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This month, a majestic sight in our night skies. Mars is the closest and brightest it's been for years. | 0:00:02 | 0:00:06 | |
Mars captures the imagination like no other planet | 0:00:06 | 0:00:09 | |
so come with us and let us take you to this amazing world. | 0:00:09 | 0:00:12 | |
Let's journey to Mars. | 0:00:12 | 0:00:14 | |
We're in Stevenage, where Airbus has built a small slice of Mars | 0:00:40 | 0:00:44 | |
here on Earth to test out prototypes for Europe's ExoMars Rover. | 0:00:44 | 0:00:49 | |
And, coming up, geologist Iain Stewart will reveal how these rocks | 0:00:49 | 0:00:53 | |
help unlock the secrets of Mars. | 0:00:53 | 0:00:56 | |
So this really is evidence that through here in the past | 0:00:56 | 0:01:00 | |
once flowed a mighty river. | 0:01:00 | 0:01:02 | |
Pete Lawrence will be showing us | 0:01:02 | 0:01:04 | |
the great things we can see on Mars from right here on Earth. | 0:01:04 | 0:01:07 | |
That's fantastic. There's so much detail there. | 0:01:07 | 0:01:10 | |
We'll be giving one of you the chance to capture your very own | 0:01:10 | 0:01:13 | |
photograph of Mars by taking control of the most powerful | 0:01:13 | 0:01:17 | |
camera in Martian orbit. | 0:01:17 | 0:01:18 | |
Away from Mars, could this be the scientific discovery of the century? | 0:01:20 | 0:01:24 | |
But, first, our journey to Mars begins above the Red Planet. | 0:01:27 | 0:01:31 | |
It's astonishing what discoveries have been made | 0:01:31 | 0:01:34 | |
without even landing on the surface. | 0:01:34 | 0:01:36 | |
Though we're used to thinking of Mars as a dry and dusty red desert, | 0:01:36 | 0:01:40 | |
it's actually an amazingly varied and even a dynamic place. | 0:01:40 | 0:01:44 | |
The HiRISE camera on NASA's Mars Reconnaissance Orbiter | 0:01:46 | 0:01:49 | |
allows us to see the planet in exquisite detail. | 0:01:49 | 0:01:52 | |
It reveals a series of extraordinary landscapes, from these vast | 0:01:54 | 0:01:59 | |
fields of ice sculpted into varied and wonderful forms... | 0:01:59 | 0:02:03 | |
To shifting seas of sand dunes, their shady sides covered in frost. | 0:02:03 | 0:02:08 | |
There are areas covered in polygons where ice has thawed and cracked, | 0:02:08 | 0:02:13 | |
creating these almost leaf-like structures. | 0:02:13 | 0:02:16 | |
And impact craters that help tell us | 0:02:16 | 0:02:18 | |
the age of the surface of the planet. | 0:02:18 | 0:02:21 | |
And the HiRISE camera has revealed that this dynamic world | 0:02:21 | 0:02:24 | |
can also change almost in front of our eyes. | 0:02:24 | 0:02:27 | |
This is an image of spring arriving at the polar ice caps on Mars. | 0:02:27 | 0:02:31 | |
Mars is tilted on its axis, just like the Earth, and so it too has seasons. | 0:02:31 | 0:02:36 | |
What you can see here in this sort of brain-like image is the ground | 0:02:36 | 0:02:40 | |
emerging through the ice as it begins to thaw. | 0:02:40 | 0:02:43 | |
But this is actually frozen water and frozen carbon dioxide, | 0:02:43 | 0:02:47 | |
otherwise known as dry ice. | 0:02:47 | 0:02:49 | |
Mars's atmosphere is so thin | 0:02:49 | 0:02:50 | |
it can't sustain liquid water on its surface in most circumstances, | 0:02:50 | 0:02:55 | |
but have a look at these images from near the Martian equator. | 0:02:55 | 0:02:58 | |
There seems to be something flowing down this slope. | 0:02:58 | 0:03:01 | |
This is quite controversial because there's debate as to what it is. | 0:03:01 | 0:03:04 | |
Some people think water, some people think it's salt water, which is | 0:03:04 | 0:03:07 | |
actually fluid at a much lower temperature. | 0:03:07 | 0:03:09 | |
Other people think it's just carbon dioxide | 0:03:09 | 0:03:12 | |
or maybe some dust rolling down a slope. | 0:03:12 | 0:03:14 | |
If not, though, this could be the first images to show liquid | 0:03:14 | 0:03:18 | |
moving on the Martian surface. | 0:03:18 | 0:03:19 | |
Now, the Martian atmosphere might be incredibly thin, but it doesn't mean | 0:03:19 | 0:03:23 | |
there's no weather there, as we can see in this image. | 0:03:23 | 0:03:25 | |
This spiral is a dust devil half a mile high, | 0:03:25 | 0:03:29 | |
a huge tornado in the Martian atmosphere. | 0:03:29 | 0:03:31 | |
Now, this is one of my favourite images. | 0:03:31 | 0:03:34 | |
This is a uniquely Martian scene. | 0:03:34 | 0:03:36 | |
This is the result of blocks of dry ice skidding down a slope, | 0:03:36 | 0:03:40 | |
almost as if they were skiing. | 0:03:40 | 0:03:43 | |
Now, we use dry ice here on Earth at room temperature | 0:03:43 | 0:03:45 | |
to create nice atmospheric smoky scenes | 0:03:45 | 0:03:47 | |
but on Mars the atmosphere's at minus 150 degrees C, | 0:03:47 | 0:03:51 | |
and so the dry ice stays frozen. | 0:03:51 | 0:03:53 | |
So what we're seeing is something that couldn't happen on Earth. | 0:03:53 | 0:03:56 | |
Mars is a funny planet. Sometimes it looks so Earth-like | 0:03:56 | 0:03:59 | |
