Episode 3 Stargazing Live


Episode 3

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Tonight we have great news. Stargazing viewers may have made a

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genuinely significant scientific discovery. Thousands of you have

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been hunting for pulsars - or elusive spinning stars. We will be

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listening to some of the new once you have found with the giant is

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behind us and also to not what it is like a walk on the moon, Ben Miller

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will join us to find out with the help of a few balloons. We have more

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from bridge in space Tim Peake about life in orbit. And the final part of

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astronaut training for Tim Peake wannabe John Bishop. So far we've

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nearly drowned him, starved him of oxygen and tonight he has to cope

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with the dreaded centrifuge. I'm lie, he's Dara O Briain and this is

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Stargazing Live. Welcome back to this beautiful clear

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night at Jodrell Bank Observatory, my goodness, we are all counting

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down to the historic my goodness, we are all counting

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show we will get a snapshot of ordinary life on the International

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Space Station. A genuinely significant discovery, that is not

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the usual kind of television, you may say that we would say that, but

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we have been speaking to a fantastic team of scientists today, we are

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excited about the thing you have found, we are talking about pulsars,

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we have one of the astronomy grates with us, the discoverer of pulsars,

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to discuss that discovery. If you have anything to ask, send us your

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questions, and if you would like to get their behind-the-scenes look,

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the usual addresses on screen out. It's also a great night to get out

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and start looking up at the stars - Lucie is out in our Dark Field

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now... I'm joined here by astronomers from the University of

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Manchester, and I know that you said it is a clear night but it is just

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clouded over! Just five minutes ago we had a fantastic view of Comet

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Catalina, near the star allocate, in the handle of the plough, but the

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clouds have come in. We are optimistic. This evening we will be

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looking at the future of the sun through our telescopes, back to you

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in the studio. First, this week has been all about astronaut Tim Peake.

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Tomorrow, we will bring his been all about astronaut Tim Peake.

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ever spacewalk, and we will be been all about astronaut Tim Peake.

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joined by Chris Hadfield. To give us an idea of the kind of training

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Tim's been through - Liz Bonnin has been at the European Space Agency's

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Astronaut Training Centre in Cologne with John Bishop - setting him a

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series of astronaut tests... She should be preparing John for his

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latest and last mission. It could well be the end of him! LAUGHTER

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Welcome to Envihab, at the German Aerospace Centre, state-of-the-art

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medical research facility, I am so excited to show you this, we speak

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about ground-breaking signs on Stargazing all of the time and this

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could be the game change that is needed for long duration manned

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missions to space. This is the short arm human centrifuge, and over here,

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training astronaut for the week, lying in one of its arms, about to

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do his last training exercises. This was the one you were dreading the

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most. Not looking forward to it, I do not even like the waltzer! I get

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motion sickness! Your mentor, Agnes Morgenstern, he he has been your

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always, and he is going to help you. You train them to get used to rocket

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launches and re-entrance. We go up to about 8G, that is to simulate an

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uncontrolled ballistic re-entry, that is when you are plummeting

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towards the ground. What does that feel like? You are pressed into your

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seat with eight times your own body weight, more than 700 kilograms of

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weight, it is like a cow sitting on your chest! 1G on earth, this

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machine can go from zero to 60, in 30 seconds, and when you were told

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you were doing this, what kind of Jeans were you thinking about?

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Re-entry is 3.5, four, at this is different, it is a different

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machine. -- what kind of G. This is reminiscent of what fighter pilots

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go through, the G-force passes from your head to your feet, there is a

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chance you could pass out through lack of blood to your brain.

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Thanks! LAUGHTER It is difficult to breathe but there

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is no danger of passing out. This herd has got to go over your head,

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the flashing lights can cause fits blackout, but there is a camera in

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there, so we are keeping a close eye on you, and so we are ready for

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this, John, are you ready? -- hood. This is so much fun! LAUGHTER

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You wanted to be an astronaut! He would join a very select set of

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people who have been in a centrifuge for the purpose of this programme.

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What is interesting, astronaut Andreas was eight G, he looked

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exactly the same as he does at 1G. Where is asked... Me, in particular!

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LAUGHTER That is about 5.5, if I remember...

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Five, coming straight through... It pulls the blood out of you and you

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Five, coming straight through... It would faint at that point. That is

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my excuse for that face! Back in October last year, we had our

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closest approach in nearly a decade from a major asteroid of

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earth-threatening size. What became known as the 'Halloween Asteroid' -

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this spookily skull-shaped thing - loomed out of deep space

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this spookily skull-shaped thing - 31st. And it was just the latest in

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a long line of close encounters. And one day, whether we like it or not,

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something very big is going to be on a collision course with earth -

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doing a lot of damage...unless we do something about it. VOICEOVER: It

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came without warning... A ten tonne rock, on a collision course with

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Earth... Nearly a thousand people have been injured by debris

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Earth... Nearly a thousand people flying glass after a media shot

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across the sky in Russia, sending fireballs crashing to. With the

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power of 13 nuclear bombs, it was a warning shot from space, telling of

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an earth-shattering disaster waiting to terror the world apart. --

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sending fireballs crashing to earth. What if next time it was bigger? Are

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we ready? Alex Gibbs is the nightwatchman, his job is to look

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we ready? Alex Gibbs is the out for asteroids that written our

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planet. As the sun sets, his watch at the Catalina sky survey telescope

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begins. The asteroids we look for really do pose a threat to the

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Earth, and we are interested in those over a certain size that could

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do damage. Catalina is among a global network of asteroid spotting

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telescopes, and here we have a live image coming back

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telescopes, and here we have a live spots that move in successive

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photographs. Four hours, there is nothing. But just after midnight, as

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we are filming, Alex spots something. -- for hours. Here we go,

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this object is moving faster than quite a lot of the stuff that we

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see, it looks interesting, it is almost definitely a near Earth

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asteroid. Brand-new discovery, Alex is keen to launch a well rehearsed

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procedure. I'm going to send this to the Minor Planet Centre, so that

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other observers around the world can follow it up. First step in

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assessing the threat to Earth. If the risk is higher, the next call is

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to Nasa. Scientists will calculate the impact site... The US president

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will be informed, and if necessary, orders are given to evacuate. What

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is the assessment tonight? Are we doomed(!) in my opinion this

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asteroid is quite small, robbery in the order of the few metres at most,

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maybe ten, small enough that even if it hit the Earth, it would burn out.

