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The Universe is filled with beautiful objects - | 0:00:02 | 0:00:06 | |
from shining stars, to amazing clusters of galaxies, | 0:00:06 | 0:00:10 | |
to clouds of gas and dust - | 0:00:10 | 0:00:13 | |
and one force has created them all. | 0:00:13 | 0:00:16 | |
Gravity. | 0:00:16 | 0:00:17 | |
This month, we're looking at how the wonderful shapes | 0:00:19 | 0:00:22 | |
and spectacular structures we see in the Universe have been created. | 0:00:22 | 0:00:25 | |
Welcome to The Sky At Night. | 0:00:25 | 0:00:27 | |
MUSIC: "Pelleas and Melisande: At the Castle Gate" by Sibelius | 0:00:27 | 0:00:31 | |
Spring is finally here and the nights are warmer, at least in theory, | 0:00:52 | 0:00:56 | |
and we've escaped the bright lights of the city to come and join | 0:00:56 | 0:00:59 | |
this rowdy bunch of amateur astronomers | 0:00:59 | 0:01:01 | |
at the Brecon Beacons AstroCamp. | 0:01:01 | 0:01:04 | |
Keen astronomers have come from hundreds of miles away | 0:01:06 | 0:01:09 | |
and they're setting up camp | 0:01:09 | 0:01:10 | |
in the hope of using the coming darkness | 0:01:10 | 0:01:14 | |
to see deep into the night sky. | 0:01:14 | 0:01:16 | |
Of course, being Britain, the weather isn't on our side | 0:01:17 | 0:01:20 | |
and it's pretty cloudy but we're hoping | 0:01:20 | 0:01:22 | |
there'll be some breaks in the cloud later on. | 0:01:22 | 0:01:25 | |
Whatever the weather, | 0:01:25 | 0:01:26 | |
we're going to use the time to explore the extraordinary ways | 0:01:26 | 0:01:29 | |
in which gravity shapes the objects in the night sky. | 0:01:29 | 0:01:33 | |
Coming up, I'll be finding out | 0:01:33 | 0:01:36 | |
how gravity makes stars and planets round. | 0:01:36 | 0:01:39 | |
And why, despite the power of this force, | 0:01:39 | 0:01:41 | |
they're often not as round as they seem. | 0:01:41 | 0:01:44 | |
Chris North and Jon Culshaw are here | 0:01:45 | 0:01:48 | |
and they'll be taking us on an intergalactic tour | 0:01:48 | 0:01:51 | |
to show us how gravity sculpts each and every galaxy. | 0:01:51 | 0:01:55 | |
And we'll be seeing gravity in action right now, | 0:01:58 | 0:02:01 | |
as it creates an extraordinary drama in Saturn's rings. | 0:02:01 | 0:02:04 | |
This is the first time | 0:02:06 | 0:02:07 | |
that we've ever seen anything like this. | 0:02:07 | 0:02:09 | |
Plus Pete Lawrence and some campers will be showing us | 0:02:09 | 0:02:13 | |
simple tricks to capture star trails. | 0:02:13 | 0:02:16 | |
Oh, that's amazing! | 0:02:16 | 0:02:18 | |
As darkness sets in, | 0:02:22 | 0:02:23 | |
we're still waiting for the clouds to properly break. | 0:02:23 | 0:02:27 | |
But some bright stars and planets, like Mars, are shining through. | 0:02:27 | 0:02:31 | |
So while we wait and hope, here's Paul Abel | 0:02:31 | 0:02:34 | |
with a guide to what it's possible to see | 0:02:34 | 0:02:37 | |
if we embrace the dark and if the skies are clear. | 0:02:37 | 0:02:40 | |
Well, here we are in Wales in a lovely dark site. | 0:02:40 | 0:02:44 | |
And viewing the night sky from a place like this | 0:02:44 | 0:02:46 | |
is really very different from viewing it from a town centre. | 0:02:46 | 0:02:49 | |
The main reason for that is there's very little light pollution here. | 0:02:49 | 0:02:52 | |
Another significant reason is that our eyes can become | 0:02:52 | 0:02:56 | |
very dark adapted in sites like this. | 0:02:56 | 0:02:58 | |
The reason we have dark adaption is | 0:02:58 | 0:03:00 | |
because our eyes manufacture a chemical called rhodopsin | 0:03:00 | 0:03:04 | |
which allows us to see in the dark. | 0:03:04 | 0:03:06 | |
Unfortunately, that chemical | 0:03:06 | 0:03:08 | |
is completely destroyed by bright, white light. | 0:03:08 | 0:03:11 | |
You can experience all of this for yourself. | 0:03:11 | 0:03:14 | |
The first thing you'll notice when you step out into a dark sky | 0:03:14 | 0:03:17 | |
are the bright objects in the sky like the moon or the planets - | 0:03:17 | 0:03:20 | |
Mars and Jupiter we have around at the moment. | 0:03:20 | 0:03:23 | |
Later on, you'll notice the bright stars, | 0:03:23 | 0:03:26 | |
like Arcturus, shining away up there. | 0:03:26 | 0:03:28 | |
After 10 or 15 minutes, | 0:03:28 | 0:03:29 | |
you'll notice the fainter stars that make out the main constellations. | 0:03:29 | 0:03:32 | |
Like the faint stars that mark out the handle of the Plough. | 0:03:32 | 0:03:35 | |
After 25 to 30 minutes, | 0:03:38 | 0:03:39 | |
you become totally dark adapted. | 0:03:39 | 0:03:41 | |
And in a dark sky like this, the sky is literally | 0:03:41 | 0:03:44 | |
ablaze with stars. | 0:03:44 | 0:03:46 | |
But perhaps | 0:03:49 | 0:03:50 | |
the most impressive thing is the sight of the Milky Way running down | 0:03:50 | 0:03:54 | |
through the constellations. | 0:03:54 | 0:03:56 | |
You can use exactly the same process for getting the most out of your | 0:03:58 | 0:04:02 | |
telescope because the more you look, the better you'll be able to see. | 0:04:02 | 0:04:06 | |
