Episode 3 Stargazing Live


Episode 3

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What a week we have had a Jodrell Bank. When we went hunting, we never

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thought we would see this. The glorious colours of the Northern

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lights. Or the extraordinary event of the sun bursting particles the

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waters. All along you have been searching the galaxies and you have

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made a remarkable discoveries, and you've had a glimpse of event that

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happened 11 million years ago. I am Brian Cox, he is Dara O'Briain, and

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this is Stargazing Live. Welcome back to Stargazing Live.

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Let's get straight onto the most exciting news of the series - an

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amazing discovery made by you over the last three nights. We asked you

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to search for hidden galaxies. And not only have you been successful

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but what you've discovered is of genuine scientific importance. So

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much so that some of the biggest telescopes around the world,

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including this one, have dropped everything to focus on what you've

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found. This is why it is pointing in this direction, it is tracking one

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of the things you found because it is so interesting. Here to tell us

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more is Chris Lintott. What did our viewers need to do? We asked people

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to look for gravitational lenses, the light where it has been bent by

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more nearby galaxies, and that bending of light means we see

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further into the past and we see distant galaxies we would not be

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able to see. You said you were hoping to get 500,000 hits by

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Thursday. We broke that easily, so now we are at 6.5 million

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classification is made by 50,000 Stargazing Live viewers. Such a big

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response that the professional community have got involved. It's

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not only the Lovell we have taken over. It's not just the quantity or

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the classifications, it's they found wonderful things. We have more 50

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candidate gravitational lenses, and we've used some of the biggest

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telescopes in the world. A genuinely global initiative. Let's go over to

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the UK, because how many telescopes there? We have used the Lovell

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telescope, and even as far away as Cambridge to track one of the

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candidates. Six radio telescopes working in congruence. One of the

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more interesting targets is is there. Over the course of the

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evening, excitement gathered, and other people in America join this.

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We got data in America, archive data, from West Virginia, the

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greenback telescope. We called our friends in Hawaii because we wanted

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to get optical and infrared data must be called the biggest telescope

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in the world. It is Hawaii but you are 13,000 feet in the mind him. The

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dome was frozen shut. They hacked away at the icicles chorus. The

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director of the Institute have away so we could get the data -- for us.

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We don't recommend you do this at home, but we were late in the bar

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last night, and we rang up the Greenback telescope. I also saw you

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ringing Chile. We called the Canary Islands, but it was snowing, but we

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still call them. They have been trained on one target in particular,

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and we will talk about that later. It's all because of the effort of

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Stargazing Live view is that we've done it. We are contributing to the

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sum total of human knowledge rather than the usual television thing.

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This is real star. Real science. We have also been getting astounding

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images sent over in the last couple of days. Look at this one. The moon,

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but a beautiful photograph by Julian Cooper from the Black Country. Also

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beautiful photos of this sunspot group. Again, this is the thing that

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gives us the possibility of Aurora Borealis tonight. We gave a

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prediction of the time that the burst of energy might arrive. That

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might not have been exactly right and we might still be waiting. It is

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ongoing. We have space observatories up there and we think it might

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arrive now. I want to show you a couple more. This is a bit of a

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cheat. We talk about amateur imagery is -- images, but this is a

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beautiful picture from Reykjavik, in Iceland. Just a few moments ago in

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Norway, Liz Bonnin took to the skies to see if any of the recent activity

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on the sun is producing any Aurora yet. How is it looking, Liz? Welcome

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back to a world first, Aurora hunting. We are crammed into a

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plane, and the equipment is working nicely. Pete Lawrence is with us on

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the flight, so let's take a look outside the window. In the last ten

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minutes, this beautiful site revealed itself. A lot of structure

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and beautiful curls at the bottom of it. Very bright tonight, isn't it?

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Very nice. Lots of structure. It's been changing as we have watched out

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of the window, lots of vertical rays. Am I wishful thinking, or can

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I see some red and brown? I can see some red at the right. That is a

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first, and we're excited about it. Let's talk about the forecasting we

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had last night. Has the corona hit the earth? What has changed between

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last night and now? It hasn't hit us. It's hard to forecast the

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arrival, and it got slow down as it headed from the sun towards us. It

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could arrive anywhere between now and 4am. It could still affect this

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beautiful light display we see tonight? Absolutely. That is the

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beauty of space weather. The aurora changing all tonight. I will leave

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you with that beautiful image, a sight for sore eyes. See you in a

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bit. Seeing different colours within the Aurora, as we have. You can see

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the red on the right, but if that is the immediate, who knows what will

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happen? There have been special Stargazing Live parties taking place

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up and down the country, and there is one in Egham, in Sussex. A

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wonderful evening at Royal Holloway University. Thousands of excuse you

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asked it -- enthusiastic stargazers, are you having a good time? What has

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that been the best thing so far? I think it was the DIY. What do you

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look forward to seeing next? Tourists in space. That is the thing

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about this, they're so many things going on. There is the option also

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to see yourself in infrared, and there is an army of astronomers and

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telescopes to look at the sky. We've even set up a field of astronomers

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away from the light so we can take some wonderful views of what the

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clear sky has to offer. And I will also show you how you can find

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galaxies through your own telescope and how to navigate through the

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stars. Back to the studio. Lots of young faces in the studio. Those

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youngsters seem to be the new co-hosts, and I know how you feel

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about this out region getting involved. Getting kids excited about

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astronomy leads to so many other things, entrepreneurialism, careers

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in science. I remember when I was about three years old watching the

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Clangers. And we are yet to find them! The great thing about them was

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the row of kids about seven or eight years old, and that is what

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astronomy did for me, and I went into physics and I caught the bug.