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For now, we are safe... What if it was bigger? And heading towards

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Earth? One ingenious solution takes some rather surprising inspiration!

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It might not look it, but this is a serious demonstration of how this

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professor plans to save the world. Essentially, the gas and the

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particles injected from the extinguisher were propelling the

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person. And that is the same principle that we want to use to

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deflect an asteroid. -- ejected. Using lasers in his laboratory at

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the University of Strathclyde, Max is going to test the theory. This is

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a sample of meteorite, made from the same material as an asteroid. It is

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suspended in front of a superpowered laser. And we will try to vaporise

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part of the meteorite. It will be like a rocket engine. It is heated

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up to 3000 degrees, creating a gas jet, a bit like a fire extinguisher.

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The jet of gas expands in one direction, the meteorite in space

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would move any opposite direction, changing trajectory. Thus saving the

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world from a catastrophic impact. Max's dream is one of a handful of

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serious projects. Like Nasa's planned to crash into

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serious projects. Like Nasa's 2022, to see if they cannot it off

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course. It is all a long way from becoming a reality. So, in the

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meantime, we rely upon Alex! And his early warning system.

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STUDIO: The Halloween Asteroid that we did not see until three weeks

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before... Interesting object, looking at this series of still

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images, it is actually a dead comet nucleus, we talked about Rosetta

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yesterday, this was a nucleus, we talked about Rosetta

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the solar system for 4.6 billion years, the interesting thing is that

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we did not see it, it came up at an angle, essentially, not one of those

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that we had seen in the surveys, taking us by surprise, when you plot

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its orbit, I can show you... taking us by surprise, when you plot

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show you what its orbit is, it is very inclined, to the plane of the

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solar system, it would have got knocked out of the plane by

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interaction with a planet that went past Jupiter, at some point. That is

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why we did not see it. We can calculate where it has been and

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where it is going to be in the future, it came passed in 1975, we

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found out, and we did not see it. Will it come past again? That is a

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40 year orbital period, yes, we know this one is not a danger but it will

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come back. It is about this one is not a danger but it will

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circumference... So that is about as big as the famous impact into

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busker, in Russia, in 1908... That flattened about five miles of

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forest. -- Tunguska. Even something 20 metres in the conference, if it

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hits a city at the right angle, it would pretty much wiped out a city,

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they are dangerous things. This is one of the reasons why, for space

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travel, for astronomy, this is very important, this is a real danger. If

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you calculate the big risk to civil as Asian, that is not

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self-inflicted, then asteroid impact, at some point, is one of

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them, and that is why, as you say, people like Tim Peake are learning

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to be engineers, to live and work in space, it is there will be

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to be engineers, to live and work in we can say this in certainty, it may

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be in 1000 years, but there will be a time when we have got to deal with

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something bigger than that. Ben Miller has joined us in the

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Darkfield. Actor, comedian, and fan of all things space! Thank you for

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joining us. Exciting to be here! Clouds are coming and going. When we

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first interested in space? Child of the late 60s, man walked on the

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moon, Apollo... 15, 16... I remember one of my first memories is seeing

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the body on the moon! I felt like I had... Not only had we gone to the

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moon, we had taken had... Not only had we gone to the

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moon! Seeing the footprints on the surface of the moon now, so

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exciting, will we ever go back? Of course we will, we must build the

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space rockets of the future, we will tell reform the moon, it will be

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amazing! Nearest neighbour, we should not forget about it, but we

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will be talking about the future of our son, and there is a magnificent

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object, when you look at it through a specialist solar filter, it really

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comes to life. Perhaps you can tell me something about the sun, it is...

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This is something that fascinates me, and I know that you are an

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expert, it gets much hotter and much colder over periods of hundreds of

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years. What is going on? It does vary a lot, sometimes it is cooler,

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sometimes it is hotter, depends upon the wavelength of light. It all

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comes down to the magnetic field. And PM and flow of the size and

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complexity, marvellous object. ISS it possible to predict if it will

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get hotter or colder in the future? Hard to predict but we're working on

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that but one question I get asked ISS how the sun ISS going to die or,

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will it end up shining forever? I have joined friends from the

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Chipping Norton amateur astronomy group to reveal how the story of the

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sun can be written in the night sky. We will look for objects telling us

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about the stages of the life of his son, from its past and its present

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and also looking into the future. The son was born four and a half

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billion years ago in a cloud of gas and dust and I have challenged Alex

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to usurp telescope to show us one of these nebula. How are you getting

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on? I am surprised because it is so windy, I was expecting the stars to

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be all over the place and this is what I have got, this six minute

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exposure. That is stunning, this is a star-forming, one of the many you

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can see in the night sky? You can find the nebula to the east of

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Orion. It is incredible to think that the sun started off this way.

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That is right. Our part of the universe would have looked like this

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for .5 billion years ago? Birth is just the first chapter in the life

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of the star, the Sunnis in the prime of its life, like 90% of the stars

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we can see. -- the sun is. One, which looks like a son, seen from

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outer space, is called Sirius and that is what you are looking at?