If we take Saturn for example, | 0:04:06 | 0:04:07 | |
initially the view is not too impressive. | 0:04:07 | 0:04:10 | |
We notice it's a planet surrounded by a ring system | 0:04:10 | 0:04:12 | |
but after five minutes, | 0:04:12 | 0:04:14 | |
the subtleties of Saturn start to come out. | 0:04:14 | 0:04:16 | |
We notice the delicate cloud bands, the pastel hues, the brighter zones, | 0:04:16 | 0:04:20 | |
and the rings themselves take on more of a 3-D effect. | 0:04:20 | 0:04:24 | |
So the moral of the story is, in order to get the best views | 0:04:24 | 0:04:27 | |
out of your telescope, spend as much time as you can looking. | 0:04:27 | 0:04:31 | |
Frustratingly we are still not getting | 0:04:33 | 0:04:36 | |
any decent holes in the clouds. | 0:04:36 | 0:04:38 | |
So let's take a look at the awesome creative power of gravity. | 0:04:38 | 0:04:41 | |
Now whatever you look at in the night sky, whether it's a star or a planet, | 0:04:41 | 0:04:45 | |
you're looking at an object that's basically a sphere. | 0:04:45 | 0:04:49 | |
The sphere is the most common shape in the Universe. | 0:04:49 | 0:04:51 | |
But when it comes to the cosmos, a sphere isn't always what it seems. | 0:04:51 | 0:04:55 | |
Perfect spheres are actually surprisingly rare in space. | 0:04:56 | 0:05:00 | |
To understand how gravity forms spheres, | 0:05:00 | 0:05:03 | |
and why they're often not perfect, you have to start with | 0:05:03 | 0:05:06 | |
how objects like stars and planets form out of stardust. | 0:05:06 | 0:05:10 | |
It's gravity that caused the planets to form in the first place. | 0:05:12 | 0:05:16 | |
But gravity is also the key to their spherical shape. | 0:05:16 | 0:05:19 | |
Let's imagine that these sugar cubes are lumps of rock | 0:05:20 | 0:05:23 | |
in the early Solar System | 0:05:23 | 0:05:25 | |
orbiting a young sun some 4.6 billion years ago. | 0:05:25 | 0:05:29 | |
Gravity pulls them towards each other | 0:05:29 | 0:05:31 | |
but gravity has no preferred direction. | 0:05:31 | 0:05:33 | |
So they come in from here, from here, from here, | 0:05:33 | 0:05:37 | |
from all over. | 0:05:37 | 0:05:38 | |
The shape you end up with | 0:05:38 | 0:05:40 | |
is the only shape that looks the same from every direction. | 0:05:40 | 0:05:43 | |
A sphere. | 0:05:43 | 0:05:45 | |
Gravity created the blue planet we call home. | 0:05:46 | 0:05:50 | |
But although it may look flawless, our planet is not perfect. | 0:05:50 | 0:05:54 | |
Imagine I start at the equator | 0:05:56 | 0:05:58 | |
and I walk all the way round the Earth. | 0:05:58 | 0:06:00 | |
By the time I get back to the beginning, | 0:06:00 | 0:06:02 | |
I would have walked 40,000km. | 0:06:02 | 0:06:04 | |
But let's say I do the same thing, but this time pole to pole. | 0:06:04 | 0:06:08 | |
By the time I get back to the beginning, | 0:06:08 | 0:06:10 | |
I would actually have walked around 130km less. | 0:06:10 | 0:06:14 | |
That's because the Earth isn't a perfect sphere. | 0:06:14 | 0:06:17 | |
It's actually a bit fatter in the middle. | 0:06:17 | 0:06:19 | |
And it's not just Earth. | 0:06:21 | 0:06:23 | |
Most of the planets in our solar system | 0:06:23 | 0:06:25 | |
also have a bulge around the equator. | 0:06:25 | 0:06:28 | |
The reason some planets grow a bit fat around the middle | 0:06:31 | 0:06:34 | |
is because of the way they rotate on their axes. | 0:06:34 | 0:06:38 | |
It's because of the phenomenon we can experience here on Earth. | 0:06:40 | 0:06:43 | |
Spinning something causes it to be thrown outwards, | 0:06:43 | 0:06:46 | |
away from the centre. | 0:06:46 | 0:06:47 | |
These chains are the only things that are keeping me | 0:06:49 | 0:06:52 | |
and this chair from flying off into the distance. | 0:06:52 | 0:06:54 | |
The same thing happens to a planet when it spins. | 0:06:57 | 0:07:00 | |
Gravity acts like the chains, pulling everything inwards. | 0:07:00 | 0:07:03 | |
But the speed of rotation pushes everything outwards. | 0:07:03 | 0:07:06 | |
Just like the chairs on this ride, | 0:07:09 | 0:07:10 | |
as a planet rotates on its axis it grows wider around the middle. | 0:07:10 | 0:07:15 | |
And, of course, the faster we go, the greater the effect. | 0:07:16 | 0:07:19 | |
In our Solar System, Jupiter spins the fastest | 0:07:25 | 0:07:28 | |
taking just ten hours to complete one rotation | 0:07:28 | 0:07:31 | |
and therefore it has an enormous bulge. | 0:07:31 | 0:07:34 | |
Its circumference is 29,000km greater | 0:07:34 | 0:07:38 | |
when measured around the equator rather than the poles. | 0:07:38 | 0:07:41 | |
Venus spins the slowest. A day on Venus is 243 Earth days. | 0:07:42 | 0:07:48 | |
As a result, Venus has no bulge at all | 0:07:48 | 0:07:51 | |
and is close to a perfect sphere. | 0:07:51 | 0:07:53 | |
In general, the faster the spin, the bigger the bulge. | 0:07:56 | 0:08:00 | |
But there is one rather big exception to the rule | 0:08:01 | 0:08:04 | |
