Episode 3 Stargazing Live


Episode 3

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Over 100,000 of you have been working hard scouring an unexplored

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area of Mars. Your efforts have paid off. You have made an

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incredible discovery on the surface of the Red Planet. We will be

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revealing all tonight. I'm Brian Cox. He is Dara O Briain. This is

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Welcome back to a very foggy Jodrell Bank Observatory. So foggy

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we can hardly see the big dish. Not a great night for stargazing. It is

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the third and final night of this year's Stargazing Live. Thank you

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for your questions. We have some remarkable viewer photographs that

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I want to show you. This is the Orion Nebula. We saw it on the

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first night. This is a picture - it is taken with a 4.5 inch reflector.

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26 30-second exposures. This was taken last night. This one,

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California Nebula. Is it because it's the shape of California?

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It was taken on the 9th. This one is the jewel in the crown in many

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ways. It may not look like it. It's - we now know - a comet. It was

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discovered, or the photograph was taken by Nick Howes in the States.

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On Monday night, the stargazers at the school - this is now a comet.

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That is a genuine discovery. As we mentioned, we have made some

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interesting discoveries on the surface of Mars. Chris Lintott will

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be back later in the programme to reveal all. There is much more to

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stargazing than these TV shows. There are over 500 events taking

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place up-and-down the country for you to get some hands-on with

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astronomy. I have some pictures. I want to show you what everybody has

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been doing. Here is one. This is the Canterbury Star Party. 1,200

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guests turned up to Canterbury on Tuesday 8th. This is them showing

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how to make rockets with a vitamin tablet. This is the Eden Project.

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1,500 guests on 8th January. Finally, this one - that is nice.

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Where was that? Birmingham. This is people from Birmingham University

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explaining how gravity works. One last picture. This one was sent in

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by Private Eye. There is Dara O Briain looking very handsome and

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Buzz Lightyear! To find an event near you, go to

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bbc.co.uk/stargazing. We will be going to see how Mark got on with

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the Herschel Telescope. Among his many claims to fame, Herschel

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coined the term "asteroid". It means star-like in Greek. In five

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weeks' time an asteroid 45 metres wide is going to pass between us

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and the Moon, coming closer to Earth than some of our satellites.

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In March, the comet Panstarrs will streak by in the sky followed by

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Ison. This was taken on 9th. Ison will pass very close to the Sun. If

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it survives that encounter with the Sun, it could break up, it will

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sweep out in January 2014 - it could be one of those comets that

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you see in a tapestry! Fantastic. We are going to pass through the

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tail of that later in March. It may give us a meteor shower. Fantastic.

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We have had lots of questions. "What is the difference between

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asteroids, comets and meteors?" We have to keep on explaining this.

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Comets are large dirty snowballs. Yes. They are icy with some rock

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mixed in. They come from distant regions of the Solar System. We

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will see that later on in regions called the Kuiper belt and the Oort

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Cloud. The comets are spectacular. We have some fantastic footage.

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This is a beautiful shot from the International Space Station. Looks

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like some kind of computer graphic. That is Comet Lovejoy. Lovejoy was

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discovered in December 2011 by Terry Lovejoy in Australia. Here it

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is passing behind the Sun. Remarkable piece of footage. Here

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is another video. This is from the Solar Observatory. The thing about

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comets - you tend to think of them streaking along. The tail is blown

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by the solar wind. The Sun is heating the comet up. You are

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getting gas and dust erupting. it is moving away from the Sun, it

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follows its own tail? Yes. Asteroids are more like rocky

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fragments of planets. Yes, this is the first asteroid we encountered

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in space. This is not a video. This is Eros. It's about 34 kilometres

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long, which is about the size of the thing that - if it hit us, it

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would be the size that killed all the dinosaurs. It doesn't cross the

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Earth's orbit at the moment. It crosses Mars' orbit, though.

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Because it continually crosses the orbit of Mars, it could be

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perturbed by Mars. We landed on the surface of that asteroid. When we

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talk about meteors and meteoroids, they interact with our atmosphere.

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Meteors are when they burn up. Meteor showers. What are they?

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is a meteor shower in December. The reason for that is that they were

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created by a comet. They are the remains of the tail of a comet.

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you think about what a comet does. It orbits the Sun. So they leave an

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ellipse of debris and that will sit there in orbit around the Sun in

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the place where the comet tracks around. The Earth passes through it

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at the same point in its orbit every year. And that is why you

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always see them coming from the same place. That is how meteor

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showers are named. So one of the things we want to

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talk about is the big asteroid coming our way very soon. It is

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called Asteroid 2012 DA14. On Friday February 15th it will pass...

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Here it is. That is how close it is going to come! These are our

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satellites. The green blobs are the satellites. It will come well

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within the orbit of the station. will pass on 15th February. This is

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going to be more pressurised Valentine's Day so do something

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good on the 14th February! It will miss us by a mile! How can we be so

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sure that this trajectory is so right? Liz Bonnin is standing by

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for us at the Goldstone Observatory. Welcome to Goldstone in the Mojave

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Desert. This is the Mars Antenna, part of NASA's Deep Space Network.

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Now, I'm inside the base of the antenna and presently, it's

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tracking the New Horizon's Mission to Pluto. Marina, you are one of

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the scientists that does that work. How does tracking an asteroid work?

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It is simple. You point it to the asteroid and you bounce on some

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mike waves. This allows you to get its location very precisely --

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microwaves. This allows you to get its location very precisely.

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were tracking Apophis last night. Scientists thought it was going to

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hit us. What is the latest? Well, we have been tracking it since late

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December and what you are seeing here are the images from this

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morning. Is that Apophis? What you are looking at, this is a 300 metre

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diameter object that is 14.5 million kilometres away and we have

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the detection. Radar data that we have collected have completely

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excluded any chance of impact. We are safe. That is good news.

