Feb. 8, 2026

Theia's Fate, Galaxy Mergers & the Mysteries of Mars' Atmosphere | Q&A

Theia's Fate, Galaxy Mergers & the Mysteries of Mars' Atmosphere | Q&A

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This episode of Space Nuts brought to you by Incogni.Reduce the volume of spam calls and emails. They can't spam you if the can't find you. To find out more and to take up our 60% off offer, visit incogni.com/spacenuts and use the cou[on code SPACENUTS at checkout.  

Theia's Fate, Galactic Mergers, and the Mysteries of Hydrogen
In this captivating Q&A edition of Space Nuts, hosts Andrew Dunkley and Professor Fred Watson tackle a range of intriguing questions from listeners, diving deep into cosmic mysteries and scientific theories. From the fate of the former planet Theia to the dynamics of galaxy mergers and the origins of hydrogen, this episode is packed with insights that will expand your understanding of the universe.
Episode Highlights:
- The Fate of Theia: Rusty from Donnybrook poses a thought-provoking question about Theia, the planet that collided with Earth. Andrew and Fred discuss the most accepted theories regarding Theia's remnants and how they may have been absorbed into Earth's mantle, leaving behind intriguing geological evidence.
- Galaxy Mergers Explained: New listener Melina asks about the merging of spiral galaxies in an expanding universe. The hosts explain how gravity can overcome the universe's expansion on galactic scales, leading to fascinating interactions and eventual mergers between galaxies.
- Olympus Mons and Mars' Atmosphere: Kevin wonders if the colossal eruptions of Olympus Mons could have contributed to Mars' atmospheric loss. Andrew and Fred explore the volcanic activity on Mars and clarify that while Olympus Mons is impressive, the planet's lack of a magnetic field is a more significant factor in its atmospheric decline.
- Hydrogen's Cosmic Origins: Five-year-old Yuki asks why hydrogen is the only element not formed in stars. The hosts explain that hydrogen was created shortly after the Big Bang, making it the most abundant element in the universe, while other elements formed later through stellar processes.

For more Space Nuts, including our continuously updating newsfeed and to listen to all our episodes, visit our website. Follow us on social media at SpaceNutsPod on Facebook, Instagram, and more. We love engaging with our community, so be sure to drop us a message or comment on your favorite platform.
If you’d like to help support Space Nuts and join our growing family of insiders for commercial-free episodes and more, visit spacenutspodcast.com/about.
Stay curious, keep looking up, and join us next time for more stellar insights and cosmic wonders. Until then, clear skies and happy stargazing.

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WEBVTT

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Hello again, thanks for joining us on a Q and

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a edition of Space Nuts. My name is Andrew Dunkley,

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and today we will be I won't Fred will be

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answering questions about the former planet known as Fear Galaxy.

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Mergers have come up. We go back to Mars with

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a theory about Olympus mons and why only hydrogen? That

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is a question that comes from a believer, a five

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year old. We'll deal with all of that today on

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this edition of Space Nuts fifteen in channel ten nine

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ignition sequence Space nuts or three two space nuts as

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can I reported Neil Goods. And to solve all of

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those little riddles, we're joined again by Professor Fred Watson,

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Astronomer at Large.

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Hello Fred, Hello Andrew, very good to see you again.

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Good to see you too. We've got a bit of

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weird noise on your line. I think it's probably just

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the Internet being the Internet, so hopefully that'll go away.

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In fact, it just did, so yeah, there you go,

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solved itself. It must have heard me winging all as well.

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I assume.

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Yep, we're doing fine. Thank you. It's good to join

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you on the questions episode of what's this called again?

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Oh Space Nuts?

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That's right, space idiots, space nuts. Yes, yeah, they're all

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good people. We might as well jump in straight away

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to our first question, and it comes from one of

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our regular contributors.

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It's Rusty today, Fred and Andrew, It's Rusty in Donnybrook.

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I've been listening to your latest episode where look at

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the relationship between Sea and the Earth before the collision,

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and I just want to make sure I've got the

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story glory straight, so I put it in my own words.

