Oct. 19, 2025
Dark Matter Dilemmas, Betelgeuse's Fate & the Mysteries of Lagrange Points
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Sponsor Details:
This episode is brought to you with the support of NordVPN....enhance your online privacy with the best in the game. To get our special Space Nuts price and bonus deal, visit www.nordvpn.com/spacenuts or use the code SPACENUTS at checkout.
Q&A Edition: Dark Matter, Betelgeuse, and Lagrange Points
In this fascinating episode of Space Nuts, hosts Andrew Dunkley and Professor Jonti Horner tackle a variety of listener questions that delve into the mysteries of the cosmos. From the enigmatic nature of dark matter and its interactions with black holes to the potential explosion of Betelgeuse and the intriguing concept of Lagrange points, this episode is packed with thought-provoking insights and scientific discussions.
Episode Highlights:
- Dark Matter vs. Black Holes: Andrew and Jonti explore the relationship between dark matter and black holes, discussing whether dark matter can be 'eaten' by black holes and the implications of such interactions for our understanding of the universe.
- Betelgeuse's Fate: The hosts address a listener's question about the distance of Betelgeuse and what it means for us if it were to explode. They explain how light travel time affects our perception of cosmic events and the philosophical implications of observing the universe.
- Lagrange Points Explained: Mark's inquiry leads to a detailed explanation of Lagrange points, their stability, and how they function within the gravitational dynamics of celestial bodies. Jonti provides a compelling analogy to help visualize these unique gravitational wells.
- Kordeski Plasma Clouds: The episode wraps up with a discussion on the Kordeski clouds, two large dust clouds located at the Earth-Moon Lagrange points. The hosts delve into their transient nature and the challenges faced in confirming their existence.
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, X, YouTube Music Music, Tumblr, Instagram, and TikTok. 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.
Got a question for our Q&A episode? https://spacenutspodcast.com/ama
Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts-astronomy-insights-cosmic-discoveries--2631155/support.
This episode is brought to you with the support of NordVPN....enhance your online privacy with the best in the game. To get our special Space Nuts price and bonus deal, visit www.nordvpn.com/spacenuts or use the code SPACENUTS at checkout.
Q&A Edition: Dark Matter, Betelgeuse, and Lagrange Points
In this fascinating episode of Space Nuts, hosts Andrew Dunkley and Professor Jonti Horner tackle a variety of listener questions that delve into the mysteries of the cosmos. From the enigmatic nature of dark matter and its interactions with black holes to the potential explosion of Betelgeuse and the intriguing concept of Lagrange points, this episode is packed with thought-provoking insights and scientific discussions.
Episode Highlights:
- Dark Matter vs. Black Holes: Andrew and Jonti explore the relationship between dark matter and black holes, discussing whether dark matter can be 'eaten' by black holes and the implications of such interactions for our understanding of the universe.
- Betelgeuse's Fate: The hosts address a listener's question about the distance of Betelgeuse and what it means for us if it were to explode. They explain how light travel time affects our perception of cosmic events and the philosophical implications of observing the universe.
- Lagrange Points Explained: Mark's inquiry leads to a detailed explanation of Lagrange points, their stability, and how they function within the gravitational dynamics of celestial bodies. Jonti provides a compelling analogy to help visualize these unique gravitational wells.
- Kordeski Plasma Clouds: The episode wraps up with a discussion on the Kordeski clouds, two large dust clouds located at the Earth-Moon Lagrange points. The hosts delve into their transient nature and the challenges faced in confirming their existence.
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, X, YouTube Music Music, Tumblr, Instagram, and TikTok. 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.
Got a question for our Q&A episode? https://spacenutspodcast.com/ama
Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts-astronomy-insights-cosmic-discoveries--2631155/support.
WEBVTT
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Hello again, thank you for joining us on Space Nuts
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Q and A edition. This is where we answer audience questions,
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or at least we read them out and pretend we
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know what.
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We're talking about.
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Today we will be answering questions about dark matter versus
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a black hole. It's a titanic struggle.
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Who would win.
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We are also going to discuss the demise of beetlejuice
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or beetlegeis, depending on how you like to pronounce it.
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We have a question about lagrange points and the Cordeleski
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plasma clouds question has.
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Come up from a YouTuber.
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We'll deal with all that right now on Space Nuts.
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Fifteen second Channel ten nine ignition Squench Space Nuts or
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three two.
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Space nuts as.
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And I reported Neils good.
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He's back again for more.