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Furthermore, we can now precisely predict its trajectory decades into

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the future. Fantastic work. As well as tracking, you get a good

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resolution from these orbits. This is Toutatis. This is a prime

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example of what radar can do. This is 4.6 kilometre-long asteroid. It

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was 7.5 million kilometres away from Earth. We are getting

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resolution to resolve surface boulders. Wonderful technology.

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Scientists are also getting a better idea of the composition of

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asteroids with their latest work. What is clear is that there are

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many more different types than previously thought. Amy Mainzer,

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another NASA scientist, taught me how to make my own.

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We have asteroids that are solid lumps of metal. Take some of this

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dirt and spoon it in. Step one - all asteroid also have some type of

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dirt? That's right. You have silicon in here, all kinds of

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heavier elements and that's going to be the basic constituent of most

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asteroids. We will pour some of that water in and make a big mess.

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One theory about why there's so much water on Earth is that some

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arrived here aboard comets and asteroids. That's not the only

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familiar substance found in them. Let's take some of this molasses.

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How much? That's pretty good. This one is carbon-rich! Now we need a

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squirt of another ingredient that has been found in the remains of

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asteroids that have landed on Earth, ammonia. Then we add our final

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ingredient - dry ice. At minus 78 centigrade, it will mimic the

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freezing conditions of the Solar System. Sprinkle that in there. We

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will freeze it up good. Let's take a look and see what we have ended

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up with. Amazing! That is what we got. In true asteroid-style, it is

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beautifully irregular. It is not completely round. Oh my goodness!

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This asteroid is a very particular kind, a randomly active main belt

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object. A Rambo, would you believe?! It is special. We have

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discovered in the last ten years or so this very unusual class of

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asteroid that becomes active. Active in what way? These things

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exhibit huge clouds of gas and dust coming off the surface. What

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happens is when the Sun hits the objects, we use this bright lamp to

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represent the Sun, what we think happens is that a smaller asteroid

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may strike the surface and scrape off some of this dirty outer layer

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and it may expose some of the ice. Look at that jet coming out from a

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tiny little hole and you can't see any of the ice exposed? That's

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right. This is a really good example of what we think happens.

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If we were orbiting the Sun, this object would have a big tail around

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it. And a big halo following it. Almost two years ago, the Hubble

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Space Telescope photographed a Rambo which grew a tail when it was

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heated by the Sun and just there is its X-shaped impact scar. Closer to

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home, what is the worst that could happen to the Rambo we have made?

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This is a good sized lump of rock. How can this really cause that much

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damage? Well, something this small obviously can't. If something were

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the size of a building, like 30 or 40 metres in diameter, it would be

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large enough to make it through the Earth's atmosphere. Now you have

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something that can cause a great deal of damage because if it is

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travelling at 10 kilometres a second or more, it packs an

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enormous punch. Amy has now joined us at Goldstone. You use Space

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Telescopes to find out potentially dangerous asteroids. Tell me about

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the project? It's a Space Telescope that used infrared light to

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discover and track near Earth asteroids. Infrared is heat. We are

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sensing heat. It gives us an idea of the size of the object. We can

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tell the difference between something that is really large but

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dark, like a piece of coal, or something that is much smaller, but

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highly reflective. OK. Getting the size is important for understanding

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We sampled some of the population and used it to look at what is out

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there. What have you come up with? For objects that are larger than a

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kilometre, like the dinosaur killing object, 90% of these have

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been found. What about the other 10%? We don't know where they are

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yet. There's another piece of not so good news which is that for

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objects larger than 100 metres, we've only discovered 25% of those.

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They can cause great damage. Absolutely. You need to continue

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this surveying work. We have a lot more work to do. What happens if a

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big one is coming at us? Ideally we will find an object 20 to 30 years

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before it will happen. If we have time like that, we can design

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strategies that would use explosives to push the asteroid

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aside or break it into pieces or maybe even devised technology to

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target out the way. How? A either gravitationally or attaching solar

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sails. Astonishing. Thank you. Come back to us when we talk about

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emissions and more about asteroids and comets. Standing by it on our

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live block is Don. He is head of NASA's near earth objects

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department. He will be informed if an asteroid is heading our way for

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a start -- he will have to inform the President. He can take your

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questions at bbc.co.uk/stargazing. A lot of people are asking where

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these objects originate from. We have a model for you. All of the

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asteroids we ever encountered... Everything comes from three places.

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We have an animation that shows just the asteroid belt ter, between

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Mars and Jupiter and it is the Mars and Jupiter and it is the

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green area. Every point is a map position of an asteroid. This is

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what it looks like. It is a bit of a mess, which is why we get impact.

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The asteroid belt is packed with Rocky objects, including this one.

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This is called Vesta. I have an image of it. It is quite a big rock.

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It is about 350 kilometres in diameter. The remarkable thing

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about Vester is I have a piece of it here. This came from there. The

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mystery will be revealed later. It mystery will be revealed later. It

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is beautiful. This is the Kuiper belt. Faces a region of IAC, rocky

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object. This is where Pluto lives. It was demoted because it turn

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Celtic is one week -- one of many objects of a large size in the

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Kuiper belt. We are on our way to Pluto at the moment. This is a

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picture of a spacecraft on its way. It left in January 2006. When it

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left Pluto was a planet. When it got to about there, Pluto was

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demoted, but by that time it was too late to stop. It makes no

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too late to stop. It makes no difference to the mission. These

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are the best images we have of Pluto now. They are from the Hubble

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Space Telescope. It is extremely cold. We don't know a lot about

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Pluto other than these images. is ice. For is an ice, about -200

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Celsius. Finally you step into this region, the far reaches of the

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solar system, the Kuiper belt. This is a picture of the Oort cloud, a

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spherical cloud. This is a disc of the solar system? Yes. This is more

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spherical. It is a vast collection of large and small lumps of ice and

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rock. It stretches out about a light year, we think. A quarter of

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the way to the nearest star. Nearly all of the Committee's wheezy come

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from either the Kuiper belt or the Oort cloud. -- comets we see.

