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- The James Webb Space Telescope
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is the largest and most
powerful telescope in space.
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Uncovering secrets of
how galaxies were formed
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and how the universe
was created.
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- The James Webb Space
Telescope is unraveling
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the mysteries of the universe.
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- We'll meet the scientists,
engineers and visionaries
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who brought this
telescope to life.
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- The early days, just a
few people, and a whiteboard,
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how do we build something
that could actually work?
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- We're on a mission to unlock
secrets from the deepest,
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darkest parts of the universe.
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- We can actually see
light that was emitted
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more than 13 billion years ago.
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We literally traveling in time.
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- It took so much ingenuity,
collaboration and dedication
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to design and develop
this telescope.
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I can't wait to see
what we discover.
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- Being a part of something
bigger than yourself,
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that is really why I did this.
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- It's time to go
"Behind the Wings".
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This is gonna be cool.
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I am Myrna James.
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I am a science journalist
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specializing in all things
technology.
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Here at Wings over the
Rockies Air & Space Museum,
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we transport the magic of space
to you right here on Earth.
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Today, we're traveling
through space and time
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alongside the James
Webb Space Telescope
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which is the most capable
telescope in the cosmos.
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Using infrared technology
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and a revolutionary
segmented mirror,
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Webb can gather six
times more light
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than the Hubble Space Telescope.
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The Webb is uncovering how
the universe was created
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and is answering
questions so profound
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we didn't even know we had them.
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With the ability
to observe galaxies
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more than 13 billion
light years from Earth,
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get ready to travel
through time.
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Webb launched in 2021
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but the idea was sparked
more than 20 years ago
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at NASA's Goddard
Space Flight Center.
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- It's human nature somehow
to be fascinated by space
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and our place in the universe.
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So I was taken by
that, just like anyone.
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When I started on
the Webb in 1997,
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there were just a few of us.
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It was just an idea
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but in front of us
was to figure out
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how do we build something
that could actually work.
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The Webb mission was
conceived in the late 1980s,
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early 1990s, to connect the dots
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between the achievement
of NASA's COBE satellite
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which showed us the oldest
light in the universe.
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Around the same time,
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the Hubble Space
Telescope was launched.
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- [Announcer] Two,
one and lift off
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of the space shuttle Discovery
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with the Hubble Space Telescope,
our window on the universe.
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- And it took its deepest
image of the cosmos
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that it was capable
of doing at that time
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and that deep field image,
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so it looked back
in time to a point
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when the universe was
about a billion years old.
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The EPOCH that COBE saw,
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the universe was a few
hundred thousand years old.
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And so between those two
EPOCHs is a mysterious,
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poorly studied EPOCH
that was referred to then
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as the cosmic dark zone.
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And it's a great
scientific interest
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because that is the point in
the evolution of the universe
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when the first stars
and galaxies formed.
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The answers to all our
questions are in starlight
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and we have to be clever enough
to extract that information.
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- In order to create a telescope
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that can see further
back in time,
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NASA needed to invent
new technology that
could gather light
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from some of the first stars
and galaxies in the universe.
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But first, they had to
overcome the challenges
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that plagued the earlier
space telescopes.
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Hubble, for instance, required
hands-on human repairs.
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- A lot of people today
don't even remember
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but when the Hubble Space
Telescope was launched,
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the primary mirror actually
wasn't quite the right shape
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and could not focus
light properly.
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- The significant
spherical aberration
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appears to be present
in the optics.
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- There was actually
multiple repair missions
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and upgrade missions for Hubble.
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The very first one was really
to fix the blurry vision
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and then from then on,
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we were really upgrading
the instruments.
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John Grunsfeld was an astronaut
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who helped to upgrade
the instruments.
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- The Hubble Space Telescope
was launched in 1990.
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In 1992, I became an astronaut.
At the edge of the telescope
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which is 2.4 meters across,
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the shape of the mirror
was wrong by about 1/40th
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of the width of a human hair
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but that was enough to make
the images slightly fuzzy.
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So for an astronomer,
that was bad.
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So instead of being
a great observatory
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in all this anticipation,
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it was a sort of
good observatory or
maybe a little less.
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As an astronomer going to
the Hubble Space Telescope,
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it's kind of the holy grail
of an astronaut's mission.
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And I had the
unbelievable fortune
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of being able to go up
three times to the Hubble
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and do all kinds of repairs
and upgrades to the telescope
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such that now Hubble's coming
up on its 33rd birthday
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on orbit and
everything's working
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and we're still doing
incredible science.
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- [Myrna] So you were
actually able to get inside
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the telescope here?
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- Yep, now clearly
this is just a model,
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the real telescope
is five times bigger,
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about the size of a tour bus.
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And what you can see is that
the telescope has handrails
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that we could use to
climb around the telescope
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but more importantly, it
was designed to be modular,
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to be fixed, not only to
put in new electronics
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but to put in new
scientific instruments.
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And so we were able to
open these doors on orbit.
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You know I was able to
climb inside the telescope
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to take out the old
scientific instruments
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and put new ones in.
