WEBVTT FILE

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(music throughout)

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Hi, I'm Doctor Marie Henderson,

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a planetary scientist at Goddard Space
Flight Center in Maryland.

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I love the moon.

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And so I became a planetary scientist.

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Study lunar volcanism and planetary
imaging.

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In addition to that,
I trained astronauts in lunar geology

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as one of the scientists on NASA's Artemis
two mission.

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The mission is due to launch early next
year, and it will be the first Artemis

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flight to the moon
and back with four astronauts on board.

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Our science team will support them
from Earth in real time as they make

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geological observations from the Orion
capsule with both their eyes and cameras.

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You'll learn more about the Artemis
two mission

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in the coming months, but for now,
I want to invite you to join me,

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NASA and explorers around the globe
and looking up

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and appreciating
our near celestial neighbor, the moon.

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As part of NASA's annual international
Observe the Moon Night.

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enjoy the upcoming show
where you'll learn more

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about the moon and NASA's
lunar science and exploration plans.

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I'm Reid Wiseman.

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And I'm Victor Glover.

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And this is how we pilot
the Orion spacecraft.

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What are the differences between
piloting an airplane and a spacecraft?

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I think the thing that I first think about

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is on a spacecraft,
it's really all about attitude.

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It's really not about thrust
and getting the airplanes flying faster.

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And the spacecraft is already going
almost 38, 39 times the speed of sound.

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So we're really controlling the attitude.
Where are we pointing?

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Where are we looking at out the windows,
where our antenna is pointing?

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The software is the primary flyer
of the spacecraft.

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I think that's the biggest difference,
especially for a, you know, a pilot coming

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into this who wants to get on the hand
controllers and, and put the aircraft

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or the spacecraft
in its proper attitude in aircraft.

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The software is really helping the pilot.

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And I think now it's almost like
we are helping the software.

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So a couple
of the things we're going to do on Artemis

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two right after liftoff,
we are going to detach the Orion

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spacecraft and service module from
the Interim Cryogenic Propulsion stage,

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which is just a lot of words
for our upper stage.

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During that,

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Victor will be physically flying
with a rotational hand controller,

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the translational hand controller, and
doing station keeping on this upper stage.

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This phase of the testing will be
to simulate the flying that we would do

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if we were docking to another spacecraft,
like our lander, or to our gateway.

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I think we should show you
how we actually control the vehicle.

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So we've been using

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terms like rotational hand
controller, rotational hand controller.

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We say RHC for short and translational
hang controller, THC for short.

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In an aircraft
you would have a stick in a throttle,

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but it's the things that you put
your hands on to control the spacecraft.

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We will pitch, roll and yaw.

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Those are the three axes
and each direction.

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And then we will also go
up, down, left, right, in and out.

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And we will assess how precisely
that we can control the spacecraft.

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But we mentioned

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earlier that the main controller
of the spacecraft is software.

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And so the main way that we interact with

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the spacecraft
is our cursor control device.

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Your another favorite.

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I know you love CCD. This thing.

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It looks awkward. It looks weird.

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But when you get to use it,
it is actually a genius piece of gear.

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And I know it is your favorite.

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Oh it is.

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This is our primary way
to interact with the spacecraft.

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And so what it does
is it allows us to determine

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where we put our focus on the display.

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So I can move the cursor
to a certain display.

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And then I can move the cursor around
to interact with certain fields of data.

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And it's one of the primary controllers,
because there are going to be times

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when we're under 4G, 8G, maybe even,

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and we won't be able to lift up our hands
and push the buttons on the display.

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So this is exactly how we will do it.

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There is far more information
on these displays than we will need to

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to fly this spacecraft normally,
but if a system goes off,

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if something goes wrong,

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we can dig down into the lowest levels
of the computer of all the systems here,

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and we can take a look
to see what's failed.

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Talk to Mission Control in Houston.

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And then right next to the displays
you see switches and toggles and dials.

