WEBVTT - Could Jupiter turn into a star?

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<v Speaker 1>Hey, Daniel, do you ever think about what the night

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<v Speaker 1>sky looked like to our ancestors? I do. I wonder

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<v Speaker 1>how it looked at them. And I also like thinking

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<v Speaker 1>even further back in the past, like what did the

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<v Speaker 1>dinosaurs see in the sky? Yeah, they probably should have

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<v Speaker 1>looked at this guy more carefully, you know, looking for

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<v Speaker 1>meteors for example. I know dinosaur astronomers totally fell down

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<v Speaker 1>on the job, but you can even think further back,

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<v Speaker 1>like the first eyeballs on Earth five million years ago,

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<v Speaker 1>you mean, like microbe astronomers, or you know, I think

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<v Speaker 1>to the future. I wonder what the night sky will

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<v Speaker 1>look like to humans billions of years from It could

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<v Speaker 1>be totally different. I mean, if there even our humans

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<v Speaker 1>then yeah. Well I'm thinking about the future cockroach astronomers

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<v Speaker 1>and hoping they will keep an eye on the stars

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<v Speaker 1>for us. Whatever they see doesn't bug them. I am

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<v Speaker 1>more hamming cartoonists and the creator of PhD comics. I'm Daniel.

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<v Speaker 1>I'm a particle physicist. And that was the first time

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<v Speaker 1>I ever said cockroach on the podcast and astronomers in

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<v Speaker 1>the same sentence Publicly. I love astronomers, I love astronomy.

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<v Speaker 1>I'm nothing but pro astronomers. I did like the idea

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<v Speaker 1>of dinosaur astronomers. That's pretty cool. My favorite story about

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<v Speaker 1>dinosaur astronomers is that they really did have a chance

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<v Speaker 1>to save themselves. Your favorite I feel like you thought

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<v Speaker 1>about this before. Well, yeah, absolutely. You know that the

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<v Speaker 1>meteor that came and wiped out the dinosaurs made a

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<v Speaker 1>near past by the Earth ten years earlier, Yeah, and

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<v Speaker 1>came close enough that they should have been able to

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<v Speaker 1>look up and see it in the sky. So if

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<v Speaker 1>they had funded their version of NASA, they could have

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<v Speaker 1>saved their own lives ten years. Do you think dinosaurs

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<v Speaker 1>could have built spaceships? And necessity is the mother of invention, right,

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<v Speaker 1>do you think they should have called the dinosaur Bruce

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<v Speaker 1>Willis put them on a spaceship and getting to deflect

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<v Speaker 1>that asteroid in ten years? Well, you know the other

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<v Speaker 1>option is what happened, So anything is better than that.

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<v Speaker 1>But anyways, welcome to our podcast. Daniel and Jorge talk

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<v Speaker 1>about dinosaur astronomers. That's all we do. Daniel and Jorge

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<v Speaker 1>digress in the very first moments of the podcast. That's

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<v Speaker 1>right now. Welcome to our podcast. Daniel and Jorge explained

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<v Speaker 1>the universe a production of I Heart Radio in which

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<v Speaker 1>we talk about all the amazing and beautiful and crazy

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<v Speaker 1>things about the universe, the violent events, the incredible drama

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<v Speaker 1>happening in the inside of stars, the tiny little particles

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<v Speaker 1>that apparently make up everything you see and touch and taste. Yeah,

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<v Speaker 1>all of the spacey stuff out there, happening in the

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<v Speaker 1>universe and even in our own backyards, or I guess

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<v Speaker 1>our solar system backyard. That's right, because when you look

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<v Speaker 1>out into the night sky, you are not seeing a

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<v Speaker 1>still picture. You are not seeing a flat image. You

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<v Speaker 1>are seeing a drama unfolding on cosmic distance sales and

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<v Speaker 1>time scales. If you were to look at the night

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<v Speaker 1>sky sped up a little bit, you would see incredible events,

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<v Speaker 1>huge explosions, massive collisions. It would put Hollywood to shame.

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<v Speaker 1>It's like a cosmological telenovella, a lot of twists and turns.

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<v Speaker 1>I don't know if anybody's really like backstabbing anybody, or

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<v Speaker 1>does the Earth have an evil twin on the other

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<v Speaker 1>side of the Sun Planet X Extreme close up. I

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<v Speaker 1>don't know if there's so much political intrigue, but there

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<v Speaker 1>is definitely drama. There are things that happened rapidly, all

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<v Speaker 1>of a sudden. There are sudden changes of fate. There

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<v Speaker 1>are things that are happening, and so I think it's

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<v Speaker 1>fun to think about how our solar system will evolve. Yeah,

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<v Speaker 1>because as we as humans found out about a hundred

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<v Speaker 1>years ago, the universe is not static. Things are changing.

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<v Speaker 1>The stars are moving, the galaxies are blazing across the universe,

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<v Speaker 1>and new stars are being born all the time. That's right.

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<v Speaker 1>And stars can change right there, formed from the collapse

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<v Speaker 1>of gases into a hot dense object that confuse eventually

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<v Speaker 1>to and into something else like a black hole or

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<v Speaker 1>a white dwarf. They go through this evolution, and so

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<v Speaker 1>it's natural to also wonder, like what about planets? Do

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<v Speaker 1>planets have future stages in their evolution? Are they like Pokemon?

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<v Speaker 1>They can evolve into different versions. They say that Earth

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<v Speaker 1>is only stage one. I don't know enough about Pokemon

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<v Speaker 1>to even really make that joke. I just watched my

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<v Speaker 1>kids play, so I can say energy cards and pokemons evolved.

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<v Speaker 1>Then we're at the end of my knowledge. I think

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<v Speaker 1>our planet is Earth type. Is it an e X

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<v Speaker 1>or a g X? Does it have the shiny glint

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<v Speaker 1>on it? It used to. I think that's right. And

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<v Speaker 1>we did a podcast recently in which we talked about

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<v Speaker 1>Jupiter and how close Jupiter was to having become a star,

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<v Speaker 1>and a bunch of listeners wrote in asking us about that.

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<v Speaker 1>Jim Sanchez, Doug Dodds, and Ryan Kyrkiss all wrote and

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<v Speaker 1>asked us like, well, is Jupiter on the verge of

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<v Speaker 1>becoming a star? Could it one day eventually become a star?

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<v Speaker 1>Because I guess it's kind of a fine line between

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<v Speaker 1>the being a giant cloud of dust and being a

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<v Speaker 1>giant gas planet and maybe being a giant ball of

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<v Speaker 1>flaming gas like the Sun. It's kind of a fine line.

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<v Speaker 1>It turns out. How final line is it either on

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<v Speaker 1>fire or you're not? That seems pretty clear cut to me. Well,

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<v Speaker 1>I mean what does it take, like a match or

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<v Speaker 1>you know, a spark. I guess that's the question we'll

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<v Speaker 1>be talking about today. That's right. So to the other program,

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<v Speaker 1>we'll be asking the question could Jupiter become a star?

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<v Speaker 1>Is it too late for Jupiter or can it still

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<v Speaker 1>you know, find the right role and suddenly be the

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<v Speaker 1>new darling of Hollywood. Hey, you know, jump on the

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<v Speaker 1>TikTok and anybody can become a star. Oh hey, that's

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<v Speaker 1>what Jupiter needs. That's right. But there was some actual

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<v Speaker 1>serious talk about this. A couple of decades ago. NASA

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<v Speaker 1>sent a probe out to study Jupiter, and they didn't

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<v Speaker 1>want the probe to infect any of Jupiter's moons where

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<v Speaker 1>we think there might potentially be life, right, my crobial life.

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<v Speaker 1>And we didn't want to cray Galileo this probe onto

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<v Speaker 1>any of Jupiter's moons because we didn't want to bring

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<v Speaker 1>any earth microbes. Right, once you bring Earth's microbes, you

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<v Speaker 1>can no longer ask like are their native microbes? And

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<v Speaker 1>so instead they crashed the probe into Jupiter itself because

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<v Speaker 1>we don't care about infect the Jupiter. I think the

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<v Speaker 1>idea was that it would burn up and get crushed

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<v Speaker 1>because Jupiter has this incredible atmosphere, so we get immolated

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<v Speaker 1>in descent, whereas the moons don't have those atmospheres, and

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<v Speaker 1>so it would actually land on the surface and potentially survive.

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<v Speaker 1>But there was some concern about that. Yeah, people were wondering, like,

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<v Speaker 1>if Jupiter is on the verge of becoming a star,

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<v Speaker 1>if it's this huge ball of gas and you drop

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<v Speaker 1>a match into it essentially, is there impossibility that it

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<v Speaker 1>could have ignited the atmosphere or Jupiter and birth a

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<v Speaker 1>new star, because I mean Jupiter. If you think about it,

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<v Speaker 1>it's a giant ball of hydrogen, right, kind of like

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<v Speaker 1>the Hindenberg. Kind of like the Hindenburg, but much bigger.