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Has done all the research, has all the answers to
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all the questions, except for those four. It's Johnny Horner,
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professor of astrophysics at the University of Southern Queensland.
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Johnny, Hello, I'm good afternoon.
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How are you doing.
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I'm all right.
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How are the renots going at your place?
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Well, not too bad. I think they've clocked off for
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lunch at the minute, so we might get away with
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it on I'm waiting for my other doctor insists I
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pay attention to her. Are you yes?
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Dogs do that? Yes, indeed they do.
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All right, let's answer some questions. Firstly, we've got a
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question from Howard. He said, first, I should say that
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I think dark matter is going to end up as
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a follergiston? Is that the word of our times?
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Sorry? Flodgist?
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Could be that of our times, a substance dreamed up
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to resolve an otherwise unsolvable problem and later discarded as
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science advances. But even so, here's my question. Since gravity
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seems to be the only force that interacts with dark matter,
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what happens when a black hole, the ultimate source of gravity,
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comes into contact with dark matter? Does it eat it?
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And if so, what happens? And if not, why not?
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I do?
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We've had questions of similar style and ilk before, and
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I can't remember what Fred said, but I think it
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said doesn't matter, you know, because dark matter? And yeah,
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but I'm sure you've done your homework, because I didn't.
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I never did homework as a kid, so why would
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I start now?
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Well, there seems to be evidence that homework is fairly pointless. Such, yes,
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my Apartner's a primary teacher, and you know, I think
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if she had her where, kids wouldn't have any homework,
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and at least until you're fairly well through secondary school,
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it doesn't seem to serve a purpose other than making
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some parents feel like their kids are getting properly worked,
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you know. So, but onto something that I actually have
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expertise in, rather than being talking about teaching what I
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clearly done that much, is a real interesting one. It's
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I get what you mean with the flogist, and I
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think possibly dark energy, i'd argue, is a bit more
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of a flogist and thing than that matter at this stage,
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because it's very clear that there is mass out there
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that it's having an effect but we can't see. And
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that's fundamentally what dark matter is. We can add up
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all of the mass of all of the things that
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we can see in the forms of dust and gas
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and stars and all the rest of it, and the
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gravitational pull within galaxies, particularly as you get further out
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into galaxies, is more significant than can be explained by
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the luminous material art and that's where dark matter comes from,
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and we see its effects even if we don't see
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it in I guess just the same way as back
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in the eighteen hundreds, astronomers saw the effects of Uranus
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of Neptune's gravity perturbing the orbit of Uranus as it
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went round the Sun, and we detected Neptune indirectly. And
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then people said, only point you tell it's goope here,
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because it must be a planet in this part of
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the sky pulling Urinus around and low, and behold, we
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found it. And this is fairly fundamental to me as
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an exoplanet science person, in that the vast majority of
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planets we found around o the cells we found indirectly.
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We see a star doing something unexplained, We see it
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winking or we see it wobbling, and we in further
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presence of a planet as an explanation for that unexplained behavior.
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And when you rule out all the other explanations, someone
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that's left as a planet, and Bob's your uncle. You've
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added one to the Italian. Like we said in the
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earlier episode, we've now passed six cells, and so whoopy
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for us, we're doing really well. So there's a lot
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of evidence that dark matter is a thing, and what
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it is nobody really knows. There's been a lot of speculation,
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but what seems to be the case is that dark
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matter is something that interacts through gravity but doesn't interact
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with anything else. It doesn't interact with light. It doesn't
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impede light because we see dust blots light, so dust
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is not dark matter. So what happens, Well, if dark
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matter interacts with gravity in just the same way as
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normal matter, then it will interact with a black hole
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in almost the same way as normal matter. And they
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almost said a little asterisk. I'll come to in a minute.
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What that means is that if something gets close enough
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to a black hole to be within its event horizon,
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then that means it would have to travel faster than
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the speed of light to escape from the gravitational pull
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of the black hole. So it's effectively been nombed. And
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you've got black holes being the pack man of the
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universe that just go around gobbling everything up. Once it
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is gobbled up, it doesn't matter if it's dark matter
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or normal matter. It's been nombed and it just adds
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to the mass of the black hole. And I guess
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the black hole is a bit like the ball, and
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it's your individuality. Indistinctiveness has been added to our own
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and the dark matter has been nombed in just the
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same way it would have been with normal matter. So
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from that point of view, there is actually no problem.
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We'd expect dark matter to be eaten and to stay eaten.
