WEBVTT - TechStuff Classic: TechStuff Goes on a Voyage

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<v Speaker 1>Welcome to text Stuff, a production from my Heart Radio.

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<v Speaker 1>Hey there, and welcome to tech Stuff. I'm your host,

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<v Speaker 1>Jonathan Strickland. I'm an executive producer with iHeart Radio and

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<v Speaker 1>I love all things tech, and today we're going to

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<v Speaker 1>listen to a classic episode titled tech Stuff Goes on

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<v Speaker 1>a Voyage. It's about the Voyager program and this episode

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<v Speaker 1>originally published on April two thousand thirteen. The Voyager program

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<v Speaker 1>is one of those really fascinating space programs that I

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<v Speaker 1>absolutely loved learning about, so I hope you guys enjoy

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<v Speaker 1>this classic episode. The first thing we wanted to talk

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<v Speaker 1>about was kind of what was the purpose of the

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<v Speaker 1>Voyager missions, which, by the way, are still going. But

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<v Speaker 1>we want to talk about kind of the timeline of

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<v Speaker 1>the missions, and then we'll get into more details about

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<v Speaker 1>the space craft itself and then follow that up with

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<v Speaker 1>a discussion about the science that has been discovered by

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<v Speaker 1>these amazing spacecraft. So going back to May nineteen seventy two,

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<v Speaker 1>that's when NASA begins to fund a mission that will

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<v Speaker 1>involve designing, building, and launching spacecraft that are meant to

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<v Speaker 1>explore the outer planets of our Solar System. And even

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<v Speaker 1>before this back in the engineer named Gary Flandreau noticed

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<v Speaker 1>that sometime in the nineteen seventies, the outer planets would

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<v Speaker 1>be aligned planetary alignment in such a way as to

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<v Speaker 1>make this very possible. And this was you know, the

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<v Speaker 1>space program was going and booming, and it was kind

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<v Speaker 1>of an incredible alignment of the stars that allowed us

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<v Speaker 1>to write when we had money to do this stuff. Right, So, so,

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<v Speaker 1>I mean that planetary alignment is really what makes the

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<v Speaker 1>voyager missions possible because you know, if the if the

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<v Speaker 1>plants were in such an alignment, so that let's say

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<v Speaker 1>that alignment, well there's still aligned properly, they're just not

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<v Speaker 1>viable for us to explore. But let's say let's say

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<v Speaker 1>like jupiters on one side of the Sun and Saturn's

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<v Speaker 1>on the other side of the Sun, then it would

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<v Speaker 1>be really tricky to design a spacecraft sector could explore both. Right, So,

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<v Speaker 1>and this particular alignment isn't going to occur again for

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<v Speaker 1>another hundred and seventy six years, so you had to

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<v Speaker 1>jump on the opportunity. And so in nineteen seventy two,

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<v Speaker 1>even though it was still years away from when this

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<v Speaker 1>alignment would occur, NASA gets on the ball and starts

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<v Speaker 1>to design this, and in nineteen seventy seven they are

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<v Speaker 1>finished with the design and the spacecraft they had been

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<v Speaker 1>designing was under the working name the Mariner Jupiter slash

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<v Speaker 1>Saturn nineteen seventy seven, but they decided to rename it

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<v Speaker 1>a little bit of a mouthfall, yeaheah. They called it Voyager,

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<v Speaker 1>and on August twenty, nineteen seventy seven, a Titan Centaur

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<v Speaker 1>rocket carried one of the two Voyager spacecraft from Cape Canaveral, Florida,

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<v Speaker 1>into the atmosphere and ultimately into space. Which one was

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<v Speaker 1>it that will launched first? It was Voyager two that

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<v Speaker 1>launched first. Which one launched second? Voyager one? Okay, So

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<v Speaker 1>so this this was basically for pr purposes because the

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<v Speaker 1>way that they were designed, Voyager one was going to

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<v Speaker 1>due to its trajectory, it was going to reach Jupiter

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<v Speaker 1>first and so start sending back images of Jupiter, you know,

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<v Speaker 1>fingers crossed if all goes well first, and NASA thought

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<v Speaker 1>that the public would be incredibly confused if if the

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<v Speaker 1>Voyager one launched first but got to the planets second,

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<v Speaker 1>whereas some for some reason launching second and getting to

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<v Speaker 1>the planet first is less confusing. No one was paying

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<v Speaker 1>attention to the launch. Yeah, goodness knows, no one pays

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<v Speaker 1>attention to something. Yeah, the one thing you're actually able

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<v Speaker 1>to watch while you're still on Earth. It still makes

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<v Speaker 1>me tear up every single time anything gets launched into space.

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<v Speaker 1>I'm like, just humanity is so beautiful. That's pretty awesome.

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<v Speaker 1>I mean when you think about what it takes to

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<v Speaker 1>get something into space, and is phenomenal the amount of

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<v Speaker 1>engineering and ingenuity that went into that. But yes, absolutely so.

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<v Speaker 1>The Voyager to launches first. The Voyager one launches about

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<v Speaker 1>sixteen days later, in fact, not about sixteen days later,

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<v Speaker 1>at launches nicely on September and it's using the same

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<v Speaker 1>sort of rocket, the Titans Centaur rocket, which, by the way,

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<v Speaker 1>I love it anyway. The initial purpose was for these

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<v Speaker 1>to explore the giant planets in the Outer Solar System.

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<v Speaker 1>Those giant planets are Jupiter, Saturn, Uranus, and Neptune. Pluto,

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<v Speaker 1>of course not a giant planet. It does not get

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<v Speaker 1>the treatment, not for these missions. Forget you Pluto. And

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<v Speaker 1>there were two separate trajectories that were being used. Voyager one,

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<v Speaker 1>of course, was designed so that the trajectory was chosen

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<v Speaker 1>so that it would reach Jupiter first, then move on

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<v Speaker 1>to Saturn, and then get flung off to head toward

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<v Speaker 1>interstellar space. Uh. Voyager too would do a visit to

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<v Speaker 1>all four of the giant planets. So that's why you

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<v Speaker 1>have the different timelines, because even though Voyager two launched first,

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<v Speaker 1>for it to be able to hit this trajectory where

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<v Speaker 1>it was going to to pass by each of the

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<v Speaker 1>four giants, it had to do that at a different Yeah.

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<v Speaker 1>So that's the you know. And if you were to

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<v Speaker 1>just look at a model of the Solar System and

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<v Speaker 1>just spin the planets around at the different rates, you

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<v Speaker 1>would see like, oh, yeah, now I understand you would

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<v Speaker 1>have to be really particular about when you would launch

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<v Speaker 1>and how you would launch for it to be able

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<v Speaker 1>to hit all of these points properly. I mean, it's

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<v Speaker 1>an amazing amount of engineering that's required and and just

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<v Speaker 1>math that's required to make sure that you've got the

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<v Speaker 1>right the right timing. Yeah, and it was it was

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<v Speaker 1>kind of shady, you know, basically until it happened, no

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<v Speaker 1>one was sure that it was going to happen, right

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<v Speaker 1>and Uh, And it's interesting because the Voyager spacecraft actually

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<v Speaker 1>used the planets themselves to help make sure they got

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<v Speaker 1>to where they needed to go. But we'll get into that.

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<v Speaker 1>It's pretty awesome though. So moving down the timeline, they

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<v Speaker 1>they've launched in nineteen seventy seven. Almost two years later,

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<v Speaker 1>on March five, nineteen seventy nine, Voyager one has its

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<v Speaker 1>closest approach to Jupiter and it captures a lot of

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<v Speaker 1>images of Jupiter and Jupiter's moons. Uh. And then July nine,

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<v Speaker 1>nineteen seventy nine, so same year, that's when Voyager two

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<v Speaker 1>passes closest to Jupiter. Uh. Then we go to the

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<v Speaker 1>next year. On November twelve, eighty Voyager one has its

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<v Speaker 1>closest approach to Saturn, and then it begins its trip

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<v Speaker 1>out of the Solar System, saying so long, suckers, and

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<v Speaker 1>starts heading off into the well. It would be the sunset,

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<v Speaker 1>except it can't be in the opposite of the sunset, right,

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<v Speaker 1>It's not the sun rise either. That's that would normally

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<v Speaker 1>be the opposite of a sunset, the sun diminishing into

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<v Speaker 1>a tin year ball. I guess not nearly as poetic.

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<v Speaker 1>But August one, that's when Voyager two gets its closest

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<v Speaker 1>approach to Saturday. But of course Voyager two is not

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<v Speaker 1>flung off into in our interstellar space right away. Instead,

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<v Speaker 1>it is then heading toward Uranus, which it passes closest

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<v Speaker 1>to on January fourth, nineteen eight six. So it took

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<v Speaker 1>five years for Voyager two to go from Saturn to Uranus. Uh,

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<v Speaker 1>and it would take um it would take a few

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<v Speaker 1>more years before it would like five well three more years,

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<v Speaker 1>I'm sorry, three more years before I would get close

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<v Speaker 1>to Neptune. But before we get to that point, seven,

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<v Speaker 1>Voyager two observes the supernova nineteen seven eight Voyager returns

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<v Speaker 1>the first color images of Neptune. So that Voyager two

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<v Speaker 1>that is, so it's getting closer to Neptune. It's still

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<v Speaker 1>not the closest it will be, but that's when we

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<v Speaker 1>first started getting color images of Neptune back from Voyager,

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<v Speaker 1>and on August nine, Voyager two as its closest approach

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<v Speaker 1>to Neptune. And that concludes the primary mission of the

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<v Speaker 1>of both Voyager spacecraft, that primary mission being the exploration

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<v Speaker 1>of those outer planets. So the cost of the missions

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<v Speaker 1>from nineteen seventy two to the time when they finished

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<v Speaker 1>their mission their primary mission was eight hundred sixty five

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<v Speaker 1>million dollars. Now, NASA points out that if you break

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<v Speaker 1>this down by the population of the United States and

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<v Speaker 1>year over year, that's about eight cents per person per year.

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<v Speaker 1>So it's it's essentially saying like, look, really in the

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<v Speaker 1>grand scheme, and it sounds like a lot of money,

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<v Speaker 1>but in the grand scheme of things, this is just

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<v Speaker 1>a tiny investment. So look at these pictures of center. Yeah. Uh,

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<v Speaker 1>keep keep calm and keep exploring, is what they said.

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<v Speaker 1>I hate that name anyway. So the that that million

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<v Speaker 1>dollars included everything include the expense of the launch vehicles,

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<v Speaker 1>the radioactive power source, which we'll get to talk about

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<v Speaker 1>in a little bit, uh, and and just the maintaining

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<v Speaker 1>of the missions. By nine, Voyager one was heading toward

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<v Speaker 1>interstellar space and on vale In Tine's Day in nineteen nine,

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<v Speaker 1>we get the final images from Voyager, which is a

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<v Speaker 1>portrait of the Solar System. Happy Valentine's Day, I gave

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<v Speaker 1>you the Solar System. Sweet Three days later, February I'm

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<v Speaker 1>sorry three days in eight years later on fantasy, I

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<v Speaker 1>should read the year before I read the day February

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<v Speaker 1>sevent have all my notes in front of me, it's just,

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<v Speaker 1>you know, my typing and viewing skills are Apparently there's

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<v Speaker 1>something to be desired. February seventeenth, the Voyager one passes

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<v Speaker 1>the Pioneer ten, which had obviously been launched previously, and

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<v Speaker 1>so that makes the Voyager one the most distant human

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<v Speaker 1>made object in space. It is still to this day

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<v Speaker 1>the most distant human made object in space. It's actually

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<v Speaker 1>most distant stir and it was because it keeps going.

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<v Speaker 1>That was good. Well, I figured it might as well

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<v Speaker 1>measure up to my reading and comprehension skills. Uh. Decenumber

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<v Speaker 1>fifteen two thousand four. Edge or one crosses the termination

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<v Speaker 1>shock comination shock. This is this is pretty cool, guys,

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<v Speaker 1>and do the heally you sheath. Yeah. So here's here's

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<v Speaker 1>some things that you need to know about our wacky

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<v Speaker 1>little solar system. Here you might ask, what's the edge

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<v Speaker 1>of the Solar System? Is it Pluto? No? No, it's

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<v Speaker 1>not Pluto. Well, I mean again, it all depends on

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<v Speaker 1>how you're defining the edge of the Solar System. But

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<v Speaker 1>the way NASA defines it, Nope, not Pluto, especially since

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<v Speaker 1>it's not it's still on a planet right now, that's

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<v Speaker 1>not it's a dwarf planet. There's that never mind, there's yeah,

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<v Speaker 1>it's you know, it's Pluto is right there with happy, sneezy,

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<v Speaker 1>sleepy Adobe doc bashful. Uh So, termination shock, that's that's

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<v Speaker 1>the point where the solar wind particles start to slow down.

