WEBVTT - InSight into Mars

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<v Speaker 1>Get in touch with technology with tech Stuff from how

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<v Speaker 1>stuff works dot com. Hey there, and welcome to tech Stuff.

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<v Speaker 1>I'm your host, Jonathan Strickland. I'm an executive producer with

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<v Speaker 1>House to Parks and I heart radio and I love

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<v Speaker 1>all things tech. And On November two, eighteen, after traveling

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<v Speaker 1>four hundred fifty eight million kilometers or three hundred million

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<v Speaker 1>miles on a trip that lasted nearly seven months, the

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<v Speaker 1>robot platform Insight touched down on the surface of Mars.

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<v Speaker 1>They marked the eighth time the United States has managed

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<v Speaker 1>to land a mission on Mars successfully. So we're gonna

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<v Speaker 1>take a look at this lander, what it does, and

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<v Speaker 1>what it's mission parameters are. Before I get into Insights specifically,

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<v Speaker 1>it's a good time to chat about the logistics of

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<v Speaker 1>just getting to Mars in general. You may have heard

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<v Speaker 1>that if we were to send people to Mars, they

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<v Speaker 1>need to stay there for about two years before they

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<v Speaker 1>could return. So why is that, Well, it's because of

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<v Speaker 1>the respective orbits of Earth and Mars. Mars is further

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<v Speaker 1>out from the Sun than the Earth is, and a

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<v Speaker 1>Martian year lasts six hundred eighty seven Earth days or

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<v Speaker 1>six hundred sixty nine souls or Martian days compared to

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<v Speaker 1>an Earth year, which has of course three hundred sixty

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<v Speaker 1>five days, unless it's a leap year. So there are

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<v Speaker 1>times when Earth and Mars are relatively close, and by

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<v Speaker 1>relatively I mean nearly thirty five million miles or fifty

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<v Speaker 1>six million kilometers apart, and there are other times when

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<v Speaker 1>they are opposite each other with the Sun in the center,

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<v Speaker 1>they're bout as far apart as they possibly can be.

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<v Speaker 1>Space travel is expensive and it requires a lot of fuel.

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<v Speaker 1>Fuel ways a lot, and the heavier year spacecraft gets,

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<v Speaker 1>the more fuel you need, so you end up in

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<v Speaker 1>this sort of cycle up to a point where you

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<v Speaker 1>have to keep adding fuel to lift not just the

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<v Speaker 1>spacecraft but the fuel you are already have in it.

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<v Speaker 1>So that means you get to be super careful with

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<v Speaker 1>how heavy your spacecraft is so that you can be

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<v Speaker 1>very efficient with the amount of fuel you're going to

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<v Speaker 1>need to get to your destination. So that includes playing

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<v Speaker 1>your trips so that you travel the shortest possible distance

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<v Speaker 1>between two points, taking the least amount of time to

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<v Speaker 1>get from point A to point B. So you want

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<v Speaker 1>to set a launch date in advance of a time

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<v Speaker 1>when Earth and Mars are going to be relatively close

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<v Speaker 1>to each other. That's the launch window we want to

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<v Speaker 1>look at. But of course Mars is moving the whole

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<v Speaker 1>time as his Earth. So really you're setting a launch

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<v Speaker 1>window to aim at the point in space where Mars

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<v Speaker 1>is going to be in several months after the launch.

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<v Speaker 1>It's actually pretty complicated stuff. I mean, they do call

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<v Speaker 1>it rocket science. Even when you take advantage of orbital paths,

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<v Speaker 1>you're still talking about a trip that will take between

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<v Speaker 1>six and eight months using conventional rockets, So you have

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<v Speaker 1>to settle in for a long trip. Now, once you

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<v Speaker 1>get to Mars, you won't be able to leave right

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<v Speaker 1>away if you have a method of leaving in the

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<v Speaker 1>first place, you would have to wait around for Earth

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<v Speaker 1>and Mars to be nearing one another again. And a

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<v Speaker 1>launch window for the minimal amount of energy needed to

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<v Speaker 1>get between the two comes around only every two Earth

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<v Speaker 1>years and two Earth months, So you need enough fuel

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<v Speaker 1>to make the trip home, or you need some way

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<v Speaker 1>to make the fuel at your destination, such as Mars,

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<v Speaker 1>so that you can make the return trip. Now, you

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<v Speaker 1>could make going to Mars a one way trip, and

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<v Speaker 1>considering how hostile the planet is and how hard it

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<v Speaker 1>would be to get back. That's probably not entirely unrealistic,

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<v Speaker 1>if I'm being honest. We'll talk more about that in

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<v Speaker 1>our next episode, but before we decide to shove someone

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<v Speaker 1>off into space for a life sentence on Mars, we

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<v Speaker 1>can send other craft to the red planet, and in

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<v Speaker 1>fact we have that includes orbiters, which, as the name suggests,

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<v Speaker 1>orbits the planet and gathers information about it. Landers, which

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<v Speaker 1>has the name suggests, lands on the planet and gathers

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<v Speaker 1>information about it. And rovers, which, again the name tells

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<v Speaker 1>you everything you need to know. It roves about on

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<v Speaker 1>the planet, gathering information and you know, doing sick donuts,

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<v Speaker 1>and the name is pretty much tell you everything you

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<v Speaker 1>need to know about them, at least in a general sense.

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<v Speaker 1>So landing on Mars, particularly if you want to do

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<v Speaker 1>a soft landing, is pretty challenging as well. That's because

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<v Speaker 1>of several factors. One is that the Martian atmosphere is

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<v Speaker 1>much thinner than Earth's, so stuff like parachutes are less effective.

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<v Speaker 1>They do work, but they don't slow down to scent

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<v Speaker 1>quite as effectively as they would if you were using

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<v Speaker 1>them on Earth. However, the atmosphere is thick enough to

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<v Speaker 1>cause heating problems. Upon entry of the atmosphere, the spacecraft

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<v Speaker 1>starts to come in at a very high speed, it

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<v Speaker 1>hits the atmosphere, starts to compress the atmosphere in front

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<v Speaker 1>of it, and it begins to heat up rapidly. So

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<v Speaker 1>whatever your spacecraft is, you need some really good heat

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<v Speaker 1>shielding to take care of that problem. That of course

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<v Speaker 1>adds to the weight of the spacecraft. And while gravity

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<v Speaker 1>on Mars is less intense than on Earth, the gravity

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<v Speaker 1>on Mars is about point three eight times out of

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<v Speaker 1>Earth's gravity. Descending from Martian orbit still means you're going

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<v Speaker 1>at a speed that's plenty fast enough to cause serious

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<v Speaker 1>damage when you hit the ground, So you have to

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<v Speaker 1>have a way to slow your descent. One way to

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<v Speaker 1>offset that incredibly fast descent is to have special retro

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<v Speaker 1>rockets on the landing craft and to fire those before

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<v Speaker 1>you land so that you have a nice and gentle touchdown.

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<v Speaker 1>That really would help slow the descent. But here's the

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<v Speaker 1>thing with these craft that we're sending the landers and

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<v Speaker 1>the rovers. For the ones that we're using for a

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<v Speaker 1>soft landing, they have to rely upon a fully automated system.