that we still don't fully understand. | 0:08:04 | 0:08:06 | |
Our sun is very large and it rotates at nearly 7,000km/hr. | 0:08:08 | 0:08:14 | |
That's incredibly fast | 0:08:14 | 0:08:16 | |
so you'd expect it to have a bulge but it doesn't. | 0:08:16 | 0:08:19 | |
It's an almost perfect sphere. | 0:08:19 | 0:08:22 | |
This astonishing discovery was only made in 2012 as a result of | 0:08:22 | 0:08:28 | |
the most detailed measurements of the sun that have ever been taken. | 0:08:28 | 0:08:32 | |
Dr Chris Scott is a solar expert and a space scientist. | 0:08:34 | 0:08:37 | |
He's been trying to understand | 0:08:37 | 0:08:39 | |
this intriguing mystery on our astronomical doorstep. | 0:08:39 | 0:08:42 | |
So why did it take so long to get this measurement? | 0:08:44 | 0:08:47 | |
It's a very difficult measurement to make. When you get up into space, | 0:08:47 | 0:08:50 | |
you can see the sun and its atmosphere | 0:08:50 | 0:08:51 | |
and it's not smooth. | 0:08:51 | 0:08:53 | |
There are eruptions of material off the surface of the sun | 0:08:53 | 0:08:56 | |
all of the time. | 0:08:56 | 0:08:57 | |
The new spacecraft that's enabled these measurements is called | 0:08:57 | 0:09:00 | |
the Solar Dynamics Observatory. | 0:09:00 | 0:09:01 | |
It's a solar telescope that's in orbit around the Earth, | 0:09:01 | 0:09:04 | |
so it's sending back something like 15,000 images a day. | 0:09:04 | 0:09:08 | |
These images it's taking are ten times HD resolution. | 0:09:08 | 0:09:11 | |
We've been able to work out that the sun is much, | 0:09:11 | 0:09:14 | |
much rounder than it has any right to be. | 0:09:14 | 0:09:16 | |
So what do you think is causing this result? | 0:09:16 | 0:09:18 | |
Well, it's another force of some sort | 0:09:18 | 0:09:20 | |
that's got to be stopping it from bulging. | 0:09:20 | 0:09:23 | |
So the theories have been perhaps that the poles | 0:09:23 | 0:09:25 | |
would be slightly hotter and so maybe would expand out | 0:09:25 | 0:09:28 | |
a little bit more so that would even up the difference. | 0:09:28 | 0:09:31 | |
It seems unlikely that it's just the right temperature | 0:09:31 | 0:09:33 | |
-to make it spherical. -Indeed. There's no evidence that there is | 0:09:33 | 0:09:36 | |
this temperature difference. It could be a magnetic field. | 0:09:36 | 0:09:38 | |
We know that the sun has a strong magnetic field, | 0:09:38 | 0:09:40 | |
it comes out of the sun at the north and south poles. | 0:09:40 | 0:09:43 | |
Could there be some concentration of magnetic field | 0:09:43 | 0:09:45 | |
that is stopping the material, | 0:09:45 | 0:09:47 | |
like an electromagnet on the fairground ride pulling the cars in? | 0:09:47 | 0:09:50 | |
Is there some force that's stopping the material from bulging out? | 0:09:50 | 0:09:53 | |
And again, there doesn't seem to be much evidence | 0:09:53 | 0:09:55 | |
that there's that strong a force. | 0:09:55 | 0:09:57 | |
So perhaps it's something in the solar interior. | 0:09:57 | 0:09:59 | |
Perhaps some part of the solar interior | 0:09:59 | 0:10:01 | |
isn't rotating as fast as we thought it was. | 0:10:01 | 0:10:03 | |
Or perhaps there's some kind of stresses going on | 0:10:03 | 0:10:05 | |
between the different layers to distribute the mass of the sun | 0:10:05 | 0:10:08 | |
in a different way from how we thought. | 0:10:08 | 0:10:11 | |
In a previous programme, | 0:10:11 | 0:10:12 | |
we looked at the sounds travelling through the sun. | 0:10:12 | 0:10:14 | |
-Do we need something like that to try and solve this mystery? -Yes. | 0:10:14 | 0:10:18 | |
It's a really cunning technique called helioseismology. | 0:10:18 | 0:10:20 | |
And it's looking at the interior of the sun by using these | 0:10:20 | 0:10:23 | |
shock waves from the explosions in the sun's atmosphere. | 0:10:23 | 0:10:26 | |
And just like we can use earthquakes on Earth to study | 0:10:26 | 0:10:29 | |
the interior of the Earth, you can do the same thing on the sun | 0:10:29 | 0:10:32 | |
by looking to see how long it takes shockwaves to propagate through | 0:10:32 | 0:10:35 | |
and that tells you something about the solar interior. | 0:10:35 | 0:10:38 | |
We've been using this technique for some time now and clearly | 0:10:38 | 0:10:42 | |
the answer is in there somewhere but we didn't know to look before. | 0:10:42 | 0:10:45 | |
-Now we know to look. -Thanks very much, Chris. | 0:10:45 | 0:10:48 | |
So we'll have to wait to resolve this particular mystery. | 0:10:48 | 0:10:53 | |
Although gravity is the master sculptor shaping the planets | 0:10:53 | 0:10:57 | |
and the stars, there are other factors at work, | 0:10:57 | 0:11:00 | |
some of which we don't yet fully understand. | 0:11:00 | 0:11:03 | |
But what fascinates me is that something as simple | 0:11:03 | 0:11:06 | |
as an object's shape can reveal so much about it. | 0:11:06 | 0:11:09 | |
Back at AstroCamp, | 0:11:15 | 0:11:17 | |
we can just see some stars poking through the odd holes in the clouds. | 0:11:17 | 0:11:21 | |
