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In July 2022, the first images
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from the James Webb
Space Telescope were released,
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to the joy of myself
and millions of astronomy fans
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all around the world.
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Oh, my gosh!
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CROWD EXCLAIMS
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Wow, look at that.
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At the time, we were all blown away
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by the stunning new images.
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Their exquisite detail reminded us
of the beauty of the universe
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in which we live.
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But as well as the pretty pictures,
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we've also been getting data
from the telescope's
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various instruments, which have
continued working throughout,
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flooding scientists with information
about planets, galaxies,
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and so much more besides.
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Now we're two years on -
and in that time,
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scientists have been busy analysing
the data and putting out papers.
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But has JWST been as exciting
and ground-breaking as we'd hoped?
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And has it been plain sailing
for the telescope itself?
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Well, tonight, we're looking
at the story so far of
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the James Webb Space Telescope.
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Welcome to The Sky At Night.
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So today, I'm on the road,
retracing the steps of
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a journey that Chris made
in the summer of 2022,
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when we got the first release
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of the data from the
James Webb Space Telescope.
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Chris had hit the road
to meet up with researchers
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around the country to find out
what they were hoping
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this new space telescope
could reveal.
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Since then, these scientists
and others have been working hard
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to understand the information
that the JWST sent back.
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And we're off to find out what
they've discovered.
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But first, what has the JWST
story been so far?
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Billions of years ago,
when the universe was young,
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the first galaxies began
to shine brightly,
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illuminated by some of
the earliest stars.
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Their light has been travelling
through the cosmos ever since,
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streaming unnoticed past the Earth
for all of human history.
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Unnoticed, that is,
until two years ago,
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when that ancient light encountered
a fragile golden mirror floating
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in space a million miles from here,
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It was brought to a focus in
some of the most delicate
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and sophisticated instruments
ever launched -
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and we can read its story
for the first time.
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This is the miracle of JWST -
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a telescope built to show us
the hidden places of the universe
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and reveal unimagined wonders.
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In the more than two years
since it launched,
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the telescope has had
its problems, sure.
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It's been hit more than
20 times by micrometeorites -
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tiny particles of dust zipping
about the solar system.
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And one of them's left a permanent
dent on one of those mirrors.
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JWST's controllers now avoid
pointing in directions where
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there are plenty of micrometeorites,
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keeping the telescope safe.
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Actually, we've learned about
the distribution of dust
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in the solar system -
a scientific reward for placing
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our telescope in such peril.
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Otherwise, despite occasional
problems getting used
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to using JWST's instruments,
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our biggest problem has been
deciding where to point.
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Astronomers around the world
have produced enough ideas
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to keep seven or eight versions
of JWST busy.
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And though it's easy to get
lost in the iconic images...
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Oh, look, the Horsehead!
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Orion! Merging galaxies!
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..the telescope actually spends
about three quarters of its time
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doing spectroscopy,
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splitting up the light it receives
into its constituent wavelengths,
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revealing what planetary
atmospheres are made of,
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what's happening deep in
the heart of star-forming regions,
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and finding out quite how far away
those oh-so-distant galaxies are.
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Answer - very.
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Together, JWST's three
instruments have shown us
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a completely new view of Mars.
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They've revealed rings around
a centaur asteroid in
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the frozen outer solar system,
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have given us a new view of
old clusters of stars in our galaxy,
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and shown a spectacular star
formation in more distant systems.
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Best of all, it gives us new views
of very familiar objects,
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like this one of the Ring Nebula,
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which shows mysterious spikes
pointing away from the centre,
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a ring that's comprised of
20,000 separate clumps of gas,
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each the mass of the Earth.
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And the telescope has also revealed
a complex soup of carbon molecules -
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unusual for a planetary nebula.
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And this is just one object.
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Imagine how much more
there is to see.
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The truth is, we could fill every
episode of The Sky At Night
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for the next 20 years with new data
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and new images from this most
marvellous of observatories.
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And, you know, we probably will.
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So, that's what
the JWST has achieved.
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But science can be more
complicated than that.
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For every answer, it reveals
another exciting question.
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I'm off to the
University of Bristol
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to find out what Dr Hannah Wakeford
has discovered since
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she met Chris two years ago.
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Hannah, good to see you again.
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Good to see you.
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So, can you believe it was two years
since you last met up with Chris?
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Not really, to be honest.
THEY CHUCKLE
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It seems like yesterday
we were just getting data down
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from the telescope.
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Well, I wanted to play you the clip
just to remind you what happened.
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So, you've been planning
these observations with colleagues
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for a long while, I know.
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How does it feel to finally have
data sitting on this computer?
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Overwhelming.
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I'm getting all teary -
every time I think about it,
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I'm just like, "This is so amazing!"
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You were truly so excited
to get the data.
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I'm still so excited
to get the data!
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Whenever I can get data,
I'm happy to get data.
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I think that's the beauty
of being an observer - is just
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we're always excited to
learn new things.
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One planet that Hannah and her team
were excited to observe
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with JWST was WASP-17b.
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And what's interesting
about this exoplanet?
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So, it is a giant planet.
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It is about twice
the radius of Jupiter,
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but only half of its mass.
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So, it's very low density.
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So, this is an artist's
impression that is now based on
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the observations we got with JWST.
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Oh, wow. So...