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wanted to work out what things were in danger of hitting. We need to

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know where the Earth is at any time. How do we were kicked out? The

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How do we were kicked out? The answer lies in the southern

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hemisphere's guy. -- southern- hemisphere sky. This is an iconic

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constellation. It even features on the Australian national flag. It

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was by interpreting patterns have stars in the sky that we began to

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make sense of our cosmic surroundings. On Earth, it is easy

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for me to work out my position relative to the object I can say. I

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can understand my place in this world. If you're an astronomer, you

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have a problem because all you can see on little points of light in

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the sky and for the early astronomers, they knew nothing more

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than that. To make progress, people began to make maps of the night sky

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end as much detail as possible. He this is an early start shot of the

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southern sky from 1801. It is a two dimensional representation of the

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position of the stars. This is the Southern Cross. When you follow

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what you get to the bright southern star. 200 years ago, the way these

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maps were made meant their accuracy was limited. When he made this map,

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he did it by hand. He looked at this guy and transcribed the

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positions of the stars on to this piece of paper. A huge opportunity

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for human error in that process. But in the late 19th century, a new

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technique allowed astronomers to achieve real precision. Photography.

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If you have a photograph, a plate and a telescope, the marks on a

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plate are not made by the human hand, they are made by photons of

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light that have travelled from the stars themselves, hundreds or even

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thousands of light-years to register their position on the map.

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By fitting a camera to a telescope, the accurate positions of thousands

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of stars could be recorded in a single exposure. Something

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astronomers hoped would help them determine our place in the universe.

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In 1887, a decision was taken to map the position of every star that

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can be seen in this guide with high precision. That was a project that

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An incredible commitment, like building a cathedral. Much of the

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southern sky was mapped here, at Sydney Observatory, and this is one

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of the photographic plate that was used Clinton's -- to construct the

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used Clinton's -- to construct the Astra graphic catalogue. An

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exposure, just over six hours, and you can see very faint black dots

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on the plate. Each one of these black dots is a star and the

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positions were measured and transcribed into here. The Astra

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graphic catalogue. This is 1893, John Reid 20th. Documenting the

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positions of the stars in this photograph. What we have here is a

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perfect representation of the positions of the stars in the sky

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from Sydney on January 20th, 1893. 750,000 stars were recorded at

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Sydney Observatory and the results were combined with surveys made at

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19 other observatories around the world, creating a single, huge

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catalogue of the stars across both hemispheres. For the very first

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time, astronomers had an accurate record of our position relative to

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4.5 million stars. That has helped us to make another intriguing

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characteristic of the stars with great precision. In the 1990s,

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these measurements were repeated, this time by a satellite the

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European Space Agency Bill. What was found was that for at least

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some of the stars, their positions had changed an appreciable amount.

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For his slow drift is unique to each star and because it takes

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years to become apparent, comparing recent satellite data with this

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catalogue has given us the most accurate ever record of this

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phenomenon. He the reason for this movement is that all of the stars

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in the Milky Way are a orbiting around the centre of the galaxy,

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but each at its own particular speed. Today, even deeper in the

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universe, it is not just stars fat have their own unique motion. -- of

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that have. By looking out beyond the stars in the Milky Way, we

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found that all the galaxies in the universe on moving relative to each

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other as well. We are part of a group loan -- known as a local

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group. 43 galaxies bound together in the same way the stars are bound

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together in the Milky Way. That group itself is moving roughly in

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that direction to something called the Super cluster, a group of 5,000

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galaxies or more, about half a billion light years in that

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direction. And we are travelling towards this enormous cluster of

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galaxies that is over 500 -- at over 500 kilometres per second.

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What we discovered over hundreds of years of astronomy, making

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precision measurements of the sky, is that everything in the universe

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is moving relative to everything else. We've learned that the stars

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and galaxies are all taking part in a vast cosmic doused which we --

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dance which we can now plot with We have all of these objects in an

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Orbit around the sun. Why are some of them suddenly lurching out on

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these crazy journeys? The answer, as with every answer, lies with

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mathematics. We've got Tim O'Brien to explain. The mathematics of

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this? You remember that all these objects orbiting around the Sun a

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doing it under Newton's law of gravity. It turns out that there's

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only four possible shapes of orbits they can have. They are really --

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the really neat bit of mascot those shapes are defined by slices

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through a core. Depending on what angle you slice through, you get a

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circular Orbit, and elliptical Orbit, a Parabolica or Orbit or a

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hyperbolical bit. Fees are in her elliptical orbits, some of them a

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more secular. But in general, everything... They go round and

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back. A most common or bits of the elliptical and hyperbolic her.

:27:30.:27:35.

Hyperbolic Orbit is open. If something gets bumped into a

:27:35.:27:38.

hyperbolic Orbit, that will go around the same place as before,

:27:38.:27:43.

but it will shoot off. Yes, and it never comes back. It goes out into

:27:43.:27:49.

interstellar space. The difference is essentially to do with energy

:27:49.:27:53.

and angular momentum. Let's say we are in the Kuiper belt and

:27:53.:27:59.

something has a gravitational interaction. It interacts with lets

:27:59.:28:06.

a Pluto. It will change the energy of that object. It will change the

:28:06.:28:09.

