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The UK space industry is booming,
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with a huge income of ยฃ17.5 billion.
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We are now one of the biggest
satellite-building nations
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in the world.
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And the race is still on for
the first orbital rocket launch
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from British soil.
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This month, the Sky at Night team
are investigating the incredible
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science and engineering that's
helping us to blast into space.
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I'll learn how to build a rocket
with a company whose aim
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is to get into orbit next year.
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This is the real thing.
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Yeah, this'll be going to space.
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I'll learn how our most important
satellites will be exposed
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to the dangers of space,
in a brand-new test facility.
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This looks amazing.
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It's such a treat to be in here.
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Radio astronomer Professor Danielle
George discovers a sci-fi solution
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to the impact of the industry
on our night skies.
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We will match the rotation of
the debris and then we will safely
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go and capture with the claw.
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And our in-house stargazing
expert Pete Lawrence tells us
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what we can all see this month.
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Welcome to The Sky at Night.
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Space, as they say, is hard.
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With something as complex
and as powerful as a rocket,
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there's lots to go wrong...
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..as demonstrated in January
by Virgin Orbit...
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The historic rocket mission launch
from Cornwall last night
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failed after the rocket LauncherOne
suffered what Virgin Orbit
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called an anomaly.
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..or the dramatic end to
SpaceX's giant Starship in April.
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Starship just experienced
a rapid unscheduled disassembly.
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These challenges haven't stopped
an increasingly wide range
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of companies, enthusiasts
and dreamers from trying
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to build their own highway
to the stars.
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I've come to Cumbernauld to visit
a start-up called Skyrora.
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Wow! It's impressive.
Yeah, so this is where...
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Euan Clark is the project's
team lead.
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He hopes they'll be the first
to launch into orbit from the UK.
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So why are you building rockets
here in Scotland?
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Currently, the satellites
will need to be transported
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to America or somewhere else
to be launched,
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so building the rockets here
means we can launch from the UK.
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Another advantage is the orbits
we want to go into
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are ideal for launch from the north
of Scotland.
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So that's into sort of polar orbits
around the earth?
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Polar orbits pass over the Earth's
polar regions from north to south.
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This is good for Earth observation
satellites, as they can observe
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most of the Earth's surface
over a 24-hour period.
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And where are we on that journey
to orbit?
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We have tested the third stage,
second stage.
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The next step is just to test
the first stage,
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and then...before bolting it
all together, ready for launch
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sometime later next year.
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This is the real thing, right? Yeah.
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This is going to be your first
attempt at orbit. Yeah.
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This will be going to space.
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Should we take a look at the rocket?
Yeah, let's go for a walk.
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The rocket is split into
three stages.
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I don't think I've ever walked round
a rocket before.
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The top of the rocket
is this third stage.
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This is where the satellite is held
inside a payload fairing.
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This is the payload fairing.
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And this is where the satellite
will sit.
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So this is the most important part
for our customers.
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Each stage has its own engines.
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So it's its own mini spacecraft,
basically. Yeah.
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So this is what'll take the
satellite and deliver it into orbit.
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The middle part of the rocket,
the second stage,
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gets the rocket into space.
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And then here we have an adaptor
that connects the second stage
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with the third stage.
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The second stage is clearly
much meatier. Yeah.
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So it's 2.2 metres in diameter
and around four to five metres long,
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and it's got one 70 kilonewton
engine on it,
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to take it just to the edge
of space.
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And finally, it's the first stage
which isn't on the factory floor yet.
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This bottom section gets the rocket
off the launchpad.
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The first stage would be behind me,
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and that'll have nine
70 kilonewton engines on it.
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And that reaches about
14 metres long,
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so it almost doubles the length
of the rocket.
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You realise it's a big thing when
you're standing next to it like this.
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Yeah, it'll be awesome to see it
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once it's stood up
right on the launchpad. Yeah.
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And when it works. When, yeah.
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Some of the engines
on the first stage
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are undergoing testing in the lab.
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So this is our engine bay.
That's where we're manufacturing,
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at the moment, three of
our 70 kilonewton engines.
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Why do you have
these different stages
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that produce the whole rocket?
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It's more efficient to do it
in stages.
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The hardest bit is to get off
the ground and get
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through Earth's atmosphere.
So it takes a lot of fuel.
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So once we've burnt off
most of that,
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we want to get rid of that weight
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and also the nine engines
in the first stage.
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We want to lose that so that
it's not holding us back.
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So we separate, drop the first stage
and then light the second stage.
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And then once the second stage
gets closer to orbit,
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we can drop that as well and get rid
of that unnecessary weight.
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So you're sort of carrying
only what you need
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for each stage of the journey? Yeah.
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This first stage
is the most powerful.
