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The Sky At Night is back,
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00:00:04,640 --> 00:00:07,880
bringing you the latest
in all things astronomical.
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00:00:07,880 --> 00:00:10,800
There's been a lot going on
since our last episode,
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and one particular object
caught our eye.
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The biggest story to hit the news
since we've been off air
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was about an asteroid
called 2024 YR4.
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The City Killer,
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an asteroid that had the potential
of hitting Earth in 2032.
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The headlines were everywhere.
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BBC NEWS THEME
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Now, an asteroid spotted late last
year is now being carefully tracked.
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Scientists are trying to work out
whether there's a chance of it
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hitting the Earth.
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{\an8}Astronomers estimate that
the space rock is roughly
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{\an8}the size of a football field.
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Suddenly, the night sky
wasn't a place of comfort.
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With that asteroid out there
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and its potential to change life
as we know it,
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looking up at the night sky wasn't
a place of quiet contemplation,
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but a place to fear.
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So the level of damage
that an asteroid the same size
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as 2024 YR4 could cause,
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it really depends on where it hits.
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We're probably talking about
the destruction of a city,
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were it to hit the land.
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Something you really don't want
landing on top of you.
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Not enough to wipe out dinosaurs
or cause a global shift in climate,
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but big enough that
you want to avoid it, for sure.
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But what lies behind the headlines?
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And are we prepared
for an asteroid strike?
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Welcome to The Sky At Night.
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On a beautiful day like today,
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it's easy to forget
that beyond that gorgeous sky,
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there could be legitimate
threats heading our way.
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I'm not talking about aliens.
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Obviously, I'm talking
about asteroids.
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Now we actually get hit
by asteroids every single day.
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In fact,
in any given 24-hour period,
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we might get hit by roughly 73
Earthling cows' worth of material.
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So why aren't we fussed about this?
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Well, the scale of this material
is such
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that it's like a sprinkling of dust,
mostly just burning up in
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the atmosphere
and not even reaching the ground.
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Bigger things do hit us too.
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The asteroid that wiped out
the dinosaurs a while back
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was tens of kilometres across,
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and something that size
is expected to hit us
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roughly every
100 million years.
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But between these extremes,
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mass extinction event,
rather nice light show,
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you have your midsize asteroids.
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Now your midsize asteroid
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could cause a heat blast
capable of vaporising solid rock.
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We're talking wind speeds
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five times the
strongest hurricanes.
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We're talking a shock wave
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that could flatten buildings
for hundreds of miles.
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That would mean a city the size
of London and the surrounding areas,
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maybe even as far as Kent, gone.
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Now, at the start of this year,
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we thought there was just such
an asteroid coming our way
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when Asteroid 2024 YR4 was spotted.
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Now, at the time, it was still
over 30 million miles away,
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but it looked like it was on course
to collide with us in 2032.
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It has since been downgraded,
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and we're now pretty confident it's
actually going to be a near miss.
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However, what it did provide is
a practice run, like a fire drill,
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or even an asteroid drill,
if you will,
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so that when the real threat
does come along, we know what to do.
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When YR4 was discovered,
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it was no more than a dot moving
amongst the background stars.
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And even once it had been found,
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it was just one of a million
asteroids in our books.
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So what was special about this one?
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To explain, I've come to
a football pitch, obviously,
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where I'm meeting my old friend,
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planetary scientist,
Dr Meg Schwamb.
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- Hey!
- Hey!
we've talked about football a lot,
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so I thought you were
the perfect person
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to bring here
and talk about YR4.
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When we were watching the odds
of it hitting the Earth go up,
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I did think of it like watching
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a striker's shot
head towards the goal.
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Yeah, definitely, exactly
that playing out, right?
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I think as the world,
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{\an8}but also astronomers
sitting there watching, right,
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{\an8}waiting to see
as they got more data,
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{\an8}as you get closer to that goal,
right,
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{\an8}of whether it's going to go in
or in this case,
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we really want it to miss.
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Yes, that's the unusual bit.
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But let's go back to the beginning.
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2024 YR4's an asteroid.
But what are asteroids?
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Asteroids are the debris left over
after planet formation.
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Most are between Mars and Jupiter.
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Some get disturbed in their orbits
and get sent inward.
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That potentially can be an orbit
that will cross the Earth.
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On the 27th of December 2024,
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YR4 was first spotted
by a telescope in Chile,
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as nothing more than
a faint point of light.
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It soon gathered a lot of attention,
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as calculations showed it had around
a 1% chance of hitting Earth.
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So in January,
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other astronomers jumped on this
and started trying to observe it.
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Everybody was jumping on it.
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Amateur astronomers,
anyone with a telescope
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that had time was jumping on this
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because very few objects
have jumped above that 1%.
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And when it hits that level
for the size
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that we thought
this object might be,
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which is about 30m to 90m,
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that's when we start worrying,
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because that's where you could do
damage on a city scale.
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What happened to the odds
of YR4 hitting us?
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It went up and it went up a lot.
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It went from about 1.2% to 2.8
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or over 3% roughly.
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And so that might feel really scary,
right?
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So it IS interesting,
I think, the fact that we went from
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a low probability and then it rose
before dropping off.
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I think it's easy
to get the impression
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that somebody made an error,
but that's not what happened.
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No. It's really trying to
understand where right in space
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the Earth is compared to
where we think
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all the possible orbits
that this object could have.
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Well, I really think we can
explain this with football,
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but I decided neither you
nor I should kick a ball.
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Definitely not.
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I've got some students here.
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Gabe! Gabe! Come here.
