Browse content similar to Second Earth?. Check below for episodes and series from the same categories and more!
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30 years ago, two astronomers made a remarkable discovery, | 0:00:02 | 0:00:04 | |
one which would change the way we view the universe for ever. | 0:00:04 | 0:00:07 | |
A planet outside our solar system, orbiting a distant star - | 0:00:07 | 0:00:12 | |
an exoplanet. | 0:00:12 | 0:00:13 | |
Since then, we have found worlds where it rains diamonds, | 0:00:15 | 0:00:19 | |
ones that boil at 3,000 degrees centigrade | 0:00:19 | 0:00:22 | |
and even a world with four suns in its sky. | 0:00:22 | 0:00:24 | |
But the big question is - will we ever find another Earth? | 0:00:27 | 0:00:32 | |
Welcome to The Sky At Night. | 0:00:32 | 0:00:34 | |
Our solar system is filled with an incredible variety of planets. | 0:01:02 | 0:01:07 | |
From small, airless and rocky worlds like Mercury | 0:01:08 | 0:01:11 | |
to gas giants like Saturn, with its spectacular rings of ice. | 0:01:11 | 0:01:15 | |
Surely our solar system couldn't be the only one to host such a wonderful variety of worlds? | 0:01:18 | 0:01:24 | |
And yet, until the 1990s, astronomers hadn't found | 0:01:27 | 0:01:30 | |
a single planet outside our solar system. | 0:01:30 | 0:01:33 | |
And then, in 1995, they found it - | 0:01:34 | 0:01:37 | |
the first really convincing evidence | 0:01:37 | 0:01:39 | |
for a planet orbiting another star. | 0:01:39 | 0:01:42 | |
Since then, we've discovered nearly 2,000, and it's involved | 0:01:42 | 0:01:44 | |
some pretty extraordinary science detective work. | 0:01:44 | 0:01:47 | |
In fact, we've found so many planets that we've reached | 0:01:47 | 0:01:50 | |
a remarkable conclusion. | 0:01:50 | 0:01:52 | |
That almost all the stars in our galaxy | 0:01:52 | 0:01:54 | |
have their own families of planets. | 0:01:54 | 0:01:57 | |
It's a really hot topic in astronomy right now. | 0:01:57 | 0:01:59 | |
We're all desperate to find another Earth. | 0:01:59 | 0:02:01 | |
Although, as we'll see later, quite what that means is open to question. | 0:02:01 | 0:02:06 | |
Coming up tonight, we'll be examining some of the latest | 0:02:08 | 0:02:10 | |
discoveries made here at the Cambridge Exoplanet Research Centre. | 0:02:10 | 0:02:16 | |
And finding out how the hunt for a second Earth, | 0:02:16 | 0:02:19 | |
a habitable planet like our own. is coming along. | 0:02:19 | 0:02:23 | |
We have found planets in all size, in all masses | 0:02:23 | 0:02:26 | |
and in many different kind of structure | 0:02:26 | 0:02:28 | |
from the one we have in the solar system. | 0:02:28 | 0:02:30 | |
Hollywood has no doubts that there are habitable planets out there. | 0:02:32 | 0:02:35 | |
Dallas Campbell finds out | 0:02:35 | 0:02:36 | |
whether exoplanets in the movies have any basis in reality. | 0:02:36 | 0:02:40 | |
And you can see there's the binary star, one is | 0:02:40 | 0:02:43 | |
a little bit whiter, one is a bit red. | 0:02:43 | 0:02:45 | |
Almost exactly like in Star Wars. | 0:02:45 | 0:02:47 | |
We'll tackle a controversial discovery that my own research | 0:02:49 | 0:02:52 | |
group have been involved in. | 0:02:52 | 0:02:54 | |
Could this really be the first discovery of an alien civilisation? | 0:02:54 | 0:02:58 | |
But first, how do you go about finding an exoplanet amongst | 0:03:00 | 0:03:04 | |
the 100 billion stars in our galaxy? | 0:03:04 | 0:03:06 | |
The first true exoplanet was discovered | 0:03:12 | 0:03:14 | |
by two astronomers in 1992. | 0:03:14 | 0:03:16 | |
Scientists found not just one | 0:03:17 | 0:03:19 | |
but at least two planetary objects orbiting around a star. | 0:03:19 | 0:03:23 | |
It was a stunning achievement. | 0:03:24 | 0:03:26 | |
These planets were four times the mass of the Earth | 0:03:26 | 0:03:29 | |
and orbited a type of star called a pulsar - a remnant of a supernova. | 0:03:29 | 0:03:34 | |
Because the pulsar permanently bathed its planets | 0:03:36 | 0:03:39 | |
in high-energy radiation, there was no chance for life. | 0:03:39 | 0:03:42 | |
So in terms of finding another Earth, | 0:03:43 | 0:03:46 | |
these planets were non-starters. | 0:03:46 | 0:03:48 | |
Nevertheless, it was a thrilling discovery, | 0:03:49 | 0:03:51 | |
and left us hungry for more. | 0:03:51 | 0:03:54 | |
What we wanted next was a planet orbiting a main sequence star | 0:03:54 | 0:03:57 | |
just like our own. | 0:03:57 | 0:03:58 | |
And, in a small observatory in France, | 0:04:00 | 0:04:03 | |
a young PhD student struck lucky. | 0:04:03 | 0:04:05 | |
Didier Queloz discovered a planet around the star 51 Pegasi. | 0:04:05 | 0:04:11 | |
51 Pegasi was the right kind of star, | 0:04:11 | 0:04:14 | |
one that wouldn't bathe its planet with deadly radiation. | 0:04:14 | 0:04:18 | |