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<v Speaker 1>That's what I mean. It's like the big balloon made

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<v Speaker 1>out of hydrogen and all you need is a little

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<v Speaker 1>flame and some oxygen. All of a sudden, it sounds

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<v Speaker 1>very unstable, does it sounds like a nine twenties idea? Yeah?

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<v Speaker 1>And you know this actually appears in science fiction as well,

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<v Speaker 1>in the well known series two thousand and one, two

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<v Speaker 1>thousand ten, etcetera. They turn Jupiter into a star on purpose. Yeah,

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<v Speaker 1>on purpose, I guess. You know. The aliens. We didn't

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<v Speaker 1>really ever understand their psychology, but they turn it into

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<v Speaker 1>a new star. They call it Lucifer. The Aliens call

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<v Speaker 1>it Lucifer. I don't remember the details that book. Who

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<v Speaker 1>calls it Lucifer, Whether it's the aliens naming it or

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<v Speaker 1>you know, earthbound cartoonists who are elected to a naming

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<v Speaker 1>committee who gave it that name. But I do remember

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<v Speaker 1>the sequel to two thousand and one two thousand and ten.

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<v Speaker 1>I think that that the end, Jupiter does become a star.

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<v Speaker 1>Sorry spoiler um, because the star at the end of

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<v Speaker 1>that movie. And I was wondered, like, oh, that's pretty interesting,

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<v Speaker 1>but what does that mean? Is that going to change

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<v Speaker 1>our solar system or what's the big deal? Yeah? Exactly,

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<v Speaker 1>So it's an interesting question. It's right here in our backyard.

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<v Speaker 1>It seems relevant. So we thought we would try to

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<v Speaker 1>figure out how close is Jupiter to becoming a star?

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<v Speaker 1>If you wanted to turn it into a star, what

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<v Speaker 1>would you have to do? So, as usual, Daniel went

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<v Speaker 1>out there into the wilds of the Internet and ask

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<v Speaker 1>people to submit their answer to the question could Jupiter

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<v Speaker 1>become a star? That's right, So thank you to everybody

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<v Speaker 1>who participated, And if you'd like to participate in future

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<v Speaker 1>rounds of person on the Internet interviews, please send us

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<v Speaker 1>a note to questions at Daniel and Jorge dot com.

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<v Speaker 1>We'd love for you to answer our questions. And before

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<v Speaker 1>you listen to these answers, think about it for a second.

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<v Speaker 1>Do you think Jupiter could become a star. Here's what

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<v Speaker 1>people had to say. I think anyone who claims to

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<v Speaker 1>know where the Jupiter can turn into a star. Absolutely

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<v Speaker 1>is probably exaggerating their knowledge in order to make up

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<v Speaker 1>one last say. I think Jupiter is like a filed

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<v Speaker 1>star because it's not massive enough to have the fusion

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<v Speaker 1>reactions at the cool The only way I can think

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<v Speaker 1>of that it could become a star would be if

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<v Speaker 1>it pulled in enough matter. Well it didn't for our reason,

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<v Speaker 1>I suppose not enough mass um. I didn't hear that

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<v Speaker 1>almost became a star. Well, well maybe it's if a

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<v Speaker 1>lot of planets I think the universe is are unlikely

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<v Speaker 1>to happen, But it happened, So perhaps it's just as

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<v Speaker 1>unlikely that Tupiter would turn into a star. But I

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<v Speaker 1>suppose it could happen. Yeah, what kind of what kind

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<v Speaker 1>of start? Jupiter is a gas giant and it's made

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<v Speaker 1>of gas, and stars are also made of gas. So

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<v Speaker 1>I think maybe if a small star came into it.

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<v Speaker 1>I suppose if it became big enough and had enough gravity,

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<v Speaker 1>it could turn on and become a star. But I'm

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<v Speaker 1>not aware that it's so it's growing. My short answer

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<v Speaker 1>is I don't think so. Yes, I think that it's

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<v Speaker 1>eight times more massive that it would need to become

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<v Speaker 1>in order for Jupiter to start burning hydrogen and fusing

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<v Speaker 1>it into helium. But even if you were to combine

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<v Speaker 1>all the planets in the Solar System, you wouldn't get

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<v Speaker 1>to the mass needed. So by natural means, no, it's

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<v Speaker 1>not possible. But theoretically could Jupiter become a star? Then yes,

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<v Speaker 1>you just need to add eight more jupiters to it.

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<v Speaker 1>If Jupiter's ape does extremely well, I think Jupiter might

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<v Speaker 1>be able to become a starmp if anyone could be

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<v Speaker 1>a start with. Oh my gosh. I believe that the

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<v Speaker 1>gas giants have cleaned up our Solar system enough that

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<v Speaker 1>it is unlikely that Jupiter would be able to get

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<v Speaker 1>enough mass to turn into a star. Well, theoretically possible

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<v Speaker 1>in time. I think the way that it might happen

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<v Speaker 1>is maybe if there are a rogue planet that collided

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<v Speaker 1>with Jupiter or sufficient other material like comets and asteroids

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<v Speaker 1>and so on, But that seems implosible. Alright. Some great

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<v Speaker 1>answers I like the one that said yes, I mean no, wait,

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<v Speaker 1>what's the star? If you're not going to be accurate,

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<v Speaker 1>you should at least be well. I guess that perfectly

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<v Speaker 1>reflects how I feel. I'm like, yes, no, wait, let's

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<v Speaker 1>define a star. Yeah. I think it is an interesting

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<v Speaker 1>question because you know, different stuff out there have evolutions,

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<v Speaker 1>you know, we see stuff changing in the universe, and

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<v Speaker 1>we haven't ever talked about the question of like, is

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<v Speaker 1>a planet stable? Could a planet just hang out forever

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<v Speaker 1>or does it have the next natural stage in its evolution? Yeah?

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<v Speaker 1>Is this possible that we suddenly have two stars in

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<v Speaker 1>our sky? You know, kind of like star wars? Yeah?

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<v Speaker 1>What would that mean for when you have to go

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<v Speaker 1>to work and abaly make our days longer? Yeah, it

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<v Speaker 1>would make our days longer and much more irregular. Right,

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<v Speaker 1>you wouldn't have regular patterns. You have times when both

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<v Speaker 1>stars were in the sky and times when only one

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<v Speaker 1>of them was in the sky. Have you ever read

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<v Speaker 1>the three body problem? You know, the calendar on that

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<v Speaker 1>planet is very complicated. All right, let's jump into it, Daniel.

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<v Speaker 1>What makes something a star versus a planet? I guess

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<v Speaker 1>let's start with that question. What happens at that fourth

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<v Speaker 1>in the road for a big ball of gas where

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<v Speaker 1>it turns into a jupiter, or it turns into a star,

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<v Speaker 1>and or can it kind of switch over? Yeah? So

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<v Speaker 1>really it's all about mass, Like if you are a

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<v Speaker 1>big enough blob of stuff, then gravity will pull you

0:12:37.200 --> 0:12:40.000
<v Speaker 1>in and compress you hard enough that you will start

0:12:40.040 --> 0:12:45.160
<v Speaker 1>to fuse. You'll create the conditions necessary to squish these

0:12:45.160 --> 0:12:48.559
<v Speaker 1>particles together so they fuse, which releases a huge amount

0:12:48.559 --> 0:12:51.280
<v Speaker 1>of energy. And that's really the distinction between a planet

0:12:51.320 --> 0:12:54.199
<v Speaker 1>and a star. A star is using, it's releasing energy,

0:12:54.240 --> 0:12:57.360
<v Speaker 1>it's burning itself, and a planet is much more inert

0:12:57.559 --> 0:12:59.760
<v Speaker 1>than no fusion happening at the center of the Earth

0:13:00.080 --> 0:13:01.960
<v Speaker 1>or at the center of Jupiter, for example, And that's

0:13:01.960 --> 0:13:04.120
<v Speaker 1>just because we don't have enough stuff, Like if we

0:13:04.200 --> 0:13:06.880
<v Speaker 1>had more stuff, it would be heavier, and things get

0:13:06.920 --> 0:13:09.680
<v Speaker 1>more compressing you sort of get to that pressure where

0:13:09.760 --> 0:13:12.160
<v Speaker 1>fusion happens. That's right. It's all about the stuff, and

0:13:12.200 --> 0:13:14.320
<v Speaker 1>it depends on which kind of stuff. Like if you're

0:13:14.440 --> 0:13:18.360
<v Speaker 1>just hydrogen, just gas, then you need less stuff. Then

0:13:18.440 --> 0:13:21.160
<v Speaker 1>if you're like a huge ball of oxygen or carbon,

0:13:21.280 --> 0:13:24.560
<v Speaker 1>because the heavier elements take higher pressure or higher temperature

0:13:24.559 --> 0:13:27.959
<v Speaker 1>conditions in order to fuse, So hydrogen is the easiest.

0:13:28.160 --> 0:13:30.160
<v Speaker 1>So if you're gonna go all hydrogen, you need a

0:13:30.160 --> 0:13:32.560
<v Speaker 1>big ball of gas. If you're gonna go all carbon

0:13:32.679 --> 0:13:35.559
<v Speaker 1>or all oxygen or something heavier, you need a bigger bone.