Orbit because these shapes are defined partly by the energy. One

:28:09.:28:14.

of these things can be perturbed spirit begins a journey into the

:28:14.:28:21.

inner solar system. Halley's Comet, which came from the Oort cloud,

:28:21.:28:26.

that comes in. It is still an ellipse. It is. A period of 76

:28:27.:28:31.

years, it comes back every 76 years. It could have jumped from a

:28:31.:28:37.

circular Orbit into an elliptical Orbit. Because of an interaction.

:28:37.:28:45.

The Oort cloud is interesting because it is so far out. Many of

:28:45.:28:50.

the perturbations come from passing stars. They are very weakly bound.

:28:50.:28:58.

The false drops away. -- force. bombed sit by passing and Zenit

:28:58.:29:02.

heads off on a new journey. These hyperbolical orbits are interesting.

:29:02.:29:06.

You don't see them coming because they come in and they have such an

:29:06.:29:11.

Orbit that they go round once and disappear. Something perturb them

:29:11.:29:20.

and dumps them. It is gone and we Bonevacia him again! Maybe some

:29:20.:29:26.

time he will pass you. Let's find out if there are clear skies where

:29:26.:29:36.
:29:36.:29:37.

you are tonight. Let's go to Susan We are up against it this evening

:29:37.:29:41.

thanks to a lot of cloud piling into the UK. To the east of the UK,

:29:41.:29:45.

we have had a weather front that has hung around for much of the day

:29:45.:29:49.

today. So that will obscure the skies here. Further west, another

:29:49.:29:52.

front that's fizzling out. We will lose the rain but the cloud is

:29:52.:29:57.

going to stick around. Between the two, a few clearer spells across

:29:57.:30:01.

the North West and for Northern Scotland. My top picks for the

:30:01.:30:11.
:30:11.:30:12.

clearest skies - it will be in the west. And give it a couple of hours

:30:12.:30:16.

and Northern Ireland will be looking almost crystal clear.

:30:16.:30:23.

More information as ever on the BBC More information as ever on the BBC

:30:23.:30:27.

Weather website. Thanks. Mark Thompson has been

:30:27.:30:32.

building a modern interpretation of William Herschel's 20-foot

:30:32.:30:42.
:30:42.:30:47.

telescope. Anyway, in a tribute to his work,

:30:47.:30:52.

Mark has been trying to re-create that telescope.

:30:52.:30:56.

Over the past three weeks, I have been working with the local

:30:56.:31:00.

community in Derby and a crack team of experts. We have had to make

:31:00.:31:06.

changes to Herschel's plans to keep everyone safe, but we have remained

:31:06.:31:11.

true to his principles. So far, we have built the supporting structure.

:31:11.:31:16.

Big, isn't it? Now we have the small matter of making the

:31:16.:31:25.

telescope. In Herschel's Telescope, right at the bottom of the tube was

:31:25.:31:29.

a piece of polished metal to reflect the light from the stars.

:31:29.:31:33.

It was shaped and positioned to focus the light towards the top of

:31:33.:31:37.

the tube and here, Herschel would have stood on this viewing platform

:31:37.:31:41.

and looked down the barrel through an eye-piece. This is our telescope

:31:41.:31:45.

tube. We will put a mirror up this far end. So light comes down the

:31:45.:31:50.

tube, hits the mirror, bounces back up the tube and then all the way up

:31:50.:31:54.

to the top into this special adjustment we have made. We have

:31:54.:31:57.

had to cut some of the tube out where the eye-piece is going to go

:31:57.:32:00.

and hopefully, we will see some stunning views of the sky through

:32:00.:32:05.

it? Want me to push? Not too much! Now we need to get it up into the

:32:05.:32:15.
:32:15.:32:16.

cradle. Chris Hill is on hand to supervise. That will do. That's it.

:32:16.:32:23.

It is finally starting to look like a telescope. Inside the university

:32:23.:32:28.

workshop, Chris is putting the final touches to the mount for the

:32:28.:32:34.

mirror. An instrumentation expert is here with the missing piece.

:32:34.:32:40.

It's arrived! We are using a modern glass mirror in our telescope.

:32:40.:32:44.

Herschel would have used a piece of metal and that would have easily

:32:44.:32:49.

tarnished. Even though he polished it for hours, it still wouldn't

:32:49.:32:56.

have been very reflective. Herschel would have been blown away by this.

:32:57.:33:00.

Yes, this would have been his Christmases! The mount has a set of

:33:00.:33:06.

screws on the back, so that the angle can be adjusted. Now, we can

:33:06.:33:10.

align the mirror. So the light from the stars is reflected through the

:33:10.:33:16.

eye-piece. Shall we put it in then? Let's try it. The time has come.

:33:16.:33:24.

Yeah. You got the screws? Back a bit. There! The first step is to

:33:24.:33:28.

cover the opening with a large sheet of paper. For the next bit,

:33:28.:33:32.

Herschel would have probably used a candle but we are going to use a

:33:32.:33:38.

laser pointer. The light travels through a small hole in the paper,

:33:38.:33:42.

down the tube and hits the mirror at the bottom. It is reflected back

:33:42.:33:47.

at an angle to hit the paper again. I need to guide Chris to adjust the

:33:47.:33:52.

mirror. Until the reflected laser light moves into position where the

:33:52.:33:56.

eye-piece will be. Chris, if you can tilt the bottom towards me so

:33:56.:34:03.

bring that away from you? Got you! Can you see it moving? Yes, keep

:34:03.:34:09.

going. Woah! Spot on! How is that looking? Perfect. Excellent. That

:34:09.:34:13.

is perfect, mate. Well done. This laser beam is simulating star light

:34:13.:34:17.

and it is bouncing back out of the tube which is where I need to look.