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Sirius is always at the foot and to the left of Orion, one of the

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easiest stars to find. The naked eye is fantastic, pair of binoculars, it

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will knock your socks off. What I love about ten to is that a twinkle

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is more than most stars. It goes, it sentiments, it has these flashes of

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colour. It looks like a diamond sparkling in the sky. Stars like

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Sirius and the sun spend the vast majority of their life in this

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middle stage. But to reveal their future, I have asked our astronomers

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to find a star that has reached old age. How are you getting on? Fine.

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It is a bright start towards Orion, very easy to find. Aldebaran has

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used up much of its fuel, Andy Serkis has cooled down, it has

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become a Red Giant. The colour really stands out through this

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eyepiece. It is very distinctive to look at, very orange, very

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attractive star. It is nice to look up but the star and think about the

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sun becoming this time of object when it approaches the end of its

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life. Our sun will become a Red Giant as the surface cools. Then, in

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around five billion years or so from now, it will start to die. Looking

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this far into the future is the hardest, the sun will end its days

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as a glowing ball of carbon and oxygen, about the size of the Earth,

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simply fading as it cools down. It will become a White Dwarf. What will

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it look like Ben? -- then? Hello. Happy started the white -- spotted

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your White Dwarf? Yes, have a go. Look carefully. There are none too

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stars, the bright one is tempted, the one like the sun, but next to

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it, only visible thanks to a filter, there is a smaller, faint White

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Dwarf called Sirius B. We can see the remnant of a star and think that

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is what is quite a become of the sun, that is fascinating to watch

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and have a look at in the night sky. There you have it, our sun will

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become dwarf in around 5 billion years. But White Dwarves themselves

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can take aliens or trillions of years to cool down and completely

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fade away and that feels like the sun will shine forever.

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In look to the future. Want to ask, have you ever seen a dead star in

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the night sky? How poetic! That reminds me of David Bowie. They are

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hard to find. I want to show you one of them. We have collided again, the

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cloud has just come over but earlier we captured a White Dwarf. , Cron

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two! White Dwarves what the sun will become in five billion years. These

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are the fading embers of stars and work with tricky to use but. This is

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to the west of Orion. -- to spot. Question, I thought all stars ended

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in a supernova. They were the famous stars but only the biggest ones die

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out this way but our sun is not big enough to produce a supernova, the

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court will collapse of the outer layers explode into the solar system

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but there was one of them we saw a couple of years ago in the Cigar

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galaxy spotted by chance during a break in the clouds. By students at

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the London University. And the supernova star is so bright, you can

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see it on the right-hand side of the Cigar galaxy and this one star

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outshone all of the others. How long does a supernova last? It just

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happened during a break in the clouds, they then will fade away

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over weeks and months. Imagine that, a break in the clouds. Could this

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ever happen? I will keep their fingers crossed! Thank you, we have

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a correction, extra live television, I said that the Halloween Asteroid

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was 20 metres in I said that the Halloween Asteroid

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is actually over one kilometre! That means that it was the side of an

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asteroid that would be a small country threat, rather than just a

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city. Just to reassure you... Don't have nightmares! Letters lift the

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mood! Everybody has been looking for a pulsar, this is the year five

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class at Harrogate Academy in Stockton-On-Tees and they have been

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doing searches for pulsars. It was not long ago that nobody knew that

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pulsars existed, that is until our next guest discovered the first one.

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One of the biggest names in astronomy, Jocelyn Bell-Burnell. How

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did you make that discovery? By accident. The classic way of making

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any discovery, also with hard work and some luck also. What were you

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looking for? I was supposed to be looking for quasars, which were very

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new, the hot, sexy topic and we did not know many of them so I was

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supposed to be finding one of them and I did but amongst all of that

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signal from the radio telescope was a tiny signal that did not make

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sense. We have some video of that telescope, that you build with your

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own hands? Along with half a dozen others. It took us two years. It

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covers an area of 57 tennis courts. What you said about the chance

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discovery, serendipity is one of the most valuable tools in science, if

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you pay attention. You see this regular radio pulse, what is your

:23:34.:23:40.

first reaction? Something is wrong. With your tools? Something mundane?

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You have to start with the mundane, you have to make sure you are not

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falling into some silly trap and shouting with enthusiasm, and that

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it really is cosmic. How long did it take you to realise this was a new

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astrophysical object, a pulsar? We had one month checking things out

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and at the end, I found a second and if you mix it, the third and fourth

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and that makes you think, is this some kind of new Star? Was predicted

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theoretically or where people waiting for an example? It was known

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the stars are very small, ten miles across. It is extreme in heart to

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see something that small garden space, people had not reckoned on is

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they a very strong magnetic fields and a sweep radio waves around the

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sky, like a lighthouse and each time it shined across the Earth, but had

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a pulse. What was the period of the one that you could see? Just over

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one second. The fastest I find was one quarter of the second but we

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know that some gold 700 times every second. You say that, ten miles, 20

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kilometres across, this is what our viewers have been looking for? These

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exotic objects. We discovered many of them, thousands in the sky, what

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is the interest today? They are of interest for several reasons. They

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way millions and millions of tonnes, in one ball ten miles across, that

:25:23.:25:27.

is very tense and the physics of that is in itself interesting. They

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are also very useful cox, they keep spending and since they have been

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found we have been able to test Einstein 's Theory of Relativity

:25:40.:25:43.

because these are very good clocks. The ones that are particularly

:25:44.:25:48.

reliable, we can look at for gravitational radiation, ripples in

:25:49.:25:54.

space time because they will bob in the ripples and you can see that.

:25:55.:25:58.

Gravitational waves. If the pulsar the ripples and you can see that.

