morning, one of schools in Dulverton has | :05:19. | :05:24. | |
allowed me to take the school assembly. I'm a bit nervous, I have | :05:24. | :05:28. | |
not done that since I was in school. If I can get the kids on board, I | :05:28. | :05:33. | |
can get the parents on board. What we need you all to do is go home | :05:33. | :05:36. | |
tonight, when you finish school, get all of your parents to turn off | :05:36. | :05:42. | |
all the lights in your house. Are you going to help us? Yeah! | :05:42. | :05:45. | |
What we need now is some kind of signal to make sure that all the | :05:45. | :05:50. | |
lights are switched off at exactly the same time. I have arranged a | :05:50. | :05:55. | |
meeting with the church bell ringers. Will everyone in Dulverton | :05:55. | :05:58. | |
hear the signal? If the wind is in the east they will hear it, if it | :05:58. | :06:01. | |
is in the west they won't. If the wind is blowing in the wrong | :06:01. | :06:06. | |
direction no-one will hear it? Crikey, this might work and it | :06:07. | :06:12. | |
might not. Now I have to see man about street lights. The majority | :06:12. | :06:15. | |
of the lights will have to be visited individually. We can't push | :06:15. | :06:21. | |
a red button and they all go off? Perhaps 20 years ago, but not now. | :06:21. | :06:27. | |
It is a big job k we do it? Yes. have visited businesses and | :06:27. | :06:30. | |
thousands, we have spoken to the local mayor, the police are | :06:30. | :06:33. | |
shutting off roads for us, posters around the town, I don't know if | :06:33. | :06:43. | |
:06:43. | :06:44. | ||
this will work f it does, it will As you can see, the residents have | :06:44. | :06:49. | |
turned out in their hundreds to support this, including some hardy | :06:49. | :06:52. | |
astronomers, we have done everything we can do. In 15 minutes, | :06:52. | :06:56. | |
when the bells cliem chime, we will be entirely in the hands of the | :06:56. | :07:00. | |
good people of Dulverton. The weather isn't looking great, we | :07:00. | :07:03. | |
will persevere, getting those lights off will be an achievement | :07:03. | :07:08. | |
in itself. We will be back shortly This is turning around in its own | :07:08. | :07:12. | |
stately well. We gave the wrong information earlier. | :07:13. | :07:21. | |
Kepler 22b, is still relatively close, 600 million light years away. | :07:21. | :07:26. | |
You have sent us in stunners from home. | :07:26. | :07:30. | |
This is a photograph of a star I know well, because we talked about | :07:30. | :07:35. | |
it on Wonders of the Universe. There it is. | :07:35. | :07:43. | |
It is star called, this is the Triang ulumGalaxy, I wasn't going | :07:43. | :07:53. | |
:07:53. | :07:53. | ||
to talk about that. But it is nice. This is the Rising Sun, and finally, | :07:53. | :07:59. | |
I think this is particularly nice, it was taken by Steve, one of the | :07:59. | :08:03. | |
astronomers we had out in the dark, muddy field over there on Monday | :08:03. | :08:07. | |
night. We do need you to keep them coming in, you will find details of | :08:07. | :08:14. | |
how to get them on the website -- to get them to us on the website. I | :08:14. | :08:20. | |
had a viewer asking for the website address. I have no idea. It is | :08:20. | :08:25. | |
below. I can't bear to read it out, I have read it out so many times. | :08:25. | :08:30. | |
You can join in on the live talk, Dr Lucie Green is standing by to | :08:31. | :08:36. | |
answer all guess, and on Stargazing Back To Earth following the | :08:36. | :08:38. | |
programme. We have questions for Brian too. We will get to the | :08:38. | :08:41. | |
questions for Brian later on. If you have a question, | :08:41. | :08:43. | |
particularly if there is anything you want to know about planets or | :08:43. | :08:49. | |
the search for life, you can get them to us by e-mailing the address | :08:49. | :08:58. | |
below, or the Twitter address. wanted you to say it! | :08:58. | :09:01. | |
Although we are spending a lot of time looking for life and exo- | :09:01. | :09:05. | |
planet, the best chance of finding life in the Solar System comes not | :09:05. | :09:07. | |
from the planet, but probably the moons. | :09:07. | :09:11. | |
We have probes all across the Solar System, the majority of the planets | :09:12. | :09:16. | |
we have probes, what are the best bets for finding them? This is a | :09:16. | :09:20. | |
picture of probably what most people think is the strongest | :09:20. | :09:25. | |
candidateor life beyond earth, this is Jupiter's moon, Europa, this was | :09:25. | :09:31. | |
taken by the Galileo Probe, it crashed into Jupiter. One of the | :09:31. | :09:35. | |
reasons it did that was to avoid Europa. It is thought it is just | :09:35. | :09:39. | |
possible we could have contaminated it if we crashed the probe in it. | :09:39. | :09:43. | |
Rather than landing the probe it was ditched? Yeah, into Jupiter. | :09:43. | :09:48. | |
The reason we are very excited by Europa, is it almost certainly has | :09:48. | :09:53. | |
an ocean of liquid water beneath the icey surface, there is probably | :09:53. | :09:57. | |
more water in the oceans of Europa, than in all the oceans of earth | :09:57. | :10:03. | |
combined. It is a fascinating world. The problem is the ice is probably | :10:03. | :10:09. | |
about 100kms thick, it would take a big drill to get through. It is a | :10:09. | :10:14. | |
target for exploration. The reason we know, this is a close-up of the | :10:14. | :10:19. | |
surface, you can see the cracks, they are very reminiscent of the | :10:19. | :10:25. | |
cracks in sea ice, when you model that, it indeed seems there are | :10:25. | :10:30. | |
cracks constantly shifting, because this ice is floating on an ocean of | :10:30. | :10:36. | |
lifting water. There is another of Jupiter's moons, Al-Ganzouri, we we | :10:36. | :10:41. | |
mentioned, -- Ganymede, it is also candidate. It has if not an ocean, | :10:41. | :10:45. | |
then liquid water beneath the surface. We think it probably looks | :10:45. | :10:49. | |
like this, this is the cross section of Ganymede, there is icey | :10:49. | :10:52. | |
sludge there. NASA are going to Mars later in the | :10:52. | :10:59. | |
year with the new Curiosity Rover, following the water and following | :10:59. | :11:04. | |
the complex carbon molecules in organic chepls treatment that will | :11:04. | :11:09. | |
specifically land in places where they need -- chemistry, that will | :11:09. | :11:16. | |
specifically land in places where there are water. You find mineral | :11:16. | :11:25. | |
deposits, this is from the Opportunity Rover, g ipsumhas been | :11:25. | :11:29. | |
found in Mars, it is only found in the presence of standing water, it | :11:29. | :11:33. | |
is probably the same on Mars, we know there was water there once. | :11:33. | :11:37. | |
That is from Mars, we will receive information next year, if we're | :11:37. | :11:43. | |
back next year we will show you the news from Mars. | :11:43. | :11:53. | |
:11:53. | :11:55. | ||
Over to Liz. Welcome back to the South African | :11:55. | :11:59. | |
astronomical observatory. We are at the one metre telescope, British- | :11:59. | :12:04. | |