:34:17.:34:23.

If I spray this, you can see where the beam is coming out the tube. It

:34:23.:34:30.

shows that we are ready for some clear skies!

:34:30.:34:35.

After all that work, the time has come to reveal the telescope. Let's

:34:35.:34:40.

cross live to Mark at the University of Derby.

:34:40.:34:50.

There is a fantastic atmosphere. We have our own Herschel quintet. We

:34:50.:34:55.

have the children from the school here. CHEERING We have also got the

:34:55.:35:03.

members of the Derby Astronomical Society. Hello, guys. Now it's

:35:03.:35:09.

taken us five weeks and hundreds of man hour. It weighs in at just

:35:09.:35:15.

under half a tonne. It is Stargazing Live's Herschel

:35:15.:35:20.

Telescope. CHEERING Now, it is the most amazing piece of kit. It has a

:35:20.:35:24.

crank to turn the whole telescope. The whole structure moves around so

:35:24.:35:28.

that you can access any part of the sky that you want to. It is the

:35:28.:35:32.

most amazing piece of kit. Hopefully, we might get a chance to

:35:32.:35:37.

look through the telescope. With me is Professor Alan Chapman. Alan,

:35:38.:35:42.

what do you make of it? It is absolutely remarkable. It is a

:35:42.:35:46.

tremendous realisation of Herschel's Telescope, using

:35:46.:35:50.

scaffolding and modern equipment. I have never seen anything like it

:35:50.:35:54.

before. Me neither! Even to the chaps pushing it around. Herschel

:35:54.:35:59.

probably used sailors! We have used the same tube dimensions, the same

:35:59.:36:04.

mirror diameter. We only had a drawing to work from. It took him a

:36:04.:36:13.

year. We did it in five weeks. That is incredible? To him it was

:36:13.:36:16.

entirely experimental and a brilliant piece of inspired

:36:16.:36:25.

engineering. Herschel was a skilled worker with his hands. He employed

:36:25.:36:32.

carpenters to do the heavy work for him. Yet, Herschel was a skilled

:36:32.:36:37.

musician. A string player, a keyboard player and I think all of

:36:37.:36:41.

those skills were necessary to the manipulation and adjustment of that

:36:41.:36:47.

instrument. I will have to stop you there. Thanks to the guys from the

:36:47.:36:51.

Derby Rugby Team. I'm really looking forward to looking through

:36:51.:36:54.

the telescope. It is still cloudy here. It is foggy in Derby. With a

:36:54.:36:58.

bit of luck, it may clear up. Do come back to us later on tonight

:36:58.:37:03.

and we will see if we can re-create the images that Herschel saw.

:37:03.:37:08.

Hopefully we will. We have been talking about asteroids and comets.

:37:08.:37:12.

Of course, we will be struck by large objects from space. It's

:37:12.:37:15.

happened all through history. It isn't necessarily a bad thing.

:37:15.:37:19.

Without these impacts, our world might not be the place that we know

:37:19.:37:23.

today. If you want to see one of the best

:37:23.:37:28.

preserved meteor impact sites on Earth, you need to travel to the

:37:28.:37:32.

Barringer crater in Arizona. Craters can be found all over the

:37:32.:37:37.

Solar System like this. The battle scars of a long history of impacts.

:37:37.:37:42.

Most are the result of one period, around 3.6 billion years ago, when

:37:42.:37:47.

the whole Solar System was turned upside-down. It was all to do with

:37:47.:37:52.

the combined gravitational force of our two biggest planets, Jupiter

:37:52.:38:00.

and Saturn. We now believe that the giant planets formed much closer to

:38:00.:38:09.

the Sun than they are today. Their orbits drifted hundreds of millions

:38:09.:38:14.

of years until Jupiter and Saturn fell into a regular pattern. Once

:38:14.:38:19.

every cycle the two planets aligned creating a gravitational surge that

:38:19.:38:29.
:38:29.:38:29.

played havoc with the orbits of all the planets. Neptune was catapulted

:38:29.:38:35.

outwards and smashed into the ring of comets surrounding the Solar

:38:35.:38:41.

of comets surrounding the Solar System with dramatic consequences.

:38:41.:38:48.

For 100 million years, the Solar System turned into a shooting

:38:48.:38:55.

gallery as the comets ploughed through it. Millions of comets were

:38:55.:39:00.

scattered in all directions peppering the planets. It was

:39:00.:39:09.

called the Late Heavy Bombardment. It created many of the craters we

:39:09.:39:15.

see throughout the Solar System today. It left scars all over our

:39:15.:39:25.
:39:25.:39:25.

Moon. And it had a lasting impact on the Earth as well. The only

:39:25.:39:29.

impact craters we see on Earth today, like this one in Arizona,

:39:29.:39:34.

were made much more recently, but they reveal the scale of these

:39:34.:39:44.
:39:44.:39:47.

impacts. Today, impacts like this are relatively rare. They will

:39:47.:39:57.
:39:57.:39:58.

happen again. But during the late Late Heavy Bombardment, the

:39:58.:40:03.

environment was changed radically and dramatically. Those changes

:40:03.:40:07.

weren't necessarily catastrophic. It's now thought that a significant

:40:07.:40:13.

amount of the water in the Earth's oceans was delivered by the impacts

:40:13.:40:17.

of water-rich comets and other objects during the Late Heavy

:40:17.:40:21.

Bombardment. That means that impacts could have played a key

:40:21.:40:31.
:40:31.:40:33.

role in the development of life on Earth. Before the Late Heavy

:40:33.:40:42.

