All language subtitles for BBC.The.Sky.at.Night.2018.The.Flying.Telescope.1080p.HDTV.x264.AAC.MVGroup.org.eng

Tonight, in a special programme,

The Sky At Night takes to the air

in a converted jumbo jet.

On board is one of the most amazing
telescopes ever built,

and we're going to see it in action.

So, welcome to The Sky At Night
at 40,000 feet.

We're on our way to NASA's
Armstrong Flight Research Center,

a couple of hours' drive from
Los Angeles, because tonight,

we're flying with SOFIA, the world's
only airborne observatory.

It may look like an
ordinary Boeing 747,

but this ex-passenger aircraft has
been specially converted to

carry a 17-tonne telescope that sees
the universe not in visible light

but in the infrared part of
the spectrum.

Visible light, the light that we can
see with our eyes,

only reveals part of the
universe around us.

In fact, over half the radiated
light comes in the form of infrared,

which tells us about the
formation of galaxies,

of stars and of planets,

and the orbit of black holes.

It tells us the secrets of our
cosmic origins.

You can record infrared light with a
thermal camera like this one,

or with the vastly more
sophisticated SOFIA,

the Stratospheric Observatory

For Infrared Astronomy.

Before we took off, I caught up with
the man who pioneered the

observation of infrared radiation

from the centre of our Milky Way
galaxy way back in 1966.

He could also be said to be the
father of SOFIA - Eric Becklin.

So, we're here with this noisy
aircraft behind us, because we want

to fly in it to go and look at the
infrared, but what is the infrared?

The infrared is the
wavelengths of light

that are beyond the red.

It's a very important extension of
the optical spectrum,

and it's basically heat waves,

so we are detecting heat waves
out in space.

So why do we need a plane to get to
these wavelengths? OK.

Because it's like it's cloudy all
the time down here on Earth

in the infrared, so we want to get
up into the stratosphere,

get into the stratosphere

above most of the water vapour
and it clears up,

especially out into what we call a
mid- and far-infrared,

where most of the radiation from our
galaxy and other galaxies

is coming out.

I want to imagine what it would be
like to be able to see

the far-infrared with my eyes,
so let's pick something from here.

Let's say I look towards the
constellation of Orion,

but in the far-infrared,
what would I see?

The picture you get of what's out
there, in a region like Orion,

where stars are forming,

is completely different when you
look in the infrared.

There are some things that are
completely invisible,

that you only see in the infrared.

There's a bar, a mission,
you see in the optical,

but in the infrared,
it comes out really bright.

And one of the things that you see
in the infrared is something called

the BN Object. You discovered that
when you were a graduate student?

That's right. And that's the
brightest source there.

That is... No, it's not the
brightest, actually.

There are some things that are
brighter,

but it was the first one found.

There are believed to be forming
stars, and they're in the

youngest stages of formation,

so this is the closest region where
massive stars are forming

The BN -
or Becklin Neugebauer - Object

is 1,400 light years away in
the Orion Nebula.

It was discovered by Eric in 1967,

the first protostar ever seen,

and since the launch of SOFIA
in 2010,

Eric and his team have been
able to explore

the infrared universe in
even more detail.

You've looked, I know, at the
centre of our galaxy,

at the centre of the Milky Way,

where there's this super-massive
black hole.

What does the infrared tell us
about the galactic centre?

Well, first of all, the infrared

is what allowed us to see that

there was a black hole there,
because there's so much dust

between us and the galactic centre

the light is completely extinguished
by a factor of a billion.

Wow! So you can't see anything.

You don't see anything, so you have
to go into the infrared,

and you can see through the dust,
just like you can a fire,

when it's smoky.

They have infrared-view cameras
and can see right down to the fire.

We do the same to the galactic
centre,

so that's how we actually saw there
was the black hole.

But now, in addition to that,

with SOFIA and the
mid- and far-infrared,

we can actually see the dust
orbiting around the black hole,

so it's very much like the fact
that planets orbit around the sun...

Yeah, yeah, yeah.

..but now we're talking about
Yeah, yeah, yeah.

..but now we're talking about
material and stars

orbiting around the black hole.
Well, it's a pleasure to be here.

I'm looking forward to getting
on board. Thank you very much.

Yeah, have a good flight.
And thank you for SOFIA!

I hope you enjoy it.
I'm sure I will. Thanks.