built in Newcastle. Normally this telescope looks at objects far | :12:04. | :12:08. | |
beyond our Solar System, take a look at this image it has taken of | :12:08. | :12:13. | |
Saturn, 900 million miles away from us. Neptune is our outer most | :12:14. | :12:18. | |
planet in the Solar System, another two billion miles outside Saturn. | :12:18. | :12:22. | |
That is not where the Solar System ends, in fact, we have still a lot | :12:22. | :12:32. | |
:12:32. | :12:36. | ||
to learn about this very mysterious The Karoo desert might look more | :12:36. | :12:40. | |
like an alien landscape than in Britain, but this place is still | :12:40. | :12:47. | |
unmistakically part of our home, planet earth. Fertile soils, the | :12:47. | :12:51. | |
warmth from our sun, a great diversity of living things. It is | :12:51. | :12:56. | |
all down to our unique position in the Solar System. Where the third | :12:56. | :13:01. | |
rock from the sun, not too hot, not too cold, just right for life to | :13:01. | :13:05. | |
flourish. Of course, we are just one of a | :13:05. | :13:15. | |
:13:15. | :13:19. | ||
family of planets. If my rucksack is the sun, we have rocky planets | :13:19. | :13:27. | |
first, Mercury, Venus, our own planet earth and Mars, then the gas | :13:27. | :13:33. | |
giants, Jupiter and Saturn, Uranus, Neptune and Pluto. Which has been | :13:33. | :13:37. | |
reclassified as a dwarf planet, it is no longer a planet. Then what | :13:37. | :13:42. | |
happens? What lies beyond our eight planets? And where does our Solar | :13:42. | :13:49. | |
System actually end? Amanda is an astronomer working here in South | :13:49. | :13:54. | |
Africa, she specialises in the distant objects that inhabit the | :13:54. | :13:57. | |
remotist regions of our Solar System. | :13:57. | :14:01. | |
If this is Neptune, what is going on between it and the nearest star, | :14:01. | :14:06. | |
over the horizon if it is four light years away or more, is it all | :14:06. | :14:10. | |
empty space? It is hardly empty space, we have discovered a lot of | :14:10. | :14:17. | |
objects out there, rocky objects, they are called the Kuiper Belt. | :14:17. | :14:22. | |
There are 70,000 out there we think. That sounds like a lot of objects | :14:22. | :14:27. | |
swimming around in the area. 70,000 are the biggest ones, if you go | :14:27. | :14:33. | |
down to the smaller ones we think it is billions. How wide is it? | :14:33. | :14:38. | |
you think of how far Neptune is from the sun, the classic Kuiper | :14:38. | :14:44. | |
Belt is that far from Neptune. is wide, does that mean Pluto is | :14:44. | :14:48. | |
officially a Kuiper Belt object? is in that Kuiper Belt, it was one | :14:48. | :14:52. | |
of the first objects to be discovered. If we have gone that | :14:52. | :14:56. | |
distance from the sun to newspaper tune again, that is the Kuiper Belt, | :14:56. | :14:59. | |
here it is at the edge of the Kuiper Belt, what happens here, is | :14:59. | :15:03. | |
this the edge of our Solar System? Not yet, we still have objects that | :15:03. | :15:08. | |
were discovered out here that have objected that go -- orbited that go | :15:08. | :15:13. | |
beyond the Kuiper Belt, we call them the scattered disc. How many | :15:13. | :15:17. | |
objects exist there? Maybe hundreds, a few very well known, though. | :15:17. | :15:23. | |
There is one called Aris, it is about three-times as far away from | :15:23. | :15:28. | |
the sun as Neptune is now. What does it look like? We have images | :15:28. | :15:33. | |
from the Hubble Space Telescope. is a bit blury? From the image you | :15:33. | :15:36. | |
are seeing reflected light, there are severe limitations to doing | :15:36. | :15:40. | |
that kind of imaging. That is the furthest object we have seen with | :15:40. | :15:44. | |
the telescope. When you get to the edge of the scattered disc, surely | :15:44. | :15:48. | |
that is the edge of the Solar System? No, there is more. Beyond | :15:48. | :15:53. | |
that is a structure that we have they areised called the Oort Cloud, | :15:53. | :16:03. | |
hundreds of thousands of objects srpbd the Solar System, two light | :16:03. | :16:07. | |
years away. Is that the end of the Solar System? If you want to call | :16:07. | :16:11. | |
it that, that is as far as we know, as far as the sun's gravitational | :16:11. | :16:15. | |
influence he can tends. I would say it is pretty much the end of the | :16:15. | :16:19. | |
Solar System. How do we know what this Oort Cloud | :16:19. | :16:25. | |
looks like if it is hypothetical? We have observational evidence in | :16:25. | :16:31. | |
the form of comets, they come from all different directions, when we | :16:31. | :16:36. | |
trace their orbits they come from far away, distant parts of the | :16:36. | :16:40. | |
Solar System. Do all comets come from the Oort Cloud? No, we had a | :16:41. | :16:50. | |
:16:51. | :16:51. | ||
comet visible from here, Comet Love Joy, take a photograph here of by | :16:51. | :16:56. | |
one of the IT guys. Your expertise is the Kuiper Belt and the | :16:56. | :16:59. | |
scattered disc, you say it is difficult to get information from | :16:59. | :17:04. | |
the images of the objects, how do you study them further? We have to | :17:05. | :17:13. | |
be creative, we have the stellar augmentation. We look at the | :17:13. | :17:16. | |
objects passing across the scattered discs, and the shadow, we | :17:16. | :17:20. | |
learn about the size, properties for the atmosphere, how the | :17:20. | :17:24. | |
atmosphere might be changing, we combine that with things we know | :17:24. | :17:29. | |
and get the density. It is easy to know where the shadows are cast on | :17:29. | :17:33. | |
the planet? It is really hard, we spend a lot of time measuring. A | :17:33. | :17:36. | |
shadow Pat can come across Sutherland and we can be lucky, | :17:36. | :17:40. | |
there is a lot of telescopes, sometimes not, then it gets | :17:40. | :17:44. | |
exciting. Last year I rented a pick-up truck in Cape Town and | :17:45. | :17:50. | |
putting a 12-portable telescope in the back, and one of our | :17:50. | :17:57. | |
instruments built for the purpose, we crossed the border in Namibia, | :17:57. | :18:02. | |
and put all this equipment out, and looking over our shoulder all the | :18:02. | :18:07. | |
time for animals. You were tracking an interesting object? It was a | :18:07. | :18:11. | |
large Kuiper Belt object, it was a strange result, it suggests the | :18:11. | :18:15. | |
object is really elongateed, that is not what we would have expected. | :18:15. | :18:24. | |
Come back to us later, I will be finding out about superWASP-. | :18:24. | :18:29. | |
Discussion as it,were the edge of the solar -- discussing as they | :18:29. | :18:34. | |
were the edge of the Solar System, which Voyager is heading there now? | :18:34. | :18:40. | |
It is one of the great stories in space exploration, launched in 1977, | :18:40. | :18:44. | |
Voyager 1 and 2. They were launched to do the grand tour of the Solar | :18:44. | :18:49. | |
System. At that time you launched a spacecraft, you could visit Jupiter, | :18:49. | :18:52. | |
Saturn, Uranus and Neptune in one mission. It happens very rarely. | :18:53. | :18:58. | |