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I feel like we're bringing
on a substitute.
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Someone much better skilled!
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So if we get Gabe to kick
the ball towards the goal.
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At first, we don't have much
information about where it's going,
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whether it's going in or not.
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Tracking the asteroid after it was
first spotted is like freezing
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the ball just after Gabe kicks it.
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It might go in the goal,
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but the goal makes up
just one small part of the area
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the ball could end up in.
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For YR4, the odds
of hitting Earth were 1%.
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No, we've got
an initial idea of position, right?
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Right when it's kicked,
we have an idea of the velocity,
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but it can go any direction.
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But a little bit later on
we've got more information
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- as the ball heads towards the goal.
- Right.
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Because if you could just stop
the ball for a second in midair,
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you now can see more
of where it's headed.
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You have extra information,
another data point, right?
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You have another position,
another possible velocity.
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This additional data
narrows the ellipse,
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removing much of the area
outside the goal.
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The goal now takes up
more of the remaining ellipse,
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and so the odds of a hit go up.
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Things are getting exciting.
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For YR4, it was over 3%.
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And that's what happened here.
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We ruled out parts of space
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where the Earth wasn't, and so
the probability of impact went up.
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And then if we let
the shot play out...
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..the third freeze frame shows
the ellipses reduce down again.
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We're now sure the ball
will miss the goal...
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Bad luck, Gabe!
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..and YR4 will miss the Earth.
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And it was observations from one
of the most advanced telescopes
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on Earth that told us that
this asteroid...would not score.
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And so we have the additional data
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from the Very Large Telescope
helped,
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because that helped with all
the other observations
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to give us enough
of the trajectory
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to show it's going to come close,
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but it's just going to eke away
and not hit the goal.
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But it's still close,
it's not like it missed by miles.
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No, and there's even
a small chance
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this object could still hit
the moon.
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That'd be pretty spectacular,
wouldn't it?
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Yes, but not threaten the Earth
in any way?
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- No.
- It would just be a good show.
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If we even see it, it might be
the far side of the moon
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and we see nothing.
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I promised I'd say, by the way,
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that Gabe missed that
on purpose for us.
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But I think the demo really works,
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- and it's good to know
that YR4, too, is missing.
- Yeah.
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But the threat is still there.
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There's many other objects
of the size
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that can do damage to cities
that we still don't know about.
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But the nice thing is
there are telescopes searching
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the skies nightly to try
to find these objects.
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- I enjoyed that.
- Good.
It's a bit like Ted Lasso.
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We brought in an American
to explain football to us!
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MEG LAUGHS
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While multiple observations
allowed us to confidently predict
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a miss for YR4,
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one day,
there WILL be a direct hit.
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So what can we do if we know
an asteroid strike is imminent?
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Maggie's taking
a tea break to explain.
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00:09:14,640 --> 00:09:17,760
Hollywood movies are
full of ideas
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of how we might handle
an asteroid strike.
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00:09:20,320 --> 00:09:22,160
But in the world of reality,
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what tools do we have
in our toolkit?
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Well, to understand this,
I'm going to use this
203
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as the asteroid
and this as planet Earth.
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Now the challenge is the asteroid
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is heading straight towards
the Earth.
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00:09:34,000 --> 00:09:35,920
So what can we do to deflect it?
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00:09:35,920 --> 00:09:38,480
Well, there's a number
of different techniques out there.
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00:09:38,480 --> 00:09:41,160
And the first one
is the nudge method.
209
00:09:41,160 --> 00:09:43,280
So... Oh, sorry, they're good.
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The first one is
where you want to use
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a projectile to hit the asteroid.
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When this happens, we'll transfer
some momentum to the asteroid.
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00:09:50,800 --> 00:09:52,560
And it will be deflected
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00:09:52,560 --> 00:09:54,600
and hopefully,
won't hit planet Earth.
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00:09:57,080 --> 00:09:59,120
And the great thing
about this method
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00:09:59,120 --> 00:10:01,720
is that it's already been tested.
217
00:10:01,720 --> 00:10:06,440
In 2022, the DART mission flew
into an asteroid, Dimorphos,
218
00:10:06,440 --> 00:10:10,080
changing its orbit significantly.
219
00:10:10,080 --> 00:10:12,080
But there are
a few problems with this.
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Firstly, how much of
a nudge do we need?
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00:10:14,640 --> 00:10:17,560
If we don't nudge far enough,
we'll still get an impact.
222
00:10:17,560 --> 00:10:20,280
And if we nudge too far,
for smaller asteroids,
223
00:10:20,280 --> 00:10:22,320
they might crumble and break up
into many pieces.
224
00:10:22,320 --> 00:10:23,360
Not good.
225
00:10:23,360 --> 00:10:27,240
The second technique I want
to talk about involves this.
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Yeah, it's a tractor,
but it's a gravity tractor.
227
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So this will actually be
a spaceship which will fly
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alongside the asteroid.
229
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Its gravitational force will pull
the asteroid towards it.
230
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This will again cause a deflection.
231
00:10:41,960 --> 00:10:44,960
The gravitational tractor technique
is quite desirable
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because we don't actually impact
the asteroid at all.
233
00:10:47,760 --> 00:10:49,680
It just sits alongside it
234
00:10:49,680 --> 00:10:51,760
and uses that gravitational force
to deflect it.
235
00:10:51,760 --> 00:10:53,240
But the problem is,
236
00:10:53,240 --> 00:10:55,640
we can't put anything
too massive in space.