If it were a little clearer we could train our telescopes | 0:11:21 | 0:11:24 | |
on some objects shaped in different ways by gravity. | 0:11:24 | 0:11:27 | |
There are two very special objects | 0:11:28 | 0:11:30 | |
to see in our night skies this month. | 0:11:30 | 0:11:32 | |
The dwarf planet Ceres and the minor planet Vesta. | 0:11:33 | 0:11:37 | |
These two unsung heroes of our solar system lie between Mars and Jupiter. | 0:11:37 | 0:11:42 | |
But what makes them fascinating is their relative sizes, | 0:11:42 | 0:11:46 | |
which means they sit either side of a very significant divide. | 0:11:46 | 0:11:49 | |
At about 1,000km across, Ceres has enough mass | 0:11:51 | 0:11:54 | |
for gravity to have carved it into a smooth sphere. | 0:11:54 | 0:11:58 | |
That makes it what is known as a dwarf planet. | 0:11:58 | 0:12:01 | |
But that's not the case for Vesta. | 0:12:02 | 0:12:04 | |
Because it is smaller, its gravity is too weak to form a sphere, | 0:12:04 | 0:12:08 | |
leaving it with a more irregular shape. | 0:12:08 | 0:12:11 | |
It fits into a lesser category, a minor planet. | 0:12:11 | 0:12:14 | |
To become a major planet like Earth or Jupiter, | 0:12:17 | 0:12:20 | |
a body needs to be spherical, which rules out Vesta. | 0:12:20 | 0:12:23 | |
But it also needs to have cleared out all | 0:12:23 | 0:12:25 | |
the material in its orbit, which is where Ceres is wanting. | 0:12:25 | 0:12:29 | |
The orbits of both Ceres and Vesta | 0:12:29 | 0:12:31 | |
lie deep within the main asteroid belt. | 0:12:31 | 0:12:33 | |
But the planets themselves aren't big enough | 0:12:33 | 0:12:35 | |
for their gravitational fields to have cleared out | 0:12:35 | 0:12:38 | |
the nearby asteroids, which is why | 0:12:38 | 0:12:40 | |
they're not major planets but they're still great to see. | 0:12:40 | 0:12:43 | |
Coming up, Pete's guide to the highlights of what to view | 0:12:47 | 0:12:50 | |
in this month's night sky. | 0:12:50 | 0:12:52 | |
We can't see much at the minute but here's Pete with some tips | 0:12:52 | 0:12:56 | |
on how to take dramatic astronomical photographs when the clouds clear. | 0:12:56 | 0:13:01 | |
It's really easy to take some | 0:13:02 | 0:13:04 | |
fabulous photographs of the night sky | 0:13:04 | 0:13:07 | |
using nothing more than just a camera and a tripod. | 0:13:07 | 0:13:09 | |
This month I'm going to show you two different techniques | 0:13:09 | 0:13:13 | |
which can be used to take some really great shots. | 0:13:13 | 0:13:15 | |
First up, a wide shot of the sky | 0:13:18 | 0:13:20 | |
that captures a panorama of the stars. | 0:13:20 | 0:13:23 | |
The best type of camera to use is a digital SLR camera. | 0:13:24 | 0:13:29 | |
Now you need to fit a fairly wide-angle lens, | 0:13:29 | 0:13:32 | |
say 50mm or shorter focal length, | 0:13:32 | 0:13:35 | |
the camera needs to be set into a manual mode | 0:13:35 | 0:13:37 | |
and you need to focus that lens as accurately as possible. | 0:13:37 | 0:13:40 | |
You must use a tripod to keep the camera steady, | 0:13:40 | 0:13:44 | |
otherwise the stars will appear blurred. | 0:13:44 | 0:13:47 | |
To get the best results it's useful to have the aperture, | 0:13:48 | 0:13:53 | |
or the opening on the lens, as wide as possible | 0:13:53 | 0:13:55 | |
because that allows all that delicate starlight to come into it. | 0:13:55 | 0:13:58 | |
So use the lowest f-number you can on your camera. | 0:13:58 | 0:14:01 | |
You want a fairly high ISO, between 400 and 1600. | 0:14:01 | 0:14:06 | |
And experiment with an exposure time of around 30 seconds. | 0:14:06 | 0:14:11 | |
Sadly the clouds are stopping us imaging tonight | 0:14:11 | 0:14:14 | |
but you should end up with a photograph like this. | 0:14:14 | 0:14:16 | |
When you start taking longer exposures of the night sky, | 0:14:19 | 0:14:22 | |
if you look at each individual star carefully, | 0:14:22 | 0:14:24 | |
you'll see they are no longer pinpricks of light | 0:14:24 | 0:14:27 | |
but they start to elongate into little lines. | 0:14:27 | 0:14:30 | |
We can use that effect creatively to take star trail photos | 0:14:30 | 0:14:34 | |
and that's our second type of astrophotography. | 0:14:34 | 0:14:37 | |
A star trail is a long exposure photograph that captures | 0:14:37 | 0:14:41 | |
the apparent motion of the stars as the Earth rotates. | 0:14:41 | 0:14:44 | |
The trick here is to do the opposite to the wide shot method. | 0:14:44 | 0:14:50 | |
To get those lovely, long streaks of brilliant light, | 0:14:50 | 0:14:53 | |
you need a long exposure time. | 0:14:53 | 0:14:56 | |
15 minutes will do but you can easily push it to 30 | 0:14:56 | 0:14:59 | |
if you're confident of clear skies. | 0:14:59 | 0:15:01 | |
'Remarkably some of the campers managed to get some images | 0:15:03 | 0:15:07 | |
'last night during a momentary break in the weather.' | 0:15:07 | 0:15:10 | |
That's amazing! | 0:15:10 | 0:15:11 | |
So you've got those lovely green lasers pointing up there | 0:15:11 | 0:15:15 | |