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<v Speaker 1>They were traveling essentially at kind of the speed of

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<v Speaker 1>sound would be, but anyway, they're traveling really fast. They

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<v Speaker 1>start slowing down because you can think of the solar

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<v Speaker 1>wind as this uh, this force that pushes out from

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<v Speaker 1>the Sun. All right, Now, think of the interstellar space

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<v Speaker 1>kind of having its own pressure. It's sort of like

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<v Speaker 1>air pressure. It's pushing in on the solar made of

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<v Speaker 1>magnetic fields instead of air pressure. So there exactly, they're

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<v Speaker 1>not air particles. It's all we're talking. There are particles

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<v Speaker 1>on space, but that's that's a different thing anyway. So

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<v Speaker 1>the solar wind is pressing against these these other pressures.

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<v Speaker 1>So once you get to the point where the solar

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<v Speaker 1>wind is slowing down, that's the termination shock. Right, there's

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<v Speaker 1>kind of a boundary with a with a shock wave

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<v Speaker 1>fare and also still not the edge of the Solar system. Also,

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<v Speaker 1>you also have the heliosphere. Now this is where we

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<v Speaker 1>still have we still have evidence of the solar wind

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<v Speaker 1>within the heliosphere. Then you have the helio pause, which

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<v Speaker 1>is the very boundary of where the solar wind is,

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<v Speaker 1>and that still is not the edge of the Solar System,

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<v Speaker 1>not according to NASA. According to NASA, really we need

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<v Speaker 1>to think of the edge of the Solar System as

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<v Speaker 1>being an area where the Sun's gravitational poll has no

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<v Speaker 1>greater effect on you than any other particular celestial body

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<v Speaker 1>out there. So, in other words, you aren't being pulled

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<v Speaker 1>towards the Solar System at that point anymore than you're

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<v Speaker 1>being pulled towards some other point, right, Yeah, so that

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<v Speaker 1>that area is ill defined by the very nature of gravity.

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<v Speaker 1>But um, that would take us a very long time

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<v Speaker 1>to get there, and we'll talk about that when we

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<v Speaker 1>get into the science section. So anyway, termination shock has

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<v Speaker 1>all these fluctuating magnetic fields due to the change and

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<v Speaker 1>the speed of the Solar wind, and that's kind of

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<v Speaker 1>why it's called what it's called. And Voyager one, like

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<v Speaker 1>I said, crossed it on December two thousand four and

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<v Speaker 1>begins to encounter the interstellar medium. That doesn't mean that

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<v Speaker 1>it's in interstellar space yet, but starting to encounter the

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<v Speaker 1>particles that would be an interstellar space September five, two

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<v Speaker 1>thousand seven, three years later, that's when Voyager two catches

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<v Speaker 1>up and crosses the termination shock at a totally different point.

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<v Speaker 1>By the way, these two spacecraft are in two totally

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<v Speaker 1>different sections of no nowhere near each other anymore, not

0:13:02.760 --> 0:13:05.360
<v Speaker 1>at all. And then in July and two thousand twelve,

0:13:05.400 --> 0:13:08.599
<v Speaker 1>Voyager one enters a new region of space which is

0:13:08.640 --> 0:13:11.160
<v Speaker 1>still inside the Solar System. It's another region of the

0:13:11.200 --> 0:13:15.080
<v Speaker 1>helio heliosphere helio she called a magnetic highway YEP. And

0:13:15.080 --> 0:13:18.560
<v Speaker 1>the directions of the particles that it's encountering are beginning

0:13:18.559 --> 0:13:21.000
<v Speaker 1>to change, which suggests that the spacecraft is at the

0:13:21.120 --> 0:13:25.760
<v Speaker 1>very edge of the heliosphere. And UM engineers didn't expect

0:13:25.760 --> 0:13:27.920
<v Speaker 1>that the data that they got back. They thought that

0:13:28.040 --> 0:13:31.160
<v Speaker 1>it would have passed beyond this point earlier, which just

0:13:31.240 --> 0:13:34.240
<v Speaker 1>tells us that our Solar system is actually larger, thought

0:13:34.280 --> 0:13:37.240
<v Speaker 1>that the Sun is more powerful than we previously expected.

0:13:37.400 --> 0:13:40.960
<v Speaker 1>Never underestimate the power of the Sun. It can turn

0:13:41.000 --> 0:13:45.240
<v Speaker 1>me read in a matter of minutes, very susceptible to

0:13:45.240 --> 0:13:47.920
<v Speaker 1>that sort of thing. So, yeah, that's we've already talked

0:13:47.920 --> 0:13:51.680
<v Speaker 1>about how they have, they left at different times in

0:13:51.720 --> 0:13:56.120
<v Speaker 1>their pathways, meant that they are traveling in different directions

0:13:56.120 --> 0:13:59.280
<v Speaker 1>and different at different speeds. Uh, and they visited different

0:13:59.480 --> 0:14:01.880
<v Speaker 1>you know, like voice You're two visited two more planets

0:14:01.920 --> 0:14:04.320
<v Speaker 1>than Voyage or one did. But we talked about how

0:14:04.320 --> 0:14:08.439
<v Speaker 1>the planets helped move the spacecraft and direct the spacecraft.

0:14:08.720 --> 0:14:12.000
<v Speaker 1>So if you guys have seen science fiction films like

0:14:12.640 --> 0:14:15.520
<v Speaker 1>Star Trek four, the Voyage Home where they sling shot

0:14:15.559 --> 0:14:18.040
<v Speaker 1>around the Sun, they're actually using the Sun's gravity to

0:14:18.160 --> 0:14:20.560
<v Speaker 1>kind of accelerate a ship to the point where it

0:14:20.600 --> 0:14:23.360
<v Speaker 1>can travel back in time. I don't understand that. By

0:14:23.360 --> 0:14:25.440
<v Speaker 1>the way, if you've got warp speed, you technically anyway,

0:14:25.520 --> 0:14:28.880
<v Speaker 1>that's another episode. We already did. That episode we did.

0:14:28.920 --> 0:14:30.840
<v Speaker 1>But anyway, they use it to sling shot around the Sun,

0:14:30.840 --> 0:14:35.360
<v Speaker 1>which magically lets them travel back in time. There's some

0:14:35.440 --> 0:14:37.480
<v Speaker 1>truth to that in the sense that we have used

0:14:37.480 --> 0:14:42.280
<v Speaker 1>that same kind of principle with designing the voyage or spacecraft. Right.

0:14:42.320 --> 0:14:45.400
<v Speaker 1>What we what we kind of realized is that if

0:14:45.440 --> 0:14:48.840
<v Speaker 1>you okay, you're you're you're moving towards the planet, you're

0:14:48.840 --> 0:14:52.200
<v Speaker 1>a probe okay, okay, and uh, as you move towards

0:14:52.200 --> 0:14:54.760
<v Speaker 1>the planet. You're going to start accelerating as the planet's

0:14:54.760 --> 0:14:57.240
<v Speaker 1>gravitational pull starts pulling you in. Right, if you only

0:14:57.280 --> 0:15:00.200
<v Speaker 1>kind of graze by it, then hypothetically you'll deseller right

0:15:00.280 --> 0:15:02.800
<v Speaker 1>on the way out because you're losing energy to that

0:15:02.800 --> 0:15:06.240
<v Speaker 1>gravitational pull. Right. And by the way, because of the

0:15:06.240 --> 0:15:14.040
<v Speaker 1>conservation of energy, technically, the planet's orbit actually slows sure infanticimally, Yeah,

0:15:14.080 --> 0:15:16.240
<v Speaker 1>it's uh say, I've got wait, wait, wait, I have

0:15:16.280 --> 0:15:17.760
<v Speaker 1>it written down. I know I've got it written down.

0:15:17.960 --> 0:15:22.840
<v Speaker 1>It's something like, uh, one foot in a trillion years. Well,

0:15:22.880 --> 0:15:24.840
<v Speaker 1>but hey, that is an impact you are. You are

0:15:24.880 --> 0:15:27.840
<v Speaker 1>making a difference. But Jupiter is going to be a

0:15:27.880 --> 0:15:32.840
<v Speaker 1>little late to its to its appointment in one trillion years. Right. However,

0:15:33.000 --> 0:15:36.040
<v Speaker 1>because planets are moving in their orbits, if you are

0:15:36.120 --> 0:15:38.760
<v Speaker 1>going on the same trajectory as a planet's orbit, you

0:15:38.800 --> 0:15:42.920
<v Speaker 1>can pick up that orbital speed as you slingshot around

0:15:42.920 --> 0:15:45.760
<v Speaker 1>the planet. Ye, And so that that has allowed the

0:15:45.840 --> 0:15:50.600
<v Speaker 1>Voyager spacecraft to get propulsion from one plant to the

0:15:50.640 --> 0:15:54.320
<v Speaker 1>next without having to have massive thrusters on board. In fact,

0:15:54.440 --> 0:15:56.600
<v Speaker 1>when we get to the actual description of the spacecraft,

0:15:56.640 --> 0:15:59.560
<v Speaker 1>you'll find out that their thrusters are not incredibly powerful

0:15:59.560 --> 0:16:02.400
<v Speaker 1>at all, but they were able to use the power

0:16:02.480 --> 0:16:06.960
<v Speaker 1>of gravity to direct and propel themselves something as large

0:16:07.000 --> 0:16:09.200
<v Speaker 1>as as Jupiter. You know, it's moving through space at

0:16:09.400 --> 0:16:13.280
<v Speaker 1>something like thirty thousand miles per hour forty tho kilometers

0:16:13.320 --> 0:16:16.720
<v Speaker 1>and uh yeah, so so and and that's yeah, it's

0:16:16.920 --> 0:16:19.840
<v Speaker 1>a completely free energy boost of about that much speed.

0:16:20.000 --> 0:16:23.880
<v Speaker 1>According to NASA, because of the use of planetary gravity,

0:16:24.280 --> 0:16:29.000
<v Speaker 1>Voyager too ended up having a fuel economy of about

0:16:29.040 --> 0:16:32.440
<v Speaker 1>thirteen thousand kilometers per leader or thirty thousand miles per gallon.

0:16:33.200 --> 0:16:36.160
<v Speaker 1>That's efficient. That beats That beats my car. That's highway miles,

0:16:36.480 --> 0:16:38.720
<v Speaker 1>city miles. They did not give me, so I don't

0:16:38.760 --> 0:16:41.880
<v Speaker 1>I don't know how it would do in the city. Uh. There,

0:16:41.920 --> 0:16:45.840
<v Speaker 1>the Voyager two's flight path got a look, like we said,

0:16:45.880 --> 0:16:49.480
<v Speaker 1>at all four of the giant plants um and uh

0:16:49.640 --> 0:16:53.440
<v Speaker 1>and it's a couple of billion miles further inside the

0:16:53.480 --> 0:16:55.960
<v Speaker 1>Solar System than the Voyager one. So the Voyager one

0:16:56.000 --> 0:16:58.640
<v Speaker 1>got a kind of a head start into interstellar space

0:16:59.440 --> 0:17:03.720
<v Speaker 1>um and is more than eleven billion or seventeen point

0:17:03.760 --> 0:17:06.960
<v Speaker 1>seven eleven billion miles or seventeen point seven billion kilometers

0:17:06.960 --> 0:17:09.639
<v Speaker 1>away from the Sun at this point more more more

0:17:09.640 --> 0:17:12.200
<v Speaker 1>than eighteen as of as of today, there's there's a

0:17:12.240 --> 0:17:14.440
<v Speaker 1>there's a tracker on on NASA nice where you can

0:17:14.560 --> 0:17:17.640
<v Speaker 1>check all this out. So uh and and uh. At

0:17:17.680 --> 0:17:23.000
<v Speaker 1>that distance, it takes hours for a for data to

0:17:23.160 --> 0:17:25.560
<v Speaker 1>go from the spacecraft to be picked up here on Earth.

0:17:25.640 --> 0:17:29.760
<v Speaker 1>About seventeen hours. Wow. Yeah, so that's a long time.

