[Music playing - no lyrics]
  My name is Stephanie Bernard
  I'm a PhD student at the University of Melbourne,   here in Melbourne
  and I'm just going to talk to you today
  a little bit about what I do as a PhD student
  and I'm going to talk to you about our Solar System
  and how we can find planets around other stars
  apart from our own Sun.
  A little bit about me...
  as I said, I'm a PhD student   at the University of Melbourne.
  I grew up in Newcastle in New South Wales
  which is at the top right of the screen
  and when I was in primary school
  I was really interested in maths and science
  and especially in astronomy
  so I wanted to know what are all the stars... out in sky.
  We can see some planets in our sky
  but also more further afield
  are there other galaxies?
  What do they look like?
  What sort of stars do they have?
  Is there life out there?
  All these sorts of things.
  I was lucky enough when I was in primary school
  to go to Parkes, to the radio telescope there
  which isn't shown on this map
  it's a bit further north
  and there there's a really, really big radio telescope
  64 metres across...
  and that was when I really decided   I want to do astronomy,
  I think this is really, really cool.
  When I was in high school, I moved to Melbourne
  and then when I finished high school
  I went to university
  and I studied physics.
  Physics is... kind of how we look at   the Universe, as a whole.
  So we want to look at
  what are the fundamental properties of the Universe?
  What are all of the atoms that are in our bodies?
  All of the electrons that give us electricity
  how do they work, what's happening with them?
  As we go out into the Universe
  we want to know
  what are the laws that govern
  how everything in the Universe happens
  like gravity, electromagnetism, all these sort of things.
  So I thought physics was really cool at university
  and I kept studying, I did a Masters
  which is like a high level undergraduate degree
  and then I started doing a PhD
  which is where I do, basically just research,
  so my work is on galaxies
  and I'm looking at a very first galaxies   that formed in the Universe.
  If we look at galaxies at different distances from us
  what we're actually seeing is   galaxies that are further away.
  We have this speed of light
  which is really, really fast
  but Space is really, really big
  and we'll look into this a bit later with the Solar System.
  So it takes time for light to reach us
  so when we look at the very, very furthest things
  we're actually seeing them really, really far back in time
  and we can look at the first stars
  which formed around 100 million years ago.
  They're a little bit too far for us   to see with current telescopes
  We can see some of the very first galaxies
  only 500 million years after the Big Bang
  and you can see on the timeline here
  from the Big Bang, which is the beginning   of the Universe, to now
  it's been 13.7 billion years
  so we're really looking at baby galaxies   in that very early Universe.
  They're really, really small
  but they're really hot and interesting to look at.
  A bit closer to home
  let's talk about our Solar System.
  When we look at our Solar System
  we have a number of different...   what we call bodies, in it
  and this is a little picture   of what they all look like.
  We have the Sun in the centre
  and the Sun is our closest star.
  Then from closest into furthest out, we have Mercury
  Venus
  Earth
  Mars
  Jupiter
  Saturn
  Uranus
  Neptune
  and in the very edges of the Solar System,
  it's not a planet anymore,
  but we have Pluto.
  When we look at the Solar System
  we tend to classify the planets
  into two different types.
  We have the inner planet   which are Mercury, Venus, Earth and Mars
  and they're much smaller
  you can kind of see in this image   that they're really hard to see, actually.
  They're made of rocks,
  some of them have water like the Earth
  and then as we go further out
  the planets get to be a bit bigger
  and they're made up of what we call gases
  so they're not solid like the Earth is
  they don't have a proper surface.
  So they're much bigger,
  they tend to have a lot more moons,
  they also have rings.
  So we know that Saturn...
  this is a little one I brought from home...
  has a beautiful ring system.
  Actually, all of the outer planets have rings
  most of them are just too faint   for us to see with our eyes.
  If we go into a bit more detail
  and we look at our Sun.