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So, people take that data,
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and then create what
they think it might look like?
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So, we talk with the artists,
and we work with them to try
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and describe what we're seeing.
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Now, the data itself looks
something like this.
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Ah, yeah - less artistic.
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It's a little bit harder to sell,
let's say.
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Data from the Hubble Space
Telescope had already revealed
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tiny particles
in the planet's atmosphere.
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But Hannah had hoped data from
JWST's mid-infrared instrument
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could finally tell them what
these particles were made of.
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With JWST, it's our only
opportunity to get these features
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way out in the infrared
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which tell us what that cloud
is actually composed of...
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Yes. ..and in this case,
are silicon dioxide.
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OK. So, if there were not these
clouds made of silicon dioxide
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in the atmosphere, we would have
measured this yellow line.
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OK.
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The peak on the grey and pink lines,
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compared to the yellow one,
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show that light from WASP-17b's
local star had been absorbed
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by a specific molecule
in the atmosphere.
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Hannah was expecting it
to be magnesium silicate -
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particles which make up
rocks and sand -
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as seen on other exoplanets.
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But that's not what they found.
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So, what we actually found
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was more of that kind of
pure quartz form.
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And this is what quartz looks
like here on the Earth.
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So, it's a solid, it's kind of
nice and glittery, and it's clear.
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When you've got
magnesium silicates -
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or iron silicates, in this case -
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you get more of that
amethyst colour.
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Yeah, so it's, like,
that's a contamination... Exactly.
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..but it leads to that
beautiful colour.
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What we actually think is happening
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is we've got these beautiful
quartz crystals
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that are being formed high
in the atmosphere.
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And then, what we found was
that these are nanocrystals.
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So, they're very,
very tiny particles,
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about 100 times smaller than
the width of a human hair.
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And that's what's really
interesting, is that tells us
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that these are likely
the precursors, the first things
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that are forming in the atmosphere.
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This discovery, along with data
from hundreds of other exoplanets
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that JWST has now studied,
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is revealing some of the very
fundamentals of our universe.
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These planets operate
as these individual little
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laboratories for us. Oh, yes.
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Because we can't create
these conditions on Earth.
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This is a high-temperature,
low-pressure,
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hydrogen-dominated environment.
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Ooh - sounds flammable.
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It's not fundable, for certain.
Yes!
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It allows us to really take these,
you know, natural test tubes
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to try and understand
what's going on.
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How would this kind of material
change under different conditions?
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And we've got hundreds of
exoplanets to look at,
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to be able to see,
if we change those conditions,
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what happens to our clouds?
I see - wow.
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So, yeah, it's remote laboratories
where you can do these experiments,
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and you get the data and can
compare. That's powerful.
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And that is the beauty of
the thousands of exoplanets,
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is that we've got enough of them
to start to really understand
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the nature of chemistry and physics
that we think we understand here.
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Hannah, thank you so much.
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It's been fantastic, as always,
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and I look forward to coming
back soon. Take care.
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I would never have envisaged that
these other-worldly atmospheres
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would reveal so much, when I worked
on the James Webb Space Telescope
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over ten years ago.
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And these atmospheres are revealing
detail that is unexpected -
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crystalline structures.
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But we're detecting this from
an atmosphere that is over
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1,000 light years away from us.
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This is the stuff that is
truly mind-boggling.
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While Hannah has been looking
at the planets around distant stars,
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it's the planets around our own star
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that, two years ago, led me
to the University of Leicester,
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just after some astonishing pictures
were hot off the press.
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Just a few days ago,
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this image of Jupiter was released.
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And what I love about this image
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is that it shows an old friend
in a new light,
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with Jupiter's belts and
the Great Red Spot
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glowing in infrared light.
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Since then,
JWST has taken a closer look
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at all four outer planets
in our solar system.
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And George is off to find out
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what they've revealed.
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As an exoplaneteer,
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I usually spend my time studying
planets orbiting distant stars.
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So, it's kind of nice for
a change of pace to learn about
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what's going on with the planets
in our own solar system.
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I'm meeting Professor Leigh Fletcher
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to find out how the last
two years have been for him.
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Welcome to Leicester.
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Thank you so much.
It's so good to be here!
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So, first of all, I just want
to remind you of what you said
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last time we were here.
OK, all right.
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So, tell us about the other planets.
What will we see?
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Uranus is coming up in August
and September.
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Saturn is coming up in October.
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And Neptune, we're going to have
an opportunity to do that
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in 2023 - so about 12 months.
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It is a tremendously exciting time.
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And it's going to keep us
with sleepless nights
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and heavy workloads, I think,
for at least five or six years.
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You said "sleepless nights
and heavy workloads" -
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has that become a reality?
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Gosh, that feels like
a lifetime ago as well.
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It's been a couple of years
now since we filmed that,
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and, honestly, all of
our dreams came true.
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We got all of the data sets
that we were planning
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when Chris and I spoke... Amazing.
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..and the data sets have
confounded us, confused us,
244
00:12:22,440 --> 00:12:23,880
got us excited.
245
00:12:23,880 --> 00:12:25,360
We're going to start with Jupiter.
246
00:12:25,360 --> 00:12:27,840
So, I hear you've had
a few surprises -
247
00:12:27,840 --> 00:12:29,040
pleasant ones, though.