Off they went, ambitious spacecraft. I remember talking to one of the | :18:58. | :19:02. | |
designers, they were designed to last two or three years, four years. | :19:02. | :19:05. | |
It was expensive saying this spacecraft will last for 20 year, | :19:05. | :19:09. | |
you have to build it like a tank. I have a picture of it there. It is | :19:09. | :19:14. | |
about the size of a bus, or a car. It is a tiny little thing. At the | :19:14. | :19:22. | |
moment Voyager 1, the most distant man made object. It is 17 million | :19:22. | :19:28. | |
kms away -- 17 million kilometres away, 14 times the distance from | :19:28. | :19:32. | |
the earth to the sun. It is powered by a little battery and can be | :19:32. | :19:38. | |
detected now. What the Voyager 1 has done and II, is the place where | :19:38. | :19:42. | |
the wind from the sun meets the wind from interstellar space, they | :19:42. | :19:46. | |
are measuring that, the instruments are still working, and they send | :19:46. | :19:50. | |
the data back. The coolist thing is they do it on a tape. Most of our | :19:50. | :19:54. | |
viewers under the age of 20 won't know what a tape is. It is a piece | :19:54. | :19:59. | |
of magnetic brown stuff used to record Top Of The Pops on. It | :19:59. | :20:05. | |
records the data, every so often it gets its transmitters point it at a | :20:05. | :20:08. | |
telescope and sends the information back. NASA are saying they are | :20:08. | :20:13. | |
turning off some of the parts of it now to conserve energy, they think | :20:13. | :20:18. | |
they can keep it going until 2025? The heat has been turned off, it is | :20:18. | :20:22. | |
one of the coldest working things we have built, it is sending | :20:22. | :20:27. | |
information and should keep working until 2025. That is a brilliant | :20:27. | :20:34. | |
example of the things we can do when we put our minds to it. Before | :20:34. | :20:38. | |
we go back to Dulverton have a look at this? This is Britain on a clear | :20:38. | :20:43. | |
night from space. You can see the major cities, London, Birmingham, | :20:43. | :20:52. | |
Manchester, Edinburgh, Newcastle. It is a mess, basically. 60% of us | :20:52. | :20:56. | |
live in a severely light polluted area, it plays havoc with | :20:56. | :20:59. | |
stargazing, it is not difficult to reduce. Several iconic buildings | :20:59. | :21:06. | |
have been leading the way for us. This is Worcester Cathedral, they | :21:06. | :21:11. | |
switched off. Here is Bristol's Clifton Suspension Bridge. | :21:11. | :21:14. | |
Even down in Cornwall, the Eden Project, they have been dimming | :21:14. | :21:19. | |
their lights for us in order to get a clear view of the sky. We have | :21:19. | :21:24. | |
the tower in Portsmouth. There it goes. | :21:24. | :21:29. | |
This is BBC Media City in Salford, witching off its lights. | :21:29. | :21:35. | |
We want to see just -- switching off its lights. We want to see the | :21:35. | :21:38. | |
big difference switching off lights can make, even in a small town. It | :21:39. | :21:44. | |
is time for Dulverton to switch off. This is it, after months of | :21:44. | :21:48. | |
planning, the bells are going to ring very soon, and hopefully it | :21:48. | :21:52. | |
will be very dark. We need everyone in Dulverton to turn their lights | :21:52. | :21:57. | |
off as soon as you hear the bells ringing. I will invite my posse to | :21:57. | :22:02. | |
help with the countdown. I was going to say, are you ready | :22:02. | :22:06. | |
for this, Dulverton? I think you are. | :22:06. | :22:11. | |
(cheering) We are now going to start the countdown. | :22:11. | :22:21. | |
:22:21. | :22:22. | ||
5-4-3-2-1. (bells ringing) This is the moment | :22:22. | :22:30. | |
where the bells should start ringing, instead, I want you all to | :22:30. | :22:39. | |
shout "ding dong". We can hear the bells, we can see | :22:39. | :22:47. | |
the lights going out. Except for the place beside you. So far the | :22:47. | :22:52. | |
lights in the street has have all gone out. It is really eerie. It is | :22:52. | :22:58. | |
bizarre. Look at that. It is a shame that you can't see the sky. | :22:58. | :23:05. | |
There it is. This is amazing, I can barely see the camera in front of | :23:05. | :23:09. | |
me, it has got so dark. We can't see the sky. What I would say, | :23:09. | :23:13. | |
eventhough it is cloudy, the sky has leapt out above our heads. We | :23:13. | :23:16. | |
have special night vision cameras, because there is no light around. | :23:16. | :23:20. | |
It looks incredible. But it is going to take a while for our eyes | :23:20. | :23:26. | |
to adapt to the darkness, come back in a few moments and see how we are | :23:26. | :23:29. | |
getting on. It is a wonderful moment that, it is easy to treat it | :23:29. | :23:34. | |
as a bit of a stunt, it is cloudy so you don't see the stars come out. | :23:34. | :23:37. | |
There is a genuine point about losing contact with the night sky. | :23:37. | :23:41. | |
If you think back to the time, you heard how old you are, you can't | :23:41. | :23:45. | |
think back to the time before electricity. But the stars were | :23:45. | :23:50. | |
visible, they were part of our lives. It is the foundation of | :23:50. | :23:54. | |
science, astronomy is the oldest science, the motivation to | :23:54. | :23:57. | |
understand the view that if you live in a city all your life, you | :23:57. | :24:00. | |
don't see it. It is a powerful thing to do. | :24:00. | :24:04. | |
It is very striking, we know we are doing it on bad day. We know the | :24:04. | :24:09. | |
weather wasn't perfect, but if they can do it for us now, there is no | :24:09. | :24:12. | |
reason they can't do it at a better time of year. Because it is the | :24:12. | :24:16. | |
last show, I usually answer the questions, but because Dara has a | :24:16. | :24:23. | |
degree of physics and cosmology from one of Ireland's premier | :24:23. | :24:27. | |
institutions. Dara will be answering the questions. | :24:28. | :24:32. | |
Katie asks, why doesn't planets twinkle in the sky? I always | :24:32. | :24:36. | |
presume it is because they were further away and more chance of | :24:36. | :24:39. | |
fragments of dust and other things to pass away. It is not, because | :24:39. | :24:43. | |
they are so far away, they are a point source of life, a single beam | :24:43. | :24:47. | |
of life light, when it hits the atmosphere and gets bounced around, | :24:47. | :24:52. | |
it gets deflected, much better than planets who have a number of points. | :24:52. | :24:56. | |
They are bigger, it is extended source, that is the term for it. It | :24:56. | :25:00. | |
is easier for them when they come into the atmosphere to remain | :25:01. | :25:05. | |
coherent. That is the only one we have time for. 100% record. If we | :25:05. | :25:10. | |
find life in the Solar System, it will only be certainly at the | :25:10. | :25:14. | |
microbe level. If we want to find substantial life forms, we have to | :25:14. | :25:20. | |
search for planets much further out in space. Take a look at this image | :25:20. | :25:27. | |
found by the Hubble Space Telescope, it is called Fomalhaut. | :25:27. | :25:31. | |
It is a star called Fomalhaut. have removed the star from the | :25:31. | :25:35. | |