  Our Sun is our local star
  it's a star like all the others in the sky
  it's just really, really close to us
  so we can see it really clearly
  and we get a lot of light and heat from it
  and actually, all the light and heat   that we get from the Sun
  is made in the core of it.
  We can't see the core
  it's really, really...
  it's in the centre of the Sun.
  What we see is its outer atmosphere
  and we know that the Sun is really, really big.
  It's around 100 times the diameter of the Earth
  where the diameter is basically   how far across it is.
  So if you had our Sun...
  and we have our Earth in the very corner...
  you might not be able to see it
  you can actually fit 100 Earths across the Sun.
  Actually the Sun is really, really big.
  If you fit them all inside
  you could fit a million Earths inside.
  This is our Earth...
  and our Sun is behind me
  so they're not to scale, as you can see
  I've just told you that this is   100 times smaller than this...
  and if we had a million of these   we could fit them all inside the Sun.
  Our Sun is made of gases like the outer planets
  but because the Sun is making its own energy,   on the inside
  it's really, really hot so the surface   of the Sun is around 5,000 degrees.
  That's hot enough to melt metals
  it's actually hot enough to vapourise some metals.
  Usually you see metals in forms like my phone
  where it's a solid
  and so imagine this is just a gas
  it's very, very hard to imagine
  but the Sun can do that.
  If we want to look at whether   we can have life on planets
  which is something that astronomers want to know about
  well... planets that are closer in to the Sun   they tend to be hotter
  because they're getting more of the light   that the Sun is emitting.
  If we look at our closest planet in to the Sun,   which is Mercury
  I have a visual here...
  On the screen is a video
  which was taken by a satellite   that's orbiting Mercury.
  You can see that it's got lots of crater
  which are... kind of pock marks on its surface
  where rocks and asteroids have hit Mercury
  over billions of years that it's been around.
  Mercury is the closest planet to the Sun
  and actually, it gets really, really hot   because it's so close.
  On the surface that's facing the Sun
  it's around 450 degrees Celcius
  it's really, really hot
  and on the side that's not getting any Sun
  it's actually really, really cold
  because Mercury is too small   to have an atmosphere.
  Earth has an atmosphere,   it's all the air we breathe
  the clouds that are in the sky
  all these sort of things
  and that help to regulate the temperature of the planet
  because the heat can travel from one side to the other
  but Mercury doesn't have this
  so it's both too hot on its side facing the Sun
  and it's too cold on the side away from the Sun.
  So we don't think it has life at all,
  it just wouldn't be able to survive there.
  If we go a little bit further out
  we might think that it's... further away from the Sun
  so it's not going to get as much light and heat
  so it's probably going to be cooler.
  Actually what we see   is that Venus is really, really hot
  it's even hotter than Mercury.
  The reason for this is because   it has a very, very thick atmosphere.
  If you look on the left
  we have a picture of Venus' surface
  and you can see again some craters
  you can also see some lines stretching through   which are canyons on its surface
  but actually what we usually see   is the clouds on its surface.
  Venus is covered in a very, very strong atmosphere
  it has lots and lots of clouds
  and they make these kind of...   patterns on its surface.
  The way that an atmosphere can keep heat in
  is called the Greenhouse Effect.
  It looks like this, so we have sunlight   coming in from the Sun...
  It comes out...like this...
  and then when it hits Venus
  the light can go through its clouds.
  Some of it will get reflected,   it will bounce straight off
  but some of it goes in past the clouds   and onto the surface.
  When it hits the surface,   the light can actually heat up the surface
  and then the surface will emit some of the light
  so it will send it back out into Space.
  Because of the clouds...
  the clouds will actually reflect this heat  back onto the planet
  rather than letting it all out into Space,   like it does on Mercury.
  So because the clouds are really, really thick
  it actually keeps   most of the heat that it takes in
  and so it gets really, really hot.