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<v Speaker 1>Because the distance between Mars and Earth is such that

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<v Speaker 1>it takes several minutes for radio signals to pass back

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<v Speaker 1>and forth between the two. Radio signals move at the

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<v Speaker 1>speed of light, but the distances involved are so great

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<v Speaker 1>that even light requires a few minutes to get the

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<v Speaker 1>job done. So if you were looking at a video

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<v Speaker 1>feed from the spacecraft, let's say that there's a live

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<v Speaker 1>camera feed and it's able to send video back to Earth.

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<v Speaker 1>This would be unrealistic, But let's say it's happening. What

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<v Speaker 1>you would actually be looking at would be video from

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<v Speaker 1>several minutes ago. The video footage would be several minutes old,

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<v Speaker 1>because that's how long it took for the information to

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<v Speaker 1>travel from the the lander or rover on Mars to

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<v Speaker 1>get to you on Earth. Sending a message to the

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<v Speaker 1>lander would obviously take more time. So let's say you

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<v Speaker 1>see a picture and you think, oh, well, that's that

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<v Speaker 1>rock over there is interesting. I want this thing to

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<v Speaker 1>go grab that rock, and you send a command to

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<v Speaker 1>the device. Well, keep in mind the picture you're looking

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<v Speaker 1>at it several minutes old. When you send the message,

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<v Speaker 1>it takes several more minutes for it to get back.

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<v Speaker 1>The device then has to react to it, and it

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<v Speaker 1>will take even more minutes for you to know that

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<v Speaker 1>anything actually happened, so there's no way to make any

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<v Speaker 1>adjustments in real time at all. So that's why the

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<v Speaker 1>system has to be fully automated. When it's landing, there's

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<v Speaker 1>no way to step in and take control of it

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<v Speaker 1>as a remote pilot, because the distances are so great

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<v Speaker 1>that by the time you're sending commands, the thing you're

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<v Speaker 1>trying to command has already crashed into Mars. So you

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<v Speaker 1>have to create this automated system. The landing process for

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<v Speaker 1>this lander would take about six and a half minutes

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<v Speaker 1>from the point it enters the Martian atmosphere to the

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<v Speaker 1>point that it landed on the surface. NASA would call

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<v Speaker 1>this the seven minutes of Terror. That six and a

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<v Speaker 1>half minutes would include every single thing that would have

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<v Speaker 1>to happen in this process of entering the atmosphere all

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<v Speaker 1>the way to the point of firing the retro gets

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<v Speaker 1>at settling down on the surface of Mars. If anything

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<v Speaker 1>were to go wrong at any stage there, whether it

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<v Speaker 1>maybe it's a parachute that fails to deploy, a thruster

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<v Speaker 1>that fires a second too late, whatever it would be,

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<v Speaker 1>all would be lost. Chances are you would have a

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<v Speaker 1>total loss of the spacecraft. In addition, that distance between

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<v Speaker 1>Earth and Mars would mean we wouldn't even know that

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<v Speaker 1>something had gone wrong until about eight minutes after it

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<v Speaker 1>had gone wrong, So if the lander were to crash

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<v Speaker 1>and be destroyed, it would have been destroyed for eight

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<v Speaker 1>minutes before we knew about it. Also, it meant that

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<v Speaker 1>picking a landing site is incredibly important. You want to

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<v Speaker 1>find the best possible site to target so that your

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<v Speaker 1>lander or rover, whatever it may be, has the best

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<v Speaker 1>possible chance of survival. NASA had to find a spot

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<v Speaker 1>that not only would be optimal for whatever the mission

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<v Speaker 1>objectives happened to be. In this case, it's all about

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<v Speaker 1>measuring various uh features of Mars, but it also has

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<v Speaker 1>to be geographically favorable for that successful landing and for

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<v Speaker 1>a continued operation. Sou with the case of the Insight,

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<v Speaker 1>it also meant that having to pick a spot that

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<v Speaker 1>would be favorable for solar panels, because that's how the

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<v Speaker 1>the Insight lander recharges its batteries. So for that reason,

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<v Speaker 1>they chose a spot near the equator because that would

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<v Speaker 1>maximize solar exposure, and because you're relying upon automated systems

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<v Speaker 1>to guide the landing craft to the surface. You also

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<v Speaker 1>have to pick a location that's relatively flat and free

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<v Speaker 1>of large rocks or boulders that could cause the craft

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<v Speaker 1>to topple over after touchdown. That is a tough thing

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<v Speaker 1>to look for on Mars. Mars is very very rocky

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<v Speaker 1>and uneven in many places, but the team in NASA

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<v Speaker 1>eventually chose a region of Mars called the Elysium Planetia.

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<v Speaker 1>That was way back in when they made that choice.

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<v Speaker 1>That first, NASA had more than twenty potential landing sites

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<v Speaker 1>identify light. Then the team directed the Mars Reconnaissance orbiter

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<v Speaker 1>to gather images of those sites so that they could

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<v Speaker 1>choose the best candidates. Each potential site measured eighty one

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<v Speaker 1>miles by seventeen miles in an elliptical shape. That's a

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<v Speaker 1>hundred thirty kilometers by twenty seven kilometers. The insight landing

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<v Speaker 1>location is about three d seventy miles or six hundred

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<v Speaker 1>kilometers away from where the curiosity rover is, so it's

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<v Speaker 1>probably not going to get a visit from its fellow

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<v Speaker 1>robot anytime soon, and a monitor the progress of the

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<v Speaker 1>actual landing. NASA sent up a pair of small satellites

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<v Speaker 1>called cube SATs. Along with the Insight These were the

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<v Speaker 1>first two cubes AT spacecraft to journey into deep space.

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<v Speaker 1>They are communications relay satellites. These particular cube SAT satellites

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<v Speaker 1>are the Jet Propulsion Laboratory designed and built them. The

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<v Speaker 1>basic unit of a cube sat is a box about

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<v Speaker 1>ten centimeters or four inches to a side, and CubeSats

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<v Speaker 1>can be made up of multiple units, and the two

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<v Speaker 1>that were hitching a ride with Insight were each six

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<v Speaker 1>units large. The job of those two satellites involved flying

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<v Speaker 1>by Mars and listening for Insights signal that would indicate

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<v Speaker 1>a successful landing. The CubeSats both have UHF capabilities, though

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<v Speaker 1>they can only receive UHF radio signals and X band capabilities,

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<v Speaker 1>which meant they could receive and transmit over those frequencies. Interestingly,

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<v Speaker 1>those satellites separated from the launch vehicle that was an

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<v Speaker 1>Atlas five rocket, and they did so independently of the

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<v Speaker 1>Insight cruise spacecraft, and so they flew to Mars on

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<v Speaker 1>their own trajectories and with their own course adjustments in

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<v Speaker 1>order to get to where they needed to be for

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<v Speaker 1>the actual landing procedure. The satellites also served as a

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<v Speaker 1>pilot program to test the viability of a bring your

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<v Speaker 1>own communications relay with a short development cycle into deep space,

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<v Speaker 1>and it worked. Now I have a lot more to

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<v Speaker 1>say about INSIGHT and what it does, but before we

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<v Speaker 1>get to that, take a quick break to thank our sponsor.

