The Mystery of 'Oumuamua The Sky at Night


The Mystery of 'Oumuamua

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Last October, astronomers made a spectacular discovery.

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For the very first time,

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they spotted an object visiting our solar system from outer space.

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It set off a hurricane of press speculation.

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Tonight, we have new, exclusive revelations

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and reveal the complete story of this mysterious visitor,

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which now goes by a suitably exotic name -

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'Oumuamua.

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To tell this detective story, I've come here to Belfast,

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which has become the centre of research into

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this cosmic visitor -

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an object called 'Oumuamua.

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When we first saw it, all we knew was that it was small

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and moving fast. The first object from deep space ever to be seen

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passing through our solar system.

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And its sudden appearance raised a whole host of questions.

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What did it look like? How had it formed?

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What was it made of? And where had it come from?

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To answer these questions,

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I'm going to piece together all the clues that scientists were able

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to extract from the small amount of data that they gathered as 'Oumuamua

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flashed through the solar system.

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This forensic analysis, including new, exclusive revelations,

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will give us the most comprehensive picture yet

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of this extraordinary object.

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Our story starts in Hawaii in mid-October last year,

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when one of the biggest telescopes in the world

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spotted something unusual.

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Now, this is the first picture taken

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of 'Oumuamua from the telescope in Hawaii.

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Looking at it, it's quite hard to spot

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but it's actually this splodge here.

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Now, you can tell it's moving really fast

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because the stars appear as points,

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whereas this is a blur across the screen.

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I called Karen Meech in Hawaii, who led the team that night,

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to find out how the discovery was made.

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Hi, Karen. Nice to meet you and thank you for waking up so early.

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-No problem.

-Now, can you take us

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through the night of the first observation?

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Well, this was discovered by the Pan-STARRS telescope in Hawaii,

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which is conducting a Nasa-funded search

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for near-Earth objects.

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And this particular night, on the 19th of October,

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one of the objects that was flagged

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had a very long streak, which meant it was moving quite fast.

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So, what had you effectively discovered by then?

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Well, at that point, people weren't sure.

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But as soon as some follow-up observations came in,

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one of the groups at the European Space Agency ground station reported

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that the orbit looked interesting.

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Namely, they said its shape didn't look circular.

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And it wasn't until a few more nights of data came in

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that we decided that this was definitively

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something from outside the solar system.

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How did you feel when you found out that it was an extrasolar object

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coming from another solar system?

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I actually sat there for a while just thinking about

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what it meant and getting more and more excited

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that this really is the first time we have

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something so close that's delivered from outside.

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The frustrating thing was that it was moving so fast.

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We only had a little over a week

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during which time it was bright enough to

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actually do the experiments we'd like to do.

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So, what that really meant was a team of people

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were working around the clock and I ended up sleeping in the office

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for most of the week, because we were putting in 18-hour workdays.

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How do you go about naming these objects?

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We thought it might be nice to have a Hawaiian name.

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And so the director suggested that we talk to

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a Hawaiian navigator and a Hawaiian linguistics expert

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on the Big Island. And they suggested a very nice name to us.

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It was 'Oumuamua, where the O means "to reach out for",

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and "mua" means "first" or "in advance of",

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and by duplicating that piece, it gives it emphasis in Hawaiian.

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So, the intent of their definition was that

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this is a scout or distant messenger

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sent out from our beginnings to reach out to us

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or build connections with us,

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so we thought it was a very appropriate name.

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Thank you so much, Karen.

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It's a fascinating story and I'm looking forward to finding out more.

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Well, thank you.

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Karen's discovery caught the imagination of scientists

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around the world.

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First indications were that 'Oumuamua

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was just a few hundred metres across

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and was travelling at over 50km per second.

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But the big story was about its origins.

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Within days, scientists had gathered enough data to start working out

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the trajectory of 'Oumuamua.

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Now, initially they assumed that it was an elliptical orbit.

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But just days later, they realised it wasn't an orbit at all.

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It was actually open.

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Now, this flagged up all sorts of questions,

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because it meant that 'Oumuamua didn't originate

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from within our solar system.

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More importantly,

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they'd only spotted it as it made its journey outward

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from the solar system. That meant they had a limited time

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to gather more data to find out what it was like, how it was made,

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and where it had come from.

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By late October, astronomers in Belfast

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and around the world were getting excited.