  So if you're cooking a pizza on Earth
  you'd put it on, say 180 degrees Celcius
  it would take you about... 20 minutes   to get a nice crispy pizza
  but if you were cooking it on Venus
  you wouldn't even have to put it into an oven
  you could just have it on the surface
  it would take about nine seconds to cook
  so it's really, really hot.
  If we go a little bit further out
  we get to our Earth,  which is our favourite.
  So we can see even in this picture   that Earth has an atmosphere,
  as I mentioned, it's got lots of clouds
  it's got lots of water as well.
  This is a little Earth ball.
  We have planets in green... sorry...   we have continents in green
  and we have lots and lots of water in blue.
  The Earth is really covered in liquid water
  that's because it's far away enough from the Sun
  that the water doesn't just boil off into Space
  and it's far enough...sorry... it's close enough in   that the water doesn't immediately freeze into ice.
  This is due to our atmosphere.
  Our atmosphere keeps the heat in
  it means that, firstly, the water   doesn't go out into Space
  but also, we don't have a very big difference
  between the temperature   during the day and during the night.
  It's only around 10 degrees,   if that.
  The problem is though,
  that if we put more and more,   what we call Greenhouse gases
  which increase the amount of heat that we keep in
  our Earth is going to keep warming   and this is a really bad thing
  because it will melt all the ice,   like in beautiful Antarctica, down the bottom.
  So this is something that scientists  are working on at the moment.
  How do we stop the Earth from warming up too much?
  Yeah.
  If we go out to the further parts of the Solar System
  we get Mars.
  Mars is our beautiful red neighbour.
  It's much smaller than Earth,  it's only around half the size of the Earth
  and because it's so small
  it only has a very, very thin atmosphere
  so it actually can't keep liquid water
  but we know that it has ice water
  so actually at its poles...
  we can see on this little... inflatable version
  we have some ice caps
  and it's possible that during the past,   when the Sun was hotter,
  this ice might have been liquid.
  So Mars might have had life on it   at some point in the past.
  As we go even further out
  we get into the gas giants.
  I've said that they don't have a solid surface   that we can stand on.
  What we actually see is that
  they're really just made up of big balls of gas.
  So they have clouds in their upper atmosphere
  and this is a video taken by the Voyager satellite   back in the 70s
  and this shows you just how much is happening   in the atmosphere of Jupiter.
  We have big cyclones
  and this, that you can see   in the bottom part of the screen,
  is actually the Great Red Spot
  and this is... two or three times the size of the Earth
  just a huge cyclone revolving around.
  The other outer planets are similar
  they're made up of gases
  but they have lots and lots of moons
  and what we think is that   most of the moons now in that atmosphere...
  and Jupiter has four very big ones
  they have a layer of ice on them
  because they're really, really far away from the Sun.
  But actually under this ice they might have   these... underground oceans
  and so it's possible in these oceans   that there might be life forming...bacterial...
  But we do see life in very, very extreme   conditions on Earth
  like in really, really hot places
  in the ocean, and also in really, really cold places
  we still see life forming
  so it's possible that, even though Jupiter the planet   can't actually have life,
  maybe its moons do.
  Yeah, this is a...
  we're sending satellites out to Jupiter
  to look at both the planet and its moons
  and we need to be really, really careful  when we send satellites out there
  that they actually don't hit the moons
  because we don't want bacteria   that might have escaped from Earth
  to get onto these moons,
  just in case there's something there   that we could kill off with our nasty bacteria.
  We have one more planet, well,   one more body out in the Solar System
  and this is called Pluto.
  You might have heard of Pluto as being a planet
  and up until 2006 it was
  but actually it's really, really small.
  If we put it next to the Earth
  you can see that it's much, much smaller that the Earth
  and actually it's only around the size of the moon.