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<v Speaker 1>The full name for INSIGHT is the Interior Exploration using

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<v Speaker 1>Seismic Investigations, GEO Daisy and Heat Transport. And I have

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<v Speaker 1>a sneaking suspicion. This is another case of a mission

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<v Speaker 1>getting a fun name and then a project team tries

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<v Speaker 1>to work backward to make that name into an acronym.

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<v Speaker 1>But I don't know that for sure. The purpose of

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<v Speaker 1>the mission is to deduce how celestial bodies that have

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<v Speaker 1>a rocky surface are formed, how do they come to be.

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<v Speaker 1>This would include planets like Earth, as well as satellites

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<v Speaker 1>like our Moon, and of course planets like Mars. The

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<v Speaker 1>Lander is going to do this by using several scientific

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<v Speaker 1>instruments to study the deep interior of Mars, and then

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<v Speaker 1>the team back on Earth is going to take the

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<v Speaker 1>information and form hypotheses to explain the formation process. The

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<v Speaker 1>Lander will also gather data that will allow scientists on

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<v Speaker 1>Earth to make educated guesses about Mars's core. So this

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<v Speaker 1>is really cool. This is all about observing planet's behavior

0:13:13.720 --> 0:13:17.160
<v Speaker 1>in a way and then drawing conclusions about what that

0:13:17.240 --> 0:13:22.000
<v Speaker 1>means for the planet, what how the planet is made up,

0:13:22.040 --> 0:13:24.240
<v Speaker 1>you know, what sort of core it has, that kind

0:13:24.280 --> 0:13:27.520
<v Speaker 1>of stuff, and it's all about working backward based upon

0:13:27.559 --> 0:13:32.200
<v Speaker 1>these observations. I love this kind of science. Insight is

0:13:32.280 --> 0:13:36.240
<v Speaker 1>kind of like the Phoenix Lander, and that both of

0:13:36.280 --> 0:13:40.600
<v Speaker 1>those are stationary robotic platforms, so it's not like the Spirit,

0:13:40.679 --> 0:13:45.080
<v Speaker 1>Opportunity or Curiosity rovers. Those are all robots with wheels

0:13:45.120 --> 0:13:47.240
<v Speaker 1>that can move around the surface of Mars. Actually, the

0:13:47.240 --> 0:13:50.760
<v Speaker 1>Opportunity and Curiosity rovers are still in operation to this day.

0:13:51.760 --> 0:13:54.640
<v Speaker 1>Opportunity landed on Mars in two thousand four and Curiosity

0:13:54.720 --> 0:13:56.840
<v Speaker 1>landed in two thousand twelve, and there's still kind of

0:13:56.920 --> 0:14:01.040
<v Speaker 1>roaming around. But insights job is to monitor conditions from

0:14:01.080 --> 0:14:04.200
<v Speaker 1>a set location over the course of a Martian year

0:14:04.320 --> 0:14:09.200
<v Speaker 1>plus forty or so martian days. Insight is a pretty

0:14:09.640 --> 0:14:13.720
<v Speaker 1>large lander. NASA describes it as being about the size

0:14:13.840 --> 0:14:18.400
<v Speaker 1>of a big nineteen sixties convertible. That's a quote, but

0:14:18.559 --> 0:14:22.280
<v Speaker 1>this is tech stuffs. Let's get technical. What are the

0:14:22.360 --> 0:14:26.680
<v Speaker 1>specs for the Insight Lander, well, it is six ms long.

0:14:26.920 --> 0:14:30.760
<v Speaker 1>That's about nineteen ft eight inches, assuming you're measuring it

0:14:30.800 --> 0:14:33.880
<v Speaker 1>when it's solar panels are deployed. Again, we'll talk about

0:14:33.880 --> 0:14:36.480
<v Speaker 1>the solar planel panels in just a minute. It's got

0:14:36.560 --> 0:14:39.560
<v Speaker 1>a width of one point five six ms that's about

0:14:39.640 --> 0:14:43.440
<v Speaker 1>five ft one inch. Uh. The deck height, so the

0:14:43.440 --> 0:14:46.720
<v Speaker 1>the top surface of the main portion of the lander

0:14:47.360 --> 0:14:51.080
<v Speaker 1>ranges from eighty three centimeters to one centimeters tall or

0:14:51.160 --> 0:14:54.560
<v Speaker 1>thirty three to forty three inches. The whole thing weighs

0:14:54.560 --> 0:14:58.480
<v Speaker 1>in at a smelt three d sixty ms. Technically that's

0:14:58.480 --> 0:15:01.800
<v Speaker 1>its mass. Uh we If we're expressing it in pounds,

0:15:01.840 --> 0:15:05.800
<v Speaker 1>it would be seven pounds here on Earth. Remember, on

0:15:05.920 --> 0:15:10.120
<v Speaker 1>Mars the mass is the same, but it weighs less

0:15:10.400 --> 0:15:12.600
<v Speaker 1>because again, mars Is gravity is a little more than

0:15:12.680 --> 0:15:15.640
<v Speaker 1>one third that of Earth's gravity. The lander has a

0:15:15.640 --> 0:15:18.760
<v Speaker 1>lot of cool gadgets attached to it. It draws power

0:15:18.840 --> 0:15:22.160
<v Speaker 1>through batteries that are recharged by those solar panels I

0:15:22.200 --> 0:15:26.920
<v Speaker 1>had mentioned. Those actually had to deploy after Insight touched down,

0:15:27.040 --> 0:15:30.400
<v Speaker 1>before they were all folded up and tucked away on

0:15:30.440 --> 0:15:34.200
<v Speaker 1>the sides of the platform for safety. About an hour

0:15:34.320 --> 0:15:39.160
<v Speaker 1>after touchdown, they began the deployment phase and this involves

0:15:39.280 --> 0:15:42.680
<v Speaker 1>unfolding and then they can start catching the sun's rays.

0:15:42.760 --> 0:15:45.200
<v Speaker 1>And there's a great website for the lander over at

0:15:45.280 --> 0:15:50.600
<v Speaker 1>NASA's Jet Propulsion Laboratory that shows animations of the solar

0:15:50.640 --> 0:15:53.960
<v Speaker 1>panels deploying as well as the other tools and how

0:15:54.000 --> 0:15:57.480
<v Speaker 1>those get deployed. The animations are fantastic, they really help

0:15:57.560 --> 0:16:00.680
<v Speaker 1>a lot, So I highly recommend if you're interested in

0:16:00.720 --> 0:16:04.520
<v Speaker 1>the Insight Lander checking out the interactive web page over

0:16:04.720 --> 0:16:09.280
<v Speaker 1>at the Jet Propulsion Laboratory because it's it's fantastic and

0:16:09.360 --> 0:16:12.400
<v Speaker 1>it looks super cool. Uh. The panels, the solar panels

0:16:12.400 --> 0:16:16.200
<v Speaker 1>are decagonal. That means they have ten straight sides and angles.

0:16:16.240 --> 0:16:19.760
<v Speaker 1>You know, an octagon is eight sides and eight angles.

