Browse content similar to Jupiter: Weather and Moons. Check below for episodes and series from the same categories and more!
Line | From | To | |
---|---|---|---|
THEME MUSIC: "At The Castle Gate" from "Pelleas and Melisande Suite" by Jean Sibelius. | 0:00:02 | 0:00:07 | |
Welcome to the Royal Observatory Greenwich, | 0:00:25 | 0:00:27 | |
the historical home of British astronomy | 0:00:27 | 0:00:30 | |
and a place with a surprising link to this month's topic. | 0:00:30 | 0:00:33 | |
The big story at the moment in our night skies, | 0:00:33 | 0:00:35 | |
is the fifth planet of the solar system, the mighty Jupiter. | 0:00:35 | 0:00:38 | |
And that's what we're going to explore in this programme. | 0:00:38 | 0:00:41 | |
Coming up, physicist Helen Czerski will be trying to uncover | 0:00:41 | 0:00:45 | |
some of the mysteries of Jupiter's atmosphere. | 0:00:45 | 0:00:48 | |
The memorable thing about the Great Red Spot | 0:00:48 | 0:00:50 | |
is it's been there for so long. | 0:00:50 | 0:00:51 | |
These features will persist for as long as the experiment runs. | 0:00:51 | 0:00:54 | |
Pete Lawrence will be showing us | 0:00:54 | 0:00:56 | |
just how easy it is for anyone to get a great view of Jupiter. | 0:00:56 | 0:01:01 | |
We'll be finding out about an astonishing new discovery, | 0:01:01 | 0:01:04 | |
water spraying out from one of Jupiter's moons. | 0:01:04 | 0:01:08 | |
We're talking about a plume of water 200km high | 0:01:08 | 0:01:12 | |
over the south pole of Europa. | 0:01:12 | 0:01:13 | |
And how the pictures you take | 0:01:13 | 0:01:15 | |
could be an essential tool in the study of the gas giant. | 0:01:15 | 0:01:19 | |
Jupiter is always a wonderful object to see in the night sky | 0:01:22 | 0:01:25 | |
but right now it's truly spectacular, outshining | 0:01:25 | 0:01:28 | |
even the brightest stars. | 0:01:28 | 0:01:30 | |
For the next few months, it'll be high in the sky after sunset | 0:01:30 | 0:01:34 | |
making this the best opportunity for British observers to get | 0:01:34 | 0:01:37 | |
a look at this fascinating world. | 0:01:37 | 0:01:39 | |
One of the joys of observing Jupiter is seeing those distinctive bands | 0:01:39 | 0:01:43 | |
and, of course, the Red Spot. | 0:01:43 | 0:01:45 | |
This image shows that in amazing detail. | 0:01:45 | 0:01:47 | |
Now the bands are actually formed by | 0:01:47 | 0:01:49 | |
a weather system which goes all | 0:01:49 | 0:01:50 | |
the way round Jupiter, with wind speeds greater than 300mph. | 0:01:50 | 0:01:55 | |
The Great Red Spot is actually three times the size of planet Earth | 0:01:55 | 0:01:58 | |
and has been raging for over three centuries. | 0:01:58 | 0:02:01 | |
And it's to this amazing weather that we turn first. | 0:02:01 | 0:02:03 | |
We sent physicist Helen Czerski | 0:02:03 | 0:02:06 | |
to see she could find out what causes this magnificent display. | 0:02:06 | 0:02:09 | |
When you look at an image of Jupiter, the most obvious thing are these | 0:02:15 | 0:02:18 | |
fabulous bands of colour that go horizontally across the surface. | 0:02:18 | 0:02:22 | |
But Jupiter doesn't really have a surface as such | 0:02:22 | 0:02:25 | |
because it's a gas giant. | 0:02:25 | 0:02:26 | |
What you see on Jupiter are swirling clouds of many different gases, | 0:02:26 | 0:02:32 | |
effectively what we're looking at | 0:02:32 | 0:02:34 | |
are just the tops of complex weather patterns. | 0:02:34 | 0:02:38 | |
But what drives this violent and long-lasting weather? | 0:02:38 | 0:02:41 | |
You'd think that - you can see so much detail - | 0:02:41 | 0:02:43 | |
the answer must be obvious but actually this is | 0:02:43 | 0:02:46 | |
one of the biggest mysteries in the Solar System. | 0:02:46 | 0:02:48 | |
One of the clearest features we can see from Earth is that | 0:02:48 | 0:02:53 | |
the atmosphere is arranged in a series of bands circling the planet. | 0:02:53 | 0:02:57 | |
These bands are iconic, | 0:02:57 | 0:02:59 | |
really strongly associated with Jupiter, | 0:02:59 | 0:03:02 | |
but this isn't the only planet to have weather in bands like this. | 0:03:02 | 0:03:07 | |
Saturn has clearly defined stripes of light and shade. | 0:03:07 | 0:03:11 | |
Neptune also has subtle visible bands. | 0:03:11 | 0:03:15 | |
The bands of weather that we are most familiar with | 0:03:16 | 0:03:18 | |
are actually here on Earth, it's just that we can't see them | 0:03:18 | 0:03:21 | |
because our atmosphere is transparent. | 0:03:21 | 0:03:23 | |
But they are there. | 0:03:23 | 0:03:26 | |
Earth's atmosphere is actually divided into distinct regions | 0:03:26 | 0:03:29 | |
known as cells. | 0:03:29 | 0:03:31 | |
Each cell is driven by hot air rising high into the atmosphere | 0:03:31 | 0:03:35 | |
and flowing either north or south. | 0:03:35 | 0:03:38 | |
There are six in total. | 0:03:38 | 0:03:39 | |
And the thing that I like about the comparison between Earth | 0:03:41 | 0:03:43 | |
and Jupiter is that we can't see those bands, those cells, | 0:03:43 | 0:03:49 | |
on Earth, but on Jupiter they are really visible. | 0:03:49 | 0:03:53 | |
Jupiter has many more cells than we have on Earth, there are at least 12. | 0:03:54 | 0:03:59 | |
And that's not just because it's bigger, the number of cells | 0:04:00 | 0:04:04 | |
