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(light dramatic music)

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Venus.

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Other than the moon, it's the brightest object

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in the night sky.

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Captivating men and women for millennia.

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Named for the Roman goddess of beauty,

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the heavenly orb has an ugly side too.

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(thunder rumbling)

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It's a very hellish place.

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Sulfuric acid at the surface.

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Seems to be an inherently volcanic world

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with an atmosphere that ran amok.

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But Earth's sister planet

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may not have always been so inhospitable.

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We think that Venus may once have looked more

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like Earth in the past.

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Now, after decades of neglect,

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planetary scientists turn their attention

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back to the solar system's second planet.

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To unlock secrets of our world's past,

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and perhaps what's ahead.

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Venus is the once and future Earth.

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Prepare to voyage to Venus.

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{\an8}(dramatic whooshing)

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{\an8}(light dramatic music)

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Okay, Peter, we copy.

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We are proceeding into the IOSPI lock checkup.

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NASA is heading out into deep space once again.

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With an initial price tag of $500 million each,

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two new programs, DAVINCI+ and VERITAS,

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will launch planetary probes designed

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to visit Venus within a decade.

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{\an8}We hope these missions will further our understanding

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{\an8}of how Earth evolved and why it's currently habitable

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when others in our solar system are not.

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By gathering new data about Venus,

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scientists also expect to learn about Earth

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and the evolution of life.

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Two rocky bodies, roughly the same size,

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astronomical next door neighbors

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both formed about four and a half billion years ago.

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How did two worlds with so much in common

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become so different?

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It's this amazing cosmic accident, right?

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{\an8}That we have two planets that are so much alike.

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{\an8}It's like every scientist's dream that you have

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{\an8}like a control case.

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Venus is very special.

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She's the most Earth-like world

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that we know the least about.

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She has this massive atmosphere,

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an atmosphere that is 100 times that of Earth's,

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{\an8}which is layered and structured

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{\an8}and telling a story that we haven't read yet.

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Inspired by the Italian artist,

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Leonardo DaVinci, Garvin and the team created

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an acronym to name their mission

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and honor the original Renaissance man.

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I was always struck by him.

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His writings in science, engineering, art,

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all came together with imaginative creation.

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Some of which even look like spacecraft

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that could go to Venus.

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Fittingly, now one bearing his name,

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will make that journey.

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Currently scheduled to launch in 2029.

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The plans include a carrier spacecraft

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which will fly by Venus twice

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before releasing the descent probe,

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protected by a heat shield seven feet in diameter.

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That will carry us into that atmosphere,

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handle the peak heating of that entry

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and then jettison the heat shield

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so our probe will be exposed to the atmosphere

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in the upper clouds around 70 kilometers.

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And that's when our mission begins.

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That multi-pronged mission,

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to examine the elemental properties

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of the Venusian atmosphere, image and identify

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the character of the landscape,

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and ultimately land on the surface.

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We are sending what I like to call

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a flying rover chemistry lab.

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And it will be in the form of a special probe,

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not unlike a diving bell that you would need

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to go into the deep ocean.

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That vehicle is designed to handle environmental changes

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that go from super cold and almost no atmosphere

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to super hot and high pressure

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all in the period of about an hour.

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That's tough.

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(dramatic whooshing)
(light dramatic music)

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Three, two, one.
<v ->Almost 60 years ago,

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Mariner 2 rocketed planetary science into high gear

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when it became the first spacecraft to successfully

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visit another planet with a flyby of Venus.

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The Soviet Union's Venera Missions landed

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multiple probes on the surface.

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Brief encounters which exposed the planet's desolation.

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The Pioneer Multiprobe was the last American mission

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to enter and study the atmosphere of Venus in 1978.

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And the Magellan spacecraft, deployed from

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the Space Shuttle Atlantis in 1989,

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was the first to map the entire surface of Venus,

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revealing volcanic activity.

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However, Mars soon stole the spotlight

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of planetary exploration.

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In part, because of the greater engineering challenges

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presented by Venus.