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And so we call those switch interface
panels or SIP panels.

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If the rotational and translational hand
controllers didn't work,

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we also have a
backup to a set of switches.

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Hi, my name is Jeff
Samarra and I work for Lockheed Martin.

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We're here in the Exploration Development
Laboratory, where we do integrated

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testing and verification and GNC fights
software for the Artemis program.

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GNC stands for guidance, Navigation
and Control.

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Guidance is basically
where do we want to go?

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Nav is where are we controls?

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How do we get where we are,
where we want to be?

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This is the software that interfaces
with both the translational

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and rotational hand controls.

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We call

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this whole stack up the crew
and service module or the CSM.

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That is the crew module,
the capsule, the spacecraft Orion,

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and then the service module made
by our partners ESA and Airbus in Europe.

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And so this is where the thrusters that
will maneuver us on the service module.

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My name is Hashid Amikan

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I am the lead of assembly integration
test team of Airbus.

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And we built the European service
module in Germany.

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When the astronaut
gives the command to go in any direction.

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The software is steering
every thrusters as needed.

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So it's a balance or a dance
between the different engines.

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So if you provide thrust on one side,
you have to counteract.

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And on the other side,

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every time you touch
the translational hand

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controller or the rotational hand
controller, those thrusters fire.

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And those thrusters are right near us.

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And you can hear a bang and it's like,
bang, bang, bang, bang.

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As you're flying this thing around,
you hear it and feel it.

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And even though it's quite well shielded
and that we're in suits and other

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things, you're still going to hear
and feel those thrusters when they fire.

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It's pretty neat.

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I cannot wait until one of us
takes controls and just steers

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this thing around
and looks out at the earth.

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We'll be farther from the earth than human beings have been in a very long time.

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Let's go, let's go.

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And liftoff of Artemis one.

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We rise together back to the moon

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and beyond.

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I'm not used to talking about trees.

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Like rocks.

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Easier seeds represent
the most optimistic of our species.

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Given our reliance on wood

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from raw material for a home
to a baseball bat and now spacecraft.

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Planting
a seedling is an investment in our future.

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The tree may not bring you fruit, but
it will bring future generations of fruit.

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In 1962.

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President Kennedy said these words
we meet in an hour of change and challenge

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and a decade of hope and fear and an age
of both knowledge and ignorance.

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The greater of our knowledge increases,
the greater of our ignorance unfolds.

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Artemis one continued
in the grand tradition of what Artemis

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two astronaut Victor Glover suggested
during his visit to Goddard.

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As vessels of humanity,

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that we take our culture with us
into the cosmos, that we should choose

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to take seeds and plant them
for future generations to enjoy.

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To remind us, earthbound explorers, that

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despite the problems we face here, we
remain connected to our future in space.

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I'm hopeful
that our all of our shared work on Artemis

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missions will bring similar
fruit to future generations.

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Hi, I'm NASA astronaut Tracy Dyson,

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orbiting 260 miles above the Earth aboard
the International Space Station.

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Tonight is time to come together
to appreciate and observe our shared moon.

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We are blessed on
the ISS to be able to observe the moon

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from space being situated
over the Earth's atmosphere.

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It's quite a sight to behold.

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The effect of the moon is most dramatic
for us over large bodies of water.

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When the moon is full, it illuminates
the whole surface of the earth

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and the ocean glistens
with a beautiful soft glow.

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Contrast that with the new moon,

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and the oceans are as black
as a starless universe.

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It's almost as if the Earth disappears.

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It's crazy.

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Wherever the moon is in its face,
when spotted, you can hear

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someone say from the cupola,
come look at this moon.

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So my crewmates and I are excited
to contribute to work that is stepping

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stone toward NASA's return to the moon
through the Artemis program.

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Stay curious and keep looking up.

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Three.

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Two. One.

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Every year,

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at the end of October

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there is a very special night in Spain

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It's a night when dozens of astronomical associations
take their telescopes out onto the streets.