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The nine engines have to get
the entire 55,000-kilo weight
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of the rocket off the ground.
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What are we looking at here?
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We've got the propellants
that come in through the top,
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through the system, the combustion
in the chamber,
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and then out the nozzle
providing the thrust.
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So fuel comes out that way, ignites,
and then that heads up?
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Yep. That's the plan.
And what fuel do these engines use?
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So they use a combination
of kerosene and HDP.
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We need the two propellants. We need
the fuel and we need oxygen.
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Because in space,
there's just a vacuum, no oxygen,
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we need to take our own.
So that's where the HDP comes in.
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What makes those a good fit
for these rockets?
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So there's a few factors.
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They're nontoxic and non-cryogenic,
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so they can be stored
on the launchpad.
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So it gives us a better
weather window.
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So if we're ready to launch,
we fuel the rocket.
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We can put it on pause for a couple
of days until the weather subsides
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and we can get launching again.
This is beginning to sound very much
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like a rocket that can take off
from Scotland.
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Yeah, cos you never know what
the weather's going to be like here.
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What are the things that can go wrong
when you're thinking about
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designing an engine
and sending it off into space?
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Everything needs to communicate
together. So for launch,
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we need the ground system
to communicate
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with the rocket on the pad,
and then hand over control, so...
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So it's flying itself essentially?
That's one of the hardest bits.
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Once the first stage has got
the rocket off the ground,
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it's the second stage that carries
the satellite payload
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through the rest of the atmosphere
and into space.
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But the challenge is keeping it
on course.
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Getting the rocket off the launchpad
is only the start
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of an engineer's worries.
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One of the things to think about
is keeping the rocket pointing
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in the right direction.
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In the old days, that meant flying
something like this gyroscope
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which, if I spin it
and then leave it,
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if I tilt it, it will always try
and come back to the same direction.
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These days, sensors on board
the rocket keep track
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of how it's moving, report to
the onboard computer
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and make necessary adjustments
to the engines if needed.
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Finally, stage three of the rocket
actually delivers
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the satellite payload to
its final destination.
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Euan is giving me a closer look
at a test model.
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It's impressive.
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So this is 2.2 metres in diameter,
and it's not actually the full size.
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There's another metre and a half
to go in the bottom of this,
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so it'll almost touch the ceiling.
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This will protect the satellite,
control the environment around it,
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and then this drops off
just before orbit.
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So what are the advantages of
this sort of third stage
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in getting satellites to orbit?
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A lot of rockets
have two stages, so...
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But with our third one, it's
the equivalent of a taxi service.
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It'll take you exactly
where you want to go.
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So we can have a lot more accuracy
when putting satellites
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into the different orbits.
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The UK is still waiting
to launch a satellite into orbit
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from its own soil, but it has used
its own rocket to launch a satellite
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into orbit from another land.
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And that rocket was the Black Arrow.
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The Black Arrow rocket was proposed
in the 1960s.
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The government wanted to see
if it could build a rocket based
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on existing British technology
that was originally designed
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to launch intercontinental
ballistic missiles.
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The launch site chosen
was the Woomera Rocket Range
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in South Australia.
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After two demonstration flights,
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Black Arrow carried its first
satellite payload in September 1970.
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But the second stage
failed to pressurise,
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and the payload was lost.
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In July 1971, the program
was cancelled on economic grounds,
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but the latest version of
Black Arrow
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had already been shipped
to Australia,
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so they decided to go ahead
with a final launch.
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This launch was successful,
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and Black Arrow placed the Prospero
satellite into Earth's orbit.
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The UK became the sixth nation
to launch its own satellite
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into orbit using its own rocket.
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It also became the first nation
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to cancel its successful
launch program.
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Instead, the focus turned
to the satellites.
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And 50 years on, the UK
has a booming satellite
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and space industry.
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And it's something I'm really proud
to be part of.
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I've spent most of my career
working on satellites -
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missions such as Aeolus,
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designed to measure the wind speed
through the Earth's atmosphere,
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to the JWST, the largest
space telescope ever built.
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I'm really passionate about
what satellites out there can do
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for us right here on Earth.
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Until now, the UK has never
been able to test its own
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fully-assembled
large scale satellites.
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But this is all about to change.
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After five years and ยฃ116 million,
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the national satellite test facility
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is due to finish construction
in just a few months' time.
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And I'm getting an early preview.
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This beast here
is a satellite test unit.
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Now, it looks absolutely enormous,
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but it's about half the size
of the sort of satellite
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that will be tested in this facility.
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When I worked on satellites
in the past, they were usually
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shipped off to Europe for testing.
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The fact that we have these
facilities right here in the UK
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is really ground-breaking.
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Now, these tests are crucial,
cos when a satellite is up there
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in space, there's no going back
to fix it.