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And so you can see this
opening was big enough,
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even for my spacewalking
partner, Steve Smith,
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who's about 6'2", in this
spacesuit to fit inside.
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- So you did eight space
walks, does it ever get old?
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- I wondered during training
whether I would ever get tired
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of getting into the spacesuit
and going into the big pool,
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we called a Neutral
Buoyancy Laboratory.
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You know, I have spent
hundreds and hundreds of dives
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in the space suit practicing
and even that is not old.
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Eight spacewalks - every one is
just spectacular and magical.
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I was on the end
of the robotic arm
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moving back towards the
Hubble Space Telescope,
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when all of a sudden I
thought, is this real?
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You know I just can't believe
that I'm here out in a vacuum
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in my space suit with the
Hubble Space Telescope
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orbiting the earth going
17,500 miles an hour.
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You know, it was kinda
silly but I just reached out
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with my index finger
and touched the Hubble
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to make sure it was real.
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And then of course it was
all work from then on.
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- So the ability to
upgrade the Hubble on orbit
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is one reason that it's
still so productive
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and still up there
after 33 years.
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And that's not true
about the Webb telescope.
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It's actually about
a million miles out.
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- The James Webb Space Telescope
is an infrared observatory,
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that's light from heat.
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And so we have to put the
James Webb Space Telescope
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really far away from the earth
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so that it wouldn't
see the Earth's warmth
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but that has a downside.
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It's too far away, it's a
million of miles from earth.
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So the James Webb Space
Telescope is high stakes
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that we can't go fix it.
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And so a lot of effort
was put into making sure
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that it would work
the first time.
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It's gonna be amazing
what we find out
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but I think the
biggest discovery
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from the James Webb
Space Telescope
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is probably gonna be
the answer to a question
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we haven't thought of.
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Something we truly discover
that we never knew about.
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- What did it take
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to build the most
powerful space telescope?
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With any project as ambitious
as the Webb telescope,
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it takes thousands of
people and many, many years.
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For some of them,
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their entire career was
riding on its success
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and it actually went perfectly.
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Webb was primarily built,
engineered and designed
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at Northrop Grumman Space Park.
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The components were
manufactured in laboratories
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across the globe,
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then were sent back to the
Space Park campus for assembly.
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- The telescope itself
and all the components
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came from different
places across the U.S.
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and across the globe.
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And over behind me,
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that's where we did all
of the engineering work
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to come up with the design,
to come up with the ideas
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of how we were gonna put
it together, et cetera.
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- So Charlie, why are
telescopes so important?
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- What made Galileo think he
needed to make a telescope?
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It is to go see the things
that we can't see
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with our naked eye.
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So we call it a telescope but
it's so much more than that.
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There are unbelievable
quantities of materials
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that went into that telescope
from all around the world.
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Exotic materials that
are really lightweight,
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some that are very
hard, very stiff,
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all kinds of different
materials that engineers used
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to put together the telescope.
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And it took millions of
hours to design it, build it,
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test it, and get it
ready for launch.
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I spent about 20 plus
years as an engineer
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working on the telescope,
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now it's time for the scientists
to use it for 20 plus years
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to make new discoveries,
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to find out things
we don't know yet.
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- Normally in a project,
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if you count up the number of
miracles that have to occur,
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if you get above one,
you're in big trouble.
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On the Webb, we had
10 technologies that
we had to invent
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just to make our concept doable.
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We realized that we had
two enormous problems
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that almost stopped the
project dead in its tracks.
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This big mirror was
bigger in diameter
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than the biggest rocket
that was problem number one.
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- This mirror was so big it
couldn't even be launched
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in a rocket, it has to
unfold and deploy in space?
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- That's right, so
Webb's mirrors are huge,
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they're six and a half meters
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and so the fairing
that we can launch from
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are about five meters
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so they're just a little
over a meter or two big.
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So what we had to do is
fold back two sections,
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one side on the left side,
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one side on the right
side of the mirror
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so that they can fit
into the launch vehicle,
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kinda standing
straight up and down.
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- Problem number two is that
to build an infrared telescope,
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the telescope has to
be very, very cold
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because everything
above absolute zero
emits infrared light.
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If we didn't make the JWST cold,
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it would be blinded by
its own infrared emission.
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How cold do we have to make it?
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Really, really cold,
almost -400 Fahrenheit.
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The JW sun shield has an
SPF of more than a million.
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If you had it on the beach,
you'd be very well protected
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and it enables the Webb to
achieve this low temperature.
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00:10:50,366 --> 00:10:53,433
- Most telescopes have
a sun shield of sorts.
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What you're probably more
familiar with are barrels
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around a telescope
that eliminates light
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00:11:00,366 --> 00:11:03,500
from entering the telescopes
that's not exactly on axis.
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That's what the sun shield
on Webb was trying to do.