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Your career has been mainly based on space hardware, mainly the James

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Webb telescope, a tremendous telescope. It is amazing. It will

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travel 1.5 kilometres away from Earth and then deploy, which looks

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challenging, but what comes out is a heat shield visit and infrared

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telescope and the biggest source of heat nearby the son, so it hides

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behind the earth and it protects it from some of the sun and it has

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Earth radiation. This is the heat shield, then? It's about the size of

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a telescope. It's going to be launched in about 2018, hopefully.

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We see the golden mirror, so what is the difference between that and the

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Hubble telescope? The Hubble telescope was mainly optical, but

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the James Webb is infrared, so it gets orange and red and the rest is

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infrared. But why? We have pictures of the Milky Way, so what is it that

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the James Webb gives us? It was called a next-generation space

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telescope. Mind you, it is coming from a long way. We can see the

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Milky Way galaxy, but here you can see the patches of dust, and of

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course a visible light, optical light, which doesn't past -- passed

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through it. But with the infrared you can see what is behind. An

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interesting look at the centre of the galaxy, the black hole obscured

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by the dust. What I find fascinating is that when people think of

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telescopes they think of visible light, but we have an amazing piece

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of equipment, a radio telescope, and the James Webb is infrared. We take

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parts of the Informatics spectrum and get a broader picture of what is

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out there. This will be coming back to earth and we will see later.

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There is a huge question about the Milky Way that spin around for

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hundreds of years, but Simon Taylor of Runcorn has sent things in over

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the last two years, and asked, if we've never been outside the Milky

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Way, how do we know what it has been looking like? Let's find out. On a

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clear, moonlit night you can see a milky glow across the night. The

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Romans called it a milky road, and when Galileo pointed his telescope

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at it, he discovered that this haze of light was in fact made up of

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distant stars. When we look out into the night sky, we see the stars and

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the glowing gas and dust which are bound together by gravity and make

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the galaxy, which we call the Milky Way. But because we are in it, it's

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very hard to work out what the shape of the galaxy actually is. One of

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the first attempts to map the galaxy was from astronomer William Herschel

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in 1785. What needed was to assume that all of the stars we can see the

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sky are roughly of the same brightness and it uniformly

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distributed. By doing that, he came up with a map, which is the shape of

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the known universe of the time. Now, this is not accurate, the many

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reasons. But one of them is that there are many stars in the Milky

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Way galaxy that cannot be seen from Earth because they are obscured by

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dust. No one appreciated the children -- true extent of the Milky

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Way until tools were developed to help them peer through the dust. In

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1955, the Stargazing Live -- Lovell telescope was built at Jodrell bank,

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and it did not look at Starlight, but was designed to capture radio

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waves. While visible light is easily blocked by dust, radio waves

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emanating from the furthest reaches of our galaxy can pass through.

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Clive Dickinson is an astronomer who choose into these electromagnetic

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waves from our Milky Way. -- choosing. -- tunes in. Obviously

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there are lots of stars in the galaxy, but when you look with the

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radio waves you get a different picture. You can still see the

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galactic plane, but you can also see completely different things, and

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different objects and different structures. What is revealed is that

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the space between the stars is far from empty. It is filled with gas,

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mostly hydrogen. And because radio telescopes can detect waves emitted

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by the hydrogen gas, they can be deduced to work out the shape of the

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Milky Way. This is a map of the hydrogen gas in our galaxy that was

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first made in the 1950s, and the hydrogen follows the distribution of

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stars in the galaxy. By measuring the velocity of that gas, and the

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brightness in any direction, you can deduce that the Milky Way is, in

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fact, a giant spiral of stars. But astronomers are now mapping more

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than hydrogen. These brands in new views of our galaxy show other

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components in our Milky Way, including the dust that obscure

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would their view 200 years ago. By combining these results, we are

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finally beginning to build a picture of what the Milky Way looks like. A

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disc of hundreds of billions of stars, gas and dust, swirling around

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a central bar into the most beautiful spiral galaxy.