0:16:19.800 --> 0:16:23.760
<v Speaker 1>A decagon is ten, so they're kind of circular in shape,

0:16:23.840 --> 0:16:27.240
<v Speaker 1>but they have those flat edges. The panels measure about

0:16:27.280 --> 0:16:31.080
<v Speaker 1>seven feet or two meters across, and there are two

0:16:31.160 --> 0:16:34.040
<v Speaker 1>of them. Has a pair of these solar panels. According

0:16:34.080 --> 0:16:37.000
<v Speaker 1>to one NASA web page, the combined surface area of

0:16:37.000 --> 0:16:40.040
<v Speaker 1>the two solar panels is quote as large as a

0:16:40.120 --> 0:16:43.640
<v Speaker 1>ping pong table end quote. So you know, some light

0:16:43.680 --> 0:16:47.280
<v Speaker 1>recreation on Mars. If you if you decide that it's

0:16:47.440 --> 0:16:50.520
<v Speaker 1>served its purpose, I guess they're able to generate about

0:16:50.520 --> 0:16:55.040
<v Speaker 1>three thousand what hours of electricity every martian day. Another

0:16:55.120 --> 0:16:59.360
<v Speaker 1>important component on this lander is its robot arm. The

0:16:59.520 --> 0:17:02.960
<v Speaker 1>arm has three degrees of freedom and those roughly translate

0:17:03.480 --> 0:17:07.600
<v Speaker 1>to a human shoulder, elbow, and wrist joint. The arm

0:17:07.680 --> 0:17:10.479
<v Speaker 1>has four motors to control the movements of the arm

0:17:10.520 --> 0:17:12.640
<v Speaker 1>and those joints. And at the end of the arm,

0:17:12.680 --> 0:17:16.480
<v Speaker 1>instead of there being a hand or like a claw,

0:17:17.040 --> 0:17:20.879
<v Speaker 1>there's actually a grapple. It's attached by a cable. It

0:17:21.040 --> 0:17:24.840
<v Speaker 1>dangles at the end of the arm, and this is

0:17:24.960 --> 0:17:27.960
<v Speaker 1>used to grasp the various tools on the platform deck

0:17:28.119 --> 0:17:31.520
<v Speaker 1>in order to lift them up and deploy them onto Mars' surface.

0:17:32.280 --> 0:17:35.480
<v Speaker 1>So it kind of looks like one of those claw

0:17:35.600 --> 0:17:39.480
<v Speaker 1>games you see in arcades or in the Toy Story film.

0:17:39.520 --> 0:17:41.800
<v Speaker 1>It kind of looks like that, except that the claw

0:17:41.960 --> 0:17:46.320
<v Speaker 1>does not descend and ascend. The cable doesn't unwind and wind.

0:17:46.880 --> 0:17:49.200
<v Speaker 1>It stays the same length, so the arm itself will

0:17:49.240 --> 0:17:53.600
<v Speaker 1>tilt up or down. But the claw does dangle from

0:17:53.640 --> 0:17:57.200
<v Speaker 1>a cable. It just the cable itself is stationary. It's

0:17:57.520 --> 0:18:00.520
<v Speaker 1>also got a firm grip, which also means it's not

0:18:00.560 --> 0:18:02.800
<v Speaker 1>really like a claw game because those things are rigged

0:18:02.840 --> 0:18:07.679
<v Speaker 1>I tell you, stupid Teddy Bear. Anyway, it's a super

0:18:07.720 --> 0:18:13.240
<v Speaker 1>cool way of manipulating objects on the lander, and again

0:18:13.280 --> 0:18:16.760
<v Speaker 1>the animations are really fun to watch. There's a camera

0:18:17.040 --> 0:18:20.960
<v Speaker 1>mounted on this arm it's actually between the elbow and

0:18:21.040 --> 0:18:24.959
<v Speaker 1>wrist joints that can provide NASA images of Mars and

0:18:25.040 --> 0:18:27.639
<v Speaker 1>help the team make sure that the instrumentation that's attached

0:18:27.680 --> 0:18:30.920
<v Speaker 1>to the platform is properly deployed. In fact, it's called

0:18:30.960 --> 0:18:34.520
<v Speaker 1>the Instrument Deployment Camera or i d C. So the

0:18:34.520 --> 0:18:37.520
<v Speaker 1>main purpose for the arm is to place the two

0:18:37.680 --> 0:18:40.600
<v Speaker 1>of the three main sensors on the platform, two of

0:18:40.640 --> 0:18:46.000
<v Speaker 1>the three main scientific experiments really on the surface of Mars.

0:18:46.000 --> 0:18:50.040
<v Speaker 1>More on those two experiments in just a moment. The

0:18:50.119 --> 0:18:53.280
<v Speaker 1>lander actually has a second camera. That one is mounted

0:18:53.680 --> 0:18:56.399
<v Speaker 1>just below the surface of the deck. This one is

0:18:56.440 --> 0:19:00.479
<v Speaker 1>called the Instrument Context Camera or i C SEE, and

0:19:00.560 --> 0:19:03.119
<v Speaker 1>it has a fish eye perspective with a field of

0:19:03.160 --> 0:19:06.560
<v Speaker 1>view of about hundred twenty degrees. It's aimed at the

0:19:06.640 --> 0:19:11.440
<v Speaker 1>ground near the lander that serves as the landers work space.

0:19:12.080 --> 0:19:15.200
<v Speaker 1>So both cameras have a resolution of one thousand, twenty

0:19:15.200 --> 0:19:18.760
<v Speaker 1>four by one pixels, which is not quite a two

0:19:18.840 --> 0:19:23.920
<v Speaker 1>megapixel image. And in an interesting analogy, NASA has compared

0:19:23.960 --> 0:19:26.919
<v Speaker 1>the mission to a human getting a medical check up.

0:19:27.200 --> 0:19:31.240
<v Speaker 1>The Insight Lander is going to check Mars's vitals, which

0:19:31.280 --> 0:19:35.800
<v Speaker 1>includes the planet's pulse, temperature, and reflexes. So what was

0:19:35.840 --> 0:19:39.040
<v Speaker 1>that all about. Well, these are all kind of cute

0:19:39.040 --> 0:19:42.879
<v Speaker 1>ways to talk about the main instruments and scientific projects

0:19:42.920 --> 0:19:46.280
<v Speaker 1>connected to the Insight Lander. So let's start with the pulse,

0:19:46.960 --> 0:19:49.920
<v Speaker 1>the pulse of the planet in this case. In this context,

0:19:50.040 --> 0:19:55.399
<v Speaker 1>it refers to the seismological events on Mars. So things

0:19:55.440 --> 0:19:58.440
<v Speaker 1>that make the earth shake, or I guess I should

0:19:58.440 --> 0:20:02.720
<v Speaker 1>say Mars shake, it's not the earth there so, or

0:20:02.760 --> 0:20:05.480
<v Speaker 1>as my former co host Crispalett would say, stuff what

0:20:05.600 --> 0:20:08.800
<v Speaker 1>makes the ground shake. One of the instruments inside has

0:20:09.280 --> 0:20:12.720
<v Speaker 1>is a special seismometer with a super cool wind and

0:20:12.840 --> 0:20:17.400
<v Speaker 1>thermal shield. The seismometer has a cable tether that connects

0:20:17.440 --> 0:20:21.000
<v Speaker 1>it back to the Insight Lander, and the cable's purpose

0:20:21.080 --> 0:20:24.160
<v Speaker 1>is twofold. It contains both the power line and the

0:20:24.240 --> 0:20:27.800
<v Speaker 1>data line for the seismometer. So this is the way

0:20:27.840 --> 0:20:31.240
<v Speaker 1>that the lander can provide electricity to the seismometer, and

0:20:31.240 --> 0:20:34.600
<v Speaker 1>the seismometer can feed data back to the lander. The

0:20:34.640 --> 0:20:36.520
<v Speaker 1>illustrations I've looked at make it a little like the

0:20:36.520 --> 0:20:40.639
<v Speaker 1>insight lander is kind of walking a weird, lumpy robot dog.