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And so the way that it works
was if this light over there
245
00:11:09,933 --> 00:11:13,300
is the sun and I wanna
look at the dark of space,
246
00:11:13,300 --> 00:11:16,166
the sun shield was always
shielding the light
247
00:11:16,166 --> 00:11:18,900
from the telescope, so
my eyes in this case,
248
00:11:18,900 --> 00:11:21,666
so that I never see the sun
249
00:11:21,666 --> 00:11:24,566
and I can look the
other direction
250
00:11:24,566 --> 00:11:28,633
into the darkness to look at
the first stars and galaxies.
251
00:11:28,633 --> 00:11:31,366
- From its sun shield, which
is the size of a tennis court,
252
00:11:31,366 --> 00:11:34,466
to the primary mirror which
is 21 feet in diameter,
253
00:11:34,466 --> 00:11:36,933
the Webb telescope is
an engineering marvel.
254
00:11:38,033 --> 00:11:40,400
- Engineering is an
empirical science.
255
00:11:40,400 --> 00:11:43,300
You have to build
prototypes, test them,
256
00:11:43,300 --> 00:11:46,866
see what went wrong, build
more prototypes and so forth.
257
00:11:46,866 --> 00:11:49,433
And on the Webb, we were
able to do all of that.
258
00:11:50,900 --> 00:11:53,400
One of the things that
makes our work difficult
259
00:11:53,400 --> 00:11:55,700
is that we have to work
260
00:11:55,700 --> 00:11:59,266
in these very, very
clean environments
261
00:11:59,266 --> 00:12:02,366
wearing special garments.
262
00:12:02,366 --> 00:12:06,833
And this is one of
those clean rooms.
263
00:12:06,833 --> 00:12:08,933
This is really one
of the largest rooms
264
00:12:08,933 --> 00:12:10,500
like this in the world.
265
00:12:10,500 --> 00:12:14,133
You can see the people are
wearing these white suits
266
00:12:14,133 --> 00:12:15,533
called bunny suits.
267
00:12:15,533 --> 00:12:18,433
And that's because the
dirtiest thing in these rooms
268
00:12:18,433 --> 00:12:19,966
is the people.
269
00:12:19,966 --> 00:12:21,833
The number of people that can
be in the room at any one time
270
00:12:21,833 --> 00:12:23,066
is limited.
271
00:12:23,066 --> 00:12:25,533
It's cleaner than the
medical operating room,
272
00:12:25,533 --> 00:12:30,600
this whole brown wall
is a giant HEPA filter.
273
00:12:31,100 --> 00:12:34,833
So the air is constantly flowing
horizontally in this room
274
00:12:34,833 --> 00:12:36,833
through that filter.
275
00:12:36,833 --> 00:12:40,466
The goal is to remove every
single particle in the air
276
00:12:40,466 --> 00:12:42,900
that can get into the hardware.
277
00:12:42,900 --> 00:12:45,600
- The James Webb Space
Telescope is not like the Hubble
278
00:12:45,600 --> 00:12:47,433
which could be repaired in orbit
279
00:12:47,433 --> 00:12:49,733
because it's a
million miles out.
280
00:12:49,733 --> 00:12:51,433
When the scientists
launched Webb,
281
00:12:51,433 --> 00:12:53,266
they had one shot
to get it right
282
00:12:53,266 --> 00:12:54,733
so they implemented of course,
283
00:12:54,733 --> 00:12:57,333
extensive testing before
it ever left the ground.
284
00:12:57,866 --> 00:13:00,433
- The testing is as
important as the flight
285
00:13:00,433 --> 00:13:03,566
and so it becomes a
constraint on the design.
286
00:13:03,566 --> 00:13:06,800
Every element of design
we have to include,
287
00:13:06,800 --> 00:13:08,000
how will we test that?
288
00:13:08,000 --> 00:13:11,233
What hardware do
we need to test it?
289
00:13:11,233 --> 00:13:15,733
We call it Ground
Support Equipment or GSE.
290
00:13:15,733 --> 00:13:18,666
So this is one of the
payload areas at Goddard
291
00:13:18,666 --> 00:13:21,866
where we're testing
space flight hardware
292
00:13:21,866 --> 00:13:24,366
and much of the testing we do
293
00:13:24,366 --> 00:13:29,433
is done in space simulation
chambers that simulate
294
00:13:29,433 --> 00:13:33,933
the vacuum and
temperature of space.
295
00:13:33,933 --> 00:13:37,766
And so, these large objects
are space simulation chambers
296
00:13:37,766 --> 00:13:41,566
where space light hardware
is being tested as we speak.
297
00:13:42,833 --> 00:13:47,400
These are giant vacuum chambers
that simulate the vacuum
298
00:13:47,400 --> 00:13:51,133
and temperature and overall
environmental conditions
299
00:13:51,133 --> 00:13:52,433
of space.
300
00:13:52,433 --> 00:13:54,933
The Webb science
instruments were tested here
301
00:13:54,933 --> 00:13:56,533
for many, many months
302
00:13:56,533 --> 00:14:00,433
to ensure that they would work
properly in the Webb mission.
303
00:14:00,433 --> 00:14:04,233
And so to do testing, we have
to simulate the environment
304
00:14:04,233 --> 00:14:06,566
as best we can
here on the earth.