248
00:12:29,040 --> 00:12:32,000
Yeah, I think, you know, if you
think about the Jovian system,
249
00:12:32,000 --> 00:12:33,720
you might ask the question
quite reasonably -
250
00:12:33,720 --> 00:12:35,520
we've been there before,
we've sent missions there -
251
00:12:35,520 --> 00:12:37,880
what else can JWST really tell you?
252
00:12:37,880 --> 00:12:41,000
And even I was surprised when
we got some of these data back.
253
00:12:41,000 --> 00:12:42,640
So, on the screen behind me
254
00:12:42,640 --> 00:12:46,040
is one of JWST's fantastic
images of Jupiter. Mm.
255
00:12:46,040 --> 00:12:48,720
And what we can do is, when you
look at Jupiter over several hours,
256
00:12:48,720 --> 00:12:51,160
you can see all the cloud
features moving around.
257
00:12:51,160 --> 00:12:53,800
We did it at a different
wavelength of light,
258
00:12:53,800 --> 00:12:56,920
and one that you can only
really access with JWST.
259
00:12:56,920 --> 00:12:59,920
And, lo and behold, out pops
a brand-new jet stream
260
00:12:59,920 --> 00:13:01,720
that's gone hidden from Earth view
261
00:13:01,720 --> 00:13:05,520
for the last four decades
of observations of this planet.
262
00:13:05,520 --> 00:13:07,960
And it was just there waiting
for us in the data.
263
00:13:07,960 --> 00:13:11,120
So, my colleagues published this
last year - and what this is,
264
00:13:11,120 --> 00:13:13,040
is a very powerful stream of air
265
00:13:13,040 --> 00:13:14,920
high above the Jovian equator
266
00:13:14,920 --> 00:13:18,000
that is somehow linked to
the atmosphere high above.
267
00:13:18,000 --> 00:13:20,480
And this is something
that was completely unexpected
268
00:13:20,480 --> 00:13:22,960
when we first started
inspecting these data.
269
00:13:22,960 --> 00:13:25,880
Seems we've learned a lot about
Jupiter's system. Mm-hm.
270
00:13:25,880 --> 00:13:28,840
Have we learned anything new
and exciting about Saturn so far?
271
00:13:28,840 --> 00:13:30,920
On the screen behind you
is the first image
272
00:13:30,920 --> 00:13:32,400
we captured of Saturn.
273
00:13:32,400 --> 00:13:35,240
The atmosphere looks fairly
bland there, but the rings
274
00:13:35,240 --> 00:13:38,000
are absolutely resplendent
in these data. Stunning.
275
00:13:38,000 --> 00:13:39,720
We saw that the rings are
276
00:13:39,720 --> 00:13:42,440
astonishingly pure, crystalline
water ice
277
00:13:42,440 --> 00:13:44,920
with just a tiny, tiny fraction
278
00:13:44,920 --> 00:13:46,920
of things like organics peppering
the rings
279
00:13:46,920 --> 00:13:48,760
to give them their glorious colours.
280
00:13:48,760 --> 00:13:50,760
We saw that
the atmosphere of Saturn,
281
00:13:50,760 --> 00:13:54,240
which is seasonal,
and we had a prediction that
282
00:13:54,240 --> 00:13:58,040
the atmospheric flows on Saturn
would shift direction,
283
00:13:58,040 --> 00:14:01,160
and those predictions were
borne out quite accurately.
284
00:14:02,680 --> 00:14:05,440
While Jupiter and Saturn
are building a more detailed
285
00:14:05,440 --> 00:14:07,320
picture of their systems,
286
00:14:07,320 --> 00:14:10,560
it is the two most distant planets
that have Leigh and his colleagues
287
00:14:10,560 --> 00:14:13,120
relooking at their models.
288
00:14:13,120 --> 00:14:17,160
So, now what about our two
big enigmas, Uranus and Neptune?
289
00:14:17,160 --> 00:14:18,920
So, you have to remember that
290
00:14:18,920 --> 00:14:21,520
Uranus and Neptune have only had
a single fly-by mission,
291
00:14:21,520 --> 00:14:24,480
the venerable Voyager 2,
back in the late 1980s.
292
00:14:24,480 --> 00:14:27,040
And since then, we've been observing
with ground-based telescopes,
293
00:14:27,040 --> 00:14:28,960
with the Hubble Space Telescope.
294
00:14:28,960 --> 00:14:31,800
And we thought we were
starting to generate a decent
295
00:14:31,800 --> 00:14:33,640
understanding of these worlds.
296
00:14:33,640 --> 00:14:38,480
And, unfortunately, when
we started to apply our models
297
00:14:38,480 --> 00:14:41,960
based on all that prior knowledge
to the new JWST data,
298
00:14:41,960 --> 00:14:44,400
we started to realise
something wasn't adding up,
299
00:14:44,400 --> 00:14:45,680
something was missing.
300
00:14:45,680 --> 00:14:49,320
It was like making a cake and having
all of the ingredients for the cake,
301
00:14:49,320 --> 00:14:51,960
but then, when you actually taste
the cake, there's something just
302
00:14:51,960 --> 00:14:53,240
not quite right in the flavour.
303
00:14:53,240 --> 00:14:56,440
And it's that missing ingredient
in our spectral models
304
00:14:56,440 --> 00:14:58,440
that we're trying to pin down
at the moment.