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Venus presents a very tough challenge:

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a big atmosphere, hard to get into,

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hard to survive at the surface where the pressure

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and temperature are equivalent to being half a mile

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deep in the ocean at temperatures that are twice

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the temperature of your oven.

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But the success of the Mars programs

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serve as scientific building blocks

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and inform what's possible elsewhere.

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What we've done at Mars is shown the next generation

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of exploration techniques, instruments,

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vehicles, science questions, computing,

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models of states of past climates.

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We can now apply what we've learned in Mars

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and in Earth to Venus.

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What a perfect time.

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Including cutting edge capabilities

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ready to be employed by these two missions,

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VERITAS and DAVINCI+.

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This is the first full-scale titanium test unit

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of DAVINCI+, about a meter across.

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We've tested this to 450 degrees centigrade

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and have confirmation that our instruments inside this,

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which look like this at small scale

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all packed in there underneath this outer pressure vessel,

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will do well.

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You can see one of the inlet systems here

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that will be ingesting gases multiple times

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through the transect of the atmosphere, some in the clouds,

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and then every couple of hundred meters

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as we come out of the clouds.

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So we'll be literally tasting Venus all the way down,

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using a system like this.

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The five primary science instruments

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will work like the five senses of the human body.

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{\an8}(light music)

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{\an8}Two analytical spectrometers to pinpoint

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{\an8}the chemical composition of the atmosphere.

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The Venus Atmospheric Structure Investigation, or VASI,

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which will measure winds, pressure and temperature.

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A student experiment named VFox to investigate the cycle

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of small levels of oxygen in the atmosphere.

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{\an8}And the Venus Descent Imager, known as VENDI,

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{\an8}located at the bottom.

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{\an8}The instruments need to fit together almost

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{\an8}like jigsaw puzzles to make the most of the volume

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that we have within this very special envelope

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of our descent sphere.

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We're gonna take a lot of that instrument capability

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and apply it to the big questions about Venus.

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Questions that scientists

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have been posing for years.

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(grounds rustling)

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(light music)

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In many respects, the investigations of Mars and Venus

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are looking for the same thing:

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evidence of water, present today,

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or perhaps long long ago.

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We wanna understand if Venus, which we think of

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as Earth's evil twin, was more like her identical twin

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in the distant past.

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That means vast surface oceans

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that could have harbored life.

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While life on Earth was rising and evolving,

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it's possible that Venus was also a place

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that those processes could happen.

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We're gonna look for chemical fingerprints

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{\an8}that may indicate that Venus was once habitable in the past.

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{\an8}So, by reading these records on Venus today,

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we might be able to infer that Venus was a nice place

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to live in the past.

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Maybe a place that we'd wanna visit.

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Understanding Venus's story

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can aid the search for life outside our solar system,

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as astronomers discover new planets around other stars.

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By studying Venus and discovering if

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it was truly habitable, we might discover that

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the habitable zone boundaries are fuzzy.

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You know, maybe you can have habitability

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beyond those boundaries in ways that are surprising.

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High resolution images will help categorize

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the makeup of Venus's surface materials.

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We wanna look for things like granites.

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Granites are really interesting because, at least on Earth,

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they form from water-rock interactions

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and also cotton and building processes.

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(thunder rumbling)

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DAVINCI+'s camera work will include

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more than static landscapes.

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VENDI will create dynamic 3D relief models

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at an incredible meter in scale.

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Layering images taken all along its descent.

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A system already successfully tested

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by matching the probe's drop speed in a helicopter.

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VENDI will be looking out the south pole of the probe.

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What the team calls the Eye of Venus,

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a window made of sapphire.

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This little piece is a really important piece of hardware.

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We've tested this in Venus-relevant conditions

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and it works great.

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As the probe is falling through the atmosphere

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this is what the camera's gonna be looking through,

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and we're gonna get spectacular views of the surface.

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We're gonna be taking thousands of images

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all the way down to the surface.

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We're gonna be able to distinguish

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different mineral types.

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It is very exciting once we get below the cloud deck.

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You might think this is a small window,

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but I don't know, I looks pretty big to me.

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This is gonna be a new world exposed.