a planet has actually depends on how quickly it's rotating. | 0:04:04 | 0:04:07 | |
Earth rotates once every 24 hours, that's what defines a day. | 0:04:09 | 0:04:14 | |
But Jupiter rotates roughly once every 10 hours, over twice as fast, | 0:04:14 | 0:04:18 | |
and if Earth did the same, our weather would be very different. | 0:04:18 | 0:04:22 | |
This is a simulation of the Earth as it is now, | 0:04:24 | 0:04:26 | |
looking slightly down from the northern hemisphere. | 0:04:26 | 0:04:29 | |
So the planet is rotating this way around. | 0:04:29 | 0:04:32 | |
What the colours represent are wind speeds high up in the atmosphere. | 0:04:32 | 0:04:36 | |
But if we change the simulation, so we speed up the rotation speed of the | 0:04:36 | 0:04:40 | |
Earth by a factor of four, a six-hour day, this is what it looks like. | 0:04:40 | 0:04:45 | |
You can see that suddenly there are many more bands | 0:04:45 | 0:04:48 | |
stretching around the planet. | 0:04:48 | 0:04:50 | |
The winds are constantly being pulled in a lateral direction, and that | 0:04:50 | 0:04:53 | |
means it's really hard for currents from the north and the south to form. | 0:04:53 | 0:04:57 | |
So the structure of Jupiter's atmosphere | 0:04:57 | 0:05:00 | |
is locked in these bands that we're all so familiar with. | 0:05:00 | 0:05:05 | |
The bands of fast-moving winds aren't the only | 0:05:05 | 0:05:08 | |
weather we can see on Jupiter, | 0:05:08 | 0:05:10 | |
there are also extraordinary vortices and spots, | 0:05:10 | 0:05:13 | |
some of which last for centuries. | 0:05:13 | 0:05:16 | |
But why did these atmospheric storms last so long? | 0:05:17 | 0:05:21 | |
I'm meeting Professor Peter Read, who is using a jug of water, | 0:05:22 | 0:05:26 | |
some sparkling dye | 0:05:26 | 0:05:27 | |
and a rotating rig to recreate a section of Jupiter's atmosphere. | 0:05:27 | 0:05:32 | |
Jupiter is quite unlike the Earth in many respects. | 0:05:32 | 0:05:35 | |
And in one important respect, | 0:05:35 | 0:05:37 | |
and that is that on the Earth, the equator is usually hot | 0:05:37 | 0:05:39 | |
and the poles are cold, | 0:05:39 | 0:05:42 | |
on Jupiter that's not the case. | 0:05:42 | 0:05:44 | |
What we tend to see is that the main temperature differences that we can | 0:05:44 | 0:05:47 | |
measure in the atmosphere are actually between the bright bands | 0:05:47 | 0:05:50 | |
and the dark bands. You will typically have | 0:05:50 | 0:05:52 | |
a bright band, which is relatively warm, | 0:05:52 | 0:05:54 | |
and then, to the north and the south of that, | 0:05:54 | 0:05:56 | |
there will be a dark band that is relatively cold. | 0:05:56 | 0:05:59 | |
That sounds amazing to me because I'm used to thinking about the Earth, | 0:05:59 | 0:06:02 | |
and the idea that the equator is hotter and the poles are cooler | 0:06:02 | 0:06:05 | |
is such a strong idea and that drives | 0:06:05 | 0:06:07 | |
all of our weather on this planet, but Jupiter is quite different. | 0:06:07 | 0:06:10 | |
And Jupiter has an extra ingredient that the Earth doesn't have and that | 0:06:10 | 0:06:13 | |
is that Jupiter itself is a source of energy from its deep interior. | 0:06:13 | 0:06:18 | |
It actually generates almost as much energy from | 0:06:18 | 0:06:22 | |
its deep interior as it receives on average from the sun. | 0:06:22 | 0:06:24 | |
With this experiment, we're trying to create a simulation of | 0:06:24 | 0:06:28 | |
what happens within one of Jupiter's bands. | 0:06:28 | 0:06:31 | |
The water is heated but the edges | 0:06:31 | 0:06:33 | |
in the centre of the vessel are cooled, | 0:06:33 | 0:06:36 | |
this represents a warm band on Jupiter surrounded by | 0:06:36 | 0:06:40 | |
colder air, and then the whole experimented is rotated. | 0:06:40 | 0:06:43 | |
After a few minutes, some vortices are created that are | 0:06:44 | 0:06:48 | |
so stable they barely appear to move. | 0:06:48 | 0:06:51 | |
So what you can see in now is a whole chain of these eddies | 0:06:52 | 0:06:56 | |
that are circulating in the same sense. | 0:06:56 | 0:06:59 | |
So if this was a band on Jupiter, | 0:06:59 | 0:07:01 | |
at the bottom of the band the winds are going this way round | 0:07:01 | 0:07:04 | |
and then you've got these eddies spinning like this, | 0:07:04 | 0:07:07 | |
-but at the top, the winds are going the other way. -That's right. | 0:07:07 | 0:07:11 | |
So this is just like the bright bands on Jupiter. | 0:07:11 | 0:07:14 | |
So in the south, the jets will be going in one direction, | 0:07:14 | 0:07:16 | |
and to the north, they'll be going in the opposite direction | 0:07:16 | 0:07:19 | |
with these vortices rolling in between them. | 0:07:19 | 0:07:21 | |
These rotating storms are trapped within the bands that have been | 0:07:21 | 0:07:25 | |
created by Jupiter's fast rotation. | 0:07:25 | 0:07:28 | |
This means they are remarkably stable. | 0:07:29 | 0:07:32 | |
On Earth, storms come and go, but on Jupiter | 0:07:32 | 0:07:34 | |
the really memorable thing about Great Red Spot | 0:07:34 | 0:07:36 | |
is it's been there for so long. | 0:07:36 | 0:07:38 | |
These little storms you've generated | 0:07:38 | 0:07:40 | |
in this experiment are just persisting. | 0:07:40 | 0:07:41 | |
These features will persist | 0:07:41 | 0:07:43 | |