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The Earth had a buddy named THEA who came a

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little too near. She hit with a splash, then made

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off with a dash. But there's no mooning for THEA

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around here, So what happened to THEA after the collision?

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The theories prior to this revelation said THEA had enough

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kinetic energy to leave the Solar System all together.

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But if the orbits were so close, that doesn't seem likely.

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So it seems to me there's three possibilities that THEA

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fell into the Sun, which would be another amazing feat

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to get that sort of precision. After the collision, Sea

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picked up a little slingshot energy and moved out further

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and became Mars, and Mars is a Mars size object

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after all. And the third possibility I can think of

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is that it picked up an unlikely amount of kinetic

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energy and became planet nine. So if it did become

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planet nine, it would have a highly eccentric orbit because

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it's too far away from us to actually see at

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the moment. But would this orbit then at some stage

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bring it back to the Inner Solar System of its origin?

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That's it? How you guys? Well, jeez, thanks, Rusty, hope

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you're will two over there in w A. What happened

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to THEA? He's come up with some interesting theories, quite

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a few ideas. I'm guessing they can't all be true.

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I think that's right. There's actually a fourth possibility I

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did to the three that that Rusty has proposed, and

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I think that's the one that's usually accepted, and there's

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kind of evidence for that. The fourth possibility is that

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basically was absorbed into the Earth. The remnants of thear

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actually in the Earth's mantle, And in fact, there's something

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called and there are two of these, a large low

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sheer velocity province in the Earth's lower mantle. And the

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hypothesis is that that is the remnants of thear so

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that we still see the evidence of that collision by

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anomalies basically in the Earth's mantle, which we investigate, you know,

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with seismology. That's how we know about what's going on

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in the mantle of the Earth. It's how we know

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about large low sheer velocity provinces. I'm kind of just

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using the words here because I'm not somebody who knows

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about the inside of the planet other than you know,

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the sketchiest outline of a core, a mantle, and a crust.

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But the mantle we know has significant structure and in

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fact money. And I have a good friend who Nick Petford,

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who is a volcanologist, and he's somebody who looks at

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these velocity structures in the in the mantle of the

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Earth and you know, the upwelling of material to form

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volcanoes and things like that. Next time we see Nick,

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I will ask him about these large scale low velocity

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shear areas and their relationship to THEA. But I think

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that's the consensus, rusty that the impact basically resulted in

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an explosion which shed something like I think one of

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the suggestions is about seventy percent of the mass of

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the Moon may have come from THEA. I'm actually I

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think that might. Let's put it this way, THEA is

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responsible for seventy to ninety percent of the total mass

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of the Moon. Under the classic giant impact scenario, where

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THEA is considerably smaller than a proto Earth, which it

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would have been, the Earth was still kind of Earthish sized.

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THEA was Mars ish sized, but the Earth would have

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probably grown a bit by absorbing the debris from THEA.

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Remember that the mass of the Moon is about one

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eightieth of the mass of the Earth, so it's a

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significantly large body compared with the other moons in the

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Solar System, but it's clearly smaller than you know, it's

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not Mars sized, And so Rusty's right in that the

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you know, the remnants of THEAR had to do something,

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but the current theory is that they were absorbed by

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the proto Earth, and we can still see evidence for them.

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Yeah, okay, so yeah, definitely not likely to be P nine.

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That would be a very odd kind of occurrence, wouldn't it.

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Yeah, well, yes, I think that kinematics don't work. You

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you know, you can't give it enough velocity and you

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need you need a lot of velocity for it to

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fall back into the Sun as well, too much energy.

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That's quite an energetic process, is getting rid of the

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orbital velocity of a body to make it fall into

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the sub It's you know, you need as much energy

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as you do to get it pushed out to the

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outer planet.

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So, yeah, didn't we talk about it once before and

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suggest that remnants of it just probably speed off into

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space never to be So again.