305
00:14:58,440 --> 00:15:00,000
But that's exciting, right?
306
00:15:00,000 --> 00:15:03,600
Because it means that we are going
to learn something fundamentally new
307
00:15:03,600 --> 00:15:06,400
about the chemical composition
of these two worlds that
308
00:15:06,400 --> 00:15:08,480
we didn't expect to be even
asking about
309
00:15:08,480 --> 00:15:10,280
when we first launched JWST.
310
00:15:11,960 --> 00:15:15,240
Research continues on
Uranus and Neptune,
311
00:15:15,240 --> 00:15:17,160
but this was to be expected.
312
00:15:17,160 --> 00:15:20,200
Leigh did say there was about
six years' work to be done,
313
00:15:20,200 --> 00:15:22,520
and we've come back after just two.
314
00:15:22,520 --> 00:15:26,200
But it's still amazes me
just how much JWST is changing
315
00:15:26,200 --> 00:15:29,120
our understanding of objects
around our own sun.
316
00:15:30,720 --> 00:15:33,160
The solar system is our
home planetary system,
317
00:15:33,160 --> 00:15:36,840
and we've been studying it with
telescopes for a while now and,
318
00:15:36,840 --> 00:15:39,640
you know, staring at it
for thousands of years.
319
00:15:39,640 --> 00:15:43,680
Is it surprising that there's
still so much more new stuff
320
00:15:43,680 --> 00:15:45,120
to learn about it?
321
00:15:45,120 --> 00:15:48,720
I think, whenever you have a
brand-new capability like JWST,
322
00:15:48,720 --> 00:15:51,560
there's always going to be
something, some wavelength of light
323
00:15:51,560 --> 00:15:53,720
that's going to deliver
something that surprises you.
324
00:15:53,720 --> 00:15:55,280
And you're absolutely right,
325
00:15:55,280 --> 00:15:57,760
the solar system has been
fabulously well studied,
326
00:15:57,760 --> 00:16:00,800
but some of the questions
that we're trying to answer now,
327
00:16:00,800 --> 00:16:02,880
like little pieces of
a jigsaw puzzle,
328
00:16:02,880 --> 00:16:06,960
they add up to a much greater,
much more impactful
329
00:16:06,960 --> 00:16:09,800
and deep understanding of this
wonderful solar system
330
00:16:09,800 --> 00:16:11,400
that we're a part of.
331
00:16:11,400 --> 00:16:13,600
Well, thank you
so much for having me.
332
00:16:13,600 --> 00:16:16,000
It's been so great chatting to you.
Always a pleasure to have you.
333
00:16:16,000 --> 00:16:18,840
Well, look forward to next time.
OK. Take care. Bye-bye.
334
00:16:21,680 --> 00:16:24,600
While Maggie and George have been
catching up with scientists
335
00:16:24,600 --> 00:16:26,600
we met two years ago,
336
00:16:26,600 --> 00:16:28,840
I've headed to
the University of Cambridge's
337
00:16:28,840 --> 00:16:31,240
Kavli Institute of Cosmology,
338
00:16:31,240 --> 00:16:36,080
where a fetching set of 1:1 scale
replicas of JWST's mirrors
339
00:16:36,080 --> 00:16:37,200
can be found.
340
00:16:38,600 --> 00:16:41,640
Because light can travel through
the universe for millions,
341
00:16:41,640 --> 00:16:43,120
or even billions of years,
342
00:16:43,120 --> 00:16:46,800
our telescopes are time machines,
showing us the past.
343
00:16:48,040 --> 00:16:50,240
And, with its 6.5-metre mirror,
344
00:16:50,240 --> 00:16:52,920
JWST is allowing us
to peer back further
345
00:16:52,920 --> 00:16:54,680
than we ever have before.
346
00:16:58,520 --> 00:17:00,800
I'm meeting Dr Sandro Tacchella,
347
00:17:00,800 --> 00:17:03,280
who studies these
very young galaxies
348
00:17:03,280 --> 00:17:05,440
to find out what has been revealed.
349
00:17:05,440 --> 00:17:06,520
Hey, how are you?
350
00:17:06,520 --> 00:17:09,520
Hi, Chris, good to see you. Nice to
see you. Thanks for having us.
351
00:17:09,520 --> 00:17:11,960
You're welcome.
Well, I'm excited by this.
352
00:17:11,960 --> 00:17:15,240
What did we know about
the early universe before JWST?
353
00:17:15,240 --> 00:17:18,320
What have we learned from all
of those years of pointing
354
00:17:18,320 --> 00:17:20,200
at these things with
the Hubble Space Telescope?
355
00:17:20,200 --> 00:17:22,680
Yes, so Hubble gave us really
already a very good overview of
356
00:17:22,680 --> 00:17:24,120
what happened in the universe
357
00:17:24,120 --> 00:17:26,680
through most of cosmic time,
which means that we are, you know,
358
00:17:26,680 --> 00:17:29,680
looking at the universe of the age
at about two to three billion years.
359
00:17:29,680 --> 00:17:31,680
That's pretty good.
That's pretty good indeed.