But in other respects the planet in orbit around it was | 0:04:18 | 0:04:21 | |
spectacularly weird. | 0:04:21 | 0:04:23 | |
It was the size of Jupiter | 0:04:24 | 0:04:25 | |
yet it took just four days to orbit its star. | 0:04:25 | 0:04:28 | |
And its surface temperature exceeded 1,000 degrees Celsius. | 0:04:30 | 0:04:34 | |
It was a type of planet that has come to be known as a "hot Jupiter". | 0:04:34 | 0:04:38 | |
It was an extraordinary discovery that | 0:04:38 | 0:04:40 | |
rewrote our understanding of what exoplanets might be like. | 0:04:40 | 0:04:44 | |
And it was just the beginning. | 0:04:44 | 0:04:46 | |
I caught up with Didier to find out | 0:04:46 | 0:04:48 | |
more about his original discovery, and what's he's been up to since. | 0:04:48 | 0:04:52 | |
Tell me about the day you discovered 51 Pegasi b? | 0:04:52 | 0:04:55 | |
Yeah, I was a PhD student at that time | 0:04:55 | 0:04:57 | |
so the first time I've saw something | 0:04:57 | 0:05:00 | |
a bit strange going on on the series of measurements I made on 51 Peg, | 0:05:00 | 0:05:06 | |
I never thought it would be a planet because it was just impossible. | 0:05:06 | 0:05:09 | |
I thought it was a bug into the instrument, | 0:05:09 | 0:05:11 | |
something was wrong with the instrument, with the machinery. | 0:05:11 | 0:05:14 | |
And it took me a long time to figure out exactly what it was. | 0:05:14 | 0:05:17 | |
Did you hope that the planet you had discovered was going to be Earth-like? | 0:05:17 | 0:05:21 | |
Well, it was impossible because the, the, the, the instrument | 0:05:21 | 0:05:25 | |
we're using, the best it could do is detecting something like Jupiter. | 0:05:25 | 0:05:29 | |
It was designed to do that. | 0:05:29 | 0:05:31 | |
It was already a tremendous achievement at that time. | 0:05:31 | 0:05:33 | |
We can do Earth right now, but at 20 years ago it was not possible. | 0:05:33 | 0:05:37 | |
But it was already so much amazing to find a planet | 0:05:37 | 0:05:41 | |
so bizarre than this one, so I didn't care at all. | 0:05:41 | 0:05:44 | |
I mean, it was really a kind of game changer situation. | 0:05:44 | 0:05:46 | |
So what method did you use to find 51 Peg? | 0:05:46 | 0:05:49 | |
So at the time, the only way to find a planet was to observe | 0:05:50 | 0:05:53 | |
the stars, and, uh, by observing the star we are measuring | 0:05:53 | 0:05:57 | |
the speed of the star, looking for tiny change of that speed. | 0:05:57 | 0:06:01 | |
So, you have a star and you have a planet going round it. | 0:06:01 | 0:06:04 | |
And as the planet goes round it caused the star to | 0:06:04 | 0:06:06 | |
move by a little bit and you're measuring that movement, that speed. | 0:06:06 | 0:06:10 | |
It's a very tiny effect. You don't see it right away, | 0:06:10 | 0:06:12 | |
you need to use quite sophisticated algorithms to build | 0:06:12 | 0:06:15 | |
the average motion that tell you | 0:06:15 | 0:06:17 | |
at the end that there is something orbiting that star. | 0:06:17 | 0:06:20 | |
So that's one method, | 0:06:20 | 0:06:21 | |
but are there other methods for detecting these exoplanets? | 0:06:21 | 0:06:24 | |
People started to look for transit at that time. | 0:06:24 | 0:06:27 | |
What will happen is there will be for short amount of time | 0:06:27 | 0:06:31 | |
a slightly change of the light, a dimming of the light | 0:06:31 | 0:06:33 | |
of the star, like, like a cloud just hiding us the sun. | 0:06:33 | 0:06:37 | |
Uh, we can use that to get the size of the planet as well | 0:06:37 | 0:06:40 | |
as the period of the planet. | 0:06:40 | 0:06:42 | |
We can also combine the two, you can get the mass from the radial | 0:06:42 | 0:06:45 | |
velocity and you can get the size from the transit | 0:06:45 | 0:06:47 | |
and we doing that today to get the density of the planet. | 0:06:47 | 0:06:51 | |
And the density helps you to understand the structure of the planet. | 0:06:51 | 0:06:54 | |
And it was really the beginning. | 0:06:54 | 0:06:55 | |
So it was a massive trigger and that's why at that time | 0:06:55 | 0:06:59 | |
we were maybe 20 people in the world doing that, | 0:06:59 | 0:07:01 | |
now there must be 5,000 people working on this. | 0:07:01 | 0:07:03 | |
So we've found these hot Jupiters and now we're finding sort of | 0:07:03 | 0:07:06 | |
smaller and smaller planets with the better sophisticated equipment. | 0:07:06 | 0:07:09 | |
Do you ever think we'll find another Earth? | 0:07:09 | 0:07:11 | |
Oh, yes, I mean, we have found already, Earth-size planet, | 0:07:11 | 0:07:15 | |
or Earth-mass planet, | 0:07:15 | 0:07:17 | |
most of them they're not exactly Earth equivalent because very often | 0:07:17 | 0:07:21 | |
they're too close to the stars, much too hot. | 0:07:21 | 0:07:24 | |