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00:10:55,640 --> 00:10:57,520
And so as it's causing
the deflection,
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00:10:57,520 --> 00:10:59,560
it needs to do that
for quite some time
239
00:10:59,560 --> 00:11:02,640
to make sure that the asteroid
will miss planet Earth.
240
00:11:02,640 --> 00:11:06,600
Now our last technique is usually
what Hollywood go for.
241
00:11:06,600 --> 00:11:09,320
And it involves using
a nuclear bomb.
242
00:11:09,320 --> 00:11:12,040
Now, if the asteroid is quite close
to Earth and we don't
243
00:11:12,040 --> 00:11:15,880
have much time, using something
like DART to move the asteroid away
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00:11:15,880 --> 00:11:19,200
might not be enough.
And that's where the nuke comes in.
245
00:11:19,200 --> 00:11:22,560
We can embed the nuke into
the asteroid and then blow it up.
246
00:11:23,880 --> 00:11:26,160
We crush up the asteroid.
247
00:11:26,160 --> 00:11:27,800
SHE LAUGHS
248
00:11:27,800 --> 00:11:29,320
I'm making a bit of a mess!
249
00:11:29,320 --> 00:11:31,320
But we need to be careful
with this technique,
250
00:11:31,320 --> 00:11:33,640
because now, instead of just
one lump heading towards Earth,
251
00:11:33,640 --> 00:11:36,040
we have multiple lumps
heading towards Earth,
252
00:11:36,040 --> 00:11:38,400
which means they'll have
a greater impact area,
253
00:11:38,400 --> 00:11:40,360
potentially affecting
many more people.
254
00:11:40,360 --> 00:11:43,840
Now, to understand which
of these tools we can use
255
00:11:43,840 --> 00:11:46,560
for an asteroid strike, we need
to get a better understanding
256
00:11:46,560 --> 00:11:49,320
of the asteroid.
One I prepared earlier!
257
00:11:49,320 --> 00:11:52,400
And it's almost as if we need an eye
in the sky.
258
00:11:52,400 --> 00:11:55,240
Cue the James Webb Space Telescope.
259
00:11:59,480 --> 00:12:01,800
When ground-based telescopes
look up at space,
260
00:12:01,800 --> 00:12:04,200
they have
the atmosphere to contend with.
261
00:12:04,200 --> 00:12:07,680
This means that images get blurred
and measurements get distorted.
262
00:12:10,280 --> 00:12:12,280
But JWST gets around this.
263
00:12:12,280 --> 00:12:15,400
By sitting a million miles
above the atmosphere,
264
00:12:15,400 --> 00:12:18,160
its highly specialised mirrors
can capture even
265
00:12:18,160 --> 00:12:20,520
the faintest
amounts of infrared light,
266
00:12:20,520 --> 00:12:23,280
allowing for incredible accuracy.
267
00:12:24,640 --> 00:12:28,280
It's further helped by
an extreme cooling system.
268
00:12:28,280 --> 00:12:32,720
The spectrograph on board JWST
is cooled to just seven degrees
269
00:12:32,720 --> 00:12:36,160
above absolute zero.
All of this allows JWST
270
00:12:36,160 --> 00:12:39,880
to completely zone in on
an object with minimal interference,
271
00:12:39,880 --> 00:12:43,840
which means astronomers can measure
the sizes of incoming asteroids
272
00:12:43,840 --> 00:12:48,120
to a level of precision just not
feasible from the ground.
273
00:12:50,280 --> 00:12:54,320
And in March, observations
from JWST revealed why R4
274
00:12:54,320 --> 00:12:56,720
was about 60 metres across.
275
00:12:56,720 --> 00:13:00,400
A detail no ground-based telescope
was able to supply.
276
00:13:02,280 --> 00:13:04,800
This key information will be
invaluable
277
00:13:04,800 --> 00:13:08,080
for any future
asteroid strikes.
278
00:13:08,080 --> 00:13:12,080
So, we know something's coming
and we know what size.
279
00:13:12,080 --> 00:13:15,880
But another thing we might want
to know is, what's it made of?
280
00:13:15,880 --> 00:13:19,760
Three, two, one,
lift-off!
281
00:13:19,760 --> 00:13:23,440
Luckily, there is one mission
that can provide some answers.
282
00:13:23,440 --> 00:13:25,360
Atlas V takes flight.
283
00:13:25,360 --> 00:13:29,200
Sending Lucy to uncover
the fossils of our solar system.
284
00:13:29,200 --> 00:13:31,760
Launched in 2021,
285
00:13:31,760 --> 00:13:34,640
the Lucy mission is on
a journey to explore
286
00:13:34,640 --> 00:13:37,880
a record breaking number
of asteroids in our solar system.
287
00:13:39,280 --> 00:13:41,560
With 11 asteroids to explore,
288
00:13:41,560 --> 00:13:43,920
the Lucy mission is on course
to provide us with
289
00:13:43,920 --> 00:13:47,480
a whole new understanding of
the smorgasbord of asteroid types
290
00:13:47,480 --> 00:13:50,000
that could be headed our way.
291
00:13:52,120 --> 00:13:54,560
I'm meeting Dr Carly Howett,
292
00:13:54,560 --> 00:13:57,800
who has worked on the mission
from the very beginning.
293
00:13:57,800 --> 00:14:00,240
- Let's talk about Lucy!
- Let's.
294
00:14:00,240 --> 00:14:03,520
Now, obviously when we think about
asteroids, we think asteroid belt.
295
00:14:03,520 --> 00:14:06,200
But that's not where Lucy's going
to end up going?
296
00:14:06,200 --> 00:14:08,520
That's right.