:25:59.:26:05.

is close to another star you can test theories of gravity with the

:26:06.:26:10.

signal again. Up to now, the theories of Einstein are doing very

:26:11.:26:15.

nicely so far! And 101 years old, the Theory of Relativity. Each one

:26:16.:26:20.

is distinctive. Are they like landmarks in space? They are like

:26:21.:26:26.

navigation beacons, each has its own flash rate and its own pattern of

:26:27.:26:31.

clashes. When we travel through the Galaxy, in spaceships, we will not,

:26:32.:26:36.

but when people do, they will use these things like navigation

:26:37.:26:40.

beacons, we get the fix on several and think, we are here. We will not

:26:41.:26:44.

review will be discovered, we will talk about that later, but the holy

:26:45.:26:49.

Grail would be to find pulsars going around other objects? With a black

:26:50.:26:54.

hole would be the ultimate? That would be good, and in a triple

:26:55.:27:00.

system would also be good but all stars that are orbiting others,

:27:01.:27:04.

there is a lot of physics in that and information to be extracted. We

:27:05.:27:12.

don't have a triple system? We do. One pulsar going around another and

:27:13.:27:18.

going around another? Going around another star and the peril of them

:27:19.:27:22.

is going around another star. I see! And the question is, does this

:27:23.:27:27.

pulsars and the White Dwarf, do they behave the same way in the gravity

:27:28.:27:32.

of the Star? It is called the principle of equivalence. And by

:27:33.:27:36.

what we have discovered, that is later on... It is actually exciting,

:27:37.:27:44.

this is not television hyperbole! We have been catching up with Tim Peake

:27:45.:27:50.

on-board the International Space Station and write down his over

:27:51.:27:53.

South Atlantic, since we started this programme on Tuesday, he has

:27:54.:27:58.

circled the planet 32 times. He has a very busy schedule carrying out

:27:59.:28:02.

experiments and this week he has been preparing for his spacewalk

:28:03.:28:07.

tomorrow but also found time to send us some specially recorded messages.

:28:08.:28:15.

Good morning, it is Saturday morning at 730 yeah. I have just woken up.

:28:16.:28:25.

Time to get breakfast and start cleaning the station, it is this

:28:26.:28:25.

morning's job. Breakfast this morning. Scrambled eggs. Tim Peake

:28:26.:28:33.

cannot just put his pan on the hop, but of the food is dehydrated, so

:28:34.:28:40.

just add water. In five minutes that will be ready to eat. Even though it

:28:41.:28:46.

is not fine cuisine, eating is a lot more fun in microgravity.

:28:47.:28:54.

Like the rest of us, news morning routine involves a quick wash and a

:28:55.:29:02.

bathroom break. Unlike the rest of us, that involves some pretty

:29:03.:29:06.

specialist equipment. How do you go to the toilet in space? It really is

:29:07.:29:14.

quite simple... Here is the tube that you go in, you take off the

:29:15.:29:18.

cap, U-turn on the phone, the air flow keeps everything going down the

:29:19.:29:27.

pipe, and also... My number two, the air flow does the same thing, simple

:29:28.:29:29.

as that! I really hope that tube has been cleaned since it was last used!

:29:30.:29:34.

It is not all experiments and spacewalking on the International

:29:35.:29:38.

Space Station, in the vacuum of space there is a vacuum cleaner!

:29:39.:29:42.

Dust will either float around indefinitely or clog up the station

:29:43.:29:47.

filters, and so team has got to do his fair share of the chores.

:29:48.:29:55.

I reckon after all of that cleaning, it is time for a copy break, let's

:29:56.:29:59.

go! -- coffee. The coffee packet is filled with

:30:00.:30:12.

nice hot water, we need a little plastic straw. Insert the straw,

:30:13.:30:23.

take off the cap... And drink! After a productive morning, it is time to

:30:24.:30:28.

unwind. By far the best thing about being in space, is the view of

:30:29.:30:37.

planet Earth, let's take a look. STUDIO: When Tim launched into space

:30:38.:30:43.

on December 15 he was momentarily exposed to three times normal

:30:44.:30:46.

gravity, his arms and legs felt three times their normal weight on

:30:47.:30:49.

earth, ever since then, he has weighed nothing, of course, and

:30:50.:30:53.

finding out how that is affecting his body is an essential part of the

:30:54.:30:57.

research that he is doing in the space station. Research on the

:30:58.:31:06.

ground aims to make space travel less arduous on the body. But the

:31:07.:31:13.

only way to do that is understand how and why it punishes us, and then

:31:14.:31:19.

try to stop it happening. Over in Cologne, Liz Bonnin is at one such

:31:20.:31:21.

facility, the German Space Agency's 'ENVIHAB'. And she is about to offer

:31:22.:31:27.

the services of John Bishop for the advancement of

:31:28.:31:27.

to this short arm human centric views test. I'm doing OK. Are you

:31:28.:31:32.

ready for this? I think so. OK, start it, we have a doctor

:31:33.:31:38.

monitoring his vital statistics, technicians making sure everything

:31:39.:31:42.

is going to go smoothly, the lead technician is here, he's in control

:31:43.:31:46.

of the test to date. It will take 45 seconds to get up to where we need

:31:47.:31:51.

him too. I can feel myself getting drawn down, the pressure is going to

:31:52.:31:57.

my legs and my feet... Make sure you keep your head very still, are you

:31:58.:32:02.

feeling all right? Yes, I am getting a sensation of almost standing up.

:32:03.:32:09.

Why does he feel that? Because the balancing system, that balances

:32:10.:32:14.

towards the feed, this is felt as the same as standing up. Please do

:32:15.:32:19.

not try to stand up, that would not be a good idea! I can feel pressure

:32:20.:32:24.

into my back as well. That is centrifugal force for you! LAUGHTER

:32:25.:32:32.