360
00:17:31,680 --> 00:17:33,800
But the growth
at earlier cosmic time -
361
00:17:33,800 --> 00:17:35,440
so that's in the
first billion years -
362
00:17:35,440 --> 00:17:37,880
is actually the most active growth
and the most interesting growth,
363
00:17:37,880 --> 00:17:40,120
in that sense, because that's
where the very first stars,
364
00:17:40,120 --> 00:17:42,880
the very first black holes
and the very first galaxies
365
00:17:42,880 --> 00:17:44,520
started to form and to assemble.
366
00:17:46,600 --> 00:17:48,320
And it's this early universe,
367
00:17:48,320 --> 00:17:51,360
when galaxies and stars
were first forming,
368
00:17:51,360 --> 00:17:54,400
that JWST is showing us
for the first time.
369
00:17:56,360 --> 00:17:59,240
Scientists around the world
are working together to build
370
00:17:59,240 --> 00:18:02,120
a detailed map of the deep cosmos
371
00:18:02,120 --> 00:18:04,320
as part of a project called JADES -
372
00:18:04,320 --> 00:18:08,040
the JWST Advanced Deep
Extragalactic Survey.
373
00:18:10,600 --> 00:18:13,520
Well, I think what we should do
is take a tour of some of the data.
374
00:18:13,520 --> 00:18:15,760
So, you've got an interactive tool?
Sure, yes.
375
00:18:15,760 --> 00:18:17,800
What you see here is a mosaic.
376
00:18:17,800 --> 00:18:21,160
So, these are basically over,
you know, 400 images that
377
00:18:21,160 --> 00:18:22,600
we have taken over
the last two years
378
00:18:22,600 --> 00:18:24,320
with the James Webb Space Telescope.
379
00:18:24,320 --> 00:18:25,720
And we have put them together.
380
00:18:25,720 --> 00:18:27,480
You know, one of the
very interesting structures
381
00:18:27,480 --> 00:18:29,080
is what we term the cosmic rose,
382
00:18:29,080 --> 00:18:30,640
OK, and you might see why.
383
00:18:30,640 --> 00:18:33,120
So, when I zoom in here,
you can see that this looks like,
384
00:18:33,120 --> 00:18:34,960
you know, a rose-like structure.
385
00:18:34,960 --> 00:18:37,360
And so, this system
is actually very distant,
386
00:18:37,360 --> 00:18:40,360
formed about two billion years
after the Big Bang.
387
00:18:40,360 --> 00:18:42,760
And what you see here
is not just a single galaxy,
388
00:18:42,760 --> 00:18:45,760
but actually a whole group
of galaxies.
389
00:18:45,760 --> 00:18:50,760
But JWST has been able to look back
at even younger galaxies.
390
00:18:50,760 --> 00:18:53,600
So, are there other places
we should visit in this image?
391
00:18:53,600 --> 00:18:56,000
So, this is one of
the deeper patches in the image.
392
00:18:56,000 --> 00:18:58,880
And what I'll show you here
is a galaxy,
393
00:18:58,880 --> 00:19:01,680
which seems to be kind of this
yellowish colour. Yeah.
394
00:19:01,680 --> 00:19:03,920
And this is basically
the most distant galaxy
395
00:19:03,920 --> 00:19:06,000
that is known to us.
That splodge there?
396
00:19:06,000 --> 00:19:07,480
Yeah, that splodge here.
397
00:19:07,480 --> 00:19:10,200
So, it's really probing, basically,
the earliest structures
398
00:19:10,200 --> 00:19:11,760
we know in the universe.
399
00:19:11,760 --> 00:19:15,600
This is the furthest back
in time we've ever seen,
400
00:19:15,600 --> 00:19:19,680
showing us the very earliest
moments of our universe's story,
401
00:19:19,680 --> 00:19:23,280
fewer than 300 million years
after the Big Bang.
402
00:19:23,280 --> 00:19:25,760
So, when you look at this image,
403
00:19:25,760 --> 00:19:28,320
there are lots of splodges
all over the place.
404
00:19:28,320 --> 00:19:30,400
What made you look at
that one in particular?
405
00:19:30,400 --> 00:19:33,520
We have been seeing this object
already in the very early data
406
00:19:33,520 --> 00:19:35,520
we obtained nearly two years ago.
407
00:19:35,520 --> 00:19:38,960
And I think the surprising thing was
that it's actually very bright.
408
00:19:38,960 --> 00:19:41,120
And so, our initial
reaction was,
409
00:19:41,120 --> 00:19:44,640
"Well, it cannot be that distant
because it's too bright."
410
00:19:44,640 --> 00:19:46,120
And so, we took better data -
411
00:19:46,120 --> 00:19:48,320
in particular,
we also took spectroscopy.
412
00:19:48,320 --> 00:19:51,040
And we could clearly see that,
no, that galaxy,
413
00:19:51,040 --> 00:19:54,600
this yellow blob here, is really
this most distant galaxy
414
00:19:54,600 --> 00:19:56,080
that we have ever seen.
415
00:19:56,080 --> 00:19:57,920
So, if this is the record-holder,
416
00:19:57,920 --> 00:20:00,520
how common are galaxies like this?
417
00:20:00,520 --> 00:20:03,320
Yes, so we don't know at the moment.
418
00:20:03,320 --> 00:20:05,320
Er, it's really...
419
00:20:05,320 --> 00:20:08,160
It's basically far off than
whatever we have seen before.