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We know enough now to take an educated guess at what the Milky Way

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looks like. About 27 light-years from the centre. But the most

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distinctive features of the spiral arms. They are the focus about one

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of the big debates about the Milky Way. How many arms are there and

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what pattern do they form? That is one thing the team here at Jodrell

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Bank have been studying. Professor Tim O'Brien is here. You have one of

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your telescopes scanning? The severed meter telescope has been

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scanning through the Milky Way and I have a live signal from it now. What

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you are seeing in this spectrum which is updated in real-time, the

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peaks in the middle are from hydrogen atoms in the spiral arms of

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the Milky Way. There is a peak along the side which is a second arm. It

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indicates a cloud of hydrogen gas as we look through the disc of the

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Milky Way. Each produces a peak in this spectrum. We just talked about

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the infrared, this is the 21 centimetre? Yes, it is the same

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thing Maggie mentioned, there is dust and it makes it difficult to

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see through it. What is this image? It is a scan we did earlier. You see

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these patterns, each of these spikes is a spiral arm. I can see three

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arms for example. It seems to reveal it into arms and three arms? It is

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difficult to see the structure of the Milky Way from inside. We were

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aware of four of them, and then there was a paper that said there

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were just two, now they reckon there are four of them again. This

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telescope, we have taken over. It is not looking it's beautiful self. But

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it is pointing at an interesting object? But beside the moon, there

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was an object discovered by our view was the other day that is billions

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of light years away. We will be showing you that later. It is not

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the only galaxy you can see from Earth. Mark Thompson can show you

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how to see our closest galactic neighbours.

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We have wonderful clear skies. The party and come local astronomers. I

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want to show you this wonderful moon. We are here to spot as many

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galaxies as we can. We shot this video in Norfolk a few days ago that

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the Andrew Meda galaxy. Jamie, what can you say? I can see a bit of a

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blur. If you look to one side, you can use a technique called averted

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vision. Have another look. Is that better? Can you see the spiral

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nature of the galaxy? Yes. It is wonderful, you are looking back in

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time, 2.5 million years. It is a weird concept. You can see it with

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binoculars and you can see it in the south-west at this time of year. I

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will leave you to enjoy that. There are a couple of other galaxies you

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can see tonight. We had some footage we took about half an hour ago

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called M81 if we look through the Hubble telescope, it looks

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spectacular. It is visible just above the plough at this time of

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night. If you want to bind the details you have two June into my

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Starcast. This is a view of M82 sometimes you can see the two

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galaxies through one telescope will stop with the big Hubble telescope,

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we get some wonderful views, sharing the turbulent nature in that galaxy

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where loads of new, young stars are starting to form. That is all we can

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see for tonight. If it is clear where you are, get outside and see

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how many galaxies you can spot. You can find information on our website.

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Now back to Brian and Dara O'Brian. We are about to explore a galaxy in

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more details. There is a new mission underway set to revolutionise our

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knowledge of the Milky Way. The chief K scientist behind this is

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Professor Gerry Gilmore. We spoke to Caroline about the nerve wracking

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nature of space exploration. What did you feel? I was there. It is an

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interesting experience. There was perceptible relief when it opened up

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and it was working. It is not just the money it is the 20 years of work

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from the 400 engineers. Tell us about the mission? GAIA is designed

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to answer the questions you were asking. It is a shield half the size

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of a tennis court, but it is a big camera and to telescope will stop it

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is taking a video of the sky for five years and will measure the

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distance of a billion objects. This is exquisite UK technology. They are

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cameras? Every one of these things is a bigger version of what you have

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in your telephone. This is only half of it. You have two touch them

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carefully. In terms of an eight megapixel camera, what is that? It

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is a Ilion pixel camera. It is very sensitive, thousands of times more

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sensitive in terms of dynamic range and quality of anything that has

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ever been made before. We need that to get that exquisite position GAIA

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is designed to get. If you put a human hair in space, this thing can

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see either side of it? From London. GAIA will locate the stars. It is

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the equivalent of locating a small coin on the moon. Also how they are

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moving? Yes, we keep doing this for five years and see how it moves. It

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allows us to measure the distance of the object. We can see where all of

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these objects are in 3-dimensional. Also how everything is moving. When

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we walk through space and we can see what is there, and where it really

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is, but how those things are moving and from that we can deduce the

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entire formation of the Milky Way and that is what GAIA is. What

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affect will this have on the industry? GAIA will rewrite the

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textbooks. People have studied with these giant telescope because they

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knew it was interesting. We haven't done that for a billion objects

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before. So GAIA will do it for a billion objects and tell us what

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looks normal. How did the Milky Way get to be the way it is? We have a

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video from last year and one of the theories. We know the Andromeda

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galaxy, one with about a trillion stars is coming towards us quite

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quickly and is going to hit us. The debate is that it has hit us before?

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That is one of the questions GAIA is designed to answer. We can

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understand one, then we have a Rosetta Stone for all of them. To

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answer that question we need to know not only were the galaxies are now,

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so GAIA will tell us that, we also need to know how much they weigh.

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That is the unique thing with GAIA. We can introduce weight, so we know

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for the first time, not only what we can see, but everything that is

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there. It is an incredible project. We will be talking to you later. In

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a moment we will be revealing a new galaxy you have discovered, but last

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night Brian looked at how we might fuel a starship puckered

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transporters to the stars as close to the speed of light. What about

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the astronauts on board? I were to find out what it would feel like.