0:20:41.280 --> 0:20:44.680
<v Speaker 1>The lander's robotic arm is responsible for lifting the seismometer

0:20:44.880 --> 0:20:47.600
<v Speaker 1>off the platform and placing it on the surface of

0:20:47.640 --> 0:20:50.800
<v Speaker 1>Mars near the lander itself. Then it has to put

0:20:50.840 --> 0:20:55.480
<v Speaker 1>the uh the thermal and wind shield over the seismometer.

0:20:56.000 --> 0:20:58.040
<v Speaker 1>The purpose of the shield is pretty much what sounds like.

0:20:58.119 --> 0:21:01.320
<v Speaker 1>It's meant to protect the seismometer from gusts of wind,

0:21:01.400 --> 0:21:06.000
<v Speaker 1>primarily that would possibly cause the seizemometer to register false readings.

0:21:06.040 --> 0:21:09.080
<v Speaker 1>If the wind pushes the seismometer around that it's going

0:21:09.119 --> 0:21:12.600
<v Speaker 1>to start registering as if there's an earthquake or Mars quake.

0:21:12.680 --> 0:21:16.080
<v Speaker 1>I guess this way, the shield blocks that wind and

0:21:16.160 --> 0:21:20.840
<v Speaker 1>the seizemometer just keeps on, you know, monitoring the movement

0:21:21.000 --> 0:21:24.800
<v Speaker 1>of the ground beneath it. The wind and thermal shield

0:21:24.920 --> 0:21:28.280
<v Speaker 1>is made out of aluminum. The main shielding part on

0:21:28.280 --> 0:21:30.280
<v Speaker 1>the top anyway, is made out of aluminum. It looks

0:21:30.320 --> 0:21:32.840
<v Speaker 1>like a dome with little lander legs almost like a

0:21:32.840 --> 0:21:36.639
<v Speaker 1>little ufo. It also has a metallic skirt that hangs

0:21:36.720 --> 0:21:40.719
<v Speaker 1>down beneath the dome. It's the thermal skirt. It's actually

0:21:40.760 --> 0:21:45.080
<v Speaker 1>made out of gold. And then this gold skirt has

0:21:45.119 --> 0:21:47.680
<v Speaker 1>a bottom edge made out of and I am not

0:21:48.280 --> 0:21:51.120
<v Speaker 1>making this up, honest to goodness, the edge is made

0:21:51.119 --> 0:21:56.120
<v Speaker 1>out of chain mail, like the stuff that nights used

0:21:56.160 --> 0:21:59.200
<v Speaker 1>to wear back in medieval times. How cool is that?

0:21:59.680 --> 0:22:03.000
<v Speaker 1>So this chain mail actually serves a couple of different purposes.

0:22:03.040 --> 0:22:05.679
<v Speaker 1>For one, it's it's heavier than the skirt is, so

0:22:05.720 --> 0:22:08.560
<v Speaker 1>it helps pull down on the skirt while the little

0:22:08.680 --> 0:22:11.879
<v Speaker 1>arm is lifting the shield up off the deck of

0:22:12.000 --> 0:22:15.760
<v Speaker 1>the lander. The chain mail provides the weight to help

0:22:15.880 --> 0:22:19.320
<v Speaker 1>pull the skirt straight so that it goes down all

0:22:19.400 --> 0:22:23.120
<v Speaker 1>around the sides of the seismometer. Also, the chain mail

0:22:23.240 --> 0:22:27.080
<v Speaker 1>is flexible, so it can drape over any small pebbles

0:22:27.160 --> 0:22:29.679
<v Speaker 1>or rocks to allow a pretty good seal of the

0:22:29.720 --> 0:22:33.400
<v Speaker 1>shield over the seismometer. The shield itself is about fourteen

0:22:33.480 --> 0:22:36.960
<v Speaker 1>inches or thirty five centimeters tall, twenty seven inches or

0:22:37.040 --> 0:22:40.119
<v Speaker 1>sixty nine centimeters in diameter, and has a mass of

0:22:40.119 --> 0:22:42.760
<v Speaker 1>twelve kilograms, which means here on Earth it would weigh

0:22:42.800 --> 0:22:46.000
<v Speaker 1>about twenty six and a half pounds. I'll finish up

0:22:46.080 --> 0:22:49.840
<v Speaker 1>this section by giving a quick overview of how seismometers work,

0:22:49.880 --> 0:22:52.439
<v Speaker 1>and then we'll talk about the other two experiments in

0:22:52.440 --> 0:22:56.160
<v Speaker 1>the next section. So typically we would pair a seismometer

0:22:56.400 --> 0:22:59.560
<v Speaker 1>up with some sort of recording device, which would mean

0:22:59.600 --> 0:23:01.919
<v Speaker 1>that we would have a seismograph. That's when you have

0:23:02.000 --> 0:23:05.080
<v Speaker 1>the two components together. So a simple version of this

0:23:05.240 --> 0:23:08.320
<v Speaker 1>one that you might see here on Earth uh, an

0:23:08.320 --> 0:23:13.720
<v Speaker 1>old school simple mechanical version of a seismometer would be

0:23:14.240 --> 0:23:17.480
<v Speaker 1>a frame that has good contact with the ground. So

0:23:17.720 --> 0:23:22.080
<v Speaker 1>you've got a frame that is set on whatever surface

0:23:22.119 --> 0:23:25.920
<v Speaker 1>you're measuring. Suspended from the top of that frame would

0:23:25.960 --> 0:23:29.200
<v Speaker 1>be a weight on a spring, and the weight would

0:23:29.200 --> 0:23:32.000
<v Speaker 1>hold some sort of writing utensil, like a pen. That

0:23:32.080 --> 0:23:35.080
<v Speaker 1>pen the end of it would rest against a strip

0:23:35.119 --> 0:23:39.200
<v Speaker 1>of paper that could be rolled or pulled in such

0:23:39.240 --> 0:23:41.520
<v Speaker 1>a way that the pen is drawing a line on

0:23:41.560 --> 0:23:44.639
<v Speaker 1>that strip strip of paper as the paper moves past it.