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There are suggestions that the supermassive black holes like the
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one we've got at the middle of the Milky Way
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are only able to be formed if that matter exists,
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and even more normal mass black holes have a restriction
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on the amount that they can eat. It's almost like
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the celestial equivalent of a gastric band or something like that.
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It's something called the Eddington limit. Material falling into a
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black hole, that is normal matter as it falls in
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gets accelerated, gets heated up in its light. And if
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you've got a black hole eating a lot of stuff,
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there's a lot of material falling and emitting incredible aunts
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of radiation. They can essentially push away or the matter
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around the black hole and force it to stop eating,
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effectively putting a limit on the amount that it can
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devour at any given time. And you do get things
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that are eating at what's called super Eddington rates, but
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that's where something's essentially pushing material in so quickly that
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it overcomes that effect. So I guess it's a bit
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like saying you can only drink so much water because
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you can only swallow so much. But if somebody shoves
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a fire hose in your mouth, the water's going to
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go somewhere. That's kind of that situation. But that puts
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a limit on how much a black hole can eat
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at a given time. At the pace at which can
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devour matter, dark matter doesn't interact with like al radiation
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or anything like that, so the Eddington limit doesn't apply
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because a black hole shining like a searchlight will not
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impede the motion of dark matter one little bit. And
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so there is an idea that actually dark matter is
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a more effective food for black holes and normal matter
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because dark matter circumvents the Gasrick band. It circumvents this
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Eddington limit that prevents a black hole from eating to excess,
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and that may actually have been a significant part of
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how the supermassive black holes that we get in the
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middle of galaxies actually got their start where they got
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their start aided by dark matter. And so it's a
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really interesting question because I had not really thought of
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this until Howard's question. Came through and added a bit
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of reading around. But it's actually one of these scenarios
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where dark matter, it seems, is a help to black
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holes rather than a hindrance, and therefore may help to
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explain why the universe is and where that we see
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it today, beyond just explaining the rotation curves of galaxies
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and things like this, which is why it was hypothesized
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in the first place.
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Okay, so you do believe there's interaction between dark matter
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and black holes.
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Of course, Yeah, and sorry, of course the sounds to dismissive.
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The reason that it's in, of course, is that dark
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matter interacts with gravity. That's fundamentally how we found it
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in the first place. And therefore, if it falls into
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a black hole, it behaves like any other kind of
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matter from the point of view gravity.
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And so therefore, and I.
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Mean, there are some suggestions that black holes are a
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significant component of dark matter.
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Yes, we can only see them when they're feeding.
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If they're not eating anything, we have no indication of
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black holes there other than its effect on the mass
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around it. You know, light gets bent around it and
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all the rest of it. Yeah, some component of dark
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matter may well be primordial black holes. That's one of
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a suggestion.
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Yeah, there's still so much to learn. We don't know
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much at all, although they also I think if I
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recall correctly say that dark matter clusters in around galaxies
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and around concentrated points, it's much thinner where the universe
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is emptier.
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Is that right?
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And that kind of makes sense as well, because if
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dark matter is feeling the effects of gravity like everything else,
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the same things that would have pulled an excess of
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visible matter together to farm galaxies would have brought together dark.
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Matter as well.
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And there is this discussion that galaxies have dark matter
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halos around them. So the rotation curves of galaxies are
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evidence for dark matter within those galaxies, meaning that there
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is more mass interior to a certain distance from the
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middle of the galaxy than we can account for by
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what we see. That means that together rotation happening quicker
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because it's more master left on, more gravitational pulse or
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faster rotation. But the massive galaxy clusters, in terms of
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how the galaxies are interacting with each other and how
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they're moving within the clusters, the mass within the cluster
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has to been bigger than the masters that the galaxies
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seem to have from the visible material, even accounting for
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the dark matterrhithm causing their rotation speeds to be higher.
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And that's suggesting that that matter is also in a
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halo around the galaxy, given that galaxy even more muster
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even more.
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Yes, it is so fascinating.
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And Flogiston was a hypothetical fire like element once thought
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to be contained within combustible bodies and released during combustion,
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a theory proposed by Johann Beecher, and it's an outdated
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theory that was eventually disproved by Antoine Levosier through his
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experience with oxygen, which demonstrated that burning is a chemical
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reaction involving the combination of a substance with oxyde, not
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the release of flogiston. There you are, all right, Howard,
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Thank you so much for a great question. Let's take
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Now back to the show.
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