image, the bright centre is gone, we can see around it. What you are | :25:35. | :25:39. | |
looking at is a very young star, a bright blue star. It is one of the | :25:39. | :25:42. | |
brightest stars in the sky, it is in the southern Hemisphere so we | :25:42. | :25:48. | |
can't see T it is a very young star. -- it. It is a very young star. You | :25:48. | :25:54. | |
are looking at a prime mordal disc. That is what our Solar System may | :25:54. | :25:58. | |
have looked like over four billion years ago. That is interesting. It | :25:58. | :26:01. | |
is a beautiful image. The most interesting thing about this n this | :26:01. | :26:05. | |
square here, it is blown up. There is a large object here. It is | :26:05. | :26:10. | |
actually a very large object. It is, in fact, a planet, in a very early | :26:10. | :26:16. | |
stages of its formation. How rare is that to see. Has it ever been | :26:16. | :26:21. | |
seen? No planet had been photographed before. They are | :26:21. | :26:26. | |
extremely faint. It was all the techniques outlined in the | :26:26. | :26:30. | |
programme. This shubl pays telescope image is a planet. It | :26:30. | :26:35. | |
wasn't moved there in -- Hubble Space Telescope image is a planet. | :26:35. | :26:40. | |
It is a long way out from the star. Is it gathering up and building up | :26:40. | :26:46. | |
dust, like the process which our planets were made. We think planets | :26:46. | :26:51. | |
begin very small, only a kilometer across or smaller, over time in | :26:51. | :26:55. | |
collisions they aggregate, the biggest ones begin to suck up all | :26:55. | :26:59. | |
the dust. Eventually in that system you will get a clean Solar System | :26:59. | :27:05. | |
like we get today. Scientists have discovered 700 exo-planets, each | :27:05. | :27:10. | |
and every one of these discoveries have been made in the last 20 years. | :27:10. | :27:19. | |
We have been looking at nebulae and planets over the years, we had to | :27:19. | :27:25. | |
get until 1982 for our first exo- planet, and here is why. | :27:25. | :27:31. | |
To understand why it is so hard to find planets orbiting distant stars, | :27:31. | :27:36. | |
you have to get a sense of how far those stars are from us here on | :27:36. | :27:43. | |
earth. If I were to build a scale model of the galaxy in the Milky | :27:43. | :27:47. | |
Way, starting here with the Solar System and this is the sun. Let's | :27:47. | :27:52. | |
say I put the earth one centimeter away. If the earth were that big, | :27:52. | :27:57. | |
the sun would be as big as this tea shop. Ignore that for a minute. | :27:57. | :28:02. | |
Let's say this is the sun and I put the earth one centimeter away. That | :28:02. | :28:06. | |
is known as one astronomical unit. To the outer planets of the Solar | :28:06. | :28:11. | |
System, Neptune, that is 30 astronomical units, 30-times | :28:11. | :28:17. | |
further away. On wards to the edge of the Solar System, there is the | :28:17. | :28:23. | |
exo-planet, Pluto. That sits around 50 astronomical units away. We have | :28:23. | :28:27. | |
about 50cms representing the size of our Solar System, out to Pluto. | :28:27. | :28:31. | |
Now, on here somewhere, on a mountain, on the earth, in Hawaii, | :28:31. | :28:40. | |
there is one of earth's most powerful telescope, the Keck | :28:40. | :28:45. | |
telescope, it took a picture of Neptune and its moon. This is the | :28:45. | :28:51. | |
most powerful photograph we have, and it is a featureless blob. At | :28:51. | :28:55. | |
its further point from the sun, Pluto is 50 astronomical units away. | :28:55. | :28:59. | |
That is nothing when you are building a model of the Milky Way. | :28:59. | :29:07. | |
Because the nearest star to our sun is 268,000 astronomical units away. | :29:07. | :29:17. | |
It is a star called Proximus Antori. I have to get much further out to | :29:17. | :29:26. | |
mark its scale. If the earth is one centimeter away from the sun in the | :29:26. | :29:32. | |
tea shop, then Proximus would be here, two kilo metres away, that is | :29:32. | :29:36. | |
the nearest star. The telescope doesn't have trouble seeing it, | :29:36. | :29:40. | |
although it is four light years away, it is 100-times the diameter | :29:40. | :29:47. | |
of Pluto, and it is a star, a giant nuclear fusion reactor, giving out | :29:47. | :29:53. | |
light. Imagine trying to see planet in orbit around Proximus Antori, | :29:53. | :29:57. | |
they are smaller than a star, they don't give out light, and they | :29:57. | :30:02. | |
reflect t they get lost in the glaer of the star. Trying to see a | :30:02. | :30:09. | |
planet around Proximus Antori, would be like trying to see a grain | :30:09. | :30:14. | |
of sand, 100 miles away, in the glare of a spotlight. Planets | :30:14. | :30:18. | |
orbiting distant stars are so far away and difficult to detect, we | :30:18. | :30:24. | |
discovered one for the first time, just 20 years ago. | :30:24. | :30:28. | |
Far too distant to be seen by any telescope on earth, it was found by | :30:28. | :30:32. | |
scientists who weren't looking for planets at all. They were looking | :30:32. | :30:38. | |
for pulsars. Pulsars are neutron stars, the | :30:38. | :30:44. | |
remains of dead stars. The leftovers of supernova explosions. | :30:44. | :30:49. | |
They are incredibly small and dense. They can be the size of a city, but | :30:49. | :30:54. | |
be more massive than the sun. They can spin very fast on their axis. | :30:54. | :31:01. | |
When they do that, you get beams of intense radiation, a spinning | :31:01. | :31:05. | |
around. Like a lighthouse beam. That lighthouse beam can cross the | :31:05. | :31:11. | |
face of the earth. So we see a series of bright, regular pulses, | :31:11. | :31:16. | |
and that is what gives them their name. The timing of the pulses is | :31:16. | :31:20. | |
so precise, that they are as accurate and reliable as an atomic | :31:20. | :31:24. | |
clock. But in 1992, scientists noticed something strange. One of | :31:25. | :31:32. | |
the pulses missed a beat. It was as if the pulsar had wobbled. Our sun | :31:32. | :31:35. | |
also wobbles as it spins on its axis. That is because it is | :31:35. | :31:39. | |
surrounded by planets. The gravitational pull of the sun keeps | :31:39. | :31:45. | |
the planets in orbit, but planets are also massive objects, they | :31:45. | :31:49. | |
exert a gravitational pull on the sun. That causes it to worbl | :31:49. | :31:55. | |
slightly. So -- wobble slightly. So scientists back in 1982, realised | :31:55. | :32:00. | |
they were seeing the same thing happening to the pulsar, those | :32:00. | :32:05. | |
precise rite Mick beams were being knocked out of -- rhythmic beams | :32:05. | :32:09. | |
were being knocked out of sync slightly by the gravitational pull | :32:09. | :32:13. | |
of the planet. The discovery proved there is a way to find planets too | :32:13. | :32:19. | |
distant to be seen. They can be detected because they cause the | :32:19. | :32:23. | |
stars they orbit around to wobble. Around three years after the first | :32:24. | :32:29. | |
one was discovered, another worbl was discovered in the orbit of the | :32:29. | :32:33. | |