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I'm sure there would have been an element of that. Yes,

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you know that that debris cloud that eventually formed the

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Moon probably lost some of its some of its material content,

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and there may even be stuff wandering around in the

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form of neuroth asteroids now that are bits and pieces

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that are left over from that. But remember this was

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you know, this was within the first couple of hundred

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million years of the history of the Solar System. So

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you're talking about things that happened a very long time ago. Yeah.

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Indeed, I'm wondering, Fred, why we've just got this sudden

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influx of people asking questions in POM. This is just

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I'm blaming Martin for that. Martin Berman Gorvine, you started

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this and now it's so I think.

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I really liked Rusty's one there about the thought that

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was very nice.

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Yeah, I don't know. I think he pushed it a

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bit on one of those one of those rhymes. Although

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there there was a regular guest, and I'm sure you

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know who I'm talking about, col Wilson, who used to

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join us on the radio once a week to do

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bush poetry, Blew the Shearer, and he often got asked

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to do shearing demonstrations and he had to tell them, look,

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I'm not a shearer. I can't the sheer a sheep

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that saved my life. It's just my show name. But

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he used to actually invent words to create rhymes. It

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was one of his wonderful traits. And yeah, I used

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to spend a lot of time with Collie as a

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terrific bloke. I think we've dealt with Rusties theories and

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they were all wrong. Thanks for Rusty. Takes Rusty great

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to hear from you. Let's take a break from the

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with anguality. Here the land space nuts. Let's move on

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to our next question, and this one I've lost here

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it is. This comes from Lena. I am a new

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listener and not as hardcore as Spacenut as most of

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your audience. It's probably a good thing, but I saw

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an article today talking about merging spiral galaxies. If the

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universe is expanding, how does something as large as a

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galaxy move toward and merge with another galaxy? It seems

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they should be moving further away from each other. That

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comes from Lena in British Columbia in Canada. I think

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we've had questions of this ilk before, but it's always

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good to go over it again because there's a lot

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more going on in the universe than just you know,

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spreading out like school children playing what's that game where

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you don't know, I don't know what you call it?

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Something that you throw a ball and try and hit

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someone in the head. Anyway, go on, that's cricket, isn't it? Dodgeball? Dodgeball?

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And there's a bunch of games like that, like Red

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Rover Crossover. Did you ever play that? Oh no, we

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mustill have a lot of fun with that.

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Anyway. Look, Lina's question is a great one, and I

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guess the simplest answer here is that, yes, galaxies are big,

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but they're tiny compared with the universe, And so the

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expansion of the universe is something that we look at

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on very large scales. You know, you're looking out billions

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of light years and seeing this expansion. It's actually, with

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today's technology, it's one of the easiest observations that you

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can make that the universe is expanding, discovered back in

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nineteen twenty nine by Edwin Hubble. So, yes, So if

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the universe is expanding in space, is getting bigger and

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naturally carrying things further and further apart, why are some

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galaxies coming towards each other? And it's because on the

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scale of a galaxy, the expansion of the universe is miniscule,

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and that by far the dominant the dominant process is gravity.

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So galaxies, which yes, are being carried gradually apart by

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the expansion of the universe, when you put them close together,

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their own gravity gives them a force that pulls them

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together that's much greater than the expansion. And we actually

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give that a name. We call this the peculiar velocities

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of galaxies, because it's a velocity peculiar to an individual galaxy.

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And the usual way that we describe it, and I

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think we've talked about this before on Space Nuts, is

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if you imagine a river flowing, which represents the kind

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of expansion of the universe, and then somebody in a

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boat is moving around on the river. They're being carried

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downstream by the river's movement, but they've got their own

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movement provided by the boat on the water. And it's

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a bit like that with galaxies. They're being carried along

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by the expansion of the universe, but a far bigger

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effect is the way gravity pulls them together. So that's

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what's pulling our galaxy and the Andromeda galaxy together. It's

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the gravitational force between them. And on the scale of

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the distance between Andromeda and our own galaxy, which is

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about two and a half million light years, the expansion

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of the universe makes virtually no difference. You only start

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really noticing it when you get to much bigger, bigger scales.

