Feb. 17, 2025
Alien Signals, Bone Density & Cosmic Disks: #496 - The Great Space Q&A Returns
Space Nuts Episode 496: Life on Other Planets, Centrifugal Forces, and Bone Density in Space
Join Andrew Dunkley and Professor Jonti Horner in this thought-provoking Q&A edition of Space Nuts, where they tackle some of the most intriguing...
Space Nuts Episode 496: Life on Other Planets, Centrifugal Forces, and Bone Density in Space
Join Andrew Dunkley and Professor Jonti Horner in this thought-provoking Q&A edition of Space Nuts, where they tackle some of the most intriguing questions from our listeners. From the possibility of detecting life on distant planets to the fascinating dynamics of centrifugal force, and the effects of zero gravity on bone density, this episode is brimming with scientific insights that will spark your curiosity about the universe.
Episode Highlights:
- Detecting Life on Distant Planets: Ron's compelling question leads the discussion on whether scientists in other solar systems could identify life on Earth using current technology, and vice versa. Jonti elaborates on the challenges and potential methods for detecting life beyond our planet.
- Spheres vs. Disks: Dean asks why celestial objects form as spheres while others appear as disks. Jonti explains the physical processes at play, including hydrostatic equilibrium and angular momentum, shedding light on the fascinating shapes of stars, planets, and galaxies.
- Bone Density in Space: Ann's insightful question about calcium loss in astronauts prompts a deep dive into the effects of microgravity on bone health. Jonti shares findings from recent studies and discusses the implications for long-term space missions.
- Centrifugal Force Explained: Aussie Dean's inquiry about the nature of centrifugal force and its measurement leads to a discussion on reference frames and how they relate to our understanding of gravity and motion on Earth.
For more Space Nuts, including our continually 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.
00:00 - Introduction to the episode and topics
02:15 - Discussion on detecting life on other planets
10:30 - Exploring the shapes of celestial objects
18:00 - Insights into bone density loss in space
26:45 - Understanding centrifugal force and reference frames
30:00 - Closing thoughts and listener engagement
✍️ Episode References
NASA's Studies on Bone Density
https://www.nasa.gov/spaceflight
Hydrostatic Equilibrium in Celestial Bodies
https://en.wikipedia.org/wiki/Hydrostatic_equilibrium
Centrifugal Force and Gravity
https://www.physicsclassroom.com/class/circles/Lesson-2/Centrifugal-Force
Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts-exploring-the-cosmos--2631155/support.
Join Andrew Dunkley and Professor Jonti Horner in this thought-provoking Q&A edition of Space Nuts, where they tackle some of the most intriguing questions from our listeners. From the possibility of detecting life on distant planets to the fascinating dynamics of centrifugal force, and the effects of zero gravity on bone density, this episode is brimming with scientific insights that will spark your curiosity about the universe.
Episode Highlights:
- Detecting Life on Distant Planets: Ron's compelling question leads the discussion on whether scientists in other solar systems could identify life on Earth using current technology, and vice versa. Jonti elaborates on the challenges and potential methods for detecting life beyond our planet.
- Spheres vs. Disks: Dean asks why celestial objects form as spheres while others appear as disks. Jonti explains the physical processes at play, including hydrostatic equilibrium and angular momentum, shedding light on the fascinating shapes of stars, planets, and galaxies.
- Bone Density in Space: Ann's insightful question about calcium loss in astronauts prompts a deep dive into the effects of microgravity on bone health. Jonti shares findings from recent studies and discusses the implications for long-term space missions.
- Centrifugal Force Explained: Aussie Dean's inquiry about the nature of centrifugal force and its measurement leads to a discussion on reference frames and how they relate to our understanding of gravity and motion on Earth.
For more Space Nuts, including our continually 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.
00:00 - Introduction to the episode and topics
02:15 - Discussion on detecting life on other planets
10:30 - Exploring the shapes of celestial objects
18:00 - Insights into bone density loss in space
26:45 - Understanding centrifugal force and reference frames
30:00 - Closing thoughts and listener engagement
✍️ Episode References
NASA's Studies on Bone Density
https://www.nasa.gov/spaceflight
Hydrostatic Equilibrium in Celestial Bodies
https://en.wikipedia.org/wiki/Hydrostatic_equilibrium
Centrifugal Force and Gravity
https://www.physicsclassroom.com/class/circles/Lesson-2/Centrifugal-Force
Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts-exploring-the-cosmos--2631155/support.