for as long as we keep the experiment running, | 0:07:43 | 0:07:45 | |
once the whole thing has settled down. | 0:07:45 | 0:07:47 | |
This is just a two-dimensional representation | 0:07:47 | 0:07:50 | |
of what might be happening on Jupiter, | 0:07:50 | 0:07:52 | |
but our knowledge doesn't go much beyond that. | 0:07:52 | 0:07:55 | |
The problem is that when we look at the planet, | 0:07:55 | 0:07:58 | |
all we can see are the tops of the clouds | 0:07:58 | 0:08:00 | |
and it's really difficult to measure what's underneath that. | 0:08:00 | 0:08:03 | |
Finding out what's happening deep within the planet | 0:08:04 | 0:08:07 | |
is the next great challenge. | 0:08:07 | 0:08:09 | |
Luckily, there's hope that we all resolve some of these | 0:08:12 | 0:08:15 | |
unanswered questions in the near future | 0:08:15 | 0:08:17 | |
because NASA's Juno probe is on its way to Jupiter. | 0:08:17 | 0:08:21 | |
It's spent the last couple of years wandering around the inner | 0:08:21 | 0:08:24 | |
Solar System picking up speed, and at the end of last year, it | 0:08:24 | 0:08:27 | |
passed by Earth for its final gravity assist. | 0:08:27 | 0:08:30 | |
Remarkably, amateur astronomers were able to image it as it flew past. | 0:08:30 | 0:08:34 | |
In this sequence of images from Peter Birtwhistle, | 0:08:34 | 0:08:37 | |
the moving dot you can see is Juno itself | 0:08:37 | 0:08:39 | |
heading off to Jupiter. | 0:08:39 | 0:08:41 | |
Juno's on-board instrumentation will allow us | 0:08:43 | 0:08:45 | |
to peer below the clouds for the first time. | 0:08:45 | 0:08:48 | |
It will fly very close to the planet, | 0:08:48 | 0:08:50 | |
a mere 5,000km above the clouds | 0:08:50 | 0:08:53 | |
and below the radiation belt, | 0:08:53 | 0:08:54 | |
which has stopped us from taking detailed data in the past. | 0:08:54 | 0:08:57 | |
It will take detailed gravitational measurements | 0:08:57 | 0:08:59 | |
and measure the atmospheric composition, | 0:08:59 | 0:09:01 | |
it will also measure the mass of Jupiter's core, if there is one. | 0:09:01 | 0:09:05 | |
It's an incredibly exciting mission but we'll have to wait | 0:09:05 | 0:09:08 | |
until 2016 for Juno to arrive. | 0:09:08 | 0:09:11 | |
Now you don't need to travel to Jupiter | 0:09:19 | 0:09:21 | |
to get a fantastic image of it. | 0:09:21 | 0:09:23 | |
It's possible to capture really | 0:09:23 | 0:09:25 | |
detailed pictures of the planet from right here on Earth. | 0:09:25 | 0:09:28 | |
And images like these, taken by amateurs, | 0:09:29 | 0:09:32 | |
actually provide a unique record that even the space probes can't match. | 0:09:32 | 0:09:36 | |
I've been speaking with Professor John Rogers, | 0:09:38 | 0:09:40 | |
who gathers these images into a database | 0:09:40 | 0:09:42 | |
that scientists can use. | 0:09:42 | 0:09:44 | |
How are amateurs helping us understand Jupiter, | 0:09:44 | 0:09:46 | |
where professionals can't? | 0:09:46 | 0:09:48 | |
Well, amateurs are able to monitor Jupiter continuously, | 0:09:48 | 0:09:50 | |
and its weather systems evolve over timescales from days, | 0:09:50 | 0:09:53 | |
to months, to years, to decades, | 0:09:53 | 0:09:56 | |
so we really need continuous observations | 0:09:56 | 0:09:58 | |
to work out what's happening. | 0:09:58 | 0:10:00 | |
They're not just doing observations, they're doing some science too? | 0:10:00 | 0:10:03 | |
Yes, well, we can actually compile a record of what's going on, | 0:10:03 | 0:10:06 | |
how spots like the Great Red Spot evolved, | 0:10:06 | 0:10:09 | |
and we are able to monitor much smaller spots as well. | 0:10:09 | 0:10:12 | |
Here for instance, you see the Great Red Spot, you can | 0:10:12 | 0:10:15 | |
also see that the belts are not symmetrical. | 0:10:15 | 0:10:18 | |
This dark belt is here but there's normally a dark belt up here, | 0:10:18 | 0:10:21 | |
which, on this occasion in 2010, has disappeared. | 0:10:21 | 0:10:24 | |
So these kind of changes are happening all the time on Jupiter, | 0:10:24 | 0:10:27 | |
sometimes they take many years to unfold, | 0:10:27 | 0:10:29 | |
and that's what amateurs can really study. | 0:10:29 | 0:10:32 | |
I'm not used to seeing Jupiter in this orientation. | 0:10:32 | 0:10:34 | |
This is the way that amateurs most commonly see it, with south up. | 0:10:34 | 0:10:37 | |
So the Great Red Spot is in the southern atmosphere | 0:10:37 | 0:10:40 | |
and that's how we put all our pictures up for display. | 0:10:40 | 0:10:42 | |
But it's not just weather that the amateurs are spotting, | 0:10:42 | 0:10:45 | |
they also find impacts. | 0:10:45 | 0:10:48 | |
In 1994, the comet Shoemaker-Levy 9 | 0:10:48 | 0:10:51 | |
crashed into Jupiter, | 0:10:51 | 0:10:53 | |
leaving dark scars in its atmosphere. | 0:10:53 | 0:10:56 | |
Since then, amateurs have discovered that these | 0:10:56 | 0:10:59 | |
kinds of impacts are more common than previously thought. | 0:10:59 | 0:11:02 | |
In 2009, quite unexpectedly, an amateur, Anthony Wesley, | 0:11:02 | 0:11:06 | |
discovered such a spot on the planet. | 0:11:06 | 0:11:08 | |
This was an image he took two nights earlier, | 0:11:08 | 0:11:11 | |
and then he saw this remarkably black spot | 0:11:11 | 0:11:13 | |
appearing and realised that this might well be an impact. | 0:11:13 | 0:11:17 | |