The asteroid belt's very cool.
297
00:14:08,520 --> 00:14:11,360
Lots of good science there.
But we're going to a different set
298
00:14:11,360 --> 00:14:14,360
of asteroids. So these are known
as Jupiter's trojan asteroids,
299
00:14:14,360 --> 00:14:16,080
but they're not orbiting Jupiter.
300
00:14:16,080 --> 00:14:18,080
They're sort of
orbiting with Jupiter.
301
00:14:18,080 --> 00:14:19,640
So why these ones in particular?
302
00:14:19,640 --> 00:14:22,440
What's special about them
versus the asteroid belt?
303
00:14:22,440 --> 00:14:25,480
Well, this region of space
that they exist in are known as
304
00:14:25,480 --> 00:14:27,960
Lagrangian points. And they're
really stable regions of space.
305
00:14:27,960 --> 00:14:30,560
If you get caught there,
the gravity of the situation
306
00:14:30,560 --> 00:14:33,520
all sort of cancels out, basically,
there's not a way, an easy way out.
307
00:14:33,520 --> 00:14:36,040
And so we think
when the solar system was formed
308
00:14:36,040 --> 00:14:38,800
and debris was flying everywhere,
anything that got caught
309
00:14:38,800 --> 00:14:41,400
in these regions
of space got stuck there.
310
00:14:41,400 --> 00:14:44,040
And so they're sort of giving us
a little glimpse back
311
00:14:44,040 --> 00:14:47,240
in what life could have been like
in the very early solar system.
312
00:14:48,880 --> 00:14:51,440
By observing more
and more asteroids,
313
00:14:51,440 --> 00:14:54,880
we can build our understanding
of what could be heading our way.
314
00:14:54,880 --> 00:14:57,920
So what do we know already
about these objects?
315
00:14:57,920 --> 00:15:00,440
- Are we able to categorise them
at all?
- A little bit, yeah.
316
00:15:00,440 --> 00:15:02,360
So we can see things from the Earth.
317
00:15:02,360 --> 00:15:04,960
We've got telescopes that point at
the sky, and largely they fall into
318
00:15:04,960 --> 00:15:07,920
a certain number of categories. So
there are things like iron asteroids
319
00:15:07,920 --> 00:15:11,560
that we think were probably
the beginnings of a planet,
320
00:15:11,560 --> 00:15:15,480
but the outside got lost, and so
we're left with this iron core,
321
00:15:15,480 --> 00:15:18,560
a bit like what would happen on
the Earth if it lost everything
322
00:15:18,560 --> 00:15:22,400
above its core. You then have sort
of stony, pebbly asteroids that,
323
00:15:22,400 --> 00:15:25,280
erm, that might be held together
quite loosely.
324
00:15:25,280 --> 00:15:28,400
And then, what we're looking at
with the Lucy mission,
325
00:15:28,400 --> 00:15:31,480
which are primitive asteroids.
So asteroids that have stayed
326
00:15:31,480 --> 00:15:34,640
a long way from the Sun,
they haven't had that thermal change
327
00:15:34,640 --> 00:15:38,720
that the Sun might produce, and we
don't really know what's going on
328
00:15:38,720 --> 00:15:40,880
in their interior. And that's
something we're going to go
329
00:15:40,880 --> 00:15:43,040
and try and find out.
So when we understand more about
330
00:15:43,040 --> 00:15:45,800
each of those classes, we'll have
a better idea of, in the future,
331
00:15:45,800 --> 00:15:48,560
if something is perhaps going
to be a bit of a threat,
332
00:15:48,560 --> 00:15:49,920
how to categorise it.
333
00:15:49,920 --> 00:15:52,160
So how is Lucy going
to be telling us more about
334
00:15:52,160 --> 00:15:54,440
what these asteroids are made of,
then?
335
00:15:54,440 --> 00:15:57,320
So it's a difficult thing to see
inside an asteroid,
336
00:15:57,320 --> 00:15:58,880
especially if you're doing a flyby.
337
00:15:58,880 --> 00:16:01,280
But we can tell a lot just
by looking at the surface.
338
00:16:01,280 --> 00:16:03,680
So we have some cameras,
we have black and white cameras
339
00:16:03,680 --> 00:16:06,040
and colour cameras,
but we also have ways
340
00:16:06,040 --> 00:16:08,160
of understanding
what the composition is.
341
00:16:08,160 --> 00:16:10,440
So we have an infrared
spectrometer which measures
342
00:16:10,440 --> 00:16:12,200
those compositional fingerprints.
343
00:16:12,200 --> 00:16:15,280
And we can understand what
the surface is made from, from that.
344
00:16:15,280 --> 00:16:17,600
And then we have
a thermal camera on there as well.
345
00:16:17,600 --> 00:16:20,600
And so by putting all of these
pieces of information together,
346
00:16:20,600 --> 00:16:22,800
along with the brightness
and the shape, and all
347
00:16:22,800 --> 00:16:24,880
that sort of good stuff,
we're going to be able to get
348
00:16:24,880 --> 00:16:27,160
a really good idea of
what's going on in these asteroids
349
00:16:27,160 --> 00:16:29,400
in a way that we haven't been able
to until now.
350
00:16:29,400 --> 00:16:31,960
How does this help us
in the context of maybe
351
00:16:31,960 --> 00:16:36,360
- a future YR4-type threat?
