WEBVTT - The Dawn Mission

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<v Speaker 1>Brought to you by Toyota. Let's go places. Welcome to

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<v Speaker 1>Forward Thinking. Hey there, and welcome to Forward Thinking, the

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<v Speaker 1>podcast that looks at the future and says Dawn go away,

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<v Speaker 1>No good for you. I'm Jonathan Strickland, I'm Laren Bulk,

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<v Speaker 1>and I'm Joe McCormick. So today we're going to talk

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<v Speaker 1>about space, the final frontier, well one of them, one

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<v Speaker 1>of the final frontiers. I mean there could be a superspace, right, yeah,

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<v Speaker 1>what the space behind space? Uh yeah, we're talking about

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<v Speaker 1>space today because we wanted to talk about NASA's Dawn mission.

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<v Speaker 1>If you've been following the space news, as I know

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<v Speaker 1>a lot of our listeners, do you are aware that

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<v Speaker 1>this spacecraft has gone in orbit around a dwarf planet,

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<v Speaker 1>series in our Solar system and serie that's C E

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<v Speaker 1>R E S No, like the Syria on your phone. Right,

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<v Speaker 1>So if you say Siri, where is Dawn, it says

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<v Speaker 1>it will be in eight hours, and you're thinking, no,

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<v Speaker 1>you're just giving more questions. Uh no, that's not the case.

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<v Speaker 1>We're talking series the planet and that or dwarf planet,

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<v Speaker 1>I should say, And that was after it already visited

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<v Speaker 1>another astronomical body vesta, And so we're gonna talk all

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<v Speaker 1>about what it did, why it's important, and what these

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<v Speaker 1>these actual astronomical bodies are because it's a really cool story.

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<v Speaker 1>Yeah yeah, So I want to start this story off

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<v Speaker 1>pre launch. Okay, all right, so like like you know,

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<v Speaker 1>two thousand like way, pre launch, like circle the formation

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<v Speaker 1>of the Solar System. Okay, that goes back before my calendar. Yes,

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<v Speaker 1>yes it does. None of us like four and a

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<v Speaker 1>half billion years ago or four and a half five

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<v Speaker 1>billion years ago, Yeah, sure, sure, so none of us

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<v Speaker 1>were there. No, I mean I know that away. I

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<v Speaker 1>thought I was going to get away. So it only

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<v Speaker 1>occurred to me to say, because you because you made

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<v Speaker 1>a point of I don't know. Okay, So at any rate,

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<v Speaker 1>the leading theory among astronomers and physicists is that everything

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<v Speaker 1>in our Solar System was once just one big, nebulous

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<v Speaker 1>cloud of of gas and dust and ice um, and

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<v Speaker 1>something would have had to have happened to kickstart the

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<v Speaker 1>formation of all the bodies in the Solar System are

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<v Speaker 1>Sun and planets and moons and asteroids and etcetera. But

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<v Speaker 1>we're not entirely sure what that is, but we think

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<v Speaker 1>it might have been a nearby star going supernova. It's

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<v Speaker 1>really cool, and it's one of those things I didn't

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<v Speaker 1>really think about the idea of, uh, what sort of

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<v Speaker 1>of circumstances would have led to all of these coalescing

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<v Speaker 1>into what we know today, And the idea that it

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<v Speaker 1>had to be or potentially had to be an external

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<v Speaker 1>source of energy is really fascinating. Yeah. I'd often heard

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<v Speaker 1>about the formation of the planets, but but I'd always

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<v Speaker 1>thought about it in terms of how the planets and

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<v Speaker 1>other rocky bodies and and gas giants and things formed

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<v Speaker 1>around the Sun. And so you have the idea of

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<v Speaker 1>the protoplanetary disks. Yeah, yeah, the Sun already being there,

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<v Speaker 1>but of course the Sun has not always been there.

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<v Speaker 1>It had to happen at some points. Yeah. So, so

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<v Speaker 1>the radiation from this explosion could have like squished and

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<v Speaker 1>pushed all the matter in this in this cloud nebula um.

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<v Speaker 1>You know, each bit formally would have been an equilibrium,

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<v Speaker 1>but but suddenly they would be exerting their gravitational force

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<v Speaker 1>on all the other bits in really new exciting ways.

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<v Speaker 1>And so as they started colliding and forming bigger, denser bits,

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<v Speaker 1>they would have started orbiting around each other. And more

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<v Speaker 1>bits would collide until the Sun would form in the center,

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<v Speaker 1>and gradually all the other stuff formed around the Sun's orbit. Yeah,

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<v Speaker 1>rocky bodies, some of them containing liquid water, like okay,

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<v Speaker 1>so not Rocky Balboa. No, not Rocky Horror. Neither of

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<v Speaker 1>those things. Both have exquisite bodies, they do well, and

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<v Speaker 1>they do contain liquid water. That's uh so, that's cool. No,

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<v Speaker 1>rocky planets as we know formed closer to the Sun

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<v Speaker 1>and gash bodies like Jupiter and all of that. Um

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<v Speaker 1>some of them having sort of rocky really icy moons

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<v Speaker 1>formed further out and between Mars and Jupiter. The asteroid

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<v Speaker 1>belt formed instead of an actual planet, which is pretty interesting. Yeah. Yeah.

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<v Speaker 1>The leading theory right now is that not that there

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<v Speaker 1>was a planet therapy and it was destroyed by aliens

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<v Speaker 1>or something like that. Yeah, yeah, pretty much. Um No,

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<v Speaker 1>we think that Jupiter's immense gravity mucked about with the

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<v Speaker 1>planetation formation process and prevented I am inventing new words, Joe. Yes. So,

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<v Speaker 1>in other words, Jupiter, being such an enormous body with

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<v Speaker 1>its own gravitational pull ends up interfering with the process

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<v Speaker 1>that would allow these bits to otherwise glom on together.

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<v Speaker 1>And eventually coalesced to another planet. Yeah. Yeah, it just

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<v Speaker 1>just got right up in its grill, and gravitationally speaking,

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<v Speaker 1>Jupiter is all like that. It does get all up

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<v Speaker 1>in the grill. So um. So. The asteroid belt contains

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<v Speaker 1>lots of bodies of different shapes and sizes and compositions,

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<v Speaker 1>and the two biggest are Vesta and Series. Alright, so

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<v Speaker 1>let's start with Vesta. What do we know about that? Well,

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<v Speaker 1>it is a rocky asteroid. I have heard Vesta has

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<v Speaker 1>more in common with the inner planets of the Solar System. Yes,

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<v Speaker 1>it was formed some like four point five billion years ago.

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<v Speaker 1>It's uh. The apparent surface is of basaltic rock, which

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<v Speaker 1>is what happens when lava cools down really fast. So

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<v Speaker 1>what they think happened is that UM lava would have

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<v Speaker 1>oozed up from the asteroids like hot Chewy set shortly

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<v Speaker 1>after its formation and then cooled down pretty quick after that. Um.

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<v Speaker 1>It was the fourth asteroid ever discovered by human people.

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<v Speaker 1>That happened on March seven, thanks to Henrich William Ober's

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<v Speaker 1>I don't I don't think I said that, right, Heinrich

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<v Speaker 1>Wilhelm Olbers. Okay, thank you, UM of Germany if you

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<v Speaker 1>couldn't figure that out, y'all, Uh, don't feel bad. Jonathan

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<v Speaker 1>served in Kaiser Wilhelm's government shortly after the dinosaurs died out,

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<v Speaker 1>and honestly, my my concept of time is somewhat elastic. Alright, So,

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<v Speaker 1>how how big is this thing? It's pretty big. It

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<v Speaker 1>is not small. It's about about and I'm about to

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<v Speaker 1>read some very very precise numbers here, five hundred and

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<v Speaker 1>seventy eight kilometers by five sixty by four eight in miles.

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<v Speaker 1>That translates to mine by three eight by two eight five.

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<v Speaker 1>So sizeable, very sizeable body. They're not really like planet

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<v Speaker 1>or moon size, but like but you know, bigger than

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<v Speaker 1>a car. Yes, four hundred three miles is significantly larger

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<v Speaker 1>than most vehicles. It's almost a sphere, but does have

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<v Speaker 1>this giant chunk that's four hundred and sixty kilometers or

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<v Speaker 1>two eight five miles across and thirteen kilometers or eight

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<v Speaker 1>miles deep that's missing from the south pole. That now,

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<v Speaker 1>that is one of the things that is particularly interesting

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<v Speaker 1>about this this asteroid body. It was one of the

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<v Speaker 1>reasons why it was a great candidate to send a

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<v Speaker 1>spacecraft to get a closer look because there appears to

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<v Speaker 1>be you know, this is a chunk missing. It's not

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<v Speaker 1>like it formed and it just has this interesting shape.

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<v Speaker 1>It looks like this. This is an area where uh,

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<v Speaker 1>something has forcibly impacted uh Vesta, and we we ended

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<v Speaker 1>up having the entire body reshaped from that impact. I mean,

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<v Speaker 1>that's how massive it was. And also this could end

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<v Speaker 1>up teaching us more about some of the stuff we

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<v Speaker 1>found here on our planet. Right. Uh. Yeah, we think

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<v Speaker 1>that as much as five percent of the meteorites that

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<v Speaker 1>fall to Earth are come from that missing chunk. Fine,

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<v Speaker 1>what's crazy? All meteorites come from this from Vesta, from Vesta. Yeah, yeah,

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<v Speaker 1>whatever happened that knocked that bit out? Uh do you

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<v Speaker 1>know how they determine that? Actually, I do know, and

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<v Speaker 1>I can tell you when we get to the part

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<v Speaker 1>about the Vesta mission. So yeah, So it's one of

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<v Speaker 1>only three non earth bodies that we have a sample

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<v Speaker 1>of here on the planet, that the other two being

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<v Speaker 1>Mars in the moon. Right. So we you know, it's

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<v Speaker 1>so neat that we ended up having this stuff like

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<v Speaker 1>it ended up landing on our planet. We know where

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<v Speaker 1>it from, or at least we we have very strong

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<v Speaker 1>belief that it came from that place. Like there's not

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<v Speaker 1>like a receipt, Like we can't say, like we could

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<v Speaker 1>go back to Vest and return it for credit. But

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<v Speaker 1>we do. But we do know, and I'll talk more

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<v Speaker 1>about how we know when we get to that part

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<v Speaker 1>of the episode. So now we move on also to

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<v Speaker 1>talk about series. The dwarf planet. Yes, uh, like Earth,

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<v Speaker 1>it has a dense core and a lighter crust, and

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<v Speaker 1>we think it might have a lot of ice beneath

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<v Speaker 1>the crust and in the mantle because the crust is

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<v Speaker 1>less dense than Earth's and um also appears to contain

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<v Speaker 1>all of these like water bearing minerals and stuff. Um,

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<v Speaker 1>it might maybe even have just a wee bit of atmosphere,

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<v Speaker 1>but we're not sure. Sort of like a whiff of atmosphere. Yeah, yeah,

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<v Speaker 1>just an idea of acting. You know. It's kind of

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<v Speaker 1>like a restaurant that's just getting started. It's got a

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<v Speaker 1>little bit of an atmosphere, but we haven't really developed

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<v Speaker 1>it yet. This series was the first dwarf planet we

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<v Speaker 1>ever discovered, though. Yes, that happened on January one, eighteen

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<v Speaker 1>o one, thanks to Giuseppe Piazzi of Italy. Excellent pronunciation

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<v Speaker 1>hold on now, would that that would be including Pluto, now,

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<v Speaker 1>wouldn't it that series was actually discovered before Pluto? Yeah, yeah,

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<v Speaker 1>Pluto also being a dwarf planet, pluto status changes on

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<v Speaker 1>a day to day basis. Yeah, it's it's real independable.