So other amateurs immediately started taking images to confirm | 0:11:17 | 0:11:20 | |
and professional scientists took this image | 0:11:20 | 0:11:23 | |
in a far-infrared wavelength. | 0:11:23 | 0:11:25 | |
The Hubble Space Telescope took this image a few days lays later. | 0:11:25 | 0:11:28 | |
The professional astronomers managed to follow this event | 0:11:28 | 0:11:30 | |
over several months, | 0:11:30 | 0:11:32 | |
while the amateurs were also tracking over several months. | 0:11:32 | 0:11:35 | |
The amateurs are the watchkeepers, they keep on eye on Jupiter | 0:11:35 | 0:11:37 | |
and alert the professionals when something exciting happens? | 0:11:37 | 0:11:40 | |
Yes, indeed. | 0:11:40 | 0:11:42 | |
More recently, amateurs have been noticing impacts while they happen. | 0:11:42 | 0:11:46 | |
They are much smaller impacts, they don't leave visible scars | 0:11:46 | 0:11:49 | |
but they're more frequent. And so three times since 2009, | 0:11:49 | 0:11:54 | |
amateurs have actually seen fireballs in the atmosphere | 0:11:54 | 0:11:56 | |
of Jupiter, which previously, if anyone had seen them, | 0:11:56 | 0:11:59 | |
they didn't notice them or didn't believe they were seeing them. | 0:11:59 | 0:12:02 | |
But now we have real webcam videos and it's clear that | 0:12:02 | 0:12:05 | |
amateurs are actually detecting flashes as they occur. | 0:12:05 | 0:12:09 | |
So how does an amateur get involved? | 0:12:09 | 0:12:12 | |
The best way for someone who hasn't done it before is to | 0:12:12 | 0:12:15 | |
contact their local astronomical society. | 0:12:15 | 0:12:17 | |
There they'll meet people who are themselves | 0:12:17 | 0:12:19 | |
getting into the same kind of observations, | 0:12:19 | 0:12:21 | |
finding out how to use the same kind of equipment, | 0:12:21 | 0:12:24 | |
and I think that it's the personal contacts | 0:12:24 | 0:12:26 | |
that are most useful to someone | 0:12:26 | 0:12:27 | |
who hasn't experienced this kind of technology before. | 0:12:27 | 0:12:30 | |
Thanks, John, that was pretty fascinating | 0:12:30 | 0:12:32 | |
-and it shows the power of amateur astronomy. -Thank you. | 0:12:32 | 0:12:36 | |
Now Pete Lawrence is here with his guide to what else you can | 0:12:43 | 0:12:46 | |
see in the night sky around Jupiter. | 0:12:46 | 0:12:49 | |
But first, he's got a simple tip that can help address | 0:12:49 | 0:12:52 | |
one of the main problems that people face when they're stargazing - | 0:12:52 | 0:12:56 | |
how to match a star chart to the real night sky. | 0:12:56 | 0:12:59 | |
And he's with the Hampshire Astronomical Group on the South Downs. | 0:12:59 | 0:13:04 | |
Jupiter is pretty easy to find at the moment | 0:13:04 | 0:13:06 | |
because it's the brightest thing visible in the early evening | 0:13:06 | 0:13:09 | |
part of the night sky, apart from when the moon's about, of course. | 0:13:09 | 0:13:13 | |
For many people, when they look up at the night sky, | 0:13:13 | 0:13:15 | |
it can be a bit of a challenge to work out what is what. | 0:13:15 | 0:13:19 | |
But there are a few simple tips you can follow which will | 0:13:19 | 0:13:22 | |
make your life easier. | 0:13:22 | 0:13:23 | |
One of most difficult things for those starting out | 0:13:23 | 0:13:27 | |
is judging scale. | 0:13:27 | 0:13:28 | |
How do you relate the distance between stars on a star chart | 0:13:28 | 0:13:32 | |
to the distance in the night sky? | 0:13:32 | 0:13:35 | |
It might sound surprising, | 0:13:35 | 0:13:36 | |
but the best thing to do is to use your hands. | 0:13:36 | 0:13:39 | |
If you hold it out at arm's length, | 0:13:41 | 0:13:43 | |
like that, the distance between your thumb | 0:13:43 | 0:13:46 | |
and little finger is the same. | 0:13:46 | 0:13:48 | |
If you've got big hands or little hands, | 0:13:48 | 0:13:50 | |
the length of your arm tends to compensate for it. | 0:13:50 | 0:13:53 | |
So if you look at Orion - you can | 0:13:53 | 0:13:54 | |
see the bright star in the upper left corner | 0:13:54 | 0:13:56 | |
and the bright star in the lower right corner - you can | 0:13:56 | 0:13:59 | |
see that it fits more or less between those two. | 0:13:59 | 0:14:02 | |
For all of us, even though | 0:14:02 | 0:14:04 | |
we've got different sized hands and different length of arms, | 0:14:04 | 0:14:07 | |
you can actually hold two fingers up as well, that's a good indicator. | 0:14:07 | 0:14:11 | |
Just starting to appreciate the scale of patterns in the night sky | 0:14:11 | 0:14:14 | |
and you can relate that back to a star chart | 0:14:14 | 0:14:17 | |
and then gradually work your way across the sky. | 0:14:17 | 0:14:20 | |
Once you understand the apparent distances between stars, | 0:14:20 | 0:14:24 | |
finding anything in the sky should be much easier. | 0:14:24 | 0:14:27 | |
Jupiter is obviously the highlight up there at the moment, | 0:14:28 | 0:14:31 | |
it's magnificent. | 0:14:31 | 0:14:32 | |
But there's a lot more to be seen around that area and I've picked out | 0:14:32 | 0:14:36 | |
some of my favourite highlights for this month's star guide. | 0:14:36 | 0:14:40 | |
The magnificent constellation of Orion lies south in the early | 0:14:42 | 0:14:45 | |
evening during February. | 0:14:45 | 0:14:47 | |
Its seven bright stars are easy to pick out | 0:14:47 | 0:14:50 | |