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To travel anywhere fast, first you have to accelerate. Apparently this

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car can go from zero to 60 mph in just six seconds. Acceleration

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creates the force that pins at you back in your chair whenever you

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change speed. And in small doses... It is a lot of fun. However, to get

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to the kind of speeds you need for intergalactic travel, you can have

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too much of a good thing. So, would my body stand any chance of handling

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the kind of acceleration needed to reach near lightspeed? To find out,

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I have come to brook city based in San Antonio in Texas. Hidden inside

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building 170 is a machine of torture. In it, over 100 astronauts

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have learned to endure the extreme acceleration of a space shuttle

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launch. It is a human centrifuge. And today, it is my turn to take a

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ride. How are you? This man is lead centrifuge technician. Basically I

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am in a space shuttle launch? Yes, we will go through the same protocol

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the astronauts go through. The centrifuges is going to spin me ever

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faster, subjecting me to the crushing force. What can the body

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take? The G will be pushing on your chest. I won't feel more sure is, I

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won't feel ill? I hope you don't. Will I feel all of my limbs heavier?

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Your ear lobes, your eyelids, everything will feel three times

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heavier. It is heavy enough as it is! Wow! This is amazing. At maximum

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acceleration, reducing 3G, my body will feel three times heavier than

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normal. It takes shuttle astronauts seven seconds to reach the speed.

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Obviously they are trained professionals. Three, two, 1...

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Liftoff. You are at 2.5 G. This is about as

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much as the shuttle or anyone on board can take for more than a few

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seconds. I am beginning to see why. It may not look it, but my arm feels

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as heavy as a bag of cement. Wave to the camera. That is getting

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uncomfortable and it would take months to get to lightspeed at this

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rate. That is not good enough, we need more G. Would you like us to

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take you 25 G for ten or 15 seconds just to see what it feels like? Go

:29:54.:30:13.

on then. 2.5, three. 4.5 and we are at five, how does it feel? Tough

:30:14.:30:23.

will stop back down now. That is tough. It is amazing. No way you

:30:24.:30:32.

could do anything at five G. Can't even talk. It would not be very

:30:33.:30:40.

flattering. He has been laughing at this all day. It is unflattering.

:30:41.:30:45.

This famously good-looking man in a centrifuges, this is what he looked

:30:46.:30:53.

at stop that was at seven. You look like an old woman out of correlation

:30:54.:31:01.

Street. Now back to Liz. What is in the sky above you? You

:31:02.:31:05.

have no idea what you have been witnessing.

:31:06.:31:12.

We were giddy, applauding and at one point we were circled by this stuff.

:31:13.:31:17.

The sky is filled with Green. There was a pink border at the bottom. It

:31:18.:31:22.

is changing every second. What have we been looking at? I have lost

:31:23.:31:27.

track of the amount of movements, the red and the pink. It is

:31:28.:31:33.

glorious. It gets confusing doesn't it? You can see how the bands fold

:31:34.:31:38.

upon themselves. They wrap around and you get various struck just. It

:31:39.:31:46.

looked like a cascade of light. We have some footage from a few moments

:31:47.:31:52.

ago. It was a multilayered, multi-structural, if that is the

:31:53.:32:07.

right terminology. I am overwhelmed, it is mind blowing, I never expected

:32:08.:32:12.

to see such beautiful displays. The fantastic thing was it that was

:32:13.:32:17.

moving dynamically. The ripples of light moving through the whole

:32:18.:32:22.

display. People describe the Aurora is a dance across the sky, and we

:32:23.:32:27.

have witnessed it, it is glorious. With regard to the different shapes,

:32:28.:32:31.

are they ever in a certain order or does it happen haphazardly? Those

:32:32.:32:39.

bright bands are characteristic, and what happens is they fold up on

:32:40.:32:42.

themselves and it gives the impression of a curtain hanging in

:32:43.:32:46.

the sky. They can also wrap up into a huge spiral structure and they

:32:47.:32:51.

look amazing. They are enormous, and go up to about 1600 kilometres. We

:32:52.:32:58.

can see it now, it is a little more diffused, but they are vertical,

:32:59.:33:03.

streaking through the colour. What is that? They are bits of the

:33:04.:33:09.

curtain which folds up on themselves. When you look from the

:33:10.:33:13.

side, you look through multiple layers of light, so they look

:33:14.:33:17.

brighter than the rest of the Aurora, and those are called Reyes.

:33:18.:33:22.

I have heard about the crowns as well. What are they? You see the

:33:23.:33:28.

rays going up vertically, but if you're underneath, and you look up,

:33:29.:33:32.

you can see those rays going up several hundred kilometres into the

:33:33.:33:36.

night sky, and via perspective they converge together, that is the

:33:37.:33:41.

Aurora Crown. On the right-hand corner of the screen we can see a

:33:42.:33:47.

new bright bit of green that defuses upwards. It is very much in real

:33:48.:33:52.

time, this is the beauty of the cameras, we can see it as it happens

:33:53.:33:57.

without a need for time-lapse. Guys, we are besides ourselves. As you can

:33:58.:34:01.

imagine from my boys. Please come back to us soon because we will try

:34:02.:34:07.

to get more footage -- as you can imagine from my voice. You can tell

:34:08.:34:14.

that you was quite overwhelmed. It is beautiful. That demonstrates the

:34:15.:34:20.

power of the stars. We think of it giving light and heat, but it is a

:34:21.:34:24.

magnetic field that is influencing particles from the stars and

:34:25.:34:28.

reaching out across 90 billion miles and causing the atmosphere to light

:34:29.:34:34.