Pegasus. It was not dead, it was a star like our sun. It was the | :32:33. | :32:43. | |
:32:43. | :32:44. | ||
unmistakable sign of a planet. They named it 51 Peg. The discover of 51 | :32:44. | :32:48. | |
Peg b was a watershed moment, it was the first time to find planet | :32:49. | :32:54. | |
orbiting a living star, beyond our Solar System. Today we found over | :32:54. | :32:57. | |
700 planets, fascinating in itself. But for me, the most interesting | :32:57. | :33:03. | |
thing is it takes us closer to a far more precious goal, which is to | :33:03. | :33:08. | |
discover an earth-like planet around a distant star, a planet | :33:08. | :33:17. | |
that maybe could have life. So I can see why a wobble would be | :33:17. | :33:22. | |
obvious in a pulsar, sending out these huge jets of radiation. A | :33:22. | :33:25. | |
star like our sun doesn't do that, what is this wobble? The only thing | :33:25. | :33:29. | |
you can do is look at the light. Stars do wobble. We have graphic | :33:29. | :33:34. | |
here, which shows a star, and a planet. The star, which is here, | :33:34. | :33:39. | |
looks as though it is orbiting as well, that is because it is. The | :33:39. | :33:43. | |
star and the planet orbit around what is called the common centre of | :33:43. | :33:46. | |
mass. The star will move a little bit. Think about the light that | :33:46. | :33:51. | |
star is emitting, now if the star is coming towards us, then the wave | :33:51. | :33:54. | |
lengths of that light become squashed, which means the light | :33:54. | :33:59. | |
moves to the blue bit, the shorter wavelength of the spectrum. If the | :33:59. | :34:03. | |
star is moving away from us, the light is stretched and the light | :34:03. | :34:08. | |
shifts to us a long wavelength edge of the spectrum. That is called the | :34:08. | :34:12. | |
Doppler shift, if you look at the spectrum of light from a star, and | :34:12. | :34:16. | |
can you see if it is moving towards us and back, and towards us and | :34:16. | :34:21. | |
back. By measuring that precisely you can infer there is a planet | :34:21. | :34:26. | |
around it. That wobble can only occur if the planet is making a | :34:26. | :34:32. | |
star? Really large planets so it is a substantial effect. The best | :34:32. | :34:37. | |
technique for finding smaller more earth-like planets the transit | :34:37. | :34:41. | |
method, which is what we have been using for our planet experiment | :34:41. | :34:45. | |
over the last three nights? That looks for the dips in the light | :34:45. | :34:50. | |
measures of distant stars. You can see it in the graphic, the planet | :34:50. | :34:54. | |
crosses the face of the star, as seen from earth, and the light will | :34:54. | :35:00. | |
drop as it leaves. 35 of the confirmed exo-planet discoveries | :35:00. | :35:04. | |
came from Kepler, the planet hunting telescope, it is possible | :35:04. | :35:09. | |
to search from earth. One of the best in the world is called | :35:09. | :35:12. | |
SuperWASP. It is based in South Africa. Run remotely from Britain | :35:12. | :35:18. | |
by scientists from Keele University. Believe it or not, by the push of a | :35:18. | :35:23. | |
button. Liz is standing next to it. If we press this, that will kick | :35:23. | :35:31. | |
off. There we go. How is that Liz? Good skills, Dara, | :35:31. | :35:39. | |
don't let all that power go to your head now. This is SuperWASP. Super | :35:39. | :35:42. | |
Wide Angle Search for Planets. When Dara isn't interfering with it, it | :35:42. | :35:49. | |
is run remotely from Keele University in Staffordshire. One of | :35:49. | :35:53. | |
their astronomers was in town earlier this week, giving it an MOT, | :35:53. | :36:00. | |
I caught up with him to find out how this gorgeous machine works. | :36:00. | :36:05. | |
So we have eight cameras here, each of which has an enormous field of | :36:05. | :36:11. | |
view. It images 1% of the sky. looks like a fairly simple set-up, | :36:11. | :36:15. | |
eight digital cameras, how do you go about finding exo-planets? | :36:15. | :36:19. | |
monitor the same patch of sky, 50 times a night, we continue to do | :36:19. | :36:22. | |
that for five months. At that point we have a measure of the brightness | :36:22. | :36:28. | |
of the stars over time, and we look for periodic dimming that could be | :36:28. | :36:33. | |
caused by a planet passing in front of the stars. We use bigger | :36:33. | :36:36. | |
telescopes using another technique to confirm it is a planet. One in | :36:36. | :36:43. | |
12 turn out to be so. How many exo- planets has SuperWASP found? 75 and | :36:43. | :36:47. | |
counting. The planets we find, because they are easiest for us to | :36:47. | :36:51. | |
find, are called hot Jupiter, planets around the size of Jupiter, | :36:51. | :36:56. | |
much closer to their star than Jupiter. Which one interests you | :36:56. | :37:05. | |
the most? One I'm fond of is WASP17b it is the first one in a | :37:05. | :37:09. | |
retrogade orbit, it spipbs one way and the star the other way. It is | :37:09. | :37:14. | |
counter to any planet known before and in the Solar System. It is | :37:14. | :37:19. | |
discoveries such as these which is refining planet theories and | :37:19. | :37:27. | |
evolution. With such confirmed exo- planets, what are the chances of | :37:27. | :37:32. | |
one of them keeping life? The ones found are increasingly like our | :37:32. | :37:35. | |
planet earth, I think the chances are very high. I think we will find | :37:35. | :37:42. | |
life on another planet, within our lifetime. | :37:42. | :37:45. | |
The reason why David isn't standing beside me right now for a bit more | :37:45. | :37:51. | |
of a chat, is he's on his way to Chile right now to verify another | :37:51. | :37:57. | |
bunch of exo-planets .5 confirmed exo-planets and counting, watch | :37:57. | :38:02. | |
this space. 75 confirmed exo- planets and founding, watch this | :38:02. | :38:11. | |
space. You saw the Lovell telescope being controlled by Dara and | :38:11. | :38:16. | |
pointed towards Kepler 22b. Why have we done that? Kepler 22b is | :38:16. | :38:20. | |
one of the best candidates for complex life outside the Solar | :38:20. | :38:24. | |
System. As I said at the start, it is 600 light years away, a long way | :38:24. | :38:27. | |
away. I don't think we will hear any signals from a civilisation. | :38:27. | :38:32. | |
You never know. It has never been done before. I'm quite excited. | :38:32. | :38:37. | |
number of our planets are in the region, we obviously are. Let me | :38:37. | :38:40. | |
talk about the habitable region. There is a zone around any given | :38:40. | :38:44. | |
star, around the sun it is the zone which the earth sits, but also | :38:44. | :38:48. | |
Venus and Mars sit in that zone. It is the zone where roughly speaking | :38:48. | :38:53. | |
the temperature will be right for things like liquid water and rich | :38:53. | :38:56. | |
oxygen atmospheres to exist on planets. It is not a given that | :38:56. | :39:00. | |
life will occur. Venus and Mars, there is no real evidence of any | :39:00. | :39:04. | |
major complex life on those, eventhough they are in the hab | :39:04. | :39:12. | |
