WEBVTT - OSIRIS-REx: NASA's Journey to the Netherworld

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<v Speaker 1>Welcome to stuff to blow your mind from housetop were

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<v Speaker 1>On September eight, Osirius REX will launch from Cape Canaveral.

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<v Speaker 1>It will orbit the Sun for a year, then use

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<v Speaker 1>Earth's gravitational field to assist it on its way to

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<v Speaker 1>the asteroid Bayning, utilizing a complex thruster array to match

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<v Speaker 1>its speed, rendezvous with the ancient rock and steal a sample,

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<v Speaker 1>and then return home. The name OSIRIS stands for Origins

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<v Speaker 1>Spectral Interpretation, Resource Identification, Security Regular Explorer or Osiris REX.

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<v Speaker 1>But you really can't name a craft like this after

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<v Speaker 1>the ancient Egyptian god of the afterlife and transition and

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<v Speaker 1>not expect us to ruminate on it. A god torn

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<v Speaker 1>to pieces and scattered across the cosmos by set, forced

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<v Speaker 1>to descend into the underworld, but not before conceiving a

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<v Speaker 1>miraculous child with isis ensuring the birth of Horace, God

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<v Speaker 1>of Kings, for ages to follow. Because what are asteroids

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<v Speaker 1>but the scattered remnants of the building blocks that are

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<v Speaker 1>created into planetary form and eventually planetary life as we

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<v Speaker 1>know it. They're shards of the nether age in our

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<v Speaker 1>Solar system, and in the case of the Venue asteroid

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<v Speaker 1>a shard that has been witnessed to the Solar System's birth,

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<v Speaker 1>and a shard that might even bring death or at

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<v Speaker 1>least phoenix like rebirth to life on Earth. Hey, welcome

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<v Speaker 1>to Stuff to blow your mind. My name is Robert

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<v Speaker 1>Lamb and my name is Christian Sager. We have a

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<v Speaker 1>special episode for you today where we are going to

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<v Speaker 1>be talking about the NASA Osyrius REX mission. For the

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<v Speaker 1>first part of the episode, Robert and I are going

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<v Speaker 1>to present to you the information about this mission. Uh

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<v Speaker 1>and in particular asteroid Baynu, which is traveling to and

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<v Speaker 1>then the latter half, we were lucky enough to get

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<v Speaker 1>Dr Amy Simon to do an interview with us. She's

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<v Speaker 1>a senior scientist at NASA on planetary atmospheres and she's

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<v Speaker 1>working on the Osiris REX mission, and she gave us

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<v Speaker 1>some really good answers to some complex questions. Yeah, and

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<v Speaker 1>you know, we in the intro here we hit a

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<v Speaker 1>little bit on the the Egyptian mythology tie and both words,

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<v Speaker 1>you know, one is the god of the of transition

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<v Speaker 1>and the underworld, and the other is kind of the

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<v Speaker 1>menu is the name of kind of an Egyptian phoenix creature.

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<v Speaker 1>So that the question that instantly enters everyone's mind. I

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<v Speaker 1>think when you encounter acronyms like this is uh, is

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<v Speaker 1>it really as cool as Osiris rex sounds because it

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<v Speaker 1>sounds amazing. Cyrus Rex sounds like what the next dinosaur

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<v Speaker 1>in Jurassic World too will be called? Yeah, and I think,

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<v Speaker 1>but I think the answer is yes. This is a

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<v Speaker 1>really fascinating mission. I think it actually holds up rather

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<v Speaker 1>well to the mythic expectations are presented by the name.

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<v Speaker 1>And that's why we're discussing it here on the show.

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<v Speaker 1>So let's start off by getting into Beanu. What is

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<v Speaker 1>this thing? You may have heard about it recently, because

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<v Speaker 1>in the last two to three days before we're recording this,

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<v Speaker 1>there has been a flurry on the internet, especially on

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<v Speaker 1>science sites, of oh, is this asteroid going to hit

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<v Speaker 1>Earth in like a century or two, right, and then

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<v Speaker 1>the the counter headlines that are like, no, stupid, this

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<v Speaker 1>asteroid is not definitely gonna hit Earth. Yeah. Um. And

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<v Speaker 1>it's interesting because in those headlines you see our fear

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<v Speaker 1>rising up about the threat of near Earth objects. And

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<v Speaker 1>on one hand, I feel like people should be more fearful,

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<v Speaker 1>but people should I mean more to the point people

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<v Speaker 1>should be more aware of the long term risk posed

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<v Speaker 1>by near earth objects, like it should be a talking

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<v Speaker 1>point for for all political candidates and not just transhumanist candidates. Interesting. Yeah,

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<v Speaker 1>well especially at don't if you remember, but earlier this

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<v Speaker 1>year there was a meteoroid caught on film, like on camera.

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<v Speaker 1>Somebody whipped out their smartphone and caught one crashing into

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<v Speaker 1>Earth and it killed a person. And it was wow,

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<v Speaker 1>like just seeing something like that that was just so real,

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<v Speaker 1>really jaw dropping. Uh. And this is I mean, that

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<v Speaker 1>was tiny compared to Benu Benu is uh. Let me

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<v Speaker 1>see here a thousand, six hundred and fifty ft wide

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<v Speaker 1>or five meters. But according to the people at NASA,

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<v Speaker 1>we don't need to worry because that is well below

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<v Speaker 1>their calculations for what would cause like a mass extinction event. Yeah,

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<v Speaker 1>this isn't gonna be to the twenty till the twenty

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<v Speaker 1>second century, so there's plenty of time for us to

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<v Speaker 1>not worry about it. And it's gonna be a one

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<v Speaker 1>chants that it'll impact the Earth. But but more to

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<v Speaker 1>the point, it's just the general idea I think of,

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<v Speaker 1>like being aware of near earth objects in the threat

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<v Speaker 1>they posed learning more about those objects so that we

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<v Speaker 1>we we can potentially intercede and protect ourselves. I think

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<v Speaker 1>that is a very important issue for for humans in general. Yeah.

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<v Speaker 1>And when we talked to Dr Amy Simon later in

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<v Speaker 1>this episode, you know, she makes it clear this isn't

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<v Speaker 1>why they chose this particular asteroid, but yes, planetary defense

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<v Speaker 1>is a part of their mission. It is something that

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<v Speaker 1>the people that has to think about. So what do

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<v Speaker 1>we know about this asteroid? Well, near Earth asteroid is

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<v Speaker 1>a is a weird term, but it's It was formally

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<v Speaker 1>called it had a very generic name r Q thirty six. Uh. And,

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<v Speaker 1>as Amy tells us later on, they renamed it Banu

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<v Speaker 1>after a contest with students coming up with names. Yeah,

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<v Speaker 1>and uh. And I think there's one one in large

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<v Speaker 1>part because it ties into the Egyptian themes President Osiris. Yeah, yeah, exactly. Uh.

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<v Speaker 1>And what's important about it is it's carbon rich. Uh.

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<v Speaker 1>And because of that, it may contain clues to the

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<v Speaker 1>origins of life in the universe and especially here on Earth.

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<v Speaker 1>It's thought to be the remnant of the building blocks

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<v Speaker 1>that formed planets, so it might contain natural resources like water, organics,

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<v Speaker 1>or metals. Uh, and I realized as we were talking

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<v Speaker 1>to Amy, because she she reminded us that it's so black,

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<v Speaker 1>it's blacker than like black ink here on Earth. It

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<v Speaker 1>only reflects three percent of the light that comes at it.

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<v Speaker 1>So this is really I mean, if it's made of metal,

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<v Speaker 1>it is the blackest of metals. It is the most

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<v Speaker 1>metal thing in space. Like imagine wearing all black on

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<v Speaker 1>a really hot day. You're getting a sense of the

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<v Speaker 1>of the situation that's going here and the resulting Yarkovsky

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<v Speaker 1>effect that that gradually pushes it, and this gradually changes

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<v Speaker 1>the the orbit of this asteroid over time, pushes it

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<v Speaker 1>causes them to migrate until it encounters the gravitational residents

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<v Speaker 1>of Saturn, and the regular tugging effective effect here eventually

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<v Speaker 1>pushes Banu into the inner Solar System, where the experience

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<v Speaker 1>is close encounters with Venus and Earth, encounters that then

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<v Speaker 1>pull apart the rubble kind of reshape it, turn it

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<v Speaker 1>inside out. Because it's worth mentioning here that it's dark, yes,

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<v Speaker 1>but it's also just kind of a loose collection of

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<v Speaker 1>boulders and rock and dust, And there's actually a theory.

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<v Speaker 1>I don't know if you ran across this one and

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<v Speaker 1>the Nathi materials that a billion years ago, the venue

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<v Speaker 1>was part of a larger proto planet and he got

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<v Speaker 1>shattered by a space collision with another asteroid. And this

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<v Speaker 1>is just kind of the rough remnants of that. Yeah.

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<v Speaker 1>The theory that I read was that it was thought

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<v Speaker 1>to have been the material of a nebula and that

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<v Speaker 1>was disrupted by an exploding star. Yeah, well that was

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<v Speaker 1>the original. Yeah. Basically, if you go back far enough,

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<v Speaker 1>about four point five billion years, you just have a

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<v Speaker 1>stellar nursery of hydrogen, helium, and dust and this is

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<v Speaker 1>the birthplace of our son. The surrounding solar system. A

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<v Speaker 1>supernova of a nearby star stirs all of this into action,

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<v Speaker 1>spinning off the cretion disc that births the star and

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<v Speaker 1>uh yeah, and so everything else is in this mix

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<v Speaker 1>as well. And this uh, this asteroid Ben who was

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<v Speaker 1>essentially you know, a call back to these earlier Yeah,

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<v Speaker 1>and the idea is essentially right like that. It's just

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<v Speaker 1>bits of dust that were like super flash heated together

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<v Speaker 1>into this molten rock that like you you refer to

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<v Speaker 1>it's sort of like a rubble pile. They think it's

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<v Speaker 1>not like one big rock. It's just like a bunch

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<v Speaker 1>of stuff fused together. Uh, and it's being propelled by

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<v Speaker 1>the Rakovsky effect that you mentioned earlier. Now, okay, just

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<v Speaker 1>real quick, some numbers on the whole, whether it's going

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<v Speaker 1>to hit us thing or not. NASA does officially classify

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<v Speaker 1>it as quote potentially dangerous, but there's only a point

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<v Speaker 1>zero three seven percent chance that it will strike Earth

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<v Speaker 1>according to their calculation. So, like, if you think about

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<v Speaker 1>this in terms of say Batman's rogue gallery, this is

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<v Speaker 1>not the Joker um, but this is also maybe not

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<v Speaker 1>what's the Vincent Price character Egghead? Yeah, it's not Egghead.