- So the more we know about asteroids,
352
00:16:36,360 --> 00:16:39,080
the better. So if we understand
what they're made from,
353
00:16:39,080 --> 00:16:41,160
if we understand
what they typically look like,
354
00:16:41,160 --> 00:16:44,240
all of those things can help us
develop our models of how these
355
00:16:44,240 --> 00:16:47,400
asteroids evolve in their orbits
over a matter of time.
356
00:16:47,400 --> 00:16:50,000
So when something starts threatening
the Earth,
357
00:16:50,000 --> 00:16:52,440
it comes close to the Earth,
the details matter.
358
00:16:52,440 --> 00:16:54,000
If we can know what they look like,
359
00:16:54,000 --> 00:16:56,640
if we know
what their interiors are like,
360
00:16:56,640 --> 00:16:59,240
we can start modelling
those very fine effects
361
00:16:59,240 --> 00:17:01,040
in a lot better detail.
362
00:17:01,040 --> 00:17:03,280
When we get all this
information about these asteroids,
363
00:17:03,280 --> 00:17:06,840
how does it help us reduce
the unknown unknowns?
364
00:17:06,840 --> 00:17:08,920
That's the $64 million question,
right?
365
00:17:08,920 --> 00:17:10,880
One of
the things that's really important,
366
00:17:10,880 --> 00:17:13,200
if you want to deflect an asteroid,
is to think about how well
367
00:17:13,200 --> 00:17:15,120
the grains are
in touch with each other.
368
00:17:15,120 --> 00:17:17,560
You can imagine if you have
something that's basically
369
00:17:17,560 --> 00:17:20,120
like little polystyrene balls
that are just touching,
370
00:17:20,120 --> 00:17:22,840
held together with gravity
or maybe static,
371
00:17:22,840 --> 00:17:25,720
and you could just shove your way
through them, right? But if you have
372
00:17:25,720 --> 00:17:28,040
something that's clumped together,
if it's really sort of
373
00:17:28,040 --> 00:17:31,960
like an iron core, that's going
to be a lot easier to move as one,
374
00:17:31,960 --> 00:17:34,240
right? If you shove it, the whole
thing's going to move
375
00:17:34,240 --> 00:17:37,520
rather than collapse. And so when we
start to think about how to deflect
376
00:17:37,520 --> 00:17:39,560
or how to interact with asteroids
377
00:17:39,560 --> 00:17:41,680
that are potentially
a threat to Earth,
378
00:17:41,680 --> 00:17:44,160
understanding what they're made
of and how they're held together
379
00:17:44,160 --> 00:17:46,000
is going to be really,
really important.
380
00:17:49,120 --> 00:17:51,640
The Lucy spacecraft is currently
passing through
381
00:17:51,640 --> 00:17:54,520
the asteroid belt towards Jupiter,
and taking in some sights
382
00:17:54,520 --> 00:17:56,400
along the way.
383
00:17:57,960 --> 00:18:01,000
In 2023,
it passed asteroid Dinkinesh,
384
00:18:01,000 --> 00:18:03,960
discovering it also had two moons.
385
00:18:05,120 --> 00:18:06,640
Not unknown for an asteroid,
386
00:18:06,640 --> 00:18:08,920
but new objects
that further our knowledge.
387
00:18:10,760 --> 00:18:13,720
So what is the next big thing
for Lucy, then?
388
00:18:13,720 --> 00:18:16,160
Well, on Easter Sunday,
so easy to remember,
389
00:18:16,160 --> 00:18:18,920
we're going to be flying past
our next main-belt asteroid.
390
00:18:18,920 --> 00:18:20,680
So this one is Donaldjohanson.
391
00:18:20,680 --> 00:18:24,120
It's larger than Dinkinesh
that we flew by before.
392
00:18:24,120 --> 00:18:25,840
Why is Donaldjohanson exciting,
then?
393
00:18:25,840 --> 00:18:27,880
Well, any time you see something new
in the solar system,
394
00:18:27,880 --> 00:18:30,640
you learn lots of things
that you didn't even know to ask.
395
00:18:30,640 --> 00:18:32,840
So there's just pure exploration,
396
00:18:32,840 --> 00:18:35,680
but we see that the way it reflects
the light's really interesting.
397
00:18:35,680 --> 00:18:37,680
So we think it's either
a really interesting shape
398
00:18:37,680 --> 00:18:39,720
or perhaps it has a moon,
we'll find out.
399
00:18:39,720 --> 00:18:41,680
Very exciting, then!
400
00:18:44,800 --> 00:18:46,120
It's reassuring to know
401
00:18:46,120 --> 00:18:49,200
that our understanding of
these potential threats is growing,
402
00:18:49,200 --> 00:18:52,520
but if an asteroid was
on course to strike,
403
00:18:52,520 --> 00:18:54,960
who will do something about it?
404
00:18:54,960 --> 00:18:57,760
Or who are we going to call?
405
00:18:57,760 --> 00:19:00,320
Maggie's in Southampton to find out.
406
00:19:01,520 --> 00:19:04,240
It turns out that
astronomy is pretty good
407
00:19:04,240 --> 00:19:06,920
at working out
the odds of an asteroid strike,
408
00:19:06,920 --> 00:19:08,960
but that might be the easy bit.
409
00:19:08,960 --> 00:19:11,600
After that comes
a complex discussion
410
00:19:11,600 --> 00:19:15,240
involving philosophy, ethics
and geopolitics.
411
00:19:20,120 --> 00:19:22,240
I'm meeting Professor Hugh Lewis,
412
00:19:22,240 --> 00:19:26,080
who represents the UK on a global
approach to asteroid threats.
413
00:19:26,080 --> 00:19:27,320
Nice to meet you.