and create a great signpost in the night sky. | 0:14:50 | 0:14:53 | |
Look out in particular for Orion's Sword that appears to hang | 0:14:53 | 0:14:57 | |
down from the belt, a region which contains the fabulous Orion Nebula. | 0:14:57 | 0:15:01 | |
Follow the line made by | 0:15:03 | 0:15:04 | |
Orion's Belt down the left | 0:15:04 | 0:15:06 | |
to locate Sirius - | 0:15:06 | 0:15:07 | |
the brightest night-time star. | 0:15:07 | 0:15:10 | |
About one-and-a-half | 0:15:10 | 0:15:11 | |
outstretched hand widths | 0:15:11 | 0:15:13 | |
above and left of Sirius is another | 0:15:13 | 0:15:15 | |
bright star called Procyon. | 0:15:15 | 0:15:18 | |
Join the dots of Sirius, Procyon | 0:15:21 | 0:15:23 | |
and orange Betelgeuse to form | 0:15:23 | 0:15:25 | |
a pattern known as | 0:15:25 | 0:15:26 | |
the Winter Triangle. | 0:15:26 | 0:15:27 | |
The winter Milky Way | 0:15:27 | 0:15:29 | |
passes through this region. | 0:15:29 | 0:15:31 | |
Scanning the area | 0:15:31 | 0:15:32 | |
with a pair of binoculars | 0:15:32 | 0:15:33 | |
reveals many faint | 0:15:33 | 0:15:34 | |
and beautiful star clusters. | 0:15:34 | 0:15:36 | |
Extend a line from Rigel, in Orion, | 0:15:41 | 0:15:44 | |
through Betelgeuse for twice the distance again - | 0:15:44 | 0:15:47 | |
that's two outstretched hand widths - | 0:15:47 | 0:15:50 | |
to arrive at a pair of stars | 0:15:50 | 0:15:51 | |
in Gemini known as Castor and Pollux. | 0:15:51 | 0:15:55 | |
They are about three finger widths apart. | 0:15:55 | 0:15:58 | |
If you traced the pattern of the famous twins back towards Orion, | 0:16:01 | 0:16:05 | |
you'll find the unmistakably bright planet Jupiter. | 0:16:05 | 0:16:10 | |
Jupiter is currently visible more or less all night long. | 0:16:12 | 0:16:15 | |
If you go out and catch it early, it's possible to see | 0:16:15 | 0:16:19 | |
a full rotation of the planet, that's one whole day on Jupiter. | 0:16:19 | 0:16:22 | |
If you get some lovely pictures of that, send them in to us | 0:16:22 | 0:16:25 | |
and we'll put the best ones up on our website. | 0:16:25 | 0:16:27 | |
Speaking of your photos, we've got | 0:16:28 | 0:16:30 | |
some great ones that have been uploaded to our website. | 0:16:30 | 0:16:33 | |
And here are a few that really stand out. | 0:16:33 | 0:16:36 | |
This is the Orion Nebula, which lies on Orion's Sword, | 0:16:39 | 0:16:43 | |
taken by Steve Richards. | 0:16:43 | 0:16:44 | |
Luke Stacy captured this image | 0:16:47 | 0:16:49 | |
of a chain of sun spots on 2nd February. | 0:16:49 | 0:16:52 | |
This shot by Mary Spicer shows how light bouncing off | 0:16:58 | 0:17:01 | |
the Earth can illuminate the parts of the moon that lie in shadow. | 0:17:01 | 0:17:05 | |
And this is Centaurus A, | 0:17:06 | 0:17:08 | |
a galaxy that lies too far south to be viewed directly from Britain. | 0:17:08 | 0:17:12 | |
It was taken over an astonishing 43 nights by Rolf Olson. | 0:17:12 | 0:17:17 | |
To send us your images, go to our website at... | 0:17:17 | 0:17:20 | |
Since we were last on air, | 0:17:23 | 0:17:25 | |
there has been plenty happening in the astronomical world | 0:17:25 | 0:17:27 | |
-and the most spectacular event has been a new supernova. -Yes. | 0:17:27 | 0:17:31 | |
A supernova is the dying throes of larger stars. | 0:17:31 | 0:17:35 | |
And we have one here captured by some UCL students. | 0:17:35 | 0:17:38 | |
So this is the M82 cigar galaxy. | 0:17:38 | 0:17:41 | |
And here, on 21st January, we have a new bright object - the supernova. | 0:17:41 | 0:17:45 | |
And what I love about this is this discovery was made by Steve Fossey | 0:17:45 | 0:17:48 | |
and a bunch of students just up the road | 0:17:48 | 0:17:50 | |
at the UCL's Mill Hill observatory. | 0:17:50 | 0:17:53 | |
But even better, it was a ten-minute gap where it wasn't cloudy. | 0:17:53 | 0:17:56 | |
-Exactly. A discovery from within the M25. -And it's perfect. | 0:17:56 | 0:18:00 | |
-It's a type 1a supernova, which are quite rare. -That's right. | 0:18:00 | 0:18:04 | |
We use these to measure how the universe is expanding. | 0:18:04 | 0:18:07 | |
So they're bright, so you can see them from a long distance away, | 0:18:07 | 0:18:10 | |
and that means we can use them | 0:18:10 | 0:18:11 | |
to work out how the universe is accelerating. | 0:18:11 | 0:18:14 | |
But, embarrassingly, we don't know what they are. | 0:18:14 | 0:18:16 | |
We've ideas that they might be a massive star spiralling | 0:18:16 | 0:18:19 | |
material down onto a white dwarf, which then explodes, but we're | 0:18:19 | 0:18:23 | |
not sure and that's why we need these local ones to try and help us. | 0:18:23 | 0:18:25 | |
This is 12 million light years away | 0:18:25 | 0:18:27 | |
-which is pretty local. -Just round the corner. | 0:18:27 | 0:18:29 | |
Yes! Is still visible now or does it decay very rapidly? | 0:18:29 | 0:18:32 | |
It will be visible for the next few months. | 0:18:32 | 0:18:34 | |
It was caught early enough that it was still brightening | 0:18:34 | 0:18:38 | |
so it will be at its brightest about now. | 0:18:38 | 0:18:40 | |
So go out, find M82. | 0:18:40 | 0:18:41 | |
If you look in binoculars, you should see it easily. | 0:18:41 | 0:18:44 | |
It won't quite make it to naked eye visibility | 0:18:44 | 0:18:46 | |