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<v Speaker 1>It would be somewhere you tell me you're the comics,

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<v Speaker 1>a real rare Batman villain like that. But the threat threat, uh,

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<v Speaker 1>one that I would immediately go to would be a

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<v Speaker 1>character named Anarchy. And the anarchy is spelled with the K.

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<v Speaker 1>It's a teenager. He's just running around Gotham causing chaotic anarchy. Yeah,

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<v Speaker 1>so that's pretty low on Batman's road gallery. That's not

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<v Speaker 1>one of his priorities. He lets Robin handle that, right.

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<v Speaker 1>But if that, but if that particular villain is just

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<v Speaker 1>going to be close enough for study, then it might

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<v Speaker 1>be a way to additionally learn how you handle villains

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<v Speaker 1>and what how villains are put together? Right? Yeah, and

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<v Speaker 1>so according to Scientific American, if Benu did hit Earth,

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<v Speaker 1>even if we did get within that very very tiny

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<v Speaker 1>window of probability, yes, it would devastate a local area,

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<v Speaker 1>but it's not gonna wipe out civilization. It's something we

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<v Speaker 1>would know is coming. We would be able to evacuate people.

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<v Speaker 1>Is to do something like on a large level, uh,

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<v Speaker 1>that would possibly cause mass extinction. The asteroid has to

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<v Speaker 1>be at least point six miles wide or out one kilometer,

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<v Speaker 1>So Bannu is nowhere near that. Um, don't worry about it,

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<v Speaker 1>no matter what headlines you see this week. All right,

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<v Speaker 1>we're gonna take a quick break and when we come back,

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<v Speaker 1>we will dive into the mission itself. Osiris Rex. Okay,

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<v Speaker 1>so we're back now, Osiris Rex. What is this all about?

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<v Speaker 1>What's the goal? Let's start there. It's a spacecraft, but

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<v Speaker 1>let's start with why they're building this spacecraft. What's the

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<v Speaker 1>whole point of it? Right? Uh? They want to take

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<v Speaker 1>this spacecraft to Banu and bring back at least two

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<v Speaker 1>point one ounces or around four pounds of sample soil

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<v Speaker 1>and rock from Banu to bring back to Earth. And

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<v Speaker 1>it's the first mission to ever try this with an asteroid, right,

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<v Speaker 1>and I want to stress it in the name itself.

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<v Speaker 1>That's the REX Regular Explore and that's all about documenting

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<v Speaker 1>the regular the layer of loose outer material at the

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<v Speaker 1>sampling site. Uh and you know, scaling down from there.

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<v Speaker 1>So you might be asking yourself, well, why do these

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<v Speaker 1>scientists just want to get this little tiny piece of

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<v Speaker 1>soil and rock bring it back here? What good is

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<v Speaker 1>that going to do us? Right? Well, the answer is

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<v Speaker 1>they think it will help us investigate how planets formed

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<v Speaker 1>and how life began because of you know that origin

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<v Speaker 1>story that we gave you earlier about Benu, and it's

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<v Speaker 1>uh history going so far back, you know, there may

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<v Speaker 1>be traces there. Yeah, there was a period of time

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<v Speaker 1>where the asteroid, these asteroids are just like pushed back

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<v Speaker 1>into the inner sellular system and they're just crashing into everything,

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<v Speaker 1>crashing into Earth. And this could have been a way

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<v Speaker 1>that some of these vital materials that would lead to

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<v Speaker 1>a life on Earth might have gotten here. Yeah, And

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<v Speaker 1>so this mission, it's the mission is there's so many

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<v Speaker 1>people contributing to there's NASA, there's several universities involved. Lockheed

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<v Speaker 1>Martin built some of the materials that are on the spacecraft,

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<v Speaker 1>but it's managed out of NASA's Godard's Space Flight Center,

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<v Speaker 1>which is up in Green Maryland for us here in America. Uh.

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<v Speaker 1>In fact, the how Stuff Works team visited there, I

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<v Speaker 1>want to say, like six months ago and shot a

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<v Speaker 1>bunch of videos just talking to different scientists there about

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<v Speaker 1>the missions that they were performing. Uh. The thing is

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<v Speaker 1>too about this is like they can look at Banu

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<v Speaker 1>with a telescope and they have lots of interpretations about

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<v Speaker 1>what its composition is. Uh, but they want to be

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<v Speaker 1>able to prove that. So part of sending the spacecraft

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<v Speaker 1>there is also to confirm or maybe deny some of

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<v Speaker 1>their interpretations and observations from a telescope. Uh. So they're

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<v Speaker 1>gonna be doing things like measuring the effect of sunlight

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<v Speaker 1>on the orbit of the asteroid. And we've mentioned this before.

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<v Speaker 1>Let me clarify this is the Yarkovsky effect. What it

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<v Speaker 1>is is when the asteroid absorbs sunlight then re emits

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<v Speaker 1>that sunlight as heat and it gets a slight push.

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<v Speaker 1>And Amy talks with us about that later. But can

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<v Speaker 1>do all sorts of things that change the trajectory of

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<v Speaker 1>the asteroid. So I think we've hit on all of

0:12:57.920 --> 0:13:00.400
<v Speaker 1>the key points in the name of the craft. We

0:13:00.440 --> 0:13:04.920
<v Speaker 1>have the origins the sea of the spectral interpretation, resource identification,

0:13:05.280 --> 0:13:08.400
<v Speaker 1>security and that actually refer that actually deals with the

0:13:08.400 --> 0:13:10.840
<v Speaker 1>measure of the measuring the effect of the sunlight on

0:13:10.920 --> 0:13:14.240
<v Speaker 1>the orbit and the Acosmy effect. And then the regular explore.

0:13:14.480 --> 0:13:17.000
<v Speaker 1>Now regulthe was a term I wasn't familiar with. It

0:13:17.040 --> 0:13:20.440
<v Speaker 1>means the layer of loose outer material that's on the

0:13:20.480 --> 0:13:24.280
<v Speaker 1>asteroid that they're going to sample, basically, right, That's that's

0:13:24.280 --> 0:13:26.920
<v Speaker 1>why it's a regular if explorer. Here's the real quick,

0:13:26.960 --> 0:13:30.400
<v Speaker 1>down and dirty stats on the spacecraft. Spacecraft of os

0:13:30.400 --> 0:13:33.920
<v Speaker 1>Iris REX. Uh. It's twenty point to five feet long,

0:13:34.280 --> 0:13:37.520
<v Speaker 1>eight feet wide, and ten point three three ft tall,

0:13:37.600 --> 0:13:41.760
<v Speaker 1>so it's no small thing. Uh. It weighs a thousand,

0:13:41.880 --> 0:13:45.200
<v Speaker 1>nine forty pounds, but that's without fuel. When you put

0:13:45.280 --> 0:13:48.440
<v Speaker 1>fuel into this thing, it weighs four thousand, six hundred

0:13:48.440 --> 0:13:51.720
<v Speaker 1>and fifty pounds. They're also going to have two solar

0:13:51.760 --> 0:13:54.720
<v Speaker 1>panels on it to generate wattage to power the thing

0:13:54.760 --> 0:13:57.960
<v Speaker 1>as well as the fuel that's in there. And in addition,

0:13:58.400 --> 0:14:01.760
<v Speaker 1>it has this y it array of communication systems so

0:14:01.800 --> 0:14:04.959
<v Speaker 1>that it can relay back to Earth both its scientific

0:14:05.080 --> 0:14:08.160
<v Speaker 1>findings and what they refer to as its health status.

0:14:08.160 --> 0:14:11.360
<v Speaker 1>So basically you know whether it's malfunctioning or not. Uh.

0:14:11.400 --> 0:14:14.600
<v Speaker 1>So they perform a lot of detailed tests on these

0:14:14.600 --> 0:14:16.880
<v Speaker 1>system to make sure that they survived the journey. That's

0:14:16.880 --> 0:14:19.440
<v Speaker 1>something we talked to Amy about later. But everything from

0:14:19.560 --> 0:14:23.480
<v Speaker 1>vibrational testing to heat and cold uh and then um

0:14:23.720 --> 0:14:27.480
<v Speaker 1>loud loud noises. They literally blast these things with air horns. Yeah,

0:14:27.440 --> 0:14:30.120
<v Speaker 1>they've really put it through hell, because that's that's kind

0:14:30.120 --> 0:14:33.400
<v Speaker 1>of what leaving the planet it amounts to. And the

0:14:33.440 --> 0:14:36.800
<v Speaker 1>reason why it has to have so many communication systems

0:14:36.800 --> 0:14:39.000
<v Speaker 1>on board is that it's going to be communicating not

0:14:39.200 --> 0:14:43.200
<v Speaker 1>just with NASA, but with three different facilities on Earth,

0:14:43.240 --> 0:14:49.000
<v Speaker 1>one in Goldstone, California, one in Spain, and one in Canberra, Australia. Uh.

0:14:49.040 --> 0:14:53.040
<v Speaker 1>They each have huge two and thirty foot diameter dishes

0:14:53.120 --> 0:14:55.920
<v Speaker 1>for communication, so they can talk to things like this

0:14:56.680 --> 0:15:00.280
<v Speaker 1>up to the size of a pizza box. Now, uh

0:15:00.400 --> 0:15:02.840
<v Speaker 1>osiris Rex is much bigger than that, obviously given the

0:15:02.840 --> 0:15:05.200
<v Speaker 1>stats I just gave you. But you know, the communication

0:15:05.240 --> 0:15:07.440
<v Speaker 1>systems on board might not be all right, So what

0:15:07.520 --> 0:15:09.760
<v Speaker 1>kind of payload are we we're talking about here. They've

0:15:09.760 --> 0:15:13.000
<v Speaker 1>built a lot of different little I'm gonna just call

0:15:13.040 --> 0:15:16.280
<v Speaker 1>him gizmos and widgets to put on board the spacecraft

0:15:16.560 --> 0:15:19.120
<v Speaker 1>for its mission. And the first one that the one

0:15:19.160 --> 0:15:20.600
<v Speaker 1>that said they seem the most proud of. There's a

0:15:20.640 --> 0:15:23.200
<v Speaker 1>lot of material on Nassa's side about This is called

0:15:23.280 --> 0:15:27.440
<v Speaker 1>oviars UH and it is the Osiris REX Visible and

0:15:27.520 --> 0:15:30.880
<v Speaker 1>infrared spectrometer UH. So basically, this is going to look

0:15:30.880 --> 0:15:34.880
<v Speaker 1>at the asteroids spectral signature and detect whether there's organics

0:15:34.960 --> 0:15:39.160
<v Speaker 1>or other mineral materials there. It measures visible and near

0:15:39.280 --> 0:15:44.720
<v Speaker 1>infrared light that's reflected and emitted from BEANU and it's key.