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I know from personal experience
that this can be quite terrifying.
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Something you've poured your heart
and soul into is rigorously tested,
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almost to destruction, but not quite.
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One of the first questions is,
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"Will your satellite survive
the launch?"
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So I'm starting at the most
nerve-racking part of the facility,
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the vibration chamber.
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Program manager Sean Stewart
is giving me privileged access.
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I want to talk to you about
sort of the violence
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of getting things into space.
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How do we ensure that
they will survive that?
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So we have two shakers here,
a vertical shaker and a horizontal.
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So when you say a shaker, well,
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is that literally what you're doing?
Shaking? Quite literally.
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The satellites, which weigh about
seven tonnes and are anything
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up to eight metres tall,
they're experiencing 1.5G.
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We replicate all the vibrations
from launch right the way
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through to separation
and placement into the orbit.
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But there's also quite
a strong noise element.
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I mean, I've felt sort of the noise
of a take-off within my lungs,
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and that can cause damage, too,
which people aren't often aware of.
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Absolutely. As the rocket's going up
through the atmosphere,
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the skin of the rocket starts to act
like the walls of a big bass drum,
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and that can set up standing waves
and harmonics within your satellite,
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and you can start to cause damage.
240
00:12:46,800 --> 00:12:49,120
So what we do here is we build
a stack of speakers,
241
00:12:49,120 --> 00:12:53,080
like you'd find at Glastonbury or a
rock concert, from floor to ceiling,
242
00:12:53,080 --> 00:12:55,560
and then we effectively play music
to our satellite.
243
00:12:55,560 --> 00:12:58,560
We play all the sounds that
it will experience at the levels
244
00:12:58,560 --> 00:13:00,200
that it will experience.
245
00:13:00,200 --> 00:13:04,920
A Boeing 747 with all of its
engines, that's 140 decibels.
246
00:13:04,920 --> 00:13:08,240
In here, we'll go to 146 decibels.
247
00:13:08,240 --> 00:13:10,280
At the NSTF,
248
00:13:10,280 --> 00:13:13,160
they'll be able to simulate
the vibration and noise
249
00:13:13,160 --> 00:13:15,880
of the specific rocket
used for the launch,
250
00:13:15,880 --> 00:13:19,600
from Ariane 5 to the Falcon 9.
251
00:13:23,720 --> 00:13:25,320
This looks amazing.
252
00:13:25,320 --> 00:13:28,920
Not many people get to come inside
our vacuum chamber, that's for sure.
253
00:13:28,920 --> 00:13:33,240
The next step for the satellite
is the thermal vacuum chamber.
254
00:13:33,240 --> 00:13:36,600
We've seen the violence of launch,
but once it gets into space,
255
00:13:36,600 --> 00:13:38,640
the satellite is still in
a hostile environment.
256
00:13:38,640 --> 00:13:41,320
We're talking about
extreme temperatures and vacuum.
257
00:13:41,320 --> 00:13:44,200
So how does this facility
actually simulate that?
258
00:13:44,200 --> 00:13:46,320
What we simulate here
is outer space.
259
00:13:46,320 --> 00:13:48,320
We bring the satellite in.
260
00:13:48,320 --> 00:13:51,440
We've translated it through
90 degrees, so it's now horizontal.
261
00:13:51,440 --> 00:13:54,480
We shut the door and then we start
to suck the air out.
262
00:13:54,480 --> 00:13:56,720
How about temperature?
What range does it do?
263
00:13:56,720 --> 00:13:59,480
So we go down to about
-180 degrees centigrade,
264
00:13:59,480 --> 00:14:02,360
and that allows the satellite
to shrink and contract
265
00:14:02,360 --> 00:14:03,720
because it's cold.
266
00:14:03,720 --> 00:14:07,200
But we can also heat up to
plus 130 degrees centigrade,
267
00:14:07,200 --> 00:14:11,480
so considerably on boiling water,
and we can do both at the same time.
268
00:14:11,480 --> 00:14:14,120
So you can have cold spots
and hot spots.
269
00:14:14,120 --> 00:14:16,800
I suppose that's important
because sometimes you have sunshine
270
00:14:16,800 --> 00:14:19,000
hitting one side of your satellite
and not the other,
271
00:14:19,000 --> 00:14:22,320
and you need to know that it will be
thermally stable in that environment.
272
00:14:22,320 --> 00:14:23,440
Very much so.
273
00:14:23,440 --> 00:14:25,760
So, cooling and heating,
how is that done here?
274
00:14:25,760 --> 00:14:28,520
We have 190,000 litres
of liquid nitrogen
275
00:14:28,520 --> 00:14:30,520
stored outside the building.