unless something odd happens | 0:18:46 | 0:18:48 | |
but it'll be an easy target for binoculars. | 0:18:48 | 0:18:50 | |
The brightest supernova | 0:18:50 | 0:18:51 | |
we've had in the northern hemisphere for years. | 0:18:51 | 0:18:53 | |
Speaking of celestial spectaculars, we had hoped before | 0:18:53 | 0:18:56 | |
Christmas that comet ISON was going to put on a great show for us | 0:18:56 | 0:19:00 | |
but it didn't quite work out like that | 0:19:00 | 0:19:02 | |
and Alan Fitzsimmons is going to tell us why. | 0:19:02 | 0:19:05 | |
People were predicting that ISON would be the comet of the century | 0:19:06 | 0:19:11 | |
that, as it came round the sun, | 0:19:11 | 0:19:13 | |
a huge tail would be created that would fill the night sky. | 0:19:13 | 0:19:16 | |
However, instead, it seems to have fizzled out. | 0:19:17 | 0:19:21 | |
But now, by pulling data from a number of scientific instruments, | 0:19:21 | 0:19:26 | |
it's possible to find out what actually happened. | 0:19:26 | 0:19:29 | |
Here we've got the comet | 0:19:29 | 0:19:31 | |
about a couple of hours before closest approach to the sun. | 0:19:31 | 0:19:34 | |
We can already see that something has happened to the comet. | 0:19:34 | 0:19:37 | |
In a normal comet, we expect to see | 0:19:37 | 0:19:39 | |
a very bright, distinct head, or coma, | 0:19:39 | 0:19:42 | |
form from all the gas | 0:19:42 | 0:19:43 | |
and small dust particles that the comet has released. | 0:19:43 | 0:19:47 | |
Here we can see the tail of the comet | 0:19:47 | 0:19:50 | |
but the head itself is already | 0:19:50 | 0:19:52 | |
not looking like a normal comet does - | 0:19:52 | 0:19:56 | |
it's spread out. | 0:19:56 | 0:19:57 | |
And even by this point, | 0:19:57 | 0:19:59 | |
a couple of hours before it reached | 0:19:59 | 0:20:01 | |
its closest point to the sun, | 0:20:01 | 0:20:02 | |
the comet nucleus itself | 0:20:02 | 0:20:04 | |
had been dispersed. Interestingly, | 0:20:04 | 0:20:06 | |
it's still far enough from the sun that it shouldn't have been | 0:20:06 | 0:20:09 | |
broken up by the gravitational field, | 0:20:09 | 0:20:11 | |
the tidal forces imparted on the nucleus by the sun, | 0:20:11 | 0:20:14 | |
but what's happened is simply its nucleus has been heated | 0:20:14 | 0:20:18 | |
so much and is releasing so much gas and material from its surface, | 0:20:18 | 0:20:22 | |
that pressure of that material building up in the comet | 0:20:22 | 0:20:26 | |
has simply broken it apart. | 0:20:26 | 0:20:28 | |
And so ISON was doomed long before it reached the sun. | 0:20:30 | 0:20:33 | |
And as it passed around our star, | 0:20:33 | 0:20:35 | |
it reappeared as nothing more than a cloud of debris. | 0:20:35 | 0:20:39 | |
But there is still a question about | 0:20:40 | 0:20:42 | |
whether anything of the nucleus had survived to live another day. | 0:20:42 | 0:20:46 | |
On December 16th, the Hubble Space Telescope went to have | 0:20:47 | 0:20:52 | |
a look at where the comet was predicted to be. | 0:20:52 | 0:20:54 | |
Now it's tracking where we expect the comet to be moving, | 0:20:54 | 0:20:59 | |
so all the background stars and galaxies appear as streaks. | 0:20:59 | 0:21:03 | |
But if there was any comet left, we would see it as a point-like | 0:21:03 | 0:21:06 | |
source here and we don't see anything. | 0:21:06 | 0:21:08 | |
So these Hubble Telescope images here | 0:21:08 | 0:21:11 | |
imply that there really isn't anything left at all of the nucleus. | 0:21:11 | 0:21:16 | |
So it's a shame. ISON is gone - | 0:21:16 | 0:21:19 | |
but it gave us a great show on its way in. | 0:21:19 | 0:21:22 | |
And we've got one more item of news this month. | 0:21:25 | 0:21:29 | |
In January, as part of Stargazing LIVE, | 0:21:29 | 0:21:31 | |
I challenged people to go online and look at pictures of galaxies | 0:21:31 | 0:21:35 | |
and look for gravitational lenses - | 0:21:35 | 0:21:37 | |
places where a distant galaxy has had its light bent | 0:21:37 | 0:21:40 | |
by a gravitational lens, by passing near a nearby galaxy. | 0:21:40 | 0:21:43 | |
We found lots of spectacular things | 0:21:43 | 0:21:46 | |
but the one we talked about on the night was this one. | 0:21:46 | 0:21:48 | |
-This is an infrared image of that galaxy. -Yes. What have we got? | 0:21:48 | 0:21:52 | |
-In the centre, that's the galaxy? -That's the nearby galaxy. | 0:21:52 | 0:21:55 | |
And the red arc that you can see, almost the red ring there, | 0:21:55 | 0:21:57 | |
is a distant galaxy whose light has been bent | 0:21:57 | 0:22:00 | |
and we're seeing it because it's being lensed by this nearby galaxy. | 0:22:00 | 0:22:03 | |
Without that galaxy, we wouldn't have a chance of seeing it? | 0:22:03 | 0:22:06 | |
Exactly. It's nature's telescope. | 0:22:06 | 0:22:07 | |
This is the infrared. What we've been doing since | 0:22:07 | 0:22:10 | |
is we've looked at it in the radio using Jodrell. | 0:22:10 | 0:22:12 | |
-This is the image that we've got. -It does look like different. | 0:22:12 | 0:22:15 | |
It does. | 0:22:15 | 0:22:16 | |
For starters, it's blobby because it's a radio image | 0:22:16 | 0:22:19 | |
and you don't get the beautiful pictures you do in the infrared. | 0:22:19 | 0:22:22 | |
The other thing, I don't know if I can convince you of this, | 0:22:22 | 0:22:25 | |