Bombardment, the Earth was a barren rock. Afterwards, it supported the

:40:42.:40:47.

oceans that would become the Crucible for life. Without the

:40:47.:40:52.

water delivered in the Late Heavy Bombardment life on Earth may never

:40:53.:40:57.

have evolved. All this may have been caused by the violent

:40:57.:41:07.
:41:07.:41:10.

gravitational pull generated by two Joining us now is Dr Richard

:41:10.:41:14.

Greenwood. We have seen one of your fantastic samples already.

:41:14.:41:19.

talked about Vesta. It is from Australia. It has a special

:41:19.:41:25.

composition that we know matches Vesta. One billion years ago, a

:41:25.:41:33.

meteorite smashed into the southern hemisphere of Vesta. They drifted

:41:33.:41:38.

into the three to one resonance with Jupiter and it is a real

:41:38.:41:42.

conveyer belt. We have ten times as many meteorites coming from Vesta

:41:42.:41:47.

as we have from the Moon, or Mars. That is remarkable. It is to do

:41:47.:41:52.

with this gravitational interaction with Jupiter throwing these things

:41:52.:41:58.

our way. Absolutely. This is iron? That is. If we pick it up, you will

:41:58.:42:01.

see it is three times denser than a rock that you find in your garden.

:42:01.:42:06.

It is pure metal. It is the core of an asteroid that melted. When it

:42:06.:42:11.

melted, the metal sank and formed a core. We used to think these were

:42:11.:42:16.

quite young. That is one of the oldest objects in the Solar System.

:42:16.:42:23.

The reason for that is - at that time, they had a short

:42:23.:42:27.

concentration of Aluminium 26. That would have been formed in a

:42:27.:42:34.

supernova. Yes. It's probably the shockwave from the supernova that

:42:34.:42:42.

triggered the collapse which formed Within two million years, which is

:42:42.:42:48.

a small length of time, it would have gone. These are relatively

:42:48.:42:53.

unstable and made in a supernova explosion? Exactly. Heated the

:42:53.:43:01.

asteroids up. That is why you get the iron sinking? That's right.

:43:01.:43:11.
:43:11.:43:11.

is not the oldest thing? This fell in Tanzania, it is called Ivuna.

:43:11.:43:18.

That is some of them there. In there, there are diamonds, graphite

:43:18.:43:26.

and they came from some of the stars that pre-dated... This is

:43:26.:43:33.

older than the Solar System? Yes. 4,567 million years. That is older.

:43:33.:43:37.

That is older. The story of the origin of the Solar System is a

:43:37.:43:41.

supernova went off, a shockwave came through this gas and dust,

:43:41.:43:45.

that caused it to collapse and pieces of that shockwave - this is

:43:45.:43:50.

from outside the Solar System? Exactly. And got trapped? Yes.

:43:50.:43:57.

Startling. Technology now allows us to get up close and personal with

:43:57.:44:01.

asteroids and comets whilst they are still in orbit. Let's go back

:44:01.:44:05.

to Liz in the Goldstone Observatory to hear more. Thank you very much.

:44:05.:44:08.

Goldstone and the rest of the Deep Space Network have communicated

:44:08.:44:12.

with some truly remarkable missions getting us very close to asteroids

:44:12.:44:16.

and comets that are speeding through space. Amy, if we can talk

:44:16.:44:26.
:44:26.:44:28.

about a few of them? Stardust? Stardust Mission flew through the

:44:28.:44:32.

comet and it collected tiny pieces of the comet and it brought them

:44:32.:44:36.

back to Earth. It has given us a new window into the Solar System.

:44:36.:44:45.

None of that material has changed for 4.5 billion years? Exactly.

:44:45.:44:50.

Deep Impact Mission does what it says on the tin? Exactly. It was

:44:50.:44:56.

two spacecraft in one. An impacter spacecraft and an observer. They

:44:56.:45:01.

separated when they got close to a comet. The observer watched and

:45:02.:45:07.

allowed us to see the inside of the comet. What have we learned from

:45:07.:45:10.

that material? It was a really surprising result. It turns out

:45:10.:45:16.

that this particular comet was more dust than water-ice. Also, the

:45:16.:45:26.
:45:26.:45:33.

They have a lot more in common than we thought. And then for Dawn

:45:33.:45:38.

Mission which sent an order to do my to it -- mighty fester. It has

:45:38.:45:42.

been orbiting Vesta and it has returned spectacular images that

:45:42.:45:46.

have allowed us to see the turbulent history that has happened

:45:46.:45:53.

to this asteroid. Two giant impact craters on the South poll of the

:45:53.:45:58.

asteroid and joy and scrapes that I even larger than the Grand Canyon.

:45:58.:46:04.

Thank you for joining us. Dawn is on its way to Ceres, the biggest

:46:04.:46:09.

rock in the asteroid belt, 950 kilometres in diameter and it has

:46:09.:46:15.

been declassified as a dwarf planet. It will reach it in 2015 and will

:46:15.:46:21.

begin its exploration then. That space around our planet is not

:46:21.:46:24.

just filled with natural objects, it is also filled with staff and we

:46:24.:46:32.

put up there. So much stuff that there's a pilot waiting to happen.

:46:32.:46:36.

He in a quiet corner of Hertfordshire is a radar tracking

:46:36.:46:41.

station that is used to monitor the movement of objects 2000 kilometres

:46:41.:46:45.

above the earth. There are lots of things we got up

:46:45.:46:52.

there. 1,000 satellites, nearly 20 telescopes and one space station.

:46:52.:46:56.