  So the New Horizons probe reached Pluto last year
  and it took these beautiful pictures of its surface
  which we couldn't see before   because it's just so small
  that even with our biggest telescopes   like the Hubble Space Telescope
  it was really, really hard to see
  and we couldn't get any sort of idea   of what it was actually like
  but now we know that it's mostly made up of ice.
  It's got some dirt on it
  which you can see in the bottom part of the planet.
  We also know that in the outer Solar System
  there are lots and lots of bodies   that are the same size as Pluto or even bigger.
  So if we wanted to keep Pluto as a planet
  we would have to add in   all these other bodies as well...
  as well as some asteroids like Ceres
  which is in the asteroid belt between Mars and Jupiter
  and it would just get very, very complicated
  you would have to learn around the names of 20 planets
  which is quite a lot.
  OK, so we've looked at our Solar System
  and we know that in our Solar System
  Earth definitely has life   because we're here
  and then it's possible that Mars   in the past might have had life
  maybe some moons around Jupiter  or even Saturn have life.
  It's also possible there are planets around other stars
  and so... in the night sky
  if we look up   we can see thousands of stars.
  Actually with the naked eye you can see 10,000 stars
  but you have to be in a really, really dark place.
  This photo was taken at the Anglo-Australian Telescope  in New South Wales
  and this is our first...what we call   Dark Sky site in Australia.
  This means that there's very, very little   what we call light pollution
  from say street lights or houses that have lights on   and these sorts of things
  and you can see lots and lots of stars,   you can also see the Milky Way
  which is passing through the centre of the image
  and so this is really our galaxy, where we live.
  We're part of the Milky Way
  and it's made up of billions of stars.
  People started to think, well,   our Sun is like a star, like any other
  and there are billions of stars in the galaxy
  so surely at least some of them   have planets around them.
  But until the 1990s no one had ever seen some...  seen any, actually.
  In the 1990s the first one was discovered
  but it was really hard to see
  and I'll tell you why it's really hard to see.
  We can actually get an idea of how   we could look for other planets
  by using just our own Solar System.
  We have the Sun which is letting out its own light
  and we have Venus, which is much smaller
  and it doesn't let its own light out
  the only way that we see Venus   is actually the light from the Sun
  being reflected towards us.
  So if we were in the centre   and Venus went between us
  it would block off some of the light of the Sun
  which is actually what we see in this image.
  We have the surface of the Sun
  and we have this little kind of hole in the surface
  and that's actually Venus   getting between us and the Sun.
  This is called a transit and it happens   every couple of hundred years
  when the orbit of Venus is lined up with the Sun.
  This actually gives us the idea   to look for planets around other stars.
  We have to be very lucky though
  because...if... we're where my head is
  and the Sun is here   and the planet is going around this way...
  we're never going to see the planet
  because it's not actually blocking   any of the light from the Sun.
  Whereas if it's edge on...  like Venus is
  then, as it passes across,   it will block some of the light.
  The most ambitious experiment to do this   is called the Kepler Telescope
  which is in Space and so the Kepler Telescope
  looks at... patches of the sky,  for a very long time
  it looks at them for years and years
  and it looks for... thousands of stars at the same time.
  It looks for this signal, which is where   a star has a particular brightness
  and then as the planet goes across
  the brightness of the star changes
  and it changes a really small amount
  because, as we know, stars are very big
  whereas planets are very, very small.
  So it's only, maybe a percent or something, that the brightness changes
  but we can actually still see this   if we look for a long enough time...
  and Kepler has been really, really successful.
  It's found thousand and thousands of planets   around other stars
  just using this method.
  Most of the planets that it finds
  are what we call gas giants, like Jupiter or Saturn
  because these planets are bigger,  they block out more of the light of the star
  and we actually find them really, really close into the star
  even closer than Mercury is
  which isn't something that we thought would happen.
  We thought that planets the size of Jupiter and Saturn
  they would have to form out   further from the star
  than we see with these planets.
  So this is a really interesting discovery   that Kepler has made.