0:23:45.160 --> 0:23:47.680
<v Speaker 1>If there's a trimmer, the frame is going to move

0:23:47.840 --> 0:23:52.800
<v Speaker 1>along with the ground, but the suspended weight will tend

0:23:53.160 --> 0:23:57.080
<v Speaker 1>to remain motionless as it is largely isolated from the

0:23:57.119 --> 0:24:00.440
<v Speaker 1>ground and the frame and an object at rest tends

0:24:00.520 --> 0:24:03.000
<v Speaker 1>to stay at rest. So you can think of it

0:24:03.080 --> 0:24:05.280
<v Speaker 1>as the frame and the earth and everything else is

0:24:05.320 --> 0:24:07.159
<v Speaker 1>moving up and down. The weight is kind of just

0:24:07.440 --> 0:24:12.080
<v Speaker 1>staying where it was, and that means that the paper

0:24:12.119 --> 0:24:14.240
<v Speaker 1>is going to be moving up and down against the pen.

0:24:14.560 --> 0:24:16.800
<v Speaker 1>Not the pen against the paper. The paper itself is

0:24:16.800 --> 0:24:18.679
<v Speaker 1>moving up and down because the ground is moving up

0:24:18.680 --> 0:24:21.200
<v Speaker 1>and down. And that means that the pen is gonna

0:24:21.200 --> 0:24:24.200
<v Speaker 1>start drawing squiggles on this paper. And so you could

0:24:24.240 --> 0:24:26.919
<v Speaker 1>look over the paper and wherever you saw squiggles, you'd say,

0:24:26.960 --> 0:24:29.000
<v Speaker 1>all right, well that was where there was an earthquake

0:24:29.119 --> 0:24:32.440
<v Speaker 1>or an aftershock, or maybe a large truck drove by

0:24:32.560 --> 0:24:35.879
<v Speaker 1>or whatever. The seismometer on the insite works on a

0:24:35.920 --> 0:24:39.080
<v Speaker 1>similar principle, except instead of holding a pen, instead of

0:24:39.080 --> 0:24:42.720
<v Speaker 1>it being mechanical, the relative motion between the weight and

0:24:42.760 --> 0:24:46.240
<v Speaker 1>the frame would create an electrical voltage, and changes in

0:24:46.320 --> 0:24:49.199
<v Speaker 1>that voltage are recorded by a computer system on the

0:24:49.240 --> 0:24:52.800
<v Speaker 1>insite and transmitted back to Earth, and those are interpreted

0:24:53.119 --> 0:24:55.840
<v Speaker 1>as the various quakes. I have a lot more to

0:24:55.840 --> 0:24:58.840
<v Speaker 1>say about the experiments aboard the Insight, but first let's

0:24:58.880 --> 0:25:09.280
<v Speaker 1>take another quick break to thank our sponsor. So the

0:25:09.359 --> 0:25:13.399
<v Speaker 1>second vital sign Insight is going to monitor is temperature.

0:25:13.880 --> 0:25:15.919
<v Speaker 1>The deck of the lander has a temperature censor of

0:25:15.960 --> 0:25:19.000
<v Speaker 1>its own to give surface readings. But what I think

0:25:19.080 --> 0:25:23.600
<v Speaker 1>is super interesting is what is called the HP three instrument.

0:25:24.240 --> 0:25:28.160
<v Speaker 1>HP three stands for heat flow and Physical Properties probe.

0:25:28.680 --> 0:25:32.280
<v Speaker 1>It's another tethered instrument that connects back to the lander,

0:25:32.720 --> 0:25:35.960
<v Speaker 1>and like the seismometer, the robotic arm has to lift

0:25:36.080 --> 0:25:39.199
<v Speaker 1>up the HP three and then place it on the

0:25:39.200 --> 0:25:42.359
<v Speaker 1>surface of Mars in the work space in front of

0:25:42.359 --> 0:25:47.520
<v Speaker 1>the lander. Inside this instrument is a probe. It looks

0:25:47.520 --> 0:25:50.520
<v Speaker 1>like almost like a spike, and it's called the mole

0:25:51.320 --> 0:25:54.320
<v Speaker 1>and it's tied. It's a type of pine traumater. I

0:25:54.359 --> 0:25:56.880
<v Speaker 1>didn't even know that was a word until I did

0:25:56.920 --> 0:25:59.840
<v Speaker 1>this research, but that essentially is a tool designed to

0:25:59.840 --> 0:26:02.760
<v Speaker 1>pay to trate a surface. That's the name pentatrometer. In

0:26:02.760 --> 0:26:06.240
<v Speaker 1>this case, we're talking about the Martian soil. So inside

0:26:06.240 --> 0:26:09.600
<v Speaker 1>this spike, which again is is got a cable out

0:26:09.680 --> 0:26:12.240
<v Speaker 1>the back of it that goes back up into the instrument.

0:26:12.760 --> 0:26:15.639
<v Speaker 1>The cable is held in a way where it can

0:26:15.720 --> 0:26:19.600
<v Speaker 1>be fed out gradually, so that as the spike is

0:26:19.640 --> 0:26:22.879
<v Speaker 1>digging down it can continue to have enough slack to

0:26:22.960 --> 0:26:27.360
<v Speaker 1>do this. But inside the spike, inside the penta traumeter

0:26:27.960 --> 0:26:31.520
<v Speaker 1>is a weight on a spring. Essentially, that's a hammer.

0:26:31.880 --> 0:26:34.920
<v Speaker 1>It's inside the spike. So imagine you've got a nail

0:26:35.359 --> 0:26:38.040
<v Speaker 1>or a railroad spike or something like that. But the

0:26:38.119 --> 0:26:42.760
<v Speaker 1>hammer for this nail or spike is actually inside the

0:26:42.840 --> 0:26:46.760
<v Speaker 1>spike or the nail itself, so it's a self hammering nail.

0:26:47.119 --> 0:26:50.240
<v Speaker 1>The mechanism draws power from the lander to pull back

0:26:50.280 --> 0:26:54.800
<v Speaker 1>the weight that compresses a spring, and then you latch

0:26:54.840 --> 0:26:58.680
<v Speaker 1>it into place. When it's completely compressed, you can unleash

0:26:58.720 --> 0:27:04.119
<v Speaker 1>this weight. The spring will expand rapidly, pushing the weight

0:27:04.160 --> 0:27:07.800
<v Speaker 1>down so that it collides with a little section at

0:27:07.840 --> 0:27:11.040
<v Speaker 1>the very tip of this probe, and it's like a

0:27:11.240 --> 0:27:15.320
<v Speaker 1>hammer knocking a nail, and it starts to hammer the

0:27:15.359 --> 0:27:18.280
<v Speaker 1>spike down. This is actually a pretty slow process. It

0:27:18.320 --> 0:27:23.000
<v Speaker 1>does not happen super fast. It's not like one, uh

0:27:23.200 --> 0:27:26.320
<v Speaker 1>one bash and suddenly the spike is several feet in

0:27:26.359 --> 0:27:28.720
<v Speaker 1>the soil. That's not the way it works. It's very gradual.