Back on board, the mission is
about to get under way.

Ready for takeoff, and for the
next ten hours, we're travelling to

the cutting edge of infrared
astronomy.

We'll be finding out how
this magnificent,

slightly odd machine operates,
and why it's so important

for astronomers to view the universe
with infrared eyes.

By climbing 40,000 feet into
the stratosphere,

SOFIA rises above 99% of our
infrared-blocking atmosphere.

And now we're up here, the first job
is to uncover the telescope

and calibrate the instruments.

Training the telescope on an object
of known brightness like Mars lets

the team calibrate the instruments
and tune out the background noise.

For the first two decades of its
life, SOFIA was a passenger jet,

but it was acquired by NASA
in 1997 and extensively modified.

Where once rows of passengers sat,

now a 17-tonne, 2.7-metre
reflecting telescope resides.

To limit the impact of having a huge
open door in flight,

the fuselage was also modified
to avoid turbulence.

As the science team settle into
the ten-hour flight,

Pilot Dean Neeley has time
to take a break from the cockpit

and tell me what it's like to fly.

So, how's your evening going?

It's great, this flight's
gone really well.

A lot of work from a lot of people
leading up to it

really made this happen,

so made it fairly easy
and smooth to execute.

And so how does flying a plane like
this compare to a normal aircraft?

It's very unique for
several reasons.

One, it's huge, as you can see.

One thing that reminded me,
as we started the engines

and began to taxi out tonight,

I always feel like I'm driving
a stadium around.

You know? You're so high in the air,
and steering this thing is

unlike anything else, so it's a
very large aircraft.

And then you take on top of that
the special design and the

modifications putting this
incredible telescope in the back.

I mean, there's nothing like it
anywhere in the world.

Because of those modifications, if
you took, say, a commercial pilot

who'd spent their life flying
747s, and you put them here

and you didn't tell them about the
back end,

do you think they'd notice,
just from the way it handles?

Honestly? No, they wouldn't,
because of the amazing way

that they did the aerodynamic
modelling and designing

with the structure in the back for
the telescope assembly.

In fact, when the whole back side of
the aircraft opens up

for the telescope to look out -
in the front,

I would never even know it except
there's a little light on the panel

that says it's open or closed.

So, in preparing for an
evening like tonight,

how much back and forth is there
with the science team?

How much negotiation about
what's possible

and what the ideal
situation would be?

What you see going on here is only
a small part of it.

So the planning for this started
many months ago. The astronomers

and the science planners putting
together a rough plan, and then

they pass that to an aircraft
planner -

typically somebody who's a
former navigator,

who understands the flying, so as
you lead up to the day of the flight

they go a few rounds starting
36 hours prior to the flight,

and then the last round
to finalise the details

of the timing and everything is
12 hours prior to the flight.

What about when we're
flying along?

We're at 43,000 feet right now in
the middle of an observation.

Are you having to do things to try
and keep the flight

as steady as possible, or does the
telescope take care of that for you?

No, the telescope does most
of the precise hard work,

and what we've got to do is
just keep the aircraft

as steady as possible,
cos it's very sensitive,

so when we make turns, we make very
small turns -

one degree at a time -

maybe one degree every 20 or 30
minutes typically,

and we make sure when we do those
turns,

we only use one or two
degrees of bank.

We have to think ahead, because we
can't just manoeuvre like a

normal aircraft would, including
climbs and descents

to different altitudes,
things like that.

Yeah I'd noticed this evening
there's some negotiation,

or at least chatter
amongst the team,

about when to climb
and how fast to climb and so on.

It seems collaborative. Yeah.

Very much so. The people driving
the airplane up in the front

have to work through the
mission director,

who is kind of like the orchestra
conductor,

working with everybody else
down here,

including the telescope operator.

The one thing you have to get used
to, as a NASA research pilot,

is when you get in a group
like this,

I have to be humble enough to
understand that I'm the dumbest guy

in the room, and just drive the
plane the way I'm supposed to.

Rather important, though. We
should let you get back to it.

Thanks for your time and enjoy the
rest of the flight.

Sure. It was great talking with you.
Thanks.

SOFIA's focus is the far-infrared,
which makes it ideal for

astronomers who want to peer
through gas and dust.

One of the biggest mysteries in
astronomy today

is how dense clumps of gas
form into stars.