0:13:35.840 --> 0:13:38.320
<v Speaker 1>But in principle, if you took the Earth and made

0:13:38.320 --> 0:13:41.600
<v Speaker 1>it much more massive, same stuff, same mixture of stuff,

0:13:41.800 --> 0:13:45.040
<v Speaker 1>it would turn into a star. Wow, how much more stuff?

0:13:45.080 --> 0:13:46.680
<v Speaker 1>I guess? I guess The question is what does it

0:13:46.720 --> 0:13:48.960
<v Speaker 1>take to be a star? How much stuff do you need?

0:13:49.040 --> 0:13:50.640
<v Speaker 1>And we can think about it in terms of like

0:13:50.800 --> 0:13:54.600
<v Speaker 1>pounds or kilograms or squirrels, but those units are hard

0:13:54.600 --> 0:13:57.319
<v Speaker 1>to grasp because the numbers are so big. Let's just

0:13:57.360 --> 0:13:59.200
<v Speaker 1>talk about in terms of stuff. So let's talk about

0:13:59.320 --> 0:14:02.760
<v Speaker 1>in terms of units of like one sun. So the

0:14:02.840 --> 0:14:05.680
<v Speaker 1>minimum amount of stuff you need to reach any sort

0:14:05.679 --> 0:14:08.960
<v Speaker 1>of fusion is about one one of the mass of

0:14:09.000 --> 0:14:11.600
<v Speaker 1>the sun of our son, of our son. Yeah, we're

0:14:11.679 --> 0:14:14.400
<v Speaker 1>using our suns as a unit. You could have something

0:14:14.559 --> 0:14:17.120
<v Speaker 1>one one of our sun and it could be a star.

0:14:17.280 --> 0:14:20.480
<v Speaker 1>That's right, And that's only like really special. That's the

0:14:20.520 --> 0:14:24.240
<v Speaker 1>absolute minimum. It gets you above the shelf for the lowest, weakest,

0:14:24.400 --> 0:14:27.000
<v Speaker 1>lamest kind of fusion. And if you reach that threshold,

0:14:27.000 --> 0:14:30.760
<v Speaker 1>you're called a brown dwarf. And it's a special kind

0:14:30.800 --> 0:14:34.640
<v Speaker 1>of fusion. It's not just hydrogen fusion. It's deuterium fusion

0:14:35.080 --> 0:14:38.240
<v Speaker 1>and deuterium, if you remember, is an isotope of hydrogen,

0:14:38.400 --> 0:14:40.880
<v Speaker 1>and the nucleus you have a proton and a neutron,

0:14:41.000 --> 0:14:44.480
<v Speaker 1>not just a proton, and that neutron is crucial because

0:14:44.680 --> 0:14:47.440
<v Speaker 1>it helps sort of bring those protons together and stick

0:14:47.480 --> 0:14:50.440
<v Speaker 1>them together. I see, um, that sounds small, like one

0:14:50.520 --> 0:14:52.880
<v Speaker 1>hundreds the size of the Sun. But that's it like

0:14:52.920 --> 0:14:56.400
<v Speaker 1>what like ten earth? That's yes, something like ten thou earths.

0:14:56.400 --> 0:14:59.280
<v Speaker 1>It's a lot bigger than the Earth, and so it's

0:14:59.320 --> 0:15:01.120
<v Speaker 1>not that small, all right. I mean, it's small compared

0:15:01.160 --> 0:15:03.800
<v Speaker 1>to our Sun, but it's a big object. And they're

0:15:03.800 --> 0:15:07.640
<v Speaker 1>called brown dwarfs, but they're pretty badly named because they're

0:15:07.680 --> 0:15:10.960
<v Speaker 1>not actually brown. They're not actually dwarves if they're ten

0:15:11.000 --> 0:15:15.320
<v Speaker 1>thousand earths. Also, so two strikes there for the physics

0:15:15.360 --> 0:15:18.760
<v Speaker 1>community in one name their dwarfs compared to the other stars.

0:15:19.120 --> 0:15:21.760
<v Speaker 1>But they don't look at all brown. They look magenta

0:15:22.000 --> 0:15:24.600
<v Speaker 1>or like orange red. And that's just because the kind

0:15:24.600 --> 0:15:26.400
<v Speaker 1>of fusion that happens in the kind of light that

0:15:26.440 --> 0:15:28.440
<v Speaker 1>they admit I see. But they're still sort of big

0:15:28.480 --> 0:15:31.920
<v Speaker 1>balls of fiery stuff. They just they don't glows brightly

0:15:32.040 --> 0:15:34.640
<v Speaker 1>and they're kind of tinged in a certain color, and

0:15:34.840 --> 0:15:37.360
<v Speaker 1>these things exist and they're not that rare in the universe.

0:15:37.560 --> 0:15:40.000
<v Speaker 1>Is one like six and a half light years away

0:15:40.000 --> 0:15:44.280
<v Speaker 1>from us. It's called Luman sixteen. And so they're not

0:15:44.280 --> 0:15:46.440
<v Speaker 1>that easy to see because they're not that bright. But

0:15:46.760 --> 0:15:49.200
<v Speaker 1>you know, theoretically we understand that they should exist and

0:15:49.200 --> 0:15:51.400
<v Speaker 1>we see them out there, and so this is totally

0:15:51.400 --> 0:15:54.480
<v Speaker 1>a possibility. It's the minimum threshold to become a star.

0:15:54.560 --> 0:15:57.560
<v Speaker 1>And then those are the smallest stars. So then what's

0:15:57.600 --> 0:15:59.680
<v Speaker 1>the next step up? Next step up is you know,

0:16:00.000 --> 0:16:02.400
<v Speaker 1>really you might call the first kind of real star,

0:16:02.480 --> 0:16:05.480
<v Speaker 1>and this is a red dwarf, a brown dwarf. People argue, like,

0:16:05.520 --> 0:16:08.160
<v Speaker 1>you know, is it a big, hot burning planet. Is

0:16:08.240 --> 0:16:10.520
<v Speaker 1>a star that's you know, it's kind of lame, but

0:16:10.560 --> 0:16:13.960
<v Speaker 1>a red dwarf nobody argues about, Like, it's definitely a star.

0:16:14.360 --> 0:16:18.280
<v Speaker 1>It burns hydrogen. Like essentially, this is the minimum star

0:16:18.360 --> 0:16:20.440
<v Speaker 1>you need if you just start from hydrogen. If you

0:16:20.440 --> 0:16:22.960
<v Speaker 1>have one tenth the mass of the Sun and a

0:16:23.080 --> 0:16:26.480
<v Speaker 1>huge ball of hydrogen gas, gravity will pull it together

0:16:26.520 --> 0:16:29.600
<v Speaker 1>and squeeze it hard enough for it to fuse fuse.

0:16:29.680 --> 0:16:32.360
<v Speaker 1>But in a brown star, there's no fusion. There is fusion,

0:16:32.400 --> 0:16:35.000
<v Speaker 1>but it's deterior and fusion. It's not hydrogen fusion. A

0:16:35.040 --> 0:16:38.240
<v Speaker 1>brown star is not hot enough to fuse hydrogen. You

0:16:38.320 --> 0:16:41.280
<v Speaker 1>need that extra neutron in the nucleus to make the

0:16:41.280 --> 0:16:43.880
<v Speaker 1>fusion happen, and so the fusion doesn't release as much

0:16:43.960 --> 0:16:47.120
<v Speaker 1>energy either. There's sort of like a cooler, weaker lam

0:16:47.200 --> 0:16:49.560
<v Speaker 1>or kind of fusion, but it's still fusion. It's just

0:16:49.640 --> 0:16:52.080
<v Speaker 1>kind of an easier fusion. It's easier and it's not

0:16:52.160 --> 0:16:54.800
<v Speaker 1>as dramatic. It doesn't produce as much energy. So that's

0:16:54.800 --> 0:16:57.520
<v Speaker 1>why the brown dwarfs aren't so luminous. All right. So

0:16:57.680 --> 0:16:59.720
<v Speaker 1>then when you get to one tenth of the mass

0:16:59.760 --> 0:17:02.040
<v Speaker 1>with the Sun, then you get the real cooking coin.

0:17:02.160 --> 0:17:04.480
<v Speaker 1>That's right, that's a legit star. It's a red dwarf,

0:17:05.040 --> 0:17:08.160
<v Speaker 1>and you know there's one that's only six years away.

0:17:08.400 --> 0:17:10.840
<v Speaker 1>It has a name that's all like letters and acronym,

0:17:10.920 --> 0:17:13.600
<v Speaker 1>so it's totally unpronounceable. But the cool thing about it

0:17:13.720 --> 0:17:16.879
<v Speaker 1>is that it's really dense, like it has one tenth

0:17:16.920 --> 0:17:19.320
<v Speaker 1>the mass of the Sun, but it's radius it's the

0:17:19.359 --> 0:17:23.920
<v Speaker 1>same as Saturn. Wow, So it's tiny, but it's it's compact.