and look at that star field behind there. | 0:15:15 | 0:15:17 | |
It was just a gap in the clouds | 0:15:17 | 0:15:19 | |
and everybody got so excited. | 0:15:19 | 0:15:20 | |
I was just trying to capture the excitement of the astronomers | 0:15:20 | 0:15:24 | |
as well as the star field so it was like combining the two. | 0:15:24 | 0:15:26 | |
-Did somebody hold a red light? -I kind of annoyed everybody | 0:15:26 | 0:15:29 | |
flashing my red light. | 0:15:29 | 0:15:30 | |
I said, "I'm just going to do it for a couple of seconds." | 0:15:30 | 0:15:33 | |
A bit of red light painting. | 0:15:33 | 0:15:34 | |
You painted everybody, yeah, in red light. | 0:15:34 | 0:15:36 | |
But that is really effective and it contrasts beautifully with | 0:15:36 | 0:15:39 | |
the green of the laser. It's really effective. | 0:15:39 | 0:15:41 | |
That's come out so well. You've got Cassiopeia down there - the W. | 0:15:41 | 0:15:45 | |
It's great you've got a bit of a horizon in there as well. | 0:15:45 | 0:15:47 | |
I think it just adds to that, | 0:15:47 | 0:15:48 | |
otherwise it just sort of loses itself so it's nice to have a tree | 0:15:48 | 0:15:52 | |
or, in this case, campervan and a few tents on the way. | 0:15:52 | 0:15:55 | |
-Brilliant result. -Thank you. | 0:15:55 | 0:15:57 | |
While you're taking your long exposures, why not take that time | 0:15:57 | 0:16:01 | |
to explore the night sky in a bit more detail. | 0:16:01 | 0:16:04 | |
So here are my highlights of this month. | 0:16:04 | 0:16:07 | |
Galaxies are plentiful in May. | 0:16:07 | 0:16:09 | |
Below Mars at the moment is as distinctive star shape | 0:16:09 | 0:16:12 | |
known as the Sail - | 0:16:12 | 0:16:14 | |
part of the constellation of Corvus. | 0:16:14 | 0:16:16 | |
Two stars in Corvus point to M104 - the famous sombrero galaxy. | 0:16:17 | 0:16:23 | |
A small telescope shows its distinctive shape well. | 0:16:23 | 0:16:26 | |
The Plough, or Saucepan, sits roughly overhead around midnight. | 0:16:28 | 0:16:32 | |
Close by the star marking the end of the Saucepan's handle, | 0:16:32 | 0:16:36 | |
you'll find the wonderful whirlpool galaxy - M51. | 0:16:36 | 0:16:40 | |
Visible in good binoculars, | 0:16:40 | 0:16:42 | |
a telescope is required to bring out its spiral shape. | 0:16:42 | 0:16:46 | |
Early in the morning of May 24, a short but intense meteor shower | 0:16:46 | 0:16:50 | |
may appear to come from the constellation of Camelopardalis. | 0:16:50 | 0:16:55 | |
If it arrives, the meteors will be due to Earth passing through | 0:16:56 | 0:16:59 | |
the debris of comet 209P/LINEAR. | 0:16:59 | 0:17:03 | |
Finally, Saturn reaches opposition on May 10, | 0:17:04 | 0:17:08 | |
making it bright in the sky. | 0:17:08 | 0:17:10 | |
Look for it due south around 1am. | 0:17:10 | 0:17:12 | |
Through a telescope at opposition | 0:17:14 | 0:17:16 | |
the rings can appear to brighten quite noticeably. | 0:17:16 | 0:17:20 | |
With the cloud set in for the night, | 0:17:27 | 0:17:29 | |
we've retreated inside to look at this month's astro news. | 0:17:29 | 0:17:33 | |
We have to start with the death of LADEE, | 0:17:33 | 0:17:36 | |
the NASA spacecraft that crashed into the moon this month | 0:17:36 | 0:17:39 | |
after completing its mission to look at the moon's atmosphere, | 0:17:39 | 0:17:42 | |
or at least the dust that's kicked up from the lunar surface. | 0:17:42 | 0:17:46 | |
And it sent back just before it died this amazing sequence of pictures. | 0:17:46 | 0:17:49 | |
So you see the lunar horizon there. | 0:17:49 | 0:17:50 | |
As we flick on, what you see is a rather magnificent lunar sunrise, | 0:17:50 | 0:17:55 | |
something we haven't really seen like this since Apollo 17. | 0:17:55 | 0:17:58 | |
It's fabulous. It's great to see it. Actually if you go back a couple, | 0:17:58 | 0:18:01 | |
go back a few minutes, what you can see here | 0:18:01 | 0:18:03 | |
is that glow is dust in the solar system, | 0:18:03 | 0:18:05 | |
what we call the zodiacal light, | 0:18:05 | 0:18:06 | |
but seen from the surface of the moon. It's a beautiful thing. | 0:18:06 | 0:18:09 | |
It is. And illuminated by the sun. Fantastic. | 0:18:09 | 0:18:11 | |
Our next story comes from the Kepler mission, | 0:18:11 | 0:18:14 | |
whose mission in life has been to go out and find exoplanets | 0:18:14 | 0:18:17 | |
and it's done a fantastic job so far. | 0:18:17 | 0:18:19 | |
But of course the Holy Grail is to find an earthlike planet | 0:18:19 | 0:18:22 | |
and it looks as if it's done just that. | 0:18:22 | 0:18:24 | |
This is an artist's impression of an exoplanet called Kepler-186f | 0:18:24 | 0:18:29 | |
and it's going around a red dwarf which is slightly colder than | 0:18:29 | 0:18:33 | |
our sun. We found this on the outskirts of the Goldilocks zone. | 0:18:33 | 0:18:37 | |
So it's an earthlike planet which could have life. | 0:18:37 | 0:18:41 | |
It's slightly bigger than Earth | 0:18:41 | 0:18:42 | |
but it's just what we've been looking for. | 0:18:42 | 0:18:44 | |