420
00:20:08,160 --> 00:20:10,480
And so, in that sense,
this galaxy is very peculiar.
421
00:20:10,480 --> 00:20:13,320
It's really bright.
It's a very early cosmic times.
422
00:20:13,320 --> 00:20:15,800
And so, it's a really one-off
record-holder at the moment.
423
00:20:15,800 --> 00:20:18,520
But it might be that,
because we have been biased in
424
00:20:18,520 --> 00:20:21,320
the way of how we thought
about these early galaxies -
425
00:20:21,320 --> 00:20:24,160
we were looking mostly
for very young systems,
426
00:20:24,160 --> 00:20:25,760
quite small systems -
427
00:20:25,760 --> 00:20:28,800
we might have seen those galaxies,
but we said, like, "Ah, no."
428
00:20:28,800 --> 00:20:32,400
So we have to go back and look
more carefully at those.
429
00:20:32,400 --> 00:20:34,400
So, maybe they are more
common than we thought.
430
00:20:35,760 --> 00:20:38,800
Finding this particular galaxy
may have been a surprise,
431
00:20:38,800 --> 00:20:42,080
but it's just one of many
that JWST is detecting
432
00:20:42,080 --> 00:20:45,120
from the very early universe.
433
00:20:45,120 --> 00:20:48,760
And the picture the telescope
is giving us is of a young universe
434
00:20:48,760 --> 00:20:50,880
full of galaxies growing quicker,
435
00:20:50,880 --> 00:20:54,240
and forming stars faster,
than had been expected.
436
00:20:57,600 --> 00:21:00,160
How much has this early
universe surprised you,
437
00:21:00,160 --> 00:21:02,360
like, compared to what you
thought you were going to get
438
00:21:02,360 --> 00:21:03,720
a couple of years ago?
439
00:21:03,720 --> 00:21:06,840
It was really, erm,
surprising in the sense of
440
00:21:06,840 --> 00:21:10,480
how much excitement it triggered
also in the general public.
441
00:21:10,480 --> 00:21:13,120
So, I think, you know,
it was beyond just like, you know,
442
00:21:13,120 --> 00:21:15,000
me looking at the screen and
being astonished by
443
00:21:15,000 --> 00:21:16,320
these beautiful images.
444
00:21:16,320 --> 00:21:21,080
For me personally, I think I was
surprised to see of how much -
445
00:21:21,080 --> 00:21:22,520
how good the telescope works.
446
00:21:22,520 --> 00:21:24,600
It's really works amazingly well.
447
00:21:24,600 --> 00:21:27,000
And, you know, like,
the images are beautiful,
448
00:21:27,000 --> 00:21:30,360
but we can take spectra and really
learn about these, you know,
449
00:21:30,360 --> 00:21:33,960
systems in really great detail
that I didn't expect to, you know...
450
00:21:33,960 --> 00:21:35,480
..only maybe dream about.
451
00:21:35,480 --> 00:21:38,200
Well, thank you very much.
It's fascinating stuff.
452
00:21:38,200 --> 00:21:39,800
Thank you very much, Chris.
453
00:21:39,800 --> 00:21:42,360
While the scientists we've
been meeting this month
454
00:21:42,360 --> 00:21:46,760
have their heads down working on
the data that JWST is supplying,
455
00:21:46,760 --> 00:21:50,040
Pete is in Bedford,
looking up to the skies.
456
00:21:52,600 --> 00:21:56,040
The pictures taken by JWST
over the last couple of years
457
00:21:56,040 --> 00:21:58,560
have been nothing short
of mind-blowing.
458
00:21:58,560 --> 00:22:01,000
And although we can't get
the same level of detail
459
00:22:01,000 --> 00:22:03,480
a million miles away here on Earth,
460
00:22:03,480 --> 00:22:08,480
we can find the objects
in those iconic JWST images.
461
00:22:10,400 --> 00:22:14,600
While what we can get from
our back gardens may not compare,
462
00:22:14,600 --> 00:22:17,920
the planets are slowly
moving out of the sun's glare
463
00:22:17,920 --> 00:22:21,680
and will become spectacular
at the end of this month.
464
00:22:21,680 --> 00:22:25,040
In particular, an early-morning view
465
00:22:25,040 --> 00:22:27,800
low over the east-northeast horizon
466
00:22:27,800 --> 00:22:29,320
before sunrise
467
00:22:29,320 --> 00:22:31,240
will reveal bright Jupiter,
468
00:22:31,240 --> 00:22:32,960
brightening Mars,
469
00:22:32,960 --> 00:22:34,920
and binocular-dim Uranus
470
00:22:34,920 --> 00:22:36,440
against the wonderful
471
00:22:36,440 --> 00:22:38,520
stars of Taurus.
472
00:22:38,520 --> 00:22:40,040
At the end of July,
473
00:22:40,040 --> 00:22:41,840
the waning crescent moon moves
474
00:22:41,840 --> 00:22:43,440
through this region too,
475
00:22:43,440 --> 00:22:45,160
presenting a lovely scene
476
00:22:45,160 --> 00:22:47,120
just asking to be photographed.