0:27:29.280 --> 0:27:33.959
<v Speaker 1>So by keeping a careful tension on the cable so

0:27:34.000 --> 0:27:37.080
<v Speaker 1>that the spike is properly positioned, and by doing this

0:27:37.160 --> 0:27:39.880
<v Speaker 1>several times, you start to drive the spike down into

0:27:39.920 --> 0:27:43.960
<v Speaker 1>the soil. It's gonna take months, but ultimately this mole

0:27:44.400 --> 0:27:47.560
<v Speaker 1>is going to dig down to a depth of about

0:27:47.600 --> 0:27:51.200
<v Speaker 1>five meters or sixteen feet, which is deeper than anyone

0:27:51.359 --> 0:27:53.920
<v Speaker 1>has dug on Mars up to this point as far

0:27:53.920 --> 0:27:57.280
<v Speaker 1>as we know anyway. But obviously this instrument is doing

0:27:57.320 --> 0:27:59.960
<v Speaker 1>more than just digging a hole on Mars. I mean,

0:28:00.000 --> 0:28:02.040
<v Speaker 1>that's super cool the way they're doing it, but that's

0:28:02.080 --> 0:28:04.760
<v Speaker 1>not the only thing it's doing. The probe and the

0:28:04.880 --> 0:28:10.080
<v Speaker 1>tether that's trailing behind it contains temperature sensors, and those

0:28:10.080 --> 0:28:13.960
<v Speaker 1>sensors will monitor the heat flowing from the interior of Mars,

0:28:14.320 --> 0:28:17.840
<v Speaker 1>which will help tell scientists what the inside of Mars

0:28:17.960 --> 0:28:21.520
<v Speaker 1>is like. It could inform scientists about how active Mars

0:28:21.720 --> 0:28:24.400
<v Speaker 1>is and whether it's made out of similar stuff as Earth.

0:28:24.760 --> 0:28:28.520
<v Speaker 1>The probe isn't just listening either. As the probe digs

0:28:28.560 --> 0:28:32.680
<v Speaker 1>down at certain stages, it will occasionally stop and it

0:28:32.720 --> 0:28:35.399
<v Speaker 1>will put out a pulse of heat of its own.

0:28:36.080 --> 0:28:39.440
<v Speaker 1>Then it will monitor how that heat flows through the

0:28:39.520 --> 0:28:43.160
<v Speaker 1>material around the probe. So if that material happens to

0:28:43.200 --> 0:28:46.720
<v Speaker 1>be a good conductor like metal, like coppers. A great

0:28:46.720 --> 0:28:50.360
<v Speaker 1>conductor of heat, the heat will decay very quickly, it'll

0:28:50.400 --> 0:28:54.280
<v Speaker 1>move outwards through this conductive material. But if it's a

0:28:54.320 --> 0:28:58.240
<v Speaker 1>poor conductor, more like glass, the heat's going to stick

0:28:58.280 --> 0:29:01.920
<v Speaker 1>around a lot longer. The HP three probe weighs in

0:29:02.040 --> 0:29:05.000
<v Speaker 1>at about six point five pounds at least it would

0:29:05.080 --> 0:29:07.440
<v Speaker 1>here on Earth. That means it has a mass of

0:29:07.520 --> 0:29:11.840
<v Speaker 1>about three kims and it only consumes to watts max

0:29:12.240 --> 0:29:15.400
<v Speaker 1>as the probe starts to dig down into the Martian soil.

0:29:16.000 --> 0:29:19.480
<v Speaker 1>The last of the three big experiments would be a

0:29:19.560 --> 0:29:23.480
<v Speaker 1>pair of RISE antennas on the deck of the lander.

0:29:23.560 --> 0:29:26.040
<v Speaker 1>These would not be removed from the deck and placed

0:29:26.040 --> 0:29:29.560
<v Speaker 1>on the Martian soil. They will stay on the lander.

0:29:30.040 --> 0:29:35.480
<v Speaker 1>RISE stands for Rotation and Interior Structure Experiment. These antennae

0:29:35.600 --> 0:29:40.760
<v Speaker 1>will track Mars's motions as it rotates, so essentially, it's

0:29:40.800 --> 0:29:44.520
<v Speaker 1>all about detecting that wobble. So how much does Mars

0:29:44.640 --> 0:29:48.480
<v Speaker 1>wobble around? Knowing how much it wobbles around will tell

0:29:48.520 --> 0:29:54.200
<v Speaker 1>scientists valuable information about Mars's core. How big is Mars's core,

0:29:54.400 --> 0:29:56.800
<v Speaker 1>Is it a solid core, is it a liquid core?

0:29:57.080 --> 0:30:00.160
<v Speaker 1>What elements besides iron might be in the core. Well,

0:30:00.160 --> 0:30:03.600
<v Speaker 1>the way Rise works is actually pretty darn simple. It

0:30:03.680 --> 0:30:06.760
<v Speaker 1>listens for an incoming signal from Earth, and then it

0:30:06.800 --> 0:30:10.000
<v Speaker 1>sends the signal back to Earth. This will reveal the

0:30:10.040 --> 0:30:14.120
<v Speaker 1>precise location of the lander, well precise location from a

0:30:14.160 --> 0:30:16.520
<v Speaker 1>few minutes in the past. Because again the signals can

0:30:16.520 --> 0:30:18.840
<v Speaker 1>only travel as fast as light, it may take a

0:30:18.880 --> 0:30:22.520
<v Speaker 1>few minutes for that to happen, depending upon where Earth

0:30:22.560 --> 0:30:25.680
<v Speaker 1>and Mars are in their respective orbits. But back on Earth,

0:30:26.080 --> 0:30:30.400
<v Speaker 1>computers will take this this return signal and analyze it

0:30:30.440 --> 0:30:35.200
<v Speaker 1>for changes and looking for evidence of Doppler shift. I've

0:30:35.200 --> 0:30:39.200
<v Speaker 1>talked about Doppler shift many times on this show, but

0:30:39.800 --> 0:30:44.720
<v Speaker 1>just so you remember, if you've got something moving in

0:30:45.080 --> 0:30:49.320
<v Speaker 1>a wave, whether it's a radio wave or a physical wave,

0:30:50.080 --> 0:30:54.080
<v Speaker 1>whatever it may be, h it has a certain frequency.