Now we've also made another discovery just in our own neighbourhood. | 0:18:44 | 0:18:47 | |
This is the artist's impression | 0:18:47 | 0:18:49 | |
of the star that's been found just seven light years away. | 0:18:49 | 0:18:51 | |
So that makes it the fourth closest star known. | 0:18:51 | 0:18:55 | |
We only found it in the last month or so. | 0:18:55 | 0:18:56 | |
The reason we've only just found it is that it's rather cool. | 0:18:56 | 0:18:59 | |
In fact so cool, that it has | 0:18:59 | 0:19:01 | |
a temperature you'd expect at the Arctic - | 0:19:01 | 0:19:04 | |
-13 degrees centigrade. | 0:19:04 | 0:19:06 | |
To me that's counterintuitive. Stars shouldn't be cold. | 0:19:06 | 0:19:09 | |
You could think of this as a really big planet | 0:19:09 | 0:19:13 | |
but it will also have weather and clouds | 0:19:13 | 0:19:15 | |
just like the giant planets do. | 0:19:15 | 0:19:17 | |
The definition planet, star, where do we lie? | 0:19:17 | 0:19:20 | |
It gets much more interesting. | 0:19:20 | 0:19:21 | |
We've never really decided so let's just say we've found a new object | 0:19:21 | 0:19:24 | |
and it's very exciting. | 0:19:24 | 0:19:26 | |
Now back to how gravity shapes the night sky. | 0:19:32 | 0:19:35 | |
Chris North and Jon Culshaw are looking at how gravity | 0:19:35 | 0:19:38 | |
works on a huge scale to create galaxies of many different shapes. | 0:19:38 | 0:19:43 | |
With most of the campers on their way to bed | 0:19:45 | 0:19:47 | |
and the cloud still thick, | 0:19:47 | 0:19:48 | |
Chris and Jon are having to resort to some well chosen | 0:19:48 | 0:19:51 | |
photographs to guide us around an extraordinary spot in the night sky. | 0:19:51 | 0:19:56 | |
One particular zone we've been looking out for tonight | 0:19:57 | 0:20:00 | |
just above the constellation of Virgo is an area where, many a time, | 0:20:00 | 0:20:04 | |
you wouldn't see too much detail in there. | 0:20:04 | 0:20:06 | |
But get to a dark sky area like the Brecon Beacons | 0:20:06 | 0:20:09 | |
and place a scope on this particular zone | 0:20:09 | 0:20:11 | |
and it comes alive wonderfully, and you can see exactly | 0:20:11 | 0:20:15 | |
why this area is called the realm of the galaxies. | 0:20:15 | 0:20:18 | |
There are dozens, if not hundreds of galaxies to look at | 0:20:18 | 0:20:21 | |
with a small telescope in this area of the sky. | 0:20:21 | 0:20:24 | |
A bigger telescope will obviously show more. | 0:20:24 | 0:20:26 | |
And something that is called the Virgo cluster. | 0:20:26 | 0:20:28 | |
This image here shows us half a dozen bright galaxies | 0:20:28 | 0:20:31 | |
and dozens more fainter ones, all different shapes and sizes. | 0:20:31 | 0:20:35 | |
You can see elliptical galaxies that look like spheres. | 0:20:35 | 0:20:38 | |
We've got a close-up of a galaxy here and it looks like a round, | 0:20:38 | 0:20:42 | |
spherical blob. There's not a lot of structure there. | 0:20:42 | 0:20:44 | |
Rather like a supermassive star. | 0:20:44 | 0:20:46 | |
And that's the combined light of billions of stars all glowing | 0:20:46 | 0:20:49 | |
together, so it's quite a humbling thought when you think of that. | 0:20:49 | 0:20:53 | |
So if we take a look at the very familiar spiral galaxy, | 0:20:53 | 0:20:57 | |
what would be the forces that would cause a galaxy to form | 0:20:57 | 0:21:00 | |
rather like this? | 0:21:00 | 0:21:01 | |
This is one of the galaxies in the Virgo cluster, | 0:21:01 | 0:21:04 | |
this is M100, Messier 100, | 0:21:04 | 0:21:05 | |
and you can really see the characteristic spiral form. | 0:21:05 | 0:21:08 | |
What this doesn't really tell is quite how flat this structure is. | 0:21:08 | 0:21:12 | |
That's very much the way that gravity evolves our own Solar System | 0:21:12 | 0:21:16 | |
around the sun, this familiar flat disc. | 0:21:16 | 0:21:19 | |
Both the Solar System and galaxies form from roughly | 0:21:19 | 0:21:22 | |
spherical-ish blobs, clumps of gas and dust. | 0:21:22 | 0:21:26 | |
They collapse under gravity. | 0:21:26 | 0:21:28 | |
If there is a preferred direction of rotation to that gas and dust, | 0:21:28 | 0:21:33 | |
then that will settle into a disc. | 0:21:33 | 0:21:34 | |
And that's what happens with spiral galaxies like this, | 0:21:34 | 0:21:37 | |
the gas and dust collects into this disc | 0:21:37 | 0:21:40 | |
and new stars form and we see the patterns we see today. | 0:21:40 | 0:21:43 | |
And then in the solar system as well, the gas and the dust | 0:21:43 | 0:21:45 | |
collect into a disc and it's out of that gas and dust that the | 0:21:45 | 0:21:48 | |
planets form and that's why they're all in the same plane. | 0:21:48 | 0:21:51 | |
Essentially the same process. | 0:21:51 | 0:21:52 | |
Just because of this common axis of rotation. | 0:21:52 | 0:21:55 | |
What's behind the formation of the elliptical galaxies? | 0:21:55 | 0:21:57 | |
Well, this is an example of an elliptical galaxy. | 0:21:57 | 0:22:00 | |
What's happened is that elliptical galaxies | 0:22:00 | 0:22:02 | |