table zone? Mars is too small, it is in the Habibi bittable zone, but, | :39:12. | :39:15. | |
Venus has the hottest surface in the Solar System other than the sun. | :39:15. | :39:20. | |
But Kepler 22b is in a similar zone around its star. Whilst you can't | :39:20. | :39:24. | |
say for certain it is a habitable planet, it could be like Venus, | :39:24. | :39:28. | |
Mars or none of the three. There is a chance that it is habitable. That | :39:28. | :39:33. | |
means there is a chance that telescope is pointing at a | :39:33. | :39:39. | |
civilisation of alien.S. Later in the show we will hear them. | :39:39. | :39:45. | |
We will explain what the discovery could mean, and to tell us why it | :39:45. | :39:49. | |
is so important is Giovanna Tinetti? It is a very exciting | :39:49. | :39:53. | |
planet, Kepler 22b, it is orbiting a star very similar to the sun, it | :39:53. | :39:57. | |
is the exact distance to the star to potentially have liquid water, | :39:57. | :40:01. | |
that is why it is so interesting. What's the next step, how are we | :40:01. | :40:05. | |
going to begin to characterise that planet and perhaps look for the | :40:05. | :40:09. | |
signs of life? Essentially what we are doing right now with planets | :40:09. | :40:15. | |
that are slightly hotter and bigger than Kepler 22b, is to use the | :40:15. | :40:20. | |
method to look at their atmosphere, trying to get the composition of | :40:20. | :40:24. | |
the atmosphere. We are looking at some light curves and preeting that | :40:24. | :40:29. | |
at different wavelengths. You have to wait until the planet comes back | :40:29. | :40:34. | |
around again and measure the light as it comes through the atmosphere? | :40:34. | :40:40. | |
Exactly what a challenge, we can do it for other planets now. Is there | :40:41. | :40:45. | |
a chance, Kepler 22b, is there a chance to map that planet out in | :40:45. | :40:50. | |
detail? I'm afraid Kepler 22b is probably too far away to do this | :40:50. | :40:53. | |
kind of measurement. We can certainly do this kind of | :40:53. | :40:57. | |
measurement and planets around a starch closer to us, certainly we | :40:57. | :41:02. | |
will do that with the dedicated space mission in the future, like | :41:02. | :41:06. | |
Echo. As the light goes through it, what are the tell tale signs, what | :41:06. | :41:12. | |
are you looking for? We look at the spectrum and look at the signature | :41:12. | :41:17. | |
of some molecules, if you are interested, we are looking for | :41:17. | :41:21. | |
molecule that is tell us something about if this planet is inhabited | :41:21. | :41:28. | |
or not. I would love to see liquid water, or some water vapour, and in | :41:28. | :41:34. | |
particular, having some signature or ozone or oxygen, like on earth, | :41:34. | :41:39. | |
that would be an interesting signature. In earth's atmosphere, | :41:39. | :41:43. | |
oxygen is only present because of the action of life in large | :41:43. | :41:46. | |
quantities, if you saw that in one of these planets, you would be | :41:46. | :41:50. | |
fairly certain there is life. We have to go back to Dulverton now, | :41:50. | :41:54. | |
I'm afraid. They have had 20 minutes to get used to the dark. | :41:54. | :41:59. | |
Usually in astronomy it takes 20 minutes for your eyes to | :41:59. | :42:06. | |
acclimatise. We will go back to see how different the place feels. That | :42:06. | :42:10. | |
was nothing more than amazing. To see the lights go out. Every single | :42:10. | :42:14. | |
light that I could see in the Main Street has gone out. It went so | :42:14. | :42:17. | |
dark. It has taken our eyes a little bit of time to adjust. It is | :42:18. | :42:23. | |
like being in the countryside but in the middle of a town. Joining me | :42:23. | :42:27. | |
is a local astronomer. What is it like having all the lights out? | :42:27. | :42:31. | |
is very much like how it was when I was younger. I could come out and | :42:31. | :42:35. | |
see the great ribbon of stars in the Milky Way, now all the fainter | :42:35. | :42:38. | |
stars have gone. It is a chance to get that back again. If it was | :42:38. | :42:42. | |
clear it would have been lovely? would have been glorious. It is | :42:42. | :42:47. | |
great to see the way it has worked. We're joined bit headmaster of the | :42:47. | :42:51. | |
local school. The entire community has come together for this? They | :42:51. | :42:54. | |
have, it really has company turd the imagination of the communety. | :42:54. | :42:57. | |
You only -- captured the imagination of the community. You | :42:58. | :43:04. | |
only go walk down the street and see the effort the shopkeepers have | :43:04. | :43:08. | |
made. Hopefully it is the start of something and we get left with a | :43:08. | :43:12. | |
legacy we have already been talking about forming a local astronomical | :43:12. | :43:17. | |
society, and having a sunnor branch based at the schools. That is in-- | :43:17. | :43:21. | |
A junior branch based at the schools. This has shown tonight, | :43:21. | :43:25. | |
regardless of the fact we can't see clear stars, everyone can take | :43:25. | :43:29. | |
responsibility for light f we can do that and think how we are using | :43:29. | :43:34. | |
it we can make a difference. If you want to learn more go to the | :43:34. | :43:39. | |
website. You can find a link to the dark skies discovery network on | :43:39. | :43:43. | |
[email protected]. You can find out where the local | :43:43. | :43:51. | |
dark spots are and recommend your own dark sites. | :43:51. | :43:55. | |
I have to say, I'm just the messenger, not the person who | :43:55. | :43:59. | |
brings the weather, one night this week we really needed those clear | :43:59. | :44:02. | |
week we really needed those clear skies. At Dulverton the rain has | :44:02. | :44:05. | |
moved in, the same across many parts of central, southern England | :44:05. | :44:10. | |
and Wales overnight. The best chance to get the telescope out, | :44:10. | :44:14. | |
eastern England, Northern Ireland, Scotland. Cloud will vair year, but | :44:14. | :44:18. | |
lengthy clearer spells, even clearer spells across parts of | :44:18. | :44:21. | |
western Scotland. Tonight, clearer spells in the north, tomorrow we | :44:21. | :44:24. | |
might reverse it a little bit. Scattering of showers expected. | :44:24. | :44:28. | |
These will be mainly to northern and western areas. Some of those | :44:28. | :44:32. | |
will be wintry. Eastern Scotland, north-east England, get out early | :44:32. | :44:36. | |
on before the cloud thickens up. For much of England aWales, away | :44:36. | :44:41. | |
from the north and west, a few hours before the cloud pushes in. | :44:42. | :44:44. | |
Into the weekend, whilst seeing plenty of showers, across eastern | :44:44. | :44:49. | |
and southern parts, the air will be fairly clear at times. A cold air | :44:49. | :44:53. | |
mass coming down from the north, the clarity of the air should | :44:53. | :44:57. | |
the clarity of the air should increase as well. Happy stargazing. | :44:57. | :45:01. | |
I thought that showed the real spirit of stargazing, eventhough it | :45:01. | :45:06. | |
is cloudy in Dulverton, even the act of making it dark, the school | :45:06. | :45:12. | |