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Michele Bannister's team were among the first to take on the quest

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to understand 'Oumuamua.

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They focused on what it looked like,

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what shape it was, and - crucially - what colour.

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So, you did what astronomers have always done,

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which is ask simple questions like, "What colour is it?"

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That can often tell us a lot.

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Yeah. So, we're seeing this object

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entirely with reflected sunlight.

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And so the colour that you get

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of the reflected surface tells you about

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potentially what the composition is.

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And, so, what colour is it?

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It's a touch redder than sunlight, but kind of pinky.

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However, you wouldn't see that if you were to look at 'Oumuamua

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with your naked eye, rather than with one of the world's biggest

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telescopes, because when it reflects the sun's light,

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it's reflecting it back at almost the same colour as the sun.

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Just a bit redder in the infrared part of the spectrum.

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This colour, a hint of pink or red

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especially noticeable in the infrared,

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is reminiscent of some objects in our own solar system.

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It could actually be a little cousin of one of the objects that you see

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in the populations known as Jupiter Trojans,

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which orbit out near Jupiter.

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Another thing your observations showed was that the brightness of

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the object was changing over time.

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Yes, we observed for about two hours.

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So, if I show you here...

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So, this gives you some idea of how

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the brightness that we measured

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-changed over time.

-You've got this

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really quite dramatic dip here. It faces quite dramatically,

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-and then recovers.

-It changes in brightness

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over a remarkable amount of contrast

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and we weren't expecting that. That was great.

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What do we think causes that variation?

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Probably the shape of the object.

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So, I have a way of showing you what effect shape is going to have on

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-the brightness of an object over time.

-OK.

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So, here I have a sun...

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-OK.

-Here I have a turntable that is rotating an object over time.

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-OK.

-So, the camera is watching this object and it can't see the shape of

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the object directly. It's just going to see its brightness.

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On the screen here, you see what the camera is measuring of how it sees

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this little object changing in brightness over time as it rotates.

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Now, the sphere - you can see you don't get much change

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-in brightness at all.

-No.

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Let's try this with something a bit stranger in shape.

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OK, I'll remove the sphere. There we go.

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Instead, put on this delightful potato asteroid here.

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-Fine.

-And you can see what the camera is seeing

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as this point of light changes in brightness

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as it turns, is when the short end is pointing towards the camera...

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-Like it is now.

-..you have minimum surface area being reflected,

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the light, so it's dimmest. And when it turns round

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and the whole side of this object is being illuminated,

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it's the brightest to the camera,

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and so you see this brightness peak.

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And what do you find? What shape is 'Oumuamua?

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It's actually got to be even more elongated than this little potato.

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This is 3:1. 'Oumuamua has to be at least 5:1,

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maybe even a bit longer.

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But this is the thing, when I saw this result

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from all this hard work of astronomers

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scrambling to telescopes, it seems to me very unlikely

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that the first interstellar visitor would be this unusual.

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Is that something that disturbs you,

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or does this make sense if you've been thinking about these things?

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The shape is a bit unusual,

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but the colour is so much like what we see in our own solar system.

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There's a kinship there. It tells you that something that formed

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around a different star and something that formed

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around our own star have a lot of similarity in their surface.

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It's a very deep thought, that.

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It's sort of a poetic... It's scientific, but it's poetic as well,

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that there is this relationship

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to something that came from so far away.

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Yeah, we're finally getting to touch something that's from

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another solar system that's larger than a grain of dust.

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Within days of being spotted,

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detailed information about 'Oumuamua was coming in.

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From Michele's light analysis, a shape was proposed.

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It was thought to be an elongated cigar shape,

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100 to 400 metres in length.

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The ratio of length to width was thought to lie

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between 10:1 and 5:1.

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And although it was dark, it seemed to have a touch of pink or red.

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By the end of November,

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the strange shape and exotic nature of 'Oumuamua had led to some

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extraordinary speculations.

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Was 'Oumuamua an alien artefact?

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It wasn't an entirely stupid question.

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'Oumuamua was so strange

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that at this stage almost anything seemed possible.

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So I met astrophysicist and expert in the search for extraterrestrials

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Duncan Forgan, to find out how scientists deal with the question of

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whether an object is natural or alien.

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So, Duncan, all this very interesting data was coming through,

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what was the press's response to it?

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It was a little bit frenzied, to be honest.