0:15:44.760 --> 0:15:48.400
<v Speaker 1>It is key to their search for organics. This is

0:15:48.440 --> 0:15:52.440
<v Speaker 1>because minerals and other materials have unique what they refer

0:15:52.520 --> 0:15:55.560
<v Speaker 1>to as fingerprints within these spectrums, so they'll hopefully be

0:15:55.560 --> 0:15:58.920
<v Speaker 1>able to see these things even before they actually touched

0:15:58.920 --> 0:16:01.760
<v Speaker 1>down for that brief second with their arm. UH. It

0:16:01.840 --> 0:16:05.200
<v Speaker 1>only operates. This is OVIRS an auto cyrus rex at

0:16:05.240 --> 0:16:09.560
<v Speaker 1>ten watts. It's less power than your standard household light bulb,

0:16:09.800 --> 0:16:12.640
<v Speaker 1>and they've built it with no moving parts to reduce

0:16:12.680 --> 0:16:15.000
<v Speaker 1>the risk of malfunctions. So this is like a pretty

0:16:15.320 --> 0:16:18.680
<v Speaker 1>pared down invention for them to measure these things and

0:16:18.760 --> 0:16:22.520
<v Speaker 1>to avoid it getting overheated by all the light and

0:16:22.560 --> 0:16:25.040
<v Speaker 1>thermal radiation that's going to be bombarding them while they're

0:16:25.040 --> 0:16:28.120
<v Speaker 1>out there. The whole thing has been analyzed to scatter

0:16:28.240 --> 0:16:31.280
<v Speaker 1>light around it and make it resistant to corrosion as well.

0:16:31.600 --> 0:16:35.520
<v Speaker 1>Now I have to admit, when it comes to space missions, UM,

0:16:35.760 --> 0:16:38.200
<v Speaker 1>I always returned to like the eight year old me

0:16:38.800 --> 0:16:41.840
<v Speaker 1>and UH and assembling Lego kits, And maybe part of

0:16:41.840 --> 0:16:44.600
<v Speaker 1>that is also also that I'm now assembling Lego kits

0:16:44.600 --> 0:16:47.880
<v Speaker 1>with with my son. But I get excited about little

0:16:47.960 --> 0:16:51.560
<v Speaker 1>robot arms, h any kind of grabb or any type

0:16:51.680 --> 0:16:54.880
<v Speaker 1>type of you know, UM, fine manipulation device on a

0:16:55.000 --> 0:16:57.960
<v Speaker 1>land or a spacecraft. And there is a really cool

0:16:57.960 --> 0:17:01.840
<v Speaker 1>one here with a very fun name. It's called togasm

0:17:02.520 --> 0:17:06.280
<v Speaker 1>or tagasm or tag asm. Tag as definitely an ASTHM

0:17:06.359 --> 0:17:10.120
<v Speaker 1>in there, the touch and go sample acquisition mechanism. So

0:17:10.359 --> 0:17:12.320
<v Speaker 1>we kind of joke with Amy later on when we

0:17:12.359 --> 0:17:15.040
<v Speaker 1>talked to her about all these acronyms that NASA comes

0:17:15.080 --> 0:17:16.480
<v Speaker 1>up with, and she was a good sport about it,

0:17:16.520 --> 0:17:20.600
<v Speaker 1>and explained why. But yet, So the arm it has

0:17:20.640 --> 0:17:24.200
<v Speaker 1>a sample return capsule that's attached to it to protect

0:17:24.240 --> 0:17:27.880
<v Speaker 1>the sample that with both a heat shield and parachutes

0:17:27.960 --> 0:17:31.240
<v Speaker 1>upon reentry. And that's important because we we talk about

0:17:31.440 --> 0:17:35.320
<v Speaker 1>um planetary contamination as a possibility with amy, So they

0:17:35.320 --> 0:17:37.280
<v Speaker 1>really want to seal this thing up tight. The arm

0:17:37.359 --> 0:17:40.600
<v Speaker 1>reaches out, grabs it, seals it within this capsule, and

0:17:40.600 --> 0:17:42.359
<v Speaker 1>then keeps it safe all the way back to its

0:17:42.440 --> 0:17:47.120
<v Speaker 1>journey to Earth through our our atmosphere. And then they're

0:17:47.119 --> 0:17:51.640
<v Speaker 1>gonna put it into a very high security laboratory here

0:17:51.640 --> 0:17:54.439
<v Speaker 1>on Earth because the sample retrieval aspects of this. And

0:17:54.440 --> 0:17:56.040
<v Speaker 1>we get into this little bit in the interview whether

0:17:56.040 --> 0:17:59.560
<v Speaker 1>here it's just amazing here this is it's quite a

0:17:59.560 --> 0:18:02.119
<v Speaker 1>feat to to send this device reach out into the

0:18:02.160 --> 0:18:05.080
<v Speaker 1>void with your technology, pinch off a little bit of

0:18:05.160 --> 0:18:07.360
<v Speaker 1>rock and bring it back. Yeah. Yeah, I mean we've

0:18:07.400 --> 0:18:09.840
<v Speaker 1>never done it before. It sounds it sounds easy when

0:18:09.880 --> 0:18:12.399
<v Speaker 1>you think about like sci fi type stuff, right, like

0:18:12.400 --> 0:18:15.080
<v Speaker 1>like just take your average summer blockbuster movie, Like if

0:18:15.080 --> 0:18:17.320
<v Speaker 1>you saw something like this happen in it, you'd go, sure,

0:18:17.480 --> 0:18:19.480
<v Speaker 1>I happen all the time. You can do that. But no,

0:18:19.560 --> 0:18:22.120
<v Speaker 1>we haven't done it yet before, Yeah, not not in

0:18:22.240 --> 0:18:25.000
<v Speaker 1>the the exact way that this one is carrying it out.

0:18:25.680 --> 0:18:31.639
<v Speaker 1>So they have another really high tech acronym device on

0:18:31.800 --> 0:18:35.520
<v Speaker 1>board this ship. It's called oh cams uh, and this

0:18:35.600 --> 0:18:38.320
<v Speaker 1>is the camera suite of three cameras that are going

0:18:38.359 --> 0:18:43.000
<v Speaker 1>to allow them to globally image and map Banu. There's

0:18:43.040 --> 0:18:46.480
<v Speaker 1>also a laser altimeter on board that they'll use to

0:18:46.520 --> 0:18:49.600
<v Speaker 1>measure the distance between the craft and Banu as it

0:18:49.600 --> 0:18:52.879
<v Speaker 1>gets closer. Uh. Now, the point of these tools is

0:18:52.920 --> 0:18:56.120
<v Speaker 1>to help them map the asteroid and recon for possible

0:18:56.200 --> 0:18:59.960
<v Speaker 1>sampling sites as they get closer. This is so detailed

0:19:00.240 --> 0:19:04.160
<v Speaker 1>that they can spot individual pebbles on its surface. Now,

0:19:04.320 --> 0:19:07.080
<v Speaker 1>remember Banu we referred to it before. It's just like

0:19:07.080 --> 0:19:10.280
<v Speaker 1>a pile of rubble in space, right. It's not smooth.

0:19:10.320 --> 0:19:13.400
<v Speaker 1>It's a lumpy, irregular shape. So it's going to need

0:19:13.440 --> 0:19:16.160
<v Speaker 1>this kind of data before they approach it. They also

0:19:16.200 --> 0:19:19.359
<v Speaker 1>have a thermal emission spectrometer that just provides them, you know,

0:19:19.440 --> 0:19:22.280
<v Speaker 1>standard temperature information. And then this is cool. M I.

0:19:22.320 --> 0:19:25.959
<v Speaker 1>T And Harvard students and some faculty got together and

0:19:25.960 --> 0:19:29.639
<v Speaker 1>put together an X ray imaging spectrometer that will observe

0:19:29.720 --> 0:19:32.880
<v Speaker 1>the X ray spectrum around Benu as well, So there's

0:19:32.920 --> 0:19:35.480
<v Speaker 1>some involvement there. And you know what, I'm gonna add

0:19:35.520 --> 0:19:36.879
<v Speaker 1>this here. I was gonna save it from the end

0:19:36.880 --> 0:19:38.840
<v Speaker 1>of the episode, but you mentioned, uh, you know the

0:19:38.880 --> 0:19:41.199
<v Speaker 1>fun part about playing with legos and kind of building

0:19:41.240 --> 0:19:44.560
<v Speaker 1>your own thing. So one of the project scientists on

0:19:44.600 --> 0:19:48.280
<v Speaker 1>the Osiris REX mission, his name is Jason Dwarkin, and

0:19:48.359 --> 0:19:51.240
<v Speaker 1>there's a video game called Cerbal Space Program. I hadn't

0:19:51.280 --> 0:19:53.080
<v Speaker 1>heard about it before this, but it's basically like a

0:19:53.880 --> 0:19:57.600
<v Speaker 1>simulator for building devices that you would launch into space

0:19:57.640 --> 0:20:01.040
<v Speaker 1>and see how they react. Right. He presented to the

0:20:01.040 --> 0:20:03.680
<v Speaker 1>fans of the video game in their forum. He said, hey,

0:20:03.680 --> 0:20:05.480
<v Speaker 1>I got a challenge for you. Can you build a

0:20:05.520 --> 0:20:10.760
<v Speaker 1>replica of Osiris Rex and successfully return an asteroid sample

0:20:10.800 --> 0:20:13.360
<v Speaker 1>to Earth? And he himself tried to do it over

0:20:13.400 --> 0:20:16.200
<v Speaker 1>and over again and he didn't have very good results. Uh.

0:20:16.240 --> 0:20:19.359
<v Speaker 1>The game essentially simulates what it's like running a space

0:20:19.400 --> 0:20:23.440
<v Speaker 1>agency on like a a sort of like alternate version

0:20:23.480 --> 0:20:26.440
<v Speaker 1>of Earth. Uh. And he found that within the game

0:20:26.520 --> 0:20:30.280
<v Speaker 1>he couldn't get the spacecraft or launch using the realistic matches,

0:20:30.520 --> 0:20:34.160
<v Speaker 1>uh sorry, masses that they're using in real time here

0:20:34.200 --> 0:20:36.800
<v Speaker 1>on Earth. But still he said, hey, I want to

0:20:36.840 --> 0:20:38.240
<v Speaker 1>see you guys do it. And there is a big

0:20:38.280 --> 0:20:40.639
<v Speaker 1>response and lots of people have been attempting this in

0:20:40.680 --> 0:20:44.640
<v Speaker 1>this video game. So this is a very fact based,

0:20:44.680 --> 0:20:47.400
<v Speaker 1>science based video game on games. That's what it sounded like. Yeah,

0:20:47.440 --> 0:20:49.479
<v Speaker 1>so you wouldn't be able to pull off what I

0:20:49.600 --> 0:20:52.760
<v Speaker 1>instantly think about, and this kind of unreal reality would

0:20:52.800 --> 0:20:56.720
<v Speaker 1>be to actually put the ghost of Wu tang Rapper

0:20:57.040 --> 0:21:00.200
<v Speaker 1>d ak O Cyrus. He would power it the stead

0:21:00.200 --> 0:21:03.040
<v Speaker 1>of the Yarkovsky effect. It's the big baby Jesus effect.