will be getting involved and the astronomical Society being formed, | :45:12. | :45:18. | |
and the schools getting involved. Try it every night of the year! We | :45:18. | :45:21. | |
set the dish moving at the beginning of the show, we now have | :45:21. | :45:26. | |
a unique chance to listen to the radio waives coming from an exo- | :45:26. | :45:32. | |
planet, Kepler 22b. What should we listen out for? We should listen to | :45:32. | :45:36. | |
what the Hubble Space Telescope usually hears, the radio waves | :45:36. | :45:43. | |
created into sound. This is space noise. It sounds like empty static. | :45:43. | :45:50. | |
That is just radio astronomy, there is data in there. Listen to this. | :45:50. | :45:54. | |
(knocking) If you heard that, would you think that's regular, that is | :45:54. | :45:57. | |
not natural. In fact, that is natural. That is the sound of a | :45:57. | :46:01. | |
pulsar. When it was first heard, the first pulsar was discovered, | :46:01. | :46:08. | |
that was named LGM1 that means "little green men 1". For a few | :46:08. | :46:12. | |
days it was thought how can something from nature be so regular. | :46:12. | :46:18. | |
If we hear that from Kepler 22b, it is a pulsar. If we hear a regular | :46:18. | :46:23. | |
beat like that, we would have to postpone the news. There is only | :46:23. | :46:25. | |
one incident where something was heard that couldn't be explained. | :46:25. | :46:31. | |
It is called the WOW signal. It is a picture of it. That is the | :46:31. | :46:35. | |
picture of the data from a radio telescope a regular strange signal | :46:35. | :46:42. | |
was heard, to this day it hasn't been explained. It is called WOW, | :46:42. | :46:45. | |
because the radio operator wrote that next to it. They have gone | :46:45. | :46:49. | |
back to the skies, and nothing has been heard since. It remains | :46:49. | :46:53. | |
genuinely unexplained. Tim comes back in, if we do hear | :46:53. | :46:57. | |
something you would really want to be here? Certainly. I have my | :46:57. | :47:03. | |
fingers crossed. Do we think we will hear anything? Tim it is | :47:03. | :47:07. | |
probably too far away even if it was a noisy civilisation. If they | :47:07. | :47:11. | |
put a beacon there. A strong enough transmitter and telescope, you | :47:11. | :47:20. | |
never know. This is the sound coming to us live from Kepler 22b. | :47:20. | :47:24. | |
(static noise) That is quiet you have now. It is quiet, that is what | :47:24. | :47:29. | |
we expected, of course. Tim, it sounds like a game, it sounds like | :47:29. | :47:33. | |
science fiction. It isn't, there is the SETI project, which this | :47:33. | :47:38. | |
telescope has been involved in, searching for signals. It is a | :47:38. | :47:41. | |
serious possibility, if you don't look you won't find anything. It is | :47:41. | :47:45. | |
worth having a look and listen in this case and analysing the signals | :47:45. | :47:55. | |
very carefully, just in case. search for exo-planets, now we can | :47:55. | :47:58. | |
focus where we look for possible civilisations. We may be closer | :47:58. | :48:05. | |
than ever to finding a planet with life, but the idea of attempting to | :48:05. | :48:08. | |
communicate with civilisations in the distance is not new. What would | :48:08. | :48:18. | |
:48:18. | :48:20. | ||
it mean to make first contact? It is easy to find the idea of UFOs | :48:20. | :48:30. | |
:48:30. | :48:31. | ||
and extraterrestrial life a bit of But for centuries scientists have | :48:31. | :48:38. | |
taken the idea of alien contact very seriously. Early astronomy | :48:38. | :48:40. | |
revealed our Solar System contained other planets, and as soon as we | :48:40. | :48:44. | |
thought there could be worlds like our's nearby. We couldn't wait to | :48:44. | :48:48. | |
tell them that we were here. We were sentient and we were dying to | :48:48. | :48:53. | |
say hello. If you look certainly at the 19th century, there was some | :48:53. | :48:57. | |
quite prominent scientific figures who had really quite practical | :48:57. | :49:02. | |
ideas for how you might try to communicate with alien life. So, | :49:02. | :49:09. | |
for example, Carl Friedrich Gauss, a very famous mathematition and | :49:09. | :49:15. | |
scientist, had an idea for cutting enormous geomet kal shapes into the | :49:15. | :49:22. | |
Siberian forest which would be -- geomet kal shapes into the Siberian | :49:22. | :49:25. | |
forest which would be seen from space. | :49:25. | :49:30. | |
He felt strongly that the sun might be a habitable place, and it might | :49:30. | :49:40. | |
:49:40. | :49:48. | ||
be worth looking for life forms we could communicate on the sun. | :49:48. | :49:53. | |
As astronomy became clear, it was thought that aliens had to be out | :49:53. | :49:59. | |
joyed suer Solar System. Science had to develop enormously before | :49:59. | :50:05. | |
messages could be sent out to other worlds. In the 1970s NASA launched | :50:05. | :50:11. | |
the Pioneer and Voyager probes, sent to look at the outer Solar | :50:11. | :50:15. | |
System. In case they came across aliens, on board they carried | :50:15. | :50:20. | |
information about us. Pioneer contains a plaque which has | :50:20. | :50:24. | |
on it the location of the Solar System, some basic scientific | :50:24. | :50:28. | |
information, and most famously a picture of two naked human beings, | :50:28. | :50:33. | |
generally thought to be average Americans, in mellow greeting. You | :50:33. | :50:38. | |
know the way average Americans are this buff and hairless. At the time | :50:38. | :50:42. | |
of the Voyager launch, more information could be encoded, | :50:42. | :50:46. | |
including an entire disc of sounds of the earth, more scientific | :50:46. | :50:50. | |
information, and images of our history and culture. Whether of | :50:50. | :50:58. | |
hunting, the moment of conception, and that guy. Images of licking, | :50:58. | :51:03. | |
biting and swallowing, as some sort of threat, presumably. To counter | :51:03. | :51:06. | |
act that, we also included greetings recorded from people from | :51:06. | :51:16. | |
:51:16. | :51:22. | ||
all over the world, in their own However, these messages would be | :51:22. | :51:27. | |
very difficult for any alien life form to find. Although the Voyager | :51:27. | :51:33. | |
I probe is now the fastest and distant human-made object in the | :51:33. | :51:38. | |
universe, it is still comparatively nearby, inconspicuous and slow. | :51:38. | :51:41. | |
Creatures from other worlds would literally have to bump into it in | :51:42. | :51:46. | |
order to retrieve the message. It won't even reach the nearest star | :51:46. | :51:51. | |
system for another 40,000 years. But there was another way in which | :51:51. | :51:58. | |
we could search for alien life, radio waves. In 1960, visionary | :51:58. | :52:02. | |
astronomer, Frank Drake, made the first deliberate attempt to detect | :52:02. | :52:05. | |
signals from other world. Scientists from around the world | :52:05. | :52:09. | |
soon joined the search, which became known asset at this, the | :52:09. | :52:15. | |
search for extra terrestrial intelligence. It dawned on radio | :52:15. | :52:20. | |