276
00:14:30,520 --> 00:14:33,280
And in any 24-hour period,
277
00:14:33,280 --> 00:14:36,760
we will use about 90,000 litres
to cool this place down.
278
00:14:36,760 --> 00:14:39,240
Wow! Impressive!
279
00:14:39,240 --> 00:14:41,240
But that sounds pricey.
280
00:14:41,240 --> 00:14:43,280
Everything in space is pricey.
281
00:14:43,280 --> 00:14:47,400
This facility not only is expensive
to be in on a daily basis,
282
00:14:47,400 --> 00:14:49,320
you'll probably be in here
for about 30...
283
00:14:49,320 --> 00:14:52,320
Between 30 and 60 days,
possibly longer.
284
00:14:55,240 --> 00:14:59,400
Last stop - the electromagnetic
compatibility facility.
285
00:15:00,600 --> 00:15:03,360
This is the EMC test facility,
286
00:15:03,360 --> 00:15:05,960
and it's designed to make sure
that your satellite
287
00:15:05,960 --> 00:15:09,000
can communicate effectively
from space.
288
00:15:09,000 --> 00:15:13,200
We're in an electrically neutral
zone, or a Faraday cage,
289
00:15:13,200 --> 00:15:15,840
and that's achieved by having
copper plates in the floor,
290
00:15:15,840 --> 00:15:18,280
the ceiling and the walls around us.
291
00:15:18,280 --> 00:15:21,160
It's a great place to test
an antenna, to see what the antenna
292
00:15:21,160 --> 00:15:24,080
is putting out and also
what it's receiving.
293
00:15:24,080 --> 00:15:29,600
The walls are covered with
over 40,000 of these blue foam cones.
294
00:15:29,600 --> 00:15:31,640
They absorb the signals.
295
00:15:31,640 --> 00:15:35,800
That means if you want to test
your new, super-secure spy satellite,
296
00:15:35,800 --> 00:15:37,400
this is the place to do it,
297
00:15:37,400 --> 00:15:41,280
because anyone out there
won't know what you're up to.
298
00:15:41,280 --> 00:15:45,400
If your satellite makes it through
this final stage unscathed,
299
00:15:45,400 --> 00:15:47,880
then it's probably ready for space.
300
00:15:51,880 --> 00:15:54,400
Space is a hostile environment,
301
00:15:54,400 --> 00:15:58,000
which is why these satellites
need to be tested thoroughly.
302
00:15:58,000 --> 00:16:00,720
And one of the potential hazards
is the sun.
303
00:16:02,760 --> 00:16:05,280
Stargazing expert Pete Lawrence
is here to tell us
304
00:16:05,280 --> 00:16:08,560
how we can observe Earth's star
this month.
305
00:16:08,560 --> 00:16:13,040
As we head into summer,
the height of the late morning sun
306
00:16:13,040 --> 00:16:17,320
means this is a great time
to try out some solar photography.
307
00:16:17,320 --> 00:16:19,640
This summer is particularly good
308
00:16:19,640 --> 00:16:22,200
because we're approaching
solar maximum.
309
00:16:22,200 --> 00:16:27,960
This is a period of peak activity
that happens around every 11 years,
310
00:16:27,960 --> 00:16:32,080
when the poles of the sun's
magnetic field switch places.
311
00:16:32,080 --> 00:16:35,800
It creates some really exciting
phenomena, but it's important
312
00:16:35,800 --> 00:16:38,320
to capture them safely.
313
00:16:38,320 --> 00:16:41,000
You should never look directly
at the sun, of course,
314
00:16:41,000 --> 00:16:44,440
and you should never point
any astronomical instruments at it,
315
00:16:44,440 --> 00:16:50,200
unless you're using certified
solar safety filters.
316
00:16:50,200 --> 00:16:52,320
As well as providing safety,
317
00:16:52,320 --> 00:16:57,520
these filters help us to see
the sun's features more clearly.
318
00:16:57,520 --> 00:17:01,800
I'm starting with a relatively
inexpensive white light filter
319
00:17:01,800 --> 00:17:04,440
and some imagery I managed
to capture earlier,
320
00:17:04,440 --> 00:17:07,640
when the sun was still shining.
321
00:17:07,640 --> 00:17:12,520
So here you can see the sun's
visible surface.
322
00:17:12,520 --> 00:17:15,120
I can also see some sunspots.
323
00:17:15,120 --> 00:17:18,280
And sunspots represent regions
on the sun's surface
324
00:17:18,280 --> 00:17:22,120
where you have a high concentration
of magnetic field lines.
325
00:17:22,120 --> 00:17:25,280
Next, I'm trying a calcium K filter.
326
00:17:26,440 --> 00:17:30,040
And this is where things start
to get a little bit more pricey.