305
00:14:06,566 --> 00:14:08,700
In addition to making sure
306
00:14:08,700 --> 00:14:11,733
that the hardware
will work in space,
307
00:14:11,733 --> 00:14:14,566
we have to make sure
that it can survive
308
00:14:14,566 --> 00:14:17,700
the rocket flight into space.
309
00:14:17,700 --> 00:14:21,600
So we typically have to
simulate that as well.
310
00:14:21,600 --> 00:14:24,666
And these big steel doors
311
00:14:24,666 --> 00:14:29,733
are labs that contain
giant vibration tables
312
00:14:29,733 --> 00:14:33,100
where we will put the payload
on the vibration table
313
00:14:33,100 --> 00:14:37,033
and shake it to simulate
the rocket flight to space.
314
00:14:37,033 --> 00:14:40,400
And we were able to
do all of the testing
315
00:14:40,400 --> 00:14:43,400
that we needed to
do to be confident
316
00:14:43,400 --> 00:14:47,633
that this enormously complex
thing would actually work.
317
00:14:47,633 --> 00:14:50,033
- Once it was built,
the big question was,
318
00:14:50,033 --> 00:14:52,133
can it successfully be launched?
319
00:14:52,133 --> 00:14:55,866
- Being in the mission control
center with 100 other people
320
00:14:55,866 --> 00:14:58,233
that had also poured
their hearts and souls
321
00:14:58,233 --> 00:14:59,633
into this telescope,
322
00:14:59,633 --> 00:15:02,966
the launch was nerve
wracking, to say the least.
323
00:15:02,966 --> 00:15:04,433
There still were some risks.
324
00:15:04,433 --> 00:15:06,933
You know we had a lot of single
point failures to overcome.
325
00:15:06,933 --> 00:15:09,500
It was also very celebratory
326
00:15:09,500 --> 00:15:11,533
because we did have
a lot of confidence
327
00:15:11,533 --> 00:15:13,533
in our partners at Arianespace
328
00:15:13,533 --> 00:15:15,333
to get us up into orbit safely.
329
00:15:15,333 --> 00:15:17,600
- [Announcer] From Jean-Luc
Voer, all systems are go.
330
00:15:17,600 --> 00:15:20,133
We're inside a minute now and
the command will be issued
331
00:15:20,133 --> 00:15:22,333
to ignite the solid
rocket boosters.
332
00:15:22,333 --> 00:15:25,300
The James Webb Space
Telescope will be on its way.
333
00:15:27,133 --> 00:15:28,533
And we have engine start.
334
00:15:31,566 --> 00:15:32,566
And lift off.
335
00:15:34,233 --> 00:15:37,133
Decollage, lift off from
a tropical rainforest
336
00:15:37,133 --> 00:15:40,866
to the edge of time itself,
James Webb begins a voyage
337
00:15:40,866 --> 00:15:43,000
back to the birth
of the universe.
338
00:15:44,733 --> 00:15:46,833
- Back in the Mission
Ops Center in Baltimore,
339
00:15:46,833 --> 00:15:50,733
we were kinda like, "Okay, get
to work, it's now our time."
340
00:15:50,733 --> 00:15:52,966
We still had six more
months of deployments
341
00:15:52,966 --> 00:15:54,966
and commissioning
to get this thing
342
00:15:54,966 --> 00:15:58,100
to do what it's now doing
and exceed expectations.
343
00:15:58,100 --> 00:16:00,733
The successful launch,
that was just the beginning
344
00:16:00,733 --> 00:16:03,866
and now we've turned it
over to the science teams
345
00:16:03,866 --> 00:16:07,366
to find out what they
can with our data.
346
00:16:07,366 --> 00:16:09,366
- There's no one better to
talk to about what goes on
347
00:16:09,366 --> 00:16:11,600
with this telescope
than Kenny McKenzie.
348
00:16:11,600 --> 00:16:13,533
- I had a eighth grade
social studies teacher,
349
00:16:13,533 --> 00:16:15,333
her name was Christa McAuliffe,
350
00:16:15,333 --> 00:16:17,600
she perished in the
Challenger disaster
351
00:16:18,366 --> 00:16:21,733
and kinda motivated me to
enter the space business.
352
00:16:21,733 --> 00:16:23,500
I entered in 1984,
353
00:16:23,500 --> 00:16:26,000
I've spent a lot of time with
a lot of different missions
354
00:16:26,000 --> 00:16:29,300
but beyond all that, this is
the most exciting one so far.
355
00:16:29,300 --> 00:16:32,600
Basically, we're on the campus
of Johns Hopkins University.
356
00:16:32,600 --> 00:16:34,333
This is the Mueller building.
357
00:16:34,333 --> 00:16:35,933
It's the home of James Webb
358
00:16:35,933 --> 00:16:38,166
Science and Data
Processing Center
359
00:16:38,166 --> 00:16:40,000
and now mission
control for James Webb.
