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Mike Brown: The search for our solar system's ninth planet
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Could the strange orbits of small, distant objects in our solar system lead us to a big discovery? Planetary astronomer Mike Brown proposes the existence of a new, giant planet lurking in the far reaches of our solar system -- and shows us how traces of its presence might already be staring us in the face.
Mike Brown - Planetary astronomer
Mike Brown scans the skies searching for and intensely studying distant bodies in our solar system in the hope of gaining insight into how our planet and the planets around it came to be. Full bio
Mike Brown scans the skies searching for and intensely studying distant bodies in our solar system in the hope of gaining insight into how our planet and the planets around it came to be. Full bio
Double-click the English transcript below to play the video.
00:13
I'm going to tell you a story
from 200 years ago.
from 200 years ago.
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In 1820, French astronomer Alexis Bouvard
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almost became the second person
in human history to discover a planet.
in human history to discover a planet.
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He'd been tracking the position
of Uranus across the night sky
of Uranus across the night sky
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using old star catalogs,
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and it didn't quite go around the Sun
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the way that his predictions
said it should.
said it should.
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Sometimes it was a little too fast,
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sometimes a little too slow.
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Bouvard knew that
his predictions were perfect.
his predictions were perfect.
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So it had to be that those
old star catalogs were bad.
old star catalogs were bad.
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He told astronomers of the day,
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"Do better measurements."
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So they did.
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Astronomers spent the next two decades
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meticulously tracking the position
of Uranus across the sky,
of Uranus across the sky,
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but it still didn't fit
Bouvard's predictions.
Bouvard's predictions.
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By 1840, it had become obvious.
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The problem was not
with those old star catalogs,
with those old star catalogs,
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the problem was with the predictions.
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And astronomers knew why.
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They realized that there must be
a distant, giant planet
a distant, giant planet
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just beyond the orbit of Uranus
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that was tugging along at that orbit,
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sometimes pulling it along a bit too fast,
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sometimes holding it back.
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Must have been frustrating back in 1840
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to see these gravitational effects
of this distant, giant planet
of this distant, giant planet
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but not yet know how to actually find it.
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Trust me, it's really frustrating.
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(Laughter)
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But in 1846, another French astronomer,
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Urbain Le Verrier,
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worked through the math
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and figured out how to predict
the location of the planet.
the location of the planet.
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He sent his prediction
to the Berlin observatory,
to the Berlin observatory,
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they opened up their telescope
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and in the very first night
they found this faint point of light
they found this faint point of light
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slowly moving across the sky
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and discovered Neptune.
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It was this close on the sky
to Le Verrier's predicted location.
to Le Verrier's predicted location.
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The story of prediction
and discrepancy and new theory
and discrepancy and new theory
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and triumphant discoveries is so classic
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and Le Verrier became so famous from it,
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that people tried to get in
on the act right away.
on the act right away.
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In the last 163 years,
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dozens of astronomers have used
some sort of alleged orbital discrepancy
some sort of alleged orbital discrepancy
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to predict the existence
of some new planet in the solar system.
of some new planet in the solar system.
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They have always been wrong.
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The most famous
of these erroneous predictions
of these erroneous predictions
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came from Percival Lowell,
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who was convinced that there must be
a planet just beyond Uranus and Neptune,
a planet just beyond Uranus and Neptune,
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messing with those orbits.
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And so when Pluto was discovered in 1930
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at the Lowell Observatory,
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everybody assumed that it must be
the planet that Lowell had predicted.
the planet that Lowell had predicted.
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They were wrong.
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It turns out, Uranus and Neptune
are exactly where they're supposed to be.
are exactly where they're supposed to be.
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It took 100 years,
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but Bouvard was eventually right.
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Astronomers needed to do
better measurements.
better measurements.
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And when they did,
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those better measurements
had turned out that
had turned out that
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there is no planet just beyond
the orbit of Uranus and Neptune
the orbit of Uranus and Neptune
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and Pluto is thousands of times too small
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to have any effect on those orbits at all.
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So even though Pluto
turned out not to be the planet
turned out not to be the planet
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it was originally thought to be,
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it was the first discovery
of what is now known to be
of what is now known to be
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thousands of tiny, icy objects
in orbit beyond the planets.
in orbit beyond the planets.