477
00:22:51,080 --> 00:22:54,600
Saturn is further to
the west of this group,
478
00:22:54,600 --> 00:22:58,840
with dim Neptune in tow
just to the east of it,
479
00:22:58,840 --> 00:23:02,720
Saturn will be reaching
its highest position in the sky
480
00:23:02,720 --> 00:23:06,920
due south under relatively dark
conditions during August -
481
00:23:06,920 --> 00:23:10,360
this being the best time to get
a steady view of the planet.
482
00:23:12,720 --> 00:23:16,240
One of the most popular images
taken by the Hubble Space Telescope
483
00:23:16,240 --> 00:23:18,800
was that of the Pillars of Creation.
484
00:23:18,800 --> 00:23:21,960
JWST took that iconic image
485
00:23:21,960 --> 00:23:23,280
to another level.
486
00:23:24,600 --> 00:23:27,320
While you may not be able
to see the Pillars themselves
487
00:23:27,320 --> 00:23:29,240
unless you have a large telescope,
488
00:23:29,240 --> 00:23:32,080
you can see the nebula
in which they're located -
489
00:23:32,080 --> 00:23:33,920
that's the Eagle Nebula.
490
00:23:33,920 --> 00:23:36,680
Now, this is best seen in
the summer months,
491
00:23:36,680 --> 00:23:40,760
when it's at its highest position
above the southern horizon,
492
00:23:40,760 --> 00:23:42,360
under dark conditions.
493
00:23:42,360 --> 00:23:44,720
The Eagle Nebula can be found
494
00:23:44,720 --> 00:23:47,160
by first identifying Altair,
495
00:23:47,160 --> 00:23:48,840
the southernmost star
496
00:23:48,840 --> 00:23:51,240
in the Summer Triangle asterism.
497
00:23:51,240 --> 00:23:55,200
This is the brightest star
in Aquila - the Eagle.
498
00:23:55,200 --> 00:24:00,040
Locate Delta Aquilae in the centre
below and right of Altair.
499
00:24:00,040 --> 00:24:02,120
Extend the line from Altair
500
00:24:02,120 --> 00:24:04,480
through Delta for three times
501
00:24:04,480 --> 00:24:06,400
that distance again,
502
00:24:06,400 --> 00:24:09,880
passing through the diamond-shaped
constellation of Scutum -
503
00:24:09,880 --> 00:24:12,120
the Shield - as you go,
504
00:24:12,120 --> 00:24:15,280
after which you will find
the Eagle Nebula -
505
00:24:15,280 --> 00:24:16,720
known as M16.
506
00:24:18,080 --> 00:24:21,120
Through small and
medium-sized telescopes,
507
00:24:21,120 --> 00:24:24,600
the Eagle Nebula appears
as a cluster of stars,
508
00:24:24,600 --> 00:24:28,040
the faint nebula gas
being hard to see.
509
00:24:28,040 --> 00:24:30,960
Long-exposure photography
or a large scope
510
00:24:30,960 --> 00:24:33,680
are needed to reveal it properly.
511
00:24:33,680 --> 00:24:35,680
While you're in the region,
512
00:24:35,680 --> 00:24:38,440
look slightly south of
the Eagle Nebula
513
00:24:38,440 --> 00:24:41,760
to see the Swan Nebula - M17.
514
00:24:41,760 --> 00:24:44,280
This is much easier to see.
515
00:24:44,280 --> 00:24:47,640
It's wonderful to think that
with amateur telescopes
516
00:24:47,640 --> 00:24:49,600
or even just your eyes,
517
00:24:49,600 --> 00:24:51,400
you can see the same objects
518
00:24:51,400 --> 00:24:54,520
as the most powerful telescope
sent into space.
519
00:24:54,520 --> 00:24:57,880
Sure, we can't see
the same level of detail,
520
00:24:57,880 --> 00:25:00,200
but it's nice to be reminded that,
521
00:25:00,200 --> 00:25:03,960
as we send telescopes deeper
and deeper into space,
522
00:25:03,960 --> 00:25:06,840
we're all looking at
the same universe.
523
00:25:06,840 --> 00:25:08,960
As ever, if you get some images,
524
00:25:08,960 --> 00:25:11,800
do share them on
The Sky At Night Flickr,
525
00:25:11,800 --> 00:25:13,560
and we'll pick some of
our favourites
526
00:25:13,560 --> 00:25:15,520
and show them next month.
527
00:25:15,520 --> 00:25:17,880
Further details can be found at...
528
00:25:21,280 --> 00:25:24,960
In the meantime, here are some of
our favourites from last month.
529
00:25:51,320 --> 00:25:54,560
JWST can do so much with
a single image.
530
00:25:54,560 --> 00:25:57,600
It can astound, amaze
and surprise us.
531
00:25:57,600 --> 00:25:59,360
And so we thought, before we go,
532
00:25:59,360 --> 00:26:01,840
we'd show you a few of
our favourite images.
533
00:26:01,840 --> 00:26:03,600
This is mine.
534
00:26:03,600 --> 00:26:06,200
It's the Cigar Galaxy - M82.
535
00:26:06,200 --> 00:26:10,760
What you can see is a powerful wind
sweeping away from the galaxy,
536
00:26:10,760 --> 00:26:12,000
driven by the star formation
537
00:26:12,000 --> 00:26:14,200
that's happening
at the galaxy's heart.
538
00:26:14,200 --> 00:26:16,800
This is my favourite JWST image.