Not too bad so far? Not so bad. You are doing brilliantly. We have

:32:33.:32:37.

already reached 2G, and we are 30 seconds into this phase, we are

:32:38.:32:44.

doing brilliantly. The idea, in the future, is that machines like this

:32:45.:32:47.

will go into space with the astronauts. Yes, and counteract the

:32:48.:32:51.

effects of microgravity on the muscles, so you would get doses of

:32:52.:32:56.

hypergravity, exercising as you would spin around, what kind of Gee,

:32:57.:33:02.

do we need to get to for that to happen? Between 1G, and 2G, to get

:33:03.:33:05.

up to that, what this would be the individual. It seems to be between

:33:06.:33:12.

1G, and 2G. This is the research you are carrying out, does this mean

:33:13.:33:16.

that this data will help in the research? Yes, it will give us

:33:17.:33:20.

information about different behaviours. Are you really going to

:33:21.:33:27.

be sending a comedian into space(!) at the very least tonight you are

:33:28.:33:31.

contributing to science! He has made it! Trying to take my mind of what

:33:32.:33:39.

is happening. You have a smile on your face, that is a bonus. Do not

:33:40.:33:47.

move your head! And I felt it, immediately, you feel a massive

:33:48.:33:48.

rush, and everything comes to your head... That has told you, you were

:33:49.:33:54.

told to keep still! That was close... One minute left at 2G, you

:33:55.:34:00.

have got this, you have got it. Well done. How long would astronauts have

:34:01.:34:07.

to train? Our idea is to have 20 minutes, nowadays, they are training

:34:08.:34:10.

to and a half hours, we can reduce this to 20 minutes. That would

:34:11.:34:14.

reduce the amount of time they must exercise, but you could make a

:34:15.:34:17.

bespoke machine, punching in your details determined on what number of

:34:18.:34:24.

GU can withstand. That would be for each astronaut. -- G. Yes, that

:34:25.:34:31.

could happen. Incredible, how far are we from making this area Lizzie?

:34:32.:34:36.

At the moment we are at the beginning, scratching the surface,

:34:37.:34:38.

we must find an answer within the next five years. Not a long time for

:34:39.:34:45.

research? We have to make sure that the data is valid, Nasa may be

:34:46.:34:50.

designing the spaceship around this centrifuge. How are you feeling? I

:34:51.:34:56.

can feel pressure along my spine, and in my neck... But it is OK...

:34:57.:34:59.

You have now completed three and in my neck... But it is OK...

:35:00.:35:04.

minutes, at 2G, and we are beginning to slow it down, how does it feel? I

:35:05.:35:10.

feel it now. I feel it... It is like my own brain is catching up with my

:35:11.:35:14.

body and meeting it on the way back! That is a beautiful way to describe

:35:15.:35:18.

it! Are you feeling like you are going in a different direction? Yes,

:35:19.:35:23.

completely. The fluids in the balancing system are adapted to that

:35:24.:35:30.

spin, if you stop, it is still swirling around, and you have a kind

:35:31.:35:35.

of vortex. Let's go in and see him, a big thumbs up, delighted to see

:35:36.:35:42.

that! There was a bag for any eventuality... (!) he did not have

:35:43.:35:47.

to use it, rate news. Is in here... INAUDIBLE

:35:48.:35:50.

I did not want to be showing everyone me dinner! Well done, you

:35:51.:36:00.

have made it! Knowing what 2G, feels like, you think he would be able to

:36:01.:36:05.

exercise during that? I can really appreciate how it changes your body,

:36:06.:36:09.

you need if you goes of this, but I can see that you can move on and

:36:10.:36:17.

exercise. Would you go higher, now that you know...? Of course I would!

:36:18.:36:19.

That was your final Astronaut Training Centre is a completed, come

:36:20.:36:24.

back to us to get the final verdict to find out if John Bishop has the

:36:25.:36:30.

right stuff to go to space! STUDIO: Well done, John, you did not vomit,

:36:31.:36:40.

you win! LAUGHTER We are still out here,

:36:41.:36:48.

unfortunately, it has clouded over, two minutes ago it snowed on us! We

:36:49.:36:48.

unfortunately, it has clouded over, cannot show you any stars at the

:36:49.:36:51.

moment, but there is something I can show you which does not need good

:36:52.:36:55.

weather, something I have on my phone, this is a prototype messaging

:36:56.:37:01.

service, Whispering Stars, I hold up my phone and move it around, and

:37:02.:37:05.

there is an arrow which point me towards a star that has a message

:37:06.:37:10.

for me... If you want to use this service and send people messages,

:37:11.:37:14.

head over to the website and click on the appropriate button --

:37:15.:37:19.

corresponding button and see if you can see the message I have left for

:37:20.:37:24.

corresponding button and see if you you. The message on my phone says,

:37:25.:37:24.

corresponding button and see if you don't forget about the planets. That

:37:25.:37:27.

is right, this is a great time for planets. We had an amazing view of

:37:28.:37:34.

the planet Venus this afternoon, that was during the daytime, we

:37:35.:37:37.

often forget that we can do it in the daytime. And then later on we

:37:38.:37:41.

have the line-up of the five planet closest to us in the dawn sky. What

:37:42.:37:44.

one planet we cannot see so easily from you, a special planet, but we

:37:45.:37:48.

know somebody who can, and that is Tim Peake.

:37:49.:37:52.

The most amazing thing about being on board the International Space

:37:53.:38:00.

Station is the view of panic error -- the view of Janet Earth, every

:38:01.:38:03.

time I looked out I see something unexpected and completely different.

:38:04.:38:11.