414
00:19:27,320 --> 00:19:29,520
We're sitting here
sort of surrounded by these flags.
415
00:19:29,520 --> 00:19:32,280
I guess this is a global threat,
416
00:19:32,280 --> 00:19:35,480
and so you are part of a network,
a global network,
417
00:19:35,480 --> 00:19:37,680
that is considering this
and looking at this
418
00:19:37,680 --> 00:19:40,680
and trying to assess
these challenges.
419
00:19:40,680 --> 00:19:42,640
Yeah, so after the incident
420
00:19:42,640 --> 00:19:45,320
involving the asteroid over Russia,
Chelyabinsk...
421
00:19:45,320 --> 00:19:47,440
- Yes.
- ..more than a decade ago now,
422
00:19:47,440 --> 00:19:49,920
that really prompted the United
Nations to take some action.
423
00:19:52,120 --> 00:19:55,240
The UN were reacting
to an 18-metre asteroid
424
00:19:55,240 --> 00:19:58,400
that flashed across Chelyabinsk
in 2013.
425
00:20:00,520 --> 00:20:04,200
It released the equivalent energy
of 20 atomic bombs
426
00:20:04,200 --> 00:20:08,160
and created a shock wave
that injured 1,500 people.
427
00:20:09,760 --> 00:20:13,400
It was a stark reminder of
the threat that asteroids can pose.
428
00:20:14,440 --> 00:20:18,240
The United Nations recommended
the creation of two groups.
429
00:20:18,240 --> 00:20:20,640
One was the International
Asteroid Warning Network,
430
00:20:20,640 --> 00:20:23,800
and that's the group of
scientists and facilities
431
00:20:23,800 --> 00:20:26,320
that would observe the solar system
432
00:20:26,320 --> 00:20:29,920
and identify
the potentially hazardous objects
433
00:20:29,920 --> 00:20:31,360
and then issue warnings.
434
00:20:31,360 --> 00:20:32,840
And then the second group
435
00:20:32,840 --> 00:20:35,760
is the Space Mission
Planning Advisory Group,
436
00:20:35,760 --> 00:20:38,880
commonly referred to as SMPAG,
erm...
437
00:20:38,880 --> 00:20:41,920
and that's the group
that I was a member of.
438
00:20:41,920 --> 00:20:44,920
- I see, yes.
- And this was the group
of engineers, scientists and experts
439
00:20:44,920 --> 00:20:49,440
who would consider
how we would go about deflecting
440
00:20:49,440 --> 00:20:52,480
or mitigating the threat from
an asteroid using a space mission.
441
00:20:52,480 --> 00:20:56,160
I think one of the challenges is
that often many countries
442
00:20:56,160 --> 00:20:59,320
are exposed to a risk
for an asteroid impact.
443
00:20:59,320 --> 00:21:01,280
- Yes.
- And the problem is
is that those countries
444
00:21:01,280 --> 00:21:04,480
don't necessarily have
the capability to take action.
445
00:21:04,480 --> 00:21:07,720
- Yes.
- So they have to rely
upon other countries who do,
446
00:21:07,720 --> 00:21:10,880
and that means that we need to have
that international response
447
00:21:10,880 --> 00:21:13,280
- and community that works together.
- Yes.
448
00:21:13,280 --> 00:21:15,680
An asteroid is heading
towards a country
449
00:21:15,680 --> 00:21:17,400
that doesn't have
a space capability,
450
00:21:17,400 --> 00:21:19,720
so it's reliant on those that do,
451
00:21:19,720 --> 00:21:22,720
and any space capability
will be quite expensive.
452
00:21:22,720 --> 00:21:25,960
- So weighing those two up
seems a challenge.
- Yeah.
453
00:21:25,960 --> 00:21:29,440
It is, and I think
that's one of the key aspects
454
00:21:29,440 --> 00:21:32,640
of the involvement through
the United Nations
455
00:21:32,640 --> 00:21:34,320
and the international community
456
00:21:34,320 --> 00:21:38,480
to understand that particular issue
and to try and address it.
457
00:21:38,480 --> 00:21:40,720
Right. Gosh, it's a quagmire.
458
00:21:40,720 --> 00:21:43,160
Are there conferences on
things like this?
459
00:21:43,160 --> 00:21:46,200
Yeah, so every two years,
scientists and engineers
460
00:21:46,200 --> 00:21:49,800
get together for the
Planetary Defence Conference.
461
00:21:49,800 --> 00:21:54,560
That sounds like...the Planetary
Defence League, superheroes!
462
00:21:54,560 --> 00:21:57,200
Yeah, I guess you can see it
in that way.
463
00:21:57,200 --> 00:21:59,000
These are people who are trying to
464
00:21:59,000 --> 00:22:01,120
understand the threat
from asteroids
465
00:22:01,120 --> 00:22:02,760
and what to do about it.
466
00:22:02,760 --> 00:22:05,920
So, at these conferences,
what sort of things do they do?
467
00:22:05,920 --> 00:22:08,920
This particular conference
is really quite unusual,
468
00:22:08,920 --> 00:22:12,600
because they run
a kind of a simulated exercise,
469
00:22:12,600 --> 00:22:15,480
where they create an asteroid,
470
00:22:15,480 --> 00:22:18,240
an asteroid that has
a potential impact with Earth,
471
00:22:18,240 --> 00:22:23,680
and they ask the participants at the
conference to play particular roles.
472
00:22:23,680 --> 00:22:26,960
It could be journalist,
it could be scientist, erm...
473
00:22:26,960 --> 00:22:30,520
it could be, erm...
you know, part of the government.