0:21:04.920 --> 0:21:08.560
<v Speaker 1>That would be pretty cool. Uh yeah, yeah, So, I

0:21:08.560 --> 0:21:11.440
<v Speaker 1>mean they're they've they've got so many collaborators on this thing.

0:21:11.440 --> 0:21:15.160
<v Speaker 1>They've got m I T, the multiple universities that contributed

0:21:15.200 --> 0:21:19.680
<v Speaker 1>to the research, NASA, Lockeed Martin, other companies. It's we

0:21:19.680 --> 0:21:22.040
<v Speaker 1>We asked her about this later, but I can't imagine

0:21:22.480 --> 0:21:24.879
<v Speaker 1>being the project manager on this thing, just trying to

0:21:24.960 --> 0:21:28.879
<v Speaker 1>keep everybody in uh communication and and and keep this

0:21:29.320 --> 0:21:33.400
<v Speaker 1>on track. Yeah. Indeed, now we've already touched a little

0:21:33.440 --> 0:21:36.560
<v Speaker 1>bit on the itinerary. It's gonna launch September eight, two

0:21:36.560 --> 0:21:40.880
<v Speaker 1>thousand and sixteen. It's seven oh five pm eastern daylight time.

0:21:41.200 --> 0:21:42.919
<v Speaker 1>It will be a position on the nose of an

0:21:42.920 --> 0:21:47.440
<v Speaker 1>Atlas five rocket for launch, and it's going to orbit

0:21:47.480 --> 0:21:49.960
<v Speaker 1>the Sun for a year, using Earth's gravitational field to

0:21:50.080 --> 0:21:53.199
<v Speaker 1>help assess its journey to being. The only thing that

0:21:53.240 --> 0:21:55.840
<v Speaker 1>I like immediately think of when I hear something like

0:21:55.920 --> 0:21:57.880
<v Speaker 1>that is the old thing they do in Star Trek

0:21:57.920 --> 0:22:00.040
<v Speaker 1>whenever they travel back in time, and they like it

0:22:00.200 --> 0:22:03.639
<v Speaker 1>them around the Sun and somehow that works and then

0:22:03.640 --> 0:22:06.320
<v Speaker 1>they go back. Yeah, this one will not be going

0:22:06.359 --> 0:22:10.000
<v Speaker 1>back in time though, it's traveling through spacetime as everything is.

0:22:10.040 --> 0:22:13.320
<v Speaker 1>So you want to get technical about it. Yes, Uh,

0:22:13.400 --> 0:22:16.880
<v Speaker 1>it's not going to reach Banu though until and it's

0:22:16.880 --> 0:22:19.560
<v Speaker 1>going to approach in August of that year. It's got

0:22:19.640 --> 0:22:22.320
<v Speaker 1>rocket thrusters that will help slow it down over the

0:22:22.320 --> 0:22:25.879
<v Speaker 1>course of that year, and then it will briefly touch it,

0:22:25.960 --> 0:22:29.280
<v Speaker 1>like very briefly to retrieve that sample. So it's just

0:22:29.280 --> 0:22:32.399
<v Speaker 1>gonna come up very slowly, touch it, grab a sample

0:22:32.400 --> 0:22:35.199
<v Speaker 1>of that arm, and then move away. And it's the

0:22:35.320 --> 0:22:38.000
<v Speaker 1>arm is built to release nitrogen gas that will stir

0:22:38.160 --> 0:22:40.600
<v Speaker 1>up the rocks so that the surface sample will be

0:22:40.640 --> 0:22:44.760
<v Speaker 1>easier to grab. And it has about three attempts worth

0:22:44.760 --> 0:22:47.399
<v Speaker 1>of nitrogen on it. But obviously they're hopening, you know,

0:22:47.600 --> 0:22:49.800
<v Speaker 1>just right on the first try it we'll get it

0:22:50.119 --> 0:22:53.720
<v Speaker 1>all right. So that's then when did when do we

0:22:53.800 --> 0:22:56.920
<v Speaker 1>get it back? One is when it's going to have

0:22:56.960 --> 0:23:00.000
<v Speaker 1>a window for departure and then it's going to return

0:23:00.080 --> 0:23:04.679
<v Speaker 1>to Earth in three uh And as we talk about

0:23:05.080 --> 0:23:08.080
<v Speaker 1>with Amy, the sample will come back. It will be

0:23:08.160 --> 0:23:11.200
<v Speaker 1>taken to the Utah Test and Training Range where it

0:23:11.200 --> 0:23:14.520
<v Speaker 1>will be studied, and then after it's vigorously studied, probably

0:23:14.560 --> 0:23:16.240
<v Speaker 1>for a couple of years, it will then be moved

0:23:16.280 --> 0:23:21.280
<v Speaker 1>to NASA's Johnson Space Flight Center in Houston. So get ready,

0:23:21.560 --> 0:23:24.639
<v Speaker 1>I mean, uh, mark your calendars because that might be

0:23:24.680 --> 0:23:29.000
<v Speaker 1>when it comes back. And then we'll do another episode. Yeah, exactly,

0:23:29.000 --> 0:23:31.760
<v Speaker 1>we'll talk about how everything panned out. Yeah, it's assuming

0:23:31.760 --> 0:23:34.040
<v Speaker 1>I'm still alive. I don't know. Three feels like a

0:23:34.080 --> 0:23:36.520
<v Speaker 1>long ways away. I know, you start looking at That's

0:23:36.560 --> 0:23:39.000
<v Speaker 1>one of the fascinating things about these missions, right, is

0:23:39.400 --> 0:23:42.000
<v Speaker 1>their their long form missions. Yeah, and I guess it's

0:23:42.000 --> 0:23:45.560
<v Speaker 1>always been the case. Really, I mean look back to

0:23:45.560 --> 0:23:49.080
<v Speaker 1>to to any of the the large scale mega projects

0:23:49.080 --> 0:23:51.919
<v Speaker 1>in space. You know, some of the earlier ones definitely

0:23:51.960 --> 0:23:55.520
<v Speaker 1>had a more accelerated time frame in many respects, but

0:23:55.560 --> 0:23:58.960
<v Speaker 1>still things like like the Voider and Pioneer missions, those

0:23:58.960 --> 0:24:02.400
<v Speaker 1>were those were in for the long haul. Yeah, absolutely, um,

0:24:02.440 --> 0:24:04.880
<v Speaker 1>and I would imagine that if you're on these teams too,

0:24:04.920 --> 0:24:08.080
<v Speaker 1>you have to think in longitudinal terms like that too.

0:24:08.160 --> 0:24:11.439
<v Speaker 1>Is even in terms of staffing, right, like like some

0:24:11.520 --> 0:24:13.800
<v Speaker 1>of the staff members may be older now and may

0:24:13.840 --> 0:24:16.439
<v Speaker 1>not be expecting to be on the team when it

0:24:16.520 --> 0:24:20.080
<v Speaker 1>comes back. They may be retired by them. So that's

0:24:20.080 --> 0:24:22.679
<v Speaker 1>what we've got for you on Osiris. Those are the

0:24:22.720 --> 0:24:26.160
<v Speaker 1>general facts. That's the plan, the mission, the itinerary, all

0:24:26.160 --> 0:24:28.440
<v Speaker 1>the stuff that's on board it. Now we're going to

0:24:28.560 --> 0:24:31.480
<v Speaker 1>talk to Dr Amy Simon and she's going to fill

0:24:31.560 --> 0:24:36.159
<v Speaker 1>us in on the war complicated scientific matters behind the mission.

0:24:45.920 --> 0:24:48.320
<v Speaker 1>What is it about Benner that makes the team think

0:24:48.400 --> 0:24:51.200
<v Speaker 1>that it may contain clues to the origins of life?

0:24:52.440 --> 0:24:55.159
<v Speaker 1>So when we were proposing the Osiros rets mission, you know,

0:24:55.200 --> 0:24:57.960
<v Speaker 1>we had a choice of hundreds of thousands of asteroids

0:24:58.000 --> 0:25:00.920
<v Speaker 1>to pick from, and the reason that menu stuck out

0:25:00.960 --> 0:25:02.919
<v Speaker 1>in the first place is, for one thing, it's a

0:25:03.040 --> 0:25:07.040
<v Speaker 1>very very dark asteroid. It's extremely black. It only reflects

0:25:07.040 --> 0:25:10.720
<v Speaker 1>about three of the sunlight that that hits it UM.

0:25:10.840 --> 0:25:12.520
<v Speaker 1>So you know, if you look around your room at

0:25:12.520 --> 0:25:14.840
<v Speaker 1>black things, so the blackest paint at your ink to

0:25:14.840 --> 0:25:18.760
<v Speaker 1>owner um, that's probably still about five six percent reflectants,

0:25:18.800 --> 0:25:21.760
<v Speaker 1>so it's even blacker than that. And the reason that

0:25:21.840 --> 0:25:24.480
<v Speaker 1>color is so important is that things that are black

0:25:24.520 --> 0:25:26.719
<v Speaker 1>tend to have a lot of carbon on them, and

0:25:26.840 --> 0:25:28.399
<v Speaker 1>most of the building blocks of life, I mean no

0:25:28.480 --> 0:25:32.920
<v Speaker 1>acids um involves hydrocarbons, and so we want to find

0:25:32.920 --> 0:25:34.600
<v Speaker 1>something that has a lot of carbon on it because

0:25:34.640 --> 0:25:37.160
<v Speaker 1>that's our best chance of looking for those building blocks,

0:25:37.640 --> 0:25:41.800
<v Speaker 1>and so that's why it was particularly interesting this asteroid UM.