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<v Speaker 1>Like we never we never know exactly what we're doing

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<v Speaker 1>dealing with when we talk about Pluto, because by the

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<v Speaker 1>time we record and by the time something publishes, things

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<v Speaker 1>have changed occasionally. So, like we've said, series is about

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<v Speaker 1>nine seventy five kilometers by nine O nine a k

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<v Speaker 1>A six or six by five five sixty five miles.

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<v Speaker 1>It's hard to picture exactly how big that is. Yeah,

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<v Speaker 1>it's bigger than a car, significantly larger than any vehicle. Yes, yeah,

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<v Speaker 1>no it is. It is difficult, right, I have those

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<v Speaker 1>problems too, because that you sit there and you think, like,

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<v Speaker 1>how long would it take me to drive? Ye, this distance?

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<v Speaker 1>That that tends to be the way we tend to

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<v Speaker 1>think about it. Uh yeah, And there's before we send

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<v Speaker 1>a spacecraft there. We had, of course observed these I

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<v Speaker 1>mean obviously that they were discovered in the nineteenth century,

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<v Speaker 1>but we've since made other observations using other equipment. Right, Well,

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<v Speaker 1>we've used telescopes like the Hubble and ground based telescopes

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<v Speaker 1>that are on Earth or close to Earth, and the

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<v Speaker 1>problem with that is when you're looking at very small

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<v Speaker 1>objects that far away, it's hard to resolve them even

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<v Speaker 1>with a very powerful telescope. Right, and there are lots

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<v Speaker 1>of things we could potentially learn from a closer examination,

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<v Speaker 1>which is precisely why these this mission exists, right the

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<v Speaker 1>Dawn mission, the Dawn Mission, the NASA's Dawn mission. So first,

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<v Speaker 1>these are protoplanets, and we know very little about protoplanets

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<v Speaker 1>in general, apart from some hypotheses we have come up with.

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<v Speaker 1>But you know, without going in and taking a closer look,

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<v Speaker 1>you can't really put those hypotheses to the test us

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<v Speaker 1>to see if you're on the right track or if

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<v Speaker 1>you need to adjust the way you were thinking. And

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<v Speaker 1>perhaps there is a different explanation for some of the

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<v Speaker 1>observations you've made. This is the way science works, in

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<v Speaker 1>other words, So that's really exciting. Will literally be learning

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<v Speaker 1>stuff we have not and perhaps could not have anticipated

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<v Speaker 1>as we go into this. We also learn more about

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<v Speaker 1>the formation of our solar system by studying these planets,

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<v Speaker 1>which will give us a few more pieces to that

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<v Speaker 1>puzzle of how we got here, and by we, I

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<v Speaker 1>mean the entire Solar system, not just the people in

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<v Speaker 1>this podcasting studio. UM. So that's really cool, always getting

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<v Speaker 1>more of a complete picture. I doubt we'll ever have

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<v Speaker 1>a complete picture, but we have that desire to continuously

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<v Speaker 1>add to our body of knowledge as far as this goes,

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<v Speaker 1>and I think this will help us add to that. Also,

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<v Speaker 1>the presence of water always leads us to the possibility

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<v Speaker 1>that the planet may have at one time supported life,

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<v Speaker 1>or perhaps there might even be a habitable ocean on Series.

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<v Speaker 1>We'll talk about that a little bit later too, and

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<v Speaker 1>we may discover there. There's one hypothesis that suggests that

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<v Speaker 1>a body like Series and a body like Vesta may

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<v Speaker 1>have been responsible for the way the Earth is right now. Uh,

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<v Speaker 1>and the idea being that something like Series might have

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<v Speaker 1>been the source of the water on Earth, and a

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<v Speaker 1>body like Vesta might have been the source of the

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<v Speaker 1>Earth's iron core. So there's some theories exactly they formed Vultron,

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<v Speaker 1>but Vultron in this case was Earth. So it's again

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<v Speaker 1>it's one of those things where the hypotheses have been proposed,

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<v Speaker 1>but now we get a chance to explore this more

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<v Speaker 1>directly and see if those still hold any you know, value,

0:13:41.880 --> 0:13:44.840
<v Speaker 1>or if in fact we have to re reconsider a thinking.

0:13:45.200 --> 0:13:48.839
<v Speaker 1>So if we're just now reaching series and Series is

0:13:49.040 --> 0:13:51.640
<v Speaker 1>very far away, we must have launched quite a while ago.

0:13:51.720 --> 0:13:55.000
<v Speaker 1>I don't remember this launch. Uh yeah, well, let me

0:13:55.000 --> 0:13:57.319
<v Speaker 1>tell you the story about how this launch came about,

0:13:57.360 --> 0:14:01.000
<v Speaker 1>because it is its own really drum addict tail like

0:14:01.080 --> 0:14:03.680
<v Speaker 1>one that could have easily like there needs to be

0:14:03.920 --> 0:14:08.439
<v Speaker 1>a documentary to explain what happened, because it was one

0:14:08.440 --> 0:14:10.800
<v Speaker 1>of those things where for a while, I'm sure the

0:14:11.840 --> 0:14:15.120
<v Speaker 1>leaders on this project were convinced that it was never

0:14:15.200 --> 0:14:19.960
<v Speaker 1>gonna happen, because they were thinking about launching a mission

0:14:20.120 --> 0:14:23.520
<v Speaker 1>to look at Vesta and Series as early as nineteen two.

0:14:24.320 --> 0:14:26.360
<v Speaker 1>So that's when you said pre launch. That's why my

0:14:26.480 --> 0:14:30.080
<v Speaker 1>go to who first was two thousand and then. Now

0:14:31.000 --> 0:14:35.520
<v Speaker 1>NASA has these pitch periods where different potential missions can

0:14:35.640 --> 0:14:40.320
<v Speaker 1>come and present to various heads at NASA and say

0:14:40.360 --> 0:14:42.440
<v Speaker 1>this is where I think we need to dedicate some

0:14:42.520 --> 0:14:44.880
<v Speaker 1>of our resources. This is the sort of mission I

0:14:44.880 --> 0:14:48.000
<v Speaker 1>think we need to do, and here's why. And they

0:14:48.360 --> 0:14:51.280
<v Speaker 1>the project leaders of what would become the Dawn Mission

0:14:51.920 --> 0:14:58.240
<v Speaker 1>went before NASA three separate times in n but didn't

0:14:58.240 --> 0:15:02.480
<v Speaker 1>receive any interest in their posed mission. It wasn't until

0:15:02.520 --> 0:15:07.680
<v Speaker 1>two thousand, when they were selected as a finalist for

0:15:08.280 --> 0:15:12.320
<v Speaker 1>NASA Discovery Mission that they finally had a chance to

0:15:12.440 --> 0:15:16.880
<v Speaker 1>really uh to to to get like established as a mission.

0:15:16.880 --> 0:15:18.760
<v Speaker 1>So that meant there have been eight years that had

0:15:18.760 --> 0:15:21.080
<v Speaker 1>gone by since they first came up with the idea

0:15:21.400 --> 0:15:23.680
<v Speaker 1>till when NASA was saying, all right, let's really look

0:15:23.680 --> 0:15:26.080
<v Speaker 1>at this as a potential mission, which also meant that

0:15:26.120 --> 0:15:28.320
<v Speaker 1>the idea itself had evolved over those eight years. They

0:15:28.400 --> 0:15:31.720
<v Speaker 1>began to tweak it, perfected, that kind of thing. So

0:15:31.760 --> 0:15:33.640
<v Speaker 1>two thousand crazy. I mean, in that span of time,

0:15:33.680 --> 0:15:36.400
<v Speaker 1>you'd have to imagine even the science that informs the

0:15:36.440 --> 0:15:40.800
<v Speaker 1>mission is probably changing. Yeah, technology of the things that

0:15:40.800 --> 0:15:44.640
<v Speaker 1>we're learning just through other missions, I mean, all of

0:15:44.640 --> 0:15:47.280
<v Speaker 1>that is making an impact. But it gets even crazier.

0:15:47.520 --> 0:15:50.040
<v Speaker 1>So in two thousand they're selected as one of these

0:15:50.080 --> 0:15:53.280
<v Speaker 1>three finalists and there to go to NASA in September

0:15:53.440 --> 0:15:58.400
<v Speaker 1>of two thousand and one. Yeah, two thousand one September,

0:15:58.960 --> 0:16:01.320
<v Speaker 1>so they're going to go and talk to NASA when

0:16:01.480 --> 0:16:05.840
<v Speaker 1>the terrorist attack happens and it cancels their meeting obviously,

0:16:05.960 --> 0:16:09.520
<v Speaker 1>I mean everything, everything, everything was canceled because of that.

0:16:09.680 --> 0:16:13.680
<v Speaker 1>So everyone goes home and the mission and it's it's

0:16:13.840 --> 0:16:17.160
<v Speaker 1>future is put on hold. But after a while things

0:16:17.200 --> 0:16:19.120
<v Speaker 1>got back on track. The mission was picked up to

0:16:19.120 --> 0:16:21.520
<v Speaker 1>be a Discovery mission, so it went from finalists who

0:16:21.600 --> 0:16:25.240
<v Speaker 1>picked for a Discovery mission. So now it's ready to go.