474
00:22:30,520 --> 00:22:34,360
And then they present you with
the information about the asteroid
475
00:22:34,360 --> 00:22:37,560
in kind of pieces, they give you a
little bit of information at a time,
476
00:22:37,560 --> 00:22:39,280
and you have to make decisions.
477
00:22:39,280 --> 00:22:43,040
Yes, so drip-feed the information,
as it would be in a real situation.
478
00:22:43,040 --> 00:22:44,600
- Exactly right.
- Right.
479
00:22:44,600 --> 00:22:47,520
And then in some cases,
the asteroid ultimately misses,
480
00:22:47,520 --> 00:22:51,120
yet you still have to run through
the scenarios
481
00:22:51,120 --> 00:22:53,000
and make sensible decisions.
482
00:22:53,000 --> 00:22:56,160
And in some cases,
the asteroid does hit.
483
00:22:56,160 --> 00:22:58,520
And I think it really does
showcase the fact
484
00:22:58,520 --> 00:23:01,600
that whenever we're dealing
with this particular threat,
485
00:23:01,600 --> 00:23:03,200
it's never certain.
486
00:23:03,200 --> 00:23:06,240
There's always a chance
that it misses us.
487
00:23:06,240 --> 00:23:09,320
But if we don't know that
for absolute certain,
488
00:23:09,320 --> 00:23:11,760
an absolute certainty is
a hard thing to get.
489
00:23:11,760 --> 00:23:13,440
And it's that kind of scenario that
they use
490
00:23:13,440 --> 00:23:14,960
at the Planetary Defence Conference.
491
00:23:14,960 --> 00:23:16,880
It's never, "It's a huge asteroid,
492
00:23:16,880 --> 00:23:19,960
- "it's definitely going to hit,
what do we do?"
- Yes!
493
00:23:19,960 --> 00:23:22,320
You have to kind of really consider
what the...
494
00:23:22,320 --> 00:23:24,240
..not just what the numbers
are telling you,
495
00:23:24,240 --> 00:23:28,120
but what the moral imperative is
in terms of protecting the planet.
496
00:23:28,120 --> 00:23:31,920
That's why it's called
"planetary defence", not UK defence.
497
00:23:31,920 --> 00:23:34,200
Yes! And so the fact
that we are working together,
498
00:23:34,200 --> 00:23:35,960
I find quite comforting.
499
00:23:37,040 --> 00:23:40,080
While space can seem like
a violent, scary place...
500
00:23:42,680 --> 00:23:45,400
..it's good to stop, look up
501
00:23:45,400 --> 00:23:47,640
and enjoy our beautiful universe,
502
00:23:47,640 --> 00:23:49,120
asteroids and all.
503
00:23:52,560 --> 00:23:55,120
You can even see a few yourselves.
504
00:23:55,120 --> 00:23:58,160
Our resident stargazer, Pete,
is on hand to guide us
505
00:23:58,160 --> 00:24:01,480
through some of the upcoming
highlights in the night sky.
506
00:24:01,480 --> 00:24:04,640
For amateur astronomers,
the big news while we were off air
507
00:24:04,640 --> 00:24:08,880
was the display of planets
that were out in force.
508
00:24:08,880 --> 00:24:12,040
Now most of them are
disappearing from view,
509
00:24:12,040 --> 00:24:15,240
but Jupiter and Mars
are still there to spot,
510
00:24:15,240 --> 00:24:17,680
visible in the early evening sky.
511
00:24:18,840 --> 00:24:21,320
Jupiter is especially obvious,
512
00:24:21,320 --> 00:24:26,040
{\an8}low above the west-northwest
horizon as darkness falls.
513
00:24:26,040 --> 00:24:28,960
{\an8}It can be seen in conjunction
with a beautifully thin,
514
00:24:28,960 --> 00:24:33,400
13%-lit waxing crescent moon
on the 30th of April.
515
00:24:33,400 --> 00:24:36,120
A wonderful sight
if the weather is clear.
516
00:24:36,120 --> 00:24:40,160
Another easy spot this month
is the Lyrid meteor shower,
517
00:24:40,160 --> 00:24:43,520
and this even has a tenuous link
to asteroids,
518
00:24:43,520 --> 00:24:46,480
because the bodies
which create the debris stream
519
00:24:46,480 --> 00:24:49,280
which passes through
the Earth's atmosphere
520
00:24:49,280 --> 00:24:50,960
to create a meteor shower,
521
00:24:50,960 --> 00:24:53,840
are comets or sometimes asteroids.
522
00:24:55,000 --> 00:24:58,280
{\an8}A meteor shower's radiant is
the small area of sky
523
00:24:58,280 --> 00:25:00,880
{\an8}its meteors appear to emanate from,
524
00:25:00,880 --> 00:25:04,160
{\an8}which in this case is near
the bright star Vega.
525
00:25:04,160 --> 00:25:08,160
{\an8}The shower reaches its peak around
midday on the 22nd of April,
526
00:25:08,160 --> 00:25:10,400
{\an8}meaning the best nights for a watch
will be
527
00:25:10,400 --> 00:25:14,160
{\an8}the nights of the 21st of April
into the morning of the 22nd,
528
00:25:14,160 --> 00:25:17,480
{\an8}and the 22nd of April
into the morning of the 23rd,
529
00:25:17,480 --> 00:25:20,720
{\an8}with the most activity seen
just before dawn.
530
00:25:20,720 --> 00:25:24,320
Watching Lyrid meteors
is a fairly relaxed affair.