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There were a lot of stories about this idea that maybe this

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weird interstellar visitor was, in fact,

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an alien spacecraft coming to visit the Earth.

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But, unfortunately, a lot of that stuff was very overbaked.

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So, how should scientists treat these stories?

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I think it's important to make sure that when you're thinking about,

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"What is this new, interesting, weird thing?"

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you make your list of natural explanations,

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-and then right at the very bottom you put the aliens explanation.

-OK.

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And you wait until you've exhausted all the natural explanations.

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And then, when nothing else is left, Sherlock Holmes-style,

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you come back to the aliens explanation.

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So, one of the things that we did was to basically check

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if 'Oumuamua was a transmitter.

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So, they wanted to see if it was emitting radio waves

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in the way that we'd expect a radio transmitter

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built by an intelligent being to work,

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so they pointed their radio telescopes at 'Oumuamua

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and checked and found nothing.

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So, what would you have done if it was found out that 'Oumuamua

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was an alien artefact?

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There are a list of protocols that people who are doing the search

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for intelligent life are supposed to follow -

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what they call a post-detection protocol, so what do you do next?

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And so one of the things you need to do is A - check your answer,

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-because if you get this wrong it could be very embarrassing.

-Yes.

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So, ask your colleagues to use a different instrument and try and do

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the same experiment and if it comes out to be the same answer

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then, OK, you've got something there. And then get more and more

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people to check and make sure that your hypothesis has been validated.

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And then you go to United Nations and tell the Secretary General,

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"By the way, there's alien life and it's coming towards us."

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-An interesting e-mail!

-Yeah.

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And then you're supposed to tell the public at large.

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-Well, thank you so much. It's been fascinating.

-Thank you.

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In mid-December, the mysteries about 'Oumuamua were still mounting,

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and scientists were beginning to wonder just where it had come from.

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Michele Bannister picks up the story.

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So, this brings me to the next question I wanted to ask, which is -

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do we know where this asteroid, this body, came from?

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It seems to me you've seen it coming in, so can we trace it back?

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That will be a work in progress.

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What we can do is say the arc that it took as it came into

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the solar system, if we extend that back and back and back

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for 100 million years...

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You know, that's the better part of halfway round the galaxy

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-as the sun's travelling.

-OK, so we've travelled a long way,

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-this thing's been moving, it's complicated.

-Yeah.

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You have to run the galaxy backwards in time and say,

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"Where were all the stars millions and millions of years ago?"

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And then say, "Was 'Oumuamua close to one of these stars?"

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And if it was, that's its last port of call.

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Now, that's not the same thing as saying that's where it's from.

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-No.

-Because the next star system that 'Oumuamua goes through,

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it'll look like it came from us.

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That's true. People will trace...

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Aliens will trace it back and think it came from here.

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But people have tried to match this trajectory,

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to do this difficult calculation - how have they got on?

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You can see it comes not close-close,

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but perhaps a little bit close to some stars.

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There's about 15 stars that are currently potential candidates that

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it could've come near in that time.

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But everything starts getting a little fuzzy, because we don't

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actually know the positions of these stars particularly well.

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About five of them are in a group of stars

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loosely called the Local Association.

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It's an amazing thought that it might be bouncing around

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and, of course, it may encounter other stars in the future.

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It has a long journey to go.

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-Michele, thank you very much.

-Thank you, Chris.

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So tracking 'Oumuamua's orbit back through time and space has suggested

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that it might come from a group of stars that astronomers call

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the Local Association.

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You might think that the Local Association would be a nice, neat

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little cluster of stars in the night sky, but it isn't that simple.

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Although they all formed around the same place

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and at around the same time,

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just 100 million years ago, they have since spread out.

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Pete Lawrence explores this Local Association,

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starting by looking towards the southern part of the sky.

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The Local Association

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is roughly in this direction here.

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Most of the stars in it are too dim to be seen

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with the naked eye, but it does include one of my favourite

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open clusters, the Pleiades.

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The Pleiades are some of our closest neighbours,

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at a distance of 440 light years.

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They're very distinctive, like a miniature Plough.

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To locate them, find Orion in the southern sky

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and follow the line of the belt up and to the right,

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past Taurus and its distinctive V,

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and then continue the line.

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You should see a little huddle

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of beautiful blue-white stars.

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These really are one of the highlights of the winter night sky,

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looking like rare jewels on black velvet.