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Here you can see the orbits of Jupiter,
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Saturn, Uranus and Neptune,
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and in that little circle
in the very center is the Earth
in the very center is the Earth
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and the Sun and almost everything
that you know and love.
that you know and love.
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And those yellow circles at the edge
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are these icy bodies
out beyond the planets.
out beyond the planets.
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These icy bodies are pushed and pulled
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by the gravitational fields of the planets
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in entirely predictable ways.
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Everything goes around the Sun
exactly the way it is supposed to.
exactly the way it is supposed to.
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Almost.
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So in 2003,
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I discovered what was at the time
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the most distant known object
in the entire solar system.
in the entire solar system.
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It's hard not to look
at that lonely body out there
at that lonely body out there
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and say, oh yeah, sure,
so Lowell was wrong,
so Lowell was wrong,
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there was no planet just beyond Neptune,
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but this, this could be a new planet.
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The real question we had was,
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what kind of orbit
does it have around the Sun?
does it have around the Sun?
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Does it go in a circle around the Sun
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like a planet should?
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Or is it just a typical member
of this icy belt of bodies
of this icy belt of bodies
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that got a little bit tossed outward
and it's now on its way back in?
and it's now on its way back in?
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This is precisely the question
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the astronomers were trying
to answer about Uranus 200 years ago.
to answer about Uranus 200 years ago.
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They did it by using
overlooked observations of Uranus
overlooked observations of Uranus
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from 91 years before its discovery
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to figure out its entire orbit.
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We couldn't go quite that far back,
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but we did find observations
of our object from 13 years earlier
of our object from 13 years earlier
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that allowed us to figure out
how it went around the Sun.
how it went around the Sun.
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So the question is,
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is it in a circular orbit
around the Sun, like a planet,
around the Sun, like a planet,
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or is it on its way back in,
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like one of these typical icy bodies?
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And the answer is
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no.
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It has a massively elongated orbit
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that takes 10,000 years
to go around the Sun.
to go around the Sun.
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We named this object Sedna
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after the Inuit goddess of the sea,
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in honor of the cold, icy places
where it spends all of its time.
where it spends all of its time.
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We now know that Sedna,
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it's about a third the size of Pluto
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and it's a relatively typical member
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of those icy bodies out beyond Neptune.
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Relatively typical,
except for this bizarre orbit.
except for this bizarre orbit.
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You might look at this orbit and say,
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"Yeah, that's bizarre,
10,000 years to go around the Sun,"
10,000 years to go around the Sun,"
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but that's not really the bizarre part.
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The bizarre part is
that in those 10,000 years,
that in those 10,000 years,
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Sedna never comes close
to anything else in the solar system.
to anything else in the solar system.
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Even at its closest approach to the Sun,
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Sedna is further from Neptune
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than Neptune is from the Earth.
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If Sedna had had an orbit like this,
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that kisses the orbit of Neptune
once around the Sun,
once around the Sun,
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that would have actually been
really easy to explain.
really easy to explain.
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That would have just been an object
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that had been in
a circular orbit around the Sun
a circular orbit around the Sun
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in that region of icy bodies,
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had gotten a little bit
too close to Neptune one time,
too close to Neptune one time,
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and then got slingshot out
and is now on its way back in.
and is now on its way back in.
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But Sedna never comes close
to anything known in the solar system
to anything known in the solar system
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that could have given it that slingshot.
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Neptune can't be responsible,
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but something had to be responsible.
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This was the first time since 1845
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that we saw the gravitational effects
of something in the outer solar system
of something in the outer solar system
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and didn't know what it was.
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I actually thought I knew
what the answer was.
what the answer was.
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Sure, it could have been
some distant, giant planet
some distant, giant planet
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in the outer solar system,
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but by this time,
that idea was so ridiculous
that idea was so ridiculous
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and had been so thoroughly discredited
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that I didn't take it very seriously.
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But 4.5 billion years ago,
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when the Sun formed in a cocoon
of hundreds of other stars,
of hundreds of other stars,
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any one of those stars
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could have gotten
just a little bit too close to Sedna
just a little bit too close to Sedna
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and perturbed it onto the orbit
that it has today.
that it has today.