327
00:17:30,040 --> 00:17:34,200
So the view, now, that I've got
shows the sunspots really clearly.
328
00:17:34,200 --> 00:17:37,720
But what really stands out
are the bright patches
329
00:17:37,720 --> 00:17:41,680
around the sunspot groups
and across the sun's disc.
330
00:17:41,680 --> 00:17:43,800
And those are known as plage.
331
00:17:45,080 --> 00:17:50,440
Plage are associated with high
concentrations of magnetic fields.
332
00:17:50,440 --> 00:17:54,200
Finally, I'm going to use
a hydrogen alpha filter.
333
00:17:54,200 --> 00:17:58,800
This allows us to see filaments
and prominences, arcs of plasma
334
00:17:58,800 --> 00:18:01,320
being moved by the magnetic fields.
335
00:18:03,080 --> 00:18:08,200
And if I move to the edge
of the sun,
336
00:18:08,200 --> 00:18:11,400
here, I've got a filament.
337
00:18:11,400 --> 00:18:15,560
And I can see that that filament
extends beyond the edge of the sun,
338
00:18:15,560 --> 00:18:18,320
so it's turning into a prominence.
339
00:18:18,320 --> 00:18:21,680
And amateurs actually named that -
they called it a filaprom.
340
00:18:21,680 --> 00:18:23,680
But they look absolutely amazing.
341
00:18:26,000 --> 00:18:29,760
The longest period of daylight,
the summer solstice, will take place
342
00:18:29,760 --> 00:18:32,440
on the 21st of June in the UK.
343
00:18:33,480 --> 00:18:36,080
For many of us, the nights
don't get fully dark.
344
00:18:36,080 --> 00:18:39,440
This actually helps us to see
brighter patterns of stars
345
00:18:39,440 --> 00:18:42,720
more clearly, as the faintest stars
are hidden.
346
00:18:44,280 --> 00:18:47,120
These patterns are known
as asterisms,
347
00:18:47,120 --> 00:18:49,760
and our summer skies
are full of them.
348
00:18:54,400 --> 00:18:58,520
At the end of June, the summer
triangle moves into position,
349
00:18:58,520 --> 00:19:04,480
formed by the three bright stars
Vega, Deneb and Altair.
350
00:19:04,480 --> 00:19:07,440
The star Deneb marks the top
of the Northern Cross,
351
00:19:07,440 --> 00:19:11,280
and the summer Milky Way
appears to flow through it.
352
00:19:12,800 --> 00:19:16,480
Follow the Milky Way south
and we can see a familiar shape.
353
00:19:16,480 --> 00:19:19,520
This asterism is known
as the teapot,
354
00:19:19,520 --> 00:19:22,840
part of the constellation
Sagittarius.
355
00:19:22,840 --> 00:19:27,000
And finally, to complete the scene,
a small group of stars slightly
356
00:19:27,000 --> 00:19:32,160
northeast of the teapot form
an asterism known as the teaspoon.
357
00:19:32,160 --> 00:19:35,520
If you manage to photograph
any of the summer asterisms
358
00:19:35,520 --> 00:19:39,280
using either your phone or
your camera, we'd love to see them.
359
00:19:39,280 --> 00:19:41,520
Send them to
The Sky at Night Flickr,
360
00:19:41,520 --> 00:19:45,600
and we'll pick our favourites and
feature them in next month's show.
361
00:19:45,600 --> 00:19:50,200
And since we've last been on air,
some of you have been sending us
362
00:19:50,200 --> 00:19:54,720
your incredible images
of the lunar occultation of Jupiter.
363
00:19:56,840 --> 00:20:01,560
But the stars are becoming harder
to observe in our night skies.
364
00:20:01,560 --> 00:20:06,040
And one reason for this is
the increasing number of satellites.
365
00:20:06,040 --> 00:20:08,360
I've come to the Glasgow
Science Centre to speak
366
00:20:08,360 --> 00:20:11,800
to Regius Professor Andy Lawrence
from the University of Edinburgh.
367
00:20:13,280 --> 00:20:16,680
He's one astronomer who's been
particularly outspoken
368
00:20:16,680 --> 00:20:21,200
about the threat of the expanding
space industry to our night skies.
369
00:20:21,200 --> 00:20:23,800
When did you first start
thinking about this problem
370
00:20:23,800 --> 00:20:25,720
that satellites cause astronomers?
371
00:20:25,720 --> 00:20:27,440
Well, for me, there was
a kind of awakening,
372
00:20:27,440 --> 00:20:29,080
I would say, in late 2019.
373
00:20:29,080 --> 00:20:31,680
Like a lot of other astronomers,
I saw an image
374
00:20:31,680 --> 00:20:36,080
from the Dark Energy Survey which
had these streaks going across it.