  But it's so sensitive that it can start to find
  planets as small as our Sun   passing infront of other stars.
  These are some examples...
  these names are kind of...  they don't really mean that much
  but you can kind of see   the sizes of them
  and then compare them to Earth   which is on the bottom left.
  You can see that actually some of them   are around the same size as Earth
  but what we want to know is...
  OK these planets are very small
  but we don't really know what their atmosphere is like
  just from this method where we look at   the brightness of the Sun.
  The next step in looking at what we call exoplanets   or planets around other stars
  is actually to get an idea of what   the atmosphere of these planets is
  and with the atmosphere we can look at things like
  do they contain water?
  Do they contain other chemicals   that we know are essential to life?
  We know that plants have particular chemicals   like chlorophyll
  which is used to transfer...carbon dioxide into energy.
  So if we manage to see a planet   that has some of these signs
  then maybe, maybe these planets   will have life around them.
  Just to finish up, really excitingly...
  just in the last couple of months...in August
  we actually found that Proxima Centauri
  which is the star that's closest to us
  it also has a planet.
  I say that Proxima Centauri is our closest neighbour
  but it's actually trillions and trillions of kilometres away.
  So it's not really easy to get there
  because if we were going... kind of at the speed of our cars
  it would take thousands and thousands of years  to get there.
  But actually there is a program   called Breakthough Starshot
  which is building these very, very small   robots and satellites
  and actually if you send out thousands   of these small robots...
  they're really, really small so you can make them   go really, really fast.
  You can make them go around   a third of the speed of light.
  Proxima Centauri is four light-years away
  so if we go a third of the speed of light
  it's going to take us around 12 to 20 years to get there.
  So that's actually really, really fast.
  We're going really, really far, across the Universe
  to get to this... star and   look at what the planet looks like.
  This is kind of our best chance at maybe even...
  being able to talk to other planets.
  We don't think that there's any life there
  because the star that it's around   is actually really, really small.
  It's smaller than our Sun and   it actually lets off very, very large flares.
  So if our Sun lets off flares   then it can disrupt our electricity
  it can let off harmful ultraviolet rays
  which will give us... diseases.
  So this star is actually probably   not very hospitable to life
  but it's really, really close
  and it's a good way for us to look at other planets   in our immediate area
  apart from the ones that are in our Solar System.
  That's it. Thanks!
  Shooting stars are actually very small...
  what we call meteoroids that are out in Space
  they're really just like grains of sand, most of them.
  When they hit the atmosphere
  they get heated up really, really fast
  and so they let off a lot light  which is what we see as the shooting star.
  So because these are so small
  they're literally just the size of grains of sand,   most of them,
  they completely burn up in the atmosphere
  and... all of the molecules and atoms   that would have made them
  become part of our atmosphere.
  Each individual one is not really... going to   affect our atmosphere too much
  but actually we pass through tonnes and tonnes   of these little grains of sand every day.
  Because our Earth is so big
  even these tonnes and tonnes of meteorites
  that we pass through,   they're really not affecting us too much.
  Yeah, they're very pretty
  but they're not going to harm us at all.
  [laughs]
  [Voice off screen]  Would they leave anything behind in the atmosphere
  when they burn up?
  [Stephanie]  Yeah, I think they would leave aside
  whatever they're made of,   so usually it's just iron and carbon
  and things that are already on the Earth to begin with.
  I think it's really interesting.
  I like to do research,   I get to look at pictures of galaxies most of the day
  which is really, really cool
  and I also get to look at some of the questions   that want to know.
  So where did galaxies   like our Milky Way come from
  because the galaxies that we see   in the very early Universe
  we think that they merge over time
  to become bigger and bigger
  and eventually they become galaxies like our own.
  Also it's really, really cool to be able to get your problem
  and figure out all the different pieces.
  Problem solving is really a big part of being a scientist
  and especially an astronomer.