0:17:24.040 --> 0:17:28.000
<v Speaker 1>It's a little dwarf. It's a little red dwarf. It's

0:17:28.000 --> 0:17:33.919
<v Speaker 1>perfectly named and is it red? So there you go

0:17:34.240 --> 0:17:37.640
<v Speaker 1>to check marks for the astronomy community terms. You're you're

0:17:37.680 --> 0:17:42.800
<v Speaker 1>up to zero then zero zero zero physicists, this is

0:17:42.920 --> 0:17:45.760
<v Speaker 1>zero public. But you know, something the size of a

0:17:45.800 --> 0:17:48.800
<v Speaker 1>planet can definitely be a star. That's not an issue.

0:17:48.800 --> 0:17:51.760
<v Speaker 1>It's not just about size, it's about mass. Remember, gravity

0:17:51.760 --> 0:17:54.440
<v Speaker 1>will gather this stuff together and make it really dense

0:17:54.520 --> 0:17:57.920
<v Speaker 1>for density. Yeah, all right, well it's clear that things

0:17:57.920 --> 0:18:00.560
<v Speaker 1>about the size of planets can become stars. And so

0:18:00.600 --> 0:18:03.600
<v Speaker 1>now let's talk about Jupiter and whether Jupiter could or

0:18:03.800 --> 0:18:06.720
<v Speaker 1>could have become a star. But first let's take a

0:18:06.800 --> 0:18:22.679
<v Speaker 1>quick break. All right, Daniel, we're talking about making a

0:18:22.720 --> 0:18:25.200
<v Speaker 1>star in our own backyard. So what do we need?

0:18:25.280 --> 0:18:29.119
<v Speaker 1>A grill, some matches, a lot of flower which is

0:18:29.119 --> 0:18:33.280
<v Speaker 1>on short supply. Oh no, better order a crate of it.

0:18:33.480 --> 0:18:36.200
<v Speaker 1>All right, So let's we're talking about whether Jupiter could

0:18:36.240 --> 0:18:38.959
<v Speaker 1>be one day become a star, which is a crazy idea.

0:18:39.400 --> 0:18:41.439
<v Speaker 1>But you're telling me that it's all about the stuff.

0:18:41.440 --> 0:18:44.439
<v Speaker 1>You have enough stuff and you're compressed enough, then almost

0:18:44.480 --> 0:18:46.959
<v Speaker 1>anything can become a star. Yeah, And so let's talk

0:18:46.960 --> 0:18:50.280
<v Speaker 1>about Jupiter. How how massive is Jupiter. Jupiter is about

0:18:50.600 --> 0:18:53.840
<v Speaker 1>one tenth of one of the mass of the Sun,

0:18:54.240 --> 0:18:57.840
<v Speaker 1>so one of the song Okay, so it's it's ten

0:18:57.920 --> 0:19:00.680
<v Speaker 1>times too small to be a brown Earth. Yeah, I

0:19:00.760 --> 0:19:03.159
<v Speaker 1>remember the threshold is one hundred of the Sun for

0:19:03.200 --> 0:19:05.760
<v Speaker 1>a brown dwarf, one tenth of the Sun for a

0:19:05.840 --> 0:19:09.879
<v Speaker 1>red dwarf. And so Jupiter it's ten times too small

0:19:09.960 --> 0:19:12.400
<v Speaker 1>to be a brown dwarf and a hundred times too

0:19:12.400 --> 0:19:14.560
<v Speaker 1>small to be a red dwarf. And it's made out

0:19:14.600 --> 0:19:17.720
<v Speaker 1>of roughly the right stuff. It's mostly hydrogen. It's just

0:19:17.880 --> 0:19:21.680
<v Speaker 1>not big enough icy and you need that stuff because

0:19:21.760 --> 0:19:23.720
<v Speaker 1>I mean, while you like, the Earth could become a

0:19:23.720 --> 0:19:26.600
<v Speaker 1>star if you compress it down enough, but there's nothing

0:19:26.640 --> 0:19:29.800
<v Speaker 1>really compressing the Earth that much except for its gravity,

0:19:29.920 --> 0:19:32.040
<v Speaker 1>and so without that stuff to create the gravity, you

0:19:32.080 --> 0:19:34.479
<v Speaker 1>can't turn into a star. Yeah, the Earth is like

0:19:34.880 --> 0:19:38.359
<v Speaker 1>one three hundred thousand's the size of the Sun, and

0:19:38.400 --> 0:19:41.680
<v Speaker 1>so we're nowhere near massive enough to ever become a star.

0:19:42.000 --> 0:19:44.840
<v Speaker 1>Jupiter is like it's in within shouting distance, you know,

0:19:45.000 --> 0:19:47.800
<v Speaker 1>like ten times too small to be a pathetic little

0:19:47.840 --> 0:19:50.680
<v Speaker 1>brown dwarf is like it's you know, ten times. It's

0:19:50.680 --> 0:19:53.120
<v Speaker 1>not a small thing to overcome, but it's still ten

0:19:53.160 --> 0:19:55.960
<v Speaker 1>times too small. Like that doesn't seem likely to happen

0:19:56.040 --> 0:19:59.239
<v Speaker 1>anytime soon. No, And Jupiter is already really big, right,

0:19:59.280 --> 0:20:01.760
<v Speaker 1>So it sends the In order for Jupiter become a star,

0:20:02.200 --> 0:20:04.680
<v Speaker 1>you have to multiply its mass by a factor of ten.

0:20:05.240 --> 0:20:10.199
<v Speaker 1>That means like gather nine more jubiters somewhere somehow and

0:20:10.359 --> 0:20:14.040
<v Speaker 1>added to junior. Al Right, well, it doesn't sound very

0:20:14.200 --> 0:20:16.440
<v Speaker 1>likely then that Jupiter is going to turn into star.

0:20:16.640 --> 0:20:19.679
<v Speaker 1>Why was NASA worried about it years ago? You know,

0:20:19.720 --> 0:20:22.200
<v Speaker 1>I think they just thought that crashing a probe into

0:20:22.240 --> 0:20:24.760
<v Speaker 1>it could spark a reaction. You know, the process we're

0:20:24.800 --> 0:20:28.159
<v Speaker 1>talking about, a sort of a natural gathering due to gravity.

0:20:28.320 --> 0:20:30.720
<v Speaker 1>You know, the Hindenburg went into flames without being the

0:20:30.760 --> 0:20:33.679
<v Speaker 1>mass of the Sun, and so people were just worried

0:20:33.680 --> 0:20:35.760
<v Speaker 1>that adding a spark to a ball of gas could

0:20:35.800 --> 0:20:38.560
<v Speaker 1>potentially ignite it. But I think that was a small

0:20:38.600 --> 0:20:42.359
<v Speaker 1>community of paranoid voices inside NASA, and most people weren't

0:20:42.400 --> 0:20:44.480
<v Speaker 1>too worried. But you know, if you know the story,

0:20:44.800 --> 0:20:47.560
<v Speaker 1>we were worried about igniting the atmosphere when we tested

0:20:47.600 --> 0:20:50.639
<v Speaker 1>the first atomic bomb in New Mexico. Really, yeah, that

0:20:50.760 --> 0:20:53.439
<v Speaker 1>was a possible concern. Yeah, before they tested it, they

0:20:53.440 --> 0:20:57.280
<v Speaker 1>did the calculations and they couldn't rule out igniting the atmosphere.

0:20:57.359 --> 0:20:59.560
<v Speaker 1>But you know, they went ahead and tried it. Anyway,

0:21:01.240 --> 0:21:03.840
<v Speaker 1>what's the worst that can happen? So it's not just

0:21:04.040 --> 0:21:08.120
<v Speaker 1>particle physicists that are potentially ending the world. Okay, oh good,

0:21:08.160 --> 0:21:12.840
<v Speaker 1>it's other kinds of physicists, that's right, and even ending

0:21:12.880 --> 0:21:16.879
<v Speaker 1>potentially other worlds. Yeah. So if you wanted to turn

0:21:16.960 --> 0:21:21.120
<v Speaker 1>Jupiter into a star, you'd have to somehow gather these materials. Yeah,

0:21:21.160 --> 0:21:23.119
<v Speaker 1>let's talk about that. If you're an alien in the

0:21:23.560 --> 0:21:25.919
<v Speaker 1>Arthursday Clark novel, how would you do it? Well, you know,

0:21:25.960 --> 0:21:28.280
<v Speaker 1>where can you get these materials? Like, what is the

0:21:28.320 --> 0:21:30.920
<v Speaker 1>source of raw materials you need to turn Jupiter into

0:21:30.960 --> 0:21:33.920
<v Speaker 1>a star. There's really the biggest things in the Solar

0:21:33.920 --> 0:21:36.399
<v Speaker 1>system are the Sun and Jupiter, and after that everything

0:21:36.440 --> 0:21:39.560
<v Speaker 1>else is a tiny detail. So the only place to