0:25:41.920 --> 0:25:44.080
<v Speaker 1>It was also nice because this asteroid is an Earth

0:25:44.119 --> 0:25:47.439
<v Speaker 1>crossing asteroid. It's a near Earth asteroid, so it's easier

0:25:47.440 --> 0:25:48.879
<v Speaker 1>to get to than some of the ones farther out

0:25:48.920 --> 0:25:52.359
<v Speaker 1>in the Solar system UM. And you know, it's just

0:25:52.440 --> 0:25:55.840
<v Speaker 1>an interesting object because it does cross the Earth's path

0:25:56.200 --> 0:25:58.080
<v Speaker 1>and so this is the type of thing we think

0:25:58.119 --> 0:26:00.679
<v Speaker 1>back in the formation of the planet and Earth that

0:26:00.800 --> 0:26:03.480
<v Speaker 1>might have helped put those hydrocarbons and things that we

0:26:03.520 --> 0:26:05.560
<v Speaker 1>needed for life here. So that's why we want to

0:26:05.560 --> 0:26:08.760
<v Speaker 1>study this particular asteroid Okay, so, so to clarify, you

0:26:08.840 --> 0:26:14.720
<v Speaker 1>mean asteroids like this potentially impacted with Earth bringing materials

0:26:14.720 --> 0:26:17.879
<v Speaker 1>like this here. That's right. We we certainly know that

0:26:17.920 --> 0:26:20.560
<v Speaker 1>at various points in the Solar System history and the

0:26:20.600 --> 0:26:23.280
<v Speaker 1>formation of the planets, that all these bodies were floating

0:26:23.320 --> 0:26:24.720
<v Speaker 1>around and a lot of them would have hit the

0:26:24.760 --> 0:26:27.680
<v Speaker 1>surfaces of the planets as they were forming. Um. And

0:26:27.720 --> 0:26:30.040
<v Speaker 1>we think commets brought water, for example, but we think

0:26:30.080 --> 0:26:33.240
<v Speaker 1>that asteroids in particular, because those are the primitive leftover

0:26:33.280 --> 0:26:36.400
<v Speaker 1>pieces from forming the Solar System, will tell us about

0:26:36.440 --> 0:26:40.000
<v Speaker 1>those things that hint very early on. Okay, uh So,

0:26:40.200 --> 0:26:42.359
<v Speaker 1>one of the things that I read about in the

0:26:42.440 --> 0:26:44.560
<v Speaker 1>fact sheets and the research that NASA has put up

0:26:44.600 --> 0:26:48.120
<v Speaker 1>online about this mission was that you're hoping that this

0:26:48.160 --> 0:26:51.560
<v Speaker 1>will affect the future of space exploration as well, because

0:26:51.680 --> 0:26:54.520
<v Speaker 1>you may rely on the materials that are found on

0:26:54.560 --> 0:26:59.200
<v Speaker 1>asteroids like this. Can you explain that a little bit further? Sure, So,

0:26:59.240 --> 0:27:01.160
<v Speaker 1>as we want to go farther out in the Solar System,

0:27:01.200 --> 0:27:03.679
<v Speaker 1>particularly with people, we run into the problem that you

0:27:03.720 --> 0:27:06.480
<v Speaker 1>can't bring everything with you that you need because humans

0:27:06.480 --> 0:27:09.960
<v Speaker 1>require a lot of resources water for example. UM. So,

0:27:10.000 --> 0:27:12.040
<v Speaker 1>what we want to do is study these objects that

0:27:12.040 --> 0:27:14.200
<v Speaker 1>are on the way to more distant places and see

0:27:14.240 --> 0:27:16.800
<v Speaker 1>what's on their surfaces. So, for example, if there was

0:27:16.800 --> 0:27:19.280
<v Speaker 1>a big cache of water ice, that's something that a

0:27:19.280 --> 0:27:21.600
<v Speaker 1>mission could go pick up and bring its water along

0:27:21.640 --> 0:27:23.879
<v Speaker 1>the way instead of having to carry everything from launch

0:27:23.920 --> 0:27:26.240
<v Speaker 1>all the way out. Got it, Okay? Like to look

0:27:26.280 --> 0:27:30.880
<v Speaker 1>for those resources, okay, And so I'm imagining that you

0:27:30.960 --> 0:27:35.920
<v Speaker 1>would either have previously identified these asteroids as water sources

0:27:36.119 --> 0:27:40.080
<v Speaker 1>through telescopic means or maybe with the spectrometer like likes

0:27:40.200 --> 0:27:44.080
<v Speaker 1>on Osiris Rex. Well, ideally we would have mapped out

0:27:44.119 --> 0:27:46.639
<v Speaker 1>a whole bunch of near Earth asteroids so that we

0:27:46.720 --> 0:27:49.120
<v Speaker 1>know those were great stopping points essentially you know, gas

0:27:49.160 --> 0:27:51.879
<v Speaker 1>stations on the way. Um. But the reality is we

0:27:51.880 --> 0:27:54.320
<v Speaker 1>won't be able to send a mission to every possible asteroids.

0:27:54.400 --> 0:27:56.280
<v Speaker 1>So what we can also do is look at the

0:27:56.320 --> 0:27:59.639
<v Speaker 1>class of asteroid. So from Earth based observations, we've been

0:27:59.680 --> 0:28:02.600
<v Speaker 1>able to put asteroids in different categories, and so if

0:28:02.600 --> 0:28:04.720
<v Speaker 1>we go to one and realize this category tends to

0:28:04.760 --> 0:28:07.200
<v Speaker 1>have a lot of water, that's probably a good stopping point.

0:28:07.880 --> 0:28:10.600
<v Speaker 1>So this is a kind of an odd ball question,

0:28:10.880 --> 0:28:15.240
<v Speaker 1>But I was going through all the literature about this

0:28:15.320 --> 0:28:18.560
<v Speaker 1>mission and all the devices that are part of its payload,

0:28:18.640 --> 0:28:21.320
<v Speaker 1>and I have to ask, why is it that NASA

0:28:21.400 --> 0:28:24.760
<v Speaker 1>loves acronyms so much. Is there a specific kind of

0:28:25.280 --> 0:28:28.479
<v Speaker 1>you know, work operating procedure that makes them useful for

0:28:28.520 --> 0:28:33.320
<v Speaker 1>your classification systems? So that's that's kind of a funny question. Um.

0:28:33.320 --> 0:28:35.439
<v Speaker 1>There's no official policy that says everything has to be

0:28:35.440 --> 0:28:38.440
<v Speaker 1>an acronym. UM, But I was thinking about this, and

0:28:38.480 --> 0:28:41.240
<v Speaker 1>I think there's two different categories of why this happens.

0:28:41.320 --> 0:28:43.600
<v Speaker 1>And one is of course that we like catching names,

0:28:44.200 --> 0:28:47.120
<v Speaker 1>you know, and and early missions Apollo Gemini, those had

0:28:47.160 --> 0:28:50.720
<v Speaker 1>obvious names. But you know, as scientists and engineers, we

0:28:50.960 --> 0:28:53.320
<v Speaker 1>tend to be pretty practical when we name things, and

0:28:53.360 --> 0:28:56.720
<v Speaker 1>so that the names get very complicated very quickly. And

0:28:56.840 --> 0:28:59.360
<v Speaker 1>so that's sort of the practical reason for doing an

0:28:59.360 --> 0:29:02.440
<v Speaker 1>acronym is that we can take something that you know,

0:29:02.480 --> 0:29:04.440
<v Speaker 1>would take forever to spill out and say every time

0:29:04.520 --> 0:29:06.720
<v Speaker 1>we say it, condense it down into an acronym, and

0:29:06.720 --> 0:29:08.760
<v Speaker 1>then just use that as a word going forward. So

0:29:09.200 --> 0:29:10.680
<v Speaker 1>that's kind of what you're seeing. And then if it

0:29:10.720 --> 0:29:12.840
<v Speaker 1>happens to be catchy at the same time, even better too.

0:29:12.880 --> 0:29:14.880
<v Speaker 1>For one so whose job is it to do that?

0:29:15.000 --> 0:29:18.200
<v Speaker 1>Is it like somebody's sitting down and has come up

0:29:18.200 --> 0:29:20.000
<v Speaker 1>with the long name and they just make it into

0:29:20.080 --> 0:29:22.600
<v Speaker 1>an acronym or they try to find like like for instance,

0:29:22.600 --> 0:29:26.160
<v Speaker 1>so cyrus obviously has some symbolic meaning to it. Is

0:29:26.200 --> 0:29:28.160
<v Speaker 1>there like a I don't know, like some kind of

0:29:28.560 --> 0:29:31.320
<v Speaker 1>public relations team that works together with you on that.

0:29:32.400 --> 0:29:35.360
<v Speaker 1>Um No. A lot of times early on the names

0:29:35.360 --> 0:29:37.320
<v Speaker 1>like O cyrus, you know, the science team comes up

0:29:37.360 --> 0:29:40.640
<v Speaker 1>with it or the principal investigator does. But sometimes we

0:29:40.680 --> 0:29:43.959
<v Speaker 1>do have naming contests. Um Benu, for example, was actually

0:29:43.960 --> 0:29:46.479
<v Speaker 1>part of a contest where students got to write in

0:29:46.840 --> 0:29:49.200
<v Speaker 1>what they thought it should be named and why, and

0:29:49.280 --> 0:29:51.280
<v Speaker 1>you know they could have chosen an acronym in this case,

0:29:51.320 --> 0:29:54.400
<v Speaker 1>they pick something along the same. Uh. You know mythology

0:29:54.520 --> 0:29:57.560
<v Speaker 1>is a cyrus That worked out very well. But there's no,

0:29:57.680 --> 0:29:59.520
<v Speaker 1>like I said, no official policy and you know we

0:29:59.560 --> 0:30:02.880
<v Speaker 1>have fun. It cool. Yeah, that sounds great. Now, there

0:30:02.920 --> 0:30:05.360
<v Speaker 1>are a lot of outside partners involved in this mission,

0:30:05.440 --> 0:30:09.600
<v Speaker 1>university's companies, students, and many of NASA's own separate units.

0:30:09.760 --> 0:30:14.120
<v Speaker 1>How do you manage the project between so many entities? Yeah,

0:30:14.160 --> 0:30:16.680
<v Speaker 1>that can be pretty complicated. Um, the reason, you know,

0:30:16.720 --> 0:30:18.760
<v Speaker 1>there's so many entities. In the first places, this is

0:30:18.800 --> 0:30:21.040
<v Speaker 1>a rather big mission and there are so many parts

0:30:21.040 --> 0:30:24.120
<v Speaker 1>to it, so anyone group probably couldn't handle the whole

0:30:24.160 --> 0:30:26.320
<v Speaker 1>thing by themselves, so you bring in the experts for

0:30:26.360 --> 0:30:29.800
<v Speaker 1>each different area. Uh. The entire mission gets managed by

0:30:29.880 --> 0:30:32.480
<v Speaker 1>NASA Goddard and so our folks are in charge of

0:30:32.520 --> 0:30:35.240
<v Speaker 1>making sure everything keeps running. And then on the science

0:30:35.280 --> 0:30:38.360
<v Speaker 1>and the mission is really managed by University of Arizona,

0:30:38.800 --> 0:30:41.200
<v Speaker 1>so they're in charge of making sure that we're going

0:30:41.280 --> 0:30:42.760
<v Speaker 1>to do all the right science and that all the

0:30:42.800 --> 0:30:45.440
<v Speaker 1>instruments are going to meet their requirements. So it's it's

0:30:45.480 --> 0:30:48.160
<v Speaker 1>even a little bit of a distributed management actually, just

0:30:48.240 --> 0:30:52.160
<v Speaker 1>to keep it all running and all the parts going smoothly. Uh.