375
00:20:36,080 --> 00:20:38,040
That kind of shocked me.
376
00:20:38,040 --> 00:20:40,720
So what are we seeing on the dome?
What are these stripes?
377
00:20:40,720 --> 00:20:47,400
Well, this is the tracks
of the 100 brightest satellites.
378
00:20:47,400 --> 00:20:50,480
So this isn't what you'd see
with your eye at any one time.
379
00:20:50,480 --> 00:20:52,880
It's kind of what you might see
if you were able to integrate,
380
00:20:52,880 --> 00:20:54,320
on the sky, the whole night.
381
00:20:54,320 --> 00:20:57,240
Yeah, they cover the whole sky.
They cover the whole sky.
382
00:20:57,240 --> 00:21:00,160
But in reality,
there's a lot more than 100.
383
00:21:01,360 --> 00:21:05,960
The number of active satellites has
increased from around 2,000 in 2018
384
00:21:05,960 --> 00:21:08,640
to more than 5,000 today.
385
00:21:08,640 --> 00:21:11,440
So how does the presence
of these satellites affect astronomy
386
00:21:11,440 --> 00:21:12,760
that we do from the ground?
387
00:21:12,760 --> 00:21:15,120
The big problem is...
388
00:21:15,120 --> 00:21:19,240
..our current obsession
is with wide field surveys.
389
00:21:19,240 --> 00:21:22,560
So with a big area of sky, there's
more of a chance of a satellite
390
00:21:22,560 --> 00:21:24,960
streaking across
during your exposure.
391
00:21:24,960 --> 00:21:27,840
One of the things that made me
realise how big a problem this was
392
00:21:27,840 --> 00:21:32,080
was seeing a satellite streak not in
an image taken from the ground,
393
00:21:32,080 --> 00:21:33,800
but from the Hubble Space Telescope.
394
00:21:33,800 --> 00:21:36,880
And even Hubble, which is in space,
gets affected by this.
395
00:21:36,880 --> 00:21:40,760
Oh, yeah, yeah. So both of the
Starlink satellites, for instance,
396
00:21:40,760 --> 00:21:43,640
and Hubble Space Telescope
are in low Earth orbit.
397
00:21:43,640 --> 00:21:48,280
Satellites can pass within
a few hundred kilometres of Hubble.
398
00:21:48,280 --> 00:21:54,360
Satellite trails on Hubble images
doubled between 2002 and 2021.
399
00:21:54,360 --> 00:21:56,440
And it's not just imagery
that's affected.
400
00:21:56,440 --> 00:21:59,560
Satellites also create
huge interference problems
401
00:21:59,560 --> 00:22:01,160
for radio astronomers.
402
00:22:01,160 --> 00:22:02,480
What's the solution?
403
00:22:02,480 --> 00:22:06,080
If you're in charge for 24 hours,
what would you do
404
00:22:06,080 --> 00:22:07,800
that would fix this problem?
405
00:22:07,800 --> 00:22:11,120
Well, the solution is regulation.
406
00:22:11,120 --> 00:22:16,240
It has to be about trying to
work out what a sensible capacity
407
00:22:16,240 --> 00:22:17,760
is for low-Earth orbit.
408
00:22:17,760 --> 00:22:21,560
Although I started from
professional worry about the effect
409
00:22:21,560 --> 00:22:26,680
on science, and I've come to see
this as an environmental problem.
410
00:22:26,680 --> 00:22:30,920
Up there in space, until recently,
it's been almost pristine,
411
00:22:30,920 --> 00:22:34,520
and that's been very beautiful
and very important.
412
00:22:34,520 --> 00:22:38,200
And we're in danger
of spoiling that.
413
00:22:38,200 --> 00:22:42,240
So I'm now... I'm a space
environmentalist, Chris.
414
00:22:44,400 --> 00:22:47,640
I've always thought the night sky
is a little bit of wilderness
415
00:22:47,640 --> 00:22:51,200
that's right there, that you can just
go out and look at
416
00:22:51,200 --> 00:22:52,840
from wherever you are.
417
00:22:52,840 --> 00:22:55,600
And I think, never mind the effects
on professional astronomy,
418
00:22:55,600 --> 00:22:58,000
if the number of satellites increases
and we lose that,
419
00:22:58,000 --> 00:23:00,760
and we're looking out
not at the cosmos
420
00:23:00,760 --> 00:23:04,320
but at stuff we've put there,
it'll just be very sad.
421
00:23:06,320 --> 00:23:11,160
It isn't just active satellites
that are causing problems.
422
00:23:11,160 --> 00:23:13,840
Dead satellites, and the pieces
of debris they create,
423
00:23:13,840 --> 00:23:16,240
are fast becoming an urgent issue.