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But binoculars or a telescope will show even more.

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And photography reveals an exquisite blue nebula,

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visible because of light reflecting off of a cloud of dust

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that the stars are moving through.

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Associations like this are often hundreds of light years across.

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For instance, there's another star in the association, which you can

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find by heading southeast from the Pleiades

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so that you're on the other side of Orion, the Hunter.

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So a fair distance away.

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Here you're in the constellation of Monoceros, the unicorn.

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And there's a faint star there

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which is a candidate for the origin of 'Oumuamua.

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The star is called Ross 614.

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You'll need a telescope to see it,

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but to find it go back to Orion and head south and east.

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Monoceros, or the unicorn,

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is a group of fairly dim stars

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between Canis Major and Canis Minor.

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And Ross 614 is about

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halfway along his front leg.

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And it's in this group...

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Oh, there it is!

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It's just 13 light years away and is a component

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in a red-dwarf binary system.

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And it's fascinating and really exciting to think that may be

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where 'Oumuamua came from.

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By now, scientists had worked out quite a bit about 'Oumuamua.

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They knew its rough size, speed and colour.

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And if it did come from the Local Association,

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they knew its age, too -

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100 million years,

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when these stars were formed.

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But two big mysteries remained.

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What was it made of and how was it formed?

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Back in Belfast, Chris met up with Alan Fitzsimmons,

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who started to investigate 'Oumuamua's composition.

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His team believed it was icy, like most small distant objects.

0:19:110:19:16

But all the images they collected told a different story.

0:19:160:19:20

Because, if it was icy, why didn't it have a tail?

0:19:200:19:24

And so you got those images back and you were expecting to see what?

0:19:270:19:30

A comet with a nice tail, I guess.

0:19:300:19:32

That's right. This object passed pretty close to the sun,

0:19:320:19:35

and so the ices there should have been heated

0:19:350:19:37

and we should have seen that material expanding

0:19:370:19:39

away to form the atmosphere of the comet and the tail,

0:19:390:19:42

but there was nothing like that.

0:19:420:19:43

It looked like an asteroid, and so we were thinking,

0:19:430:19:46

"What is this thing?"

0:19:460:19:48

What did you do next?

0:19:480:19:49

The important thing then was to figure out how this object was

0:19:490:19:52

reflecting light because that could give us to a clue

0:19:520:19:54

to what it was made of. To do that,

0:19:540:19:56

we needed to get spectroscopy of the object.

0:19:560:19:58

So, what did the spectrum show?

0:19:580:20:00

Well, we saw the signature of carbon.

0:20:000:20:02

-Carbon?

-Yeah.

0:20:020:20:04

Now, when we think of an icy comet,

0:20:040:20:06

we think of something that's mostly made of water ice,

0:20:060:20:09

although there may be some carbon monoxide and carbon dioxide.

0:20:090:20:13

This is an object that could have been out there between the stars for

0:20:130:20:16

millions or billions of years.

0:20:160:20:18

And so it's been sitting out there and during that time

0:20:180:20:22

it's been affected by the cosmic rays,

0:20:220:20:25

high-energy particles that fill our galaxy.

0:20:250:20:28

OK, so it's the cosmic rays that might have changed the surface.

0:20:280:20:32

-What would they have done to it?

-They take those ices on the surface,

0:20:320:20:35

and in particular they take the carbon,

0:20:350:20:37

and the carbon rearranges itself

0:20:370:20:40

to form new molecules and new compounds.

0:20:400:20:43

And so what does that look like? How can we see what's happening?

0:20:430:20:46

I can explain using this demo, now...

0:20:460:20:48

-OK.

-Basically a meringue - egg whites and sugar - OK?

0:20:480:20:53

And we can add some energy. Now, we're not going to use cosmic rays.

0:20:530:20:56

We're going to use a little blowtorch here.

0:20:560:20:59

-OK. Well, safety first.

-Safety first indeed.

0:20:590:21:02

I do this every time I cook, you know. Very sensible. OK.

0:21:020:21:05

-There we go.

-And now,

0:21:070:21:09

if we add energy to that we'll see a chemical transformation

0:21:090:21:12

to a different substance.

0:21:120:21:14

It's a very different material on the surface,

0:21:140:21:17

with the meringue intact inside.