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If DAVINCI+ will explore Venus close-up,

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VERITAS, launching in 2028,

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will examine the planet from a distance in orbit.

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We will enhance the science that can be obtained

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from both missions by having these two missions together.

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So we can compare the visual images

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that they will take to our radar images

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and that will enhance our ability to interpret

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the radar images, just as the global context

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that we provide enhances their ability

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to interpret their local observations.

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Three decades ago, Smrekar collaborated

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on the successful Magellan mapping mission.

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Now using radar technologies developed to study Earth,

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VERITAS will return data from Venus

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100 times more detailed than its predecessors.

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The size that VERITAS wants to accomplish

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is looking at the planet holistically.

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We want to understand what makes rocky planets tick.

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We wanted to understand the geologic engine

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inside the planet, how that interacts with the surface,

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how it drives volcanism, how it drives faulting,

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and what that means for the atmosphere.

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Examining landscape features

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also found on Earth.

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Like fault lines, volcanic calderas and lava flows,

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and searching for evidence of subduction.

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That's when tectonic plates edge under one another

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into the hot molten interior.

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VERITAS will test theories about

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the formation of continents

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(light dramatic music)
VERITAS will help us

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tell Earth's origin story.

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That process of subduction led to

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the formation of continents.

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Continents may have changed the composition of the oceans.

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Ultimately, though,

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it's about the water here on Earth and there on Venus.

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So VERITAS will employ a spectrometer

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designed to see through the clouds and map rock composition.

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Also looking for granite, like here on Earth.

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By looking for the chemical fingerprints

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of continental analogs on Venus,

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we will also be pinning down that history of surface water.

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You know, we'll get a better idea of how old

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those continents are, if they have the right composition

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to have formed the presence of water.

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And we'll also look for water coming

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out of the interior today,

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that would be just hugely important for understanding

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the evolution of the history of water

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on the surface and in the atmosphere of Venus.

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But those ancient oceans are long since gone,

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and the teams of VERITAS and DAVINCI+ want to know why.

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Why the divergent pathway relative to our Earth?

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Why didn't she stay cool and neat and oceanic?

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What went wrong? What went right for her history?

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How can we disentangle that history?

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Because that's important.

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It may be that Venus is a magic mirror

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that's reflecting the future of Earth back to our planet.

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So these same processes involving, you know,

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the shutdown of geological activity as the planet cools.

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These are also gonna play out on Earth

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billions of years into the future.

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Understanding Venus better

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should cast light on Earth's present and future states, too.

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We can validate and improve our climate models

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that we're using to study climate change here on Earth

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by applying those models to Venus.

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The Venus system is different, it's a lot more extreme,

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but if our models, when we take them from Earth

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and we apply them to Venus, if they don't break,

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then that means those models are more robust.

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Some have theorized, as the oceans boiled away,

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microorganisms may have migrated to the upper levels

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of the cloud decks.

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In 2020, an international team of researchers

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announced the discovery of small levels of phosphene.

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A potential bio-signature in the Venusian atmosphere.

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Analysis was reached using Earth-based radio telescopes.

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Questions about the phosphene news persist,

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and even the lead researcher suggested

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the best way to test their results was to go to Venus.

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{\an8}So maybe the only thing to do is to send a spacecraft

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{\an8}that can really sample and see if there

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{\an8}are life forms there.

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Now that's something VERITAS and DAVINCI+

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will do, providing an unprecedented database to learn from.

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The experts that build the models

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can test their theories with real data.

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If there are intriguing chemical signatures there,

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we will be able to confirm that they are there,

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but also understand the context of the environment

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that we found them in.

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Piece that VERITAS will contribute to

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is understanding volcanism.

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That's one hypothesis that has been put forward

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as a way to produce phosphine in the atmosphere.

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For those involved with these new

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missions to Venus, the green lights

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validate years of persistence,

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passionate work and proposal refinements.

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Doing planetary science as a career

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takes a lot of patience and it takes a lot of fortitude.

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This is beyond words.

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We are so ready to bring Venus into focus for humanity

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because we think she has a story we have to tell.

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(light dramatic music)