360
00:16:40,000 --> 00:16:44,900
During the commissioning and
instrument activation phase,
361
00:16:44,900 --> 00:16:47,233
both of these two rooms
were completely full
362
00:16:47,233 --> 00:16:50,466
with probably 100
engineers at any one time.
363
00:16:50,466 --> 00:16:53,266
- So in this room is where
the deployment of the mirrors
364
00:16:53,266 --> 00:16:55,266
was commanded really.
365
00:16:55,266 --> 00:16:58,466
- We conducted all of
the deployment activities
366
00:16:58,466 --> 00:17:01,333
from solar array deployment
367
00:17:01,333 --> 00:17:04,100
which was the primary and
most crucial deployment
368
00:17:04,100 --> 00:17:07,566
that we had to do
for us to have power.
369
00:17:07,566 --> 00:17:09,133
So the solar array
has to come out.
370
00:17:09,133 --> 00:17:10,166
If you don't have a solar array,
371
00:17:10,166 --> 00:17:11,833
your mission is basically done.
372
00:17:11,833 --> 00:17:13,300
So that was a very exciting,
373
00:17:13,300 --> 00:17:15,900
very positive start
to our mission.
374
00:17:15,900 --> 00:17:17,433
- [Myrna] What was the mood
in the room at that time?
375
00:17:17,433 --> 00:17:20,066
- [Kenny] It was
very, very nervous,
376
00:17:20,066 --> 00:17:21,666
of course, as you
would fully expect.
377
00:17:21,666 --> 00:17:25,300
People were on their
feet, everybody had a job
378
00:17:25,300 --> 00:17:27,133
and we all worked
very well together
379
00:17:27,133 --> 00:17:29,866
and we were able to
deploy it perfectly.
380
00:17:29,866 --> 00:17:33,000
- [Announcer] And we have a
fully deployed JWST observatory.
381
00:17:33,000 --> 00:17:35,700
(group applauding)
382
00:17:35,700 --> 00:17:36,766
- [Crew Member] Yes.
383
00:17:36,766 --> 00:17:38,366
- After 30 days, we were elated.
384
00:17:38,366 --> 00:17:40,033
I mean, we were tired
but we were elated.
385
00:17:40,033 --> 00:17:42,533
We had another five
and a half months to go
386
00:17:42,533 --> 00:17:44,400
with all the instrument
commissioning activities
387
00:17:44,400 --> 00:17:46,200
but we felt comfortable
388
00:17:46,200 --> 00:17:48,166
that all the subsystems
were working.
389
00:17:48,166 --> 00:17:50,833
The communications were good.
390
00:17:50,833 --> 00:17:55,900
Beyond all reasonable
expectations worked as designed.
391
00:17:56,700 --> 00:17:57,800
- That's incredible.
392
00:17:57,800 --> 00:17:59,100
- It was very incredible.
393
00:18:00,500 --> 00:18:02,766
- [Myrna] It's really just the
beginning of a whole new era.
394
00:18:02,766 --> 00:18:04,066
- You know, we're still a baby,
395
00:18:04,066 --> 00:18:07,600
we've been up on orbit
for just over 12 months.
396
00:18:07,600 --> 00:18:11,733
We continue to explore
and develop and uncover
397
00:18:11,733 --> 00:18:13,200
amazing items,
398
00:18:13,200 --> 00:18:16,600
it's a good time to be
part of the Webb program.
399
00:18:16,600 --> 00:18:21,200
- Okay, this is the real time
screen of what's happening?
400
00:18:21,200 --> 00:18:24,633
- Yeah, depicted on this
screen basically is the view
401
00:18:24,633 --> 00:18:26,933
of the observatory
as it sits in space.
402
00:18:26,933 --> 00:18:29,133
We use the deep space network
403
00:18:29,133 --> 00:18:32,733
which is three different
complexes located geographically
404
00:18:32,733 --> 00:18:34,266
around the world.
405
00:18:34,266 --> 00:18:37,166
Gives you a visualization
of where this observatory
406
00:18:37,166 --> 00:18:39,366
and a telescope are pointed.
407
00:18:39,366 --> 00:18:40,800
- So scientists from
all over the world
408
00:18:40,800 --> 00:18:42,866
are so excited about this data.
409
00:18:42,866 --> 00:18:44,300
How do they use it?
410
00:18:44,300 --> 00:18:47,300
- For each program, it looks
at a different part of the sky.
411
00:18:47,300 --> 00:18:48,800
And the longer you stare,
412
00:18:48,800 --> 00:18:51,100
the more light that you're
actually gonna receive.
413
00:18:51,100 --> 00:18:52,366
Some of these observations
414
00:18:52,366 --> 00:18:55,733
may be in the order
of two or three hours
415
00:18:55,733 --> 00:18:58,466
and some are up to
20, 25, 30 hours.
416
00:18:58,466 --> 00:18:59,866
- [Myrna] So where
are we in the process
417
00:18:59,866 --> 00:19:01,166
of getting this data?
418
00:19:01,166 --> 00:19:02,733
- We're at the tip
of the iceberg.