But there's also a lot of junk, affectionately known as space

:46:56.:47:02.

debris. So space debris is effectively all of the stuff in

:47:02.:47:07.

space we know longer use or need. It could be dead satellites, did

:47:07.:47:12.

rockets, fragments, pieces of electronic circuits, pieces of

:47:12.:47:14.

paint from the outside of the spacecraft. They are floating

:47:14.:47:22.

around. The Final Frontier is packed with rubbish, litter.

:47:22.:47:27.

There's everything from an astronauts glove, that one stage in

:47:27.:47:33.

Orbit for a month, to particles of you're in, flushed from early space

:47:33.:47:39.

craft. There are bits of rock left by the Apollo missions. Even 32

:47:39.:47:46.

nuclear reactors that used to power satellites. This shows you a

:47:46.:47:50.

simulation of what we can see in Orbit. It ranges from debris close

:47:50.:47:57.

to the Earth to places where TV satellites up operating. Fees range

:47:57.:48:01.

in size from some things are size of a mobile phone up to a space

:48:01.:48:05.

station. Her these objects mean we are getting tight for space in

:48:05.:48:10.

space. We've realised over many years that although the universe is

:48:10.:48:15.

potentially infinite, the space around the Earth is very finite.

:48:15.:48:18.

But the problem isn't just that it is crowded up there, it is also

:48:18.:48:25.

dangerous. All these objects are hurtling about at over 25,000

:48:25.:48:32.

kilometres per hour. It is like a cloud of flying pockets. It has a

:48:32.:48:37.

high energy moving at that speed. A pound coin in Orbit around the

:48:37.:48:41.

earth has the same energy as a minibus travelling at 1,000

:48:41.:48:46.

kilometres an hour. If that hit a spacecraft, it would destroy it.

:48:46.:48:52.

1983, a chip of paint collided with the Space Shuttle. The impact was

:48:52.:48:59.

enough to crack its 1.5 centimetre thick windscreen. In 2009 a US and

:48:59.:49:04.

Russian satellite hit each other. Both were completely destroyed and

:49:04.:49:11.

created up to 1,500 new bits of junk. It can only get worse. In 60

:49:11.:49:15.

years we've gone from no man-made objects in Orbit to an estimated 35

:49:15.:49:22.

million. And the worry is that areas of space we rely on to send

:49:22.:49:25.

satellites for navigation, weather forecasting and TV will soon become

:49:25.:49:33.

no-go areas. Currently there's no working answer, but all sorts of

:49:33.:49:38.

plans are being hatched. From sales that would slow an object down so

:49:38.:49:44.

they fell back to earth to giant balloons that would inflate to help

:49:44.:49:51.

put the brakes on. But the UK's largest space company has come up

:49:51.:50:00.

Astrium in Stevenage is better known for building satellites that

:50:00.:50:07.

get sent to space. But engineer Jamie's job is to use his harpoon

:50:07.:50:13.

to drag them back to work. We've got a harpoon we are going to fire.

:50:13.:50:18.

It goes into the barrel inside a protective chamber. I will put some

:50:18.:50:23.

goggles on. For harpoon uses compressed air rather than

:50:23.:50:29.

explosives to fire. It is safer for space. We are ready to fire now.

:50:30.:50:39.
:50:40.:50:43.

Turn the firing switched on. Sadly At the moment, Jamie is test firing

:50:43.:50:48.

his harpoon into pieces of actual satellite. It's early days, but

:50:48.:50:52.

when complete the harpoons will have a spring loaded barrel and her

:50:52.:50:59.

capers. If the system works, the harpoon will be mounted on a

:50:59.:51:05.

satellite that will Chasetown space junk, harpoon it and tow it back

:51:05.:51:10.

towards earth where we it will burn up socially in the atmosphere. --

:51:10.:51:15.

safely. This only works with large objects. In Orbit, pig objects are

:51:15.:51:21.

just thousands of small objects waiting to happen. -- big object.

:51:21.:51:25.

Something has to be done and this could be the big thing -- best

:51:25.:51:31.

thing. But until somebody can enforce an intergalactic litter

:51:31.:51:35.

campaign, the research has to continue.

:51:35.:51:40.

This is a vivid demonstration of the problem. This is lent was by

:51:40.:51:48.

the National Space Centre a, a panel from a satellite. That is a

:51:48.:51:52.

great picture with us shuttle underneath. The office was in Orbit

:51:52.:52:00.

for six years. They saw this Goring. These are impact of micro meteors.

:52:00.:52:06.

Invisible to the human eye. They are travelling between 8 and 9

:52:07.:52:09.

kilometres per second and up to 30 kilometres per second. A tremendous

:52:09.:52:18.

amount of energy. The plasma Burns. If you lift it up, you can see...

:52:18.:52:25.

This is the spacecraft... That is a whole and that is a whole. You can

:52:25.:52:33.

see the Dent. Minuscule pieces of dust. Back over to mark in Dobbie.

:52:33.:52:38.

Last time we saw him he had unveiled our version of Herschel's

:52:38.:52:44.

telescope. Have they observed anything with it?

:52:44.:52:47.

Unfortunately not. It is amazing standing on this platform like

:52:47.:52:51.

Herschel did all those years ago. Herschel did it in the damp English

:52:51.:52:55.

weather. I'm safer than he is because I have harnessed to make

:52:55.:53:01.

sure I don't fall off. There have been times observers have fallen

:53:01.:53:04.

off those platforms. We can't show you any pictures, but it is

:53:04.:53:08.

incredible to think that Herschel spent many years observing the

:53:08.:53:13.