and sometimes it does something like this that's uniquely Martian. | 0:03:59 | 0:04:03 | |
A little later we'll be giving you an exciting opportunity | 0:04:03 | 0:04:06 | |
to take control of the HiRISE camera and get your very own image of Mars. | 0:04:06 | 0:04:10 | |
Thanks to HiRISE and the other orbiting cameras, | 0:04:10 | 0:04:13 | |
we've been able to explore the Mars of today. | 0:04:13 | 0:04:16 | |
And what's really exciting is trying to understand the Mars of the past. | 0:04:16 | 0:04:20 | |
Today the Red Planet is a hostile environment for life | 0:04:22 | 0:04:26 | |
but it now seems, over 3½ billion years ago, it was very different. | 0:04:26 | 0:04:31 | |
This history has been uncovered by a succession of rovers | 0:04:33 | 0:04:36 | |
that have travelled to Mars as our surrogate explorers. | 0:04:36 | 0:04:39 | |
In 2004, two rovers, Spirit and Opportunity, arrived on the planet. | 0:04:41 | 0:04:47 | |
They were designed to survive for 90 days | 0:04:47 | 0:04:49 | |
but Opportunity is still going strong, 10 years later. | 0:04:49 | 0:04:54 | |
And then, in 2012, the much larger Curiosity rover arrived. | 0:04:54 | 0:04:58 | |
In just a single decade these missions have | 0:05:00 | 0:05:03 | |
transformed our understanding of Mars by allowing us | 0:05:03 | 0:05:06 | |
to read the secrets contained within its rocks. | 0:05:06 | 0:05:09 | |
Geologist Iain Stewart has been investigating how | 0:05:10 | 0:05:13 | |
the rocks on Mars have allowed us to search for signs of ancient water | 0:05:13 | 0:05:17 | |
and recreate the planet's astonishing past. | 0:05:17 | 0:05:21 | |
Inside here is something really precious. | 0:05:21 | 0:05:24 | |
That...is a slice of another planet. | 0:05:25 | 0:05:29 | |
This tiny rock is a bit of a meteorite | 0:05:29 | 0:05:32 | |
which fell in Oman in the desert in 1999. | 0:05:32 | 0:05:35 | |
But actually it's from Mars. | 0:05:35 | 0:05:38 | |
It's one of about 130 or so meteorites that came from Mars, | 0:05:38 | 0:05:42 | |
blasted off by asteroid impacts. | 0:05:42 | 0:05:45 | |
The thing is, you can tell a lot about a place and its past | 0:05:45 | 0:05:49 | |
from the rocks that it leaves behind. | 0:05:49 | 0:05:51 | |
So this, I know, is an igneous rock, it's a basalt, | 0:05:51 | 0:05:56 | |
which means at some point in the past | 0:05:56 | 0:05:58 | |
volcanoes were erupting on Mars. | 0:05:58 | 0:06:01 | |
This little rock tells us a great deal about how Mars formed | 0:06:01 | 0:06:05 | |
but it doesn't help us with the really big question - | 0:06:05 | 0:06:10 | |
could the planet have once harboured life? | 0:06:10 | 0:06:13 | |
The Mars rovers are roaming the surface of the Red Planet, | 0:06:16 | 0:06:20 | |
searching for rocks that reveal clues | 0:06:20 | 0:06:22 | |
to what the environment was like in the past. | 0:06:22 | 0:06:25 | |
Reading this evidence is a skill we've perfected here on earth. | 0:06:27 | 0:06:30 | |
This rock face is part of the Jurassic coastline in Devon. | 0:06:32 | 0:06:36 | |
It was formed around 240 million years ago | 0:06:36 | 0:06:39 | |
and it provides a detailed record of different environmental conditions. | 0:06:39 | 0:06:44 | |
There's a whole set of layers in this cliff, and the thing is, | 0:06:44 | 0:06:47 | |
if you know how to read them properly, | 0:06:47 | 0:06:49 | |
you can create these different environments. | 0:06:49 | 0:06:52 | |
So here we've got a layer of cobbles, | 0:06:52 | 0:06:54 | |
there's a layer of sand coming through | 0:06:54 | 0:06:57 | |
and here's more of these cobbles, sand, cobbles, | 0:06:57 | 0:07:00 | |
and then we get this, it's more of a soil. | 0:07:00 | 0:07:02 | |
This is an ancient land surface. | 0:07:02 | 0:07:03 | |
Then, above that, it's just sand blown around by the wind. | 0:07:03 | 0:07:08 | |
Now, these, these are really distinctive. | 0:07:08 | 0:07:11 | |
You can see how beautifully rounded all those pebbles are. | 0:07:11 | 0:07:14 | |
Look at them, incredible. | 0:07:14 | 0:07:16 | |
So they would have started off as just general angular rocks | 0:07:16 | 0:07:19 | |
but what's made them all smooth is water. | 0:07:19 | 0:07:23 | |
They've been churned around in a turbulent flow. | 0:07:23 | 0:07:25 | |
Imagine a big river of debris coming along, | 0:07:25 | 0:07:28 | |
knocking the edges off the clasts as they go, | 0:07:28 | 0:07:31 | |
just creating these beautifully smooth pebbles. | 0:07:31 | 0:07:34 | |
So this really is evidence that through here in the past | 0:07:34 | 0:07:37 | |
once flowed a mighty river. | 0:07:37 | 0:07:39 | |
The one key condition that most scientists agree | 0:07:40 | 0:07:44 | |
is needed for life to have existed on Mars is water. | 0:07:44 | 0:07:47 | |
So the rovers have been searching for rounded pebbles | 0:07:47 | 0:07:51 | |
that might be signs of riverbeds. | 0:07:51 | 0:07:53 | |
But just along the coast, there's a different kind of rock formation | 0:07:53 | 0:07:57 | |
that shows a very different kind of evidence of contact with water. | 0:07:57 | 0:08:01 | |