SOFIA's High-resolution Airborne
Wideband Camera +,

or HAWC+,

is used to investigate just that.

I caught up with project scientist
Kimberly Ennico Smith

on the much quieter upper deck.

So, one of the reasons we're here on
this marvellous aircraft is

to learn about star formation.

What do we know and what are the
mysteries of star formation?

Big questions, Chris, and questions
that we've been asking

for a long time,

and learning as we go,
but if you think about it,

some of the big questions about
stars and how they formed are still

unanswered. There's a mystery out
there. Why, when we look at

our Milky Way, when we look at other
galaxies,

why are stars forming in certain
regions

and stars are not forming
in other regions?

What makes those places special?
What makes them different?

And it's infrared that matters
because that's where the action is?

These wavelengths of light longer
than our eyes can see allows us

to peer deep into clouds that we
wouldn't see in the visible,

and that means we can get at the
heart of, you know,

where stars are forming.

A lot of the images that we are
taking in the infrared

don't show the stars at all.

They're showing the dust from which
stars are forming,

or into which stars are going after
they head at the end of their lives.

So the study of dust is equally
important to the study of stars.

What does HAWC actually see?

HAWC's an infrared camera, so it's
taking pictures and it works

the far-infrared, and we're looking
at the far-infrared and so we're

going to be measuring cold things,
as dust being emitted, cold dust.

I know there are results
already, so can you

say something about what
HAWC's found so far?

Yeah. So it's not published yet.
Even better.

I know, but it's just really
exciting.

So one of the new developments
in star formation theory

is the observations that there are
these structures called filaments.

So, you've got some images here.
So this is optical, I guess.

That's in the optical, and you see
this filament?

It's this long string-like
snake-like cloud.

They could be several degrees
on the night sky.

And in the longer wavelengths here,
you're seeing the gas along

the filaments glowing,
the re-emitting of the light.

It's the opposite, right?
In the optical, the filament's dark,

but here it's the thing that's
glowing brightly.

And then you see the hot spots,
those eyes? Oh, yeah, yeah.

Those are where stars are forming
or they've just formed.

When Herschel did this all-sky
survey and found these

filaments are everywhere in the
Milky Way, some of the filaments

have stars and some of them don't,
so there's a mystery.

We're thinking this is how stars are
forming along these filaments,

but, you know, what can create the
stars from forming?

What might stop them?

Might speed them up?
A lot of mysteries.

So stars are forming in these
filaments,

but it's not that the whole
filament suddenly lights up?

Bits of the filament...
No, little bits.

Sort of like on your Christmas tree
with your fairy lights, right?

Fairy lights on your tree.

By looking at the light from the
filaments in detail,

HAWC+ can detect magnetic fields
within them -

perhaps a clue to how and why the
stars are forming.

So, what's interesting with
the new data from HAWC+ on SOFIA

is measuring the magnetic fields
on filament scales -

actually looking at the shape,
the orientation of the field -

and we're finding they're
perpendicular

to the direction of the filament.

So the filament goes across like
this...?

And the magnetic field is
going down like that. Or like this.

Material would tend to flow along
the magnetic fields, presumably?

One could guess, or it could
be a barrier.

It's unclear, so one idea is
just like, you know,

a hedgerow on the countryside and
it's a windy day and you have...

You know, this time of year, we have
lots of leaves falling down.

Yeah, yeah, yeah.

If you have that wind blowing
perpendicular to the hedgerow...

Yeah, yeah, yeah.

..the leaves start accumulating.

Yeah. Could the magnetic fields...

If they're perpendicular,
there'll be a channel to, you know,

add material or create instabilities

for which, chaotically, things will
collapse and form stars.

So those are then the places
where stars will form? Could be.

And the critical thing here is that
the instrument HAWC+

allows you to look at what's going
on in the filament.

Previously, we've only had a really
broad-brush look. That's right.

Now we can zoom in and see where the
action's happening.

It's clear we're just at the
beginning of what HAWC+ will do,

so I'm looking forward to seeing the
rest. Thank you very much.

Thank you. And it's a pleasure to
host BBC Sky At Night... Thank you.

..on the world's premiere
flying observatory.

We're well into the flight now,

we're about 1,000 miles off the
coast of California.

The telescope is looking at its
science targets.

The plane is moving around a bit,
even though we're up at 40,000 feet,

which begs the question,
why would you put a telescope

on a vibrating platform like an
aeroplane at all?