539
00:26:16,800 --> 00:26:18,680
It shows you the Goods-North region.
540
00:26:18,680 --> 00:26:22,440
It has been imaged with JWST
in nine different filters,
541
00:26:22,440 --> 00:26:26,040
and what you can see here are
about 50,000 different galaxies.
542
00:26:26,040 --> 00:26:28,880
But there is one particular galaxy
that is highlighted.
543
00:26:28,880 --> 00:26:30,280
This is GN-z11,
544
00:26:30,280 --> 00:26:33,520
this is the most distant galaxy
with a known black hole.
545
00:26:33,520 --> 00:26:37,640
So, this is my favourite
JWST picture.
546
00:26:37,640 --> 00:26:40,000
It is actually a spectrum
547
00:26:40,000 --> 00:26:43,640
which includes the JWST information
548
00:26:43,640 --> 00:26:47,600
from the clouds in
the atmosphere of WASP-17b,
549
00:26:47,600 --> 00:26:50,000
and the information that
we had previously from
550
00:26:50,000 --> 00:26:52,440
the Hubble Space Telescope.
551
00:26:52,440 --> 00:26:56,160
So, this is my favourite JWST image.
552
00:26:56,160 --> 00:26:57,600
And it is, believe it or not,
553
00:26:57,600 --> 00:26:59,800
the Horsehead Nebula.
554
00:26:59,800 --> 00:27:03,240
It's looking over the very top
of the horse's head,
555
00:27:03,240 --> 00:27:05,920
which has been an object
very iconic to me,
556
00:27:05,920 --> 00:27:08,040
as I've been growing up
with astronomy.
557
00:27:08,040 --> 00:27:10,800
So, this image is blowing
my mind because,
558
00:27:10,800 --> 00:27:14,280
as JWST is looking over the top
of the Horsehead into deep space,
559
00:27:14,280 --> 00:27:15,720
what can it see?
560
00:27:15,720 --> 00:27:17,080
Galaxies.
561
00:27:17,080 --> 00:27:19,280
It's an incredible image.
562
00:27:19,280 --> 00:27:20,760
This is my favourite picture.
563
00:27:20,760 --> 00:27:23,920
This is an image of HIP 6546 b.
564
00:27:23,920 --> 00:27:26,960
Now, actual images
of exoplanets are a rarity,
565
00:27:26,960 --> 00:27:29,320
because direct imaging is so hard.
566
00:27:29,320 --> 00:27:32,800
But this was JWST's first
attempt at direct imaging -
567
00:27:32,800 --> 00:27:35,520
and we got this stunning picture
in four different colours,
568
00:27:35,520 --> 00:27:37,360
which is marvellous.
569
00:27:37,360 --> 00:27:41,120
So, I think my favourite image
from JWST so far has been
570
00:27:41,120 --> 00:27:42,960
this image of the ice giant Uranus.
571
00:27:42,960 --> 00:27:46,200
I was so looking forward to seeing
what Uranus and Neptune would
572
00:27:46,200 --> 00:27:48,360
look like through
this fabulous new facility.
573
00:27:48,360 --> 00:27:50,000
So, when these images came out,
574
00:27:50,000 --> 00:27:51,720
I almost had tears in my eyes.
575
00:27:51,720 --> 00:27:54,960
This is a destination
that humanity now needs to send
576
00:27:54,960 --> 00:27:57,000
its next robotic explorer to.
577
00:27:57,000 --> 00:28:00,360
And here, James Webb has captured
it in all of its glory.
578
00:28:00,360 --> 00:28:03,800
One of my favourite pictures
taken by Webb so far is this one,
579
00:28:03,800 --> 00:28:06,240
and it's because of a few
different aspects.
580
00:28:06,240 --> 00:28:08,920
Firstly, I love
the beautiful images,
581
00:28:08,920 --> 00:28:10,480
but this is raw data.
582
00:28:10,480 --> 00:28:12,320
Secondly, it was taken by NIRSpec,
583
00:28:12,320 --> 00:28:14,400
which is one of the instruments
that I worked on.
584
00:28:14,400 --> 00:28:17,560
And thirdly, this is showing
one of the earliest galaxies
585
00:28:17,560 --> 00:28:19,760
that ever existed in the universe.
586
00:28:19,760 --> 00:28:22,800
The fact that we can build
an instrument that goes up in space
587
00:28:22,800 --> 00:28:24,840
and tells us this level of detail
588
00:28:24,840 --> 00:28:27,400
is still quite mind-boggling to me.
589
00:28:27,400 --> 00:28:30,920
If this is what JWST
has achieved in just two years,
590
00:28:30,920 --> 00:28:35,200
its potential over the next 10,
or even 20, must be enormous.
591
00:28:35,200 --> 00:28:38,040
I can't wait to find out
what it's going to tell us.
592
00:28:38,040 --> 00:28:41,080
In the meantime, we're filming
our annual Question Time show
593
00:28:41,080 --> 00:28:42,240
in a few months.
594
00:28:42,240 --> 00:28:45,160
So, if you have a question
for this year's expert panel,
595
00:28:45,160 --> 00:28:48,680
go to our website right now
to find out how to submit it.
596
00:28:48,680 --> 00:28:51,360
Until next time, goodnight.
47067
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