And potentially an even more favourable environment | 0:08:01 | 0:08:04 | |
to search for life. | 0:08:04 | 0:08:06 | |
What we've got in front of us here is just a wall of sand, | 0:08:06 | 0:08:09 | |
just layer upon layer of sand dunes piled on top of each other. | 0:08:09 | 0:08:13 | |
But in amongst it there's these little bands. There's another one. | 0:08:13 | 0:08:17 | |
And they get a little bit thicker | 0:08:17 | 0:08:18 | |
and they look different to the sand above. | 0:08:18 | 0:08:21 | |
In fact, if you look in here, how crumbly this is. | 0:08:21 | 0:08:25 | |
Because what we've got here is a deposit that's been laid down | 0:08:28 | 0:08:31 | |
by really fine sediment settling out of standing water. | 0:08:31 | 0:08:36 | |
Essentially this is a temporary lake among the sand. | 0:08:36 | 0:08:40 | |
You only get rocks with this incredibly fine-grained structure | 0:08:41 | 0:08:45 | |
if they were formed when water becomes really still, | 0:08:45 | 0:08:48 | |
as it is in lakes and ponds. | 0:08:48 | 0:08:51 | |
I've just taken a big dollop of sand here | 0:08:51 | 0:08:53 | |
and as I swirl it around you see that, as long as I keep | 0:08:53 | 0:08:55 | |
the swirl going, then most of the sediment is still in the water. | 0:08:55 | 0:08:59 | |
But watch what happens if I stop the flow. | 0:08:59 | 0:09:03 | |
Immediately the finer sediment, the mud and the silt, just settles out. | 0:09:03 | 0:09:07 | |
So that means that whenever we see a kind of thin band of really | 0:09:07 | 0:09:11 | |
fine sediment, we know that it must have fallen out from still water. | 0:09:11 | 0:09:16 | |
This kind of sediment is much more likely to preserve signs of life | 0:09:18 | 0:09:22 | |
because it formed in a much gentler way. | 0:09:22 | 0:09:25 | |
Using these geological tricks we've built up this detailed | 0:09:25 | 0:09:29 | |
and compelling picture of the history of water on Earth. | 0:09:29 | 0:09:33 | |
But what does all this mean for Mars? | 0:09:33 | 0:09:37 | |
NASA's Mars Curiosity rover | 0:09:38 | 0:09:40 | |
has been taking close-up images of rocks on Mars | 0:09:40 | 0:09:44 | |
and sending them back to Earth for scientists to analyse. | 0:09:44 | 0:09:48 | |
Sanjeev Gupta is a geologist on the Curiosity team. | 0:09:50 | 0:09:53 | |
So this is a photograph taken by Curiosity, is that right? | 0:09:53 | 0:09:56 | |
That's right, this is Curiosity in Gale Crater. | 0:09:56 | 0:09:58 | |
You can see these beautiful planes that Curiosity is driving over, | 0:09:58 | 0:10:02 | |
searching for rock layers that might contain evidence for past life. | 0:10:02 | 0:10:06 | |
So what kind of rocks did it encounter, then? | 0:10:06 | 0:10:09 | |
So here we are, we can see these beautiful rock layers here. | 0:10:09 | 0:10:13 | |
-If we zoom in, you can see... -Oh, wow. | 0:10:13 | 0:10:16 | |
..that it's actually made up of lots and lots | 0:10:16 | 0:10:20 | |
of small particles, pebbles. | 0:10:20 | 0:10:23 | |
But what's really exciting about this rock | 0:10:23 | 0:10:26 | |
-is that the pebbles themselves are actually rounded. -Mm. | 0:10:26 | 0:10:30 | |
So we actually interpret this rock layer to be actually | 0:10:30 | 0:10:34 | |
-an ancient stream bed. -That's so cool. | 0:10:34 | 0:10:36 | |
That's the first time we've had that sort of evidence. | 0:10:36 | 0:10:38 | |
Now, rivers aren't that great for looking for ancient life. | 0:10:38 | 0:10:41 | |
You know, you can imagine these pebbles are being | 0:10:41 | 0:10:44 | |
tumbled in these flows and it's just too high energy. | 0:10:44 | 0:10:46 | |
And what geologists really look for, for searching, | 0:10:46 | 0:10:49 | |
are quiet water environments, calm environments, | 0:10:49 | 0:10:52 | |
where particles, sediment particles, | 0:10:52 | 0:10:54 | |
can settle out of suspension and trap organic matter, for example. | 0:10:54 | 0:10:58 | |
You know, the best environment would be an ancient lake. | 0:10:58 | 0:11:02 | |
Now, we never dared expect to find an ancient lake, | 0:11:02 | 0:11:05 | |
but this is what we saw. | 0:11:05 | 0:11:06 | |
So here's one of the first-ever drill holes | 0:11:07 | 0:11:10 | |
-on the surface of another planet. -That's extraordinary. | 0:11:10 | 0:11:13 | |
-That's something we do all the time on Earth. -That's right. | 0:11:13 | 0:11:16 | |
This is one of the first ones. | 0:11:16 | 0:11:18 | |
And you can see this drill hole is about 2½ centimetres in diameter | 0:11:18 | 0:11:21 | |
and you can see the rock powder | 0:11:21 | 0:11:23 | |
that's resulted in the drill tailings over here. | 0:11:23 | 0:11:25 | |
The next image is just fantastic | 0:11:25 | 0:11:27 | |
because this is actually an angled view into that drill hole. | 0:11:27 | 0:11:30 | |
Into the hole. | 0:11:30 | 0:11:31 | |
And you can see the grains over here, very, very fine-grained. | 0:11:31 | 0:11:34 | |
-This hole is about 2½cm across. -So these are smaller than sand grains. | 0:11:34 | 0:11:38 | |
They're smaller than sand grains. | 0:11:38 | 0:11:41 | |