531
00:25:24,320 --> 00:25:26,560
All you have to do
is make yourself comfortable,
532
00:25:26,560 --> 00:25:28,760
find a good dark location
533
00:25:28,760 --> 00:25:30,960
and keep watching the sky.
534
00:25:30,960 --> 00:25:35,440
Look at a height about two-thirds of
the way up the sky in any direction.
535
00:25:35,440 --> 00:25:38,640
If you want to try your luck
photographing Lyrid meteors,
536
00:25:38,640 --> 00:25:40,240
it's fairly easy to do.
537
00:25:40,240 --> 00:25:44,040
You just need a camera
with a wide-angle fast lens.
538
00:25:44,040 --> 00:25:46,840
You need to set the camera's ISO
fairly high
539
00:25:46,840 --> 00:25:49,040
and fully open the lens,
540
00:25:49,040 --> 00:25:51,240
and then just take
continuous images,
541
00:25:51,240 --> 00:25:53,280
hoping to grab a meteor trail.
542
00:25:54,640 --> 00:25:56,960
If your sky is light-polluted
and bright,
543
00:25:56,960 --> 00:25:59,440
your image may look like this.
544
00:25:59,440 --> 00:26:03,800
If so, reduce the exposure length
until they aren't overexposed
545
00:26:03,800 --> 00:26:06,000
and you can still see stars.
546
00:26:06,000 --> 00:26:09,040
Then just let it run
for as long as you are out,
547
00:26:09,040 --> 00:26:11,920
or your batteries allow,
and see what happens.
548
00:26:11,920 --> 00:26:14,560
You never know, you might get lucky.
549
00:26:14,560 --> 00:26:17,080
But it's common to take
thousands of images
550
00:26:17,080 --> 00:26:20,720
without a single meteor
on any one of them.
551
00:26:20,720 --> 00:26:22,480
But if you have more advanced kit,
552
00:26:22,480 --> 00:26:25,840
there are two actual asteroids
we'd like to point out.
553
00:26:25,840 --> 00:26:28,560
Neither of them are going to be
hitting the Earth,
554
00:26:28,560 --> 00:26:31,160
but they are fairly easy to see.
555
00:26:31,160 --> 00:26:33,800
The first is 4 Vesta,
556
00:26:33,800 --> 00:26:36,960
which, with a diameter of 330 miles,
557
00:26:36,960 --> 00:26:39,080
is the largest asteroid
558
00:26:39,080 --> 00:26:43,760
in the main asteroid belt
which lies between Mars and Jupiter.
559
00:26:45,600 --> 00:26:47,280
{\an8}To locate the asteroid,
560
00:26:47,280 --> 00:26:49,720
{\an8}use the two brightest stars
in Libra,
561
00:26:49,720 --> 00:26:52,560
{\an8}Alpha Librae, or Zubenelgenubi,
562
00:26:52,560 --> 00:26:56,760
{\an8}and Beta Librae, or Zubeneschamali.
563
00:26:56,760 --> 00:26:59,600
{\an8}Vesta will be located
in northern Libra,
564
00:26:59,600 --> 00:27:03,920
heading towards the border with
Virgo as we head into next month.
565
00:27:03,920 --> 00:27:07,880
Record the suspected star field
over several days
566
00:27:07,880 --> 00:27:10,000
where you think Vesta is located.
567
00:27:10,000 --> 00:27:12,360
If you've got it right,
comparing the records
568
00:27:12,360 --> 00:27:16,400
should reveal Vesta
as a moving star-like dot.
569
00:27:17,520 --> 00:27:20,480
Owners of smart telescopes
have got it easy
570
00:27:20,480 --> 00:27:24,320
as all they have to do is
search for Vesta and start imaging.
571
00:27:24,320 --> 00:27:26,440
For those that like
a bit of a challenge,
572
00:27:26,440 --> 00:27:28,280
then there's 9 Metis,
573
00:27:28,280 --> 00:27:31,520
which comes to opposition
on the 9th of May.
574
00:27:31,520 --> 00:27:33,800
"Opposition "is a term
which describes
575
00:27:33,800 --> 00:27:37,960
when an object is in the opposite
position in the sky to the Sun,
576
00:27:37,960 --> 00:27:40,800
so that means
it's the best time to see it.
577
00:27:42,720 --> 00:27:45,080
It's currently also within Libra,
578
00:27:45,080 --> 00:27:48,440
and we can use the same two stars
we used to locate Vesta
579
00:27:48,440 --> 00:27:50,360
to find 9 Metis.
580
00:27:50,360 --> 00:27:55,040
Just as with Vesta, record
the star field over several nights.
581
00:27:55,040 --> 00:28:00,160
Align the stars and
look for the moving object.
582
00:28:00,160 --> 00:28:02,360
Whether you're snapping Jupiter
with your phone
583
00:28:02,360 --> 00:28:05,200
or you manage to track Metis
across the sky,
584
00:28:05,200 --> 00:28:08,000
we'd love to see
any photographs you've got,
585
00:28:08,000 --> 00:28:10,520
so send them in
to our Flickr account.
586
00:28:10,520 --> 00:28:12,640
You can find details of this at
587
00:28:12,640 --> 00:28:17,440
www.bbc.co.uk/skyatnight
588
00:28:17,440 --> 00:28:20,520
and we'll show
some of our favourites.
589
00:28:20,520 --> 00:28:23,400
Meanwhile, here are
some of the pictures you've sent in
590
00:28:23,400 --> 00:28:25,000
while we were off air.
591
00:28:49,000 --> 00:28:52,160
Happy stargazing! Goodnight.
50245
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