So we don't really, really know what we're finding these days. | 0:07:24 | 0:07:26 | |
But we have planet in all, in all size, in all masses, | 0:07:26 | 0:07:30 | |
and in many different kind of structure from the one | 0:07:30 | 0:07:34 | |
we have in the solar system. | 0:07:34 | 0:07:35 | |
So we're finding more and more and hopefully, that um, | 0:07:35 | 0:07:38 | |
-another Earth will be out there one day. -Oh, yeah, there are. | 0:07:38 | 0:07:41 | |
Because right now we're finding an average one planet for each star. | 0:07:41 | 0:07:45 | |
So if you look at the star, uh, tonight, | 0:07:45 | 0:07:48 | |
on all the star you seeing by the naked eyes they're planets. | 0:07:48 | 0:07:51 | |
Some of them we are found them, other we have not yet found them. | 0:07:51 | 0:07:54 | |
It means that maybe they are solar system equivalent just | 0:07:54 | 0:07:57 | |
waiting for us to be found. | 0:07:57 | 0:07:58 | |
-Hm, exciting times ahead. -It is definitely exciting, yes. | 0:07:58 | 0:08:01 | |
Well, thank you, that was wonderful. | 0:08:01 | 0:08:04 | |
As we hunt for a second Earth, | 0:08:13 | 0:08:15 | |
we have to think about what it is that we are really looking for. | 0:08:15 | 0:08:19 | |
What is it that makes a planet earthlike? | 0:08:19 | 0:08:22 | |
Is it rocky? Is there liquid water on it surface? | 0:08:22 | 0:08:26 | |
What gravity would it have? | 0:08:26 | 0:08:28 | |
And would we be able to breathe if we were standing on the planet? | 0:08:28 | 0:08:32 | |
Astronomers are only just beginning to work out what | 0:08:34 | 0:08:37 | |
conditions are like on exoplanets. | 0:08:37 | 0:08:39 | |
But that hasn't stopped Hollywood from creating its own alien worlds. | 0:08:39 | 0:08:44 | |
And most of them are very much habitable. | 0:08:44 | 0:08:47 | |
Dallas Campbell investigates how plausible Hollywood's | 0:08:47 | 0:08:50 | |
exoplanets really are. | 0:08:50 | 0:08:52 | |
I went to see Star Wars when it first came out, aged seven, | 0:09:01 | 0:09:05 | |
at the ABC Cinema Haymarket, Newcastle-upon-Tyne. | 0:09:05 | 0:09:09 | |
It was one of those cinema experiences that will be forever etched on my brain. | 0:09:09 | 0:09:15 | |
It ignited my lifelong love affair with science fiction movies. | 0:09:15 | 0:09:19 | |
Amazingly, many of the distant worlds featured in these films were | 0:09:21 | 0:09:24 | |
being imagined by writers | 0:09:24 | 0:09:26 | |
and directors decades before the first exoplanets were found. | 0:09:26 | 0:09:30 | |
The planet Tatooine from Star Wars, for example, you've got this | 0:09:31 | 0:09:35 | |
wonderful, evocative desert landscape, and Luke Skywalker stands there contemplating his destiny, | 0:09:35 | 0:09:42 | |
bathed in the afternoon light from not one but two suns. | 0:09:42 | 0:09:47 | |
Although it has two suns, | 0:09:58 | 0:09:59 | |
in almost every other respect Tatooine feels reassuringly earthlike, | 0:09:59 | 0:10:04 | |
which makes sense, given that it was filmed in Tunisia. | 0:10:04 | 0:10:07 | |
But the same can't be said for this planet. | 0:10:07 | 0:10:09 | |
If I owned this place and hell, | 0:10:10 | 0:10:12 | |
I'd rent this place out and live in hell. | 0:10:12 | 0:10:15 | |
This is Crematoria from The Chronicles Of Riddick, | 0:10:17 | 0:10:20 | |
and in it the protagonist has to deal with furnace-like temperatures during the day, | 0:10:20 | 0:10:24 | |
so up to 372 degrees, | 0:10:24 | 0:10:26 | |
and then at night it gets down to minus 182 degrees - | 0:10:26 | 0:10:30 | |
with only a 20-minute window where the characters can actually | 0:10:30 | 0:10:35 | |
walk about safely on the surface. | 0:10:35 | 0:10:37 | |
Interstellar is about the search for a second Earth. | 0:10:50 | 0:10:53 | |
As food resources run out humanity must find a new home. | 0:10:53 | 0:10:57 | |
And en route they have a close encounter with a very strange water world called Miller, | 0:10:57 | 0:11:02 | |
which has 30% more gravity than Earth, | 0:11:02 | 0:11:04 | |
huge tidal waves and is orbiting an enormous black hole called Gargantua. | 0:11:04 | 0:11:10 | |
It's our only chance to save people on Earth. | 0:11:10 | 0:11:13 | |
If I can find a way to transmit the quantum data I'll find in there, | 0:11:13 | 0:11:16 | |
they might still make it. | 0:11:16 | 0:11:17 | |
Let's just hope there's still someone there to save. | 0:11:19 | 0:11:22 | |
That's just a few examples of the artistic licence used by writers and directors | 0:11:24 | 0:11:29 | |
in describing exoplanets. | 0:11:29 | 0:11:32 | |
But what about real life? | 0:11:32 | 0:11:33 | |
How close are we to finding anything like what we see in the movies? | 0:11:33 | 0:11:37 | |
I'm going to go and see exoplanet expert Ruth Angus to find out. | 0:11:37 | 0:11:41 | |
So how realistic are some of these exoplanets that we | 0:11:43 | 0:11:46 | |