Thunderstorms over planet Earth. -- the view of planet Earth. Lights on

:38:12.:38:18.

the cities, thunderstorms, and by daytime, magnificent cloud

:38:19.:38:21.

formations. Whole weather systems that are covering vast areas of the

:38:22.:38:27.

globe. It is truly stunning and truly beautiful.

:38:28.:38:32.

STUDIO: All week we have been attempting demonstrations to look at

:38:33.:38:39.

the physics of space exploration, proper science. Proper science! The

:38:40.:38:46.

gyroscope shed, we had a tanker... There it is... Collapsing in a

:38:47.:38:53.

vacuum! Today we are exploring gravity with the help of Ben Miller

:38:54.:38:58.

and these helium balloons! LAUGHTER Looking very comfortable... I should

:38:59.:39:04.

explain what we are trying to do here, we are... We have helium

:39:05.:39:08.

balloons, essentially, we can see what an astronaut on Mars could

:39:09.:39:17.

actually do. The jumping is amazing! Apart from the slight wedgie

:39:18.:39:26.

effect... That is really good! I think I want a go! LAUGHTER

:39:27.:39:37.

There is a points to this! LAUGHTER The point is, when the Mars Rover

:39:38.:39:44.

goes and lands on Mars, built in Britain, by the way, the chassis of

:39:45.:39:47.

the Rover, it must dig down below the Martian service, to look for

:39:48.:39:52.

life which may exist below the surface, digging on Mars is

:39:53.:39:58.

difficult... Echoes, as Ben will demonstrate, it gives you do not

:39:59.:40:01.

have the weight, you have only half the weight, you can see... You

:40:02.:40:04.

cannot apply the force downwards on the drill... LAUGHTER

:40:05.:40:11.

Or on the shovel, to get through the surface, it means it is a terrific

:40:12.:40:21.

engineering challenge... LAUGHTER If only we had this man on Mars!

:40:22.:40:29.

LAUGHTER We would be absolutely fine!

:40:30.:40:32.

LAUGHTER We could have a really great act!

:40:33.:40:39.

That is actually really liked! People will be able to do a

:40:40.:40:44.

piggyback, important in space! All week we have been asking you to find

:40:45.:40:49.

new pulsars, extraordinarily dense spinning stars... I'm doing this

:40:50.:40:54.

really seriously!... Here is a story about how pulsars can be such

:40:55.:40:55.

essential tools for astronomers. VOICEOVER: Smartphones and Wi-Fi,

:40:56.:41:11.

online shopping and microwave meals. These technologies have shaped the

:41:12.:41:14.

world, where would we be without them? Greenbank, West Virginia, that

:41:15.:41:24.

is where. It is a nice, quiet, simple life. Very little crime, not

:41:25.:41:31.

a lot to do. This is not a town that time forgot, it has just turned its

:41:32.:41:38.

bank on modern technology. No microwave, no cell phone, no Wi-Fi.

:41:39.:41:44.

For folks that visit here, sometimes they break out in hives and rashes

:41:45.:41:47.

because they are not comfortable without being connected. -- it has

:41:48.:41:52.

turned its back on modern technology. The time warp existence

:41:53.:41:56.

is because of this. The Greenbank telescope. It is the largest movable

:41:57.:42:04.

structure on the planet. It is so sensitive that the town-macro boss

:42:05.:42:07.

residents have to live in total radio silence. -- Green Bank. It is

:42:08.:42:16.

all to help Professor Scott Ransom. Scott is searching for a whole new

:42:17.:42:22.

way to observe the universe. Everything we know about the

:42:23.:42:25.

universe we have found out so far using the electromagnetic spectrum,

:42:26.:42:29.

just like liked that your eyes can see. Light reveals stars, galaxies,

:42:30.:42:35.

universe teeming with wonderful objects. But there is more, we win

:42:36.:42:45.

over 96% of the universe is invisible. For now, at least. Scott

:42:46.:42:53.

wants to reveal it. Not by waves of light, but with mysterious waves

:42:54.:43:00.

that no one has detected before. Gravitational waves. If we can start

:43:01.:43:06.

measuring gravitational waves and Gravitational waves. If we can start

:43:07.:43:06.

doing astronomy with them, it is looking at the universe in a whole

:43:07.:43:14.

different way. Gravitational waves are ripples in space-time. Nobody

:43:15.:43:19.

knows for sure that they exist. We do know that massive object, like

:43:20.:43:26.

black holes, distort space time. It is thought that massive things

:43:27.:43:29.

moving will create waves in space time.

:43:30.:43:38.

These gravitational think are coming from many different

:43:39.:43:39.

sources throughout the universe, they are flowing through us, through

:43:40.:43:43.

the Earth, through the solar system, that means our bodies and a tiny --

:43:44.:43:47.

at a tiny level are being stretched and compressed. These movements are

:43:48.:43:54.

small, under the nucleus of an atom. So there are effects are easily

:43:55.:43:57.

drowned out by electronic interference. -- so their effects.

:43:58.:44:07.

To search for them, Scott needs an enforcer to keep the airwaves clean

:44:08.:44:10.

in Greenbank, and that enforcer is Chuck. I am looking for unknown

:44:11.:44:16.

radio signals. Something that is screwing up the data, it is our job

:44:17.:44:22.

to figure out what it is. -- Green Bank. And if it is something that we

:44:23.:44:28.

can fix, we found a heater in a doghouse that was causing

:44:29.:44:30.

interference, all kinds of things can cause problems.

:44:31.:44:36.

If Chuck can help keep the airwaves clear, and help tune into these

:44:37.:44:44.

mystery swathes, it might reveal but we have never seen before. Like

:44:45.:44:49.

directly observing the inside of a black hole. Or detecting dark

:44:50.:44:54.

matter. The invisible stuff that makes up much of the universe. But

:44:55.:45:00.

to find gravitational waves, Scott must play detective. He is trying to

:45:01.:45:07.

observe their tiny but potentially measurable effects on pulsars. That

:45:08.:45:15.

sound you can hear is a pulsar and we can measure with high precision

:45:16.:45:22.

the rate at which it is rotating and that lets us do the science with it.