0:21:170:21:19

Now... This is great cooking,

0:21:190:21:22

but what's this got to do with an interstellar asteroid

0:21:220:21:25

-or interstellar comet?

-Well, instead of egg whites, of course,

0:21:250:21:29

and sugar, we have ice, we believe, that we start off with.

0:21:290:21:32

And instead of a blowtorch,

0:21:320:21:34

we have energy deposited on the surface by cosmic rays.

0:21:340:21:37

But only on the surface?

0:21:370:21:39

That's right. Now, over about 100 million years,

0:21:390:21:42

this chemical transformation can go down about half a metre or so.

0:21:420:21:48

Within that depth, we could still have ice there.

0:21:480:21:52

And the important thing is this not only changes the surface properties

0:21:520:21:56

and how it reflects light, this new crust of carbon-based material

0:21:560:22:01

also insulates the interior.

0:22:010:22:04

So it locks in, perhaps, the ice that's still there.

0:22:040:22:07

That's right, and when we do the calculations we find that

0:22:070:22:11

even though 'Oumuamua passed within the orbit of Mercury,

0:22:110:22:14

passed very close to the sun,

0:22:140:22:17

that heat from the sun could not have penetrated

0:22:170:22:20

within more than half a metre.

0:22:200:22:22

So the ice would have remained locked up

0:22:220:22:24

and that explains why we didn't see a comet,

0:22:240:22:27

we saw something that looked initially like an asteroid.

0:22:270:22:31

We'll look forward to hearing about whatever comes next.

0:22:310:22:33

-Alan, thank you very much.

-Thank you.

0:22:330:22:36

By Christmas, scientists had a pretty good understanding

0:22:470:22:50

what 'Oumuamua was made of. But then came a new and exciting discovery -

0:22:500:22:55

revealed tonight for the very first time.

0:22:550:22:58

A powerful new theory started to emerge,

0:23:030:23:07

based on a detailed analysis of the light reflected off 'Oumuamua.

0:23:070:23:13

It suggested not just how it was formed, but also where it came from.

0:23:130:23:19

To find out more,

0:23:200:23:22

Chris met lead scientist on this new research Wes Fraser.

0:23:220:23:26

So, Wes, taking a close look at this thing,

0:23:280:23:30

it turns out to be even more complicated than we thought.

0:23:300:23:32

-What's going on?

-Well, I was weirded out by the fact

0:23:320:23:36

that no-one publishing all these papers coming out of 'Oumuamua

0:23:360:23:40

could actually determine how quickly it was rotating.

0:23:400:23:43

And so one morning, one Friday morning, I just thought,

0:23:430:23:46

"I'm just going to pull all of this together and see what I can see.

0:23:460:23:48

"Now that we've got many days' worth of observations,

0:23:480:23:51

"surely we can pull all of this data together and just figure out how quickly this thing is spinning."

0:23:510:23:55

Wes's new investigation compares the light we might expect

0:23:580:24:01

from a spinning object, shown with the dotted line,

0:24:010:24:04

with the data that Wes actually gathered.

0:24:040:24:07

So, if you look at the plot here,

0:24:080:24:10

it works in some places,

0:24:100:24:12

but it completely fails in others -

0:24:120:24:14

where the curve is low,

0:24:140:24:15

the data are high.

0:24:150:24:17

-Yeah, yeah. Look, down here in day five - it's way off.

-Yes, exactly.

0:24:170:24:19

Or even in the first couple of days, there's something odd going on.

0:24:190:24:22

It was exactly the comparison between night two and night five

0:24:220:24:25

that really... "OK, there's something weird going on here."

0:24:250:24:28

-OK.

-And so we started to look at it a little bit,

0:24:280:24:30

and it was very clear that, in fact, this thing is tumbling.

0:24:300:24:33

So, what do you mean by "tumbling"?

0:24:330:24:34

Tumbling is an unusual state of rotation.

0:24:340:24:37

We can demonstrate this with a simple ping-pong paddle.

0:24:370:24:40

So, when we throw it like this...

0:24:400:24:42

..just spins on a single axis and it remains that way.

0:24:470:24:50

But when we throw it like this...

0:24:500:24:52

..it immediately enters tumbling.

0:24:550:24:57

It spins like this at the start,

0:24:570:24:58

but then quickly starts to wobble around chaotically.

0:24:580:25:01

And that's what we call tumbling.