see in the movies? | 0:11:46 | 0:11:47 | |
I guess the most famous one is Tatooine in Star Wars, | 0:11:47 | 0:11:50 | |
with its binary star system. | 0:11:50 | 0:11:51 | |
Could something like that happen? | 0:11:51 | 0:11:53 | |
-If so, have we found anything like that? -Yes, absolutely. | 0:11:53 | 0:11:57 | |
We've found more than one, actually. | 0:11:57 | 0:11:58 | |
The first one we found was Kepler-16b, we found it in 2011, | 0:11:58 | 0:12:02 | |
and it's the first circumbinary planet. | 0:12:02 | 0:12:06 | |
So that means it's a binary star, two stars that orbit each other, | 0:12:06 | 0:12:10 | |
and a planet on the outside that orbits both of them. | 0:12:10 | 0:12:13 | |
-So the planet has two stars. -So the stars are orbiting each other, | 0:12:13 | 0:12:16 | |
in a little sort of merry dance, and the planet is going round - oh, wow! | 0:12:16 | 0:12:19 | |
So here's a video of that system and you can see there's the binary | 0:12:19 | 0:12:23 | |
star in the centre, one is a little bit more massive than the other | 0:12:23 | 0:12:26 | |
and it's slightly whiter, and the other is a little red. | 0:12:26 | 0:12:30 | |
Almost exactly like in Star Wars. | 0:12:30 | 0:12:31 | |
It is, it is almost exactly like in Star Wars, yeah. | 0:12:31 | 0:12:34 | |
And is the planet that's orbiting this system, would it be a rocky | 0:12:34 | 0:12:36 | |
planet looking a little bit like Tunisia by any chance? | 0:12:36 | 0:12:41 | |
We should be so lucky! | 0:12:41 | 0:12:42 | |
No, unfortunately, this planet is a Saturn-like planet. | 0:12:42 | 0:12:45 | |
The reason why this is such a benchmark system is | 0:12:45 | 0:12:48 | |
because before we found Kepler-16b, we didn't actually know | 0:12:48 | 0:12:51 | |
whether you could form an exoplanet in a binary system. | 0:12:51 | 0:12:54 | |
And that's because the gravitational pull acting on the planet | 0:12:54 | 0:12:57 | |
varies all the time because these two stars are moving. | 0:12:57 | 0:13:00 | |
So that means that the planet is kind of, like, | 0:13:00 | 0:13:03 | |
walking drunkenly around in space, and if that kind of drunken walk | 0:13:03 | 0:13:07 | |
gets too extreme it's going to spiral inwards and plunge into | 0:13:07 | 0:13:11 | |
-the surface of one of the stars or it will be flung outwards completely. -Right. | 0:13:11 | 0:13:14 | |
So we didn't know whether we would find any planets in stable | 0:13:14 | 0:13:18 | |
orbits around binary stars. | 0:13:18 | 0:13:20 | |
Kepler-16b showed us that they do exist and we can find them. | 0:13:20 | 0:13:23 | |
What about some of these exotic exoplanets that we | 0:13:23 | 0:13:25 | |
see in the movies? | 0:13:25 | 0:13:27 | |
Something like Crematoria, which is | 0:13:27 | 0:13:28 | |
the aptly named planet in The Chronicles Of Riddick. | 0:13:28 | 0:13:31 | |
This sort of extremely hot during the day, extremely cold at night. | 0:13:31 | 0:13:36 | |
Is that just complete fantasy or is that possible? | 0:13:36 | 0:13:39 | |
Well, we have managed to map the temperature on the planet WASP-43b, | 0:13:39 | 0:13:44 | |
so we actually know what the temperature of the day side is | 0:13:44 | 0:13:48 | |
and we know what the temperature of the night side is. | 0:13:48 | 0:13:50 | |
And in this graphic, | 0:13:50 | 0:13:51 | |
we can see in the day it's really hovering up around 1,500 Kelvin, | 0:13:51 | 0:13:57 | |
and in the night it drops all the way back down to, almost to zero. | 0:13:57 | 0:14:02 | |
I find it amazing that we have the technology that enables us | 0:14:02 | 0:14:05 | |
to do that. | 0:14:05 | 0:14:06 | |
One of the things about the planet Miller in Interstellar, | 0:14:06 | 0:14:09 | |
is that it's orbiting a black hole and you get into all | 0:14:09 | 0:14:12 | |
kinds of exotic physics - time dilation and all this sort of stuff. | 0:14:12 | 0:14:16 | |
But the fact that its orbiting a black hole, is, | 0:14:16 | 0:14:18 | |
is a really interesting idea. | 0:14:18 | 0:14:20 | |
Is that at all feasible? | 0:14:20 | 0:14:22 | |
Yeah. | 0:14:22 | 0:14:23 | |
There's no reason why you can't have a planet orbiting a black hole. | 0:14:23 | 0:14:26 | |
And in fact there is some evidence to suggest that we've even | 0:14:26 | 0:14:31 | |
seen a super Jupiter being eaten by a black hole. | 0:14:31 | 0:14:35 | |
Uh, and so this, this graphic shows you. | 0:14:35 | 0:14:38 | |
So this is the planet here | 0:14:38 | 0:14:40 | |
and the black hole is somewhere in here, you can't quite see it, | 0:14:40 | 0:14:44 | |
but material is streaming from the planet onto the black hole. | 0:14:44 | 0:14:48 | |
I'm trying to imagine what you might see, | 0:14:48 | 0:14:50 | |
because obviously a black hole, it's not actually emitting anything. | 0:14:50 | 0:14:53 | |