419
00:19:02,733 --> 00:19:06,200
We were very successful
in conserving fuel,
420
00:19:06,200 --> 00:19:09,666
so we anticipate having
a 20-year fuel budget
421
00:19:09,666 --> 00:19:13,800
which will allow us to
do imaging and so forth
422
00:19:13,800 --> 00:19:15,233
as long as the instruments
423
00:19:15,233 --> 00:19:18,033
are able to allow
us to take data.
424
00:19:19,533 --> 00:19:22,200
- Over here is actually
one of the main places
425
00:19:22,200 --> 00:19:25,366
that we align the
telescope from.
426
00:19:25,366 --> 00:19:29,266
And up here you can see, we
call it the commissioning flow.
427
00:19:29,266 --> 00:19:32,833
These are all the steps that
we did to align the telescope
428
00:19:32,833 --> 00:19:34,800
over about a three month period.
429
00:19:34,800 --> 00:19:36,666
As we went through
the entire process,
430
00:19:36,666 --> 00:19:38,566
you know we X'd them all out.
431
00:19:38,566 --> 00:19:40,833
And there's one particular
step in the middle there
432
00:19:40,833 --> 00:19:43,766
where we got the very first
images that were focused
433
00:19:43,766 --> 00:19:45,100
and that's why it says champagne
434
00:19:45,100 --> 00:19:46,666
because after all those years,
435
00:19:46,666 --> 00:19:48,933
that was the moment we knew
we built the right telescope.
436
00:19:48,933 --> 00:19:50,566
- Wow, the moment to celebrate?
437
00:19:50,566 --> 00:19:52,133
- The moment to celebrate.
438
00:19:52,133 --> 00:19:54,333
When you look at it from
the 20,000 foot level,
439
00:19:54,333 --> 00:19:55,800
things went amazingly well,
440
00:19:55,800 --> 00:19:58,266
probably better than
any of us expected.
441
00:19:58,266 --> 00:20:00,233
And the thing that
was really special
442
00:20:00,233 --> 00:20:02,766
is that when we got to
the final performance,
443
00:20:02,766 --> 00:20:06,433
it's almost performing twice
as well as we expected.
444
00:20:06,433 --> 00:20:08,700
- [Myrna] So why is this
so important to you, Lee?
445
00:20:08,700 --> 00:20:10,166
- These kinds of missions,
446
00:20:10,166 --> 00:20:12,733
these missions that
bring back amazing images
447
00:20:12,733 --> 00:20:16,800
and help us understand how
we got here, they inspire.
448
00:20:16,800 --> 00:20:18,333
They inspire young people
449
00:20:18,333 --> 00:20:19,766
and I think that's
what it's all about.
450
00:20:19,766 --> 00:20:23,033
It shows what human beings
are capable of doing
451
00:20:23,033 --> 00:20:24,233
when we work together.
452
00:20:24,233 --> 00:20:26,066
And maybe that's a
lesson that we can apply
453
00:20:26,066 --> 00:20:28,266
to other challenges that
we have here on Earth.
454
00:20:28,266 --> 00:20:30,766
- It's so inspiring
for science in general.
455
00:20:30,766 --> 00:20:32,533
- We could be
learning new physics,
456
00:20:32,533 --> 00:20:34,233
physics that then relates
457
00:20:34,233 --> 00:20:36,133
to what's happening
here on the earth.
458
00:20:36,133 --> 00:20:39,000
We still have a lot
of the universe that
we don't understand
459
00:20:39,000 --> 00:20:41,333
from dark energy to dark matter
460
00:20:41,333 --> 00:20:44,533
and the Webb telescope will
contribute to that as well.
461
00:20:44,533 --> 00:20:46,666
It's been a little over
a year and of course,
462
00:20:46,666 --> 00:20:48,166
you know we've come really far
463
00:20:48,166 --> 00:20:51,033
in terms of how well it's
performing, getting it operating
464
00:20:51,033 --> 00:20:53,266
but from a science perspective,
465
00:20:53,266 --> 00:20:54,900
we're really just getting going.
466
00:20:54,900 --> 00:20:57,133
From now on, every
field is a deep field
467
00:20:57,133 --> 00:20:59,733
and that's sort of
the way it's been.
468
00:20:59,733 --> 00:21:01,700
This is gonna be a very
exciting few years,
469
00:21:01,700 --> 00:21:03,833
maybe some of the most
exciting few years
470
00:21:03,833 --> 00:21:06,433
in the history of
understanding our universe.
471
00:21:06,433 --> 00:21:09,200
- The telescope is
built, deployed,
472
00:21:09,200 --> 00:21:12,100
and the science is rolling
in, the data is epic.
473
00:21:13,166 --> 00:21:15,000
So you were the
principal investigator
474
00:21:15,000 --> 00:21:17,066
for that first batch of images,
475
00:21:17,066 --> 00:21:19,633
how were those images
received by the public?
476
00:21:19,633 --> 00:21:21,333
- It was a very
interesting process,
477
00:21:21,333 --> 00:21:24,100
it took us years to
prepare for this.