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When that cluster of stars
dissipated into the galaxy,
dissipated into the galaxy,
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the orbit of Sedna would have been
left as a fossil record
left as a fossil record
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of this earliest history of the Sun.
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I was so excited by this idea,
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by the idea that we could look
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at the fossil history
of the birth of the Sun,
of the birth of the Sun,
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that I spent the next decade
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looking for more objects
with orbits like Sedna.
with orbits like Sedna.
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In that ten-year period, I found zero.
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(Laughter)
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But my colleagues, Chad Trujillo
and Scott Sheppard, did a better job,
and Scott Sheppard, did a better job,
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and they have now found several objects
with orbits like Sedna,
with orbits like Sedna,
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which is super exciting.
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But what's even more interesting
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is that they found that all these objects
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are not only on these distant,
elongated orbits,
elongated orbits,
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they also share a common value
of this obscure orbital parameter
of this obscure orbital parameter
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that in celestial mechanics we call
argument of perihelion.
argument of perihelion.
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When they realized it was clustered
in argument of perihelion,
in argument of perihelion,
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they immediately jumped up and down,
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saying it must be caused
by a distant, giant planet out there,
by a distant, giant planet out there,
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which is really exciting,
except it makes no sense at all.
except it makes no sense at all.
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Let me try to explain it
to you why with an analogy.
to you why with an analogy.
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Imagine a person walking down a plaza
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and looking 45 degrees to his right side.
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There's a lot of reasons
that might happen,
that might happen,
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it's super easy to explain, no big deal.
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Imagine now many different people,
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all walking in different
directions across the plaza,
directions across the plaza,
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but all looking 45 degrees
to the direction that they're moving.
to the direction that they're moving.
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Everybody's moving
in different directions,
in different directions,
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everybody's looking
in different directions,
in different directions,
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but they're all looking 45 degrees
to the direction of motion.
to the direction of motion.
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What could cause something like that?
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I have no idea.
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It's very difficult to think of any reason
that that would happen.
that that would happen.
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(Laughter)
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And this is essentially
what that clustering
what that clustering
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in argument of perihelion was telling us.
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Scientists were generally baffled
and they assumed it must just be a fluke
and they assumed it must just be a fluke
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and some bad observations.
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They told the astronomers,
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"Do better measurements."
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I actually took a very careful look
at those measurements, though,
at those measurements, though,
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and they were right.
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These objects really did all share
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a common value of argument of perihelion,
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and they shouldn't.
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Something had to be causing that.
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The final piece of the puzzle
came into place in 2016,
came into place in 2016,
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when my colleague, Konstantin Batygin,
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who works three doors down from me, and I
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realized that the reason
that everybody was baffled
that everybody was baffled
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was because argument of perihelion
was only part of the story.
was only part of the story.
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If you look at these
objects the right way,
objects the right way,
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they are all actually lined up
in space in the same direction,
in space in the same direction,
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and they're all tilted in space
in the same direction.
in the same direction.
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It's as if all those people on the plaza
are all walking in the same direction
are all walking in the same direction
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and they're all looking
45 degrees to the right side.
45 degrees to the right side.
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That's easy to explain.
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They're all looking at something.
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These objects in the outer solar system
are all reacting to something.
are all reacting to something.
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But what?
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Konstantin and I spent a year
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trying to come up with any explanation
other than a distant, giant planet
other than a distant, giant planet
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in the outer solar system.
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We did not want to be the 33rd and 34th
people in history to propose this planet
people in history to propose this planet
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to yet again be told we were wrong.
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But after a year,
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there was really no choice.
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We could come up with no other explanation
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other than that there is a distant,
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massive planet on an elongated orbit,
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inclined to the rest of the solar system,
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that is forcing these patterns
for these objects
for these objects
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in the outer solar system.
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Guess what else a planet like this does.
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Remember that strange orbit of Sedna,
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how it was kind of pulled away
from the Sun in one direction?
from the Sun in one direction?
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A planet like this would make
orbits like that all day long.
orbits like that all day long.
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We knew we were onto something.
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So this brings us to today.
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We are basically 1845, Paris.