And these layers have basically built up through time in an ancient lake, | 0:11:41 | 0:11:45 | |
and this is a perfect environment to look for clues for ancient life. | 0:11:45 | 0:11:49 | |
Curiosity has been able to go even further, | 0:11:51 | 0:11:54 | |
creating the clearest picture yet of Mars over 3½ billion years ago. | 0:11:54 | 0:11:59 | |
Using its on-board laboratory, it's analysed these samples | 0:11:59 | 0:12:02 | |
to show that not only did Mars have water | 0:12:02 | 0:12:05 | |
but that the water would have been fresh. | 0:12:05 | 0:12:08 | |
It's amazing to think how much we've managed to learn | 0:12:09 | 0:12:12 | |
by studying the rocks on another planet | 0:12:12 | 0:12:14 | |
without having to actually go there ourselves. | 0:12:14 | 0:12:17 | |
The picture it reveals is Mars over 3½ billion years ago, | 0:12:17 | 0:12:21 | |
awash with fresh water | 0:12:21 | 0:12:23 | |
and prime with the ingredients to support life. | 0:12:23 | 0:12:26 | |
Not only that, but we now have a good idea about where to look | 0:12:28 | 0:12:31 | |
for direct signs of past life on Mars. | 0:12:31 | 0:12:34 | |
And that's exactly what the next rover will do. | 0:12:36 | 0:12:38 | |
Mars has captivated us for millennia and one of the reasons is | 0:12:46 | 0:12:50 | |
that as our next-door neighbour, it's an unmissable presence in our skies. | 0:12:50 | 0:12:54 | |
And so Pete Lawrence begins this month's Star Guide | 0:12:55 | 0:12:59 | |
with some tips on how to observe Mars. | 0:12:59 | 0:13:02 | |
Now is a great time to go and view magnificent Mars | 0:13:02 | 0:13:05 | |
and you can see it up there just off to the left of the moon. | 0:13:05 | 0:13:09 | |
The reason why this is such a good time to look for it | 0:13:09 | 0:13:12 | |
is that the Earth is currently located between Mars and the sun | 0:13:12 | 0:13:15 | |
and that means that Mars is at its closest to us. | 0:13:15 | 0:13:18 | |
This occurs roughly every two years or so. | 0:13:18 | 0:13:21 | |
When it happens, Mars appears bright in the sky | 0:13:21 | 0:13:24 | |
and is really easy to find with the naked eye. | 0:13:24 | 0:13:27 | |
The motion of Mars across the night sky is extraordinary. | 0:13:29 | 0:13:33 | |
It appears to wander back and forth, performing a giant loop. | 0:13:33 | 0:13:37 | |
Mars isn't actually moving around the solar system | 0:13:38 | 0:13:41 | |
in an unruly fashion. | 0:13:41 | 0:13:43 | |
What's happening is that we're seeing an illusion | 0:13:43 | 0:13:45 | |
caused by the fact that the Earth is orbiting the sun faster than Mars. | 0:13:45 | 0:13:50 | |
As we overtake the Red Planet, | 0:13:50 | 0:13:52 | |
so Mars appears to loop back on itself in the sky, | 0:13:52 | 0:13:55 | |
an effect known as retrograde motion. | 0:13:55 | 0:13:58 | |
Of course, its most obvious attribute is its colour. | 0:13:59 | 0:14:03 | |
The colour comes from the rocks on the surface of the planet | 0:14:03 | 0:14:06 | |
but it's not uniformly red, which means with a good telescope | 0:14:06 | 0:14:10 | |
you can still see some splendid features on its surface. | 0:14:10 | 0:14:13 | |
And that's exactly what the members of the Bedford Astronomical Society are doing. | 0:14:14 | 0:14:20 | |
Oh, this looks interesting. | 0:14:20 | 0:14:21 | |
Well, that's an image we captured of Mars last Friday. | 0:14:21 | 0:14:23 | |
I was really pleased with it, we got some nice detail showing up. | 0:14:23 | 0:14:26 | |
You've got that lovely V shape feature there, | 0:14:26 | 0:14:29 | |
which is Syrtis Major of course. | 0:14:29 | 0:14:31 | |
And then further to the south of Syrtis Major | 0:14:31 | 0:14:35 | |
-you've got that bright patch there. -It's so bright. | 0:14:35 | 0:14:38 | |
It looks to me like it's a polar cap, but it's not, is it? | 0:14:38 | 0:14:41 | |
No, it's the Hellas Basin, this huge impact feature. | 0:14:41 | 0:14:44 | |
It's nine kilometres deep and it just must be | 0:14:44 | 0:14:47 | |
full of cloud at the moment, which is why it's so white and shiny. | 0:14:47 | 0:14:51 | |
But that bright patch you've got at the top there, that is a polar cap. | 0:14:51 | 0:14:54 | |
That's a genuine polar cap but it's decreasing all the time. | 0:14:54 | 0:14:57 | |
That's fantastic, so much detail. | 0:14:57 | 0:14:59 | |
Now, we've seen some fabulous images of Mars tonight | 0:15:01 | 0:15:04 | |
and if you manage to get any of your own, send them through | 0:15:04 | 0:15:07 | |
and we'll put up a selection on our website. | 0:15:07 | 0:15:09 | |
Now, Mars is an amazing object to view and observe at the moment | 0:15:11 | 0:15:15 | |
but there's plenty on offer around that part of the sky as well, | 0:15:15 | 0:15:18 | |
so here's this month's Star Guide. | 0:15:18 | 0:15:20 | |
Mars is currently rising in the south-east in the constellation | 0:15:20 | 0:15:24 | |
of Virgo as darkness falls, and throughout the month tracks west. | 0:15:24 | 0:15:29 | |
It begins close to the bright white star Spica | 0:15:29 | 0:15:32 | |