0:17:29.840 --> 0:17:32.720
<v Speaker 1>So the way that let me let me find my

0:17:32.760 --> 0:17:35.159
<v Speaker 1>note on it that it's really interesting the way that

0:17:35.160 --> 0:17:38.080
<v Speaker 1>they receive those radio signals because they're they're pretty far away,

0:17:38.080 --> 0:17:40.639
<v Speaker 1>they're getting increasingly difficult to check all the times. They

0:17:40.640 --> 0:17:43.720
<v Speaker 1>have a whole series of two and thirty ft radio

0:17:43.800 --> 0:17:48.400
<v Speaker 1>dishes right basically to pull Voyager data. These are the

0:17:48.520 --> 0:17:52.240
<v Speaker 1>deep space antenna that they have to pick up this information,

0:17:52.800 --> 0:17:56.280
<v Speaker 1>um and uh. And they actually upgraded those over the

0:17:57.240 --> 0:18:00.359
<v Speaker 1>course of the life of the Voyager program. When they

0:18:00.400 --> 0:18:03.360
<v Speaker 1>first started, they were significantly smaller, and they didn't have

0:18:03.440 --> 0:18:06.760
<v Speaker 1>to be as big because the Voyager spacecraft were relatively

0:18:07.000 --> 0:18:10.080
<v Speaker 1>closer to the Earth. Uh. And now now we've got

0:18:10.200 --> 0:18:12.239
<v Speaker 1>to a point where we keep upgrading the antenna so

0:18:12.280 --> 0:18:15.480
<v Speaker 1>that we can continue to pick up these increasingly weak signals,

0:18:15.920 --> 0:18:20.160
<v Speaker 1>so it's pretty amazing. According to NASA, the emissions from

0:18:20.560 --> 0:18:24.080
<v Speaker 1>Earth to Neptune required the equivalent of eleven thousand work

0:18:24.160 --> 0:18:29.280
<v Speaker 1>years of human work. Eleven thousand work years, which they said,

0:18:29.280 --> 0:18:31.000
<v Speaker 1>there's only a third of what it took to build

0:18:31.240 --> 0:18:35.240
<v Speaker 1>the Great Pyramid. So well, hey, so you know we're slack,

0:18:35.280 --> 0:18:38.280
<v Speaker 1>and yes, you know, really they're just saying, look how

0:18:38.320 --> 0:18:40.560
<v Speaker 1>much more efficient we are. They were piling up rocks,

0:18:40.640 --> 0:18:45.120
<v Speaker 1>we were sending spacecraft into space. Um and uh, and

0:18:45.160 --> 0:18:47.600
<v Speaker 1>again we've learned that the Solar System is actually larger

0:18:47.600 --> 0:18:51.360
<v Speaker 1>than what we have previously anticipated and um. So by

0:18:51.400 --> 0:18:54.280
<v Speaker 1>the time the Voyager two flew by Neptune, the two

0:18:54.320 --> 0:18:58.680
<v Speaker 1>spacecraft together had transmitted about five trillion bits of scientific

0:18:58.760 --> 0:19:01.560
<v Speaker 1>data back at Earth and it was someone's job to

0:19:01.600 --> 0:19:04.280
<v Speaker 1>look at all that. But yeah, the deep space tracking

0:19:04.320 --> 0:19:06.119
<v Speaker 1>antennas are the ones we were talking about earlier that

0:19:06.160 --> 0:19:08.080
<v Speaker 1>have been upgrades several times, and that that kind of

0:19:08.720 --> 0:19:12.560
<v Speaker 1>that's the brief overview of the mission, and next we're

0:19:12.600 --> 0:19:15.080
<v Speaker 1>going to take a look at the spacecraft itself and

0:19:15.160 --> 0:19:19.399
<v Speaker 1>also some kind of cool records that are above the

0:19:20.119 --> 0:19:22.879
<v Speaker 1>two spacecraft. But before we do that, let's take a

0:19:23.160 --> 0:19:33.720
<v Speaker 1>quick pause to thank our sponsored. Okay, let's talk about

0:19:33.760 --> 0:19:36.000
<v Speaker 1>the actual spacecraft for a minute. We know what they

0:19:36.000 --> 0:19:38.680
<v Speaker 1>were supposed to do and what they have done. Um

0:19:38.720 --> 0:19:41.440
<v Speaker 1>so uh And one thing I did not mention, I

0:19:41.480 --> 0:19:44.880
<v Speaker 1>guess is that the whole inner interstellar travel stuff that's

0:19:44.880 --> 0:19:47.000
<v Speaker 1>totally planned as well, in fact, has been added on

0:19:47.080 --> 0:19:50.400
<v Speaker 1>as a secondary mission. The primary mission was the outer planets.

0:19:50.840 --> 0:19:54.560
<v Speaker 1>Secondary is what's up with this interstellar stuff we don't

0:19:54.600 --> 0:19:57.400
<v Speaker 1>know anything about. Well, they realize that their power sources

0:19:57.440 --> 0:20:01.440
<v Speaker 1>would work until about and so figured well, hey, let's

0:20:01.440 --> 0:20:05.160
<v Speaker 1>just kind of roll with it. Yeah. Yeah, so that's five.

0:20:05.240 --> 0:20:08.399
<v Speaker 1>That's about when we expect the power resources to be

0:20:08.840 --> 0:20:11.040
<v Speaker 1>to the point where they can no longer power the

0:20:11.480 --> 0:20:14.679
<v Speaker 1>transmitter to send us back data. And we'll talk about that.

0:20:14.680 --> 0:20:17.520
<v Speaker 1>That's one of the things that that's interesting about this spacecraft.

0:20:17.520 --> 0:20:20.520
<v Speaker 1>There are a lot of interesting things. So both of them, uh,

0:20:20.600 --> 0:20:23.280
<v Speaker 1>because because they're identical, Yes, they are identical. So each

0:20:23.320 --> 0:20:26.280
<v Speaker 1>one of them weighs just under a ton. And now

0:20:26.280 --> 0:20:29.359
<v Speaker 1>when they were on top of the the launch vehicle,

0:20:29.560 --> 0:20:32.600
<v Speaker 1>they weighed a lot more than that, but the spacecraft

0:20:32.600 --> 0:20:35.560
<v Speaker 1>themselves are just under a ton each unearthed obviously, because

0:20:35.560 --> 0:20:39.360
<v Speaker 1>weight is all relative to where you are. Yes, uh,

0:20:39.400 --> 0:20:42.040
<v Speaker 1>And they are each made up of about sixty five

0:20:42.240 --> 0:20:46.280
<v Speaker 1>fouls and individual parts. But these parts are often made

0:20:46.359 --> 0:20:50.000
<v Speaker 1>up of tinier components. So they have a term they

0:20:50.119 --> 0:20:54.040
<v Speaker 1>use which is equivalent parts. And equivalent parts means like

0:20:54.320 --> 0:20:56.240
<v Speaker 1>if you were to look at, for example, if I

0:20:56.280 --> 0:20:59.880
<v Speaker 1>were to say my computer is part uh, is one

0:21:00.080 --> 0:21:03.080
<v Speaker 1>part of the equipment that I use, someone else could

0:21:03.080 --> 0:21:05.919
<v Speaker 1>point out, well, that computer has multiple chips in it,

0:21:06.119 --> 0:21:10.160
<v Speaker 1>and those chips have transistors, and so really that one

0:21:10.200 --> 0:21:12.720
<v Speaker 1>part is a representation of lots and lots and lots

0:21:12.760 --> 0:21:14.960
<v Speaker 1>of parts. So NASA was like, well, if you want

0:21:14.960 --> 0:21:17.640
<v Speaker 1>to know how many equivalent parts there are, there about

0:21:17.720 --> 0:21:22.359
<v Speaker 1>five million of them. Compare that to your old standard

0:21:22.359 --> 0:21:26.000
<v Speaker 1>definition color television. There will be about two thousand, five

0:21:26.200 --> 0:21:30.000
<v Speaker 1>D equivalent parts. So lots more than a color TV,

0:21:30.280 --> 0:21:32.800
<v Speaker 1>which is kind of what you want when you're when

0:21:32.800 --> 0:21:34.919
<v Speaker 1>you're expo space. Yeah, you need a little bit more

0:21:34.920 --> 0:21:38.000
<v Speaker 1>than it than your average standard definition color television. I agree,

0:21:38.040 --> 0:21:43.600
<v Speaker 1>I would hope. So yeah, also larger than your standard yes, well,

0:21:43.680 --> 0:21:47.919
<v Speaker 1>unless you're a crazy rich person. The main body is

0:21:47.960 --> 0:21:50.440
<v Speaker 1>a is a ten sided box that's about six ft

0:21:50.480 --> 0:21:54.359
<v Speaker 1>or one point eight meters across, and that's where the

0:21:54.400 --> 0:21:58.000
<v Speaker 1>fuel tank, the and and some of the electronic instruments. Yeah,

0:21:58.480 --> 0:22:00.200
<v Speaker 1>and we'll talk about those instruments. They are all lot

0:22:00.240 --> 0:22:06.120
<v Speaker 1>of them. Yeah, they're they were. They both have areas

0:22:06.160 --> 0:22:10.080
<v Speaker 1>that are hardened against radiation and shielded. And the reason

0:22:10.119 --> 0:22:12.119
<v Speaker 1>for that is obviously that when you go into space,

0:22:12.400 --> 0:22:14.919
<v Speaker 1>you are going to encounter things that you would not

0:22:15.040 --> 0:22:17.119
<v Speaker 1>encounter here on the surface of the planet. And the

0:22:17.160 --> 0:22:21.880
<v Speaker 1>reason for that is that the Earth atmosphere and magnetos

0:22:21.880 --> 0:22:27.040
<v Speaker 1>sphere mag magnetosphere sphere still makes me think that we're

0:22:27.040 --> 0:22:30.440
<v Speaker 1>watching x men. I would say, I would say magnetosphere.

0:22:30.560 --> 0:22:36.280
<v Speaker 1>I know you would, but shere it is the sphere

0:22:36.320 --> 0:22:40.600
<v Speaker 1>in which magneto travels, and it's also a magnetic field

0:22:40.760 --> 0:22:45.280
<v Speaker 1>that surrounds the Earth, penetrates and binds us together like

0:22:45.359 --> 0:22:48.439
<v Speaker 1>the force. Now, what it does is actually repels certain

0:22:48.480 --> 0:22:53.200
<v Speaker 1>types of waves and particles, which allows us to remain. Yeah,

0:22:53.359 --> 0:22:56.600
<v Speaker 1>we do. We're not being bombarded by cosmic radiation or

0:22:56.760 --> 0:22:59.680
<v Speaker 1>gamma raise or things like that, because that would be

0:22:59.720 --> 0:23:01.560
<v Speaker 1>a much were sunburned than that other sa burned than

0:23:01.560 --> 0:23:04.240
<v Speaker 1>we were talking. The combination of the of our atmosphere

0:23:04.240 --> 0:23:08.280
<v Speaker 1>and the magnetosphere or magnetosphere protectas, and so the thing

0:23:08.320 --> 0:23:09.679
<v Speaker 1>is that when you're out in space, you don't have

0:23:09.680 --> 0:23:12.399
<v Speaker 1>the benefit of that protection. So that's why both of

0:23:12.440 --> 0:23:16.879
<v Speaker 1>them have these these shielding areas and casings that are

0:23:16.920 --> 0:23:19.840
<v Speaker 1>hardened against radiation to protect them if they were to

0:23:19.960 --> 0:23:24.000
<v Speaker 1>encounter any of these waves or particles. Clearly very important,

0:23:24.160 --> 0:23:27.919
<v Speaker 1>interesting little side fact. So Earth has a magneto sphere,

0:23:28.960 --> 0:23:32.360
<v Speaker 1>Mars doesn't, So if we were to make a colony

0:23:32.400 --> 0:23:35.359
<v Speaker 1>on Mars we would not have that protection that we

0:23:35.359 --> 0:23:37.840
<v Speaker 1>would we need to compensate for it in some wame, right,

0:23:37.840 --> 0:23:40.400
<v Speaker 1>So you wouldn't want to go on any long strolls

0:23:40.440 --> 0:23:44.400
<v Speaker 1>on the Martian soil without some serious protection. So that's

0:23:44.480 --> 0:23:47.720
<v Speaker 1>all of those All of those fashionable space bikinis that

0:23:47.760 --> 0:23:50.880
<v Speaker 1>were that were really popular back in the nineties would

0:23:50.960 --> 0:23:53.240
<v Speaker 1>not probably be good. The interesting thing I heard was

0:23:53.320 --> 0:23:55.359
<v Speaker 1>I was I was listening and I'll go ahead. It

0:23:55.480 --> 0:23:58.359
<v Speaker 1>was a skeptic skuide to the universe. A great podcast

0:23:58.520 --> 0:24:01.600
<v Speaker 1>has no affiliation with us, but they are fantastic, very fun,

0:24:02.240 --> 0:24:05.800
<v Speaker 1>interesting educational podcast. They had a recent episode where um

0:24:05.840 --> 0:24:10.119
<v Speaker 1>they had an astronomer on talking about things like Mars

0:24:10.400 --> 0:24:11.960
<v Speaker 1>and they were even talking about, all right, let's let's

0:24:11.960 --> 0:24:14.879
<v Speaker 1>look into a science fiction future where we can terraform Mars,

0:24:15.200 --> 0:24:17.600
<v Speaker 1>so we're able to transform Mars so that the actual

0:24:17.720 --> 0:24:22.520
<v Speaker 1>surfaces habitable. And even then, because of the lack of

0:24:22.520 --> 0:24:25.840
<v Speaker 1>the magnetosphere, you would still be prone to things like

0:24:25.880 --> 0:24:28.639
<v Speaker 1>cosmic radiation, gamma radiation. You would you would still be

0:24:28.680 --> 0:24:30.760
<v Speaker 1>vulnerable with that, so you would not be able to

0:24:30.840 --> 0:24:33.760
<v Speaker 1>terraform it for any extended length of time. Eventually that

0:24:33.960 --> 0:24:37.119
<v Speaker 1>stuff would kill the life on that planet. Right, because

0:24:37.280 --> 0:24:39.480
<v Speaker 1>things like gamma radiation, for example, aren't as cool is

0:24:39.520 --> 0:24:41.960
<v Speaker 1>for example, teenage meeting nincha turtles make it sound or

0:24:42.160 --> 0:24:45.680
<v Speaker 1>almost mostly you just die. Yeah, yeah, it's not. It's