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Yeah, they will come a point in time where all

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these galaxy mergers will finished, They'll be done and dusted,

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and the universe will keep expanding and eventually it'll just

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be darkness. There'll be nothing.

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Yeah. If that's assuming dark aage big crunch, right, yeah,

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I mean dark energy. We're now just starting to see

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the first signs that maybe over the last few billion

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years it's decreased. And so the acceleration of the universe

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it's still accelerating. The expansion is still getting faster, but

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it's getting faster at a slower rate, if I put

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it that way. So the acceleration itself looks as though

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it's declining. And that's why some people are still talking

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about the big crunch or they're going to have gibb again.

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It's it's because if the acceleration eventually goes away and

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becomes a deceleration, then yeah, you're going to get a

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big crunch.

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Yeah, yeah, it's you know, could go either way at

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this stage the way they're talking. We we have witnessed

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some galaxy e mergers, haven't we. It doesn't. Our own

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galaxy actually contain a couple of other galaxies that have

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been sucked into our void.

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Yeah, two quite big ones. Actually, what the things we

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call the large and small Madrilanic clouds. They are satellite

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galaxies of our own and they're being stripped of their

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stars by our own galaxy. It's gravitational pull and will

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eventually be part of the halo of our own galaxy.

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But we see we also see examples in deep space

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of big galaxies actually merging. The most famous is the

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Antenna Galaxies, two galaxies which are merging and pulling off

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spiral arms off each other.

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Quite it all happens in slow motion, though, doesn't it.

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And and when people, you know, think about galaxy merger merges,

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they're thinking all this drama and collisions and generally doesn't

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turn out that way.

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Well, you're talking about processes that take millions of years,

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and yeah, and you know it's and and in fact,

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galaxies probably when they collide, you don't get stars actually

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colliding because there's so much space between the stars. But

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what you get is the effect of clouds of gas colliding,

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and that spawns new star formation, so you might get

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lots of hot young stars being born in a galaxy collision.

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All right, here's my horrible attempt at poetry. It's more

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of a dance than a glance.

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I like that.

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Yeah, yeah it is.

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Actually that's exactly what it is.

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Yeah, there we go. All right. I hope that answers

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your question. Lena, Thanks for sending it in and thanks

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for listening to Space Nuts, which is what you're doing

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right now with Andrew Dunkley and Professor Fred Watson.

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We choose to go to the moon and this decay

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and do the other thing not because they are easy,

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but because.

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They are hard, these nuts. Our next question comes from Kevin,

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and he said, I've been listening with much learning and

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enjoyment to all the previous podcasts. I'm about halfway through them,

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so he's at around two hundred and nearly three hundred,

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I imagine, so let's just wait for him to catch up.

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He says, your discussions of Mars and its lack of

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atmosphere made me wonder if perhaps what must have been

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an enormous eruption of Olympus Olympus Mons is what might

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have killed the planet, or at least its atmosphere. That

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comes from Kevin, So, yeah, I'm very impressed by Olympus

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Monds because it is the biggest volcano in the Solar System,

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and it's staggeringly huge. But could an Olympus Mons eruption

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have stripped the atmosphere of Mars?

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Probably not, the I mean the eruptions of Olympus Mons

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would certainly have sent a lot of gas into the atmosphere.

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Olympus Mons has probably taken a long long time to grow.

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It's you know, it will have had eruptions kind of

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like some of the bigger volcanoes on Earth, and they

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took a long long time, so it's not like one

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big explosion. And that's why Olympus Mons is so high.

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It's because it's over a hot spot in Mars's mantle

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that just keeps on pushing out material, or did for

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a long period of time, and without the plate tectonics

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that carry the surface crossed over the hot spot and

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results in a chain of volcanoes like we see in Hawaii.