424
00:23:17,680 --> 00:23:20,920
A few months ago, on March 14th,
the International Space Station
425
00:23:20,920 --> 00:23:24,960
had to make an urgent manoeuvre
to avoid a passing chunk of debris.
426
00:23:24,960 --> 00:23:27,360
It was the second time that month
that Mission Control had
427
00:23:27,360 --> 00:23:31,600
had to tell the station to dodge and
weave to keep the astronauts safe.
428
00:23:31,600 --> 00:23:35,200
In the past, astronauts have had to
shelter in the station's lifeboats
429
00:23:35,200 --> 00:23:38,520
as their home passed through
clouds of orbital debris.
430
00:23:38,520 --> 00:23:42,400
The point is this - low-Earth orbit
is increasingly crowded.
431
00:23:42,400 --> 00:23:46,040
Keeping track of the thousands
of active satellites run by SpaceX
432
00:23:46,040 --> 00:23:49,160
and all the rest is one thing,
but it's fragments of material
433
00:23:49,160 --> 00:23:51,880
from defunct missions
that really cause a problem,
434
00:23:51,880 --> 00:23:56,840
made worse by missile tests run by
the US, Russia, China and India,
435
00:23:56,840 --> 00:23:59,280
each of which has blown up
a satellite in orbit,
436
00:23:59,280 --> 00:24:02,320
creating thousands of pieces
of shrapnel each time.
437
00:24:02,320 --> 00:24:04,120
Man down!
438
00:24:04,120 --> 00:24:07,360
You might remember this
from the 2013 film Gravity,
439
00:24:07,360 --> 00:24:09,640
where the astronauts are interrupted
in repairing
440
00:24:09,640 --> 00:24:12,880
the Hubble Space Telescope
by a deadly debris cloud.
441
00:24:13,960 --> 00:24:18,280
But this scenario isn't
as farfetched as it sounds.
442
00:24:18,280 --> 00:24:21,960
We're currently tracking
23,000 pieces of debris
443
00:24:21,960 --> 00:24:26,480
larger than ten centimetres, each of
which moves in its orbit faster
444
00:24:26,480 --> 00:24:28,080
than a speeding bullet.
445
00:24:28,080 --> 00:24:32,160
And the high-velocity collisions
that they cause can be devastating,
446
00:24:32,160 --> 00:24:35,320
and they can cause more problems
by creating more debris.
447
00:24:35,320 --> 00:24:39,800
This is the so-called
Kessler Syndrome, a runaway process
448
00:24:39,800 --> 00:24:42,200
in which each collision
leads to more fragments,
449
00:24:42,200 --> 00:24:47,360
which cause more collisions, until
the entire orbital space is filled
450
00:24:47,360 --> 00:24:49,280
and it becomes impossible to use.
451
00:24:49,280 --> 00:24:52,680
Bad news if you want that holiday
in a 21st-century space hotel,
452
00:24:52,680 --> 00:24:57,080
or if you depend on satellites
for navigation or communication.
453
00:24:57,080 --> 00:25:00,520
The solution? It's time we cleaned up
our act in space.
454
00:25:03,320 --> 00:25:05,440
Someone who is
particularly interested
455
00:25:05,440 --> 00:25:09,920
in possible space junk solutions
is Professor Danielle George.
456
00:25:09,920 --> 00:25:12,000
She's a radio frequency engineer
457
00:25:12,000 --> 00:25:14,960
and has worked on incredible
telescopes around the world.
458
00:25:16,760 --> 00:25:18,520
Now I work on both sides -
459
00:25:18,520 --> 00:25:21,840
radio astronomy, which we know
is being negatively affected
460
00:25:21,840 --> 00:25:24,520
by the excess of satellites
and space junk,
461
00:25:24,520 --> 00:25:28,480
but I've also worked on creating
satellites that are launched
462
00:25:28,480 --> 00:25:31,320
to unravel some of the greatest
scientific mysteries.
463
00:25:31,320 --> 00:25:34,480
But it's these satellites that,
once they're launched
464
00:25:34,480 --> 00:25:36,920
and they've done their work,
are left in space
465
00:25:36,920 --> 00:25:38,920
and add to the problem.
466
00:25:40,880 --> 00:25:44,600
I'm visiting a company that's
developing technology to help solve
467
00:25:44,600 --> 00:25:46,280
the space junk problem.
468
00:25:47,640 --> 00:25:51,160
Valentin Valhondo
is the program manager.
469
00:25:51,160 --> 00:25:53,160
This is incredible.
470
00:25:55,400 --> 00:25:58,000
So, Valentin, just tell us
about space junk.
471
00:25:58,000 --> 00:25:59,920
How big a problem is it?