0:24:45.680 --> 0:24:50.560
<v Speaker 1>not attractive. In fact, uh NASA said that because of

0:24:50.600 --> 0:24:54.560
<v Speaker 1>the distance from the the the Voyager spacecraft passed close

0:24:54.640 --> 0:24:57.640
<v Speaker 1>enough to Jupiter that it received more than a thousand

0:24:57.680 --> 0:25:00.280
<v Speaker 1>times the radiation that would be a lethal bull of

0:25:00.359 --> 0:25:05.960
<v Speaker 1>radiation for human Yeah, for a human person, yes, um, So,

0:25:06.080 --> 0:25:08.800
<v Speaker 1>moving on to more things that are on board this

0:25:08.680 --> 0:25:11.840
<v Speaker 1>these spacecraft. It has a it has a twelve foot

0:25:11.960 --> 0:25:15.480
<v Speaker 1>or a three point seven meter high gain antenna which

0:25:15.520 --> 0:25:17.880
<v Speaker 1>looks like a satellite dish. Yeah, this is what allows

0:25:17.920 --> 0:25:21.040
<v Speaker 1>it to transmit and receive data to and from Earth,

0:25:21.680 --> 0:25:24.720
<v Speaker 1>and no matter where it goes, the the antenna is

0:25:24.800 --> 0:25:28.080
<v Speaker 1>programmed to always point towards Earth. Yes, that's it's actually

0:25:28.119 --> 0:25:32.920
<v Speaker 1>got a gyroscopic UH system so that no matter how

0:25:32.960 --> 0:25:36.760
<v Speaker 1>it's oriented, it can it can readjust its attitude so

0:25:36.840 --> 0:25:39.840
<v Speaker 1>that the UH the antenna is pointing towards US, so

0:25:39.880 --> 0:25:42.000
<v Speaker 1>we can have the best chants possible to pick up

0:25:42.000 --> 0:25:45.520
<v Speaker 1>those radio transmissions. UM. It has a lot of different

0:25:45.560 --> 0:25:49.840
<v Speaker 1>instruments aboard, including besides the high gain antenna, it's got

0:25:49.840 --> 0:25:53.680
<v Speaker 1>a low energy charged particle instrument and ultra violet spectrometer

0:25:53.800 --> 0:25:56.840
<v Speaker 1>which currently only the voyager one is using to collect data.

0:25:57.640 --> 0:26:01.000
<v Speaker 1>Has both narrow and wide angle imaging instruments also known

0:26:01.080 --> 0:26:05.239
<v Speaker 1>as cameras. It's got a fancy, fancy eight hundred by

0:26:05.240 --> 0:26:07.840
<v Speaker 1>eight hundred cameras because this was launched in the nineteen

0:26:07.920 --> 0:26:11.399
<v Speaker 1>seventies seemed pretty cool at the time. UH as a

0:26:11.440 --> 0:26:15.120
<v Speaker 1>cosmic ray instruments so it can detect and measure cosmic rays,

0:26:15.160 --> 0:26:20.080
<v Speaker 1>a photopolarimeter, which I have no idea what it does.

0:26:20.119 --> 0:26:22.160
<v Speaker 1>I was. I ran into it and I thought that's

0:26:22.160 --> 0:26:24.720
<v Speaker 1>really cool, and I never actually looked more into it

0:26:24.760 --> 0:26:28.280
<v Speaker 1>because I was lucky that I could say it. There's

0:26:28.280 --> 0:26:33.919
<v Speaker 1>an infrared interferometer spectrometer UH, an optical calibration targeting system,

0:26:34.200 --> 0:26:38.639
<v Speaker 1>a planetary radio astronomy and plasma wave antenna. Each spacecraft

0:26:38.680 --> 0:26:41.440
<v Speaker 1>have two of those UM and also known as the

0:26:41.520 --> 0:26:45.520
<v Speaker 1>Planetary radio Astronomy Instrument or p r A has the

0:26:45.960 --> 0:26:49.800
<v Speaker 1>plasma instrument. Voyager ones plasma instrument is non functional, but

0:26:49.920 --> 0:26:53.000
<v Speaker 1>all other instruments are in working order, and Voyager two

0:26:53.080 --> 0:26:57.719
<v Speaker 1>is still collecting data through its plasma instruments. It's got UH.

0:26:58.040 --> 0:27:00.840
<v Speaker 1>It also gets its power from three D O isotope

0:27:00.880 --> 0:27:06.200
<v Speaker 1>thermoelectric generators and currently it gets about three D and

0:27:06.280 --> 0:27:10.240
<v Speaker 1>fifteen watts of power. And now the spacecraft are designed

0:27:10.320 --> 0:27:13.119
<v Speaker 1>so that all of their systems can operate at about

0:27:13.200 --> 0:27:18.160
<v Speaker 1>four hundreds of power, so it's able to UH. It's

0:27:18.160 --> 0:27:20.800
<v Speaker 1>still getting power, but it's not enough power to operate everything.

0:27:20.840 --> 0:27:23.399
<v Speaker 1>And in fact, they designed the Voyager spacecraft with this

0:27:23.560 --> 0:27:27.560
<v Speaker 1>in mind, the idea being that as the power as

0:27:27.600 --> 0:27:30.040
<v Speaker 1>the power supply begins to decrease, it begins to shut

0:27:30.160 --> 0:27:37.280
<v Speaker 1>down unnecessary instruments. So originally there were eleven different UM

0:27:37.920 --> 0:27:41.040
<v Speaker 1>projects that were involved in gathering data from the Voyager

0:27:41.119 --> 0:27:43.439
<v Speaker 1>systems and processing that data here on Earth. There were

0:27:43.440 --> 0:27:46.040
<v Speaker 1>eleven of them. Currently only five of them are still

0:27:46.119 --> 0:27:50.200
<v Speaker 1>in operation because the other systems have been progressively shut

0:27:50.280 --> 0:27:53.880
<v Speaker 1>down to make sure that the Voyager spacecraft can still

0:27:54.160 --> 0:27:58.520
<v Speaker 1>send us information. And like you said, by five or so,

0:27:59.200 --> 0:28:01.560
<v Speaker 1>that's when we aspect the power to have run down

0:28:01.720 --> 0:28:03.600
<v Speaker 1>enough where we're not going to be able to get

0:28:03.640 --> 0:28:05.840
<v Speaker 1>any more information from them, because it's just not gonna

0:28:05.880 --> 0:28:08.560
<v Speaker 1>have the power necessary to broadcast right right Well, because

0:28:08.600 --> 0:28:10.720
<v Speaker 1>the way that this this engine of sorts works is

0:28:10.760 --> 0:28:14.040
<v Speaker 1>that pellets of plutonium dioxide release heat through their own

0:28:14.119 --> 0:28:17.679
<v Speaker 1>natural decay process, and so once they have finished decaying,

0:28:18.119 --> 0:28:22.800
<v Speaker 1>that's it. Yeah, that's true. And then I forgot. There

0:28:22.840 --> 0:28:27.280
<v Speaker 1>also some magnet magnetometer boom, which is designed toss to

0:28:27.680 --> 0:28:30.440
<v Speaker 1>measure magnetic fields. So that was one of those things

0:28:30.480 --> 0:28:32.440
<v Speaker 1>we didn't really know a lot about the magnetic fields

0:28:32.440 --> 0:28:35.760
<v Speaker 1>of the Elder planets before we sent these these spacecraft up.

0:28:35.800 --> 0:28:38.200
<v Speaker 1>That's one of the really huge sources of information that

0:28:38.280 --> 0:28:40.680
<v Speaker 1>it is it has sent us. Yeah, and uh so

0:28:40.960 --> 0:28:44.280
<v Speaker 1>then it has a flight data subsystem which handles all

0:28:44.360 --> 0:28:47.840
<v Speaker 1>the information, and it has an eight track digital tape recorder.

0:28:48.680 --> 0:28:50.479
<v Speaker 1>So you've got an eight track up there. It's uh.

0:28:51.080 --> 0:28:54.760
<v Speaker 1>So the FDS configures controls, collects data from the various instruments,

0:28:54.960 --> 0:28:57.120
<v Speaker 1>and the tape recorder handles the data from the plasma

0:28:57.160 --> 0:29:01.040
<v Speaker 1>wave subsystem because that's the one that gets the highest

0:29:01.400 --> 0:29:04.000
<v Speaker 1>density of data and the shortest amount of time. So

0:29:04.480 --> 0:29:08.040
<v Speaker 1>the data tape recorder was the cutting edge technology to

0:29:08.840 --> 0:29:12.560
<v Speaker 1>handle that that information. And according to NASA, the tape

0:29:12.560 --> 0:29:14.880
<v Speaker 1>in the digital recorder won't wear out until the tape

0:29:14.920 --> 0:29:17.400
<v Speaker 1>has moved back and forth through a distance that is

0:29:17.440 --> 0:29:20.240
<v Speaker 1>equivalent to the width of the United States. Uh. That

0:29:20.520 --> 0:29:24.240
<v Speaker 1>is not terribly precise, because the United States is not

0:29:24.400 --> 0:29:27.560
<v Speaker 1>a perfect rectangle, but in general, I would say that's

0:29:27.600 --> 0:29:30.360
<v Speaker 1>probably about three thousand miles, which is around four thousand,

0:29:30.440 --> 0:29:32.600
<v Speaker 1>eight hundred kilometers. I assume what they mean is that

0:29:32.720 --> 0:29:35.120
<v Speaker 1>it's it's doing fine. Yeah, So what they're saying is

0:29:35.200 --> 0:29:39.480
<v Speaker 1>that that tape is capable of traveling that collective amount

0:29:39.520 --> 0:29:42.920
<v Speaker 1>of distance without breaking. So you've got to remember the

0:29:42.960 --> 0:29:45.240
<v Speaker 1>tape itself is not that long. It's just saying that

0:29:45.320 --> 0:29:46.880
<v Speaker 1>they would you know, by the time you would go

0:29:47.040 --> 0:29:48.720
<v Speaker 1>through all this tape and is worn out you could

0:29:48.760 --> 0:29:52.320
<v Speaker 1>have gone all the way across the United States using

0:29:52.400 --> 0:29:55.760
<v Speaker 1>that same distance of tape being played through. Just kind

0:29:55.800 --> 0:29:58.960
<v Speaker 1>of that's kind of impressive. There has a command computer

0:29:59.040 --> 0:30:02.920
<v Speaker 1>subsystem which p it's sequencing and control functions, which includes

0:30:02.960 --> 0:30:08.040
<v Speaker 1>fault detection, corrective routines, antenna pointing data, and spacecraft sequencing data.

0:30:08.480 --> 0:30:12.280
<v Speaker 1>The fault detection involves seven top level fault protection routines

0:30:12.360 --> 0:30:14.560
<v Speaker 1>and each one is able to detect and correct for

0:30:14.720 --> 0:30:18.640
<v Speaker 1>several possible failures. Basically, it just means that there's the

0:30:19.000 --> 0:30:22.960
<v Speaker 1>computer has multiple modules and they compare data back and

0:30:23.040 --> 0:30:25.880
<v Speaker 1>forth between each other and and it will decide if

0:30:26.000 --> 0:30:28.760
<v Speaker 1>if one module is differing from the others, that that

0:30:28.840 --> 0:30:31.200
<v Speaker 1>one's faulty and to cut it out of the system. Yes,

0:30:31.560 --> 0:30:34.000
<v Speaker 1>And it also means that both of the spacecraft are

0:30:34.040 --> 0:30:39.320
<v Speaker 1>capable of shutting down systems if it needs to automatically autonomously.

0:30:39.440 --> 0:30:42.080
<v Speaker 1>Because which is so important, because we can't broadcast to

0:30:42.200 --> 0:30:44.760
<v Speaker 1>these things. They broadcast to us, but they don't have receivers.

0:30:44.880 --> 0:30:48.280
<v Speaker 1>Their antenna could receive information. Yeah, but it means that

0:30:48.320 --> 0:30:50.320
<v Speaker 1>it would take seventeen hours for the information to get

0:30:50.320 --> 0:30:52.040
<v Speaker 1>to us. In seventeen hours for the information to get

0:30:52.040 --> 0:30:54.800
<v Speaker 1>back and by then whatever the problem was is probably

0:30:55.360 --> 0:30:58.960
<v Speaker 1>not the biggest issue at that point, right, So, yeah,

0:31:00.000 --> 0:31:02.920
<v Speaker 1>that it was important to have something to connect autonomously

0:31:03.040 --> 0:31:05.720
<v Speaker 1>if if you know, if the communication is a barrier.

0:31:05.760 --> 0:31:08.520
<v Speaker 1>The same sort of thing with the Curiosity Rover when

0:31:08.520 --> 0:31:10.080
<v Speaker 1>it was landing on the surface of Mars. You know,

0:31:10.600 --> 0:31:12.440
<v Speaker 1>a lot of that landing. In fact, all of the

0:31:12.560 --> 0:31:15.720
<v Speaker 1>landing was autonomous because there was no time for us

0:31:15.800 --> 0:31:18.400
<v Speaker 1>to send any adjustments to the system. It's like you're

0:31:18.440 --> 0:31:20.480
<v Speaker 1>on your own. By the time we would be able

0:31:20.520 --> 0:31:22.880
<v Speaker 1>to send an adjustment, it would have already either crash

0:31:23.040 --> 0:31:26.480
<v Speaker 1>or landed safely. So you had to design a spacecraft

0:31:26.560 --> 0:31:28.920
<v Speaker 1>that could do this or else it just wouldn't work.