and ends the month just south of the middle bright star Porrima. | 0:15:32 | 0:15:36 | |
Porrima sits at the bottom of a large semicircular pattern of stars | 0:15:36 | 0:15:40 | |
known as the Bowl of Virgo. | 0:15:40 | 0:15:43 | |
If you have a telescope, select a low-power eyepiece | 0:15:43 | 0:15:47 | |
and sweep through the region close to the top of the Bowl. | 0:15:47 | 0:15:49 | |
It's known as the Realm of Galaxies. | 0:15:49 | 0:15:53 | |
This part of the sky is full of distant galaxies | 0:15:53 | 0:15:55 | |
which appear like faint smudges. | 0:15:55 | 0:15:58 | |
The region to the left of the bowl | 0:15:59 | 0:16:01 | |
currently plays host to dwarf planet Ceres and minor planet Vesta. | 0:16:01 | 0:16:05 | |
Vesta is currently on the verge | 0:16:07 | 0:16:09 | |
of naked eye visibility from a dark sky site | 0:16:09 | 0:16:12 | |
but both objects are well within binocular range. | 0:16:12 | 0:16:15 | |
Finally, let's return to Mars. | 0:16:16 | 0:16:19 | |
The most distinctive feature you can pick out with a telescope | 0:16:19 | 0:16:22 | |
is known as the Syrtis Major, a large dark V shaped pattern. | 0:16:22 | 0:16:27 | |
The best time to look for it throughout April | 0:16:27 | 0:16:30 | |
is around 11pm between the 18th and the 28th. | 0:16:30 | 0:16:33 | |
More from Mars in a few minutes. | 0:16:39 | 0:16:41 | |
But first, last month we showed you how to take | 0:16:41 | 0:16:44 | |
amazing images of the night sky with a smartphone, | 0:16:44 | 0:16:47 | |
and you've been sharing your results with us. | 0:16:47 | 0:16:51 | |
This image by Andrew Carter shows the Clavius crater | 0:16:51 | 0:16:54 | |
on the moon in fantastic detail. | 0:16:54 | 0:16:56 | |
Paul Newton caught Venus transiting the sun. | 0:16:58 | 0:17:01 | |
And you can make out the shadow of Jupiter's moon Io | 0:17:04 | 0:17:08 | |
in this image by Damian Weatherly. | 0:17:08 | 0:17:11 | |
And Michelle Reitsma managed to capture Saturn and its famous rings. | 0:17:11 | 0:17:15 | |
Now it's time for this month's astro news, and there's been | 0:17:19 | 0:17:22 | |
a lot happening in the astronomical world since we were last on air. | 0:17:22 | 0:17:25 | |
Certainly has. For starters, the solar system has a new member, and here it is. | 0:17:25 | 0:17:30 | |
-This is 2012 VP113. -Snappy! -It will get a better name soon. | 0:17:30 | 0:17:33 | |
But what we can see here is images taken over six hours | 0:17:33 | 0:17:36 | |
and coloured so that you can see that something's moving. | 0:17:36 | 0:17:39 | |
And that's actually a dwarf planet in the outer solar system. | 0:17:39 | 0:17:43 | |
Now this thing's in a really unusual orbit, | 0:17:43 | 0:17:46 | |
much further out than Pluto, 2½ times as far from the sun as Neptune is | 0:17:46 | 0:17:50 | |
and orbiting in a place where it's got no right to be. | 0:17:50 | 0:17:53 | |
The only other thing around there is something called Sedna, | 0:17:53 | 0:17:56 | |
which we found just over a decade ago, | 0:17:56 | 0:17:58 | |
but those two things are on orbits that we can't explain using | 0:17:58 | 0:18:02 | |
conventional solar system mechanics, so it's a very exciting time. | 0:18:02 | 0:18:05 | |
And another potential dwarf planet. | 0:18:05 | 0:18:07 | |
That's right, another dwarf planet, assuming it holds up. | 0:18:07 | 0:18:10 | |
We don't quite know its size yet. | 0:18:10 | 0:18:11 | |
But there have been other weird discoveries | 0:18:11 | 0:18:13 | |
-in the outer solar system as well. -And this time much closer to home. | 0:18:13 | 0:18:16 | |
There was a collection of asteroid-like bodies | 0:18:16 | 0:18:18 | |
that lie between Saturn and Uranus. They're called the centaurs. | 0:18:18 | 0:18:22 | |
And one of these, the largest one, | 0:18:22 | 0:18:23 | |
has actually been discovered to have rings. | 0:18:23 | 0:18:25 | |
This is an artist's impression of it. | 0:18:25 | 0:18:28 | |
So that's the object, and here are the two rings around it. | 0:18:28 | 0:18:31 | |
Now, this was actually discovered in about 20 seconds of data. | 0:18:31 | 0:18:34 | |
Because the asteroid was passing in front of a star | 0:18:34 | 0:18:36 | |
and you get a dip in the light level, an occultation. | 0:18:36 | 0:18:39 | |
Usually with a large object like this, you'll just get a single dip, | 0:18:39 | 0:18:42 | |
but what happened here is they got five, | 0:18:42 | 0:18:44 | |
four little ones and one big one, | 0:18:44 | 0:18:46 | |
which actually was an indication of you're passing through these rings. | 0:18:46 | 0:18:49 | |
It's the first time that we've seen rings on a body this size | 0:18:49 | 0:18:52 | |
and the mystery is, why were they formed, where did they come from? | 0:18:52 | 0:18:56 | |
You just don't get them on things this size. | 0:18:56 | 0:18:58 | |
But I think we'll be looking out for them in the future. | 0:18:58 | 0:19:00 | |
Of course the story dominating the news at the moment | 0:19:00 | 0:19:02 | |
is the results from BICEP2 in the South Pole, | 0:19:02 | 0:19:05 | |