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We are talking about the Night of the Moon

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When, together, they all share their passion for the heavens

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People approach the telescopes, intrigued, curious.

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Is it here?

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Goodness, how cool!

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My goodness, what a blast, huh?

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Wow!

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Oh, how cool!

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How handsome!

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Wow, it looks perfect! It's amazing!

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Almost as if I were there!

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Man, it looks super cool!

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Cool!

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It’s super cool!

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Those are the craters of the Moon. Oh, really?

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Wow, what a blast!

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Wow, how cool!

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Look! Look! Look what the Moon looks like!

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Wow, how cool!

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Can you see the craters on the Moon?

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It's gorgeous!

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Amazing, huh?!

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How cool!

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Stand here

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Look over here. Wait wait.

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Look over there. Like this, with one eye.

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What do you see?

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The Moon

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The Moon, yeah?

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In prehistoric times

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we humans established a very close relationship with the sky.

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For hundreds of thousands of years,

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when we had not yet invented writing,

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the calendar or the compass,

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reading the sky allowed us to locate ourselves in space and time.

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Knowing the sky was simply a matter of survival.

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We have lost this close relationship we had with heavens.

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And yet, looking at it, understanding it and studying it,

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continues to move and touch us.

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Man, what a blast!

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It just doesn't seem real.

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Hi, I'm Zena from the German
Aerospace Center in Cologne,

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and my favorite way to observe
the moon is from my balcony.

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In 2009, NASA
launched the Lunar Reconnaissance Orbiter,

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a bold mission
to map our moon in such detail

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that future crewed and robotic
missions could not only land safely,

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but also go to scientifically
important locations.

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With the start of the Artemis missions.

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The future is now as NASA prepares
to send humans to the lunar south pole.

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This region is of

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particular scientific interest
because it features areas of extended sun.

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That illumination and permanent shadow
is known to contain resources like water,

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and sits on the rim of the oldest impact
crater in the Earth-Moon system.

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Over the years, LRO, a suite of scientific
instruments, has delivered

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his promised, giving us incredible
new views and data on this terrain,

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helping us
build a roadmap for exploration.

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So follow this series
as we take a look at how the LRO mission

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is laying the groundwork
for Artemis science.

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One of the instruments on

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LRO is the Lunar Orbiter Laser
Altimeter, or Lola.

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It provides
topographic data on the lunar surface,

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revealing slopes and surface roughness,
helping us create models of lunar gravity

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and surface brightness, as well as high
resolution 3D maps of the moon.

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In this visualization,
the colors correspond to different

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elevations found amongst the craters
and mountains of the South Pole region.

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Having accurate elevation data
is essential for landing site selection.

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Surface navigation.

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Identifying areas
where resources can be found

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and planning
the design of future lunar infrastructure.

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In addition, studying the elevation
and topography

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of the moon contributes
to scientific research

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about its geological history,
formation processes, and ongoing changes.

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By analyzing elevation data.

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Scientists can learn more about the moon's
past volcanic activity, impact

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history, and tectonic processes.

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The global

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terrain mapping by Lola
also makes it possible to simulate

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sunlight and shadow on the moon
at any date, in the past or future.

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Here we see a visualization of the region
in 2028, depicting the changes

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in shadowing in two hour intervals
over the course of the year.

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This information is vital to Artemus
for planning exploration endeavors,

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since the low sun angles
and terrain of the South Pole produce

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a uniquely challenging
lighting environment.

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In the years since LRO was launched,

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there have been over 60,000 orbits
of the spacecraft

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and 10 billion laser shots
at the lunar surface,

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making those data a vital resource
for both human and robotic

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explorers that arrive at the South Pole
in the coming years.

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It's one piece in
how LRO is helping NASA usher

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in a new generation of lunar science.

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And I'm David.

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Here we are in Melbourne
and we like to observe the moon

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00:18:07.533 --> 00:18:10.533
reflecting off the Yarra River
in Melbourne.