0:31:29.280 --> 0:31:31.480
<v Speaker 1>Pretty impressive in the nineteen seventies for for the amount

0:31:31.520 --> 0:31:34.200
<v Speaker 1>of computing power that was going. Oh yeah, definitely. And

0:31:34.320 --> 0:31:36.720
<v Speaker 1>it also had an attitude in art or still has.

0:31:36.800 --> 0:31:38.520
<v Speaker 1>I don't know why I'm using the past tense. It's

0:31:38.520 --> 0:31:43.320
<v Speaker 1>still out there. The Attitude and Articulation Control Subsystem, which

0:31:43.400 --> 0:31:45.520
<v Speaker 1>is also known the A A c S. It's in

0:31:45.600 --> 0:31:48.880
<v Speaker 1>charge of maintaining the spacecraft orientation and positions the scan platform.

0:31:48.920 --> 0:31:50.480
<v Speaker 1>So this is what we're talking about. The system that's

0:31:50.680 --> 0:31:53.320
<v Speaker 1>that's in charge of making sure that dad antenna has

0:31:53.320 --> 0:31:56.080
<v Speaker 1>pointed back at Earth. And also that the scan platform,

0:31:56.120 --> 0:31:59.960
<v Speaker 1>which is really you know, the instrumentation panel this point

0:32:00.000 --> 0:32:02.280
<v Speaker 1>in the right direction to get the data that the needs.

0:32:03.240 --> 0:32:06.440
<v Speaker 1>And uh it's yeah, it's got a three access stabilization

0:32:06.520 --> 0:32:10.080
<v Speaker 1>system and use the celestial or gyro referenced attitude control

0:32:10.160 --> 0:32:13.120
<v Speaker 1>to make the high gain antenna point back to Earth. Now,

0:32:13.560 --> 0:32:16.240
<v Speaker 1>we talked about the fact that there is an interesting

0:32:17.160 --> 0:32:21.680
<v Speaker 1>gold plated copper disc on board each of the two

0:32:21.800 --> 0:32:26.959
<v Speaker 1>Voyager spacecraft, right the golden records there refer So this is, uh,

0:32:27.160 --> 0:32:29.680
<v Speaker 1>this was a really cool idea. You know who, of

0:32:29.760 --> 0:32:32.160
<v Speaker 1>course was the chairman for this, Carl Sagan. Yes, he

0:32:32.320 --> 0:32:34.959
<v Speaker 1>he had billions and billions of suggestions, but not all

0:32:35.000 --> 0:32:37.040
<v Speaker 1>of them can make it onto the disc obviously, right.

0:32:37.080 --> 0:32:39.880
<v Speaker 1>And these are these are these these gold plated copper

0:32:39.960 --> 0:32:43.600
<v Speaker 1>discs engraved like vinyl records. Yeah yeah, and kids ask

0:32:43.640 --> 0:32:47.320
<v Speaker 1>your parents, no, no, dear, no no, no. Kids are

0:32:47.360 --> 0:32:49.640
<v Speaker 1>hipsters these days. They know they know things about vinyl.

0:32:49.880 --> 0:32:53.160
<v Speaker 1>It's cool. Kids tell your older siblings because they missed

0:32:53.200 --> 0:32:56.280
<v Speaker 1>down the whole hipster generation. Um, all right, so so yeah,

0:32:56.480 --> 0:32:59.480
<v Speaker 1>you're talking about a disk that has physical grooves that

0:32:59.600 --> 0:33:03.160
<v Speaker 1>are in it that can be read using a stylist

0:33:03.200 --> 0:33:06.320
<v Speaker 1>and cartridge, which which were included. They included the cartridge

0:33:06.320 --> 0:33:10.120
<v Speaker 1>and stylists. They did not include a turntable, so aliens

0:33:11.400 --> 0:33:14.000
<v Speaker 1>they have to build it. But they did leave instructions

0:33:14.040 --> 0:33:17.040
<v Speaker 1>written in a symbolic language to say here's how you

0:33:17.080 --> 0:33:19.720
<v Speaker 1>would construct something that would be able to play these things.

0:33:20.280 --> 0:33:23.479
<v Speaker 1>They were their twelve inches in diameter, and they are

0:33:23.560 --> 0:33:26.200
<v Speaker 1>designed to be played back at sixteen and two thirds

0:33:26.320 --> 0:33:30.480
<v Speaker 1>revolutions per minute, so actually fairly slowly. I mean, you know,

0:33:30.600 --> 0:33:33.680
<v Speaker 1>we think about the the forty five or thirty three

0:33:33.760 --> 0:33:37.120
<v Speaker 1>revolutions per minute for for your average albums, and this

0:33:37.320 --> 0:33:41.440
<v Speaker 1>is a sixteen and two thirds. So on these Golden

0:33:41.520 --> 0:33:45.120
<v Speaker 1>records are lots and lots of stuff. Actually, um, it's

0:33:45.480 --> 0:33:48.960
<v Speaker 1>including things like greetings from in fifty five different languages,

0:33:49.360 --> 0:33:52.160
<v Speaker 1>including some that aren't being used anymore. They are not

0:33:52.320 --> 0:33:55.440
<v Speaker 1>being used in a very long time, like which is

0:33:55.520 --> 0:33:59.680
<v Speaker 1>a Sumerian language which was last used around four thousand BC. UH,

0:34:00.040 --> 0:34:02.560
<v Speaker 1>a selection of nature sounds yep, yep, So if you

0:34:02.640 --> 0:34:04.840
<v Speaker 1>ever wanted to hear what frogs burping sounded like and

0:34:04.920 --> 0:34:08.040
<v Speaker 1>you were from from some distant planet. Here's an opportunity

0:34:08.080 --> 0:34:12.840
<v Speaker 1>to a lot of So you're for Ford Prefect and

0:34:12.880 --> 0:34:14.279
<v Speaker 1>you're on your way to Earth. This is a good

0:34:14.320 --> 0:34:16.640
<v Speaker 1>way to do some homework before you get there. All right,

0:34:16.680 --> 0:34:19.200
<v Speaker 1>a lot of traditional music, some some Native American chance

0:34:19.200 --> 0:34:21.320
<v Speaker 1>and Scottish bagpipes. I've got to talk about some of

0:34:21.320 --> 0:34:25.160
<v Speaker 1>the music that's on here for African ritual music. There's

0:34:25.560 --> 0:34:28.400
<v Speaker 1>a bunch of classical music, all right. So yeah, I

0:34:28.760 --> 0:34:31.360
<v Speaker 1>wrote down some of my favorites. This is this is Obviously,

0:34:31.600 --> 0:34:33.719
<v Speaker 1>there are lots and lots of musical tracks that are

0:34:33.800 --> 0:34:36.400
<v Speaker 1>on the records. These are just the ones that I

0:34:36.520 --> 0:34:39.360
<v Speaker 1>personally wrote down because I I they resonate with me.

0:34:39.960 --> 0:34:41.320
<v Speaker 1>It's not to say that the other ones are not

0:34:41.560 --> 0:34:44.279
<v Speaker 1>as good, right, I may not be familiar with some

0:34:44.400 --> 0:34:48.319
<v Speaker 1>of them. But there's the brandon Burg Concerto number two

0:34:48.480 --> 0:34:51.120
<v Speaker 1>in F. Actually it's just the first movement. That's by

0:34:51.160 --> 0:34:56.239
<v Speaker 1>a guy named Batch. Johann Batch wrote that, Um, if

0:34:56.239 --> 0:34:59.520
<v Speaker 1>you've heard he's just some dude. Really yeah, yeah, obviously

0:34:59.560 --> 0:35:02.040
<v Speaker 1>box Edinburg can chair to a number two. N f uh.

0:35:02.200 --> 0:35:06.520
<v Speaker 1>Then there's a Melancholy Blues which was performed by Louis Armstrong.

0:35:07.080 --> 0:35:11.400
<v Speaker 1>Stravinsky's The Right of Spring was included back actually was

0:35:11.680 --> 0:35:13.840
<v Speaker 1>pretty well represented on this record. He also had the

0:35:13.840 --> 0:35:16.959
<v Speaker 1>well tempered Clavia on there. There was the first movement

0:35:17.000 --> 0:35:21.080
<v Speaker 1>of Beethoven's Fifth Symphony, you know, the dah There was

0:35:21.120 --> 0:35:24.000
<v Speaker 1>a navajo tribes chant, and then of course the most

0:35:24.080 --> 0:35:28.200
<v Speaker 1>important i think musical work that was included out of

0:35:28.320 --> 0:35:30.520
<v Speaker 1>all the pieces that were on there. As as we

0:35:30.600 --> 0:35:33.520
<v Speaker 1>all know from the documentary Back to the Future, It's

0:35:33.600 --> 0:35:36.520
<v Speaker 1>saved Marty McFly, It'll save the human race. We're talking

0:35:36.560 --> 0:35:43.480
<v Speaker 1>about Chuck Berry's Johnny be Good. Yeah. Um, there's actually

0:35:43.560 --> 0:35:47.120
<v Speaker 1>a book all about the process that they used to

0:35:47.239 --> 0:35:50.399
<v Speaker 1>select which sounds went on the Golden Record, right, Yeah.

0:35:50.560 --> 0:35:53.120
<v Speaker 1>It finally came out with a CD companion at some point.

0:35:53.120 --> 0:35:55.799
<v Speaker 1>I'm sure it's on digital. The book itself is out

0:35:55.840 --> 0:35:57.800
<v Speaker 1>of print, but you can sometimes find copies. It is

0:35:57.840 --> 0:36:01.359
<v Speaker 1>called Murmurs from Earth, So if you want to learn

0:36:01.440 --> 0:36:05.719
<v Speaker 1>more about how they came about choosing which sounds go

0:36:05.920 --> 0:36:09.600
<v Speaker 1>in there. Um, that's it's it's a really well done piece.

0:36:09.719 --> 0:36:11.799
<v Speaker 1>It's it's something that I've I've heard nothing but good

0:36:11.880 --> 0:36:13.600
<v Speaker 1>things about it. I personally have not had a chance

0:36:13.680 --> 0:36:16.120
<v Speaker 1>to read it. By the time I learned about it

0:36:16.160 --> 0:36:18.839
<v Speaker 1>was running on a print, so it's kind of fine.

0:36:19.120 --> 0:36:21.440
<v Speaker 1>But there's also a bunch of images on the desks,

0:36:21.480 --> 0:36:24.719
<v Speaker 1>including a star map clearly showing the location of Earth.

0:36:26.760 --> 0:36:30.440
<v Speaker 1>Here's what humans taste like, maps of Earth images. I'm

0:36:30.480 --> 0:36:33.279
<v Speaker 1>just I'm just ignoring that entirely. There are people who

0:36:33.320 --> 0:36:35.760
<v Speaker 1>have said what a huge mistake it was to essentially

0:36:35.800 --> 0:36:40.080
<v Speaker 1>include directions directly to us. I think, well, I think

0:36:40.120 --> 0:36:43.120
<v Speaker 1>it's pretty ridiculous because the odds of anyone and the

0:36:43.160 --> 0:36:47.400
<v Speaker 1>odds of anyone finding the voyagers as big as it

0:36:47.480 --> 0:36:51.000
<v Speaker 1>turns out, really big, no, no, no, bigger than that. Not.

0:36:51.520 --> 0:36:53.800
<v Speaker 1>You might think it's a long walk to the chemist

0:36:53.800 --> 0:36:56.200
<v Speaker 1>style on the corner, but that's just nuts compared to space.

0:36:56.760 --> 0:36:59.239
<v Speaker 1>But it's going to be tens of thousands of years

0:36:59.360 --> 0:37:05.680
<v Speaker 1>before either the voyager craft encounter anything near another star. Yeah, exactly.

0:37:05.800 --> 0:37:08.440
<v Speaker 1>So really, by the time, I'm betting we will have

0:37:08.600 --> 0:37:12.279
<v Speaker 1>either kill ourselves off or hit the Singularity. And and

0:37:12.400 --> 0:37:14.759
<v Speaker 1>plus on top of that, you know, it would all

0:37:14.760 --> 0:37:19.640
<v Speaker 1>depend on from one direction the other creatures were approaching Earth,

0:37:19.920 --> 0:37:21.720
<v Speaker 1>Because I mean, there's there are a lot of different

0:37:21.800 --> 0:37:24.000
<v Speaker 1>vectors you could take and only a couple of them

0:37:24.040 --> 0:37:27.920
<v Speaker 1>would intersect with the pathway of either voyagers. Way more

0:37:28.000 --> 0:37:31.600
<v Speaker 1>vectors than most science fiction movies are willing to acknowledge.