0:16:25.840 --> 0:16:28.920
<v Speaker 1>On Christmas Eve two thousand three, the project has canceled

0:16:29.080 --> 0:16:31.880
<v Speaker 1>due to budget cuts on Christmas Eve. On Christmas Eve,

0:16:32.040 --> 0:16:36.800
<v Speaker 1>but Mr screws Right apparently whoever was in charge of

0:16:36.840 --> 0:16:40.480
<v Speaker 1>the budget was visited by three Spirits and reconsidered. And

0:16:40.560 --> 0:16:44.280
<v Speaker 1>also another big thing that happened was the project partner,

0:16:44.520 --> 0:16:49.280
<v Speaker 1>Orbital Sciences Corporation, offered to continue working on the mission

0:16:49.440 --> 0:16:53.760
<v Speaker 1>at cost, so not not charging anything that would result

0:16:53.800 --> 0:16:57.880
<v Speaker 1>in a profit, but providing their their part at cost

0:16:58.000 --> 0:17:01.080
<v Speaker 1>if it would mean the mission could continue. And things

0:17:01.120 --> 0:17:04.440
<v Speaker 1>kept moving. Two thousand five, so we're still not into

0:17:04.440 --> 0:17:07.679
<v Speaker 1>the point where anything is launched yet. Two five it

0:17:07.720 --> 0:17:10.240
<v Speaker 1>gets in trouble again. The projects in trouble again because

0:17:10.520 --> 0:17:14.640
<v Speaker 1>NASA administration changed. Now I don't know if you guys

0:17:14.720 --> 0:17:17.160
<v Speaker 1>have ever you know, we we've experienced this a little

0:17:17.200 --> 0:17:19.040
<v Speaker 1>bit in our company. Just one of those moments where

0:17:19.080 --> 0:17:21.200
<v Speaker 1>you don't really know what's going to happen because there's

0:17:21.240 --> 0:17:24.159
<v Speaker 1>a big change of leadership way above your pay grade,

0:17:24.560 --> 0:17:26.280
<v Speaker 1>and you just don't know how that's going to trickle

0:17:26.280 --> 0:17:28.920
<v Speaker 1>down and affect you. We've been very fortunate here and

0:17:28.960 --> 0:17:32.800
<v Speaker 1>how stuff works. Um, but I have also been at

0:17:32.800 --> 0:17:36.600
<v Speaker 1>other jobs where a big boss has changed and suddenly

0:17:36.640 --> 0:17:39.119
<v Speaker 1>everyone feels like they're defending their job, like they have to,

0:17:39.240 --> 0:17:42.680
<v Speaker 1>they have to justify why their job exists. The same

0:17:42.720 --> 0:17:45.080
<v Speaker 1>thing is true at NASA with projects where there's a

0:17:45.080 --> 0:17:48.840
<v Speaker 1>big administrative change in NASA, often you have people who

0:17:48.920 --> 0:17:52.960
<v Speaker 1>have to defend their missions, their projects to the new

0:17:53.000 --> 0:17:56.200
<v Speaker 1>administration to convince them that this is in fact worthy

0:17:56.280 --> 0:18:01.120
<v Speaker 1>of funding. And that started up again. So the project

0:18:01.119 --> 0:18:05.440
<v Speaker 1>got shut down two thousand six, but the Jet Propulsion

0:18:05.560 --> 0:18:09.600
<v Speaker 1>Laboratory protested the shutdown. There was a review, and as

0:18:09.640 --> 0:18:13.880
<v Speaker 1>a result of the review, the project was reinstated. So

0:18:13.960 --> 0:18:15.760
<v Speaker 1>this this is just like I mean, this is in

0:18:15.800 --> 0:18:19.720
<v Speaker 1>a way, this part is more crazy than any of

0:18:19.760 --> 0:18:22.640
<v Speaker 1>the science and technology behind it. It's just the fact

0:18:22.640 --> 0:18:24.480
<v Speaker 1>that all these hoops had to be jumped through in

0:18:24.560 --> 0:18:27.120
<v Speaker 1>order for this to even happen. So at two thousand seven,

0:18:27.119 --> 0:18:30.480
<v Speaker 1>the project finally got full approval, full backing from Nasson.

0:18:30.520 --> 0:18:34.000
<v Speaker 1>It was officially official and stuff. So the team had

0:18:34.000 --> 0:18:36.600
<v Speaker 1>hoped to launch the spacecraft between June and July two

0:18:36.640 --> 0:18:40.640
<v Speaker 1>thousand seven, but bad weather scrapped those plans. I know, right,

0:18:41.359 --> 0:18:43.840
<v Speaker 1>It's like there was a black cat that crossed the road.

0:18:44.119 --> 0:18:45.600
<v Speaker 1>They had to go. They had to They had the

0:18:45.600 --> 0:18:51.399
<v Speaker 1>wheel the Dawn spacecraft under a couple of mirrors broke

0:18:51.440 --> 0:18:54.600
<v Speaker 1>on the way there. It was just crazy. But they

0:18:54.640 --> 0:18:57.840
<v Speaker 1>were able to push the launch back to September two

0:18:57.960 --> 0:19:00.600
<v Speaker 1>thousand seven, and and it did go up. It did,

0:19:00.640 --> 0:19:02.919
<v Speaker 1>It did go up. Everything was fine. And here's the

0:19:02.920 --> 0:19:06.080
<v Speaker 1>cool thing. So you know, we talk about things like

0:19:06.080 --> 0:19:08.480
<v Speaker 1>like missions to Mars and how you have a limited

0:19:08.520 --> 0:19:10.800
<v Speaker 1>window when you can launch right because of the way

0:19:10.840 --> 0:19:12.720
<v Speaker 1>that Mars and Earth line up in there, and you

0:19:12.760 --> 0:19:15.120
<v Speaker 1>want to get them when the right so that way

0:19:15.160 --> 0:19:18.120
<v Speaker 1>you are expending the least amount of fuel and thus

0:19:18.160 --> 0:19:20.160
<v Speaker 1>you have you don't have to have too, you don't

0:19:20.160 --> 0:19:22.359
<v Speaker 1>have to add more weight to your launch vehicle. There

0:19:22.359 --> 0:19:23.680
<v Speaker 1>are a lot of reasons, right, I mean, it's a

0:19:23.800 --> 0:19:27.359
<v Speaker 1>very big picture kind of thing. The Dawn spacecraft had

0:19:27.400 --> 0:19:29.920
<v Speaker 1>a little bit more flexibility because it doesn't depend upon

0:19:30.000 --> 0:19:36.120
<v Speaker 1>chemical rockets for its propulsion in space. Ion propulsion drive

0:19:36.200 --> 0:19:40.239
<v Speaker 1>ion thrusters. What. So we've talked like crazy science. I know,

0:19:40.520 --> 0:19:42.520
<v Speaker 1>I know, we've talked about ion thrusters a couple of

0:19:42.560 --> 0:19:45.159
<v Speaker 1>times in the podcast, and there's only been a few,

0:19:45.720 --> 0:19:50.440
<v Speaker 1>relatively few examples of ion thrusters used uh in space missions.

0:19:50.480 --> 0:19:53.760
<v Speaker 1>So here's what an ion thruster is. You use a gas.

0:19:54.200 --> 0:19:56.480
<v Speaker 1>You are energizing a gas. You're essentially bombarding it with

0:19:56.520 --> 0:20:00.480
<v Speaker 1>electrons so that those electrons can freely roam in at gas.

0:20:00.480 --> 0:20:03.680
<v Speaker 1>That's that's where it becomes ionized. I can actually conduct

0:20:03.680 --> 0:20:08.680
<v Speaker 1>electricity that way. The Dawn spacecraft uses xenon gas and

0:20:08.960 --> 0:20:14.680
<v Speaker 1>it emits this charged ion gas as exhaust, So that

0:20:14.800 --> 0:20:19.120
<v Speaker 1>is what actually creates the propulsion, which is really neat.

0:20:19.400 --> 0:20:23.119
<v Speaker 1>It means also that it has a very gentle but

0:20:23.280 --> 0:20:29.040
<v Speaker 1>steady acceleration, so it doesn't chemical rockets can accelerate very rapidly, right,

0:20:29.400 --> 0:20:34.840
<v Speaker 1>and you can make these incredibly uh powerful motions, whereas

0:20:34.880 --> 0:20:39.960
<v Speaker 1>ion thrusters, they are much more gradual in their acceleration.

0:20:40.400 --> 0:20:43.080
<v Speaker 1>The flip side of that is that the top speed

0:20:43.119 --> 0:20:45.920
<v Speaker 1>for a chemical rocket is much lower than the top

0:20:45.960 --> 0:20:48.000
<v Speaker 1>speed for an ion thruster, because even though an ion

0:20:48.040 --> 0:20:51.480
<v Speaker 1>thruster is going to take longer to accelerate to a

0:20:51.520 --> 0:20:54.800
<v Speaker 1>really fast speed, it can continue to do so much

0:20:54.880 --> 0:20:57.560
<v Speaker 1>longer than a chemical rocket, like like a factor of

0:20:57.680 --> 0:21:02.000
<v Speaker 1>ten more because it like uses its fuel more slowly.

0:21:02.200 --> 0:21:06.160
<v Speaker 1>And also it just it has a continuous acceleration acceleration

0:21:06.240 --> 0:21:08.520
<v Speaker 1>thrust as opposed to chemical rockets where you get that

0:21:08.520 --> 0:21:11.920
<v Speaker 1>that amazing amount thrust at the beginning, but it's not

0:21:12.040 --> 0:21:15.679
<v Speaker 1>something that can continue perpetually because then you use up

0:21:15.680 --> 0:21:19.360
<v Speaker 1>all your fuel. So yeah, very much, it's very much

0:21:19.400 --> 0:21:22.719
<v Speaker 1>like it's because it's it's making very very good use

0:21:22.720 --> 0:21:24.120
<v Speaker 1>of the fuel. But this is the sort of thing

0:21:24.160 --> 0:21:28.879
<v Speaker 1>that is not necessarily going to work well for every mission.

0:21:28.960 --> 0:21:32.080
<v Speaker 1>It's good for particular ones, like like the Dawn mission.