So what would the view be like? | 0:14:53 | 0:14:55 | |
Well, in this example, you'd see this very bizarre | 0:14:55 | 0:14:57 | |
kind of arc of light stretching from you to the black hole. | 0:14:57 | 0:15:02 | |
So what's that? What is that light? | 0:15:02 | 0:15:04 | |
Where is that light coming from? | 0:15:04 | 0:15:05 | |
That's, that's the dust and gas falling off the planet into | 0:15:05 | 0:15:09 | |
-the black hole and crossing the event horizon. -So the raw materials that we find that makes up planets. | 0:15:09 | 0:15:13 | |
The raw materials, yeah, exactly. | 0:15:13 | 0:15:15 | |
So this material as it's falling into the black hole gets | 0:15:15 | 0:15:18 | |
extremely hot and it starts to give off radiation, it glows. | 0:15:18 | 0:15:22 | |
So you would see the kind of glowing signature | 0:15:22 | 0:15:25 | |
of this accreting material. | 0:15:25 | 0:15:27 | |
Do science fiction writers, are they creative enough, do you think? | 0:15:27 | 0:15:30 | |
Do you think they are slightly limited by their own imagination? | 0:15:30 | 0:15:33 | |
And actually what's really interesting is the stuff that's actually out there? | 0:15:33 | 0:15:36 | |
Things like, uh, you know, a super Jupiter being eaten by a black hole | 0:15:36 | 0:15:40 | |
and a planet made of diamonds and this sort of stuff? | 0:15:40 | 0:15:43 | |
I'm sure that's true. The old expression "stranger than fiction" | 0:15:43 | 0:15:46 | |
is absolutely applicable to exoplanets. | 0:15:46 | 0:15:48 | |
There are lots of things that we've found that are stranger than things we can imagine | 0:15:48 | 0:15:51 | |
and that's the beauty of the exoplanet world - we are discovering things we didn't even | 0:15:51 | 0:15:55 | |
know were possible and new physics is being discovered all the time. | 0:15:55 | 0:15:58 | |
Thank you very much, that was fascinating. | 0:15:58 | 0:16:00 | |
One of the greatest success stories in exoplanet research has been | 0:16:07 | 0:16:10 | |
Nasa's Kepler space telescope. | 0:16:10 | 0:16:12 | |
It has found over half of the exoplanets we know about today. | 0:16:12 | 0:16:17 | |
Five, four, three, two... | 0:16:17 | 0:16:20 | |
engine start. | 0:16:20 | 0:16:21 | |
One, zero, and lift off of the Delta Two rocket with Kepler, | 0:16:21 | 0:16:27 | |
on a search for planets in some way like our own. | 0:16:27 | 0:16:30 | |
Kepler was launched in March 2009. | 0:16:32 | 0:16:34 | |
Its mission was to survey our region of the Milky Way, | 0:16:34 | 0:16:38 | |
to try and find another Earth. | 0:16:38 | 0:16:40 | |
And it's discovered more than a thousand planets. | 0:16:42 | 0:16:45 | |
One of most interesting findings of the Kepler space mission | 0:16:47 | 0:16:49 | |
to date has been the discovery of a class of planet | 0:16:49 | 0:16:52 | |
known as "Super Earths". | 0:16:52 | 0:16:54 | |
They seem to be fairly common throughout the galaxy | 0:16:54 | 0:16:57 | |
and yet none exist within our own solar system. | 0:16:57 | 0:17:00 | |
They're larger than Earth but smaller than an icy giant. | 0:17:00 | 0:17:03 | |
We don't know what they're made of. Are they rocky or icy? | 0:17:03 | 0:17:07 | |
It remains a mystery, at least for now. | 0:17:07 | 0:17:09 | |
Perhaps even more exciting is the recent discovery of | 0:17:11 | 0:17:14 | |
Kepler-452b, 1,400 light years away. | 0:17:14 | 0:17:18 | |
It's probably the most earthlike planet we've found so far. | 0:17:18 | 0:17:22 | |
It's a rocky world that's orbiting in the habitable zone | 0:17:22 | 0:17:25 | |
of its parent star, where there could be liquid water. | 0:17:25 | 0:17:29 | |
But there's still a lot we don't know about the planet, | 0:17:29 | 0:17:32 | |
for example what its atmosphere is made of. | 0:17:32 | 0:17:35 | |
Kepler has done a tremendous job in finding | 0:17:37 | 0:17:39 | |
exoplanets virtually everywhere it's looked, but it's not designed to | 0:17:39 | 0:17:44 | |
give us the detailed information to tell us what those planets would be like. | 0:17:44 | 0:17:48 | |
Our best bet for finding another Earth is to build | 0:17:48 | 0:17:51 | |
new instruments that can take a closer look. | 0:17:51 | 0:17:53 | |
That's what Nasa is doing. | 0:17:55 | 0:17:58 | |
Its Tess planet finder launches in just two years' time. | 0:17:58 | 0:18:01 | |
Its mission is to detect small planets orbiting bright host stars. | 0:18:03 | 0:18:07 | |
Bright stars will reveal more detailed | 0:18:09 | 0:18:11 | |
information about their planets, enabling us | 0:18:11 | 0:18:14 | |
to better identify those that are truly earthlike. | 0:18:14 | 0:18:17 | |
Of course, the ultimate prize isn't just | 0:18:22 | 0:18:25 | |
finding a planet that is like Earth, it's finding intelligent life. | 0:18:25 | 0:18:30 | |
We don't really know how that would manifest itself, | 0:18:31 | 0:18:34 | |