0:21:39.600 --> 0:21:41.919
<v Speaker 1>get this up is from the Sun. So you have

0:21:41.960 --> 0:21:45.359
<v Speaker 1>to basically steal from the Sun, siphon off a huge

0:21:45.400 --> 0:21:49.440
<v Speaker 1>amount of matter, and you know, feed that into Jupiter somehow. Really,

0:21:49.480 --> 0:21:52.760
<v Speaker 1>there's not enough gas floating around or asteroids floating around

0:21:52.800 --> 0:21:55.400
<v Speaker 1>to kind of feed Jupiter. There's only a tiny little

0:21:55.400 --> 0:21:57.440
<v Speaker 1>bit of gas and asteroids. Most of the stuff is

0:21:57.480 --> 0:22:00.399
<v Speaker 1>coalesced into the Sun and into Jupiter. And you know,

0:22:00.440 --> 0:22:03.040
<v Speaker 1>even Jupiter is like a tiny fracture. Remember it's one

0:22:03.119 --> 0:22:05.719
<v Speaker 1>one thousands of the mass of the Sun. So if

0:22:05.720 --> 0:22:08.359
<v Speaker 1>you like made a bar chart of all the stuff

0:22:08.359 --> 0:22:10.639
<v Speaker 1>in this solar system, it would basically just be the

0:22:10.680 --> 0:22:13.800
<v Speaker 1>Sun and then you know, a few crumbs. So Jupiter

0:22:13.880 --> 0:22:15.960
<v Speaker 1>is just like the biggest crumb, and after that there's

0:22:16.000 --> 0:22:19.159
<v Speaker 1>basically nothing of note. Al Right, So you would need

0:22:19.200 --> 0:22:22.000
<v Speaker 1>Jupiter to be ten times bigger, and so maybe let's

0:22:22.000 --> 0:22:24.680
<v Speaker 1>talk about how that would look like, Like, let's say

0:22:24.760 --> 0:22:27.280
<v Speaker 1>we increase the massive Jupiter by two how would it

0:22:27.320 --> 0:22:30.200
<v Speaker 1>look different. It wouldn't have enough energy to fuse, right,

0:22:30.560 --> 0:22:32.800
<v Speaker 1>and so it just looks like a bigger Jupiter. It

0:22:32.960 --> 0:22:35.400
<v Speaker 1>just you know, be bigger and fatter, and it would

0:22:35.400 --> 0:22:39.200
<v Speaker 1>have just as many crazy storms, but really no fundamental change.

0:22:39.359 --> 0:22:42.119
<v Speaker 1>It might emit more radiation because it would have more

0:22:42.160 --> 0:22:45.399
<v Speaker 1>activity in the interior do the increased pressure, Like the

0:22:45.440 --> 0:22:47.560
<v Speaker 1>surface would look sort of the same, would just be bigger.

0:22:47.560 --> 0:22:49.359
<v Speaker 1>It would just be bigger yeah, and the service would

0:22:49.359 --> 0:22:52.480
<v Speaker 1>look sort of the same. But we don't really understand jupiters,

0:22:52.520 --> 0:22:55.720
<v Speaker 1>like cloud patterns and what's going on there, the crazy vortices,

0:22:56.160 --> 0:22:58.840
<v Speaker 1>the red spot. That's the kind of thing we don't understand.

0:22:59.280 --> 0:23:03.400
<v Speaker 1>And if we preet Jupiter's mass, then all the features

0:23:03.400 --> 0:23:06.399
<v Speaker 1>that contribute to that craziness would be doubled, and so

0:23:06.440 --> 0:23:08.720
<v Speaker 1>we'd probably get it, as you know, twice as many

0:23:08.760 --> 0:23:11.080
<v Speaker 1>bands and much more craziness, and maybe the red spot

0:23:11.119 --> 0:23:13.359
<v Speaker 1>would be even more insane. Right, But there are a

0:23:13.359 --> 0:23:15.879
<v Speaker 1>lots of questions about these gas giants. Remember, Saturn has

0:23:15.880 --> 0:23:19.320
<v Speaker 1>a hexagon on his north pole that we don't understand either, Right.

0:23:19.520 --> 0:23:21.960
<v Speaker 1>We did a whole podcast about that mystery. It would

0:23:21.960 --> 0:23:24.600
<v Speaker 1>be a fascinating experiment to do to double the massive

0:23:24.640 --> 0:23:27.040
<v Speaker 1>Jupiter and just see what happens, Like, hey, turn that

0:23:27.160 --> 0:23:29.880
<v Speaker 1>knob and see how crazy these planets get. Yeah, let's

0:23:29.920 --> 0:23:33.280
<v Speaker 1>do it, Daniel, Okay, I'll write a proposal. What's the

0:23:33.280 --> 0:23:35.919
<v Speaker 1>worst that can happen? Well, what what would be happening

0:23:35.920 --> 0:23:37.639
<v Speaker 1>on the inside, Like I know that the inside of

0:23:37.720 --> 0:23:40.720
<v Speaker 1>Jupiter there's like what is it frozen hydrogen or something?

0:23:41.040 --> 0:23:46.159
<v Speaker 1>Metallic hydrogen? Metallic hydrogen yea oceans of liquid hydrogen is

0:23:46.200 --> 0:23:49.280
<v Speaker 1>all these layers of more and more compressed hydrogen, and

0:23:49.400 --> 0:23:52.000
<v Speaker 1>as you add more stuff to it than those layers

0:23:52.040 --> 0:23:55.040
<v Speaker 1>get denser and denser, right until at the very core

0:23:55.240 --> 0:23:57.640
<v Speaker 1>that's where the fusion would begin. When you get enough

0:23:57.680 --> 0:24:00.560
<v Speaker 1>match you sort of like gradually approved and you get

0:24:00.560 --> 0:24:04.920
<v Speaker 1>these layers and layers of more intensely squeezed hydrogen. Okay,

0:24:04.960 --> 0:24:07.440
<v Speaker 1>so then as I increased man, let's say I'm I'm

0:24:07.440 --> 0:24:10.600
<v Speaker 1>pouring more hydrogen into Jupiter. Now we're at like four

0:24:10.640 --> 0:24:13.480
<v Speaker 1>times the size of Jupiter right now or the mass?

0:24:13.720 --> 0:24:17.040
<v Speaker 1>Do things still change? Like, you know, does it suddenly

0:24:17.080 --> 0:24:19.840
<v Speaker 1>become more solid at the core or does it become

0:24:19.920 --> 0:24:23.000
<v Speaker 1>like a this nebulous ball of gas or does it

0:24:23.040 --> 0:24:25.520
<v Speaker 1>Would it look the same just bigger. It would look

0:24:25.560 --> 0:24:27.400
<v Speaker 1>the same, just bigger. I don't know that you would

0:24:27.440 --> 0:24:30.240
<v Speaker 1>see much different from the outside. Like again, we don't

0:24:30.280 --> 0:24:32.600
<v Speaker 1>understand the patterns on the surface, so it's hard to

0:24:32.640 --> 0:24:35.160
<v Speaker 1>predict what those would look like. But on the inside

0:24:35.160 --> 0:24:37.800
<v Speaker 1>you be getting new layers, you'd be getting the core

0:24:37.840 --> 0:24:40.960
<v Speaker 1>would be denser. Right as you add more mass, you're

0:24:41.000 --> 0:24:44.639
<v Speaker 1>creating new layers in the core that are denser and hotter,

0:24:44.960 --> 0:24:47.160
<v Speaker 1>and eventually you're gonna make the one that's going to fuse.

0:24:48.720 --> 0:24:50.639
<v Speaker 1>I wonder if it would grow another eye. Wouldn't that

0:24:50.720 --> 0:24:55.159
<v Speaker 1>be cool? Totally awesome. In fact, we wonder if that happened,

0:24:55.200 --> 0:24:57.800
<v Speaker 1>if it was typical or unusual. So really, we should

0:24:57.880 --> 0:25:00.800
<v Speaker 1>replicate this project. We should make like d you know,

0:25:00.960 --> 0:25:03.959
<v Speaker 1>double jupiters or ten quad jupiters, just to see if

0:25:03.960 --> 0:25:06.760
<v Speaker 1>it's a systematic or not. Wow. I mean, while we're

0:25:06.760 --> 0:25:09.760
<v Speaker 1>scooping matter out of the sun and playing god, let's

0:25:09.760 --> 0:25:13.640
<v Speaker 1>be systematic about it, all right. So now let's say

0:25:13.680 --> 0:25:15.919
<v Speaker 1>I keep going and I'm now I've pumped up Jupiter

0:25:16.119 --> 0:25:19.399
<v Speaker 1>up to one on the size of the mass of

0:25:19.440 --> 0:25:21.840
<v Speaker 1>the Sun, where it could become a brown dwarf. I

0:25:21.880 --> 0:25:25.040
<v Speaker 1>guess would it just automatically turn into a brown dwarf

0:25:25.320 --> 0:25:27.320
<v Speaker 1>or does it need like some kind of event to

0:25:27.400 --> 0:25:30.760
<v Speaker 1>trigger it, or does it happen slowly? Jupiter wouldn't actually

0:25:30.760 --> 0:25:32.280
<v Speaker 1>turn into a brown dwarf if you've got it to

0:25:32.320 --> 0:25:35.440
<v Speaker 1>one mass of the Sun, because that's a special kind

0:25:35.440 --> 0:25:38.600
<v Speaker 1>of process. It needs deuterium. And if we're just adding hydrogen,

0:25:38.760 --> 0:25:41.760
<v Speaker 1>remember which just protons and electrons that needs to get

0:25:41.760 --> 0:25:44.680
<v Speaker 1>to one tenth the mass of the Sun. Deuterium is

0:25:44.720 --> 0:25:47.639
<v Speaker 1>a special thing, and you need a proton and a

0:25:47.680 --> 0:25:51.679
<v Speaker 1>neutron and the electron around it, and the neutron helps

0:25:51.720 --> 0:25:54.359
<v Speaker 1>that fusion happen. You might think like, well, that's weird.