0:21:32.119 --> 0:21:34.840
<v Speaker 1>It's a it's a perfect implementation for the Dawn mission,

0:21:34.840 --> 0:21:36.800
<v Speaker 1>and it has turned out to be that way. So

0:21:36.840 --> 0:21:41.200
<v Speaker 1>the ion thrusters came online on October sixth, two thousand seven,

0:21:41.840 --> 0:21:45.360
<v Speaker 1>and from the Dawn Mission Journal entry for October seven,

0:21:45.480 --> 0:21:47.280
<v Speaker 1>two thousand seven. By the way, the I don't know

0:21:47.320 --> 0:21:48.520
<v Speaker 1>if you guys had a chance to look at the

0:21:48.560 --> 0:21:51.760
<v Speaker 1>mission journal at all. But the the project leader from

0:21:51.840 --> 0:21:56.199
<v Speaker 1>Jet Provulsion Laboratories who wrote the mission journal, he is

0:21:56.240 --> 0:21:59.200
<v Speaker 1>a poet as well as an engineer, like he uses

0:21:59.240 --> 0:22:02.480
<v Speaker 1>such poetic language to explain what is happening and the

0:22:02.960 --> 0:22:06.000
<v Speaker 1>you know, like the the that there are now two

0:22:07.280 --> 0:22:10.919
<v Speaker 1>uh to two bodies in the asteroid belt, one brand

0:22:10.920 --> 0:22:14.800
<v Speaker 1>new and one ancient. Beyond words that are rendezvousing. I mean,

0:22:14.800 --> 0:22:17.000
<v Speaker 1>it's like you're reading and like, holy cow, this guy

0:22:17.080 --> 0:22:19.560
<v Speaker 1>must love science fiction because he's got a he's got

0:22:19.560 --> 0:22:22.280
<v Speaker 1>a really eloquent way of putting it. Everyone that I

0:22:22.400 --> 0:22:26.120
<v Speaker 1>that I read, um either interviews or papers from connected

0:22:26.160 --> 0:22:30.440
<v Speaker 1>with this mission, was just delightful to read. It was altering.

0:22:30.560 --> 0:22:34.640
<v Speaker 1>It's not dry engineering text in other words, So if

0:22:34.680 --> 0:22:36.879
<v Speaker 1>you are interested in this, I highly recommend going to

0:22:36.960 --> 0:22:39.560
<v Speaker 1>the NASA website and looking at the mission Journal. But

0:22:39.600 --> 0:22:41.359
<v Speaker 1>this is an excerpt. This one is more of a

0:22:41.400 --> 0:22:45.480
<v Speaker 1>technical explanation of the ion thrusters. While the three ion

0:22:45.560 --> 0:22:48.080
<v Speaker 1>thrusters are the most familiar part of the i p

0:22:48.400 --> 0:22:52.320
<v Speaker 1>S the ion propulsion system, they are not it's only elements.

0:22:52.359 --> 0:22:55.520
<v Speaker 1>The system includes two computer controllers, only one is used

0:22:55.520 --> 0:22:58.440
<v Speaker 1>at a time. When mission control selects one of the

0:22:58.520 --> 0:23:03.560
<v Speaker 1>one hundred twelve throttle levels, each corresponding to a certain

0:23:03.560 --> 0:23:07.760
<v Speaker 1>power consumption and thrust. The operating controller translates the command

0:23:07.840 --> 0:23:11.399
<v Speaker 1>into currents and voltages that must be applied to parts

0:23:11.680 --> 0:23:14.800
<v Speaker 1>of the thruster and the flow rate of xenon propellant

0:23:14.920 --> 0:23:18.680
<v Speaker 1>to the thruster. The controller also provides the principal communications

0:23:18.720 --> 0:23:22.320
<v Speaker 1>between the main spacecraft computer and the rest of the IPS,

0:23:22.359 --> 0:23:26.320
<v Speaker 1>accepting commands and reporting on the IPS performance. While the

0:23:26.320 --> 0:23:29.600
<v Speaker 1>controller is the brain of the system, the two power units,

0:23:29.640 --> 0:23:31.680
<v Speaker 1>again only one is used at the time, are the

0:23:31.720 --> 0:23:35.600
<v Speaker 1>braun Following instructions from the controller. A power unit receives

0:23:35.600 --> 0:23:37.920
<v Speaker 1>power from the solar rays at about one hundred volts

0:23:37.960 --> 0:23:40.639
<v Speaker 1>and converts it to more than one thousand volts for

0:23:40.800 --> 0:23:45.359
<v Speaker 1>use by the thruster. One hundred and twelve throttle levels. Yeah,

0:23:45.400 --> 0:23:49.440
<v Speaker 1>that a hundred and twelve speed bikes. What we're talking about?

0:23:49.040 --> 0:23:53.920
<v Speaker 1>Why doesn't it just go up to one? Because because

0:23:54.240 --> 0:23:59.119
<v Speaker 1>this exactly, I gotta tell you that working the clutch

0:23:59.160 --> 0:24:01.560
<v Speaker 1>gets a little sticky. Between sixty seven and sixty eight,

0:24:01.640 --> 0:24:03.639
<v Speaker 1>it does. Okay, well, you know, you gotta be a

0:24:03.680 --> 0:24:06.639
<v Speaker 1>little careful. Now, everything has its So when it was

0:24:06.800 --> 0:24:10.120
<v Speaker 1>using the ion propulsion as as thrust, which it did

0:24:10.119 --> 0:24:12.440
<v Speaker 1>not do for the entire journey, that would have made

0:24:12.440 --> 0:24:15.359
<v Speaker 1>it go far too fast for by the time it

0:24:15.400 --> 0:24:18.000
<v Speaker 1>was reaching its destination. But when it was using it,

0:24:18.000 --> 0:24:20.679
<v Speaker 1>it was applying thrust on an average of six days

0:24:20.920 --> 0:24:25.320
<v Speaker 1>sixteen hours per week, so out of every week only, uh,

0:24:25.359 --> 0:24:27.520
<v Speaker 1>you know, you had six days and sixteen hours of

0:24:27.560 --> 0:24:31.720
<v Speaker 1>it being used. As as as acceleration, the brakes would

0:24:31.760 --> 0:24:34.639
<v Speaker 1>be used for times when they needed to orient the

0:24:34.680 --> 0:24:37.199
<v Speaker 1>the spacecraft so that the antenna was facing back to

0:24:37.240 --> 0:24:39.480
<v Speaker 1>Earth so they could beam back engineering information just to

0:24:39.480 --> 0:24:43.480
<v Speaker 1>make sure everything was going well. So that communication time

0:24:43.520 --> 0:24:46.280
<v Speaker 1>obviously got longer and longer as the spacecraft got further

0:24:46.440 --> 0:24:50.240
<v Speaker 1>from the Earth. Now, one of the maneuvers that the

0:24:50.320 --> 0:24:55.560
<v Speaker 1>Dawn spacecraft made was one of my favorites in space travel,

0:24:55.680 --> 0:24:59.959
<v Speaker 1>the slingshot maneuver. Yeah, yeah, in February of two thousand nine,

0:25:00.240 --> 0:25:03.840
<v Speaker 1>it kind of ricocheted through Mars orbit in order to

0:25:03.840 --> 0:25:05.960
<v Speaker 1>pick up speed on its way to Vestep right, So

0:25:06.000 --> 0:25:08.720
<v Speaker 1>it uses the gravity well of a planet in order

0:25:08.800 --> 0:25:13.280
<v Speaker 1>to accelerate. Yeah, which is you know, it's that's awesome. Right,

0:25:13.320 --> 0:25:18.120
<v Speaker 1>whenever you can make use of the the actual elements

0:25:18.119 --> 0:25:20.679
<v Speaker 1>of space itself to help you on your journey, and

0:25:20.720 --> 0:25:23.520
<v Speaker 1>that thus reduced the amount of effort you have to

0:25:23.600 --> 0:25:26.400
<v Speaker 1>do yourself. Yeah, it's it's sort of like a it's

0:25:26.400 --> 0:25:29.320
<v Speaker 1>sort of like a skateboarder in a silly action movie,

0:25:29.400 --> 0:25:32.600
<v Speaker 1>kind of like catching the rear bumper of a car

0:25:33.000 --> 0:25:36.960
<v Speaker 1>and then then using that cars forward momentum to to

0:25:37.160 --> 0:25:39.919
<v Speaker 1>drive itself forward faster or and what action movie do

0:25:39.960 --> 0:25:44.920
<v Speaker 1>you have in mind? Back to the future action There

0:25:45.000 --> 0:25:47.320
<v Speaker 1>was no there was no word whether or not Power

0:25:47.320 --> 0:25:51.160
<v Speaker 1>of Love was playing at the same time. So there's

0:25:51.160 --> 0:25:55.680
<v Speaker 1>some other stuff that's aboard. There's some other stuff that's

0:25:55.680 --> 0:25:59.040
<v Speaker 1>aboard the spacecraft. Besides it's it's propulsion thrusters, I mean, yeah,

0:25:59.040 --> 0:26:02.720
<v Speaker 1>getting the soap, getting their nose. Yes, the Dawn mission,

0:26:04.200 --> 0:26:05.880
<v Speaker 1>I was. I was so hoping we could get through

0:26:05.880 --> 0:26:09.280
<v Speaker 1>without having to talk about that. Well, obviously, from the

0:26:09.400 --> 0:26:12.680
<v Speaker 1>amazing images we've seen already, it must have an awesome

0:26:12.760 --> 0:26:18.760
<v Speaker 1>camera and a photographer he's great. Obviously, it's an automated camera. Yes,

0:26:19.119 --> 0:26:22.480
<v Speaker 1>it was made in Germany. Uh, and it does not

0:26:22.720 --> 0:26:25.560
<v Speaker 1>just take those pretty pictures. It's also being used for

0:26:25.840 --> 0:26:30.119
<v Speaker 1>for orbit navigation. Um AND is mapping the surfaces topography

0:26:30.119 --> 0:26:33.400
<v Speaker 1>and can even help us determine what the surfaces of

0:26:33.440 --> 0:26:36.720
<v Speaker 1>these things are made of based on the reflective and

0:26:36.720 --> 0:26:39.679
<v Speaker 1>refractive properties of the stuff down. They're going to be

0:26:39.760 --> 0:26:43.360
<v Speaker 1>very important as we get to it a little bit later. Yes, Um,

0:26:43.400 --> 0:26:48.920
<v Speaker 1>there's also a visible and Infrared Mapping spectrometer UM. That's

0:26:48.960 --> 0:26:53.000
<v Speaker 1>a mapping the body's surfaces and helping determine their composition

0:26:53.000 --> 0:26:56.560
<v Speaker 1>and temperature and properties UM AND and that works of

0:26:56.600 --> 0:26:59.040
<v Speaker 1>course by taking you know, very detailed note of the

0:26:59.080 --> 0:27:03.119
<v Speaker 1>wavelengths of light that the surfaces are reflecting. UM. There's

0:27:03.160 --> 0:27:07.119
<v Speaker 1>also a gamma ray and neutron spectrometer good, so I

0:27:07.160 --> 0:27:10.639
<v Speaker 1>can detect like the Hulk, Yeah, excellent. Yeah, the Hulk

0:27:10.880 --> 0:27:18.639
<v Speaker 1>probably lives on series UM constantly playing that sad music,

0:27:19.359 --> 0:27:21.479
<v Speaker 1>just just blogging with his thumb out and there's no

0:27:21.520 --> 0:27:28.119
<v Speaker 1>one there, sad Hulk um. Uh. These are these are

0:27:28.119 --> 0:27:31.240
<v Speaker 1>good for for determining the precise elements that are present

0:27:31.520 --> 0:27:34.400
<v Speaker 1>on those surfaces and it and it works by measuring

0:27:34.440 --> 0:27:37.520
<v Speaker 1>the effects of energetic particles that are bombarding the surfaces.