but Chris has recently been involved in a discovery that has got | 0:18:34 | 0:18:37 | |
some people very excited. | 0:18:37 | 0:18:39 | |
I don't normally talk about my own research on the programme, | 0:18:41 | 0:18:43 | |
but in the last few weeks we've announced a remarkable, strange discovery, | 0:18:43 | 0:18:47 | |
probably the strangest thing we've seen in the universe in the last 20 years. | 0:18:47 | 0:18:52 | |
And according to the internet and the newspapers we've discovered | 0:18:52 | 0:18:55 | |
alien spaceships in orbit around a star 1,500 light years away. | 0:18:55 | 0:19:00 | |
That's not quite what happened. | 0:19:00 | 0:19:02 | |
We've been running a project for the last few years called Planet Hunters | 0:19:02 | 0:19:05 | |
which has invited hundreds of thousands of people to go online | 0:19:05 | 0:19:09 | |
and to look through this data from Kepler and try and find planets. | 0:19:09 | 0:19:13 | |
And we've found planets, but a few of the volunteers pointed us | 0:19:13 | 0:19:17 | |
to this one particular star which is behaving really oddly. | 0:19:17 | 0:19:20 | |
This is its brightness over the course of three or four years. | 0:19:20 | 0:19:25 | |
You can see most of the time it's fairly stable, | 0:19:25 | 0:19:28 | |
but there are these dips. | 0:19:28 | 0:19:29 | |
Just like you'd expect if there was a planet, | 0:19:29 | 0:19:31 | |
but the dips happen randomly, | 0:19:31 | 0:19:33 | |
some of them are huge, | 0:19:33 | 0:19:34 | |
so at one point something blocks out 20% of the star's light. | 0:19:34 | 0:19:38 | |
That's way too much for this to be a normal planet | 0:19:38 | 0:19:41 | |
and the fact that they're irregular means this can't be something | 0:19:41 | 0:19:44 | |
on a circular orbit that blocks out the star's light again and again and again. | 0:19:44 | 0:19:48 | |
Something really odd is going on here. | 0:19:48 | 0:19:50 | |
In fact, this is the only star amongst the 150,000 | 0:19:50 | 0:19:54 | |
that's doing anything like this. | 0:19:54 | 0:19:56 | |
So the obvious question is what's blocking the light from the star? | 0:19:56 | 0:19:59 | |
We think this might be not exoplanets, | 0:19:59 | 0:20:01 | |
but a family of exocomets. | 0:20:01 | 0:20:04 | |
If you have a comet on an elliptical orbit about the star | 0:20:04 | 0:20:08 | |
AND that comet has broken up, so that you have a string of comets - | 0:20:08 | 0:20:12 | |
rather like what happened to Shoemaker-Levy 9 | 0:20:12 | 0:20:15 | |
when it hit Jupiter a couple of decades ago - | 0:20:15 | 0:20:17 | |
then, as each of those pieces of comet pass by the star, | 0:20:17 | 0:20:21 | |
we'd see a dip. | 0:20:21 | 0:20:22 | |
And so you see there's one here, there's one here, | 0:20:22 | 0:20:25 | |
and then this sudden flurry of large bits that block light out. | 0:20:25 | 0:20:29 | |
But we don't really understand what's going on and | 0:20:29 | 0:20:31 | |
so we should consider everything, | 0:20:31 | 0:20:33 | |
including the idea that this is some sort of alien civilisation. | 0:20:33 | 0:20:37 | |
In fact, people are taking the idea so seriously, | 0:20:37 | 0:20:41 | |
that astronomers have already pointed radio telescopes at | 0:20:41 | 0:20:44 | |
this star just to listen out, Seti-style, for any signals | 0:20:44 | 0:20:47 | |
that might be coming our way from what's become the most interesting star in the galaxy. | 0:20:47 | 0:20:52 | |
When it comes to finding exoplanets, | 0:21:00 | 0:21:02 | |
you need more than even the best home telescope. | 0:21:02 | 0:21:06 | |
But Pete's here to show us | 0:21:06 | 0:21:07 | |
another way we can all connect with the thrill of exoplanet discovery. | 0:21:07 | 0:21:11 | |
It's actually not too bad an evening, | 0:21:12 | 0:21:14 | |
it started off rather cloudy today but the skies have cleared | 0:21:14 | 0:21:18 | |
and I can see some stars shining away up there, | 0:21:18 | 0:21:21 | |
there's a bit of haze in the west, but that was forecast to come in. | 0:21:21 | 0:21:24 | |
I'm just glad we can see some stars. | 0:21:24 | 0:21:25 | |
What I'm looking for is a huge pattern in the sky that | 0:21:25 | 0:21:29 | |
looks like a giant square, and that's the square of Pegasus. | 0:21:29 | 0:21:33 | |
And early evening about this time of year, it's quite high up | 0:21:33 | 0:21:37 | |
in the sky towards the south-east direction. | 0:21:37 | 0:21:41 | |
It's pretty prominent, just look for this giant square. | 0:21:41 | 0:21:44 | |
Once you've located it, look to the right-hand side of the square. | 0:21:44 | 0:21:49 | |
Close to the mid point there is a faint star, | 0:21:49 | 0:21:52 | |
and that's called 51 Pegasi. | 0:21:52 | 0:21:53 | |
OK, well, I think I have a photograph of 51 Pegasi there, | 0:21:57 | 0:22:00 | |