0:37:31.760 --> 0:37:34.600
<v Speaker 1>There's more than just ship spaceship battles, than just the

0:37:34.640 --> 0:37:38.359
<v Speaker 1>single plane. Yeah. Uh So there was also an hour

0:37:38.520 --> 0:37:41.520
<v Speaker 1>long recording of the brain waves of a woman named

0:37:41.560 --> 0:37:44.960
<v Speaker 1>Anne Druian, who would become Carl Sagan's wife. Yep, she's

0:37:44.960 --> 0:37:49.200
<v Speaker 1>an author. She concentrates mainly on cosmology and science, and

0:37:50.040 --> 0:37:51.960
<v Speaker 1>she she signed up for this. She volunteered to have

0:37:52.040 --> 0:37:54.239
<v Speaker 1>her brain waves reported. Yea. She and Carl Sagan had

0:37:54.280 --> 0:37:55.759
<v Speaker 1>talked about it, and she thought it was a really

0:37:55.840 --> 0:37:59.600
<v Speaker 1>interesting idea, and so she went in for the process

0:37:59.760 --> 0:38:03.160
<v Speaker 1>where her brainless waves and her heartbeat were read and

0:38:03.320 --> 0:38:06.279
<v Speaker 1>then transferred into data analog data, we have to say,

0:38:06.320 --> 0:38:10.239
<v Speaker 1>because it's an analog disc and um. She says that

0:38:10.360 --> 0:38:13.440
<v Speaker 1>what she did was she she thought about big historical

0:38:13.760 --> 0:38:16.480
<v Speaker 1>moments that were very important in the development of human history,

0:38:16.880 --> 0:38:20.399
<v Speaker 1>and then she spent some time thinking about the current

0:38:20.480 --> 0:38:23.560
<v Speaker 1>situation on Earth, how what that's like things and and

0:38:23.680 --> 0:38:30.560
<v Speaker 1>not sugarcoating at things like violence between people and the Yeah.

0:38:30.640 --> 0:38:32.680
<v Speaker 1>So she really spent some time thinking about things that

0:38:32.800 --> 0:38:35.160
<v Speaker 1>she felt needed to be addressed. And then she said

0:38:35.719 --> 0:38:37.520
<v Speaker 1>that she took the liberty towards the end of the

0:38:37.560 --> 0:38:39.400
<v Speaker 1>session to take a little bit of time and think

0:38:39.440 --> 0:38:41.800
<v Speaker 1>about what it's like to fall in love, which I

0:38:41.880 --> 0:38:45.040
<v Speaker 1>think is amazing, just the most wonderful suite. Ye. Yeah,

0:38:45.160 --> 0:38:47.879
<v Speaker 1>so now we those aliens can't tell us they don't

0:38:47.920 --> 0:38:49.920
<v Speaker 1>know how to love because she thought about it for

0:38:50.360 --> 0:38:54.520
<v Speaker 1>for a while, darn it. Um. So, yeah, those radio

0:38:54.520 --> 0:38:56.800
<v Speaker 1>signals do take a long time to get to us. So.

0:38:58.000 --> 0:39:01.719
<v Speaker 1>But and and the record that's on there, if you

0:39:01.800 --> 0:39:04.279
<v Speaker 1>want to hear some of the stuff, Uh, there are

0:39:04.440 --> 0:39:05.920
<v Speaker 1>there are a lot of different sites out there that

0:39:06.080 --> 0:39:09.080
<v Speaker 1>that keep all the things that aren't on there. It

0:39:09.160 --> 0:39:11.919
<v Speaker 1>tells you what's there, and most of that's pretty easy

0:39:12.000 --> 0:39:13.880
<v Speaker 1>to get access to and listen to. I'll try that.

0:39:13.920 --> 0:39:16.040
<v Speaker 1>We'll try to find one and link it up on social. Yeah,

0:39:16.080 --> 0:39:17.640
<v Speaker 1>we'll see if we can find something. And you know,

0:39:17.719 --> 0:39:20.280
<v Speaker 1>maybe I'll see if I can make it a Spotify

0:39:20.360 --> 0:39:22.799
<v Speaker 1>playlist or something and get a uku lele and play

0:39:22.880 --> 0:39:26.239
<v Speaker 1>Johnny be Good on the ukulele. That's uh, that would

0:39:26.239 --> 0:39:28.520
<v Speaker 1>probably be Johnny please stop. That would be the name

0:39:28.560 --> 0:39:31.640
<v Speaker 1>of that song. All right, So, um, anyway, that's that's

0:39:31.719 --> 0:39:35.719
<v Speaker 1>kind of the the wrap up of the spacecraft and

0:39:35.800 --> 0:39:38.080
<v Speaker 1>the stuff that was aborted. But we still haven't talked

0:39:38.080 --> 0:39:40.200
<v Speaker 1>about the actual science that's returned. So we're going to

0:39:40.320 --> 0:39:42.279
<v Speaker 1>do that in just a moment, but before we do,

0:39:42.800 --> 0:39:53.120
<v Speaker 1>let's take a quick moment to thank our other sponsor. Okay,

0:39:53.200 --> 0:39:55.040
<v Speaker 1>so we've talked about what the mission was, we talked

0:39:55.040 --> 0:39:58.040
<v Speaker 1>about the spacecraft. Let's talk about what the spacecraft found.

0:39:58.920 --> 0:40:01.399
<v Speaker 1>So out of the all in investigation teams that were

0:40:01.480 --> 0:40:04.000
<v Speaker 1>originally involved in the Voyager mission, like I said earlier,

0:40:04.080 --> 0:40:06.359
<v Speaker 1>only five of them are still supported. And those five

0:40:06.440 --> 0:40:12.680
<v Speaker 1>are magnetic field investigation, low energy charged particle investigation, cosmic

0:40:12.880 --> 0:40:16.520
<v Speaker 1>ray investigation, plasma investigation, which is only active on the

0:40:16.560 --> 0:40:19.800
<v Speaker 1>Voyager too because the Voyager ones doesn't work anywhere, and

0:40:19.960 --> 0:40:24.080
<v Speaker 1>plasma wave investigation. So plasma investigation plasma wave investigation two

0:40:24.080 --> 0:40:26.000
<v Speaker 1>different things, right, and these are clearly the more important

0:40:26.040 --> 0:40:27.960
<v Speaker 1>ones because there's not all that much too. For example,

0:40:28.000 --> 0:40:32.400
<v Speaker 1>take pictures of Yeah, once you're done taking the photo

0:40:32.480 --> 0:40:36.120
<v Speaker 1>of the Solar system from way the heck out there,

0:40:36.560 --> 0:40:40.239
<v Speaker 1>there's really no purpose to keep going to that. So yeah,

0:40:40.280 --> 0:40:44.759
<v Speaker 1>that's been shut down. Um, and uh, the five instruments

0:40:44.840 --> 0:40:49.680
<v Speaker 1>that support these five missions are the Magnetic Field Instrument

0:40:49.880 --> 0:40:53.840
<v Speaker 1>or MG, the low energy Charged Particle Instrument, the l

0:40:53.920 --> 0:40:57.920
<v Speaker 1>e CP Cosmic ray instrument that's the CRS, the plasma

0:40:57.920 --> 0:41:00.880
<v Speaker 1>instrument that's p l S, and the Plasma Wave Instrument

0:41:00.920 --> 0:41:05.640
<v Speaker 1>that's p WS. And really at this point, uh, now

0:41:05.680 --> 0:41:08.520
<v Speaker 1>that we've finished taking photos and measurements of all the planets,

0:41:08.560 --> 0:41:11.640
<v Speaker 1>which that was the main science before was really getting

0:41:11.680 --> 0:41:14.680
<v Speaker 1>good images and getting some good scientific data about the

0:41:14.880 --> 0:41:17.400
<v Speaker 1>actual plants and their moons. It was the origin of

0:41:17.480 --> 0:41:19.719
<v Speaker 1>the program. Yeah, before they kind of realized, oh hey,

0:41:19.840 --> 0:41:22.040
<v Speaker 1>we can do more stuff out there. Yeah, so now

0:41:22.400 --> 0:41:24.800
<v Speaker 1>now we're we've switched it over to interstellar. But some

0:41:24.920 --> 0:41:27.680
<v Speaker 1>of the stuff they found because of these and then

0:41:27.840 --> 0:41:31.359
<v Speaker 1>later on have have expounded upon by sending out other

0:41:31.520 --> 0:41:35.720
<v Speaker 1>orbiters like Cassini for example. But some of the stuff

0:41:35.719 --> 0:41:39.600
<v Speaker 1>they discovered were like they took a closer look at Europa,

0:41:39.640 --> 0:41:42.520
<v Speaker 1>which is one of Jupiter's moons, and saw that it

0:41:42.640 --> 0:41:46.680
<v Speaker 1>had a water ice surface, and originally they thought that

0:41:46.760 --> 0:41:51.080
<v Speaker 1>maybe Europa could have an ocean underneath that ice, but

0:41:51.360 --> 0:41:54.640
<v Speaker 1>some scientists now say they think that it's probably more

0:41:54.760 --> 0:41:59.200
<v Speaker 1>like a slush or maybe even solid solid ice, but

0:41:59.400 --> 0:42:02.839
<v Speaker 1>that was a stability um. They the Voyager spacecraft also

0:42:02.920 --> 0:42:06.960
<v Speaker 1>observed Pale, which is the largest of the volcanoes on Io,

0:42:07.320 --> 0:42:11.120
<v Speaker 1>which is the another moon of U, and they observed

0:42:11.160 --> 0:42:15.799
<v Speaker 1>that Paley was erupting sulfur and sulfur dioxide, and these

0:42:15.920 --> 0:42:18.480
<v Speaker 1>eruptions were going up to heights that are equivalent to

0:42:18.560 --> 0:42:23.560
<v Speaker 1>about thirty times the elevation of Mount Everest, the tallest

0:42:23.640 --> 0:42:26.520
<v Speaker 1>mountain on Earth. Multiply that by well, tallest mountain on

0:42:26.600 --> 0:42:30.120
<v Speaker 1>the surface, like not underwater, because you could look at

0:42:30.200 --> 0:42:34.640
<v Speaker 1>underwater and there's but the above water. It's the tallest

0:42:34.680 --> 0:42:37.239
<v Speaker 1>mountain on Earth. Multiply that by thirty times. That's how

0:42:37.440 --> 0:42:40.520
<v Speaker 1>high up these eruptions were going. Not necessarily a good

0:42:40.600 --> 0:42:44.000
<v Speaker 1>vacation spot. Now. The scientists also point out that Io's

0:42:44.000 --> 0:42:46.480
<v Speaker 1>gravity is about six times weaker than that of Earth's,

0:42:46.560 --> 0:42:49.360
<v Speaker 1>so it's closer to what our moon has. But the

0:42:49.400 --> 0:42:53.120
<v Speaker 1>fallout zone for the the the sulfur dioxide that was

0:42:53.200 --> 0:42:57.120
<v Speaker 1>being thrust into the atmosphere of Io was about the

0:42:57.120 --> 0:43:02.560
<v Speaker 1>size of France. Yeah, so uh that was when I

0:43:02.640 --> 0:43:04.520
<v Speaker 1>read that, I was like, wow, that is a huge,

0:43:05.040 --> 0:43:10.600
<v Speaker 1>huge volcano. Um. Now the see what. We also had

0:43:10.640 --> 0:43:15.239
<v Speaker 1>some information about Saturn's largest moon, which is called Titan. Uh.

0:43:15.360 --> 0:43:19.600
<v Speaker 1>It discovered the oceans of ethane and methane aboard aboard

0:43:19.719 --> 0:43:22.719
<v Speaker 1>on Titan, not a board Titan. It is technically a

0:43:22.760 --> 0:43:29.960
<v Speaker 1>space that's not nothing satellite satellite, but it's a natural satellite,

0:43:30.000 --> 0:43:32.560
<v Speaker 1>not a man made one. And it has also discovered

0:43:32.560 --> 0:43:35.720
<v Speaker 1>that has the Titan, the the largest moon of Saturn,

0:43:35.800 --> 0:43:39.040
<v Speaker 1>has a dense atmosphere and lots of hydrocarbons and maybe

0:43:39.840 --> 0:43:42.560
<v Speaker 1>it could possibly at some point in the past have

0:43:42.640 --> 0:43:46.959
<v Speaker 1>supported life. The methane is a possible indication that living

0:43:47.040 --> 0:43:49.560
<v Speaker 1>things once lived there. Now that does not necessarily the

0:43:49.600 --> 0:43:51.840
<v Speaker 1>hydrocarbons as well, but that does not necessarily mean that

0:43:52.000 --> 0:43:56.200
<v Speaker 1>life ever was on Titan, but it's a possibility. Voyager

0:43:56.239 --> 0:43:59.800
<v Speaker 1>also took images of Uranus's rings, which are very difficult

0:43:59.840 --> 0:44:03.520
<v Speaker 1>to they're very faint right um, And but they did that.