0:27:37.560 --> 0:27:40.240
<v Speaker 1>I mean, you know, there are so many particles out

0:27:40.240 --> 0:27:43.919
<v Speaker 1>there in space that are bombarding everything. Um, the researcher

0:27:44.240 --> 0:27:47.080
<v Speaker 1>that I read and an interview from likes to call

0:27:47.119 --> 0:27:50.840
<v Speaker 1>it splat because because that's just what's going on all

0:27:50.920 --> 0:27:55.440
<v Speaker 1>over our galaxy. All yeah, um so uh so yeah,

0:27:55.480 --> 0:27:58.600
<v Speaker 1>so there's radioactive stuff on the surfaces, there's energetic particles

0:27:58.640 --> 0:28:02.680
<v Speaker 1>bombarding the surfaces, and all of those create radiation coming

0:28:02.760 --> 0:28:07.160
<v Speaker 1>up off of the not planet things. I keep wanting

0:28:07.200 --> 0:28:09.280
<v Speaker 1>to say planets, and I'm like, no, they're tot's not planets,

0:28:10.480 --> 0:28:14.080
<v Speaker 1>asteroid and dwarf planet. It just seems like if you

0:28:14.119 --> 0:28:17.440
<v Speaker 1>wanted to be mean, you could say pseudo planets. If

0:28:17.440 --> 0:28:19.840
<v Speaker 1>you want to be If you want to be diplomatic,

0:28:19.920 --> 0:28:25.240
<v Speaker 1>NG say objects objects proto planets, proto planets. At any rate,

0:28:25.280 --> 0:28:28.760
<v Speaker 1>if you very carefully measure that radiation, you can extrapolate

0:28:28.800 --> 0:28:31.879
<v Speaker 1>what must be down there. Um uh you know, either

0:28:31.960 --> 0:28:35.920
<v Speaker 1>being bombarded or or giving off that radiation itself. Uh.

0:28:35.920 --> 0:28:38.880
<v Speaker 1>And then this is my favorite. Uh, they have a

0:28:38.880 --> 0:28:42.400
<v Speaker 1>gravity science unit. I first imagined that this would just

0:28:42.440 --> 0:28:54.520
<v Speaker 1>be an Apple science unit, very little joke grenade for Joe. There. No,

0:28:55.080 --> 0:28:58.800
<v Speaker 1>this this sucker is our way of peeking into the

0:28:58.880 --> 0:29:03.760
<v Speaker 1>objects interiors without actually landing on them UM. And you know,

0:29:03.960 --> 0:29:05.800
<v Speaker 1>you can tell a lot about the inside of a

0:29:05.840 --> 0:29:09.440
<v Speaker 1>space thing by measuring its gravitational field, especially if you've

0:29:09.520 --> 0:29:12.880
<v Speaker 1>got some information about what is on the surface. You

0:29:12.920 --> 0:29:17.120
<v Speaker 1>can extrapolate the density of the thing and therefore the

0:29:17.160 --> 0:29:21.080
<v Speaker 1>composition of the interior based on how the thing is

0:29:21.160 --> 0:29:24.560
<v Speaker 1>pulling and pushing at objects that are near it UM

0:29:24.600 --> 0:29:28.200
<v Speaker 1>And the gravity science unit does this using radio waves UM,

0:29:28.280 --> 0:29:30.720
<v Speaker 1>so it bounces radio waves off of the surface and

0:29:30.760 --> 0:29:33.520
<v Speaker 1>back to the unit in in route that the waves

0:29:33.600 --> 0:29:38.320
<v Speaker 1>get Doppler shifted by the gravity of the thing. So

0:29:38.320 --> 0:29:42.160
<v Speaker 1>so by measuring that Doppler effect really precisely, you can

0:29:42.280 --> 0:29:44.520
<v Speaker 1>figure out how much force the thing is exerting on

0:29:44.600 --> 0:29:47.640
<v Speaker 1>the spacecraft from moment to moment, and then deduce some

0:29:47.760 --> 0:29:50.840
<v Speaker 1>models about what must be in the interior to be

0:29:50.960 --> 0:29:53.040
<v Speaker 1>creating that force. Right, Because of course we know that

0:29:53.080 --> 0:29:58.160
<v Speaker 1>gravity is a function of mass one one part of that, right,

0:29:58.440 --> 0:30:00.760
<v Speaker 1>So the mass is also going to be dependent upon

0:30:01.000 --> 0:30:03.840
<v Speaker 1>what matter is there and the density of that matter.

0:30:03.920 --> 0:30:06.000
<v Speaker 1>So if you're able to measure the gravity, you can

0:30:06.000 --> 0:30:08.880
<v Speaker 1>start to make some good guesses about the nature of

0:30:08.920 --> 0:30:12.520
<v Speaker 1>the matter that is actually there. That's really neat. I

0:30:12.600 --> 0:30:14.680
<v Speaker 1>never really considered it that way, I would have thought

0:30:14.720 --> 0:30:16.360
<v Speaker 1>like I tend to think of it the other way around,

0:30:16.360 --> 0:30:18.240
<v Speaker 1>where you get a good idea of what the matter is,

0:30:18.280 --> 0:30:21.080
<v Speaker 1>and therefore you can guess how how strong the gravitational

0:30:21.120 --> 0:30:22.960
<v Speaker 1>poll is going to be. Actually, wouldn't have to guess.

0:30:22.960 --> 0:30:24.680
<v Speaker 1>You would know if you know what the stuff is

0:30:24.680 --> 0:30:28.480
<v Speaker 1>made of. But that's really really interesting. Uh So let's

0:30:28.520 --> 0:30:31.800
<v Speaker 1>talk a little bit about the Don's mission and its

0:30:31.880 --> 0:30:35.720
<v Speaker 1>encounters with Vesta and with Series. Right, So, before it

0:30:35.800 --> 0:30:39.200
<v Speaker 1>got to Series, which it's orbiting now, it had to

0:30:39.280 --> 0:30:41.800
<v Speaker 1>run in with the asteroid Vesta, not not a little

0:30:42.120 --> 0:30:44.840
<v Speaker 1>literal run in. It didn't know, Yeah, I know, it

0:30:44.960 --> 0:30:49.400
<v Speaker 1>sought Vesta out. This was an intended encounter. They hung

0:30:49.400 --> 0:30:51.560
<v Speaker 1>out for a while, you know, the exchange numbers, that

0:30:51.640 --> 0:30:54.480
<v Speaker 1>kind of thing. Uh. This would have taken place between

0:30:54.520 --> 0:30:58.160
<v Speaker 1>two thousand and eleven two thousand twelve and Yeah. So

0:30:58.200 --> 0:31:00.480
<v Speaker 1>in order to get to Vesta, Don had travel two

0:31:00.520 --> 0:31:05.480
<v Speaker 1>point eight billion kilometers or one point seven billion miles there,

0:31:05.640 --> 0:31:08.040
<v Speaker 1>so longer than the length of a car, longer than

0:31:08.200 --> 0:31:11.960
<v Speaker 1>longer than a car. The journey lasted nearly four years

0:31:12.360 --> 0:31:14.640
<v Speaker 1>to get there. Uh, and it confirmed a lot of

0:31:14.640 --> 0:31:17.160
<v Speaker 1>what we suspected about Vesta, which is fine. Like that

0:31:17.280 --> 0:31:19.200
<v Speaker 1>was again one of those things where we had some

0:31:19.320 --> 0:31:21.760
<v Speaker 1>hypotheses and this is a way of finding out if

0:31:21.840 --> 0:31:23.680
<v Speaker 1>we were on the right track. So one of those

0:31:23.720 --> 0:31:27.360
<v Speaker 1>was that Vesta is related to three classes of meteorites, Howard,

0:31:27.560 --> 0:31:33.040
<v Speaker 1>it's eucrites and diogenites, collectively referred to as H. E.

0:31:33.200 --> 0:31:36.160
<v Speaker 1>D meteorites. I've never heard of these before. Do you

0:31:36.200 --> 0:31:39.920
<v Speaker 1>know what the differences? Well, there used to be shimp bights,

0:31:40.120 --> 0:31:43.880
<v Speaker 1>but he left and was replaced by diagenites. Come on, now,

0:31:47.040 --> 0:31:50.360
<v Speaker 1>you made a dawn dish, all right. So the giant

0:31:50.400 --> 0:31:52.560
<v Speaker 1>crater at the south pole of Vesta that Lauren was

0:31:52.600 --> 0:31:55.040
<v Speaker 1>talking about earlier, it did suggest that perhaps there was

0:31:55.080 --> 0:31:58.200
<v Speaker 1>some sort of enormous impact that blasted a huge chunk

0:31:58.280 --> 0:32:00.640
<v Speaker 1>off of Vesta, and at that chunk either are broken

0:32:00.680 --> 0:32:03.760
<v Speaker 1>too smaller pieces, many of which ended up entering Earth's

0:32:03.760 --> 0:32:07.680
<v Speaker 1>atmosphere and became meteorites. And this was a way of saying,

0:32:07.800 --> 0:32:09.600
<v Speaker 1>let's take a closer look and see if that in

0:32:09.680 --> 0:32:14.760
<v Speaker 1>fact is accurate. They use spectral analysis essentially, because we

0:32:14.840 --> 0:32:20.640
<v Speaker 1>knew what the meteorites were made of. They're on Earth exactly. Yeah,

0:32:20.640 --> 0:32:22.760
<v Speaker 1>we had a real good look at them, and so

0:32:22.960 --> 0:32:26.720
<v Speaker 1>using spectral analysis originally from things like the Hubble telescope,

0:32:26.760 --> 0:32:29.360
<v Speaker 1>it looked like the Vesta was a really good candidate.