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NASA's Artemis two

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00:18:13.766 --> 00:18:17.266
is the first crewed lunar mission
in over 50 years

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for astronauts will venture around
the moon, preparing humanity

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00:18:21.266 --> 00:18:25.766
for a long term lunar presence
for scientific discovery and exploration.

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00:18:28.666 --> 00:18:30.700
The ten day test flight will demonstrate

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a range of deep space
exploration capabilities with crew.

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The mission will prove the Orion
spacecraft is ready to keep astronauts

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alive in deep space,
and allow the crew and ground teams

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to practice operations
essential to the success of future

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missions.

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On launch day, the Artemis

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two crew suits up, undergoes final checks
and rides, and the crew transportation

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vehicles to launch pad 39 B at NASA's
Kennedy Space Center in Florida.

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Stacked on the mobile
launcher, NASA's 322ft tall

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cells, or Space Launch System rocket
with the Orion spacecraft awaits the crew

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00:19:10.133 --> 00:19:12.966
having made its four mile journey
from the Vehicle Assembly

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Building
on the crawler transporter to the pad.

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00:19:16.833 --> 00:19:18.600
The launch team fills the SLS

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00:19:18.600 --> 00:19:22.366
propellant tanks with over
700.000 gallons of liquid oxygen

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00:19:22.366 --> 00:19:26.500
and liquid hydrogen and verifies
guidance, communications, and avionics.

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00:19:27.100 --> 00:19:30.900
At 12 seconds before liftoff,
the hydrogen burn off Igniters fire.

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00:19:31.233 --> 00:19:35.200
About six seconds later,
the rocket's four Rs 25 engines ignite.

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When the countdown reaches zero.

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The umbilical retract,

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giving SLS and the crew in Orion
the clearance to begin the journey.

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00:19:47.300 --> 00:19:50.400
The 6
million pound moon rocket produces 8.8

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00:19:50.400 --> 00:19:53.433
million pounds of thrust to accelerate
toward space.

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75% of this power comes from the 217 story
solid rocket boosters,

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00:19:59.533 --> 00:20:02.666
each producing 3.6
million pounds of thrust.

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00:20:07.966 --> 00:20:10.433
About two minutes
when the boosters are released,

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00:20:10.433 --> 00:20:14.633
their solid propellant
consumed the core stage and its Rs 25

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00:20:14.633 --> 00:20:18.300
engines continue to propel Orion
and the crew to space.

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After three minutes,
the protective fairings surrounding

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Orion's service module are ejected,
exposing its solar arrays.

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00:20:28.866 --> 00:20:32.366
Six seconds later, the launch abort system
is ejected from Orion.

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00:20:32.666 --> 00:20:35.766
The crew has safely reached Earth orbit,
though they could still abort

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00:20:35.800 --> 00:20:38.800
using service module engines.

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About eight minutes after launch,
the SLS core stage engines shut down

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00:20:43.700 --> 00:20:46.700
and the Interim Cryogenic
Propulsion Stage, or ICPS

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00:20:46.700 --> 00:20:49.600
and Orion separate from the core stage.

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Orion and the ICPS are now flying free.

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00:21:01.366 --> 00:21:04.166
Orion's four solar arrays deploy, powering

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00:21:04.166 --> 00:21:07.766
the spacecraft and charging its batteries
for when it moves out of direct sunlight

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00:21:07.766 --> 00:21:10.766
during the journey to the moon and back.

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After a 90 minute orbit,
the engine of the rocket's upper stage

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00:21:17.200 --> 00:21:20.900
or ICPS, ignites
to raise Orion to a high Earth orbit.

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00:21:22.133 --> 00:21:24.000
The Artemis two crew and mission control

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00:21:24.000 --> 00:21:27.400
in Houston
then began a nearly 24 hour systems check.

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00:21:27.566 --> 00:21:31.866
While the astronauts are still relatively
close to Earth, familiarizing themselves

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with their new home
for the next several days.