478
00:21:24,100 --> 00:21:27,566
And of course, we had
this task of demonstrating
479
00:21:27,566 --> 00:21:32,666
to the world that
this $10 billion
observatory was worth it.
480
00:21:33,300 --> 00:21:36,100
That we could produce something
that anybody would look
481
00:21:36,100 --> 00:21:39,000
at and say, wow, this gotta
be making amazing science.
482
00:21:39,000 --> 00:21:42,566
And that included producing
these beautiful color images.
483
00:21:42,566 --> 00:21:44,233
And so, of course, we
were worried about that.
484
00:21:44,233 --> 00:21:46,633
We were nervous, I mean,
can we actually do that?
485
00:21:46,633 --> 00:21:49,133
We didn't know what the
images would look like.
486
00:21:49,133 --> 00:21:50,933
Like this is such
a new observatory
487
00:21:50,933 --> 00:21:52,966
with such new capabilities,
488
00:21:52,966 --> 00:21:55,100
that we could try and
predict what we would see
489
00:21:55,100 --> 00:21:56,900
but we couldn't
really predict it.
490
00:21:56,900 --> 00:21:59,400
And all the data that
the observatory takes
491
00:21:59,400 --> 00:22:01,566
really is the
property of the world.
492
00:22:01,566 --> 00:22:03,566
And so, eventually
it all becomes public
493
00:22:03,566 --> 00:22:04,933
and anybody can
download the data
494
00:22:04,933 --> 00:22:06,933
and you don't even
have to be a scientist
495
00:22:06,933 --> 00:22:09,100
to download the images
and look at them.
496
00:22:10,166 --> 00:22:12,333
- So Klaus, you saw
the first images
497
00:22:12,333 --> 00:22:15,000
as they were coming down
from this telescope.
498
00:22:15,000 --> 00:22:17,466
- Right, I saw the
first color images,
499
00:22:17,466 --> 00:22:21,100
the first science images that
we took, the ones you've seen.
500
00:22:21,100 --> 00:22:25,933
For example, the cosmic cliffs
or the first deep field.
501
00:22:25,933 --> 00:22:29,666
The primary feeling I had
was really of loneliness
502
00:22:29,666 --> 00:22:31,333
because the first
image came down,
503
00:22:31,333 --> 00:22:32,700
it was sort of late at night.
504
00:22:32,700 --> 00:22:34,333
I didn't download it
here in the office,
505
00:22:34,333 --> 00:22:36,566
I actually downloaded it
in my basement at home.
506
00:22:36,566 --> 00:22:39,766
So I was sitting there this
evening in my basement all alone
507
00:22:39,766 --> 00:22:43,133
and I was looking at this
image of the deepest view
508
00:22:43,133 --> 00:22:45,233
of the universe that
anybody had seen
509
00:22:45,233 --> 00:22:46,766
and it was profound loneliness
510
00:22:46,766 --> 00:22:48,766
because I couldn't
share it with anybody.
511
00:22:50,100 --> 00:22:53,400
- So the colors are gorgeous
and what do they mean?
512
00:22:53,400 --> 00:22:55,800
- So the colors mean
something physically.
513
00:22:55,800 --> 00:22:57,233
So when we pick a filter,
514
00:22:57,233 --> 00:22:59,700
what that does is it actually
picks out a signature
515
00:22:59,700 --> 00:23:02,933
of a specific molecule
or a specific element.
516
00:23:02,933 --> 00:23:06,333
So here I have pulled up
an image that uses a filter
517
00:23:06,333 --> 00:23:09,000
that sees organic molecules.
518
00:23:09,000 --> 00:23:13,433
So 4.6 billion years ago, our
solar system looked like that.
519
00:23:13,433 --> 00:23:15,600
All this stuff
around you see here,
520
00:23:15,600 --> 00:23:18,000
that's the organic material
that we are made of
521
00:23:18,000 --> 00:23:20,133
that ends up on the
planets in there.
522
00:23:20,133 --> 00:23:22,533
- [Myrna] It makes me feel
like I'm part of the universe.
523
00:23:22,533 --> 00:23:25,633
- Oh, you are very much
part of the universe, right?
524
00:23:25,633 --> 00:23:26,766
As Carl Sagan said,
525
00:23:26,766 --> 00:23:29,500
"We're the universe's way
of thinking about itself."
526
00:23:30,666 --> 00:23:33,233
- So we're starting
to get this data now,
527
00:23:33,233 --> 00:23:35,866
is it creating more
questions than answers?
528
00:23:35,866 --> 00:23:36,200
- Oh yes,
529
00:23:37,033 --> 00:23:38,266
it's creating more questions
than answers, absolutely.
530
00:23:38,266 --> 00:23:40,266
And I think that's where
we want to be, right?
531
00:23:40,266 --> 00:23:42,566
If we are starting to
run out of questions,
532
00:23:42,566 --> 00:23:43,700
we are not doing
something right,
533
00:23:43,700 --> 00:23:45,200
that's not how science works.