0:30:52.200 --> 0:30:55.440
<v Speaker 1>So getting back to you were talking about how heavily

0:30:55.480 --> 0:30:59.080
<v Speaker 1>carbon based venu is, can you talk us through how

0:30:59.120 --> 0:31:02.640
<v Speaker 1>it is that you interpret what the asteroids composition is

0:31:02.800 --> 0:31:07.400
<v Speaker 1>just based on telescopic observations and then when Osirius rex

0:31:07.440 --> 0:31:11.200
<v Speaker 1>get that gets there, how will the spectrometer observations either

0:31:11.360 --> 0:31:16.280
<v Speaker 1>confirm or refute the interpretations you've made from telescopes. So

0:31:16.320 --> 0:31:19.479
<v Speaker 1>with telescope observations even though it is an earth crossing asteroid,

0:31:19.560 --> 0:31:21.720
<v Speaker 1>it doesn't get that close to us. So when we

0:31:21.760 --> 0:31:24.640
<v Speaker 1>observe it from a ground based telescope, we don't see

0:31:24.680 --> 0:31:28.040
<v Speaker 1>the surface in detail, and so we'll get say, for example,

0:31:28.120 --> 0:31:31.480
<v Speaker 1>spectrum or imaging in different colors, and we can get

0:31:31.520 --> 0:31:34.400
<v Speaker 1>some sense of what's probably on the surface. Again that

0:31:34.480 --> 0:31:37.480
<v Speaker 1>this object is very black, it probably has carbon, but

0:31:37.560 --> 0:31:40.640
<v Speaker 1>what we can't see is a very fine composition. So

0:31:40.720 --> 0:31:44.320
<v Speaker 1>if there is that little pocket of hydrocarbons or water

0:31:44.480 --> 0:31:47.000
<v Speaker 1>or some other mineral that we're interested in, we can't

0:31:47.040 --> 0:31:49.479
<v Speaker 1>see that from the ground based observations because we're not

0:31:49.560 --> 0:31:51.920
<v Speaker 1>really resolving the surface. We just don't have that kind

0:31:51.920 --> 0:31:56.080
<v Speaker 1>of spatial resolution. So when we get there with our spectrometers,

0:31:56.120 --> 0:31:58.520
<v Speaker 1>we're going to map out the entire surface, and so

0:31:58.640 --> 0:32:01.440
<v Speaker 1>for example, if there's small craters, or there's little pockets

0:32:01.440 --> 0:32:04.120
<v Speaker 1>of of soil and regulars that are really rich in

0:32:04.160 --> 0:32:06.400
<v Speaker 1>some mineral, we'll see that when we can't see that

0:32:06.440 --> 0:32:09.360
<v Speaker 1>from the earth based observation. So it's kind of taking

0:32:09.440 --> 0:32:12.040
<v Speaker 1>that really distant view and zooming in now and now

0:32:12.080 --> 0:32:14.040
<v Speaker 1>we're gonna look at it very up close and try

0:32:14.120 --> 0:32:18.200
<v Speaker 1>to find those little pockets of of interesting material. Okay,

0:32:18.520 --> 0:32:21.920
<v Speaker 1>so I'm particularly interested in the testing. I watched a

0:32:22.000 --> 0:32:24.160
<v Speaker 1>video that I think you you might have been featured

0:32:24.160 --> 0:32:28.680
<v Speaker 1>in actually talking about UM the spaceship, sorry, the spacecraft

0:32:28.720 --> 0:32:30.360
<v Speaker 1>and how it's going to survive its journey and the

0:32:30.440 --> 0:32:33.160
<v Speaker 1>vibration tests you've put it through. But through other research

0:32:33.200 --> 0:32:35.760
<v Speaker 1>we've done here at how stuff works, I know about

0:32:35.840 --> 0:32:40.040
<v Speaker 1>like creating really loud air horns to test space machinery.

0:32:40.280 --> 0:32:42.760
<v Speaker 1>So what other stuff have you done to torture this

0:32:42.800 --> 0:32:45.920
<v Speaker 1>thing and make sure that it can survive its journey. Yes,

0:32:46.000 --> 0:32:48.640
<v Speaker 1>we we torture these spacecraft and the instruments pretty hard,

0:32:48.760 --> 0:32:50.800
<v Speaker 1>um in part because you know, they have to survive

0:32:50.840 --> 0:32:52.840
<v Speaker 1>the launch, and once they're out there, we can't go

0:32:52.880 --> 0:32:56.040
<v Speaker 1>back and fix them. And so what we do is, UM,

0:32:56.080 --> 0:32:58.400
<v Speaker 1>this is a case where we have these crazy test

0:32:58.440 --> 0:33:01.240
<v Speaker 1>procedures written up where we're going to test everything to

0:33:01.440 --> 0:33:03.240
<v Speaker 1>the limits we think is going to see in space,

0:33:03.320 --> 0:33:06.000
<v Speaker 1>and then a little bit beyond that. And so one

0:33:06.040 --> 0:33:09.080
<v Speaker 1>of the first things we do is vibration testing. And

0:33:09.120 --> 0:33:11.400
<v Speaker 1>in that case, what we do is basically we're gonna

0:33:11.400 --> 0:33:13.520
<v Speaker 1>shake the instrument or the spacecraft as hard as we

0:33:13.560 --> 0:33:16.600
<v Speaker 1>expect to see it launch because that's typically your your

0:33:16.680 --> 0:33:20.520
<v Speaker 1>biggest vibration sources, that that huge launch vehicle. So we'll

0:33:20.560 --> 0:33:22.600
<v Speaker 1>shake it really hard to make sure nothing falls off,

0:33:22.680 --> 0:33:25.840
<v Speaker 1>nothing breaks, everything is still working. So that's that's one

0:33:25.840 --> 0:33:28.880
<v Speaker 1>of the critical tests that we do. Another one we

0:33:28.920 --> 0:33:32.720
<v Speaker 1>do is is basically electromagnetic interference. So we want to

0:33:32.760 --> 0:33:35.760
<v Speaker 1>make sure that none of the different instruments or spacecraft

0:33:35.760 --> 0:33:38.000
<v Speaker 1>systems are going to interfere with each other, and so

0:33:38.080 --> 0:33:42.080
<v Speaker 1>we'll basically blast it with different uh types of electromagnetic

0:33:42.280 --> 0:33:45.080
<v Speaker 1>radiation and make sure nothing breaks. And so that's probably

0:33:45.080 --> 0:33:47.680
<v Speaker 1>when you don't hear is much about make sure they

0:33:48.080 --> 0:33:52.360
<v Speaker 1>electronics don't get affected by each other. Essentially, um we

0:33:52.440 --> 0:33:55.080
<v Speaker 1>do as the thermal testing. That one is actually quite interesting,

0:33:55.120 --> 0:33:58.360
<v Speaker 1>thermal vacuum testing, and so you know, we take things

0:33:58.640 --> 0:34:02.400
<v Speaker 1>to very extremely cold temperatures hundreds of degrees below zero.

0:34:02.640 --> 0:34:04.880
<v Speaker 1>And most people would probably believe that about space, that

0:34:04.920 --> 0:34:07.280
<v Speaker 1>it gets that that cold, but what they don't probably

0:34:07.280 --> 0:34:09.239
<v Speaker 1>consider is that we also take it to you know,

0:34:09.280 --> 0:34:13.359
<v Speaker 1>four hundred degrees above zero, because things also get very

0:34:13.400 --> 0:34:16.520
<v Speaker 1>hot in space, and that's because you're directly exposed to

0:34:16.520 --> 0:34:18.839
<v Speaker 1>the sun with no atmosphere in between. So we don't

0:34:18.840 --> 0:34:20.840
<v Speaker 1>tend to think about those temperatures here on Earth, but

0:34:20.920 --> 0:34:23.879
<v Speaker 1>that atmosphere protects you from cold and hot and so

0:34:24.760 --> 0:34:27.960
<v Speaker 1>we take it, you know, ridiculously cold temperatures and extremely

0:34:28.000 --> 0:34:30.480
<v Speaker 1>hot temperatures and we make sure again nothing breaks. We

0:34:30.560 --> 0:34:33.520
<v Speaker 1>have you know, special epoxies and seals and things like

0:34:33.560 --> 0:34:35.799
<v Speaker 1>that on different parts of the spacecraft and instruments, so

0:34:35.840 --> 0:34:37.359
<v Speaker 1>you want to make sure that those things aren't going

0:34:37.400 --> 0:34:40.000
<v Speaker 1>to be affected by the temperature. So you know, we

0:34:40.040 --> 0:34:42.160
<v Speaker 1>do this in stages. You'll do one of these tests

0:34:42.239 --> 0:34:45.719
<v Speaker 1>UM for example, uh, this thermal tests, and then you'll

0:34:45.760 --> 0:34:47.520
<v Speaker 1>take it's a vibration, and then you'll take it back

0:34:47.520 --> 0:34:49.399
<v Speaker 1>to the thermal tests. So we do it a couple

0:34:49.400 --> 0:34:51.359
<v Speaker 1>of different ways to make sure none of these things

0:34:51.360 --> 0:34:54.440
<v Speaker 1>have affected any part of the spacecraft. Okay, wow, so

0:34:54.480 --> 0:34:57.040
<v Speaker 1>that's yeah, that's like years of work, I would assume,

0:34:57.160 --> 0:34:59.320
<v Speaker 1>doing all of that testing and making sure that it

0:34:59.360 --> 0:35:02.799
<v Speaker 1>can survive all those scenarios. It is and when you know,

0:35:02.840 --> 0:35:05.640
<v Speaker 1>this testing is fairly complicated. To get to those cold temperatures,

0:35:05.680 --> 0:35:08.280
<v Speaker 1>we use liquid nitrogen and in some cases liquid helium

0:35:08.320 --> 0:35:11.280
<v Speaker 1>even UM, and that sort of test is is fairly

0:35:11.320 --> 0:35:14.520
<v Speaker 1>complicated and expensive. So it's not something that you just

0:35:14.560 --> 0:35:17.000
<v Speaker 1>do during normal work hours. You have to do this

0:35:17.040 --> 0:35:19.720
<v Speaker 1>testing seven because when you're in the chamber and running

0:35:19.719 --> 0:35:22.080
<v Speaker 1>those things, you don't want to stop the test. So

0:35:22.080 --> 0:35:23.880
<v Speaker 1>so not only is it long, it's also you know,

0:35:23.960 --> 0:35:26.440
<v Speaker 1>very long hours. We have people working over night ships

0:35:26.480 --> 0:35:30.960
<v Speaker 1>to do this testing. Okay, yeah that I remember reading

0:35:31.000 --> 0:35:33.360
<v Speaker 1>about one of the air horns that the European Space

0:35:33.400 --> 0:35:36.200
<v Speaker 1>Agency has and that could just like absolutely annihilate a

0:35:36.280 --> 0:35:39.319
<v Speaker 1>human being if you were exposed to it. So we