472
00:25:59,920 --> 00:26:03,160
So the way I like to explain
the space industry nowadays,
473
00:26:03,160 --> 00:26:08,280
this is - if you imagine a highway
network of cars moving very fast,
474
00:26:08,280 --> 00:26:09,920
over the last 60 years,
475
00:26:09,920 --> 00:26:13,480
we have been using it without any
tow truck services or maintenance.
476
00:26:13,480 --> 00:26:16,880
We are currently developing
a mission for the UK Space Agency.
477
00:26:16,880 --> 00:26:19,640
In that mission, we will launch
a spacecraft,
478
00:26:19,640 --> 00:26:23,600
and we will plan to remove
two UK satellites from orbit.
479
00:26:25,640 --> 00:26:29,520
The company are developing
a satellite dubbed the Claw.
480
00:26:29,520 --> 00:26:32,200
The idea is that it will use
a pincer motion
481
00:26:32,200 --> 00:26:34,840
to collect pieces of debris
in outer space.
482
00:26:35,960 --> 00:26:37,720
And so what are you testing here?
483
00:26:37,720 --> 00:26:41,640
So, here, we're testing one of
the critical phases of the mission.
484
00:26:41,640 --> 00:26:45,120
We are testing the last approach
before capture.
485
00:26:45,120 --> 00:26:49,600
On one side, we have the cameras
that we will have on the spacecraft.
486
00:26:49,600 --> 00:26:52,200
Uh-huh. And on the other side,
in that robot,
487
00:26:52,200 --> 00:26:54,960
we have a realistic presentation
of the debris
488
00:26:54,960 --> 00:26:57,760
that we will want to capture.
489
00:26:57,760 --> 00:27:03,480
Pieces of debris will be spinning
in orbit at 28,000km per hour.
490
00:27:03,480 --> 00:27:06,320
The claw needs to accurately
track their motion,
491
00:27:06,320 --> 00:27:09,400
and it has to do this
in the darkness of space.
492
00:27:13,600 --> 00:27:17,040
So how do you determine where
the debris is when you're in space?
493
00:27:17,040 --> 00:27:19,080
The sun will illuminate the target.
494
00:27:19,080 --> 00:27:21,480
But it's a very directional light.
495
00:27:21,480 --> 00:27:23,080
It only comes from the side.
496
00:27:23,080 --> 00:27:25,480
We may even have
too-strong reflections...
497
00:27:25,480 --> 00:27:27,400
Yeah. ..that may blind our cameras,
498
00:27:27,400 --> 00:27:31,320
so our algorithms will need to be
able to reconstruct the whole motion
499
00:27:31,320 --> 00:27:34,320
of the spacecraft, only by
looking at the part
500
00:27:34,320 --> 00:27:36,320
that is illuminated. Yeah.
501
00:27:36,320 --> 00:27:39,960
After we have determined
how the debris is spinning,
502
00:27:39,960 --> 00:27:43,160
we will compute a safe trajectory
to capture it.
503
00:27:43,160 --> 00:27:45,320
We will synchronise the motion.
504
00:27:45,320 --> 00:27:49,360
We will have a propulsion system
that will fire small thrusters,
505
00:27:49,360 --> 00:27:52,120
and then we will safely go
and capture with the claw.
506
00:27:52,120 --> 00:27:55,080
So you're literally sort of
emulating how the satellite
507
00:27:55,080 --> 00:28:00,040
is moving in space to capture it?
That's correct, yes.
508
00:28:01,200 --> 00:28:03,240
If the claw doesn't
synchronise perfectly
509
00:28:03,240 --> 00:28:04,960
with the spinning space junk,
510
00:28:04,960 --> 00:28:10,040
it could break off more pieces
of debris, making the problem worse.
511
00:28:10,040 --> 00:28:12,320
Once its prey is safely captured,
512
00:28:12,320 --> 00:28:14,560
it can drag it down
to a lower orbit,
513
00:28:14,560 --> 00:28:17,360
where the debris will burn up
in the Earth's atmosphere.
514
00:28:19,560 --> 00:28:22,120
I'm really impressed with
what companies like this
515
00:28:22,120 --> 00:28:24,400
are trying to do.
516
00:28:24,400 --> 00:28:28,880
Earth's orbit allows us to study
our planet, to send communications
517
00:28:28,880 --> 00:28:30,240
and so much more.
518
00:28:30,240 --> 00:28:32,680
And it's important that
we do it sustainably,
519
00:28:32,680 --> 00:28:35,920
so that future generations
can enjoy its benefits too.
520
00:28:37,440 --> 00:28:38,760
That's all we've got time for.
521
00:28:38,760 --> 00:28:40,920
But join us next month,
when we're meeting the man
522
00:28:40,920 --> 00:28:44,400
who's trying to talk to aliens.
Goodnight.
43625
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