British night sky with the weather to contend with. We did get some

:53:13.:53:18.

clear skies a few nights ago. We managed to record some images of

:53:18.:53:19.

managed to record some images of things in the sky. The first

:53:19.:53:23.

things in the sky. The first picture we got was Jupiter. Moving

:53:23.:53:28.

very gracefully across the screen, caused by the rotation of the Earth.

:53:28.:53:30.

The telescope doesn't have the The telescope doesn't have the

:53:30.:53:35.

drive system so you can't see the object being tracked. A picture of

:53:35.:53:45.

a beautiful Binary Star system in Cygnus. We have the picture of a

:53:45.:53:52.

star cluster inside the Orion nebula. We have a final image of

:53:52.:53:56.

Uranus which Herschel discovered with a slightly smaller telescope.

:53:56.:54:00.

There's a very slight distortion which is caused by the orientation

:54:01.:54:05.

of the optics in a telescope. He will have had to have contended

:54:05.:54:09.

with these poor images. We can't show you anything live tonight, but

:54:09.:54:13.

it is great to follow in Herschel's footsteps. Without greater

:54:13.:54:16.

astronomers like him, we would not have learned as much about the

:54:17.:54:21.

universe as we can see now. It is great that we can leave his

:54:21.:54:24.

telescope to the residents of Derby so hopefully in the years to come

:54:24.:54:28.

they can enjoy the night sky like Herschel did all those years ago.

:54:28.:54:33.

Back to the studio. They are beautiful images and that

:54:33.:54:37.

talent the scope will be in Derby for the next three years. --

:54:37.:54:42.

telescope. This week you have been doing your own pioneering

:54:42.:54:47.

scientific work thanks to our online experiment. We asked you to

:54:47.:54:51.

study Mars's surface looking for unusual features. I spend a lot of

:54:51.:54:58.

time looking at this guy thinking it is amazing. In this case, the

:54:58.:55:01.

hyperbolic and third -- adjectives are appropriate. This is wonderful

:55:01.:55:08.

and amazing. Real science in two days. More than 100,000 people have

:55:08.:55:12.

helped us explore an area about the size of Holland. It was

:55:13.:55:18.

Switzerland! We are working our way up. We found some great stuff. We

:55:18.:55:21.

were looking at the Antarctic region of Mars and these strange

:55:21.:55:25.

France which we think on from material suddenly erupting

:55:25.:55:27.

material suddenly erupting underneath the surface of Mars. We

:55:27.:55:31.

had this idea that it has to do with ice under the surface that was

:55:31.:55:38.

being heated up. It is the time lapse. Yes. It was a year on Mars

:55:38.:55:44.

has put together by users. At some point in the year, in the Martian

:55:44.:55:48.

spring, these things erupt as the planet heats up? That is what we

:55:48.:55:53.

now know. I can tell you for sure because we only find these around

:55:53.:55:59.

March in the Marshin calendar. They happen close to the equator and

:55:59.:56:02.

then they head closer to the polls and we thought they were rare, but

:56:03.:56:06.

look at this. This whole region of ground would have erupted

:56:06.:56:14.

underneath your feet. Don't go there in the spring! What about

:56:14.:56:18.

this are titters -- artistic impression. We discovered that. Our

:56:18.:56:22.

viewers discovered that is what is happening. We know when and where

:56:22.:56:25.

it happens and we now know it is much more common than we thought.

:56:25.:56:32.

That is because people used pattern recognition skills. More than that.

:56:32.:56:35.

A good scientific experiment always leaves you with more questions.

:56:35.:56:39.

We've no idea what this is. This is a type of terrain I'd never seen

:56:39.:56:45.

before. It has angular features. These moved from year to year. No

:56:45.:56:49.

idea what this is. It is something to do with ice escaping from

:56:50.:56:53.

underneath and going into the Martian atmosphere. People will be

:56:53.:56:57.

working on this the years. Wonderful. We have more time in the

:56:57.:57:06.

show afterwards. I pledged applied to somebody. -- a pint. Tell us

:57:06.:57:11.

what to think that is. The best week, I will buy you another pint.

:57:11.:57:16.

I'm very excited. What is that? other guy is still waiting for his

:57:16.:57:21.

plight. Before we go, just time to say goodbye to Liz and NASA. How

:57:21.:57:30.

has it been? 30 seconds. Thanks. It's been such a privilege to meet

:57:30.:57:34.

all of the people behind so many or inspiring endeavours. What struck

:57:34.:57:37.

inspiring endeavours. What struck me most is how every single mission

:57:37.:57:41.

seems impossible on paper. I'm not sure what impresses any more, for

:57:41.:57:46.

fact they are able to dream up crazy schemes like lowering a road

:57:46.:57:51.

on to Mars using as Guy Cramer and sampling, it as they hurtle through

:57:51.:57:54.

space or the fact they are able to make those ideas a reality. They

:57:54.:58:00.

are always thinking ahead. By the mid- 2020s, there's talk of putting

:58:00.:58:04.

a man on an asteroid, and a few decades after that a man on another

:58:04.:58:08.

planet. It is an exciting time. Sadly, it is time for us to say

:58:08.:58:15.

goodbye to everybody at NASA and you at home. At night from NASA.

:58:15.:58:22.

Thank you for wearing your telescope hat especially! Don't

:58:22.:58:25.

forget there are hundreds of stargazing events happening up and

:58:25.:58:29.

down the country. Details are on the website, bbc.co.uk/stargazing.

:58:29.:58:36.

Don't forget about our Star Guide. We're going to be back in a second,

:58:37.:58:42.

but do you want to wrap up? discoveries on Mars are real

:58:42.:58:45.

scientific discoveries. Chris was telling me there's going to be a

:58:45.:58:50.

paper written. There's a scientific paper written and everybody

:58:50.:58:53.

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