0:32:29.400 --> 0:32:31.760
<v Speaker 1>And then using the closer look with Don we were

0:32:31.800 --> 0:32:34.320
<v Speaker 1>able to say that, yeah, it does look like this

0:32:34.360 --> 0:32:38.560
<v Speaker 1>stuff is in fact, uh, the same, the exact same

0:32:38.600 --> 0:32:41.120
<v Speaker 1>stuff that we found back on Earth. All of that

0:32:41.200 --> 0:32:44.800
<v Speaker 1>seems to be holding true, So that hypothesis looks like

0:32:44.960 --> 0:32:49.320
<v Speaker 1>it's pretty accurate now. Also, we saw that Vesta seems

0:32:49.320 --> 0:32:52.320
<v Speaker 1>to have kind of like an onion like layering, and

0:32:52.360 --> 0:32:57.800
<v Speaker 1>these different layers have different densities and compositions. So a

0:32:57.920 --> 0:32:59.720
<v Speaker 1>big chunks you know you talked about how it was

0:32:59.720 --> 0:33:02.600
<v Speaker 1>eight aisles deep on that south pole means that several

0:33:02.680 --> 0:33:05.720
<v Speaker 1>layers are represented by those meteorites. That's why we get

0:33:05.800 --> 0:33:08.640
<v Speaker 1>different types of stuff. It's like almost on the way

0:33:08.680 --> 0:33:13.760
<v Speaker 1>to be in a blooman onion exactly. Well, we're totally

0:33:14.120 --> 0:33:16.240
<v Speaker 1>goofing off on this one. I love it, by the way,

0:33:16.280 --> 0:33:18.680
<v Speaker 1>I'm not I'm not criticizing. I'm having a good time.

0:33:19.480 --> 0:33:23.720
<v Speaker 1>So the mission also found evidence of hydrated materials, which

0:33:23.760 --> 0:33:26.240
<v Speaker 1>sounds exactly what it what you you know, it means

0:33:26.240 --> 0:33:28.880
<v Speaker 1>what you think it means hydrated, means there's some sort

0:33:28.920 --> 0:33:32.640
<v Speaker 1>of water involved, whether it's water that's captured within certain minerals,

0:33:32.880 --> 0:33:35.920
<v Speaker 1>not water like water pooling on the surface of Vesta,

0:33:35.920 --> 0:33:38.840
<v Speaker 1>because Vesta was believed to be way too hot and

0:33:38.840 --> 0:33:42.000
<v Speaker 1>and not hydrated like hail hydrated. No, not that kind

0:33:42.000 --> 0:33:44.640
<v Speaker 1>of cut cut off one meteorite and tool rise to

0:33:44.640 --> 0:33:47.080
<v Speaker 1>take its place. That's not the way it works. Sorry

0:33:47.160 --> 0:33:49.920
<v Speaker 1>I interact. No, it's fine, but but one of the

0:33:50.000 --> 0:33:52.600
<v Speaker 1>things about that is that the Howardites class of meteorites

0:33:52.640 --> 0:33:56.680
<v Speaker 1>have carbonaceous material in it, meaning that it's carbon rich. Now,

0:33:56.720 --> 0:33:58.320
<v Speaker 1>carbon rich is one of those things you would not

0:33:58.440 --> 0:34:00.880
<v Speaker 1>expect to find on a body like Vesta. You wouldn't

0:34:00.880 --> 0:34:04.040
<v Speaker 1>expect to find water or carbon rich material. So what's

0:34:04.120 --> 0:34:07.640
<v Speaker 1>up with that? I just said that it looks like H. E. D.

0:34:07.800 --> 0:34:12.640
<v Speaker 1>Meteorites have originated from this massive collision that happened in

0:34:12.719 --> 0:34:15.360
<v Speaker 1>Vesta's past. How could that be if, in fact this

0:34:15.400 --> 0:34:18.480
<v Speaker 1>planet wouldn't have had carbon rich material or water on it. Well,

0:34:18.880 --> 0:34:22.680
<v Speaker 1>the thought is that whatever slammed into it did have

0:34:22.840 --> 0:34:26.399
<v Speaker 1>carbon rich material and water on it, and so some

0:34:26.480 --> 0:34:29.120
<v Speaker 1>of it ended up going off into space and becoming

0:34:29.400 --> 0:34:32.560
<v Speaker 1>other chunks of rock eventually becoming meteorites that land here

0:34:32.600 --> 0:34:34.680
<v Speaker 1>on Earth, and some of it said I think I'll

0:34:34.719 --> 0:34:37.240
<v Speaker 1>stick around. Yeah, So if you look at the pictures

0:34:37.239 --> 0:34:39.680
<v Speaker 1>of Vesta, you will see in some of the images

0:34:39.719 --> 0:34:42.520
<v Speaker 1>they'll be darker spots along it that tends to be

0:34:42.560 --> 0:34:46.520
<v Speaker 1>that carbonaceous material, the the type of meteorites or the

0:34:46.520 --> 0:34:50.160
<v Speaker 1>type of rocks that were mentioning here. And so it's

0:34:50.600 --> 0:34:53.000
<v Speaker 1>they a lot of the study I've read, people have

0:34:53.120 --> 0:34:56.680
<v Speaker 1>suggested that they didn't originate on Vesta. This was stuff

0:34:56.719 --> 0:34:59.600
<v Speaker 1>that was deposited on Vesta as a resort, the result

0:35:00.080 --> 0:35:03.520
<v Speaker 1>of collisions. So I thought that was pretty cool. Yeah. Yeah.

0:35:03.760 --> 0:35:07.520
<v Speaker 1>Of course after it left Vesta, Dawn was on track

0:35:07.560 --> 0:35:09.760
<v Speaker 1>to meet up with Series. So right now the Dawn

0:35:09.800 --> 0:35:14.240
<v Speaker 1>spacecraft is has entered Series orbit. It entered on March sixth,

0:35:14.280 --> 0:35:17.359
<v Speaker 1>I believe, or did it in around March six There

0:35:17.400 --> 0:35:18.759
<v Speaker 1>is that one we found out about it, or I

0:35:18.800 --> 0:35:21.000
<v Speaker 1>guess would be the same time. It's not that far away,

0:35:21.239 --> 0:35:23.360
<v Speaker 1>It's not it's not all that far away, um, I

0:35:23.400 --> 0:35:25.160
<v Speaker 1>mean it is very far away. It's not so far

0:35:25.239 --> 0:35:27.560
<v Speaker 1>that it would take us like days to the radio.

0:35:28.000 --> 0:35:30.799
<v Speaker 1>I mean even even in Mars. You're talking like less

0:35:30.800 --> 0:35:33.360
<v Speaker 1>than twenty minutes to get the information. Okay, okay, So

0:35:33.920 --> 0:35:37.680
<v Speaker 1>it entered orbit around Series. Now on the approach, it

0:35:37.800 --> 0:35:41.880
<v Speaker 1>started getting some really good pictures of Series. On Monday,

0:35:42.000 --> 0:35:46.399
<v Speaker 1>January nineteen, so a few months ago, NASA released some

0:35:46.520 --> 0:35:51.799
<v Speaker 1>photos of Series that were taken on Janu and it

0:35:51.840 --> 0:35:55.799
<v Speaker 1>was blurry, but you could clearly see, for example, a

0:35:55.920 --> 0:36:00.200
<v Speaker 1>white spot on the surface of Series. It's something that

0:36:00.200 --> 0:36:03.800
<v Speaker 1>seemed to be reflecting way more sunlight than the rest

0:36:03.840 --> 0:36:06.480
<v Speaker 1>of the surface of the object. And this wasn't the

0:36:06.480 --> 0:36:09.000
<v Speaker 1>first time that we realized there was a bright spot

0:36:09.040 --> 0:36:11.399
<v Speaker 1>on the surface of Series, but suddenly we could see

0:36:11.440 --> 0:36:14.480
<v Speaker 1>it a lot more starkly than ever before. And a

0:36:14.480 --> 0:36:17.160
<v Speaker 1>lot of people started asking what is it. And it's

0:36:17.200 --> 0:36:20.319
<v Speaker 1>really cool because initially the scientists said, we don't know.

0:36:20.520 --> 0:36:24.160
<v Speaker 1>My thought was that it was the Hulk. He had

0:36:24.200 --> 0:36:27.960
<v Speaker 1>fashioned a very highly reflective sign because the thumb sticking

0:36:27.960 --> 0:36:30.440
<v Speaker 1>out wasn't working out and it said will work for

0:36:30.520 --> 0:36:34.400
<v Speaker 1>gamma rays. Nice well. So there have been subsequent photos

0:36:34.440 --> 0:36:37.279
<v Speaker 1>taken with better resolution and still we don't know. We

0:36:37.320 --> 0:36:39.600
<v Speaker 1>don't know what it is. It Uh. It turns out

0:36:39.640 --> 0:36:42.279
<v Speaker 1>there are actually multiple spots on the surface that have

0:36:42.360 --> 0:36:46.600
<v Speaker 1>a much higher albedo a higher reflective index um than

0:36:46.680 --> 0:36:49.080
<v Speaker 1>the rest of the surface, and the main bright spot

0:36:49.080 --> 0:36:52.399
<v Speaker 1>actually has a sort of dimmer companion right next to it.

0:36:52.760 --> 0:36:55.759
<v Speaker 1>There are other bright freckles. I've seen them called on

0:36:55.800 --> 0:36:58.360
<v Speaker 1>the surface of series. You should check out the photos.

0:36:58.400 --> 0:36:59.920
<v Speaker 1>If you haven't seen them, look this up because it

0:37:00.040 --> 0:37:02.719
<v Speaker 1>looks really cool and really strange and people don't know

0:37:02.760 --> 0:37:04.960
<v Speaker 1>the answer yet. Yeah. I love the one that has

0:37:05.040 --> 0:37:07.640
<v Speaker 1>the pair of the spots, the bright one and the

0:37:07.719 --> 0:37:11.359
<v Speaker 1>slightly dimmer companion that are very close together. Like if

0:37:11.400 --> 0:37:13.600
<v Speaker 1>you weren't if your vision wasn't good, you might think

0:37:13.600 --> 0:37:16.040
<v Speaker 1>it's one spot, but it's too. It is too when

0:37:16.040 --> 0:37:20.239
<v Speaker 1>you look at it more closely, and it is strangely

0:37:20.280 --> 0:37:23.080
<v Speaker 1>compelling to see because it almost looks like light is

0:37:23.120 --> 0:37:28.080
<v Speaker 1>being admitted from there. They're very bright. Space dot Com

0:37:28.160 --> 0:37:31.280
<v Speaker 1>wrote this up when when the new higher resolution photos

0:37:31.280 --> 0:37:33.320
<v Speaker 1>come out and they got a statement from Mark Raymond,

0:37:33.360 --> 0:37:36.440
<v Speaker 1>the Dawn mission director and chief engineer, and I love

0:37:36.520 --> 0:37:38.960
<v Speaker 1>this quote. He said, we do not know what the

0:37:38.960 --> 0:37:41.799
<v Speaker 1>white spot is, but it's certainly intriguing. In fact, it

0:37:41.840 --> 0:37:43.880
<v Speaker 1>makes you want to send a spacecraft out there to