have formed from the mergers, | 0:22:02 | 0:22:04 | |
the combinations, the collisions | 0:22:04 | 0:22:06 | |
between other galaxies over billions of years. | 0:22:06 | 0:22:08 | |
And because that's lots of things combining together, | 0:22:08 | 0:22:11 | |
there's no one favoured direction | 0:22:11 | 0:22:13 | |
and you don't get this flat disc that we see in the spiral galaxies. | 0:22:13 | 0:22:16 | |
Isn't it fascinating to think that at | 0:22:16 | 0:22:18 | |
the centre of galaxies, where the stars are much more dense | 0:22:18 | 0:22:21 | |
and much more tightly packed, imagine being on a planet | 0:22:21 | 0:22:25 | |
orbiting one of those stars, what kind of a night sky would you see? | 0:22:25 | 0:22:28 | |
There'd certainly be many, many more stars in the sky. | 0:22:28 | 0:22:31 | |
And one of the reasons we can look at the Virgo cluster | 0:22:31 | 0:22:34 | |
and study it in the detail we can | 0:22:34 | 0:22:36 | |
is because we are looking out of our own Milky Way galaxy. | 0:22:36 | 0:22:38 | |
If we were in the centre of a galaxy | 0:22:38 | 0:22:40 | |
and there were stars all around, we wouldn't be able to do | 0:22:40 | 0:22:42 | |
extragalactic astronomy and look at other clusters. | 0:22:42 | 0:22:45 | |
There might be no evidence we were inside a cluster | 0:22:45 | 0:22:47 | |
or group of galaxies at all. | 0:22:47 | 0:22:49 | |
So we really are in quite a special location here to be able to | 0:22:49 | 0:22:53 | |
look out of our galaxy and see the rest of the Universe. | 0:22:53 | 0:22:56 | |
Next, we're sticking with gravity | 0:23:00 | 0:23:02 | |
but this time how we can see it in action closer to home. | 0:23:02 | 0:23:06 | |
Now one of the most beautiful things | 0:23:06 | 0:23:08 | |
to look at in the night sky must be Saturn. | 0:23:08 | 0:23:11 | |
The sixth planet in the solar system orbiting about nine times | 0:23:11 | 0:23:14 | |
further out from the sun than we do. | 0:23:14 | 0:23:16 | |
And with relatively basic equipment it's possible to get | 0:23:16 | 0:23:18 | |
a beautiful view of its magnificent rings. | 0:23:18 | 0:23:20 | |
And it's to these rings that we turn next because we've seen something | 0:23:20 | 0:23:24 | |
that's never been seen before - a moon forming amongst the rings. | 0:23:24 | 0:23:28 | |
Earlier today, | 0:23:28 | 0:23:29 | |
I talked to Dr Caitriona Jackman about these observations, | 0:23:29 | 0:23:32 | |
and about what they might mean for the early Solar System. | 0:23:32 | 0:23:35 | |
The NASA spacecraft Cassini has been orbiting Saturn | 0:23:37 | 0:23:40 | |
for the last ten years. | 0:23:40 | 0:23:42 | |
And in that time, it sent back incredible images | 0:23:42 | 0:23:45 | |
of the gas giant, of its moons | 0:23:45 | 0:23:47 | |
and of its glorious rings. | 0:23:47 | 0:23:50 | |
Cassini sent back some of the most spectacular images of the last | 0:23:51 | 0:23:54 | |
decade but the one that people are excited about right now is this. | 0:23:54 | 0:23:57 | |
So what are we looking at? | 0:23:57 | 0:23:59 | |
So this is a beautiful image that the Cassini spacecraft cameras | 0:23:59 | 0:24:01 | |
have taken when this spacecraft was looking down on top of the rings | 0:24:01 | 0:24:05 | |
and this is an image of a very bright feature | 0:24:05 | 0:24:08 | |
on the outer edge of the A ring. | 0:24:08 | 0:24:09 | |
So we're actually looking at this blob down here in the corner? | 0:24:09 | 0:24:13 | |
It's a very special blob. | 0:24:13 | 0:24:14 | |
It's actually the formation of a brand-new moon. | 0:24:14 | 0:24:18 | |
So it's material clumping together under its own self gravity | 0:24:18 | 0:24:22 | |
and in doing so dragging material out of the rings with it. | 0:24:22 | 0:24:25 | |
So a very small moon at the centre, | 0:24:25 | 0:24:27 | |
probably less than a kilometre in diameter, | 0:24:27 | 0:24:30 | |
but as it's orbiting around within the rings, | 0:24:30 | 0:24:33 | |
it's dragging local ring material and collecting it onto itself. | 0:24:33 | 0:24:36 | |
So how unusual is this? | 0:24:36 | 0:24:38 | |
This is a one-off. | 0:24:38 | 0:24:39 | |
This is the first time that we've ever seen anything like this. | 0:24:39 | 0:24:42 | |
This is our first time that | 0:24:42 | 0:24:43 | |
we've ever seen a moon being born in real-time. | 0:24:43 | 0:24:47 | |
-Saturn already has 60 moons. -It does. -Is it continually producing more? | 0:24:47 | 0:24:51 | |
We don't think so. | 0:24:51 | 0:24:53 | |
And what makes this opportunity so rare is that, as you say, | 0:24:53 | 0:24:57 | |
Saturn has more than 60 moons | 0:24:57 | 0:24:58 | |
and has some very famous icy moons in particular, | 0:24:58 | 0:25:01 | |
like Enceladus, and it is thought that Saturn's rings | 0:25:01 | 0:25:05 | |
used to be a lot bigger and that moons like Enceladus | 0:25:05 | 0:25:08 | |
were formed from the rings. | 0:25:08 | 0:25:10 | |
As those moons were formed by material in the rings | 0:25:10 | 0:25:13 | |