0:44:03.600 --> 0:44:07.640
<v Speaker 1>They also observed Saturn's rings and saw that they were

0:44:07.760 --> 0:44:10.680
<v Speaker 1>made of about ten thousand strands of ice particles and

0:44:11.040 --> 0:44:15.400
<v Speaker 1>car sized icebergs, and that if you look at them proportionally,

0:44:16.000 --> 0:44:20.319
<v Speaker 1>their thickness is much much, much, much much smaller than

0:44:20.440 --> 0:44:22.960
<v Speaker 1>the width of the ring. So if you think of

0:44:23.040 --> 0:44:26.279
<v Speaker 1>it as like a one of those things called they're

0:44:26.320 --> 0:44:30.799
<v Speaker 1>not the Frisbees, but you know the rings, they're they're

0:44:30.840 --> 0:44:32.759
<v Speaker 1>hollow in the middle, right, there's there, so it's just

0:44:32.880 --> 0:44:34.880
<v Speaker 1>a it's a disc that doesn't have a center to it.

0:44:35.480 --> 0:44:39.279
<v Speaker 1>Um the width of the band is much wider than

0:44:39.480 --> 0:44:42.400
<v Speaker 1>the thickness of the band, is what they discovered. So

0:44:42.520 --> 0:44:46.000
<v Speaker 1>that was kind of interesting. Uh, now we're talking more

0:44:46.120 --> 0:44:51.120
<v Speaker 1>about the interstellar work, so they're still inside the heliosphere, right,

0:44:51.200 --> 0:44:52.759
<v Speaker 1>And I did want to mention at some point here

0:44:53.080 --> 0:44:56.160
<v Speaker 1>on March, and we mentioned this in another podcast that

0:44:56.320 --> 0:44:59.560
<v Speaker 1>we were recording. Right around March twenty UM, there were

0:44:59.719 --> 0:45:02.920
<v Speaker 1>there were false reports that that it had left the

0:45:02.920 --> 0:45:05.879
<v Speaker 1>helo sphere and entered interstellar space, and those were those

0:45:05.880 --> 0:45:08.520
<v Speaker 1>were false reports. Yeah, NASA came out and said, no,

0:45:09.880 --> 0:45:12.840
<v Speaker 1>we've not seen the changes in the magnetic radiation that

0:45:12.880 --> 0:45:15.000
<v Speaker 1>we are expecting to see. That. They did say that

0:45:15.120 --> 0:45:18.000
<v Speaker 1>they had seen some changes in particle movement, which at

0:45:18.080 --> 0:45:21.879
<v Speaker 1>first would have indicated that the spacecraft had moved out

0:45:21.920 --> 0:45:25.000
<v Speaker 1>of the heliosphere, but then they found from the magnetic

0:45:25.120 --> 0:45:28.320
<v Speaker 1>movement that's not the case. So it's it's one of

0:45:28.360 --> 0:45:30.160
<v Speaker 1>those things where again we keep finding out the Solar

0:45:30.200 --> 0:45:33.240
<v Speaker 1>System is larger as we learn more about how it's behaving.

0:45:33.760 --> 0:45:37.879
<v Speaker 1>So now the next step in this you could think

0:45:37.920 --> 0:45:41.480
<v Speaker 1>of the interstellar exploration and being in three phases. The

0:45:41.560 --> 0:45:43.960
<v Speaker 1>first was crossing the termination shock, which both of the

0:45:44.000 --> 0:45:46.719
<v Speaker 1>spacecraft have already done. The next is the exploration of

0:45:46.760 --> 0:45:50.080
<v Speaker 1>the Helio sheath, which is happening right now, and then

0:45:50.160 --> 0:45:53.080
<v Speaker 1>the third is interstellar exploration, which is when the spacecraft

0:45:53.160 --> 0:45:58.600
<v Speaker 1>have passed beyond the Helio Pause boundary. Now Helio Pause boundary,

0:45:58.600 --> 0:45:59.560
<v Speaker 1>you can think of this as kind of like a

0:45:59.640 --> 0:46:05.200
<v Speaker 1>bubble around the Sun that completely encompasses the the entire

0:46:05.280 --> 0:46:08.279
<v Speaker 1>Solar System. It's not a perfectly round bubble, so don't

0:46:08.280 --> 0:46:11.400
<v Speaker 1>think like that, but it's it's this whibbli wabbli area. Uh,

0:46:11.560 --> 0:46:14.400
<v Speaker 1>And beyond this boundary there's no solar wind or magnetic

0:46:14.520 --> 0:46:18.000
<v Speaker 1>field from the Sun. However, there's still the gravitational influence

0:46:18.120 --> 0:46:21.120
<v Speaker 1>of the Sun at that point, but particles and waves

0:46:21.120 --> 0:46:23.319
<v Speaker 1>in this area of space are unaffected by our Sun,

0:46:23.480 --> 0:46:25.920
<v Speaker 1>and we don't really know a whole lot about them

0:46:25.960 --> 0:46:28.319
<v Speaker 1>because we haven't been able to observe them directly through

0:46:28.520 --> 0:46:30.719
<v Speaker 1>any kind of spacecraft. Right. Yeah, and and this is

0:46:30.920 --> 0:46:34.520
<v Speaker 1>this is a hypothetical heliopause. Yeah, we have not encountered

0:46:34.560 --> 0:46:36.960
<v Speaker 1>it yet, so but it's still not technically the edge

0:46:37.000 --> 0:46:38.960
<v Speaker 1>of the Solar System if you if you ask NASA,

0:46:39.040 --> 0:46:41.520
<v Speaker 1>the edge of the Solar System would be that area

0:46:41.640 --> 0:46:45.399
<v Speaker 1>where there's no longer that gravitational factor from the Sun,

0:46:45.920 --> 0:46:48.839
<v Speaker 1>which would require us to travel about two light years

0:46:48.840 --> 0:46:50.640
<v Speaker 1>away from the Sun. So that will take us about

0:46:50.680 --> 0:46:54.399
<v Speaker 1>forty thousand years for those spacecraft to get there, which

0:46:54.520 --> 0:46:58.319
<v Speaker 1>is a you know, set your alarms because it's gonna

0:46:58.360 --> 0:47:00.440
<v Speaker 1>take a while. So in other words, it'sman tells you

0:47:00.560 --> 0:47:03.640
<v Speaker 1>that the voyager has passed outside the Solar System, your

0:47:03.800 --> 0:47:07.319
<v Speaker 1>response should be wow, which alien warped it away from there?

0:47:07.400 --> 0:47:10.120
<v Speaker 1>Because there's no way that it's done that, at least

0:47:10.160 --> 0:47:12.320
<v Speaker 1>not by the definition that NASA makes. Now, if they're

0:47:12.320 --> 0:47:15.320
<v Speaker 1>talking about the helio pause, that's a different story. Different

0:47:15.360 --> 0:47:17.440
<v Speaker 1>that's a different story. And I think they are anticipating

0:47:17.520 --> 0:47:19.600
<v Speaker 1>that within our lifetimes. Yeah, they said they said they

0:47:19.640 --> 0:47:22.239
<v Speaker 1>expected it to happen within ten to twenty years of

0:47:22.520 --> 0:47:26.240
<v Speaker 1>passing the termination shock. So now it's just probably probably

0:47:26.280 --> 0:47:30.319
<v Speaker 1>hopefully fingers crossed before before that plutoni and dioxide runs

0:47:30.320 --> 0:47:35.560
<v Speaker 1>out right before around that area. So, uh, Lauren, you

0:47:35.640 --> 0:47:39.480
<v Speaker 1>had an interesting idea. One that an experimental idea that

0:47:39.560 --> 0:47:41.239
<v Speaker 1>we thought we would try, which is that you sent

0:47:41.320 --> 0:47:43.359
<v Speaker 1>out a tweet saying, hey, guys, if you have any

0:47:43.600 --> 0:47:47.400
<v Speaker 1>anything interesting that you want to ask or goofy that

0:47:47.520 --> 0:47:50.200
<v Speaker 1>you want to ask us about our podcast about the

0:47:50.280 --> 0:47:53.440
<v Speaker 1>Voyage spacecraft, now's the time to do it. And people did.

0:47:53.880 --> 0:47:55.880
<v Speaker 1>A couple of people did anyway, So hopefully we'll be

0:47:55.920 --> 0:47:57.879
<v Speaker 1>able to do this in the future and get even

0:47:57.960 --> 0:48:00.920
<v Speaker 1>more discussion. But this was a fun first attempt. So

0:48:01.120 --> 0:48:04.360
<v Speaker 1>here's some of the questions we received. Ian on Twitter

0:48:04.480 --> 0:48:06.560
<v Speaker 1>asked a whole bunch of questions that I'm going to

0:48:06.640 --> 0:48:10.160
<v Speaker 1>tackle one at a time. The first was how fast

0:48:10.239 --> 0:48:14.760
<v Speaker 1>are the Voyager spacecraft traveling? Good question, Ian, So Voyager

0:48:14.800 --> 0:48:17.719
<v Speaker 1>one's traveling at about three point six astronomical units per

0:48:17.800 --> 0:48:20.359
<v Speaker 1>year and Voyager two is poking along at three point

0:48:20.480 --> 0:48:23.640
<v Speaker 1>three astronomical units per year. Now, that might not tell

0:48:23.680 --> 0:48:26.320
<v Speaker 1>you very much unless you know how long an astronomical

0:48:26.480 --> 0:48:29.319
<v Speaker 1>unit is. It's a measurement of distance that's based upon

0:48:29.440 --> 0:48:32.359
<v Speaker 1>the mean distance between Earth and the Sun, and that's

0:48:32.400 --> 0:48:36.359
<v Speaker 1>equivalent to about a hundred and forty nine million, five thousand,

0:48:36.400 --> 0:48:40.280
<v Speaker 1>eight hundred swenty one kilometers or two million, nine hundred

0:48:40.320 --> 0:48:43.600
<v Speaker 1>fifty five thousand, eight hundred seven miles. And because Jonathan

0:48:43.640 --> 0:48:45.839
<v Speaker 1>loves you, he did the math yep. So let's talk

0:48:45.840 --> 0:48:48.560
<v Speaker 1>about how this sucker breaks down. So remember, Voyager one's

0:48:48.600 --> 0:48:51.320
<v Speaker 1>going at three point six astronomical units per year. That

0:48:51.360 --> 0:48:56.400
<v Speaker 1>means it's traveling about five hundred thirty nine million kilometers

0:48:56.480 --> 0:49:00.880
<v Speaker 1>per year or three hundred thirty five million in miles

0:49:00.960 --> 0:49:05.080
<v Speaker 1>per year, and that breaks down to four kilometers per

0:49:05.120 --> 0:49:08.400
<v Speaker 1>hour or thirty eight thousand, one seventy six miles per hour.

0:49:08.520 --> 0:49:13.120
<v Speaker 1>Either way, it's going wicked fast. Voyager two is three

0:49:13.160 --> 0:49:15.480
<v Speaker 1>point three astronomical units per year. That breaks down to

0:49:15.560 --> 0:49:19.760
<v Speaker 1>four four million kilometers per year or fifty six thousand,

0:49:20.280 --> 0:49:22.920
<v Speaker 1>eighteen kilometers per hour, and in miles, it's three hundred

0:49:22.960 --> 0:49:25.959
<v Speaker 1>seven million miles per year or thirty five thousand miles

0:49:26.040 --> 0:49:29.560
<v Speaker 1>per hour. Slightly less wicked fast, but still wicked fast,

0:49:29.880 --> 0:49:33.040
<v Speaker 1>but still faster than than me. For example, his next question.

0:49:33.080 --> 0:49:37.240
<v Speaker 1>Ian's next question was are they accelerating? No, next question

0:49:37.400 --> 0:49:40.440
<v Speaker 1>was how long will you remain in contact. Well, like

0:49:40.560 --> 0:49:42.080
<v Speaker 1>we said, we're not really sure. It's all going to

0:49:42.160 --> 0:49:44.920
<v Speaker 1>depend upon the power supply. Uh. And also whether or

0:49:44.960 --> 0:49:47.200
<v Speaker 1>not our antenna here on Earth can continue to pick

0:49:47.239 --> 0:49:52.080
<v Speaker 1>up that week signal, but we expect around five will

0:49:52.120 --> 0:49:54.600
<v Speaker 1>be the last we hear of them. Uh. And then

0:49:54.719 --> 0:49:58.399
<v Speaker 1>Ian and also a listener named Jonathan. Also they both

0:49:58.400 --> 0:50:02.800
<v Speaker 1>asked that we somehow reference a film, Star Trek the

0:50:02.840 --> 0:50:06.160
<v Speaker 1>motion Picture. Okay, what does Voyager have to do with

0:50:06.200 --> 0:50:09.640
<v Speaker 1>Star Trek the Motion Picture? Well, in a way, Voyager

0:50:09.800 --> 0:50:12.400
<v Speaker 1>is the bad guy in Star Trek the motion Picture.

0:50:12.680 --> 0:50:15.239
<v Speaker 1>In another way, the whole film is the bad guy

0:50:15.280 --> 0:50:18.160
<v Speaker 1>because the thing is slow as heck. I watched it.