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It all built this one big volcano. So it's a

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process that took a long time, and maybe it did

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play a role in the changes in Mars's atmosphere. But

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we think the main reason why Mars lost its atmosphere

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is because it is a world that is too small

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to sustain plate tectonics. It doesn't have a magnetic field,

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so the subatomic particles from the Sun bombard the atmosphere continuously,

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and we think that's one of the main reasons why

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why it eventually lost lost its atmosphere. I mean, it's

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not most altogether. It's still got zero point six of

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a percent of the Earth's atmospheric pressure at the surface.

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That's enough for winds to blow and you know, to

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sort of blow dust clouds onto solar panels of spacecraft

312
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and things of that sort. But it's certainly not an

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atmosphere that we would recognize as being similar to Earth's.

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So I think, I think it's a good question. Actually,

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I think Olympus Mons and the neighboring volcanoes, there's there's

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more than one big volcano, the Olympus Mons is the biggest.

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They probably would have affected the atmosphere of Mars, but

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they're probably not the root cause why the atmosphere drifted

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into space.

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Yeah, it's more likely it was because Mars just couldn't

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hold itself together. Basically, it didn't have the gravity.

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It's yeah, it doesn't have the gravity to keep it

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hot enough to sustain plate tectonics or a magnetic dynabo basically,

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which is a magnetic field.

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Yeah, but Olympus Mons is fascinating for a few reason,

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So correct me if I'm wrong. But I think right now,

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as Mars is Olympus Mon's summit actually peaks out of

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the atmosphere. Is that right? It's sticking up that high?

329
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Yeah, it's certainly. I mean the atmosphere is like Earth's atmosphere.

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It gradually disappears as you go higher. But yeah, I

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mean effectively the summit is the pressure will be considerably

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lower there than it is delm what you might call

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the surface of Mars.

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This is one honking big shield volcano, though, isn't it

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like twenty one point two eighty seven kilometers in height

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thirteen point two miles or sixty and forty feet. Someone's

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going to climb that one day and stick a flag

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in it. It's two and a half times the elevation

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of Mount Everest. And this is something about Mars that

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astounds me. It's a smaller planet, but all its features

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geographically just make ours look like tidley wings. And it

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span is six hundred kilometers six hundred kilometers wide.

343
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Yep, that's that's extra.

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I just can't imagine it. I'd love to be able

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to stand there and have a look in my last

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five seconds of life, because I didn't take my breathing apparatus.

347
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But it is an amazing world.

348
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It's got cliffs as well around its base which are

349
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pretty spectacular. I think they're killing meters as well, so

350
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you know, it's quite quite, quite an extraordinary world.

351
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Yeah. Well, the Coldera itself is fifty miles across, and

352
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you compare that to Kilaweo, which is like a couple

353
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of miles across. It's amazing. No. I love that question,

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and yeah, good thinking, but probably not. And it sort

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of brings back the same argument on Earth that people

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say our global warming is caused by volcanoes and cows.

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It's got nothing to do with the billions of cars

358
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that we're driving around every day. But I think they've

359
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proven that's just not the case as far as i'm aware.

360
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Thanks for your question, Kevin, lovely to hear from you.

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Our final question comes from Yuki Hi. I'm Yuki. I

362
00:23:33.599 --> 00:23:37.240
am five years old and I live in Canberra. We

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00:23:37.359 --> 00:23:40.160
listen to your podcast nearly every day. My question is

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00:23:40.359 --> 00:23:45.319
why is hydrogen the only element that isn't made in stars?

365
00:23:45.440 --> 00:23:49.000
Why was hydrogen the only element around just after the

366
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Big Bang and not others?

367
00:23:52.960 --> 00:23:57.759
Yeah, that's a great question. Yeah, and congratulations to your

368
00:23:57.839 --> 00:24:00.799
ki on being able to even think of a question.

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Like that at the age of five, because I certainly

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wouldn't have.

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Been now I wouldn't either. I was still trying to

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fix the wheel on my conquered toy.