which, if confirmed, could lead to some Nobel Prizes. | 0:19:05 | 0:19:08 | |
But, more importantly, it seems to be telling us about a time | 0:19:08 | 0:19:11 | |
just a ten-million-billion-billion-billionth of a second after the Big Bang, | 0:19:11 | 0:19:15 | |
when something called cosmic inflation took place, | 0:19:15 | 0:19:18 | |
with the universe expanding from a tiny subatomic particle to something | 0:19:18 | 0:19:22 | |
much larger, setting the stage for everything that's happened since. | 0:19:22 | 0:19:26 | |
The idea of inflation was introduced to explain | 0:19:28 | 0:19:31 | |
some oddities about the universe around us. | 0:19:31 | 0:19:35 | |
No matter which direction you look, | 0:19:35 | 0:19:36 | |
on a large scale everything's the same. | 0:19:36 | 0:19:39 | |
You get the same number of galaxies | 0:19:39 | 0:19:41 | |
and the universe is at the same temperature. | 0:19:41 | 0:19:44 | |
It seems like a cosmic coincidence. | 0:19:44 | 0:19:46 | |
What you might expect is a universe that's far lumpier. | 0:19:46 | 0:19:50 | |
The expansion introduced by inflation | 0:19:52 | 0:19:55 | |
means that any lumpiness would be smoothed away. | 0:19:55 | 0:19:58 | |
But, until last month, | 0:19:59 | 0:20:01 | |
we had no direct evidence that inflation took place at all. | 0:20:01 | 0:20:04 | |
One of the leaders of the experiment that may have discovered | 0:20:10 | 0:20:13 | |
the signature of cosmic inflation is Clem Pryke. | 0:20:13 | 0:20:15 | |
Now, to look for the signal, you have to go, of all places, | 0:20:17 | 0:20:20 | |
to the South Pole. So here's your Antarctic telescope | 0:20:20 | 0:20:23 | |
and BICEP2 is actually in this dish here. | 0:20:23 | 0:20:26 | |
Yeah, in this conical-shaped shield is the BICEP 2 telescope itself. | 0:20:26 | 0:20:29 | |
-And why Antarctica? -So we go to Antarctica | 0:20:29 | 0:20:32 | |
because the atmosphere there is fantastically dry. | 0:20:32 | 0:20:35 | |
-Now, this is counterintuitive... -This is water that you're sitting on. | 0:20:35 | 0:20:38 | |
When you get off the plane, you're standing on two miles thick of ice, | 0:20:38 | 0:20:41 | |
10,000 feet of ice, and they tell you it's a hyper desert. | 0:20:41 | 0:20:44 | |
And what little moisture there is in the atmosphere | 0:20:44 | 0:20:46 | |
is in the form of ice and not liquid water. | 0:20:46 | 0:20:48 | |
Liquid water is a killer for these kinds of observations, | 0:20:48 | 0:20:51 | |
because it basically renders the atmosphere opaque. | 0:20:51 | 0:20:53 | |
So essentially we can look straight out into outer space without the atmosphere getting in the way. | 0:20:53 | 0:20:57 | |
OK, and you're looking at the cosmic microwave background, | 0:20:57 | 0:21:00 | |
the oldest light we can see. | 0:21:00 | 0:21:02 | |
Here's an image of the whole sky in microwaves and it's a picture | 0:21:02 | 0:21:06 | |
of the universe as it was, what, 400,000 years or so | 0:21:06 | 0:21:09 | |
after the Big Bang. | 0:21:09 | 0:21:10 | |
Right, so these blobs, these hot and cold spots, | 0:21:10 | 0:21:12 | |
red and blue spots, are places where there's a little more matter | 0:21:12 | 0:21:16 | |
and a little less matter. | 0:21:16 | 0:21:18 | |
And these blobs actually evolved into the galaxy clusters | 0:21:18 | 0:21:21 | |
and galaxies that we see in the universe today. | 0:21:21 | 0:21:24 | |
Now, what BICEP2 has given us, or seems to have given us, | 0:21:24 | 0:21:27 | |
is the first evidence, first direct evidence, for this inflation. | 0:21:27 | 0:21:31 | |
So what is it in this light that gives you this signal? | 0:21:31 | 0:21:34 | |
So inflation was already a popular theory, | 0:21:34 | 0:21:38 | |
but in some sense it was kind of made up to fit observational facts. | 0:21:38 | 0:21:42 | |
But what it also does is made an additional prediction | 0:21:42 | 0:21:44 | |
which was not observed, which hadn't been observed... | 0:21:44 | 0:21:47 | |
And this is to do with gravitational waves, ripples in space. | 0:21:47 | 0:21:50 | |
Essentially ripples in space-time. | 0:21:50 | 0:21:52 | |
So, that was an additional prediction, | 0:21:52 | 0:21:54 | |
so when you have a theory, | 0:21:54 | 0:21:55 | |
which is a very nice theory, a lot of people like it, | 0:21:55 | 0:21:58 | |
-you want to find some prediction that it makes that you can additionally go and check. -Right. | 0:21:58 | 0:22:01 | |
And that's... So the detection of these gravitational waves | 0:22:01 | 0:22:04 | |
-has been called a smoking gun for inflation. -Right. | 0:22:04 | 0:22:07 | |
Now what they do is they impart on the polarisation pattern | 0:22:07 | 0:22:10 | |
of the microwave background a small additional signature, | 0:22:10 | 0:22:14 | |
-a small degree of swirliness, as it were. -OK, so let's have a look. | 0:22:14 | 0:22:17 | |
This is the patch of sky, | 0:22:17 | 0:22:19 | |
this is the BICEP2 result with that swirliness | 0:22:19 | 0:22:22 | |
that we were talking about, | 0:22:22 | 0:22:23 | |