astronomers in the 1950s that these big radio telescopes can be | :52:20. | :52:24. | |
limitless in size. They are capable of enormous sensitivity. They | :52:24. | :52:28. | |
communicate not just across terrestrial distances or | :52:28. | :52:33. | |
interplanetary distances, but truly interstellar distances. The fact we | :52:33. | :52:37. | |
can search for messages throws up another question, what do we do if | :52:37. | :52:43. | |
we find one? And what if by sending a message we attract the attention | :52:43. | :52:48. | |
of great big extraterrestrial monsters who want to eat us. Even | :52:48. | :52:52. | |
if their intentions are benign, we could be opening ourselves up to | :52:52. | :52:58. | |
unexpected dangers. Afterall, our own history of encountering foreign | :52:58. | :53:03. | |
culture offers a cautionary tale. Very often they started like | :53:03. | :53:08. | |
Captain Cook arriving in Hawaii, with best intentions, handshakes | :53:08. | :53:14. | |
and smiles wall the way round. But Captain Cook still didn't survive | :53:14. | :53:18. | |
the encounter. Despite all the friendship and treaties, within 150 | :53:18. | :53:25. | |
years, 90% of people in Hawaii were dead, because of diseases that were | :53:25. | :53:30. | |
unintentionally introduced. Even when things are all shand shake and | :53:30. | :53:35. | |
-- handshake and friendly there can be terrible consequences. None the | :53:35. | :53:40. | |
less, the SETI post detection task group is standing by, should an | :53:40. | :53:46. | |
alien signal arrive. Professor Paul Davies could be among the first to | :53:46. | :53:50. | |
receive a message from ET, his response might not use words at all. | :53:50. | :53:53. | |
The things we would truly share are the things that are literally | :53:53. | :53:58. | |
universal throughout the universe, that is mathematics and fistics, | :53:58. | :54:02. | |
the laws of physics are the same throughout the universe, and | :54:02. | :54:08. | |
mathematics are the same throughout by that definition. One could build | :54:08. | :54:12. | |
a broader dialogue, and after thousands of messages back and | :54:12. | :54:16. | |
forth we could tell them about our politics and sport. We can hope | :54:16. | :54:21. | |
that their politics and sport doesn't include eating us! The | :54:21. | :54:24. | |
truth is, whatever the price, receiving an alien message will | :54:24. | :54:29. | |
confirm what some of us are desperate to know, that we aren't | :54:29. | :54:36. | |
alone in the universe. Three nights ago we asked you to do | :54:36. | :54:44. | |
something very special, we wanted you to help us find a Stargazing | :54:44. | :54:47. | |
exo-planet. Chris Lintott is in charge. Have we found planet? | :54:47. | :54:51. | |
have, we think we have. We were looking for the dips in light in | :54:51. | :54:56. | |
the stars' brightness when planets get in front of the parent star. We | :54:56. | :55:01. | |
found one in particular that two people told us they were the dips, | :55:01. | :55:06. | |
we went back into the data and found five of the tips, each 90 | :55:06. | :55:09. | |
days apart. We think it is planet that goes around this particular | :55:09. | :55:15. | |
star once every 90 days. How many people responded? Over 100,000 | :55:15. | :55:20. | |
people, well over a million classifications, one million and | :55:20. | :55:23. | |
84,000 classifications. These are ordinary people, watchers of | :55:23. | :55:29. | |
Stargazing? They went to the website, the PlanetHunters, lock | :55:29. | :55:35. | |
logged on and -- logged on and did what people are still doing now | :55:35. | :55:42. | |
Let's see the data. I want to name it. This is Lee | :55:42. | :55:47. | |
Threplton, and then Chris Holmes, on the right, later on, that is 90 | :55:47. | :55:51. | |
days later. We are looking at the light from the star, characteristic | :55:51. | :55:55. | |
dip of the planet crossing the face of the star. If you look to 90 days | :55:55. | :55:59. | |
after, that we dug into the computer. It should be noted there | :55:59. | :56:09. | |
:56:09. | :56:10. | ||
were others who spotted these planets they were after Threpl to n | :56:10. | :56:11. | |
and Holmes. Those names down the bottom of the screen have | :56:11. | :56:14. | |
identified it and others too. is lots more we have got there. | :56:14. | :56:18. | |
More data we are put anything right now. If anyone else wants a planet | :56:18. | :56:24. | |
named after them they can go there. We have an artist's impression of | :56:24. | :56:30. | |
the planet. It is Neptune-sized. It is gaseous, it is a hot Neptune, it | :56:30. | :56:36. | |
goes around its star in 90 days, as close to the star as Mercury. | :56:36. | :56:46. | |
:56:46. | :56:46. | ||
is the planet we are unofficially and bindingly calling planet | :56:46. | :56:51. | |
Threplton-Holmesb. Where is it? outside now, stair ten degrees in | :56:51. | :56:59. | |
the North West, between Deneb and deep Veg a. You need a pretty big | :56:59. | :57:05. | |
telescope but they found it on-line, but they found it. It is gas planet, | :57:05. | :57:09. | |
we wouldn't necessarily find life? It is too hot, it is in The Golden | :57:09. | :57:12. | |
Calf zone t might have a moon, you withstand on one of the moons and | :57:12. | :57:19. | |
look at the wonder that is Threplton-Holmes. Thank you, this | :57:19. | :57:25. | |
is incredible for me, our audience has found a new planet around a | :57:25. | :57:29. | |
distant star. And named after two guys we have never met. What an | :57:29. | :57:34. | |
amazing way to bring the programme to a close. Goodbye to Liz in South | :57:34. | :57:39. | |
Africa, we found a planet Liz, can you believe that? That is such | :57:39. | :57:43. | |
brilliant news. Isn't it astounding what we can achieve in this day and | :57:43. | :57:47. | |
age. I know we have had cloudy skies the last three nights t has | :57:47. | :57:50. | |
been a privilege to be here and learn about the skies in the | :57:50. | :57:55. | |
company of hugely inspirational astronomers, a big thank you to | :57:55. | :57:58. | |
them, they have been wonderful. Armed with the telescopes they are | :57:59. | :58:03. | |
helping us take huge leaps in our understanding of the universe, | :58:03. | :58:07. | |
especially in the hot topic of exo- planets. They are revealing how | :58:07. | :58:09. | |
much there is left to learn about the universe, not just in deep | :58:10. | :58:14. | |
space, but also within our very own solar siste. It is really a very | :58:14. | :58:18. | |
exciting time to be an -- system. It is really a very exciting time | :58:18. | :58:22. | |
to be an astronomer. That is all from the team in South Africa, back | :58:22. | :58:28. | |
to you at Jodrell Bank Observatory. That is a glorious sky, finally | :58:28. | :58:32. | |
seeing a good sky over South Africa. Stay with us for Back To Earth, | :58:32. | :58:36. | |
coming up immediately afterwards. We have many questions to raise | :58:36. | :58:45. | |
about the inhabitants of Threpleton-Holmes. There is warring | :58:45. | :58:52. | |
factions I'm sure. There is more information on the website. Find | :58:52. | :59:02. | |
:59:02. | :59:03. |