and of course on the back of my camera it'll look just like a regular star. | 0:22:00 | 0:22:04 | |
The planet is there, we know it's there, it's been detected | 0:22:04 | 0:22:07 | |
and confirmed by a number of different sources. | 0:22:07 | 0:22:10 | |
The planet going around 51 Pegasi has a name, it's formal name is | 0:22:10 | 0:22:14 | |
51 Pegasi b, but there is an unofficial name as well, which is Bellerophon. | 0:22:14 | 0:22:18 | |
Now Bellerophon in mythology was the person that tamed the flying horse | 0:22:18 | 0:22:23 | |
Pegasus, so it's rather nice being in the constellation of Pegasus itself. | 0:22:23 | 0:22:27 | |
So, I think with exoplanets and regular telescopes it's really | 0:22:28 | 0:22:33 | |
a journey of the imagination, you can see the star there | 0:22:33 | 0:22:36 | |
through the eyepiece or on the back of the camera, but it's your | 0:22:36 | 0:22:39 | |
mind that takes you into that system to imagine what it must look like. | 0:22:39 | 0:22:44 | |
Absolutely fantastic. | 0:22:44 | 0:22:46 | |
Go to the website to find out more about how to locate 51 Pegasi, | 0:22:48 | 0:22:51 | |
to see this month's Star Guide, and also to learn about an exciting | 0:22:51 | 0:22:56 | |
new project The Sky At Night has been involved in. | 0:22:56 | 0:22:58 | |
This month, we're trying out a brand-new BBC messaging tool | 0:23:00 | 0:23:04 | |
called Whispering Stars. | 0:23:04 | 0:23:06 | |
It's a prototype at the moment but we'd love you to have a go. | 0:23:06 | 0:23:10 | |
On the star map, you can click on any star with a circle round it. | 0:23:10 | 0:23:14 | |
Not only will you see information from Pete about that star, | 0:23:14 | 0:23:17 | |
but you can also leave your own message. | 0:23:17 | 0:23:20 | |
Then I can share a link to that message via e-mail or social media. | 0:23:21 | 0:23:25 | |
The recipient can find your message using a computer or a smartphone. | 0:23:26 | 0:23:30 | |
I've got a new message, just have to click to find it | 0:23:31 | 0:23:34 | |
and it points me up into the sky towards whichever star | 0:23:34 | 0:23:38 | |
the message is attached to, | 0:23:38 | 0:23:39 | |
so apparently I should keep going. | 0:23:39 | 0:23:41 | |
Back this way, it's this one here, | 0:23:41 | 0:23:43 | |
which looks like it is...Vega. | 0:23:43 | 0:23:47 | |
And here's the message from Maggie, which says, | 0:23:47 | 0:23:50 | |
"Dear Chris, I know you like astrophotography | 0:23:50 | 0:23:52 | |
"but did you know that Vega was the first star to be photographed?" | 0:23:52 | 0:23:56 | |
So a message sent through the stars - sort of - and you can go to our | 0:23:56 | 0:24:00 | |
website at bbc.co.uk/skyatnight to use Whispering Stars for yourself. | 0:24:00 | 0:24:05 | |
We'll be using it to try and send you information over the next few months. | 0:24:05 | 0:24:09 | |
Even if we find another rocky planet, just like ours, | 0:24:16 | 0:24:19 | |
orbiting a star similar to ours, even orbiting at the right distance, | 0:24:19 | 0:24:24 | |
there's another piece of information | 0:24:24 | 0:24:26 | |
we need before we can confirm we've found another Earth. | 0:24:26 | 0:24:29 | |
And that information is the atmospheric composition of that exoplanet. | 0:24:29 | 0:24:33 | |
And rather astonishingly, we're doing just that. | 0:24:33 | 0:24:36 | |
Chris has been talking to Nikku Madhusudhan, who is leading | 0:24:36 | 0:24:40 | |
the research into exoplanet atmospheres here at Cambridge. | 0:24:40 | 0:24:44 | |
So we've discovered all of these planets, we know, I dunno, | 0:24:44 | 0:24:47 | |
what size they are, what mass they are, but it's not really enough. | 0:24:47 | 0:24:50 | |
I want to know what they're like. | 0:24:50 | 0:24:51 | |
Do we have any prospect of trying to understand that? | 0:24:51 | 0:24:54 | |
-To, to investigating these planets properly? -No, absolutely. | 0:24:54 | 0:24:57 | |
So the way you do that is, you know, transiting planets, for example, | 0:24:57 | 0:25:00 | |
what the transit method is | 0:25:00 | 0:25:02 | |
is when the planet's star system is aligned | 0:25:02 | 0:25:04 | |
in such a way that you can infer the planet going in front of the star. | 0:25:04 | 0:25:09 | |
-Yeah, we see these dips in the star light. -Exactly. | 0:25:09 | 0:25:11 | |
And we say, OK, there's a planet there. | 0:25:11 | 0:25:13 | |
As it turns out, the dip in the starlight is just a little | 0:25:13 | 0:25:16 | |
bit more if you have an atmosphere on top of the planet. | 0:25:16 | 0:25:19 | |
Because the atmosphere blocks the light from the star as well. | 0:25:19 | 0:25:22 | |
Yeah, yeah, but the key point is that the atmosphere blocks | 0:25:22 | 0:25:25 | |
the light in some wavelengths and not in others. | 0:25:25 | 0:25:28 | |
And so that means if you have a transiting planet you can say | 0:25:28 | 0:25:31 | |