Making sure SOFIA's telescope stays
trained on its targets

is Emily Bevins

Tonight, the team are using the
telescope to investigate

how stars evolve, but the ability to
continually swap out and

customise different instruments for
different tasks means that

SOFIA has been able to investigate
many different phenomena,

from dust circling around black
holes

to the activity of passing comets,

and it will soon have another
string to its bow -

it will be able to probe
how planets form...

..because NASA's currently building
the next generation instrument,

the High Resolution MidInfrarEd
Spectrometer,

or HIRMES.

Before taking off,
I met with Sam Richards,

who's one of the team designing and
building the instrument.

So, Sam, thanks for talking to us.

You're working on the next
generation of instrument for SOFIA,

something called HIRMES. What is
HIRMES and what's it going to do?

HIRMES is looking primarily at
protoplanetary discs,

and these are discs

around other stars where once,

a long time ago in our solar system,

it was just a disc of material,
you know, dust and ice.

This is the leftovers from
star formations.

Exactly, yeah.

So it accumulates around in a disc
around a star,

and then those discs, those
particles, can join together

and they build up small little
pebbles,

and then the pebbles become rocks,

and rocks become asteroids
and comets and things like this,

and, eventually, you get planets.

It's always amazed me that we don't
really understand that process,

how the dust sticks together.
Exactly.

So we have our own solar system,

which is one data point,

and we know it fairly well
but we still don't know

why it's in the order that it is,

and where all this material
and chemicals came from,

so this is one of the key reasons
why HIRMES is being made,

so with the high-resolution
aspects of it,

we can understand how this material
is moving around other stars,

and then how the different
components, like the water

and the ice and the oxygen and
all these kind of

key life-building components,

how they come together and
then they evolve over time

to eventually create what would
be a solar system like the Earth

and with gas giants like Jupiters
and Saturns and things like this.

Why is it important to look at the
water and the oxygen?

What stories do those tell us?

One of the big questions about
how Earth got its water

and why it has so much water is,
how did we get here?

Because we think the early Earth
was dry.

Yes. It lost all its water and
we've got to get it back somehow.

We need the high-resolution science
to be able to figure out

exactly how all this chemistry
moves around in a disc.

Yeah, so that's the point, isn't it?

It's telling you what's happened to
this material over time. Yeah.

So we're on this long journey to
figure out

where our solar system fits into
the story of all the other

potential solar systems out there,

and then we can figure out which
family tree that we came from,

and then kind of backdate the models
that way.

So, this is exciting stuff
and this will depend on HIRMES,

which I think will start
flying, what, next year?

Something like that. Yeah. HIRMES
is currently in the kind of

building phase, so we're currently
putting the components together,

and to achieve this type of science
you really need

a high level of complexity,

which you can't really do
from space,

and SOFIA's the perfect platform
for this type of instrument.

You're fairly new to the project.

You've flown on SOFIA before,
so what was the first flight like?

I'm a total fan boy, so when it
comes to NASA

and this type of mission, you know,
you get to don the flight suit,

all the patches, and you really
get to enjoy

being in the moment there

and something that's very different
to ground-based observatories.

Well, good luck. I hope all goes
well and I look forward to seeing

the results from HIRMES.
It's really exciting.

Yes, thank you. We're excited too.

Back on the plane,
operations are in full swing.

Although SOFIA is based in
California,

it's actually a joint venture
between NASA

and the German space agency,
the DLR.

And on board tonight, the instrument

is the German REceiver for Astronomy

at Terahertz frequencies,

or GREAT for short.

GREAT looks at the extreme
end of the infrared,

searching for atoms and molecules
amongst interstellar gas clouds,

because by looking at them,
we can work out how stars evolve

in the crucial first few million
years of their lives.

Instrument Scientist Karl Jacobs

tells me more about what they're
trying to find.

By expanding our view into
the infrared,

SOFIA shows us snapshots of stars
and planetary systems of all ages,

of our own solar system, and build a
clearer picture of the universe.

It's about 3.30 in the morning.
We've just landed.

I'm pretty tired
and so are the crew.

It'll take them weeks and months to
analyse all the data that they got

just from this evening's flight.

One thing's for sure, though.

This is a marvellous way to fly
and to see the universe.

When come back next month, we'll be
on the edge of the solar system.

Until then, good night.