0:25:54.400 --> 0:25:57.800
<v Speaker 1>How's a neutron help fusion happen. It's neutral anyway, right,

0:25:58.320 --> 0:26:01.600
<v Speaker 1>Remember neutrons and these ound objects of quarks that have

0:26:01.680 --> 0:26:04.720
<v Speaker 1>the strong force. The neutron is what helps hold things together,

0:26:05.119 --> 0:26:08.600
<v Speaker 1>like in heavier elements. The neutron is the reason why

0:26:08.640 --> 0:26:11.520
<v Speaker 1>the element is stable. It keeps the protons separated, and

0:26:11.560 --> 0:26:15.040
<v Speaker 1>the little residual strong force from the quarks helps tie

0:26:15.080 --> 0:26:18.119
<v Speaker 1>everything together. So the neutrons are like the little helper

0:26:18.119 --> 0:26:22.120
<v Speaker 1>assistant particles making the fusion happen. The Brown Doors used

0:26:22.160 --> 0:26:26.120
<v Speaker 1>this special channel only available when you have deterior So

0:26:26.320 --> 0:26:29.919
<v Speaker 1>Jupiter isn't mostly deterium, it's mostly hydrogen. Oh man, alright,

0:26:29.960 --> 0:26:32.920
<v Speaker 1>So I did all this work. I inflated Jupiter to

0:26:33.080 --> 0:26:38.080
<v Speaker 1>ten times in size, and apparently nothing happens. Yeah, exactly.

0:26:38.240 --> 0:26:40.879
<v Speaker 1>So let's let's keep going. Let's keep pressing the accelerator

0:26:41.200 --> 0:26:44.040
<v Speaker 1>and see what happens to juventer. But first, let's take

0:26:44.040 --> 0:27:00.639
<v Speaker 1>a quick break, all right, Daniel. If I pop Jupiter

0:27:00.800 --> 0:27:03.679
<v Speaker 1>to one one hundreds the size of the Sun or

0:27:03.680 --> 0:27:05.720
<v Speaker 1>the mass of the Sun, nothing would happen. I would

0:27:05.720 --> 0:27:07.800
<v Speaker 1>need to take it to one tenth of the mass

0:27:07.800 --> 0:27:10.040
<v Speaker 1>of the Sun in order for Jupiter to be a star.

0:27:10.200 --> 0:27:13.159
<v Speaker 1>That's right, Make a blob of gas that's one tenth

0:27:13.200 --> 0:27:16.760
<v Speaker 1>the mass the Sun. Then gravity will coalesce it and

0:27:16.840 --> 0:27:19.159
<v Speaker 1>it will start to fuse, and it will start to glow,

0:27:19.280 --> 0:27:21.200
<v Speaker 1>and it will be a new star and you can

0:27:21.280 --> 0:27:25.840
<v Speaker 1>name it whatever you like. Well, now I feel all

0:27:25.840 --> 0:27:28.000
<v Speaker 1>this pressure to come up with a grid name. But

0:27:28.200 --> 0:27:31.399
<v Speaker 1>basically you need a hundred jupiters. You need Juiver to

0:27:31.400 --> 0:27:34.960
<v Speaker 1>be a hundred times bigger or more massive in order

0:27:35.040 --> 0:27:37.160
<v Speaker 1>for it to ever become a star. And even then

0:27:37.200 --> 0:27:38.879
<v Speaker 1>it would be a red dwarf, which is not like

0:27:38.920 --> 0:27:41.320
<v Speaker 1>the shiniest, prettiest kind of star. That's right. It would

0:27:41.359 --> 0:27:43.920
<v Speaker 1>be much smaller than our star and not as bright.

0:27:44.560 --> 0:27:46.880
<v Speaker 1>And would it ignite right away? Or is this like

0:27:46.880 --> 0:27:49.520
<v Speaker 1>like a slow burn where it slowly turns into a

0:27:49.520 --> 0:27:51.840
<v Speaker 1>red torch. Well, it depends on how dense it is

0:27:51.880 --> 0:27:53.480
<v Speaker 1>when you start, Like if you just start from a

0:27:53.520 --> 0:27:57.000
<v Speaker 1>big diffused cloud of gas the way our solar system started.

0:27:57.240 --> 0:27:59.160
<v Speaker 1>Then it's going to take a long time for gravity

0:27:59.200 --> 0:28:01.520
<v Speaker 1>to pull that together. There. If you start from a

0:28:01.560 --> 0:28:04.800
<v Speaker 1>place where it's already pretty dense, like about it Densis Jupiter,

0:28:05.359 --> 0:28:07.400
<v Speaker 1>then it's not going to take gravity that long because

0:28:07.440 --> 0:28:10.639
<v Speaker 1>everything is already pretty close together. But it'll start to

0:28:10.680 --> 0:28:13.280
<v Speaker 1>burn from the inside, right, and then that we'll have

0:28:13.320 --> 0:28:15.159
<v Speaker 1>to heat the next layers and the next layers and

0:28:15.160 --> 0:28:17.159
<v Speaker 1>the next layers, and so this isn't the kind of

0:28:17.160 --> 0:28:19.680
<v Speaker 1>thing that's going to happen, you know, in five seconds.

0:28:19.880 --> 0:28:21.560
<v Speaker 1>But it's also not going to take a billion years.

0:28:21.560 --> 0:28:23.720
<v Speaker 1>Oh I see. It's gonna start at the inside, and

0:28:23.760 --> 0:28:26.560
<v Speaker 1>then it's the heat the explosion of that. It's going

0:28:26.600 --> 0:28:30.360
<v Speaker 1>to gradually make it to the surface, and then that's

0:28:30.359 --> 0:28:34.000
<v Speaker 1>when you'll see its glow exactly. And it's just like

0:28:34.240 --> 0:28:36.840
<v Speaker 1>any other kind of fire, you know, the energy put

0:28:36.840 --> 0:28:40.520
<v Speaker 1>out by it sustains it, keeps that temperature hot, keeps

0:28:40.520 --> 0:28:44.640
<v Speaker 1>those fusion processes going. All right, Well, it sounds like

0:28:44.880 --> 0:28:47.800
<v Speaker 1>we're not likely to get a hundred jupiters all in

0:28:47.960 --> 0:28:51.080
<v Speaker 1>the same spot suddenly, although it's kind of cool to

0:28:51.080 --> 0:28:53.840
<v Speaker 1>think about, and so maybe um step aster, what is

0:28:53.880 --> 0:28:56.840
<v Speaker 1>the future of Jupiter. What's going to happen to it.

0:28:56.840 --> 0:28:59.280
<v Speaker 1>It's not going to become a star, but what is

0:28:59.280 --> 0:29:01.160
<v Speaker 1>it going to become? Yeah, and you know, even if

0:29:01.240 --> 0:29:03.520
<v Speaker 1>Jupiter did become a star, like if it turned on,

0:29:03.920 --> 0:29:05.920
<v Speaker 1>I just want to mention that it's not going to

0:29:05.960 --> 0:29:08.480
<v Speaker 1>be as bright as our sun. And it's much further

0:29:08.720 --> 0:29:11.280
<v Speaker 1>from us, right, Jupiter is much further from us than

0:29:11.360 --> 0:29:13.840
<v Speaker 1>the Sun is. So even if it became a star,

0:29:14.240 --> 0:29:17.200
<v Speaker 1>it wouldn't be nearly as bright in our sky as

0:29:17.280 --> 0:29:19.040
<v Speaker 1>the Sun. It wouldn't even be as bright in the

0:29:19.080 --> 0:29:22.120
<v Speaker 1>sky as the moon is. Actually, one of our sharp

0:29:22.160 --> 0:29:25.680
<v Speaker 1>listeners did this calculation, Dmitri Rudoi, found that a red

0:29:25.760 --> 0:29:28.200
<v Speaker 1>dwarf would be a bit brighter than the moon in

0:29:28.240 --> 0:29:31.360
<v Speaker 1>our sky. Thanks for keeping us honest, Dmitri. So it

0:29:31.360 --> 0:29:34.120
<v Speaker 1>would just be like a fairly bright star in the sky.