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(Laughter)
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We see the gravitational effects
of a distant, giant planet,
of a distant, giant planet,
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and we are trying to work out
the calculations
the calculations
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to tell us where to look,
to point our telescopes,
to point our telescopes,
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to find this planet.
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We've done massive suites
of computer simulations,
of computer simulations,
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massive months of analytic calculations
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and here's what I can tell you so far.
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First, this planet,
which we call Planet Nine,
which we call Planet Nine,
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because that's what it is,
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Planet Nine is six times
the mass of the Earth.
the mass of the Earth.
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This is no slightly-smaller-than-Pluto,
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let's-all-argue-about-
whether-it's-a-planet-or-not thing.
whether-it's-a-planet-or-not thing.
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This is the fifth largest planet
in our entire solar system.
in our entire solar system.
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For context, let me show you
the sizes of the planets.
the sizes of the planets.
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In the back there,
you can the massive Jupiter and Saturn.
you can the massive Jupiter and Saturn.
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Next to them, a little bit smaller,
Uranus and Neptune.
Uranus and Neptune.
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Up in the corner, the terrestrial planets,
Mercury, Venus, Earth and Mars.
Mercury, Venus, Earth and Mars.
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You can even see that belt
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of icy bodies beyond Neptune,
of which Pluto is a member,
of which Pluto is a member,
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good luck figuring out which one it is.
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And here is Planet Nine.
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Planet Nine is big.
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Planet Nine is so big,
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you should probably wonder
why haven't we found it yet.
why haven't we found it yet.
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Well, Planet Nine is big,
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but it's also really, really far away.
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It's something like
15 times further away than Neptune.
15 times further away than Neptune.
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And that makes it about 50,000 times
fainter than Neptune.
fainter than Neptune.
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And also, the sky is a really big place.
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We've narrowed down where we think it is
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to a relatively small area of the sky,
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but it would still take us years
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to systematically cover
the area of the sky
the area of the sky
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with the large telescopes that we need
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to see something that's
this far away and this faint.
this far away and this faint.
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Luckily, we might not have to.
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Just like Bouvard used
unrecognized observations of Uranus
unrecognized observations of Uranus
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from 91 years before its discovery,
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I bet that there are unrecognized images
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that show the location of Planet Nine.
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It's going to be a massive
computational undertaking
computational undertaking
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to go through all of the old data
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and pick out that one faint moving planet.
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But we're underway.
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And I think we're getting close.
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So I would say, get ready.
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We are not going to match Le Verrier's
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"make a prediction,
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have the planet found in a single night
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that close to where
you predicted it" record.
you predicted it" record.
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But I do bet that within
the next couple of years
the next couple of years
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some astronomer somewhere
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will find a faint point of light,
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slowly moving across the sky
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and triumphantly announce
the discovery of a new,
the discovery of a new,
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and quite possibly not the last,
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real planet of our solar system.
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Thank you.
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(Applause)
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ABOUT THE SPEAKER
Mike Brown - Planetary astronomerMike Brown scans the skies searching for and intensely studying distant bodies in our solar system in the hope of gaining insight into how our planet and the planets around it came to be.
Why you should listen
Mike Brown has discovered dozens of dwarf planets (and demoted one object from planet to dwarf planet) and is currently hot on the trail of Planet Nine -- a hypothesized body that is possibly the fifth largest planet of our solar system.
Brown is the Richard and Barbara Rosenberg Professor of Planetary Astronomy at the California Institute of Technology and has been on the faculty there since 1996. He has won many awards and honors for his scholarship, including the Urey Prize for best young planetary scientist from the American Astronomical Society's Division of Planetary Sciences; a Presidential Early Career Award; a Sloan Fellowship; the 2012 Kavli Prize in Astrophysics; and, of course, the one that started his career, an honorable mention in his fifth-grade science fair. He was inducted into the National Academy of Science in 2014. He was also named one of Wired Online's Top Ten Sexiest Geeks in 2006, the mention of which never ceases to make his wife laugh.
Brown received his AB from Princeton in 1987 and his MA and PhD from University of California, Berkeley, in 1990 and 1994, respectively. He is the author of How I Killed Pluto and Why It Had It Coming, a memoir of the discoveries leading to the demotion of Pluto.
Mike Brown | Speaker | TED.com