:45:23.:45:26.

You are listening to light waves from a spinning pulsar, converted to

:45:27.:45:30.

sign. The tone does not change unless something disturbs the

:45:31.:45:36.

pulsar. Like a ripple in space time. The gravitational waves, moving

:45:37.:45:43.

through space, compress space time and that causes a change in the

:45:44.:45:48.

tone, much like if I have a tuning fork, the Doppler effect causes the

:45:49.:45:57.

change in its tone, like this. If Scott can spot a pitch change in the

:45:58.:46:03.

pulsars he is monitoring... He will have detected a ripple in space

:46:04.:46:11.

time. For the very first time, he will have proved that gravitational

:46:12.:46:14.

waves exist, but he cannot do this alone. As long as the observatory is

:46:15.:46:20.

here, that is a good thing for the community. For the sake of science,

:46:21.:46:27.

we can do without cellphones. It will be such an historic discovery,

:46:28.:46:30.

people around the world are racing to beat Scott and the good people of

:46:31.:46:34.

Green Bank. Using everything from giant lasers to space probes. The

:46:35.:46:43.

first detection of gravitational waves will definitely get the Nobel

:46:44.:46:47.

Prize so I am hoping we will be the first but who knows? Were joined by

:46:48.:47:00.

Tim O'Brien, Chris and Jocelyn Bell-Burnell. People are trying to

:47:01.:47:08.

beat the observatory, and one is Jodrell Bank? Were all hunting for

:47:09.:47:13.

gravitational waves and to be the first to get there. Let us look at

:47:14.:47:18.

the scientific discoveries we have made. We announced this at the

:47:19.:47:23.

start, an incredible thing has been discovered? We did not know this

:47:24.:47:29.

would work but the Stargazing Live audience have come through once

:47:30.:47:35.

would work but the Stargazing Live again, we have looked at 3 million

:47:36.:47:36.

separate observations across hundreds of thousands of parts of

:47:37.:47:40.

the sky and we have found a good handful of pulsars were things we

:47:41.:47:44.

think might be pulsars and we have been using the telescope to follow

:47:45.:47:51.

up on this. A handful of pulsars? That would be very heavy material

:47:52.:47:56.

indeed! There is lots more work to do and we have started to put the

:47:57.:48:00.

results on the website but I thought we would talk about one particular

:48:01.:48:05.

discovery that we have been able to confirm using the telescopes. This

:48:06.:48:09.

is what we started looking at life on the television? Reset the

:48:10.:48:13.

telescope turning and this busy pulsar we have got the results from

:48:14.:48:18.

and it did turn out to be a pulsar. We looked at the data overnight and

:48:19.:48:26.

this is a pulsar. This is how it appeared on the website, this is

:48:27.:48:30.

data from a survey done by a telescope in Germany, there are

:48:31.:48:34.

pulses, that could be anything, somebody's mobile phone, another

:48:35.:48:39.

source but we looked at this with the Lovell Telescope and let us

:48:40.:48:47.

see... This is 30 minutes of observation, the pulses arriving in

:48:48.:48:51.

this sequence and we can turn this into a signed. That is the sound of

:48:52.:49:01.

a pulsar? This is the new pulsar that viewers discovered. We should

:49:02.:49:03.

just visualise this because this is a star of the size of a city? 1.5

:49:04.:49:13.

times the size of the sun. And that is the spinning red? About 30 times

:49:14.:49:19.

every second and that buzz that you can hear is the sound. That is

:49:20.:49:26.

pretty fast and the reason is that we know that this pulsar is in a

:49:27.:49:30.

binary system so it is in orbit around something else and we know

:49:31.:49:35.

that because that's tone has been changing over the time that we have

:49:36.:49:40.

had the observation so we had the archive of observations from last

:49:41.:49:42.

night and that spin rate has slightly changed. Five millionths of

:49:43.:49:51.

a second. It seems to be moving. From the observation people looked

:49:52.:49:54.

at and the observation from last night. Do we know what it is moving

:49:55.:49:58.

around? The likely candidates are the dead remnants of a partner star,

:49:59.:50:06.

either a White Dwarf, or it would be another neutron star, it is right on

:50:07.:50:12.

the border and with the properties we know about today, we cannot tell

:50:13.:50:17.

you which it is but what the team will do is watch this thing

:50:18.:50:21.

continuing around its orbit and once we have got the orbit we can work

:50:22.:50:28.

out the mass. We spoke earlier about the system, these global systems

:50:29.:50:33.

which are fascinating objects and also for

:50:34.:50:37.

which are fascinating objects and Relativity. Quite an exciting

:50:38.:50:42.

discovery, but are not many of them but can you give us some sense of

:50:43.:50:47.

what the system is like? We know all about 2500 pulsars but only a couple

:50:48.:50:51.

of hundred that are in binary systems. This one feels different,

:50:52.:51:03.

what strikes me is when we saw the Jodrell data stacking up, like Joy

:51:04.:51:07.

division cover... It has a very sharp cut-off point, that particular

:51:08.:51:15.

pulsar, slow rise and then donk! It is unusual. I do not know what this

:51:16.:51:23.

is telling us. This has definitely got structure, it has got three

:51:24.:51:26.

different peaks. If we use the Lighthouse

:51:27.:51:28.

different peaks. If we use the light keeps flashing when it goes

:51:29.:51:33.

past us and we're seeing some structure around the thing that is

:51:34.:51:37.

emitting that light, right down at the pulsar level. We have the

:51:38.:51:44.

distance measured? We do. We actually have a map. We look at

:51:45.:51:50.

where these pulses are arriving in different parts of the radio

:51:51.:51:55.

spectrum and that is the sun and the Milky Way and we can add the pulsar

:51:56.:52:00.

to that, it is 18,000 light years away, the green dot, out in the

:52:01.:52:10.