0:37:43.920 --> 0:37:48.200
<v Speaker 1>find out. Okay, look what we do. Yeah, yeah, and

0:37:48.200 --> 0:37:50.400
<v Speaker 1>that's what he said, and of course that's exactly what

0:37:50.400 --> 0:37:54.120
<v Speaker 1>we're doing. So as Dawn brings series into sharper focus,

0:37:54.120 --> 0:37:56.760
<v Speaker 1>we will be able to see with exquisite detail what

0:37:57.239 --> 0:38:00.359
<v Speaker 1>what it is, what the white spot is. And I'm

0:38:00.480 --> 0:38:02.520
<v Speaker 1>very excited to find out because there have been all

0:38:02.600 --> 0:38:05.960
<v Speaker 1>these conjectures and people have said it could be cryo

0:38:06.160 --> 0:38:10.360
<v Speaker 1>volcanoes or or ice guyser's you know, shooting up ice

0:38:10.520 --> 0:38:14.720
<v Speaker 1>or materials from underneath the in the icy mantle. Another

0:38:14.800 --> 0:38:17.239
<v Speaker 1>idea I read, I think I read this in a

0:38:17.280 --> 0:38:19.640
<v Speaker 1>piece on I O nine that was interesting that said

0:38:19.680 --> 0:38:23.640
<v Speaker 1>it could be exposed icy crust from recent impacts. So

0:38:23.680 --> 0:38:25.759
<v Speaker 1>in other words, like you've got like the you've got

0:38:25.800 --> 0:38:29.160
<v Speaker 1>the thin, thinner outer layer that got chipped away by

0:38:29.160 --> 0:38:32.840
<v Speaker 1>an impact, and now you're seeing the icy goodness underneath.

0:38:34.000 --> 0:38:36.879
<v Speaker 1>Yeah yeah, yeah. So so the other places where we're

0:38:36.920 --> 0:38:40.200
<v Speaker 1>not seeing this brightly reflective surface, or places where like

0:38:40.320 --> 0:38:43.360
<v Speaker 1>dust is settled over time and it's sort of dulling

0:38:44.120 --> 0:38:47.359
<v Speaker 1>the normally shiny surface. So one can only imagine what

0:38:47.400 --> 0:38:50.000
<v Speaker 1>it would look like if this is the case. Yeah maybe, no, no,

0:38:50.080 --> 0:38:54.160
<v Speaker 1>maybe if we like polish it up, yeah, yeah, that

0:38:54.200 --> 0:38:57.080
<v Speaker 1>would be awesome. I also remember seeing one person who

0:38:57.160 --> 0:39:00.520
<v Speaker 1>had suggested that it may also be that the uh

0:39:00.719 --> 0:39:04.080
<v Speaker 1>it's deposits of some sort of highly reflective mineral at

0:39:04.120 --> 0:39:07.279
<v Speaker 1>that particular spot, which is also a possibility. That's one

0:39:07.320 --> 0:39:09.359
<v Speaker 1>of the other things they'll be looking at, and they'll

0:39:09.360 --> 0:39:12.640
<v Speaker 1>be using lots of different methodologies to test these different

0:39:12.760 --> 0:39:15.200
<v Speaker 1>hypotheses to find out which ones are the ones that

0:39:15.239 --> 0:39:17.560
<v Speaker 1>are accurate. Yeah, I'm really excited to find out what

0:39:17.600 --> 0:39:20.520
<v Speaker 1>it is. Now here's a funny thing, a little peak

0:39:20.560 --> 0:39:23.359
<v Speaker 1>behind the curtain, as Jonathan would say, we record these

0:39:23.400 --> 0:39:25.279
<v Speaker 1>podcasts a little bit ahead of time, so it'll be

0:39:25.320 --> 0:39:28.239
<v Speaker 1>really funny if they find out the answer between the

0:39:28.280 --> 0:39:30.160
<v Speaker 1>time we record this and the time it comes out.

0:39:30.200 --> 0:39:33.360
<v Speaker 1>Hopefully that won't happen. But this is today, is Friday,

0:39:33.360 --> 0:39:38.200
<v Speaker 1>March thirteenth, So if we just sounded like idiots, um,

0:39:38.440 --> 0:39:44.439
<v Speaker 1>that's why. That's that's one of the specific reason why

0:39:44.480 --> 0:39:48.040
<v Speaker 1>for this thing right now. Yeah. So there's another interesting

0:39:48.120 --> 0:39:51.000
<v Speaker 1>thing that they're going to be investigating, and Jonathan, you

0:39:51.040 --> 0:39:55.360
<v Speaker 1>brought this up earlier, is the possibility of oceans on series,

0:39:55.480 --> 0:39:59.840
<v Speaker 1>not even just oceans, but possibly habitable oceans, which is great,

0:40:00.120 --> 0:40:02.520
<v Speaker 1>The awesome I mean, it does seem like kind of

0:40:02.520 --> 0:40:05.040
<v Speaker 1>a far off chance. It's not like that they think

0:40:05.080 --> 0:40:08.120
<v Speaker 1>they're likely to find this, but just the possibility is insane.

0:40:08.200 --> 0:40:10.800
<v Speaker 1>On something like if you look at pictures of Series,

0:40:11.080 --> 0:40:13.680
<v Speaker 1>it doesn't look like something that would host life. It

0:40:13.680 --> 0:40:16.120
<v Speaker 1>looks like the moon. It's this kind of like crazy

0:40:16.200 --> 0:40:19.680
<v Speaker 1>dead rock in the middle of space. But before the

0:40:19.760 --> 0:40:23.080
<v Speaker 1>Dawn mission reached Series, scientists had suspected that a good

0:40:23.080 --> 0:40:26.680
<v Speaker 1>bit of Series mass was made of water. So NASA

0:40:26.719 --> 0:40:30.840
<v Speaker 1>says that if of Series mass is H two O

0:40:31.040 --> 0:40:34.440
<v Speaker 1>is water, that would mean Series has more fresh water

0:40:34.560 --> 0:40:40.040
<v Speaker 1>than Earth. That's not more water, but more freshwater. So

0:40:40.160 --> 0:40:42.920
<v Speaker 1>if it does have a substantial amount of water, is

0:40:42.960 --> 0:40:46.800
<v Speaker 1>any of it liquid And if it's liquid, could it

0:40:46.920 --> 0:40:50.839
<v Speaker 1>support life? That might not be as crazy as it sounds. Um,

0:40:50.880 --> 0:40:53.520
<v Speaker 1>if Series does have a substantial amount of ice, the

0:40:53.719 --> 0:40:57.040
<v Speaker 1>rock and the ice could separate into different layers that

0:40:57.080 --> 0:41:00.200
<v Speaker 1>onion effect you were talking about. And some sigh, just

0:41:00.239 --> 0:41:02.920
<v Speaker 1>think that the icy mantle of Series was once an

0:41:03.000 --> 0:41:07.920
<v Speaker 1>underground ocean. So underground ocean, Yeah, okay, that's great. Yeah,

0:41:07.960 --> 0:41:11.239
<v Speaker 1>it's sort of similar to uh, though not exactly the same,

0:41:11.239 --> 0:41:12.960
<v Speaker 1>but sort of similar to what you've heard about might

0:41:13.000 --> 0:41:16.120
<v Speaker 1>be the case on Europa where there is there is

0:41:16.160 --> 0:41:19.480
<v Speaker 1>frozen ice on the surface, but then probably liquid water

0:41:19.640 --> 0:41:25.240
<v Speaker 1>underneath it. But anyway, that's something that maybe possible on Series,

0:41:25.239 --> 0:41:27.280
<v Speaker 1>and we want to find out if that's the case,

0:41:27.640 --> 0:41:30.000
<v Speaker 1>and if there is any liquid water, then there's always

0:41:30.040 --> 0:41:32.960
<v Speaker 1>the chance that we could find evidence of life, which

0:41:33.280 --> 0:41:37.880
<v Speaker 1>obviously be incredibly exciting. Yes, I'm betting on cave dwelling

0:41:38.000 --> 0:41:40.799
<v Speaker 1>ice frogs. Yeah, there's a piece you can look at

0:41:40.880 --> 0:41:43.680
<v Speaker 1>in Science magazine called don Probe to look for a

0:41:43.719 --> 0:41:46.920
<v Speaker 1>Habitable Ocean on Series by Eric Hand in February of

0:41:46.960 --> 0:41:49.600
<v Speaker 1>this year. On top of the water, one of the

0:41:49.640 --> 0:41:52.279
<v Speaker 1>other things we could do is learn more about the

0:41:52.320 --> 0:41:54.840
<v Speaker 1>early formation of the Solar System. Like Lauren was talking

0:41:54.880 --> 0:42:00.080
<v Speaker 1>about early on, these objects out in space can and

0:42:00.160 --> 0:42:03.560
<v Speaker 1>help give us clues about what happened when they were

0:42:03.600 --> 0:42:08.759
<v Speaker 1>created and therefore how everything was created right right right,

0:42:08.880 --> 0:42:11.879
<v Speaker 1>and it may also lead to us learning about how

0:42:11.960 --> 0:42:15.120
<v Speaker 1>the Earth got its water. I think the reason why

0:42:15.160 --> 0:42:17.120
<v Speaker 1>this is also really cool is that the more we

0:42:17.239 --> 0:42:19.880
<v Speaker 1>learn about these processes, the more we know what to

0:42:19.960 --> 0:42:23.240
<v Speaker 1>look for when we're looking outside of our Solar System.

0:42:23.600 --> 0:42:27.680
<v Speaker 1>Things that if we know the various criteria that came

0:42:27.719 --> 0:42:30.160
<v Speaker 1>together to form our solar system. If we can look

0:42:30.200 --> 0:42:34.480
<v Speaker 1>for other similar systems, then that increases our chances to

0:42:34.520 --> 0:42:38.480
<v Speaker 1>find other planets that could potentially support life. Yeah, and

0:42:38.480 --> 0:42:41.160
<v Speaker 1>and just getting more data about these things that we've

0:42:41.200 --> 0:42:45.520
<v Speaker 1>only been able to study via via telescope so far. Uh,

0:42:45.840 --> 0:42:49.560
<v Speaker 1>lets us check back in the data from those telescopes

0:42:49.680 --> 0:42:53.319
<v Speaker 1>and see more patterns of where we got it right,

0:42:53.320 --> 0:42:56.800
<v Speaker 1>where we got it wrong, and therefore make better guesses

0:42:56.840 --> 0:42:59.680
<v Speaker 1>about other things that we're seeing through those telescopes. It's awesome,

0:43:00.120 --> 0:43:01.960
<v Speaker 1>so awesome, And I one of the other things we

0:43:02.000 --> 0:43:05.000
<v Speaker 1>can talk about that you know, we have a little

0:43:05.000 --> 0:43:07.359
<v Speaker 1>section in our notes about the future of asteroids, and

0:43:07.400 --> 0:43:11.000
<v Speaker 1>one of the things I wanted to mention is that water.