clumping together, they took a lot of material with them | 0:25:13 | 0:25:15 | |
and so the rings that we have today are quite depleted | 0:25:15 | 0:25:19 | |
relative to what they once were. | 0:25:19 | 0:25:21 | |
-So this is 2013 this image, so from last year? -Yes. | 0:25:21 | 0:25:24 | |
Do we know how our new moon is doing? | 0:25:24 | 0:25:26 | |
-I kind of want it to succeed. -Yeah, I want it to succeed too | 0:25:26 | 0:25:29 | |
but we're not sure what's happening to one part of it. | 0:25:29 | 0:25:32 | |
It's broken in two. | 0:25:32 | 0:25:34 | |
So object one is moving in through the rings and, as of last week, | 0:25:34 | 0:25:38 | |
it's causing a lot of disturbance locally and it's pulling | 0:25:38 | 0:25:41 | |
and tugging at the ring material near it. | 0:25:41 | 0:25:43 | |
Object two has gone the other way. | 0:25:43 | 0:25:45 | |
So object two has migrated out of the rings | 0:25:45 | 0:25:48 | |
and it's actually too small to be observed directly by Cassini. | 0:25:48 | 0:25:51 | |
-We may catch it again on a further orbit. -I hope so. | 0:25:51 | 0:25:54 | |
And of course this tells us about the rings | 0:25:54 | 0:25:56 | |
but it's also just telling us about physics. | 0:25:56 | 0:25:58 | |
If we go back five billion years | 0:25:58 | 0:25:59 | |
or so to a Solar System that looks something like this, | 0:25:59 | 0:26:02 | |
this disc of material from which the planets are forming | 0:26:02 | 0:26:05 | |
-looks rather like a ring system. -It does, yes. | 0:26:05 | 0:26:07 | |
So this is a disc that formed from the solar nebula | 0:26:07 | 0:26:11 | |
and from this disc you had planets and proto-planets forming | 0:26:11 | 0:26:14 | |
and then migrating outwards from the point of formation. | 0:26:14 | 0:26:18 | |
And so observing the formation of a moon like this, | 0:26:18 | 0:26:21 | |
and then its subsequent migration out, | 0:26:21 | 0:26:23 | |
is kind of a window on what might have happened | 0:26:23 | 0:26:26 | |
in the formation of the early Solar System. | 0:26:26 | 0:26:28 | |
And so Cassini has been there ten years | 0:26:28 | 0:26:30 | |
and we are still getting fabulous science from it. | 0:26:30 | 0:26:33 | |
What's next for the mission? | 0:26:33 | 0:26:35 | |
Cassini has got another three years to go. | 0:26:35 | 0:26:37 | |
It is going to finish in September of 2017 with a plunge through | 0:26:37 | 0:26:40 | |
Saturn's atmosphere | 0:26:40 | 0:26:41 | |
where the spacecraft will automatically vaporise. | 0:26:41 | 0:26:44 | |
-That's to get it out of the way. -Yes. -It has to end up somewhere | 0:26:44 | 0:26:47 | |
-and we don't want it crashing into anything. -Absolutely. | 0:26:47 | 0:26:49 | |
Before it vaporises, we're going to make | 0:26:49 | 0:26:51 | |
the best use of the time that we have left. | 0:26:51 | 0:26:53 | |
The final phase of the mission | 0:26:53 | 0:26:55 | |
will take the spacecraft just above the upper | 0:26:55 | 0:26:57 | |
atmosphere of Saturn and between the inner edge of the D ring. | 0:26:57 | 0:27:01 | |
That's a unique vantage point... | 0:27:01 | 0:27:02 | |
-That's between Saturn and the rings. -Absolutely. | 0:27:02 | 0:27:05 | |
So you're looking outwards at the rings for the first time ever. | 0:27:05 | 0:27:08 | |
That's going to shed light not only on Saturn's ring system | 0:27:08 | 0:27:12 | |
but on discs more generally and on how rings | 0:27:12 | 0:27:15 | |
and moons form more generally in the Solar System. | 0:27:15 | 0:27:17 | |
-And how gravity works wherever it is in the Universe. -Yes. | 0:27:17 | 0:27:20 | |
I look forward to seeing those images | 0:27:20 | 0:27:21 | |
and to hearing you talking about the results. | 0:27:21 | 0:27:24 | |
Thank you for now. Thanks a lot. | 0:27:24 | 0:27:25 | |
Last month we launched a competition to give one viewer the chance | 0:27:33 | 0:27:37 | |
to take control of HiRISE - | 0:27:37 | 0:27:39 | |
the most powerful camera in Martian orbit - | 0:27:39 | 0:27:42 | |
and choose a location for it to image. | 0:27:42 | 0:27:44 | |
We can announce the winner is John Green from Cambridge. | 0:27:44 | 0:27:47 | |
He's chosen a spot in the canyon Hebes Chasma | 0:27:47 | 0:27:51 | |
that he thinks has an odd black mark. | 0:27:51 | 0:27:55 | |
Hopefully the satellite will take the image in the next few months | 0:27:57 | 0:28:00 | |
and we'll put it on our website as soon as it reaches Earth. | 0:28:00 | 0:28:04 | |
Well, that's it for this programme. | 0:28:05 | 0:28:07 | |
Wonderful star parties are happening all over the country | 0:28:07 | 0:28:10 | |
so check on our website to find out what's happening near you. | 0:28:10 | 0:28:13 | |
When we come back next month, we'll be talking about the awesome power | 0:28:13 | 0:28:16 | |
of impacts - from asteroids in our Solar System to the distant cosmos. | 0:28:16 | 0:28:20 | |
-In the meantime, get outside and get looking up. -Good night. | 0:28:20 | 0:28:24 | |
MUSIC: "Pelleas and Melisande: At the Castle Gate" by Sibelius | 0:28:24 | 0:28:28 |