up. It is beautiful. You say all that, and I am thinking Mavis Riley,

:34:35.:34:38.

the old woman from Coronation Street. You look like Mavis Riley, I

:34:39.:34:47.

am like Eric pickles. -- Pickles. We have been building up this discovery

:34:48.:34:53.

all night, but it's quite a big one. Let's look at the images that the

:34:54.:34:57.

viewers were the first to find. Six people on the first night saw a

:34:58.:35:02.

close-up of the image, so let's zoom in on the galaxy. This is the

:35:03.:35:05.

infrared image we showed people, and you can see that lens. There were

:35:06.:35:18.

six people on the very first night is spotted this. You are looking at

:35:19.:35:24.

the nearby galaxy, a couple of billion light years away, so nearby

:35:25.:35:30.

in astronomy terms. This red ring, I think it is a ring, that is a

:35:31.:35:33.

distant galaxy and we are seeing that as it was about 11 billion

:35:34.:35:41.

years ago. To be clear, the light from the galaxy, 11 billion light

:35:42.:35:46.

years away. Well, further than that, so it's actually about 40 billion

:35:47.:35:53.

will -- years away. The starters, we are looking back at when the

:35:54.:35:58.

universe was getting going -- for starters. This galaxy is quite big.

:35:59.:36:02.

It's very active, and we know it is forming stars at a rate of about 100

:36:03.:36:07.

times that of the Milky Way, so about a hundred huge stars every

:36:08.:36:13.

year. The really exciting thing is what happens when we switch to the

:36:14.:36:17.

radio. We will show you the radio image, and the scientists we work

:36:18.:36:22.

with haven't seen it yet and we wanted to share this with all of the

:36:23.:36:27.

collaborators. So this is from a little telescope, five other

:36:28.:36:31.

telescopes. If you are a professional astronomer, this is

:36:32.:36:36.

exciting. This blog here is the result of yesterday evening's

:36:37.:36:42.

observations. -- this blob. It shows is a nice narrow arc, so perfectly

:36:43.:36:49.

convincing as a lens, but there is more radio emission here than we

:36:50.:36:54.

expected. Brighter than we expected. An unusual object, in that sense? We

:36:55.:37:01.

get the Radio 2 ways, from the young stars. We can predict that, but we

:37:02.:37:06.

might also get it from the gas spiralling in and growing a black

:37:07.:37:09.

hole at the centre of the galaxy. We are watching the early stages of the

:37:10.:37:14.

galaxy. It might be young galaxies merging together. This kind of black

:37:15.:37:21.

hole normally means a collision, so these could be proto- galaxies.

:37:22.:37:27.

Billions of years ago as well, so close to the beginning of the

:37:28.:37:32.

universe. We still have to name it, and we want you to do that as well,

:37:33.:37:38.

so please send suggestions. The only thing is that it needs to have the

:37:39.:37:43.

number nine at the stars. We will give you a decision on that and we

:37:44.:37:46.

will have it by the end of the show. And that will be its name. There

:37:47.:37:51.

will be scientific papers with the name on it, and that's wonderful. To

:37:52.:37:56.

find out what the conditions are like for stargazing outside, here is

:37:57.:38:03.

Helen Willetts. It was not the best weather for getting out Stargazing

:38:04.:38:07.

Live, but I can tell you there are going to be more clear skies

:38:08.:38:11.

tonight. It won't be warm if you head out and about, widespread frost

:38:12.:38:15.

coming and icy patches, and some patchy cloud, but if we are lucky

:38:16.:38:22.

enough to see Aurora Borealis, and talking to my colleagues at the

:38:23.:38:25.

space centre, it could arrive, we might see it in northern England and

:38:26.:38:28.

Northern Ireland, but if we don't see it, plenty more to look at in

:38:29.:38:32.

the sky and we should have plenty of clear skies. Come tomorrow, there

:38:33.:38:38.

will still be cloud across southern and eastern areas, but for many,

:38:39.:38:42.

with the cold light, it could be clear and plenty to see. If you are

:38:43.:38:48.

not lucky enough to see Aurora Borealis, Jupiter is meant to be

:38:49.:38:51.

bright in the sky, and the good news is that into the weekend, Friday and

:38:52.:38:55.

Saturday, it looks clearer, but it will be cold, so wrap up warm.

:38:56.:39:01.

Mark is under the stars in egg, with a huge crowd of other stargazers.

:39:02.:39:12.

Hello, I'm still here. Now, all evening I've been at the Royal

:39:13.:39:15.

Holloway University at one of the biggest star spectaculars in the

:39:16.:39:19.

country - and this is where lots of budding scientists start their

:39:20.:39:21.

astronomy careers. This is where many budding scientists start their

:39:22.:39:26.

careers. And one of the first things any beginner has to is learn their

:39:27.:39:29.

way around the night sky. So I've decided to enlist the help of Royal

:39:30.:39:32.