373
00:24:08.519 --> 00:24:11.200
Yes, that's right. I think I was at that level,

374
00:24:11.640 --> 00:24:16.559
and that look, the the bottom line is that hydrogen

375
00:24:17.839 --> 00:24:21.240
it was created in the aftermath of the Big Bang.

376
00:24:21.279 --> 00:24:23.839
I think sort of three minutes after the Big Bang,

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the temperature had cool enough that you could start to

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form atoms. And the atom that was was produced was

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the simplest it's one proton. It's the simplest atomic nucleus.

380
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And so that was what basically condensed out of the

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00:24:46.759 --> 00:24:49.759
of the of the aftermath of the Big Bang. As

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00:24:49.839 --> 00:24:56.480
as energy became matter, you got protons forming, and hydrogen

383
00:24:56.799 --> 00:25:03.319
is protons. In fact, in that period you also got

384
00:25:03.359 --> 00:25:07.680
the start of the process that does produce other elements

385
00:25:07.720 --> 00:25:11.839
in stars, what we call nuclear synthesis, where the nuclei

386
00:25:11.960 --> 00:25:15.880
of atoms, the centers of the atoms stick together, and

387
00:25:16.200 --> 00:25:18.680
it did. That process did start. So I think it

388
00:25:18.839 --> 00:25:21.079
come from the percentage it's something like twenty percent. I

389
00:25:21.160 --> 00:25:23.920
think of the aftermath of the Big Bang is helium,

390
00:25:24.279 --> 00:25:31.000
which is the next most complex atomic nucleus, and formed

391
00:25:31.039 --> 00:25:36.079
by hydrogen atoms coming together, but then the temperature dropped

392
00:25:36.119 --> 00:25:40.680
far enough that you didn't get the extension of that

393
00:25:40.920 --> 00:25:48.319
process into the formation of other atoms. So it basically

394
00:25:48.440 --> 00:25:53.359
had to wait until stars started to form because of

395
00:25:53.359 --> 00:25:58.000
the gravitational pull of these clouds of hydrogen together that

396
00:25:58.359 --> 00:26:03.759
raised the temperature again enough to start forming other elements.

397
00:26:04.640 --> 00:26:07.440
And so that's basically what it's all about. It's just

398
00:26:07.559 --> 00:26:10.920
the simplest of atoms is the hydrogen atom. That is

399
00:26:10.960 --> 00:26:14.839
why that was created. And you know, we nearly got

400
00:26:14.880 --> 00:26:21.079
more elements being created in the Big Bang, but only helium.

401
00:26:21.240 --> 00:26:24.039
Actually there's a bit of lithium and other stuff as

402
00:26:24.079 --> 00:26:31.440
well tiny amounts of other nuclei. But it's true to

403
00:26:31.480 --> 00:26:36.079
say that the star formations, star formation, and the interiors

404
00:26:36.079 --> 00:26:39.559
of stars is what led to the huge array of

405
00:26:39.599 --> 00:26:41.640
elements that we see now, all the elements of the

406
00:26:41.680 --> 00:26:45.519
periodic table. That's a fantastic question. It is.

407
00:26:46.240 --> 00:26:49.039
When you look at the list of the top ten

408
00:26:49.480 --> 00:26:54.240
gases in the universe by order of concentration, hydrogen is

409
00:26:54.400 --> 00:26:58.160
far and away the most dominant, with seventy four to

410
00:26:58.160 --> 00:27:00.960
seventy five percent of what they did scrub is baryonic

411
00:27:01.039 --> 00:27:04.920
mass helium at twenty four to twenty five percent, which

412
00:27:05.000 --> 00:27:09.039
leaves almost no room for anything else. Oxygen is less

413
00:27:09.039 --> 00:27:11.599
than one percent carbon, less than half a percent, neon,

414
00:27:11.799 --> 00:27:16.079
less than point one and then it just dwindles away.

415
00:27:16.559 --> 00:27:19.200
At number ten, you've got sulfur at point zero zero

416
00:27:19.759 --> 00:27:27.359
point zero four to four percent concentrations. They're staggering numbers

417
00:27:27.359 --> 00:27:28.279
when you're really.