-so these little arrows are the polarisation signal. -Right. | 0:22:23 | 0:22:27 | |
But here we've subtracted out the expected part, as it were, | 0:22:27 | 0:22:30 | |
and we are left with the so-called B-mode, | 0:22:30 | 0:22:32 | |
which is the swirliness of the pattern. | 0:22:32 | 0:22:34 | |
Only gravitational waves, crucially, only gravitational waves, | 0:22:34 | 0:22:37 | |
can make the swirly part of the pattern. | 0:22:37 | 0:22:39 | |
And so it's the detection of this swirliness is the signature | 0:22:39 | 0:22:42 | |
of that inflationary moment. | 0:22:42 | 0:22:44 | |
It's the signature of gravity waves, | 0:22:44 | 0:22:46 | |
and the only plausible source for such strong, | 0:22:46 | 0:22:48 | |
relatively strong gravitational waves, is the inflationary theory. | 0:22:48 | 0:22:52 | |
The competing theories don't predict... | 0:22:52 | 0:22:54 | |
So that's why this is such an exciting result. | 0:22:54 | 0:22:57 | |
I think you were surprised by the signal, weren't you? | 0:22:57 | 0:22:59 | |
Not that necessarily it was there, | 0:22:59 | 0:23:01 | |
but it was stronger than some people thought. | 0:23:01 | 0:23:03 | |
Yeah, so it's perhaps about as strong as was originally | 0:23:03 | 0:23:07 | |
expected from the simplest inflationary theories, | 0:23:07 | 0:23:09 | |
the ones that were formulated back in the '80s. | 0:23:09 | 0:23:12 | |
Since then, more sophisticated theories | 0:23:12 | 0:23:14 | |
have tended to predict lower levels, | 0:23:14 | 0:23:16 | |
so this week's result was quite a surprise. | 0:23:16 | 0:23:18 | |
There must be personal satisfaction in this. | 0:23:18 | 0:23:20 | |
People have been talking, it's too early to talk about this, | 0:23:20 | 0:23:23 | |
but people have been talking about Nobel prizes | 0:23:23 | 0:23:25 | |
and speculating and so on. | 0:23:25 | 0:23:26 | |
Do you wander round the lab, late at night, thinking, | 0:23:26 | 0:23:28 | |
"Well, you know, maybe this is it"? | 0:23:28 | 0:23:31 | |
Well, it's only been a week. | 0:23:31 | 0:23:33 | |
But before that, we were just very focused on doing | 0:23:33 | 0:23:36 | |
the most careful possible job that we could in the data analysis | 0:23:36 | 0:23:40 | |
and just really being as sure as we possibly could be. | 0:23:40 | 0:23:42 | |
Very nerve-racking, actually, to be sitting on something like this. | 0:23:42 | 0:23:45 | |
-Yeah. -Quite stressful. -All right, well, we'll let you get back to it. | 0:23:45 | 0:23:49 | |
-Thanks a lot. -Thank you very much. | 0:23:49 | 0:23:50 | |
Now back to Mars. | 0:23:56 | 0:23:58 | |
And a mission that's been planned to take our exploration of the planet | 0:23:58 | 0:24:01 | |
to a whole new level. | 0:24:01 | 0:24:03 | |
The European Space Agency ExoMars mission is aiming to be | 0:24:03 | 0:24:07 | |
the first rover to directly search for life on the Red Planet. | 0:24:07 | 0:24:11 | |
It will be equipped with a drill that will let it dig two metres | 0:24:13 | 0:24:16 | |
below the Martian surface | 0:24:16 | 0:24:18 | |
to a level protected from deadly solar radiation. | 0:24:18 | 0:24:21 | |
If all goes to plan, it will be travelling to Mars in 2018. | 0:24:23 | 0:24:27 | |
I'm currently standing on what appears to be | 0:24:28 | 0:24:31 | |
a patch of the Red Planet right here on Earth. | 0:24:31 | 0:24:34 | |
This is the Mars Yard, built by Airbus, | 0:24:34 | 0:24:37 | |
to test the ExoMars rover, and put it through its paces. | 0:24:37 | 0:24:40 | |
Now, that's really necessary, | 0:24:40 | 0:24:42 | |
because ExoMars is going to go to a very alien environment. | 0:24:42 | 0:24:45 | |
I've got Abbie Hutty here, | 0:24:45 | 0:24:47 | |
who's the structural engineer on the ExoMars project. | 0:24:47 | 0:24:50 | |
So what are the challenges that ExoMars | 0:24:50 | 0:24:52 | |
will face on the real Martian surface? | 0:24:52 | 0:24:54 | |
One of the first things that we've got to consider is that | 0:24:54 | 0:24:57 | |
Mars is really very cold, so we've got night-time temperatures | 0:24:57 | 0:25:00 | |
that go down to -125 degrees Celsius. | 0:25:00 | 0:25:03 | |
-That's brisk! -Yeah, a little bit chilly. | 0:25:03 | 0:25:05 | |
Then during the day it might not even get much warmer than -85, | 0:25:05 | 0:25:09 | |
so you're going all the way between those two, and materials, | 0:25:09 | 0:25:13 | |
as we know, expand and contract | 0:25:13 | 0:25:15 | |
as they go through the different temperatures. | 0:25:15 | 0:25:18 | |
That's especially a problem where you've got structures that might | 0:25:18 | 0:25:21 | |
be made of more than one different type of material, | 0:25:21 | 0:25:23 | |
because where those two materials meet, | 0:25:23 | 0:25:25 | |
they actually just tear themselves apart from each other. | 0:25:25 | 0:25:28 | |
I guess radiation is a problem, too? | 0:25:28 | 0:25:30 | |
Well, yes, we've only got 1% of the atmosphere on Mars | 0:25:30 | 0:25:34 | |
to what we have on Earth, so down on the Martian surface, | 0:25:34 | 0:25:37 | |
you are receiving a lot more of that radiation dose | 0:25:37 | 0:25:40 | |