Holloway's Physics department to bring to life the one constellation

:39:33.:39:36.

everyone should know and I'm also going to use some ingenious BBC

:39:37.:39:39.

software to create a human constellation. There is the gang of

:39:40.:39:41.

students, we have armed them with torches. There you go, guys! With a

:39:42.:39:44.

bit of BBC magic, we will try to create a human constellation. If you

:39:45.:39:49.

look at the sky on any night, you can seek seven bright stars. There

:39:50.:39:54.

they are appearing, and as those stars form, it is a shape we are

:39:55.:40:01.

familiar with, the Plough. It's one we can see at any time of night from

:40:02.:40:06.

the UK. The lines are wobbly, but maybe that is gravitational lenses.

:40:07.:40:10.

You should be able to see this at any time of night, but the itself is

:40:11.:40:15.

Ursa Major. Those are the stars slowly appealing -- appearing, and

:40:16.:40:21.

they are slowly joining up the lines, that is the great Bear, the

:40:22.:40:26.

name of the constellation, where we find MA and M 82. -- M81. I can't

:40:27.:40:36.

quite see a bear, even squinting, but if you look now, you can make

:40:37.:40:42.

the shape of the bear. The important thing about this constellation is

:40:43.:40:47.

that there are two stars at the end of the bowl that point towards

:40:48.:40:51.

Polaris, the North polar Star, and that is the only fixed star in the

:40:52.:40:58.

sky. If you can find the poll by looking at those two points, you can

:40:59.:41:03.

find anything in the night sky -- pole. And that means navigating is

:41:04.:41:09.

easy, as I found, when I took to the seas. I might know my way around the

:41:10.:41:14.

night sky, but I don't know how to use the knowledge down here on

:41:15.:41:19.

Earth. Fortunately, I'm not alone. With me is natural navigation expert

:41:20.:41:28.

Tristan Gooley. Without even knowing where we are starting, we are

:41:29.:41:32.

navigating to Alderney. Tristan, nice to meet you. Alderney is 50

:41:33.:41:40.

miles from England, and just three miles across, so it will make for a

:41:41.:41:46.

small target as night falls. Before we can think about finding the

:41:47.:41:49.

island, we need to think exactly where the boat is. We are not using

:41:50.:41:56.

GPS, radar, any modern gizmos. I have even had my phone taken of me.

:41:57.:42:01.

With the sun setting, we better make a start. To calculate position on

:42:02.:42:05.

Earth, we need to work out which area of the night sky we are under.

:42:06.:42:11.

And Polaris, the star always due north, is the perfect place to

:42:12.:42:17.

start. If you're standing on the North Pole, the star directly above

:42:18.:42:22.

your head would be Polaris, and if you travel south, that star gets

:42:23.:42:26.

steadily lower and lower, and if you reach the equator, it will be on the

:42:27.:42:30.

horizon. We are halfway between the equator and the North Pole, so we

:42:31.:42:34.

should expect the North Star to be halfway between the horizon and

:42:35.:42:40.

directly above. Tristan uses the sextant to measure Polaris and give

:42:41.:42:44.

us the latitude, how far north or south we are. But what about East or

:42:45.:42:49.

West? That is trickier. Unlike Polaris, all the other stars move

:42:50.:42:54.

around the sky through the night. Tristan sets his sights on Vega, so

:42:55.:43:02.

we can work out how long that -- how far along the path it is. Timing is

:43:03.:43:09.

critical. Now! Like every star, the timing of the path is predicted.

:43:10.:43:20.

That is 59 degrees and 47 minutes. Its position at any moment depends

:43:21.:43:23.

on how far east or west you are, the longitudinal. The time now is for 30

:43:24.:43:32.

a.m. And 50 seconds. Now we know the longitudinal attitude, we can

:43:33.:43:35.

pinpoint where we are on the map, so we can tell what direction Alderney

:43:36.:43:42.

should be. -- 4.30am. We are about five miles from land, so we can

:43:43.:43:46.

pretty much say it is five miles due south. It is a pretty creepy

:43:47.:43:52.

experience heading into the darkness. I can barely see anything

:43:53.:43:56.

ahead of me. We are having to put our faith completely in the stars.

:43:57.:44:03.

The signpost now is the star due south at this time of night. If we

:44:04.:44:08.

look up, you can see Pegasus. If we look at the bottom left-hand star,

:44:09.:44:14.

that is very close to the North Star, so that's a good one to follow

:44:15.:44:19.

now. We sail into the darkness were a couple of hours and the stars

:44:20.:44:25.

constantly move on, so once again, it's time to realign the sites.

:44:26.:44:29.

Judging by where Polaris is, we properly need to head for the group

:44:30.:44:38.

of stars called Cetus. If we look at that group of stars, and you lower

:44:39.:44:42.

your gaze to the horizon, what do you see? I can see a clump of

:44:43.:44:47.

lights, where I am confident that that is Alderney. Looks good to me.

:44:48.:44:55.

The constellation known as the sea monster is currently south of us,

:44:56.:44:59.

and it is guiding us in. One hour later, out of the inky blackness, we

:45:00.:45:03.

see the shape of Alderney. We have made it. You can see where the Pope

:45:04.:45:12.

kisses the ground. I can feel it coming on. We have travelled well

:45:13.:45:17.

over 50 miles and managed to hit a small target using just the stars to

:45:18.:45:21.

navigate by, but unfortunately, it has turned cloudy, so no way I can

:45:22.:45:25.

enjoy a nice dark skies that Alderney has to offer. I guess it is

:45:26.:45:38.

time for bed. Navigating by the stars seems archaic, but the

:45:39.:45:43.

commander of the space shuttle navigates by the stars as well.