something about what its atmosphere is made of? | 0:25:31 | 0:25:33 | |
Exactly, you can infer its chemical composition. | 0:25:33 | 0:25:36 | |
OK, so Earth is mostly nitrogen, bit of oxygen, | 0:25:36 | 0:25:38 | |
bit of carbon dioxide, what do we see on these exoplanets? | 0:25:38 | 0:25:41 | |
Yep, so the exoplanets, um, that we are most | 0:25:41 | 0:25:45 | |
able to study today are the big and hot ones. | 0:25:45 | 0:25:49 | |
It's because the bigger the planet, | 0:25:49 | 0:25:50 | |
the bigger the starlight you're blocking. | 0:25:50 | 0:25:52 | |
Yeah, the bigger the dip. | 0:25:52 | 0:25:54 | |
The bigger the dip, so it's just easier to find them. | 0:25:54 | 0:25:56 | |
And hot because the hotter the atmosphere is the more | 0:25:56 | 0:26:00 | |
-puffier it is. -Hm. -Right, so, so the bigger it is. | 0:26:00 | 0:26:05 | |
So the hotter the atmosphere, the bigger the atmosphere, and the more light it blocks. | 0:26:05 | 0:26:09 | |
Right, so most of the results to date have come from these | 0:26:09 | 0:26:13 | |
objects called hot Jupiters. | 0:26:13 | 0:26:14 | |
What do we know about the conditions? | 0:26:14 | 0:26:16 | |
We know they're large, that means they must be made of gas, mostly. | 0:26:16 | 0:26:19 | |
-What do we know about the atmosphere? -We are finding less water than we would expect | 0:26:19 | 0:26:24 | |
if the planets formed in a solar-like environment | 0:26:24 | 0:26:27 | |
-Oh, OK. -And they could be less by even a factor of ten. | 0:26:27 | 0:26:31 | |
One explanation is that maybe these objects have clouds in their atmospheres. | 0:26:31 | 0:26:37 | |
So you're, you're saying the water would be hidden? By the clouds? | 0:26:37 | 0:26:40 | |
-Yeah, exactly. -So you only see the bit of the atmosphere above the clouds? | 0:26:40 | 0:26:44 | |
-Exactly, so, so that's one way. -So it's a straightforward explanation - | 0:26:44 | 0:26:48 | |
astronomers being confused by clouds is common here on Earth as well. | 0:26:48 | 0:26:52 | |
It's not only on Earth, not only a terrestrial experience, | 0:26:52 | 0:26:55 | |
even when you go to exoplanets clouds are a headache. | 0:26:55 | 0:26:58 | |
But there is a subtlety. | 0:26:58 | 0:26:59 | |
Clouds are not the same clouds we have here. | 0:26:59 | 0:27:03 | |
Right, so on Earth they are water clouds. | 0:27:03 | 0:27:05 | |
-But these are planets at a few thousand degrees. -Of course, so... | 0:27:05 | 0:27:09 | |
So you can't have water clouds. | 0:27:09 | 0:27:11 | |
So you may have to invoke iron clouds, | 0:27:11 | 0:27:14 | |
or silicate clouds, you see it in rocks, | 0:27:14 | 0:27:16 | |
on Earth rocks are made of silicates, | 0:27:16 | 0:27:19 | |
so you might be able to make | 0:27:19 | 0:27:20 | |
clouds out of those same silicates, hanging up in the atmosphere. | 0:27:20 | 0:27:24 | |
Wow, suddenly it's a place to me, | 0:27:24 | 0:27:25 | |
because we are talking about what they're like. | 0:27:25 | 0:27:28 | |
I can, I sort of feel they're real. | 0:27:28 | 0:27:30 | |
-Yeah. -Remarkable stuff, and we'll come back | 0:27:30 | 0:27:32 | |
and see how you're getting on in a few years perhaps. | 0:27:32 | 0:27:34 | |
-Thank you very much. -Thank you, thank you. | 0:27:34 | 0:27:37 | |
It's amazing we've come so far in just 20 years. | 0:27:37 | 0:27:40 | |
Going from no exoplanets to about 2,000 now! | 0:27:40 | 0:27:42 | |
And turning them from just points on a graph, from just data, | 0:27:42 | 0:27:45 | |
to real places with atmospheres, and rain, | 0:27:45 | 0:27:49 | |
and even clouds to annoy the astronomers! | 0:27:49 | 0:27:52 | |
What I'm fascinated by, is if we did find an earthlike planet, | 0:27:52 | 0:27:55 | |
I mean, even signs of life, what would we do then? | 0:27:55 | 0:27:57 | |
We'd have to go, wouldn't we? | 0:27:57 | 0:27:59 | |
If you looked at the sky and you could say that star has an earthlike planet, | 0:27:59 | 0:28:02 | |
the right temperature, with life in its atmosphere - you'd have to send a probe. | 0:28:02 | 0:28:06 | |
-It'd take thousands of years to get there! -We still should send something, I mean, maybe not us, | 0:28:06 | 0:28:10 | |
-but we should send something just so we know we're on our way. -I have to agree, you're right! | 0:28:10 | 0:28:14 | |
That's it for this month. Next month we have a Christmas special! | 0:28:19 | 0:28:22 | |
We'll be taking an astronomical look at the mystery surrounding | 0:28:22 | 0:28:25 | |
the Star of Bethlehem. | 0:28:25 | 0:28:27 | |
Was it just a conjunction of planets | 0:28:27 | 0:28:29 | |
or something more exciting like a comet, | 0:28:29 | 0:28:31 | |
or a supernova? | 0:28:31 | 0:28:32 | |
In the meanwhile, get outside and get looking up. | 0:28:32 | 0:28:36 | |
Goodnight. | 0:28:36 | 0:28:37 |