0:25:010:25:03

This thing's been travelling in space for a long time.

0:25:030:25:05

How does it end up tumbling like this?

0:25:050:25:07

We think it was due to a collision.

0:25:070:25:10

And so at some early stage of its life,

0:25:100:25:13

it was just spinning normally like everything else

0:25:130:25:16

and then it suffered a collision.

0:25:160:25:18

That would impart enough energy on one particular spot

0:25:200:25:23

in such a way as to then be confused in how it spins.

0:25:230:25:26

And so where would that have happened? Out in empty space?

0:25:260:25:29

No, so we can pretty safely assume that the collision that caused this

0:25:290:25:33

thing to tumble was in its original stellar system,

0:25:330:25:37

before it got kicked out.

0:25:370:25:40

So this thing's carrying information

0:25:400:25:42

-about the early days of a different solar system?

-In a way, yeah.

0:25:420:25:46

It's hard to know if it was during planet formation

0:25:460:25:50

or after the planet formation process.

0:25:500:25:52

Certainly more collisions happen while planets

0:25:520:25:54

are growing than afterwards, so that's a very good guess.

0:25:540:25:57

It now seems that Wes's result may tell us something profound.

0:26:020:26:06

'Oumuamua could be a relic from the formation of another solar system.

0:26:060:26:11

There is a chance that this tumbling occurred while planets were forming,

0:26:130:26:16

and so this is actually a moderately violent process.

0:26:160:26:20

So you can produce, you know, rocks and boulders and pebbles this way,

0:26:200:26:23

but eventually you do produce the planets in the process.

0:26:230:26:26

At that point, those collisions become violent and very destructive.

0:26:260:26:31

This may very well be where 'Oumuamua's shape has come from.

0:26:310:26:34

It's most likely where its tumbling has come from as well.

0:26:340:26:37

And we do know that objects are kicked out of our solar system,

0:26:370:26:40

as well - they have been and continue to do so.

0:26:400:26:43

So, while this is a bit of space that has, you know,

0:26:430:26:47

come its way to us, we are of course sending bits of ourselves naturally

0:26:470:26:50

to other places as well in a similar way.

0:26:500:26:53

You make it sound like the galaxy's full of these things.

0:26:530:26:55

Must be. Very, very much so.

0:26:550:26:58

-Yes.

-So, how come this is the first one we've seen?

0:26:580:27:01

How many more are there that we're missing?

0:27:010:27:03

Our best guess at the moment -

0:27:030:27:04

and this is pretty uncertain cos we've only ever seen one -

0:27:040:27:06

but our best guess is, at least within our own solar system,

0:27:060:27:10

there are about 10,000 of these currently passing

0:27:100:27:12

-within the orbit of Neptune.

-There are 10,000 of these...

0:27:120:27:16

-That's right.

-..going through the solar system today?

0:27:160:27:18

-Today.

-Not this year, not...

-Yep.

-So, why don't you see them?

0:27:180:27:21

For every one of those that we see, there's 10 or 100 that we miss.

0:27:210:27:25

And that just because of the fact that they're moving.

0:27:250:27:27

And so it was a fantastic job of the discoverers to find this thing.

0:27:270:27:31

-It's a fantastic discovery.

-Well, lots more to look forward to...

0:27:310:27:34

-Yes, indeed.

-..and it will be intriguing to find out

0:27:340:27:36

-whether this one is particularly unusual.

-That's right.

0:27:360:27:39

-Wes, thank you very much.

-Thank you.

0:27:390:27:40

The discovery of 'Oumuamua

0:27:460:27:48

has been one of the great scientific stories of the last 12 months.

0:27:480:27:52

This is our first deep-space object.

0:27:520:27:56

And this is now the most complete picture we have of 'Oumuamua.

0:27:560:28:00

It's now suggested that 'Oumuamua's origins

0:28:070:28:10

lay in the chaos of planetary formation...

0:28:100:28:13

..around a distant star...

0:28:170:28:19

..perhaps 100 million years ago.

0:28:210:28:24

That's it from Belfast for this month

0:28:270:28:29

and we're taking a break next month, but we'll be back in April.

0:28:290:28:32

In the meantime, don't forget to check out our website

0:28:320:28:35

for Pete's star guide and for our special weekly weather forecast.

0:28:350:28:39

And, of course, get outside and get looking up. Goodnight.

0:28:390:28:44

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