0:50:18.400 --> 0:50:21.040
<v Speaker 1>I watched it not for anticipation of this podcast. I

0:50:21.120 --> 0:50:24.160
<v Speaker 1>watched it justly, and I had not seen it since

0:50:24.200 --> 0:50:25.960
<v Speaker 1>I was a kid. And I don't think I ever

0:50:26.120 --> 0:50:27.680
<v Speaker 1>sat through it all the way through when I was

0:50:27.719 --> 0:50:29.319
<v Speaker 1>a kid. I don't think I sat through it all

0:50:29.320 --> 0:50:31.200
<v Speaker 1>the way there was an adult, I can't. I can't

0:50:31.200 --> 0:50:32.840
<v Speaker 1>say that i've seen it since I was about a

0:50:33.840 --> 0:50:37.319
<v Speaker 1>laundry and now Star Trek two amazing movie. Star Trek

0:50:37.400 --> 0:50:40.759
<v Speaker 1>the motion Picture not so much. But in that story

0:50:40.880 --> 0:50:42.759
<v Speaker 1>and this is gonna sound really familiar to anyone who

0:50:42.760 --> 0:50:45.200
<v Speaker 1>watched Star Trek four because it's a very similar story.

0:50:45.960 --> 0:50:49.120
<v Speaker 1>A probe that has this weird energy field around it

0:50:49.360 --> 0:50:52.560
<v Speaker 1>enters our Solar system. Actually first it's just moving through space,

0:50:52.880 --> 0:50:57.400
<v Speaker 1>but everything it encounters it's starting to deactivate, and everyone's

0:50:57.640 --> 0:51:01.000
<v Speaker 1>kind of upset because because that's as head of right

0:51:01.040 --> 0:51:03.520
<v Speaker 1>to Earth. So what do we do? How do we

0:51:03.600 --> 0:51:06.279
<v Speaker 1>stop this? And of course the only person who can

0:51:06.360 --> 0:51:10.240
<v Speaker 1>stop it as Kirk, who commandeers this starship, Starship Enterprise.

0:51:10.280 --> 0:51:12.480
<v Speaker 1>He is no longer the captain of the Enterprise at

0:51:12.520 --> 0:51:15.200
<v Speaker 1>that point. He's teaching at star Fleet, but the Enterprise

0:51:15.320 --> 0:51:18.040
<v Speaker 1>is is docked in a space station around Earth, and

0:51:18.120 --> 0:51:21.520
<v Speaker 1>so he, after a very long tour of the ship,

0:51:21.920 --> 0:51:24.480
<v Speaker 1>of the outside of the ship that Scotty takes him on,

0:51:25.040 --> 0:51:28.000
<v Speaker 1>eventually gets on board. And this movie moves slowly, is

0:51:28.040 --> 0:51:31.000
<v Speaker 1>what I'm saying. And just they go and investigate this, uh,

0:51:31.120 --> 0:51:36.160
<v Speaker 1>this probe that's called VJER and UH and VJR is

0:51:36.280 --> 0:51:42.160
<v Speaker 1>this artificially intelligent vehicle and actually the vehicle contains a

0:51:42.320 --> 0:51:46.280
<v Speaker 1>smaller probe like vehicle inside of it. Ultimately they discovered

0:51:46.360 --> 0:51:50.400
<v Speaker 1>that what Vijure really is is Voyager six, which doesn't

0:51:50.440 --> 0:51:53.719
<v Speaker 1>exist yet. No, there's only Voyager one and two. But

0:51:53.920 --> 0:51:55.719
<v Speaker 1>in this in the movie, it was Voyager six that

0:51:55.800 --> 0:51:58.000
<v Speaker 1>was supposedly launched towards the end of the twentieth century,

0:51:58.040 --> 0:51:59.560
<v Speaker 1>which I don't know if you notice, we're not in

0:51:59.600 --> 0:52:02.840
<v Speaker 1>the any or um, so you know, same thing like

0:52:03.320 --> 0:52:06.080
<v Speaker 1>I think the Eugenics Wars and Star Trek two that

0:52:06.120 --> 0:52:08.120
<v Speaker 1>are that ever mentioned that con was part of that

0:52:08.200 --> 0:52:10.799
<v Speaker 1>was supposed to take place in nine, So we had

0:52:10.800 --> 0:52:12.640
<v Speaker 1>a lot of catching up to do. Uh, Not that

0:52:12.719 --> 0:52:15.719
<v Speaker 1>I want those to happen anytime soon. But the the

0:52:16.239 --> 0:52:19.600
<v Speaker 1>VJRE was called vitre because it could no longer uh

0:52:20.320 --> 0:52:24.279
<v Speaker 1>see the letters that were missing, So all the missing

0:52:24.400 --> 0:52:26.360
<v Speaker 1>letters were gone, so all that was left was the

0:52:26.480 --> 0:52:30.239
<v Speaker 1>v g e R. So it's Vidre uh and uh.

0:52:30.480 --> 0:52:32.800
<v Speaker 1>And in the story, what you find out is that

0:52:32.880 --> 0:52:37.760
<v Speaker 1>aliens had encountered the Voyager six probe and had enhanced

0:52:37.800 --> 0:52:40.640
<v Speaker 1>it so that it could learn everything that is learnable

0:52:41.040 --> 0:52:43.400
<v Speaker 1>and then returned the information to Earth. So it was

0:52:43.520 --> 0:52:46.960
<v Speaker 1>trying to do a uh. Originally it was supposed to

0:52:47.000 --> 0:52:50.759
<v Speaker 1>be a benevolent thing, but because vjer had gained sentience,

0:52:51.200 --> 0:52:54.360
<v Speaker 1>it no longer completely understood the parameters of its mission,

0:52:54.520 --> 0:52:57.279
<v Speaker 1>and so it started to go a little bonkers um

0:52:57.640 --> 0:53:01.440
<v Speaker 1>and then of course the some remembers aboard the Enterprise

0:53:01.560 --> 0:53:06.480
<v Speaker 1>end up essentially reasoning with the artificially intelligent probe. So Veder,

0:53:06.600 --> 0:53:08.160
<v Speaker 1>like I said, it's kind of the bad Guy and

0:53:08.239 --> 0:53:10.600
<v Speaker 1>Star Trek the motion picture. If you feel like I

0:53:10.719 --> 0:53:19.480
<v Speaker 1>spoiled that movie, I didn't. It's really I mean, I mean,

0:53:19.520 --> 0:53:22.839
<v Speaker 1>and I say this as someone who loves Star Trek. Okay, don't,

0:53:22.920 --> 0:53:25.040
<v Speaker 1>don't get me wrong, I just I feel like that

0:53:25.200 --> 0:53:28.960
<v Speaker 1>movie was a lot of the movie is played for grandeur,

0:53:29.080 --> 0:53:31.040
<v Speaker 1>and the problem is that we've all gotten used to

0:53:31.239 --> 0:53:34.520
<v Speaker 1>seeing these amazing sort of visuals that are even more

0:53:34.560 --> 0:53:37.719
<v Speaker 1>amazing than what was available back then. So to kind

0:53:37.719 --> 0:53:40.799
<v Speaker 1>of have this big reveal moment and you look at

0:53:40.840 --> 0:53:43.520
<v Speaker 1>the picture and you're like, yeah, okay, it happens on

0:53:43.640 --> 0:53:46.600
<v Speaker 1>TV every week. Yeah, So that's that's a problem alright.

0:53:46.680 --> 0:53:49.080
<v Speaker 1>So uh then we also had a listener who has

0:53:49.160 --> 0:53:52.600
<v Speaker 1>to handle REDNA maybe that's his name, who asked, what

0:53:52.680 --> 0:53:55.800
<v Speaker 1>about future missions with better equipment? Well, we had the

0:53:55.840 --> 0:53:59.279
<v Speaker 1>Cassini orbiter, but we also NASA had proposed a couple

0:53:59.320 --> 0:54:03.160
<v Speaker 1>of joint mission with the European Union. Um, but they

0:54:03.280 --> 0:54:05.480
<v Speaker 1>haven't really worked out. One of them was the Jupiter

0:54:05.680 --> 0:54:10.040
<v Speaker 1>Europa orbiter, but that was essentially scrapped because of budget problems.

0:54:10.080 --> 0:54:13.120
<v Speaker 1>And the other was the Titan Saturn system mission, which

0:54:13.400 --> 0:54:17.200
<v Speaker 1>was shelved in order for NASA to concentrate on the

0:54:17.280 --> 0:54:22.239
<v Speaker 1>Jupiter Europa or better. Yeah so, but but originally those

0:54:22.280 --> 0:54:25.040
<v Speaker 1>were supposed to launch in twenty Now because of the

0:54:25.080 --> 0:54:27.400
<v Speaker 1>budget cutbacks and everything, and you know the fact that

0:54:27.480 --> 0:54:29.520
<v Speaker 1>there just hasn't been the time to develop it, that

0:54:29.760 --> 0:54:32.439
<v Speaker 1>that launch window is kind of closed at this point.

0:54:33.040 --> 0:54:36.399
<v Speaker 1>So um, as far as I know right now, there

0:54:36.520 --> 0:54:41.360
<v Speaker 1>are no definitive deep space or outer planet missions planned.

0:54:41.360 --> 0:54:44.640
<v Speaker 1>I think right now people are really concentrating on Mars,

0:54:44.880 --> 0:54:48.319
<v Speaker 1>Mars and the Moon and Earth orbit. Those are those

0:54:48.360 --> 0:54:52.080
<v Speaker 1>are I mean the things that are I hesitate to

0:54:52.120 --> 0:54:56.320
<v Speaker 1>stay easier but maybe more achievable. Yeah, I have I

0:54:56.400 --> 0:54:59.279
<v Speaker 1>have heard that that that future Moon landings have been

0:54:59.360 --> 0:55:02.400
<v Speaker 1>scrapped in favor of future Mars land Yeah. I mean,

0:55:02.480 --> 0:55:05.520
<v Speaker 1>it's you know, and and this changes from one administration

0:55:05.560 --> 0:55:08.359
<v Speaker 1>to another because because a lot of these considerations are

0:55:08.400 --> 0:55:11.600
<v Speaker 1>not just technological or scientific, they're also political. I mean,

0:55:11.800 --> 0:55:15.160
<v Speaker 1>the whole space race was political, the fact that if

0:55:15.200 --> 0:55:17.879
<v Speaker 1>there had not been that rivalry between the United States,

0:55:19.320 --> 0:55:20.879
<v Speaker 1>but you know, we we can send we can send

0:55:20.920 --> 0:55:23.160
<v Speaker 1>this rocket not only to your face, but all the

0:55:23.200 --> 0:55:25.120
<v Speaker 1>way to the moon. Yeah, So I mean that was

0:55:25.360 --> 0:55:28.400
<v Speaker 1>that was you know, without that kind of pressure than

0:55:28.440 --> 0:55:32.120
<v Speaker 1>it makes it harder for scientists to get the money

0:55:32.200 --> 0:55:34.000
<v Speaker 1>they need to be able to do the science they do.

0:55:34.200 --> 0:55:35.840
<v Speaker 1>That's a sad fact of the world is that, you know,

0:55:36.000 --> 0:55:38.120
<v Speaker 1>money in a way does make the world go round.

0:55:39.160 --> 0:55:41.880
<v Speaker 1>And that wraps up another classic episode of tech stuff.

0:55:41.920 --> 0:55:45.480
<v Speaker 1>Hope you guys enjoyed it. This was a lot of

0:55:45.640 --> 0:55:48.560
<v Speaker 1>fun for us to do. I really had a great

0:55:48.600 --> 0:55:51.120
<v Speaker 1>time with it. I want to do more episodes that

0:55:51.160 --> 0:55:54.960
<v Speaker 1>are space related about specific projects. I've done everything from

0:55:55.080 --> 0:55:58.600
<v Speaker 1>like the Gimin E program or Gimini program to uh,

0:55:58.840 --> 0:56:01.880
<v Speaker 1>you know, like the Apollo O missions, the Space Shuttle missions.

0:56:02.360 --> 0:56:04.239
<v Speaker 1>But I want to look at more of the satellite

0:56:04.280 --> 0:56:06.759
<v Speaker 1>type stuff too. I think that those are really fascinating

0:56:06.800 --> 0:56:08.480
<v Speaker 1>and I've only done a few of them. So if

0:56:08.480 --> 0:56:11.520
<v Speaker 1>there are any specific topics, whether they are space related

0:56:11.640 --> 0:56:14.560
<v Speaker 1>or otherwise, let me know, you know, ones that you

0:56:14.600 --> 0:56:17.040
<v Speaker 1>want to hear anyway, let me know about it. Reach

0:56:17.080 --> 0:56:19.319
<v Speaker 1>out on Twitter or on Facebook. The handle for both

0:56:19.440 --> 0:56:21.880
<v Speaker 1>is text Stuff h SW and I'll talk to you

0:56:21.960 --> 0:56:30.680
<v Speaker 1>again really soon. Text Stuff is an I Heart Radio production.

0:56:30.960 --> 0:56:33.719
<v Speaker 1>For more podcasts from I Heart Radio, visit the I

0:56:33.880 --> 0:56:37.040
<v Speaker 1>Heart Radio app, Apple Podcasts, or wherever you listen to

0:56:37.160 --> 0:56:38.080
<v Speaker 1>your favorite shows.