0:43:11.200 --> 0:43:14.720
<v Speaker 1>The presence of water is a huge, huge deal for us,

0:43:14.760 --> 0:43:20.080
<v Speaker 1>Like for many reasons for extended space exploration, being able

0:43:20.200 --> 0:43:25.399
<v Speaker 1>to potentially harvest water from other bodies would allow us

0:43:26.239 --> 0:43:29.520
<v Speaker 1>a lot more freedom, a lot more flexibility, and also

0:43:29.640 --> 0:43:32.680
<v Speaker 1>creates the potential for things like terraforming down the road.

0:43:32.760 --> 0:43:36.279
<v Speaker 1>If you're talking about bringing water in order to not

0:43:36.480 --> 0:43:41.080
<v Speaker 1>just have something drinkable, but perhaps to help facilitate an

0:43:41.160 --> 0:43:43.680
<v Speaker 1>atmosphere on a planet, that sort of stuff. I mean,

0:43:44.040 --> 0:43:46.640
<v Speaker 1>this is a big deal, another big thing about the

0:43:46.640 --> 0:43:48.799
<v Speaker 1>presence of water in space, because I mean, one of

0:43:48.800 --> 0:43:51.360
<v Speaker 1>the things we should mention is, well, we've got plenty

0:43:51.360 --> 0:43:53.600
<v Speaker 1>of water, why don't we just take some water into space. Well,

0:43:53.640 --> 0:43:58.080
<v Speaker 1>it's really expensive to ship stuff into space gallons and

0:43:58.120 --> 0:44:01.279
<v Speaker 1>gallons of fresh water is not a very smart way

0:44:01.280 --> 0:44:03.640
<v Speaker 1>to invest in your your your payloads. So if you

0:44:03.640 --> 0:44:07.520
<v Speaker 1>could actually access water once you're already out of Earth orbit,

0:44:08.480 --> 0:44:10.840
<v Speaker 1>that that's a really cool thing. So asteroids that have

0:44:10.880 --> 0:44:12.920
<v Speaker 1>water on them could be harvest, like you said, not

0:44:12.960 --> 0:44:15.440
<v Speaker 1>just for drinkable water, not just for terraforming and stuff

0:44:15.480 --> 0:44:19.600
<v Speaker 1>like that, but to make rocket fuel. That's because water

0:44:19.640 --> 0:44:22.520
<v Speaker 1>has hydrogen and oxygen, the chemical elements you would use

0:44:22.560 --> 0:44:24.759
<v Speaker 1>to make certain kinds of rocket fuel that we use

0:44:24.840 --> 0:44:27.280
<v Speaker 1>in our reaction drives today. And while you might argue

0:44:27.280 --> 0:44:29.520
<v Speaker 1>that we have plenty of water right now, it is

0:44:29.560 --> 0:44:32.040
<v Speaker 1>a limited supply. It's not like we're getting tons of

0:44:32.040 --> 0:44:34.959
<v Speaker 1>water from outside sources. So if you keep shipping water

0:44:35.040 --> 0:44:38.520
<v Speaker 1>off the planet, I probably wouldn't be worried about that

0:44:38.560 --> 0:44:42.719
<v Speaker 1>for a while. I wouldn't either. I'm just thinking, really

0:44:42.719 --> 0:44:48.680
<v Speaker 1>long term. Yeah. Yeah, the the Earth's water cycle is closed. Yeah. Now,

0:44:48.760 --> 0:44:51.920
<v Speaker 1>if we were to, say, end up siphoning water off

0:44:51.960 --> 0:44:55.320
<v Speaker 1>of asteroids to bring it back here, uh, that seems

0:44:55.360 --> 0:44:58.760
<v Speaker 1>like it would be a pretty enormous effort. I would

0:44:58.760 --> 0:45:01.080
<v Speaker 1>have to think the steaks would be incredibly high for

0:45:01.160 --> 0:45:04.200
<v Speaker 1>us to put forth that kind of investment. But never

0:45:04.200 --> 0:45:06.840
<v Speaker 1>say never. No, I think it's more the idea that

0:45:06.920 --> 0:45:10.320
<v Speaker 1>we would use this in space where we don't have access,

0:45:10.520 --> 0:45:13.120
<v Speaker 1>like if we were to create another space station further

0:45:13.160 --> 0:45:15.560
<v Speaker 1>out from the Earth. This would be a great source

0:45:15.600 --> 0:45:17.120
<v Speaker 1>to be able to get water. And of course we

0:45:17.120 --> 0:45:21.920
<v Speaker 1>would still be implementing the same water reclamation programs that

0:45:21.960 --> 0:45:25.600
<v Speaker 1>we have on other types of spacecraft to extend use

0:45:25.640 --> 0:45:29.000
<v Speaker 1>of water as long as possible, because you know, just

0:45:29.040 --> 0:45:30.600
<v Speaker 1>because you have an access to it doesn't mean you know,

0:45:31.920 --> 0:45:34.719
<v Speaker 1>you can stop by the series quickie mart and you know,

0:45:34.840 --> 0:45:37.040
<v Speaker 1>pick up a few gallons, say a bunch of astronauts

0:45:37.080 --> 0:45:39.520
<v Speaker 1>just brushing their teeth with the water running just bluggle

0:45:39.719 --> 0:45:44.400
<v Speaker 1>lobs of water just floating around like crazy. We we

0:45:44.440 --> 0:45:47.040
<v Speaker 1>could get more. That's just right over there. That's that

0:45:47.080 --> 0:45:49.160
<v Speaker 1>makes me think of a crazy question. I can't believe

0:45:49.200 --> 0:45:52.840
<v Speaker 1>I didn't think to look this up beforehand. Uh could

0:45:52.840 --> 0:45:55.480
<v Speaker 1>you walk on series? Does it have enough gravity too

0:45:55.640 --> 0:45:58.759
<v Speaker 1>that you could actually, you know, walk around on it.

0:45:58.800 --> 0:46:02.560
<v Speaker 1>I have a question. I don't. It would have to be,

0:46:02.600 --> 0:46:05.560
<v Speaker 1>it would be. I mean it's it is definitely it's

0:46:05.560 --> 0:46:09.040
<v Speaker 1>smaller than our moon. I just looked it up real quick.

0:46:09.120 --> 0:46:12.319
<v Speaker 1>Right now. It looks like the gravity on series the

0:46:12.440 --> 0:46:16.640
<v Speaker 1>downward acceleration is zero point to seven per second squared,

0:46:16.680 --> 0:46:19.399
<v Speaker 1>whereas on the Moon it's one point six ms per

0:46:19.400 --> 0:46:22.040
<v Speaker 1>second squared, right, and the moon is is one six

0:46:23.440 --> 0:46:29.480
<v Speaker 1>could be nine per second square, so so very little gravity.

0:46:29.560 --> 0:46:35.240
<v Speaker 1>Don't jump real baby. It was second a stroll on Series,

0:46:35.320 --> 0:46:37.600
<v Speaker 1>and everything was nice until I sneezed and the next

0:46:37.600 --> 0:46:43.239
<v Speaker 1>thing I knew. But at any rate, Uh, we've been

0:46:43.280 --> 0:46:46.680
<v Speaker 1>fascinated with this whole story, everything from all that went

0:46:46.719 --> 0:46:50.160
<v Speaker 1>into getting the mission together before it even launched to

0:46:50.760 --> 0:46:53.640
<v Speaker 1>the stuff that we're seeing now, the images that are

0:46:53.680 --> 0:46:56.799
<v Speaker 1>returning and the information that's returning from the mission. And

0:46:56.840 --> 0:46:58.960
<v Speaker 1>also we should point out this is this is an

0:46:58.960 --> 0:47:02.640
<v Speaker 1>historic mission for an other reason. It's the first spacecraft

0:47:02.960 --> 0:47:07.880
<v Speaker 1>to visit two different uh proto planets at all, like,

0:47:07.960 --> 0:47:09.319
<v Speaker 1>not only the first one to go to a pro

0:47:09.400 --> 0:47:12.759
<v Speaker 1>planet like like series in that sense, but to go

0:47:12.840 --> 0:47:16.200
<v Speaker 1>to two different ones. So that was a cool thing

0:47:16.239 --> 0:47:18.520
<v Speaker 1>as well. We will keep our eyes on the news

0:47:18.560 --> 0:47:21.680
<v Speaker 1>that comes out of the mission, and uh, like Joe said,

0:47:21.719 --> 0:47:24.439
<v Speaker 1>I hope that this episode comes out before any other

0:47:24.480 --> 0:47:28.319
<v Speaker 1>breaking news. Um. I mean, if if it turns out

0:47:28.360 --> 0:47:30.759
<v Speaker 1>that there's some major thing that happens between when we've

0:47:30.800 --> 0:47:34.080
<v Speaker 1>recorded this and when it publishes, that's awesome, right. I

0:47:34.080 --> 0:47:35.680
<v Speaker 1>mean it's not like it's not like we're gonna be

0:47:35.800 --> 0:47:38.759
<v Speaker 1>unhappy that it happened. We'll just be unhappy that we

0:47:38.840 --> 0:47:44.080
<v Speaker 1>look dumb. So but this was a really fun topic

0:47:44.120 --> 0:47:47.120
<v Speaker 1>to cover. I mean, we always love covering space topics.

0:47:47.120 --> 0:47:49.719
<v Speaker 1>It's one of our favorite subjects to cover on here,

0:47:49.760 --> 0:47:52.880
<v Speaker 1>Space AI and three D printing, that's kind of our

0:47:52.960 --> 0:47:55.799
<v Speaker 1>bread and butter. But of course we love all topics

0:47:55.880 --> 0:47:59.279
<v Speaker 1>about the future. So if there's anything out there that

0:47:59.360 --> 0:48:02.560
<v Speaker 1>you dear listeners would love us to cover. Maybe there's

0:48:02.560 --> 0:48:04.720
<v Speaker 1>some topic but you're just dying to hear more about,

0:48:05.040 --> 0:48:07.239
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0:48:07.280 --> 0:48:09.879
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0:48:09.880 --> 0:48:13.479
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0:48:13.680 --> 0:48:16.480
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0:48:16.520 --> 0:48:20.000
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0:48:20.120 --> 0:48:23.160
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0:48:23.280 --> 0:48:25.440
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0:48:25.760 --> 0:48:28.200
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0:48:28.719 --> 0:48:36.160
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0:48:36.200 --> 0:48:49.160
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