  So if you like... doing maths
  and you get to sit down with the maths problem
  and... figure out all the pieces,   then that's really good
  but even... being more creative...thinking
  OK, if I know this, how does that relate   to this other thing that I've got?
  Being able to think creatively   is a really important part as well.
  Yeah, I get to use really big telescopes as well...
  [Voice off screen]  I understand you use computer programming
  quite a bit in your work as well.
  [Stephanie]  Yes, computer programming
  is a really big part of doing physics
  but also most science, it's really useful to know.
  Learning how computers work
  and how we can use them to make our lives easier
  is a really big part of it.
  If I wanted to take...
  I have several gigabytes of pictures of galaxies
  and I want to know,   how do I get the information
  from these gigabytes of pictures   as efficiently as possible?
  I don't want to look at   each single pixel of each image
  to work out what it's got in it.
  I want the computer to be able to look at it and say
  OK, this is what you've got
  this is what's interesting,   let's have a bit of a further look.
  Yeah, so it's made of... silicon,
  it's made of carbon
  it's made of iron
  it's made of lots of different metals.
  All these things... get mix together in the core
  and our core is like the core of the Sun
  it's very, very dense and very, very hot.
  As we go out in the Earth...
  we have this layer called the mantle
  which is where all the magma is
  and magma comes out of volcanoes,  it's lava.
  All this silicon and carbon and iron and other metals...
  it eventually... gets out onto the surface of the Earth
  and then it hardens and becomes rocks.
  Different types of volcanoes   produce different types of rocks
  and also when the... continents shift apart
  we get rocks forming there.
  All of these are made of slightly different things
  depending on... the time that they formed   in the Earth's history
  yeah, lots of different things
  but it's mostly these heavier kind of elements.
  [Voice off screen]  I've heard that we're actually made out of
  an old star, like an exploded star.
  [Stephanie] Yes, absolutely...  [voice] Is that true?
  [Stephanie]  Yes, in the beginning, at the Big Bang
  there was only hydrogen and helium
  and so these are the lightest elements
  and we know that, we ourselves are made of carbon
  and we're made of oxygen and... iron   and all those sort of things
  so to get from hydrogen we actually have to have stars
  because stars are the only things  in the Universe
  that are big enough and hot enough
  to actually take these very light hydrogen atoms
  and they fuse them together to helium.
  Helium can fuse into carbon.
  Carbon can fuse into oxygen
  and so we build up these heavier and heavier elements   inside stars, actually.
  Once the star dies,
  it will let out all of these new elements   out into the Universe
  and then these new elements   get formed into new stars
  and eventually into planets like our own.
  I said that our galaxy, The Milky Way,   contains billions of stars
  and we think that, actually, most stars   will have planets around them.
  Based on what Kepler has found around other stars
  we actually think that...
  most stars will have at least one planet   and probably more.
  We know that our own star   has eight planets around it.
  So in our galaxy there are probably   tens of billions of planets
  and then our galaxy   isn't the only one in the Universe.
  In the Universe, there are   billions and billions of galaxies
  and so each of them is made up of billions of stars
  so there are just a huge number   of planets in the Universe
  and any one of them...
  most of them are not hospitable for life
  even in our own Solar System
  we only know of one that definitely has life
  but... even if there's a very small chance
  out of billions and billions of planets
  and billions and billions of galaxies
  it's very likely that there'll be a few   that will have some life on them.
  When I was your age, as I mentioned,
  I went to the Parkes Radio Telescope
  and they were playing a video on quasars.
  Quasars are...
  you know what a black hole is?
  It's something that's so dense   that even light can't escape.
  We know that every galaxy, almost,   has a black hole in its centre.
  Our galaxy has a black hole in its centre
  and that's got the same mass in it   as billions of stars
  so it's really, really big.