0:29:34.520 --> 0:29:39.040
<v Speaker 1>Oh really, even as is without inflating in Jupiter. If

0:29:39.080 --> 0:29:42.400
<v Speaker 1>suddenly Jupiter ignited became a star, which we said, well,

0:29:42.480 --> 0:29:45.280
<v Speaker 1>it couldn't happen. But even if you turn Jupiter into

0:29:45.320 --> 0:29:47.800
<v Speaker 1>a red dwarf, if you made it a hundred times

0:29:47.840 --> 0:29:50.600
<v Speaker 1>as big and it ignited and it was a red dwarf,

0:29:50.680 --> 0:29:53.120
<v Speaker 1>it wouldn't be as bright as our Sun, and it's

0:29:53.200 --> 0:29:56.040
<v Speaker 1>much further away from us, so it would appear dimmer

0:29:56.080 --> 0:29:58.440
<v Speaker 1>in our sky, So it wouldn't be very bright. Oh,

0:29:58.520 --> 0:30:02.040
<v Speaker 1>the distance from us to the Sun is much closer

0:30:02.080 --> 0:30:06.479
<v Speaker 1>than us to Jupiter. Yeah. Wow, Jupiter six times as

0:30:06.520 --> 0:30:09.440
<v Speaker 1>far away from the Sun as we are, which means

0:30:09.480 --> 0:30:13.280
<v Speaker 1>that at its closest approach, it's like four times as

0:30:13.320 --> 0:30:16.120
<v Speaker 1>far away from Earth as the Sun is. And so

0:30:16.200 --> 0:30:18.960
<v Speaker 1>that makes it one is bright if it was the

0:30:19.040 --> 0:30:21.520
<v Speaker 1>same brightness as the Sun, but it's going to be,

0:30:21.600 --> 0:30:25.000
<v Speaker 1>you know, much smaller than the Sun at the minimum threshold,

0:30:25.560 --> 0:30:27.840
<v Speaker 1>and so maybe just not that bright in the sky

0:30:28.120 --> 0:30:30.440
<v Speaker 1>compared to the Sun or even the Moon. So pretty

0:30:30.520 --> 0:30:34.600
<v Speaker 1>much nothing would change if Jupiter suddenly became a star. Yeah,

0:30:34.600 --> 0:30:36.280
<v Speaker 1>it wouldn't really change at all. I mean, it wouldn't

0:30:36.320 --> 0:30:39.000
<v Speaker 1>be as bright as elon Musk's star link satellites. Even

0:30:39.680 --> 0:30:43.280
<v Speaker 1>we wouldn't get that dramatic too, suns floating in the sky.

0:30:43.520 --> 0:30:47.240
<v Speaker 1>Look Skywalker looking out into the sundown of two stars.

0:30:47.560 --> 0:30:49.760
<v Speaker 1>It would just be like a bright star in the sky. Yeah,

0:30:49.880 --> 0:30:51.520
<v Speaker 1>And so for that to happen to have like two

0:30:51.520 --> 0:30:55.360
<v Speaker 1>effective suns in your sky. You really need a second

0:30:55.400 --> 0:30:59.320
<v Speaker 1>star that's as big, as bright and as close. That's

0:30:59.400 --> 0:31:02.320
<v Speaker 1>really critical, and that that would probably be kind of

0:31:02.360 --> 0:31:04.320
<v Speaker 1>a mess, wouldn't it, Like if you had would be

0:31:04.320 --> 0:31:07.959
<v Speaker 1>acute these sons that close together to each other and

0:31:08.040 --> 0:31:11.000
<v Speaker 1>to you, It wouldn't be a happy, happy solar system. Yeah.

0:31:11.040 --> 0:31:13.760
<v Speaker 1>And if you somehow created that son and then inserted

0:31:13.840 --> 0:31:16.520
<v Speaker 1>in there our existing solar system, there's no way that

0:31:16.560 --> 0:31:18.760
<v Speaker 1>any of our orbits would be stable, right, would like

0:31:19.000 --> 0:31:22.960
<v Speaker 1>completely gravitationally perturbed all the orbits. Like say, for example,

0:31:23.280 --> 0:31:26.720
<v Speaker 1>a huge sun came and ate Jupiter, like some sun

0:31:26.840 --> 0:31:29.720
<v Speaker 1>from another solar system happened to intersect our solar system

0:31:29.720 --> 0:31:31.480
<v Speaker 1>and just gobbled up Jupiter, and then we call that

0:31:31.560 --> 0:31:34.440
<v Speaker 1>the new Jupiter for some reason, that would totally destroy

0:31:34.480 --> 0:31:36.600
<v Speaker 1>our solar system, Like Earth would get flung out into

0:31:36.680 --> 0:31:39.560
<v Speaker 1>interstellar space. There's almost no chance that all the planets

0:31:39.600 --> 0:31:42.840
<v Speaker 1>would then like suddenly fall into a new stable set

0:31:42.840 --> 0:31:46.360
<v Speaker 1>of orbits around this pair of suns. Like that's very

0:31:46.440 --> 0:31:51.400
<v Speaker 1>totally disrupt our our orbits and probably tosses out into space. Yeah, yeah,

0:31:51.440 --> 0:31:53.280
<v Speaker 1>we'd become a rogue planet. We'd end up with no

0:31:53.480 --> 0:31:57.200
<v Speaker 1>stars all right. Well, so then what is more likely

0:31:57.240 --> 0:32:00.640
<v Speaker 1>to happen to Jupiter. What is Jupiter's most like feature?

0:32:00.760 --> 0:32:03.600
<v Speaker 1>Jupiter future is actually not that exciting. I mean, planets

0:32:03.640 --> 0:32:07.280
<v Speaker 1>are pretty stable. They're just hunks of stuff that are

0:32:07.360 --> 0:32:09.560
<v Speaker 1>mostly inert. I mean the stuff going on in the

0:32:09.600 --> 0:32:12.160
<v Speaker 1>center of the Earth, but it's not burning itself, it's

0:32:12.200 --> 0:32:16.200
<v Speaker 1>not consuming itself. So like stars have a lifespan because

0:32:16.240 --> 0:32:19.840
<v Speaker 1>they're burning their fuel and eventually they can't manage that

0:32:19.880 --> 0:32:22.880
<v Speaker 1>anymore and they collapse. Right The fire from that fusion

0:32:22.920 --> 0:32:25.880
<v Speaker 1>is sustaining them. But we're not really burning anything here

0:32:25.920 --> 0:32:28.720
<v Speaker 1>on Earth, and Jupiter isn't burning anything. It's just a

0:32:28.840 --> 0:32:30.840
<v Speaker 1>lump of stuff in space. And they can do that

0:32:30.960 --> 0:32:33.880
<v Speaker 1>basically forever. Lump of gas. Yeah, Like if you just

0:32:33.920 --> 0:32:35.480
<v Speaker 1>have a blob of gas, it can just be a

0:32:35.480 --> 0:32:38.520
<v Speaker 1>blob of gas forever. Yeah, exactly. And you know, the

0:32:38.560 --> 0:32:41.160
<v Speaker 1>Earth has an uncertain future because we're so close to

0:32:41.200 --> 0:32:44.400
<v Speaker 1>the Sun that when the Sun evolves and becomes a

0:32:44.480 --> 0:32:47.520
<v Speaker 1>red giant, it's going to become much much larger. In

0:32:47.560 --> 0:32:49.480
<v Speaker 1>the end stages of its life, it's going to grow

0:32:50.000 --> 0:32:53.320
<v Speaker 1>and eventually the Earth will be inside the Sun. Like

0:32:53.400 --> 0:32:55.760
<v Speaker 1>the Sun will grow so large that where we are

0:32:55.800 --> 0:32:59.440
<v Speaker 1>currently will be inside the radius of the Sun, but

0:32:59.560 --> 0:33:03.360
<v Speaker 1>for jim But Jupiter it's much further away. It's got

0:33:03.400 --> 0:33:06.760
<v Speaker 1>a good spot, so they're not going to be consumed

0:33:06.760 --> 0:33:09.360
<v Speaker 1>by the Sun or maybe even affected by it. Yeah,

0:33:09.400 --> 0:33:13.120
<v Speaker 1>when the Sun goes red giant and absorbs the Earth,

0:33:13.200 --> 0:33:15.760
<v Speaker 1>Jupiter will be fine out there. I mean the radiation

0:33:15.800 --> 0:33:17.800
<v Speaker 1>from the Sun will increase, the heat from the Sun

0:33:17.840 --> 0:33:20.440
<v Speaker 1>will increase, and so that will increase the amount of

0:33:20.480 --> 0:33:23.480
<v Speaker 1>solar radiation that lands on Jupiter. So it might get

0:33:23.560 --> 0:33:26.640
<v Speaker 1>like more violent storms on its surface, it might affect

0:33:26.640 --> 0:33:29.000
<v Speaker 1>that red spot, might heat it up a little bit,

0:33:29.240 --> 0:33:31.080
<v Speaker 1>but it's not going to be a big change for Jupiter.