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Once in high

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00:21:49.366 --> 00:21:52.366
Earth orbit,
Orion separates from the upper stage.

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00:21:52.533 --> 00:21:57.766
The expended ICPS and Orion stage adapter
serve as a target for a manual handling

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00:21:57.766 --> 00:22:00.900
test called the Proximity Operations
Demonstration.

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Preparing future

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00:22:02.200 --> 00:22:06.033
crews for rendezvous, docking,
and undocking with other spacecraft.

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During the demonstration, Artemis

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00:22:09.466 --> 00:22:12.833
two astronauts use cameras
and line of sight through Orion's windows

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00:22:12.833 --> 00:22:15.833
to pilot the spacecraft
as they approach and back away.

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00:22:16.000 --> 00:22:19.366
Assessing Orion's handling
qualities, hardware and software.

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00:22:25.366 --> 00:22:25.800
Following

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00:22:25.800 --> 00:22:29.333
the demonstration, spacecraft
data is collected to verify system

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00:22:29.333 --> 00:22:32.866
performance, such as life support,
communications, and navigation,

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00:22:33.133 --> 00:22:36.133
ensuring Orion and the crew are ready
for the voyage ahead.

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00:22:43.166 --> 00:22:46.533
About 23 hours
later, Orion's service module performs

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00:22:46.533 --> 00:22:50.966
the Trans Lunar Injection Burn,
or TLI, pushing Orion out of Earth orbit

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00:22:50.966 --> 00:22:53.966
and on an approximately four day
trip to the moon.

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00:22:54.266 --> 00:22:56.900
Ultimately, the crew's figure eight flight
path extends

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00:22:56.900 --> 00:22:59.900
more than 230,000 miles from Earth.

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00:23:01.233 --> 00:23:04.900
During the trip, the astronauts continue
to evaluate the spacecraft's systems

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00:23:04.900 --> 00:23:07.900
and practice emergency procedures
like testing the radiation

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00:23:07.900 --> 00:23:10.900
shelter.

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00:23:12.966 --> 00:23:13.466
The Artemis

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00:23:13.466 --> 00:23:16.900
two crew travels about 4600 miles
beyond the moon,

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00:23:17.066 --> 00:23:21.666
becoming the first humans to lay eyes
on the lunar far side in over 50 years.

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00:23:22.066 --> 00:23:25.700
Their observations will help us prepare
for future missions at the moon.

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00:23:26.566 --> 00:23:29.500
During this period,
there will be an anticipated communication

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00:23:29.500 --> 00:23:32.500
blackout between mission control
and the spacecraft

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00:23:33.300 --> 00:23:35.900
as the crew returns
from the far side of the moon.

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00:23:35.900 --> 00:23:39.033
Orion is drawn home
by Earth's gravity in a free return

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00:23:39.033 --> 00:23:42.166
trajectory,
ensuring a fuel efficient four day trip.

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00:23:53.866 --> 00:23:55.533
Before entering the atmosphere.

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00:23:55.533 --> 00:23:58.533
Orion's crew module separates
from the service module.

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00:24:00.433 --> 00:24:03.466
12 thrusters
ensure Orion is properly oriented

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00:24:03.466 --> 00:24:06.766
at an altitude of about 75 miles
from Earth's surface.

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00:24:13.700 --> 00:24:16.800
Orion and the crew enter
Earth's atmosphere at a speed of nearly

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00:24:16.800 --> 00:24:22.166
25.000mph. decelerating at a rate
up to four times the force of gravity.

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00:24:22.300 --> 00:24:25.300
The crew will feel four times
heavier than they do on Earth.

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00:24:25.866 --> 00:24:28.500
Orion's heat shield protects
the spacecraft from temperatures

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00:24:28.500 --> 00:24:31.700
of about 5000°F, about half as hot

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00:24:31.700 --> 00:24:34.700
as the surface of the sun.