but in the infrared we saw that red ring, | 0:22:25 | 0:22:27 | |
in the radio, it's only one arc. | 0:22:27 | 0:22:28 | |
It definitely looks one-sided. | 0:22:28 | 0:22:31 | |
-So where's the rest of it gone? -Exactly. It's quite confusing. | 0:22:31 | 0:22:34 | |
Our best guess at the minute is that the radio | 0:22:34 | 0:22:37 | |
and the infrared radiation come from different parts of the galaxy. | 0:22:37 | 0:22:40 | |
So the infrared comes from star formation spread out through | 0:22:40 | 0:22:42 | |
the whole galaxy - and the galaxy's forming stars at a great rate, | 0:22:42 | 0:22:45 | |
about 100 times that of the Milky Way. | 0:22:45 | 0:22:47 | |
And the radio, we think, comes from right in the centre, | 0:22:47 | 0:22:50 | |
from the nucleus where material is spiralling onto | 0:22:50 | 0:22:53 | |
what must be a growing black hole in the centre of this galaxy. | 0:22:53 | 0:22:56 | |
This is what I love. Looking at the sky | 0:22:56 | 0:22:58 | |
in different bands of the electromagnetic spectrum | 0:22:58 | 0:23:00 | |
gives you a very different viewpoint and different understandings. | 0:23:00 | 0:23:03 | |
That's right. We knew that was true. | 0:23:03 | 0:23:05 | |
It's only the second time that we've seen this | 0:23:05 | 0:23:07 | |
misalignment between a radio lens and an infrared lens. | 0:23:07 | 0:23:10 | |
A perfect ring in the infrared and nice to blobby arc in the radio. | 0:23:10 | 0:23:13 | |
It's quite fun. | 0:23:13 | 0:23:15 | |
If you go to the Sky At Night website, | 0:23:15 | 0:23:16 | |
we've actually put some more data online. If you follow the link, | 0:23:16 | 0:23:19 | |
you might be able to discover your own lensed galaxy. | 0:23:19 | 0:23:22 | |
Well, back to Jupiter, and we're in the Endeavour Room | 0:23:28 | 0:23:30 | |
of the Royal Observatory Greenwich, | 0:23:30 | 0:23:32 | |
which these days is a library but which used to house | 0:23:32 | 0:23:35 | |
some of the largest telescopes on the site. | 0:23:35 | 0:23:37 | |
It was in this room, in 1908, that British astronomer | 0:23:37 | 0:23:40 | |
Melotte discovered a moon of Jupiter. | 0:23:40 | 0:23:43 | |
This is the image and this dot here is the moon we now call Pasiphae. | 0:23:43 | 0:23:48 | |
Exciting things are happening with the moons of Jupiter | 0:23:48 | 0:23:51 | |
and to discuss them I'm joined by Dr Leigh Fletcher, | 0:23:51 | 0:23:53 | |
an expert on the Jupiter system. | 0:23:53 | 0:23:55 | |
-Leigh, welcome to the programme. -Thank you. | 0:23:55 | 0:23:57 | |
We're going to talk about Europa, | 0:23:57 | 0:23:59 | |
where jets of water have been discovered shooting into space. | 0:23:59 | 0:24:02 | |
We knew there was water on Europa already. | 0:24:02 | 0:24:04 | |
We did. Europa has always been a tantalising place for us | 0:24:04 | 0:24:07 | |
to one day go and explore and now more so with this new result of | 0:24:07 | 0:24:11 | |
plumes of water vapour being emitted from the south pole of Europa. | 0:24:11 | 0:24:15 | |
It's going to be a fabulous thing for us to go and look at one day. | 0:24:15 | 0:24:18 | |
Europa's an icy moon and that's what we see when we look at the surface. | 0:24:18 | 0:24:21 | |
Europa is the second of four Galilean satellites in orbit | 0:24:21 | 0:24:25 | |
around the Jupiter. It's about the size of our own moon. | 0:24:25 | 0:24:28 | |
If you look at it here on the screen, you can see. | 0:24:28 | 0:24:30 | |
It's an icy ball, Europa is, | 0:24:30 | 0:24:32 | |
and the different colours that you see across the surface | 0:24:32 | 0:24:35 | |
are contaminants in the ice itself. | 0:24:35 | 0:24:38 | |
It almost looks like you've got a frozen ice raft, | 0:24:38 | 0:24:41 | |
frozen then into a body of liquid water that has re-frozen. | 0:24:41 | 0:24:45 | |
We call it chaos terrain. | 0:24:45 | 0:24:47 | |
-We can zoom in to get a proper look. -Yeah. -There we go. | 0:24:47 | 0:24:50 | |
This is one of the key pieces of evidence which suggests | 0:24:50 | 0:24:53 | |
that beneath this terrain there is liquid water. | 0:24:53 | 0:24:56 | |
Liquid water in our solar system locked away beneath the icy service. | 0:24:56 | 0:25:01 | |
We've been talking about this for years. There's an annoying catch, | 0:25:01 | 0:25:04 | |
isn't there, that the ice is pretty thick? | 0:25:04 | 0:25:06 | |
This is the typical thing within our solar system of the ability | 0:25:06 | 0:25:10 | |
to sense what we really want to see, which is that ocean, | 0:25:10 | 0:25:13 | |
is forbidden to us because it's hidden away, | 0:25:13 | 0:25:16 | |
locked away, or so we thought. | 0:25:16 | 0:25:17 | |
But now, with the discovery of these water vapour plumes, | 0:25:17 | 0:25:21 | |
we have a tantalising chance to fly through those plumes | 0:25:21 | 0:25:24 | |
-and sniff out the composition. -Let's look at that that new observation. | 0:25:24 | 0:25:27 | |
This was released at the end of last year. | 0:25:27 | 0:25:29 | |
It's a Hubble Space Telescope observation. | 0:25:29 | 0:25:31 | |
And I have to say, Leigh, looking at this, | 0:25:31 | 0:25:33 | |
it's not hugely convincing. | 0:25:33 | 0:25:35 | |
I'm very sorry that you're disappointed but this is actually | 0:25:35 | 0:25:38 | |
a really exciting discovery that the folks with | 0:25:38 | 0:25:40 | |