0:35:39.360 --> 0:35:43.440
<v Speaker 1>have warning like fall over the place during testing. Yeah,

0:35:43.760 --> 0:35:45.319
<v Speaker 1>all right, we're gonna take a quick break and we'll

0:35:45.320 --> 0:35:49.800
<v Speaker 1>be right back with Dr Amy A. Simon. Hey, everybody,

0:35:49.840 --> 0:35:51.479
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0:35:51.520 --> 0:35:54.240
<v Speaker 1>things done just one click of your mouth. I can't

0:35:54.239 --> 0:35:56.719
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0:35:56.800 --> 0:35:58.879
<v Speaker 1>get your mailing and shipping done without leaving your desk

0:35:58.920 --> 0:36:01.319
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0:36:01.320 --> 0:36:03.759
<v Speaker 1>PC or Mac into your own personal post office that

0:36:03.840 --> 0:36:06.120
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0:36:06.160 --> 0:36:09.120
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0:36:09.160 --> 0:36:11.960
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0:36:12.000 --> 0:36:14.480
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0:36:14.520 --> 0:36:16.440
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0:36:16.880 --> 0:36:18.720
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0:36:18.719 --> 0:36:20.359
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0:36:20.360 --> 0:36:22.640
<v Speaker 1>bit of merch or correspondence, and we want you to

0:36:22.640 --> 0:36:24.920
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0:36:25.000 --> 0:36:27.640
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0:36:30.160 --> 0:36:32.160
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0:36:32.200 --> 0:36:34.880
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0:36:35.200 --> 0:36:37.120
<v Speaker 1>So don't wait. Go to stamps dot com right now

0:36:37.120 --> 0:36:39.080
<v Speaker 1>before you do anything else, click on the microphone at

0:36:39.120 --> 0:36:41.600
<v Speaker 1>the top of the homepage and type in stuff that

0:36:41.719 --> 0:36:49.560
<v Speaker 1>stamps dot com, enter stuff and start mailing things. So

0:36:49.640 --> 0:36:52.560
<v Speaker 1>the planetary defense angle of the mission has received a

0:36:52.640 --> 0:36:57.080
<v Speaker 1>lot of attention recently due to frankly hysterical reports in

0:36:57.120 --> 0:36:59.520
<v Speaker 1>the media about to ben whose a slim chance of

0:36:59.600 --> 0:37:02.759
<v Speaker 1>hitting our then I believe the century. How big of

0:37:02.760 --> 0:37:05.239
<v Speaker 1>a factor is that in this mission? And can you

0:37:05.280 --> 0:37:08.080
<v Speaker 1>explain to our audience why it is a ultimately a

0:37:08.160 --> 0:37:12.400
<v Speaker 1>slim chance? Right? So you know, it was not a

0:37:12.400 --> 0:37:15.279
<v Speaker 1>deciding factor in which asteroid we went to um. It

0:37:15.400 --> 0:37:17.600
<v Speaker 1>is an Earth crossing asteroid and it turns out it

0:37:17.600 --> 0:37:22.400
<v Speaker 1>does have currently about a one um of impacting. But

0:37:22.480 --> 0:37:24.600
<v Speaker 1>what people need to understand is how we come up

0:37:24.640 --> 0:37:27.920
<v Speaker 1>with that number. And so when an asteroids first discovered,

0:37:27.960 --> 0:37:29.640
<v Speaker 1>we have one point of data where it was in

0:37:29.680 --> 0:37:33.080
<v Speaker 1>the sky, and to actually make it a discovery, we

0:37:33.120 --> 0:37:35.760
<v Speaker 1>need a second point. So we follow it up. Um,

0:37:35.840 --> 0:37:38.120
<v Speaker 1>we take those two points or three points however a

0:37:38.239 --> 0:37:40.080
<v Speaker 1>few we have, and we actually run it through a

0:37:40.120 --> 0:37:42.640
<v Speaker 1>model assuming all the gravity we know about from the

0:37:42.640 --> 0:37:45.960
<v Speaker 1>planets in the Sun, and we run it forward and

0:37:46.000 --> 0:37:49.480
<v Speaker 1>we basically see when it would cross the Earth orbit

0:37:49.520 --> 0:37:52.880
<v Speaker 1>at the same time the Earth is nearby, and we

0:37:52.880 --> 0:37:54.719
<v Speaker 1>put error bars on that, and that's how we come

0:37:54.760 --> 0:37:58.360
<v Speaker 1>up with a number. And basically what happens is going forward,

0:37:58.400 --> 0:38:00.759
<v Speaker 1>people take more and more observation, and so every once

0:38:00.760 --> 0:38:02.480
<v Speaker 1>in a while, I see about an asteroid that has

0:38:02.520 --> 0:38:04.680
<v Speaker 1>a one and one chance, one and two chance of

0:38:04.760 --> 0:38:07.120
<v Speaker 1>hitting us, and then we take some more observations and

0:38:07.160 --> 0:38:09.319
<v Speaker 1>suddenly it's one in a million. And it's because these

0:38:09.320 --> 0:38:11.719
<v Speaker 1>things don't move in a straight line, right, So so

0:38:11.760 --> 0:38:14.600
<v Speaker 1>we need more observations to basically fill in that curve

0:38:14.640 --> 0:38:17.479
<v Speaker 1>and figure out where it's going to go. But there's

0:38:17.520 --> 0:38:20.120
<v Speaker 1>one other factor that we don't know about, and that's

0:38:20.120 --> 0:38:26.759
<v Speaker 1>how the asteroid is reacting to being pushed by sunlight effect, right,

0:38:26.800 --> 0:38:29.759
<v Speaker 1>the Arkowski effect, which is actually kind of complicated where

0:38:29.760 --> 0:38:32.719
<v Speaker 1>you have sunlight and in this case that the photons

0:38:32.760 --> 0:38:35.440
<v Speaker 1>coming out the sun act as particles, so they exert

0:38:35.440 --> 0:38:37.880
<v Speaker 1>a pressure. They're pushing on the asteroid in one direction,

0:38:38.760 --> 0:38:42.080
<v Speaker 1>but especially these very black asteroids, they heat up. Now

0:38:42.080 --> 0:38:45.879
<v Speaker 1>they're also rotating, so as it turns and it's cooling off,

0:38:45.920 --> 0:38:48.200
<v Speaker 1>it radiates to space. Well, now it's going to get

0:38:48.200 --> 0:38:50.879
<v Speaker 1>pushed in a different direction. And so it's a very

0:38:50.960 --> 0:38:53.560
<v Speaker 1>very very tiny effect, but it adds up over a century,

0:38:54.200 --> 0:38:57.719
<v Speaker 1>and that's a tiny little tweak on that orbit that's

0:38:57.719 --> 0:38:59.640
<v Speaker 1>really hard to quantify. And so that's one of the

0:38:59.640 --> 0:39:02.360
<v Speaker 1>goals of our mission is to actually measure that effect,

0:39:02.680 --> 0:39:04.880
<v Speaker 1>be able to look at the incoming and outgoing radiation

0:39:04.920 --> 0:39:07.400
<v Speaker 1>and figure out how much does that work, because that

0:39:07.560 --> 0:39:09.560
<v Speaker 1>that's one big unknown and a lot of our models

0:39:09.560 --> 0:39:12.799
<v Speaker 1>of these asteroid trajectories. It was kind of fascinating to

0:39:12.800 --> 0:39:16.160
<v Speaker 1>me Amy because you know, I spent time researching all

0:39:16.160 --> 0:39:19.040
<v Speaker 1>about the mission, and then it wasn't until after I

0:39:19.040 --> 0:39:21.520
<v Speaker 1>had read probably for like three hours about your mission

0:39:21.840 --> 0:39:26.040
<v Speaker 1>that I googled asteroid Benu, and just every news story

0:39:26.080 --> 0:39:28.440
<v Speaker 1>that came up was like, oh my god, this asteroid

0:39:28.520 --> 0:39:30.680
<v Speaker 1>may hit Earth, and you know, and it just was

0:39:30.719 --> 0:39:33.520
<v Speaker 1>so interesting to me that to see how the media

0:39:33.560 --> 0:39:36.640
<v Speaker 1>had absolutely like blown this so out of proportion for

0:39:36.680 --> 0:39:40.640
<v Speaker 1>a good click baby headline. It does happen. But but

0:39:40.680 --> 0:39:44.440
<v Speaker 1>again typically, and you know, we we scientists, reports the numbers,

0:39:44.560 --> 0:39:47.520
<v Speaker 1>and what people do with those numbers is always you know,

0:39:47.640 --> 0:39:51.000
<v Speaker 1>hard and hard to predict, I guess, but again, they

0:39:51.040 --> 0:39:53.800
<v Speaker 1>tend to come out with with a very higher number,

0:39:53.840 --> 0:39:56.320
<v Speaker 1>you know, one and three thousand chance, but if you

0:39:56.520 --> 0:39:58.960
<v Speaker 1>looked at the uncertainty on that, it's huge, and as

0:39:59.000 --> 0:40:00.920
<v Speaker 1>the uncertainty comes down on you know, it becomes that

0:40:01.000 --> 0:40:04.319
<v Speaker 1>one in a million probability. So you know, we're we're

0:40:04.360 --> 0:40:07.319
<v Speaker 1>again just reporting numbers and people don't necesarily understand how

0:40:07.400 --> 0:40:10.160
<v Speaker 1>we interpret that. But as we get more information, typically

0:40:10.360 --> 0:40:13.799
<v Speaker 1>that chance goes way down. So one last question, and

0:40:13.800 --> 0:40:16.440
<v Speaker 1>this is kind of a weird one, but I'm curious

0:40:16.680 --> 0:40:21.040
<v Speaker 1>is the Cyrus rex team at all concerned about the hypothetical,

0:40:21.160 --> 0:40:26.640
<v Speaker 1>sort of science fiction possibility of planetary contamination from the

0:40:26.719 --> 0:40:31.080
<v Speaker 1>sample being brought back to Earth from Benu. That's actually

0:40:31.080 --> 0:40:34.160
<v Speaker 1>a very good question. Um. So when we have Mars missions,

0:40:34.160 --> 0:40:36.600
<v Speaker 1>we worry about forward contamination. We don't want to bring

0:40:36.680 --> 0:40:40.000
<v Speaker 1>Earth stuff to Mars and which would basically make it

0:40:40.040 --> 0:40:42.360
<v Speaker 1>difficult for us to interpret anything we found on Mars

0:40:42.920 --> 0:40:45.360
<v Speaker 1>in this case, because that surface has been exposed you

0:40:45.400 --> 0:40:48.680
<v Speaker 1>know for um, you know, many millions, billions of years.