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00:24:35.666 --> 00:24:36.933
To slow its descent,

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00:24:36.933 --> 00:24:40.600
Orion begins a precise deployment sequence
of 11 parachutes.

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00:24:41.033 --> 00:24:43.733
Three forward bay cover parachutes
first separate

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00:24:43.733 --> 00:24:46.733
the protective thermal cover
that sits over the ship's

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00:24:48.000 --> 00:24:51.666
two drogues, slow and stabilized
the crew module, then cut free.

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00:24:52.133 --> 00:24:54.833
Three pilot chutes lift
the three main parachutes,

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00:24:54.833 --> 00:24:59.433
deployed at an altitude of 9000ft
and traveling 130mph.

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00:24:59.900 --> 00:25:04.233
These should slow the crew module
to a speed of less than 20mph.

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00:25:06.400 --> 00:25:07.666
After traveling more than

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00:25:07.666 --> 00:25:11.566
595.000 nautical miles. Orion splashes

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00:25:11.566 --> 00:25:15.266
down in the Pacific Ocean, about 50
nautical miles from the California coast.

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00:25:15.433 --> 00:25:20.100
Just 16 minutes after entering
Earth's atmosphere after splashdown,

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00:25:20.100 --> 00:25:24.733
a recovery team that includes the US Navy,
Air Force and NASA approaches Orion.

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00:25:25.033 --> 00:25:26.633
The team ensures it's safe for the crew

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00:25:26.633 --> 00:25:30.566
to exit before divers help the astronauts
onto an inflatable front porch,

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00:25:30.800 --> 00:25:33.800
hoist them into helicopters
and fly to the recovery ship.

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00:25:35.000 --> 00:25:38.500
Orion is towed into the ship
for its return to Kennedy Space Center.

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00:25:38.833 --> 00:25:41.366
Their mission complete,
the crew is flown back to land

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00:25:41.366 --> 00:25:44.533
and step on solid ground
for the first time in ten days.

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00:25:45.433 --> 00:25:46.800
This is Artemis.

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00:25:46.800 --> 00:25:49.433
To learn more about Artemis at NASA.

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00:25:49.433 --> 00:25:51.900
Dot gov slash Artemis.

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00:25:51.900 --> 00:25:53.633
Aloha.

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00:26:01.300 --> 00:26:02.800
There’s been

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00:26:02.800 --> 00:26:05.800
a lot of excitement
about space suits lately.

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00:26:07.300 --> 00:26:10.400
But what about that iconic puffy
marshmallow suit that we used

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00:26:10.566 --> 00:26:12.200
to walk on the moon?

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00:26:12.200 --> 00:26:16.200
This is what we call
an Extravehicular Mobility Unit, or EMU.

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00:26:16.333 --> 00:26:19.333
And these suits
truly are in a class of their own.

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00:26:20.033 --> 00:26:20.900
Since Apollo,

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00:26:20.900 --> 00:26:24.566
we've retooled and reimagined
what can be accomplished on a spacewalk.

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00:26:24.966 --> 00:26:29.100
And the current spacesuit that NASA uses
is based on a design that first flew

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00:26:29.100 --> 00:26:33.866
in 1981 through rigorous maintenance,
safety testing, and upgrades.

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00:26:34.100 --> 00:26:37.733
This suit has allowed us to perform
some incredibly monumental achievements

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00:26:38.200 --> 00:26:41.133
in space,
walk our way into the record books.

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00:26:41.133 --> 00:26:45.600
You may have all come on different ships,
but we're in the same boat now.

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00:26:46.000 --> 00:26:48.633
A space suit is not something
you simply wear.

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00:26:48.633 --> 00:26:51.633
It's more like an astronaut's
very own personal vehicle.

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00:26:51.833 --> 00:26:54.866
A spacesuit is basically
a self-contained environment.

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00:26:54.900 --> 00:26:58.133
It is a mini spacecraft
that is tightly wound around

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00:26:58.133 --> 00:27:01.133
a human body, containing everything
they need to survive.