the Hubble Space Telescope made just that while ago. | 0:25:40 | 0:25:43 | |
Don't forget that you're seeing this from planet Earth, | 0:25:43 | 0:25:46 | |
five astronomical units away. | 0:25:46 | 0:25:48 | |
Five times as far away from the sun as the Earth is. | 0:25:48 | 0:25:50 | |
Absolutely. All the way out at the orbit of Jupiter. | 0:25:50 | 0:25:53 | |
This is an artist's impression superimposing the two together. | 0:25:53 | 0:25:57 | |
What they're looking at here is | 0:25:57 | 0:25:58 | |
ultraviolet emission from hydrogen and oxygen. | 0:25:58 | 0:26:01 | |
So this is water that has been spewed out of the moon | 0:26:01 | 0:26:03 | |
-and has then been disassociated, split apart... -By the sun's light. | 0:26:03 | 0:26:08 | |
Exactly, by UV radiation. | 0:26:08 | 0:26:09 | |
We can see that emanating from the south pole. | 0:26:09 | 0:26:12 | |
We're talking about a plume of water 200km high | 0:26:12 | 0:26:16 | |
over the south pole of Europa. | 0:26:16 | 0:26:18 | |
I can tell you we didn't expect to see that. | 0:26:18 | 0:26:20 | |
How have we got water at the south pole? | 0:26:20 | 0:26:22 | |
What's going on here is we've got these cracks, and these fissures | 0:26:22 | 0:26:25 | |
and stripes, which are undergoing different amounts of stress | 0:26:25 | 0:26:29 | |
as the moon goes round Jupiter. | 0:26:29 | 0:26:31 | |
The orbit of Europa around Jupiter is not perfectly circular | 0:26:31 | 0:26:35 | |
and that means sometimes it's closer to Jupiter, | 0:26:35 | 0:26:37 | |
where the gravity's stronger, | 0:26:37 | 0:26:38 | |
and sometimes it's further away, where the gravity is weaker. | 0:26:38 | 0:26:41 | |
Jupiter's a big thing, its pull is pretty significant. | 0:26:41 | 0:26:44 | |
It's an immense gravitational field, | 0:26:44 | 0:26:46 | |
that means, when Europa is far away from the moon... | 0:26:46 | 0:26:49 | |
Like this observation. | 0:26:49 | 0:26:50 | |
Like this observation in December 2012, things are relaxed, | 0:26:50 | 0:26:54 | |
you're able to emanate these plumes out of the south pole. | 0:26:54 | 0:26:57 | |
Now the team also have observations from just a month earlier. | 0:26:57 | 0:27:00 | |
At that point, Europa was much closer in to Jupiter, | 0:27:00 | 0:27:03 | |
so where the gravity field is stronger, | 0:27:03 | 0:27:06 | |
if you like, no plumes were observed at that point. | 0:27:06 | 0:27:08 | |
So you have this situation, extremely dynamically rich, | 0:27:08 | 0:27:11 | |
where the plumes are only emanating their material into space | 0:27:11 | 0:27:15 | |
when the stress is at its lowest point - | 0:27:15 | 0:27:17 | |
at the furthest distance away from Jupiter. | 0:27:17 | 0:27:20 | |
Now this is a fabulously exciting discovery. | 0:27:20 | 0:27:23 | |
It provides access to this water - | 0:27:23 | 0:27:24 | |
the stuff we thought was locked up under the surface - | 0:27:24 | 0:27:27 | |
and you have a mission, or you're part of a team | 0:27:27 | 0:27:29 | |
working on a mission, called JUICE, which is heading to Europa. | 0:27:29 | 0:27:32 | |
How does this change your plans? | 0:27:32 | 0:27:34 | |
It's being built by the European Space Agency to launch in 2022, | 0:27:34 | 0:27:38 | |
or thereabouts and, at the moment, | 0:27:38 | 0:27:40 | |
we are scheduled to have two flybys of Europa in 2031. | 0:27:40 | 0:27:44 | |
We are going to be up close and personal with those plumes, able to | 0:27:44 | 0:27:47 | |
look at the light as it is being filtered and scattered through them. | 0:27:47 | 0:27:50 | |
We've even got instruments on-board capable of detecting | 0:27:50 | 0:27:53 | |
the sorts of materials that are emanating. | 0:27:53 | 0:27:55 | |
There's a huge caveat to that, I should say. | 0:27:55 | 0:27:58 | |
What if this material isn't coming from the ocean? | 0:27:58 | 0:28:00 | |
Maybe it's the action of something heating up | 0:28:00 | 0:28:03 | |
in just the very top layers. | 0:28:03 | 0:28:05 | |
Even then, it's still exciting because it's a way | 0:28:05 | 0:28:07 | |
we can sample the surface materials | 0:28:07 | 0:28:08 | |
from our spacecraft without landing on the surface. | 0:28:08 | 0:28:11 | |
So when does JUICE get there? | 0:28:11 | 0:28:13 | |
JUICE will get there in 2030 and it will fly by Europa twice in 2031. | 0:28:13 | 0:28:17 | |
-Fabulous. Come back and tell us about it and good luck. -Thank you. | 0:28:17 | 0:28:20 | |
-Leigh, thanks a lot. -Thank you. | 0:28:20 | 0:28:22 | |
So that's it for this month, but do remember to keep on sending | 0:28:28 | 0:28:31 | |
your pictures in, especially if you manage to get | 0:28:31 | 0:28:34 | |
a full rotation of Jupiter, and we'll put the best on our website. | 0:28:34 | 0:28:37 | |
When we come back next month, will be listening to the cosmos - | 0:28:37 | 0:28:39 | |
studying sound waves to find out what they can tell us | 0:28:39 | 0:28:42 | |
about the Universe's hidden secrets. | 0:28:42 | 0:28:45 | |
And we'll also be looking at how to get | 0:28:45 | 0:28:46 | |
wonderful images of the night sky with just a smartphone. | 0:28:46 | 0:28:49 | |
-So remember, get outside and get looking up. -Good night. | 0:28:49 | 0:28:53 | |
THEME MUSIC: "At The Castle Gate" from "Pelleas and Melisande Suite" by Jean Sibelius | 0:28:53 | 0:28:58 |