418
00:27:28.759 --> 00:27:31.880
Yeah, so you go down the list. The bottom line

419
00:27:31.920 --> 00:27:35.559
is that the Big Bang hydrogen is still around. In fact,

420
00:27:35.640 --> 00:27:38.960
it it makes up quite a large percentage of the

421
00:27:38.960 --> 00:27:42.200
items in your body as well. Yeah.

422
00:27:42.279 --> 00:27:48.240
Yeah, well it's everywhere, isn't it. And that's the bottom line.

423
00:27:48.279 --> 00:27:52.440
And the way the Big Bang happened and everything that

424
00:27:52.559 --> 00:27:56.799
went on afterwards, you know, one smidgy little thing didn't happen,

425
00:27:56.839 --> 00:28:01.079
we probably wouldn't be here. Yeah, that's right. It's a

426
00:28:01.119 --> 00:28:04.799
scary thought. But then again, there's so much we don't know.

427
00:28:05.759 --> 00:28:10.799
U People believe in multiverses because they say, you know,

428
00:28:10.880 --> 00:28:14.640
the conditions are exactly right for life to form in

429
00:28:14.680 --> 00:28:17.759
our universe, and they might not have been. Yes, maybe

430
00:28:17.759 --> 00:28:22.279
there are lots of other universes where life didn't form.

431
00:28:22.519 --> 00:28:28.880
Well, yeah, the mathematics supports the theory, doesn't it. Oh gosh,

432
00:28:29.920 --> 00:28:34.359
the brain hurting part of the show just happened. So anyway, Yeah,

433
00:28:35.240 --> 00:28:37.319
it just keeps us thinking and it keeps us looking

434
00:28:37.400 --> 00:28:40.039
for answers, and that's what it's all about. Yuki. Great

435
00:28:40.079 --> 00:28:43.119
to hear from you, and hope all is well in Canberra.

436
00:28:43.440 --> 00:28:46.279
And a reminder, if you would like to send us questions,

437
00:28:47.119 --> 00:28:49.319
we welcome them with open arms. You can send them

438
00:28:49.440 --> 00:28:53.200
through our website space nuts dot io and just click

439
00:28:53.279 --> 00:28:55.480
on the ask Me Anything link at the top. It

440
00:28:55.519 --> 00:28:58.680
says a M A and we will do our best.

441
00:28:58.680 --> 00:29:01.200
Don't forget to tell us who you are and where

442
00:29:01.240 --> 00:29:05.559
you're from, and we will put your question on if

443
00:29:05.559 --> 00:29:07.359
we haven't had it before, and even if we have,

444
00:29:07.480 --> 00:29:11.039
we might revisit them. We do that from time to time.

445
00:29:11.759 --> 00:29:14.559
Keep them coming. And if you haven't asked a question

446
00:29:14.599 --> 00:29:16.799
before and you've always wanted to, please send it in.

447
00:29:17.079 --> 00:29:21.440
We'd love to hear from you. And we're just about done. Fred,

448
00:29:21.480 --> 00:29:22.519
thank you very much.

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00:29:23.519 --> 00:29:27.200
Great pleasure. Andrew Or was good and hopefully we'll chat

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again soon.

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I hope, so that'll be good. Professor Fred Watson, Astronomer

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at Large. And thanks to Hu in the studio who

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didn't have a hydrogen problem, but he did have a

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methane problem. But he'll be out of an emergency surgery

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very very soon, hopefully for next week's episode. And from

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me Andrew Dunkley, thanks for your company. Catch you on

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the next episode of Space Nuts. Bye bye.

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You'll be listening to the Space Nuts podcast.

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00:29:52.359 --> 00:29:58.440
Available at Apple Podcasts, Spotify, iHeartRadio, or your favorite podcast player.

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00:29:58.640 --> 00:30:01.720
You can also stream onto the at fights dot com.

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This has been another quality podcast production from fights dot com.