0:33:31.160 --> 0:33:33.200
<v Speaker 1>So Jupiter is in a pretty good spot. It's happy

0:33:33.240 --> 0:33:35.840
<v Speaker 1>to sit there forever and not really do anything. It

0:33:35.840 --> 0:33:37.479
<v Speaker 1>sounds like we're going to have to move to Jupiter

0:33:38.280 --> 0:33:42.400
<v Speaker 1>in a few billion years. I wouldn't recommend it. Jupiter

0:33:42.480 --> 0:33:44.640
<v Speaker 1>is not that great a place to land, as the

0:33:44.680 --> 0:33:49.760
<v Speaker 1>Galileo probe discovered. But maybe one of the moons of Jupiter, right,

0:33:50.000 --> 0:33:52.200
<v Speaker 1>they're saying we could potentially live in one of them.

0:33:52.200 --> 0:33:54.600
<v Speaker 1>There's water maybe in some of them. Yeah, there's lots

0:33:54.600 --> 0:33:57.320
<v Speaker 1>of moons of Jupiter. That we think might already have life.

0:33:57.360 --> 0:34:00.720
<v Speaker 1>We did some fun podcast episodes about what's happening in

0:34:00.760 --> 0:34:04.719
<v Speaker 1>the potential underground oceans on some of those frozen moons.

0:34:05.040 --> 0:34:06.760
<v Speaker 1>Some of them have like a thick layer of ice

0:34:06.840 --> 0:34:10.200
<v Speaker 1>with water underneath, and so that could be a nice

0:34:10.200 --> 0:34:12.600
<v Speaker 1>place to live. Absolutely. Yeah, there's a big ball of

0:34:12.640 --> 0:34:14.680
<v Speaker 1>ice and water out there just waiting for us. Yeah,

0:34:14.719 --> 0:34:17.120
<v Speaker 1>assuming the aliens don't come and turn Jupiter into a star.

0:34:17.360 --> 0:34:19.759
<v Speaker 1>But but they can't. They would have to grow it

0:34:19.800 --> 0:34:22.480
<v Speaker 1>by a hundred. They would have to grow by a hundred, Yeah, exactly,

0:34:22.520 --> 0:34:24.839
<v Speaker 1>So they have to steal all that mass from our Sun.

0:34:25.320 --> 0:34:27.239
<v Speaker 1>So I don't know what the aliens were thinking in

0:34:27.239 --> 0:34:30.840
<v Speaker 1>two thousand ten. Well, I wonder if the future Jupiter

0:34:31.280 --> 0:34:34.879
<v Speaker 1>juve and astronomers are then gonna be laughing at our astronomers,

0:34:34.920 --> 0:34:38.200
<v Speaker 1>just like we were just laughing at the dinosaur astronomers saying, man,

0:34:38.239 --> 0:34:41.560
<v Speaker 1>that should have seen the sun, should have known that

0:34:41.560 --> 0:34:43.360
<v Speaker 1>the Sun was going to turn the red giant and

0:34:43.719 --> 0:34:45.600
<v Speaker 1>gone it out of the way. Yeah, well that's gonna

0:34:45.600 --> 0:34:47.600
<v Speaker 1>be in like a billion years, and so I hope

0:34:47.640 --> 0:34:50.040
<v Speaker 1>that we're still doing astronomy in a billion years, and

0:34:50.080 --> 0:34:52.040
<v Speaker 1>then we have those kind of things to think about

0:34:52.360 --> 0:34:54.759
<v Speaker 1>and to worry about. But I also hope that in

0:34:54.760 --> 0:34:57.600
<v Speaker 1>a billion years, we've gotten off the planet and we

0:34:57.719 --> 0:35:02.279
<v Speaker 1>have our Jovian Moon calling ease and astronomy happening in

0:35:02.320 --> 0:35:04.840
<v Speaker 1>the outer reaches the Solar system, and maybe even developed

0:35:04.840 --> 0:35:07.759
<v Speaker 1>warp drive to go do other solar systems. Yeah, I

0:35:07.800 --> 0:35:09.359
<v Speaker 1>guess that's what you could do it you can build

0:35:09.400 --> 0:35:12.319
<v Speaker 1>a wormhole that connects Jupiter in the Sun to sort

0:35:12.320 --> 0:35:17.799
<v Speaker 1>of shunt material from the Sun directly into Jupiter. Oh no, now,

0:35:17.920 --> 0:35:21.600
<v Speaker 1>now we sparked imagination of a physicist. What's the worst

0:35:21.600 --> 0:35:23.680
<v Speaker 1>that can happen if we create a wormhole like a

0:35:23.800 --> 0:35:27.200
<v Speaker 1>nice Jupiter and the Sun? Yeah, exactly. Well, Fortunately I

0:35:27.239 --> 0:35:29.399
<v Speaker 1>don't know any engineers willing to actually build this thing

0:35:29.440 --> 0:35:33.600
<v Speaker 1>for me, so I'm free to speculate wildly. Oh good, Yeah, well,

0:35:33.800 --> 0:35:36.239
<v Speaker 1>we'll all make a pack. All of us engineers will

0:35:36.280 --> 0:35:38.960
<v Speaker 1>make a pack. Not to help any physicists do any

0:35:39.000 --> 0:35:42.080
<v Speaker 1>kind of crazy stuff. Don't answer emails from Daniel, even

0:35:42.080 --> 0:35:44.239
<v Speaker 1>if it seems like a good idea, yeah, even if

0:35:44.239 --> 0:35:49.960
<v Speaker 1>he has money. Don't did reply? All right, Well, it

0:35:50.000 --> 0:35:51.879
<v Speaker 1>sounds like a lot of the people who maybe we're

0:35:51.920 --> 0:35:53.919
<v Speaker 1>worried that Jupiter was going to turn into a star.

0:35:54.080 --> 0:35:57.160
<v Speaker 1>Can rest easy because it doesn't sound like Jupiter is

0:35:57.239 --> 0:36:00.520
<v Speaker 1>going to be a star anytime soon, or and even

0:36:00.560 --> 0:36:04.439
<v Speaker 1>become a star anytime soon. Or maybe that's right. Even

0:36:04.440 --> 0:36:08.200
<v Speaker 1>though Jupiter totally dwarfs us, it's really small compared to

0:36:08.200 --> 0:36:11.800
<v Speaker 1>the thresholds necessary to become even the dimmest, lamest kind

0:36:11.840 --> 0:36:15.440
<v Speaker 1>of star. And it's much much smaller than those cosmic

0:36:15.520 --> 0:36:18.799
<v Speaker 1>giants that are out there fusing and illuminating the cosmos.

0:36:19.200 --> 0:36:21.279
<v Speaker 1>And so while there is a lot of drama out

0:36:21.320 --> 0:36:24.279
<v Speaker 1>there in the universe, stars collapsing and forming and all

0:36:24.320 --> 0:36:27.160
<v Speaker 1>sorts of crazy things happening, it seems like Jupiter it's

0:36:27.239 --> 0:36:31.640
<v Speaker 1>pretty solid. So rest easy and relaxed because Jupiter is

0:36:31.680 --> 0:36:34.319
<v Speaker 1>just gonna keep on floating out there, keeping its big

0:36:34.360 --> 0:36:37.360
<v Speaker 1>red eye on. That's right, and we recommend you invest

0:36:37.600 --> 0:36:41.239
<v Speaker 1>in Jovian moon real estate. Can you is that? Listen

0:36:41.239 --> 0:36:44.000
<v Speaker 1>on redfin Send me a check and I will send

0:36:44.000 --> 0:36:48.840
<v Speaker 1>you a title to your new property. It sounds like

0:36:48.880 --> 0:36:52.359
<v Speaker 1>you could get arrested for that, Daniel, But all right, well,

0:36:52.400 --> 0:36:54.560
<v Speaker 1>we hope you enjoyed Dad. Thanks for joining us, and

0:36:54.600 --> 0:36:56.680
<v Speaker 1>thanks for sending in your Questions. If you like a

0:36:56.800 --> 0:36:59.400
<v Speaker 1>question answered on the podcast, please send it to us

0:36:59.400 --> 0:37:02.160
<v Speaker 1>to question at Daniel and Jorge dot com. See you

0:37:02.239 --> 0:37:12.640
<v Speaker 1>next time. Thanks for listening, and remember that Daniel and

0:37:12.719 --> 0:37:16.000
<v Speaker 1>Jorge Explain the Universe is a production of I Heart Radio.

0:37:16.280 --> 0:37:19.000
<v Speaker 1>For more podcast For my heart Radio, visit the I

0:37:19.200 --> 0:37:22.840
<v Speaker 1>heart Radio app, Apple Podcasts, or wherever you listen to

0:37:22.920 --> 0:37:23.880
<v Speaker 1>your favorite shows.