0:30:54.640 --> 0:30:58.040
<v Speaker 1>And if the wave is coming from a stationary object

0:30:58.480 --> 0:31:01.360
<v Speaker 1>and then it hits a different state stionary object, any

0:31:01.440 --> 0:31:05.040
<v Speaker 1>reflective waves. Reflective waves that come back to the source

0:31:05.240 --> 0:31:08.080
<v Speaker 1>are going to be unchanged except for their direction. Right

0:31:08.400 --> 0:31:12.200
<v Speaker 1>that you're gonna get back the same frequency of wave

0:31:12.400 --> 0:31:15.920
<v Speaker 1>if both objects are stationary, But if the objects are

0:31:15.960 --> 0:31:18.920
<v Speaker 1>moving closer to each other, the returning wave is going

0:31:18.960 --> 0:31:20.880
<v Speaker 1>to be compressed, so it's going to be at a

0:31:20.960 --> 0:31:24.040
<v Speaker 1>higher frequency. If the two objects are moving away from

0:31:24.040 --> 0:31:26.920
<v Speaker 1>each other, the wave is going to be elongated to

0:31:27.040 --> 0:31:31.040
<v Speaker 1>a lower frequency. And by measuring these changes, scientists will

0:31:31.080 --> 0:31:34.000
<v Speaker 1>be able to figure out how much Mars is wobbling

0:31:34.040 --> 0:31:38.600
<v Speaker 1>around as it orbits the Sun. Now, Earth wobbles every

0:31:38.680 --> 0:31:42.040
<v Speaker 1>eighteen years thanks to the Moon's pull on us, and

0:31:42.080 --> 0:31:46.760
<v Speaker 1>we already know that Mars does in fact wobble, In fact,

0:31:46.840 --> 0:31:49.320
<v Speaker 1>it wobbles over the course of a single Martian year,

0:31:49.680 --> 0:31:53.000
<v Speaker 1>but we don't know to what degree how much does

0:31:53.040 --> 0:31:55.320
<v Speaker 1>it wobble. We know it does, we just don't know

0:31:55.760 --> 0:32:00.160
<v Speaker 1>how uh intense that wobble is. So the Rye his

0:32:00.200 --> 0:32:03.280
<v Speaker 1>instruments will provide more information to fill in this knowledge gap.

0:32:03.680 --> 0:32:07.200
<v Speaker 1>And the amount of wobble planet has depends partly on

0:32:07.320 --> 0:32:12.040
<v Speaker 1>what is in the delicious neugute center of that planet. So,

0:32:12.080 --> 0:32:14.680
<v Speaker 1>as NASA points out in a really helpful web page,

0:32:14.920 --> 0:32:17.560
<v Speaker 1>a hard boiled egg is going to spend faster than

0:32:17.600 --> 0:32:21.920
<v Speaker 1>a raw egg. Also, planets that have liquid cores will

0:32:21.960 --> 0:32:25.200
<v Speaker 1>wobble more when they spend. Planets with a solid core

0:32:25.280 --> 0:32:28.239
<v Speaker 1>will wobble less, and this in turn can help us

0:32:28.280 --> 0:32:31.480
<v Speaker 1>make other hypotheses about why Mars has a very weak

0:32:31.600 --> 0:32:35.640
<v Speaker 1>magnetic field in comparison to Earth's magnetic field. So it's

0:32:35.680 --> 0:32:38.640
<v Speaker 1>all about learning more about why is Mars the way

0:32:38.840 --> 0:32:43.880
<v Speaker 1>it is and more about how Mars actually is. There

0:32:43.920 --> 0:32:46.560
<v Speaker 1>are other instruments on the lander that aren't getting quite

0:32:46.560 --> 0:32:49.720
<v Speaker 1>the same level of coverage. The lander has an atmospheric

0:32:49.760 --> 0:32:52.800
<v Speaker 1>pressure sensor, for example. It also has a uh F

0:32:53.040 --> 0:32:55.960
<v Speaker 1>antenna to allow the lander to communicate to satellites that

0:32:55.960 --> 0:32:59.800
<v Speaker 1>are in Martian orbit, which includes the Mars Reconnaissance Orbiter

0:33:00.160 --> 0:33:02.960
<v Speaker 1>and the Mars Odyssey Orbiter, both of which pass over

0:33:03.120 --> 0:33:06.640
<v Speaker 1>in Sight two times every Martian day. And there are

0:33:06.680 --> 0:33:08.600
<v Speaker 1>other satellites that can chat with as well, like the

0:33:08.640 --> 0:33:14.000
<v Speaker 1>European Space Agencies Trace Gas Orbiter or NASA's Mars Atmosphere

0:33:14.000 --> 0:33:18.040
<v Speaker 1>and Volatile Evolution Orbiter also known as MAVEN. It can

0:33:18.040 --> 0:33:20.080
<v Speaker 1>talk to those in a pinch if it needs to.

0:33:20.560 --> 0:33:23.720
<v Speaker 1>So Insight will stand on Mars doing its thing for

0:33:23.960 --> 0:33:27.440
<v Speaker 1>at least a Martian year plus some change, maybe longer

0:33:27.640 --> 0:33:31.320
<v Speaker 1>things continue to work out properly. Sometimes these missions can

0:33:31.360 --> 0:33:36.960
<v Speaker 1>go well beyond their initial projected phase, and if NASA

0:33:36.960 --> 0:33:39.640
<v Speaker 1>can figure out other things to do with the material

0:33:39.720 --> 0:33:43.440
<v Speaker 1>that's already there, then that is incredibly helpful. There's some

0:33:43.520 --> 0:33:46.120
<v Speaker 1>other elements on it as well. There's a reflective surface,

0:33:46.160 --> 0:33:48.320
<v Speaker 1>for example. They could be used to locate the precise

0:33:48.680 --> 0:33:51.200
<v Speaker 1>position of the lander. You just direct a laser at

0:33:51.240 --> 0:33:53.720
<v Speaker 1>it and look for the reflection. I'm sure we'll learn

0:33:53.920 --> 0:33:58.000
<v Speaker 1>tons of interesting things about Mars using this device, and

0:33:58.080 --> 0:34:02.080
<v Speaker 1>probably a lot about Earth as well, which pretty exciting stuff. Now,

0:34:02.080 --> 0:34:04.520
<v Speaker 1>in our next episode, I'm gonna stick with Mars for

0:34:04.520 --> 0:34:06.760
<v Speaker 1>a little bit. I'm gonna talk about the various proposals

0:34:06.800 --> 0:34:09.840
<v Speaker 1>to send people to Mars and what that would entail,

0:34:10.040 --> 0:34:11.759
<v Speaker 1>and we'll talk about why it would be super hard

0:34:11.840 --> 0:34:14.840
<v Speaker 1>to do and why some people like Bill and the

0:34:14.880 --> 0:34:18.000
<v Speaker 1>Science Guy are skeptical that we're ever going to actually

0:34:18.280 --> 0:34:23.000
<v Speaker 1>go there for a prolonged stay. And maybe we'll also

0:34:23.280 --> 0:34:25.879
<v Speaker 1>talk about why Elon Musk thinks there's a decent chance

0:34:25.920 --> 0:34:28.600
<v Speaker 1>he's gonna end up there. So tune in tomorrow to

0:34:28.640 --> 0:34:31.360
<v Speaker 1>hear that episode. If you guys have any suggestions for

0:34:31.520 --> 0:34:35.160
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0:34:38.520 --> 0:34:41.000
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0:34:41.000 --> 0:34:43.439
<v Speaker 1>want to know more, or a person in tech let

0:34:43.440 --> 0:34:45.920
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0:34:46.040 --> 0:34:48.880
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0:34:48.920 --> 0:34:52.399
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0:34:52.480 --> 0:34:55.040
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0:34:55.080 --> 0:34:57.680
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0:34:57.680 --> 0:35:01.160
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0:35:01.200 --> 0:35:03.160
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0:35:05.800 --> 0:35:07.600
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0:35:07.640 --> 0:35:10.839
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0:35:10.960 --> 0:35:19.480
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0:35:19.520 --> 0:35:22.000
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