:45:44.:45:54.

Let's play guess the planet. That is Mars. Has the biggest volcano in the

:45:55.:46:03.

solar system. Next one, what do we have there? That is Mercury. No way

:46:04.:46:09.

would we have had pictures like this without messenger being in orbit.

:46:10.:46:13.

What is fascinating is in these permanently shadowed craters,

:46:14.:46:21.

Mercury only presents one place, you can get zones that are so cold, you

:46:22.:46:27.

can get water and ice mixed in with the pebbles. There is water on

:46:28.:46:35.

Mercury, frozen solid. And planet you cannot recognise easily?

:46:36.:46:46.

Neptune. Nobody has ever seen this planet. This has been worked out by

:46:47.:46:52.

a team of scientists at Exeter University. This is remarkable, it

:46:53.:47:01.

is a genuine simulation. A planet we have never seen. This is how they

:47:02.:47:08.

did it. Planets beyond our solar system are

:47:09.:47:12.

very far away and we have little hope of imaging verse surfaces. So

:47:13.:47:17.

finding anything out about what these worlds are like, might seem

:47:18.:47:22.

like an impossible task. But a team of planet hunters at Exeter

:47:23.:47:27.

University are gearing up to do just that. With a new technique that may

:47:28.:47:31.

one day help us identify another habitable Earth. Planets can be

:47:32.:47:42.

detected by the almost imperceptible dip they cause as they pass in front

:47:43.:47:47.

of their staff. And that is all of the scientists have to work with.

:47:48.:47:52.

But with some ingenious methods they are beginning to construct these

:47:53.:48:03.

distant worlds. This stock has been working on one of the current

:48:04.:48:06.

planets. Orbiting around a star 150 light years away. When I started

:48:07.:48:14.

there was only one planet we could study the atmosphere of. This is an

:48:15.:48:24.

image of the host star. David measures precisely how the light

:48:25.:48:31.

from the host star changes as this iris filters it through its

:48:32.:48:34.

atmosphere. Starlight is made up of many different colours. And by

:48:35.:48:43.

analysing the colours that are absorbed by the planet's atmosphere

:48:44.:48:48.

when it passes across the star, David can work out what is in the

:48:49.:48:53.

atmosphere and even how thick it is. Unfortunately, it does not sound

:48:54.:49:06.

very welcoming. It looks quite alien, it is mainly made of hydrogen

:49:07.:49:16.

and helium. They have also detected sodium in the atmosphere and not a

:49:17.:49:19.

place that could support life as we know it. But even if they found

:49:20.:49:24.

oxygen and nitrogen, an earthlike atmosphere, to predict if it could

:49:25.:49:29.

be habitable we have to see how the atmosphere behaves. And that is how

:49:30.:49:36.

David was Makro Collie comes in. We are trying to interpret these

:49:37.:49:41.

observations of these climates. To do this Nathan's team have

:49:42.:49:47.

reconstruct did its atmosphere in the most sophisticated climate

:49:48.:49:52.

prediction model around. The Met Office's model of planet Earth. This

:49:53.:50:00.

brings the planet to life. This is the night side facing away from the

:50:01.:50:08.

start. This is the heart day side, temperatures of a few thousand

:50:09.:50:13.

degrees. And the arrows represent the wind flying past, incredibly

:50:14.:50:21.

fast. With this model we can dive through its atmosphere and it

:50:22.:50:25.

reveals 3000 miles down there are even stormy conditions. Very violent

:50:26.:50:34.

region, and nastier place to be, for a human anyway. Although this might

:50:35.:50:43.

not be the earthlike than it we are looking for, Nathan hopes modelling

:50:44.:50:48.

its atmosphere will help the search. Models like this can make a

:50:49.:50:51.

contribution in trying to find an alert analogue or an alert to win

:50:52.:50:55.

and trying to understand that atmosphere. -- and Earth twin. You

:50:56.:51:06.

can see the behaviour of the fluids? The model predicts there is an

:51:07.:51:14.

equatorial band, so a Jetstream at the equator. Also a couple of

:51:15.:51:22.

storms, that is Jupiter's red spot. This is orbiting around what we call

:51:23.:51:36.

a K star. But it is the M stars that are the most common in the galaxy.

:51:37.:51:42.

What these models have shown is that does not preclude the existence of

:51:43.:51:47.

life potentially on these planets. These storms distribute the heat

:51:48.:51:53.

around the planet. So we can add myth about 75% of the stars in the

:51:54.:51:59.

galaxy could support life. But this cannot support life? Know it also

:52:00.:52:09.

has silicon rain, so it rains glace. If you do last 20 years ago, perhaps

:52:10.:52:16.

ten years ago, we did not know about the other solar systems in the

:52:17.:52:23.

galaxy. Now we have over 1000 planets beyond the solar system

:52:24.:52:29.

confirmed. Many of them looking at a planet as it passes across the

:52:30.:52:34.

star. This is an encyclopaedia of the planets passing by. The most

:52:35.:52:37.

interesting than it is, the most interesting candidates are the 12

:52:38.:52:42.

planets that have been found and are most likely to be second earths.