534
00:23:45,200 --> 00:23:49,100
We wanna answer questions but
we want to make more questions
535
00:23:49,100 --> 00:23:51,066
than we have answers.
536
00:23:51,066 --> 00:23:52,233
There'll be future telescopes
537
00:23:52,233 --> 00:23:53,500
because we need that to answer
538
00:23:53,500 --> 00:23:55,166
all those new questions we have.
539
00:23:56,566 --> 00:23:59,866
- You and so many people
have dedicated their careers
540
00:23:59,866 --> 00:24:00,866
to this project.
541
00:24:01,100 --> 00:24:04,400
How does it feel now that it's
up and it's running so well?
542
00:24:04,400 --> 00:24:08,466
- It's performing better than
expected across the board.
543
00:24:08,466 --> 00:24:11,500
And that is true in terms
of its lifetime expectancy,
544
00:24:11,500 --> 00:24:14,500
and its optical performance
is about a factor of two
545
00:24:14,500 --> 00:24:17,866
better than the
expected performance.
546
00:24:17,866 --> 00:24:20,966
How stable it is when
it looks at an image
547
00:24:20,966 --> 00:24:24,033
is about a factor of seven
better than expectations.
548
00:24:24,033 --> 00:24:25,600
So yeah, it's incredible
549
00:24:25,600 --> 00:24:27,766
to see how well it's
performing up there.
550
00:24:29,366 --> 00:24:31,333
- One of the great
things about science
551
00:24:31,333 --> 00:24:33,266
is that we learn new things
552
00:24:33,266 --> 00:24:35,566
and often those new
things that we learn
553
00:24:35,566 --> 00:24:37,966
overturn a previous idea.
554
00:24:37,966 --> 00:24:39,500
That's certainly
gonna be the case
555
00:24:39,500 --> 00:24:41,000
with the James Webb
Space Telescope.
556
00:24:41,000 --> 00:24:45,233
It sees the universe so much
more clearly, so much deeper,
557
00:24:45,233 --> 00:24:47,366
I think there's some
big surprises in store
558
00:24:47,366 --> 00:24:49,233
that James Webb will give us.
559
00:24:49,233 --> 00:24:51,133
- The Webb is giving humanity
560
00:24:51,133 --> 00:24:56,200
its very first high definition
view of the infrared universe
561
00:24:57,000 --> 00:24:59,400
and the view is fantastic.
562
00:24:59,400 --> 00:25:02,466
- The great thing that
I took away from Webb
563
00:25:02,466 --> 00:25:06,633
and being part of this project
is helping to build something
564
00:25:06,633 --> 00:25:10,866
that fundamentally contributes
to humanity's knowledge.
565
00:25:10,866 --> 00:25:14,566
- My dream is to continue
trying to do hard things.
566
00:25:14,566 --> 00:25:17,766
I love the idea that I've
gotten to work with a team
567
00:25:17,766 --> 00:25:21,666
that has enabled the science
classes that my kids will take
568
00:25:21,666 --> 00:25:24,266
aren't going to be the same
science classes I took.
569
00:25:24,266 --> 00:25:26,166
That's very exciting.
570
00:25:26,166 --> 00:25:28,900
- Building the first
segmented space telescope,
571
00:25:28,900 --> 00:25:31,600
this is sort of like
landing on the moon
572
00:25:31,600 --> 00:25:35,666
for telescopes in a sense
that it's the first of a kind
573
00:25:35,666 --> 00:25:37,866
but a segmented
telescope is scalable.
574
00:25:37,866 --> 00:25:39,400
We can build bigger and bigger.
575
00:25:39,400 --> 00:25:40,600
And then after that,
576
00:25:40,600 --> 00:25:42,400
we can think about
assembling telescopes
577
00:25:42,400 --> 00:25:44,933
that are made up of
segments like this.
578
00:25:44,933 --> 00:25:46,833
And that's what we're
gonna need someday
579
00:25:46,833 --> 00:25:50,933
if we wanna take an image
of a planet just like Earth
580
00:25:50,933 --> 00:25:53,533
around another star
in high definition.
581
00:25:53,533 --> 00:25:57,333
The Webb telescope is the
first step on that journey.
582
00:25:57,333 --> 00:25:59,400
- With its successful
launch and deployment,
583
00:25:59,400 --> 00:26:02,866
Webb is expected to support
scientific observation
584
00:26:02,866 --> 00:26:06,600
for about 20 years unveiling
the secrets of the universe
585
00:26:06,600 --> 00:26:08,766
one discovery at a time.
586
00:26:08,766 --> 00:26:11,733
All of us at Wings Over the
Rockies Air & Space Museum
587
00:26:11,733 --> 00:26:15,033
look forward to uncovering more
mysteries beyond our planet
588
00:26:15,033 --> 00:26:16,466
and sharing them with you.
589
00:26:16,466 --> 00:26:19,100
We'll see you next time
on "Behind the Wings".
590
00:26:19,566 --> 00:26:22,833
(bright upbeat music)
48225
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