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00:27:01.400 --> 00:27:04.133
Because we are going back

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00:27:04.133 --> 00:27:07.466
to the moon
and on to Mars, exploration spacesuits

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00:27:07.466 --> 00:27:11.700
have to solve the challenges from the past
and anticipate those in the future.

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00:27:11.766 --> 00:27:15.800
Some of the biggest
environmental challenges that we're seeing

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00:27:15.866 --> 00:27:19.933
is finding a balance
between mobility and lunar dust.

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00:27:20.233 --> 00:27:22.966
In other words, exploration is dirty work.

396
00:27:24.266 --> 00:27:26.333
Looks like you guys have been playing
and I call them.

397
00:27:26.333 --> 00:27:28.933
I don't know how
we will get it all to the best we can.

398
00:27:28.933 --> 00:27:30.166
Yeah, like,

399
00:27:30.166 --> 00:27:33.200
how are we going to clean these guys off
before they're allowed to go back inside?

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00:27:33.233 --> 00:27:34.900
There's many ways.

401
00:27:34.900 --> 00:27:37.566
And do we know if they work?
We have to find out.

402
00:27:37.566 --> 00:27:40.800
And when your life depends on a good seal
and perfectly performing

403
00:27:40.800 --> 00:27:43.800
fabrics, dust is kind of a big deal.

404
00:27:44.833 --> 00:27:45.600
Lunar regolith.

405
00:27:45.600 --> 00:27:49.533
It looks like it's it's
just a fine grained material.

406
00:27:49.533 --> 00:27:52.033
When you when you see the pictures
of the Apollo boots and it and stuff.

407
00:27:52.033 --> 00:27:56.566
But, you're going to see anywhere
from broken rock shapes

408
00:27:57.266 --> 00:27:59.766
to fractured glass shapes.

409
00:27:59.766 --> 00:28:01.433
That's what it looks like
under the microscope

410
00:28:01.433 --> 00:28:05.166
of such a small particle size range
that it gets in everything.

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00:28:05.500 --> 00:28:08.233
The Apollo
missions only needed their suits to last

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00:28:08.233 --> 00:28:11.266
for a few moonwalks,
but these missions to the Moon

413
00:28:11.266 --> 00:28:15.200
and Mars could be weeks, months,
and even years long demanding

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00:28:15.200 --> 00:28:18.966
the most innovative solutions from NASA
and our industry partners.

415
00:28:19.366 --> 00:28:24.733
Whether we put a protective layer,
whether we are able to charge the suit

416
00:28:24.733 --> 00:28:29.866
to repel dust, there are multiple things
that we're looking at.

417
00:28:29.966 --> 00:28:32.500
So we still have a lot of challenges
and work.

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00:28:32.500 --> 00:28:35.933
The original EMUs were designed
for the astronauts of that era.

419
00:28:36.433 --> 00:28:39.900
Since then, our astronaut classes
have become far more diverse,

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00:28:39.900 --> 00:28:43.466
and the next generation of spacesuits
can follow well suit.

421
00:28:44.633 --> 00:28:45.233
As NASA

422
00:28:45.233 --> 00:28:49.433
works together with industry partners
on exploration spacesuits, follow along

423
00:28:49.466 --> 00:28:52.466
and be part of our journey to the moon

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00:28:52.533 --> 00:28:55.533
and beyond.

425
00:28:55.833 --> 00:28:58.833
Thank you so much for tuning in
to this year's International Observe

426
00:28:58.833 --> 00:29:02.533
the Moon Show, and for celebrating
the moon with us, wherever you may be.

427
00:29:02.866 --> 00:29:07.633
Wishing you clear skies and see you on
September 19th, 2026 for the next

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00:29:07.633 --> 00:29:09.600
International Observe the Moon Night.

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00:29:09.600 --> 00:29:12.600
See you later.