and that can be really damaging for your electronics | 0:25:40 | 0:25:42 | |
and also for optical devices, | 0:25:42 | 0:25:44 | |
like lenses can blacken with that radiation dose | 0:25:44 | 0:25:48 | |
and that can obviously have a huge impact on how far you can see | 0:25:48 | 0:25:52 | |
or your senses that require those optics. | 0:25:52 | 0:25:55 | |
So, this is a prototype called Bryan, | 0:25:55 | 0:25:58 | |
one of a series of prototypes | 0:25:58 | 0:25:59 | |
and, looking at it, the wheels are a bit freaky. | 0:25:59 | 0:26:02 | |
-How do these work? -Well, we've actually had to | 0:26:02 | 0:26:05 | |
develop these specifically for the Mars project | 0:26:05 | 0:26:07 | |
because we can't take rubber tyres with us. | 0:26:07 | 0:26:10 | |
Rubber is an organic molecule. | 0:26:10 | 0:26:12 | |
Yes, and you are looking for signs of life. | 0:26:12 | 0:26:14 | |
Absolutely, so we've got very strict regulations in place | 0:26:14 | 0:26:17 | |
to make sure that we don't take anything with us | 0:26:17 | 0:26:19 | |
that could be in any way confused for an organic molecule. | 0:26:19 | 0:26:22 | |
So we have developed these wheels. | 0:26:22 | 0:26:24 | |
They are entirely metallic, | 0:26:24 | 0:26:26 | |
but you've also got to retain the flexibility of the wheel... | 0:26:26 | 0:26:28 | |
That you'd get from rubber. | 0:26:28 | 0:26:30 | |
..so we've got these very thin wafers of metal | 0:26:30 | 0:26:33 | |
that actually are still flexible because they are so thin. | 0:26:33 | 0:26:37 | |
But how do you navigate across the Martian surface? | 0:26:37 | 0:26:39 | |
Well, that's one of the really big developments with ExoMars | 0:26:39 | 0:26:42 | |
and that is one of the reasons that we've got this Mars Yard here. | 0:26:42 | 0:26:45 | |
Because you've got such a long-distance to Mars, | 0:26:45 | 0:26:48 | |
it means you've actually got a 22-minute delay | 0:26:48 | 0:26:51 | |
between sending your signal and it being received, | 0:26:51 | 0:26:53 | |
so all of our rovers are going to be able to | 0:26:53 | 0:26:56 | |
actually autonomously navigate around the surface. | 0:26:56 | 0:26:59 | |
We've got two cameras at the top of the mast so we can see in 3-D. | 0:26:59 | 0:27:02 | |
It can build up a map of how big the obstacles are | 0:27:02 | 0:27:07 | |
and where they are in front of it and then it can actually classify | 0:27:07 | 0:27:10 | |
the different areas into, | 0:27:10 | 0:27:12 | |
"This is too big a rock, I can't climb over this," | 0:27:12 | 0:27:14 | |
or, "This is a safe, flat bit, this is good to climb over," | 0:27:14 | 0:27:16 | |
and then it can pick its own path through that map. | 0:27:16 | 0:27:20 | |
Well, I can't wait until ExoMars gets to Mars | 0:27:20 | 0:27:22 | |
and thank you so much for sharing this with us. | 0:27:22 | 0:27:24 | |
-Absolutely, it's been a pleasure. -Thank you. | 0:27:24 | 0:27:27 | |
Now for that special treat we mentioned earlier. | 0:27:33 | 0:27:35 | |
The team behind the HiRISE camera | 0:27:35 | 0:27:37 | |
that showed us the amazing images earlier in the programme | 0:27:37 | 0:27:40 | |
are giving you the opportunity to take control | 0:27:40 | 0:27:42 | |
and select the location for the next image of Mars. | 0:27:42 | 0:27:45 | |
It's a spectacular opportunity | 0:27:45 | 0:27:47 | |
and what we need is a scientific justification for your choice, | 0:27:47 | 0:27:50 | |
so it could be an unusual formation, | 0:27:50 | 0:27:52 | |
some strange colours, or maybe a famous place | 0:27:52 | 0:27:55 | |
that you would like to see for the first time with HiRISE resolution. | 0:27:55 | 0:27:58 | |
To take part, you can go to our website and tell us | 0:27:58 | 0:28:01 | |
where you think the camera should be pointed. | 0:28:01 | 0:28:03 | |
We will close the entries on 27th April | 0:28:03 | 0:28:06 | |
and we will announce the winner in next month's programme. | 0:28:06 | 0:28:09 | |
It's a fantastic opportunity, so please do enter. | 0:28:09 | 0:28:13 | |
Well, we can't leave you without showing one last image | 0:28:13 | 0:28:15 | |
from the Martian surface and here it is. | 0:28:15 | 0:28:19 | |
This is an image taken by the Curiosity rover on 31st January. | 0:28:19 | 0:28:23 | |
Rising high in the Martian sky is a fabulous evening star. | 0:28:23 | 0:28:28 | |
But that is no star, that is Earth and I find it wonderful and humbling | 0:28:28 | 0:28:32 | |
that we can see ourselves in the sky of an alien world. | 0:28:32 | 0:28:36 | |
It is a fantastic image, but that's it for this programme. | 0:28:36 | 0:28:39 | |
Next month, we will be coming from the Brecon Beacons AstroCamp, | 0:28:39 | 0:28:42 | |
where we will be looking deep into space. | 0:28:42 | 0:28:44 | |
And you will also have the chance to discover your very own asteroid | 0:28:44 | 0:28:47 | |
as part of a real scientific search for near-Earth asteroids. | 0:28:47 | 0:28:51 | |
-So, until then, get outside and get looking up! -Good night. | 0:28:51 | 0:28:56 |