:52:43.:52:48.

They are in what is called the habitable zone of the staff. We can

:52:49.:52:56.

also tell about the gases within the atmosphere? We can look at the

:52:57.:53:02.

atmosphere to ask questions such as is their oxygen in the atmosphere?

:53:03.:53:08.

Carbon dioxide, so the likes of Venus, it's atmosphere is too dense.

:53:09.:53:14.

But we can look for industrial pollutants in the atmosphere. If you

:53:15.:53:21.

found CFC which are not created naturally. You would know there is

:53:22.:53:27.

industrial civilisation. We're not far away from being able to do that.

:53:28.:53:36.

For the final time, we are crossing over to Liz who has been circling

:53:37.:53:45.

the skies in Norway. We are still admiring the aurora borealis. It has

:53:46.:53:54.

changed quite a lot? Yes, it has actually hit now. I am not landing

:53:55.:54:02.

now. This could burst into a multicoloured ray of light? This is

:54:03.:54:13.

the beginning of it. It is changing by the second. Do Rohrer occur

:54:14.:54:22.

regularly? There is always something there, whether it be a faint glow up

:54:23.:54:27.

to a full-blown display like we are going to get now. As we're looking

:54:28.:54:32.

at this appear, there is the equivalent happening in the South?

:54:33.:54:42.

Yes, in the southern Oval as well. We have been sending our hunters out

:54:43.:54:50.

to get us some pictures. This was captured in Tasmania several hours

:54:51.:54:57.

ago. It is beautiful. Seven hours ago then, that would have been

:54:58.:55:02.

manifesting itself appear, the equivalent of it somewhere in the

:55:03.:55:07.

zone? Yes, the northern zone as well. So many questions from viewers

:55:08.:55:14.

about the nature of this. Someone asking, are they identical in

:55:15.:55:20.

appearance? As one happens up here, the exact same patterns and

:55:21.:55:26.

features, happens down there? If you are standing the same distance, yes

:55:27.:55:31.

that is what would happen. When it comes to them being mirrored image

:55:32.:55:37.

of each others, one is mirroring the other in shape and position? It was

:55:38.:55:42.

thought for a long time that was the case, but in 2002 a couple of NASA

:55:43.:55:48.

spacecraft by chance just imaged both ovals so they were able to

:55:49.:55:52.

compared them. There are subtle differences. When things come from

:55:53.:55:57.

the solar wind it can make both ovals move in opposite directions.

:55:58.:56:01.

On the regions of maximum at liberty in the ovals tilt towards the dawn

:56:02.:56:07.

side of the Earth as well. It is nearly time for us to say goodbye,

:56:08.:56:13.

but it has been glorious. We are still waiting for changes in

:56:14.:56:17.

colours. It has been an ambitious mission over the last three nights

:56:18.:56:25.

and a privilege to observe this. We were lucky when we were on the

:56:26.:56:29.

ground? Extremely lucky, I have known people who waited two weeks

:56:30.:56:35.

and saw nothing at all. There is so much to learn, but somewhere in the

:56:36.:56:40.

not too distant future, not only will we be able to admire this, we

:56:41.:56:45.

will have learned enough to say exactly what is going on at that

:56:46.:56:50.

moment in time. VAT for me is thrilling and it brings home are

:56:51.:56:54.

intrinsic relationship with our start. That is it from us. We will

:56:55.:56:59.

keep rolling until the end of the show. It has been an honour to be

:57:00.:57:07.

part of this live from 30,000 feet. It is good night from northern

:57:08.:57:14.

Norway. I don't know what to say without being hyperbolic. We knew it

:57:15.:57:21.

was a gamble and we knew we could not get nothing. Mark, how are you

:57:22.:57:32.

getting on? We have had a wonderful evening, the

:57:33.:57:37.

unforgettable human constellation. A Milky Way projection the size of a

:57:38.:57:42.

house and there is a simulator somewhere. Not forgetting the

:57:43.:57:47.

wonderful clear skies, we have seen beautiful images are planets and

:57:48.:57:52.

beautiful images of galaxies. These guys are going to be here for some

:57:53.:57:55.

time yet so I am going to join the party. So from me and everyone here,

:57:56.:58:04.

goodbye. Rebecca, some names coming in. Nine Jodrell Scope, I like that.

:58:05.:58:16.

We will be discussing this in a moment. Thank you for all of you who

:58:17.:58:24.

have taken part. What a wonderful way to finish the series. Let's take

:58:25.:58:30.

a last look at those images captured from the Ark ticks circle. It is

:58:31.:58:36.

incredible. Thanks to all of our viewers who have sent in

:58:37.:58:40.

photographs, or just watching at home. The show may be over for

:58:41.:58:49.

another year, joiners in two minutes per K9's space tributes. The first

:58:50.:58:56.

time we made this programme four years ago was to encourage you to

:58:57.:59:02.

look up and go outside. We have described the planets, the space

:59:03.:59:07.

probes orbiting the planets, let your imagination fly and we will see

:59:08.:59:13.

you next year. Also in two minutes as well.

:59:14.:59:22.

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