  Ours isn't eating anything at the moment
  it's what we call passive
  it's just kind of quiet   and it doesn't do anything
  but some galaxies they're actually   eating up gas and stars and things around them
  and they let out lots and lots of light
  and so they had this video on how this happens
  and I thought it was so cool
  and I was like...   there's these things in the Universe
  that are just eating up whole stars and gas
  and they let out light and we can see them
  and so I think that was...
  why I decided I wanted to do astronomy.  [laughs]
  Yes, that's a good question.
  Back in the 1990s when I was a kid
  we did actually think that...
  it was a very plausible possibility   that the Big Bang would happen
  and the Universe expands
  and then if there's enough matter in the Universe
  then eventually it would actually start to collapse
  so gravity would take over   and it would come back in
  and cause this big crunch.
  Of course in this... the Earth and the Sun   would get crushed up as well
  and then it might become a new Big Bang
  so it might rebound and become a new Universe.
  Since then we've actually discovered   this thing called dark energy
  which is some sort of force in the Universe   that's... pulling everything apart.
  So the expansion of the Universe   is actually accelerating
  so rather than going like this....  where it accelerates at a time
  it actually starts off small and then it goes...
  much, much faster than we thought it was
  and in this case, actually, we don't think   that there's enough matter in the Universe
  in all the stars and galaxies   and this thing that's called dark matter
  which is most of actually   what the matter in the Universe is...
  that actually, there's not enough of this
  to make it pull back in and become a big crunch
  which is a shame because it's a nice idea  about how the Big Bang happened.
  At the moment we really don't know   why the Big Bang happened
  all that we know is that
  the evidence that we have strongly suggests   that we had this Big Bang, in the past,
  we just don't know why.
  The first telescopes were made in the 1600s.
  Galileo was one of the first people to use a telescope
  and he discovered moons around Jupiter
  Really, kind of, since even the ancient Greeks
  we've know that Space is quite large
  during that time actually people thought that
  the Sun and the other planets and the stars   orbited around the Earth
  rather than the other way around
  where the Earth orbits around the Sun.
  But even then...yeah... they knew that
  the distance from the Sun to the Earth was really large.
  They could work out how big the Earth was
  just using trigonometry
  which you guys will learn in maths in high school
  and just using shadows and how... you know...
  how long shadows were   at different times of the day
  at different times of the year.
  Yes, so even 2000 years ago we kinda knew
  some of the basic things about the Universe.
  Dark matter is... this thing  we don't really know what it's made of
  but we can see its effect on the Universe.
  We can see that... it's certainly affected by gravity
  it doesn't really interact with matter
  like the atoms in our bodies, or in stars or galaxies.
  But we know that when we look at galaxies
  there's too much matter in them
  so they're rotating faster than they should be...
  and we can see actually in galaxy clusters as well
  the properties that they have,   implies that they have
  lots and lots of dark matter in them.
  So we can't see it
  but we, kind of, can see   what it does to the Universe
  and we have some ideas what it might be
  it might actually be very small black holes.
  It might be... planets that we just can't see   because they're very, very faint.
  Or it might be... more interesting things like
  what we call subatomic particles
  like smaller than atoms...
  even the ones that make up our cells and everything
  and that's what... particle colliders
  in Europe and the US are trying to find actually.
  They send very, very high energy protons at each other
  and they look at, is there any kind of mass
  that they don't detect from this...
  because then they think that maybe
  they've actually created dark matter in their colliders.
  My favourite planet is Saturn
  because it's got these beautiful big rings
  and if you get to look at it through a telescope
  it actually looks like a picture.
  It looks like it's got this... yellow planet
  in the centre and it's surrounded   by these beautiful rings
  and actually, if you have a big enough telescope
  you can see there's this gap in the rings
  which is formed by some of the moons around it
  and it's just very pretty.
  [laughs]
  It's a bit of a mystery as well
  we don't really know   exactly how these rings formed.
  We thing that they actually   must still be forming... as we speak.
  Yeah, it's a very interesting planet, I think.
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