0:40:48.680 --> 0:40:51.239
<v Speaker 1>We're not too worried about Earth contamination, although we do

0:40:51.360 --> 0:40:53.839
<v Speaker 1>have a requirement on our spacecraft to keep it very

0:40:53.920 --> 0:40:56.279
<v Speaker 1>very clean because again we want to interpret anything we

0:40:56.320 --> 0:40:59.319
<v Speaker 1>see or find there um. But on the other hand,

0:40:59.400 --> 0:41:02.560
<v Speaker 1>coming back act, so that's you know, backwards contamination Earth

0:41:02.920 --> 0:41:06.000
<v Speaker 1>is important on every sample return mission, and so this

0:41:06.080 --> 0:41:09.520
<v Speaker 1>actually goes into a Level four biohazard lab. It'll be

0:41:09.600 --> 0:41:13.680
<v Speaker 1>yet basically a sealed container and it won't be opened

0:41:13.719 --> 0:41:16.840
<v Speaker 1>until it's in a very special safe lab. Not because

0:41:16.840 --> 0:41:19.880
<v Speaker 1>we're worried about space microbes or anything really, but mostly

0:41:19.920 --> 0:41:22.480
<v Speaker 1>we don't want to contaminate our sample. Um. But we

0:41:22.680 --> 0:41:25.960
<v Speaker 1>we do have requirements on how the sample is handled.

0:41:26.160 --> 0:41:28.560
<v Speaker 1>And there's a whole Planetary Protection office that now, so

0:41:28.600 --> 0:41:30.800
<v Speaker 1>that's dedicated to this topic and tells us what we

0:41:30.920 --> 0:41:33.480
<v Speaker 1>must do to make sure that we don't have contamination

0:41:33.520 --> 0:41:36.080
<v Speaker 1>in either direction. Oh okay, wow. I thought that this

0:41:36.160 --> 0:41:38.640
<v Speaker 1>was just maybe some kind of thing that I had

0:41:39.640 --> 0:41:41.360
<v Speaker 1>cooked up in my own head that would be like

0:41:41.400 --> 0:41:43.640
<v Speaker 1>a problem. But it seems like it's a very realistic

0:41:43.680 --> 0:41:46.680
<v Speaker 1>thing that you have your best people working on. Oh. Absolutely,

0:41:46.719 --> 0:41:48.720
<v Speaker 1>you know, And again I wasn't classified as a problem

0:41:48.800 --> 0:41:51.360
<v Speaker 1>so much as we we do have people that that

0:41:51.520 --> 0:41:55.120
<v Speaker 1>worry about such things and and have very strict protocols

0:41:55.120 --> 0:41:58.440
<v Speaker 1>and procedures in place, just even to ensure the integrity

0:41:58.440 --> 0:42:01.680
<v Speaker 1>of the science. That's great now in terms of of

0:42:02.040 --> 0:42:05.640
<v Speaker 1>missions that have essentially you reached out into space and

0:42:05.719 --> 0:42:09.200
<v Speaker 1>brought back material samples. Just to give everyone a little

0:42:09.239 --> 0:42:11.600
<v Speaker 1>little more scope, like how does that how does this

0:42:11.680 --> 0:42:13.719
<v Speaker 1>fit in with the with the collection of samples, Like

0:42:13.760 --> 0:42:17.160
<v Speaker 1>how how many different samples roughly have been brought back

0:42:18.280 --> 0:42:23.200
<v Speaker 1>from asteroids or the moon, et cetera. So during the

0:42:23.239 --> 0:42:25.440
<v Speaker 1>Apollo years we brought back quite a few moon rocks.

0:42:25.440 --> 0:42:28.040
<v Speaker 1>So that's that's a pretty big cache of of samples

0:42:28.120 --> 0:42:29.440
<v Speaker 1>right there. But in that case, you know, we had

0:42:29.440 --> 0:42:31.560
<v Speaker 1>astronauts who could pick them up and bring them back,

0:42:31.600 --> 0:42:34.879
<v Speaker 1>so we could bring back um, I want to stay

0:42:34.920 --> 0:42:37.520
<v Speaker 1>on the order of of rocks. I'm not sure the

0:42:37.520 --> 0:42:41.000
<v Speaker 1>exact number, but in terms of actually doing this robotically,

0:42:41.120 --> 0:42:42.840
<v Speaker 1>that's been a lot more of a challenge because you

0:42:42.840 --> 0:42:44.120
<v Speaker 1>have to figure out how are you going to pick

0:42:44.160 --> 0:42:47.000
<v Speaker 1>these things up. And so we have samples from the

0:42:47.000 --> 0:42:49.880
<v Speaker 1>Stardust mission, which essentially used what's called aero jail to

0:42:49.960 --> 0:42:53.560
<v Speaker 1>catch dust screens that flew into the spacecraft. Um, it's

0:42:53.760 --> 0:42:58.120
<v Speaker 1>very tiny, tiny amounts. Uh in Genesis also did something similar,

0:42:58.600 --> 0:43:01.600
<v Speaker 1>and then the Japanese mission how Abusa, brought back some

0:43:01.680 --> 0:43:04.080
<v Speaker 1>grains from an asteroid surface, but again it was kind

0:43:04.080 --> 0:43:07.680
<v Speaker 1>of just what they could capture without touching. Uh. This

0:43:07.760 --> 0:43:09.360
<v Speaker 1>is the first mission that's actually going to try to

0:43:09.360 --> 0:43:11.560
<v Speaker 1>touch the surface and pick up a pretty big sample,

0:43:11.680 --> 0:43:13.440
<v Speaker 1>and so we can bring up we have a requirement

0:43:13.480 --> 0:43:16.560
<v Speaker 1>for sixty grams, but we can pick up to two

0:43:17.040 --> 0:43:19.960
<v Speaker 1>of soil and rocks at small rocks, and so you

0:43:20.000 --> 0:43:21.840
<v Speaker 1>know that's our goal is to have a pretty big sample.

0:43:22.080 --> 0:43:23.960
<v Speaker 1>This will be the first time we've done that robotically.

0:43:25.200 --> 0:43:27.439
<v Speaker 1>All right, Amy, Well, thank you for joining us here

0:43:27.480 --> 0:43:30.400
<v Speaker 1>on Stuffed to Boil your Mind. We really enjoyed getting

0:43:30.400 --> 0:43:32.719
<v Speaker 1>to pick your brain a bit about this. Uh, this

0:43:33.040 --> 0:43:35.880
<v Speaker 1>just really fascinating mission. Well, thank you so much for

0:43:35.920 --> 0:43:47.239
<v Speaker 1>having me on. All right, so there you have it,

0:43:47.280 --> 0:43:51.319
<v Speaker 1>an introduction to this fascinating mission o Cyrus Rex. We've

0:43:51.360 --> 0:43:53.920
<v Speaker 1>got to discuss the craft, the destination and we got

0:43:53.960 --> 0:43:56.040
<v Speaker 1>to talk to an expert about it. And if you

0:43:56.120 --> 0:43:58.759
<v Speaker 1>want more information about it, if you want to just

0:43:58.840 --> 0:44:01.239
<v Speaker 1>really get into the nitty ready and just follow the

0:44:01.600 --> 0:44:05.239
<v Speaker 1>Osiris Rex odyssey, you can head on over to Asteroid

0:44:05.360 --> 0:44:09.360
<v Speaker 1>Mission dot org. Yeah, they have tons of materials on

0:44:09.400 --> 0:44:12.440
<v Speaker 1>their NASA's public relations team is working over time to

0:44:12.560 --> 0:44:15.880
<v Speaker 1>educate us the public about what they're doing with this mission.

0:44:15.880 --> 0:44:18.200
<v Speaker 1>They have like stream of blog posts up to the

0:44:18.280 --> 0:44:21.840
<v Speaker 1>Dave videos and it's it's really cool. Uh And I,

0:44:22.239 --> 0:44:24.239
<v Speaker 1>you know, honestly wish that we had had more time

0:44:24.280 --> 0:44:26.399
<v Speaker 1>with it, but I took a good three or four

0:44:26.400 --> 0:44:28.880
<v Speaker 1>hours with it to get us prep to talk to Amy.

0:44:29.120 --> 0:44:32.600
<v Speaker 1>So if you have, you know, maybe some more ideas

0:44:32.640 --> 0:44:35.480
<v Speaker 1>about Osiris Rex, or maybe maybe there's a mission that

0:44:35.600 --> 0:44:37.600
<v Speaker 1>NASA is doing that you think we should cover, or

0:44:37.640 --> 0:44:40.120
<v Speaker 1>there's something more space related that you'd like us to cover,

0:44:40.160 --> 0:44:43.120
<v Speaker 1>because we just did uh moons of Saturn. We've talked

0:44:43.120 --> 0:44:47.440
<v Speaker 1>about Jupiter before I personally would love to take a

0:44:47.480 --> 0:44:51.319
<v Speaker 1>look at Mars' moon Phobos. Oh yeah, there are more

0:44:51.320 --> 0:44:53.960
<v Speaker 1>moons out there, so we have to go check those

0:44:54.000 --> 0:44:56.279
<v Speaker 1>out as well. But if you've got suggestions like that,

0:44:56.400 --> 0:44:58.000
<v Speaker 1>or you just want to reach out to us, you

0:44:58.000 --> 0:45:02.719
<v Speaker 1>can do that on social media. We are on on Facebook, Twitter, Tumbler,

0:45:02.840 --> 0:45:07.000
<v Speaker 1>and Instagram, all those platforms. Pretty much our handle is

0:45:07.040 --> 0:45:09.040
<v Speaker 1>blow the Mind. It might be a little bit different,

0:45:09.080 --> 0:45:12.120
<v Speaker 1>but you'll find us if you search for that. Uh,

0:45:12.160 --> 0:45:14.719
<v Speaker 1>and you can always go to stuff to Blow your

0:45:14.719 --> 0:45:18.960
<v Speaker 1>Mind dot com. That is the mothership where we have everything,

0:45:19.080 --> 0:45:22.719
<v Speaker 1>every podcast, every video, every article that we work on

0:45:22.719 --> 0:45:25.480
<v Speaker 1>on these things. Not to mention that those social media

0:45:25.560 --> 0:45:29.120
<v Speaker 1>feeds have us sharing all the weird science stuff that

0:45:29.160 --> 0:45:32.279
<v Speaker 1>we come across throughout the week as well. Indeed, and

0:45:32.320 --> 0:45:33.520
<v Speaker 1>if you want to get in touch with us the

0:45:33.560 --> 0:45:35.120
<v Speaker 1>old fashioned way, if you want to hit us up

0:45:35.120 --> 0:45:37.759
<v Speaker 1>with an email, you can find us at blow the Mind,

0:45:37.800 --> 0:45:49.040
<v Speaker 1>at how stuff works dot com well more. Almost the

0:45:49.120 --> 0:45:51.479
<v Speaker 1>path ands over their topics is a house stoff works

0:45:51.480 --> 0:46:11.160
<v Speaker 1>dot com. The point four point four proper part