Perseus spiral. This is about 20 kilometres across! 18,000 light

:52:11.:52:17.

years away! We actually have the people who discovered this? There

:52:18.:52:24.

are quite a few of them and the names run the website of some of the

:52:25.:52:32.

first, we have got them. We have the Flynn family, are you excited? Very!

:52:33.:52:40.

How many would you look through? Hundreds! It does take a while to

:52:41.:52:49.

find these things! This is very serious stuff! Did you have any

:52:50.:52:54.

sense that this was going to be something big? Did it stand out? No,

:52:55.:53:02.

there were loads, we could not find any until nine! How did you feel? We

:53:03.:53:08.

spoke yesterday about this and when you look at data, you find something

:53:09.:53:13.

and for a moment, for a few hours, you were the only people on Earth

:53:14.:53:18.

and in human history to know about the existence of that thing. How did

:53:19.:53:25.

that make you feel? Really excited! We have a smaller problem, I'll be

:53:26.:53:35.

going to name it after Neeve or after Aidan? We decided to name it

:53:36.:53:49.

after one of the guinea pigs! So... So it shall be called O-M. It is

:53:50.:53:55.

good we had that committee meeting! That is the level at which these

:53:56.:54:01.

things happen! He named his after his guinea pigs! Well done to the

:54:02.:54:07.

family. This is a genuinely exciting discovery? It is really good. We

:54:08.:54:16.

don't know just how good it will be, we only have these few observations,

:54:17.:54:22.

it might turn out to be great. You will not tell anyone precisely where

:54:23.:54:26.

it is? People want to make sure they can get all the information first.

:54:27.:54:38.

The other thing, especially these other candidates that we think are

:54:39.:54:38.

promising, these possible pulsars, if they are true, another thing we

:54:39.:54:42.

have shown is that there is a lot more in this data that most

:54:43.:54:46.

astronomers had anticipated. This will go on? Were used to skimming

:54:47.:54:52.

off the top of his observations and looking for the brighter ones but if

:54:53.:54:55.

there are extra pulsar is in that noise, we will make more of an

:54:56.:55:01.

array. Someone else who needs to be things -- congratulated after

:55:02.:55:06.

arduous work at the Astronaut Training Centre, it is John Bishop.

:55:07.:55:11.

Is he ready for space? I think he is, he survived three days of

:55:12.:55:15.

astronaut training and this, I have to say city! I have loved this, I

:55:16.:55:22.

have gained a real appreciation of the commitment that the astronauts

:55:23.:55:27.

go in for but also the commitment of everyone around them, and the level

:55:28.:55:31.

of science going on every day. What surprised you the most? That they

:55:32.:55:40.

had a suit to fit me! Somewhere between an astronaut and a

:55:41.:55:48.

ghostbuster, I feel like! I think just the whole amenity, it is one of

:55:49.:55:54.

those things, people going into the Space Station, it is out of this

:55:55.:55:58.

world, obviously, but all the way down, at every level, people are

:55:59.:56:02.

contribute in. The amount of things they think of, no stone is left

:56:03.:56:07.

unturned. How do you think he has done? Brilliantly, really well. We

:56:08.:56:14.

even have something for you to complete that suit! Your own little

:56:15.:56:23.

personal patch! That is my patch? It even has a microphone on it! You are

:56:24.:56:27.

personal patch! That is my patch? It officially part of the gang. You

:56:28.:56:31.

have done so incredibly well. Yes, I am so proud of you. Some of those

:56:32.:56:35.

things were very hard, but well done. He is on the crew for the next

:56:36.:56:44.

mission? It does not matter! This is me dressing up for my no doubt! We

:56:45.:56:50.

have had an amazing time. Over the next three days we will see just how

:56:51.:56:55.

much goes into getting an astronaut ready for space and we have also

:56:56.:56:58.

seen the extraordinary amount of science that takes place, science

:56:59.:57:02.

football ultimately contribute to the success of long-term space

:57:03.:57:05.

exploration, missions that are just within our grasp and it has been a

:57:06.:57:11.

privilege to meet you and play with John Bishop, it has been great fun,

:57:12.:57:16.

good night from us! Take care. Thank you very much. And to everyone there

:57:17.:57:23.

at the German Aerospace Centre. And that has cost you ?40 because he

:57:24.:57:29.

survived! Yes! To all of the guests because -- Tim O'Brien, Lucie Green,

:57:30.:57:39.

need, Aden and the guinea pigs! Very complicated name! Yes. Pulsar O-M.

:57:40.:57:47.

That is all we have time for. OK, I must say, I am very excited about

:57:48.:57:59.

this discovery. How long will we be trawling through these results? Four

:58:00.:57:59.

months at least. We have done six years of work in done two days, the

:58:00.:58:05.

team will be very busy. And it helped to train all of these

:58:06.:58:10.

computer algorithms so we will be better at finding pulsars. And you

:58:11.:58:13.

have got some new PHD students, there! Definitely! Thank you all

:58:14.:58:21.

again, tomorrow, the first ever there! Definitely! Thank you all

:58:22.:58:22.

spacewalk for Tim Peake, we will watch all seven hours and we will

:58:23.:58:27.

bring you the highlights from nine o'clock tomorrow on BBC Two. Until

:58:28.:58:29.

then, goodbye! So, no-one pays tax here?

:58:30.:59:02.

No-one pays taxes.

:59:03.:59:06.

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