WEBVTT
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Hi there, Andrew Dunkley here, Thanks for joining us on
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a Q and A edition of Space Nuts, and coming up,
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we're going to answer a question from Ron. He wants
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to know if we could see a planet that sustains life,
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would we know it? And vice versa. If there was
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an alien race out there and they spotted Earth, would
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they know we are here? Good question. Dean is a
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bit confused about spheres versus discs. Why does it happen?
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Why aren't they all spheres or all discs? And has
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a brilliant question love this one about bone density in
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space and some of the problems that are associated with
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being in zero gravity for long periods of time, and
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Dean two, it's not the same. Dean is asking us
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about centrifugal force. We'll cover all that in this episode
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of Space.
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Nuts fifteen, Channel ten nine.
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Ignition Space Nuts Guy or three spaces hasn't actually bought it?
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Neils Good Here he is again.
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Professor John T. Horder, Professor of estrophysics at the University
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of Southern Queensland.
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Johnty, Hello, Hey, how are you going?
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I'm all right? A question without notice?
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Yes?
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Did you ever sort of have people review at school?
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Like John ty Horner said in the corner eating his
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Christmas pie, down came the comet that made Johnty vomit,
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and now he only is flies.
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Oh that's brilliant. That would have been far more pleasurable
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than marchall skill experience. It's probably not worth getting into
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too depressing a thing, but up until I got to
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Upper Clamento University, I had a horrendous, horrendous time at
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school because I was I grew up in a very
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working class area, lost social economic area with hugely high unemployment,
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neurly the minor strikes in the eighties, and I was
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an only child, so I'm not necessarily blessed with the
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best social aptitude particular that age. But I was smart
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enough to be very smart, but not smart enough to
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realize that there were the right way and the wrong
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way to go about that. So I had a horrible,
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horrible time for the twelve years at school. In terms
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of bully I was catastrophically bullied, but you know, it
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mainly who I am today, so I'm not going to
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complain too much about it. But yeah, it's a curse
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of having aspiration and the curse of being smart in
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an area where that wasn't a common thing. You know,
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a lot of empathy for the kids who went to
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school with because you're talking about an area where many
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of them didn't have any family members who were employed
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because of what was going on. There was a huge
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epidemic of men taking their own lives because of all
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the things that were going on. So it was a
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pretty rough time, a pretty rough place. But such as
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life unfortunately, you know.
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Yeah, yeah, I certainly had my share of bullying at school,
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and yeah, not often, wasn't an every day thing. It was,
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I suppose, looking back, reasonably rare. But it never sits well,
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it's it's a horrible thing.
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At least, he says. Nowadays, there is more being done
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to counter and more al wavers of it, because you know,
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the impression back when I was at school was he
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just needed to manna, which is an awful phrase, and
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everybody has to deal with it. It's a formative experience,
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and he just couldn't tell us. As long as you
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weren't getting naive to something it were, they weren't interested.
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I used to talk to my boys about it and
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ask them how they were going, and they always said, no,
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we never had any trouble, but then teachers would tell
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me otherwise, so they're obviously not keen to talk about it.
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But my middle son, who was always very tall through school,
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he was he tired above all the other kids. I
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think he was the second tallest kid in his year
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and in the school in general. And I said to
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him one day that you get bullied, and he went no,
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because he was big. He was a big kid, and
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no one, no one went near him. His height was
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actually a good defense mechanism. It's funny how it works out.
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But there's a lot about anthropology, I suppose when.
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You're talking about it. It's all interesting about the edges
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in which kids develop awareness of self and the edges
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at which they develop empathy and kindness and all those
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kind of things in a specific center rather than the
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general sense. It's really interesting.
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Yeah, it is, all right. Let's deal with some questions,
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and our first question comes from Ron. He said, if
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scientists in a distant solar system were searching for exoplanets
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using the same technology that we're using, and if they
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were to observe our planet, would they be able to
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tell with any degree of certainty that there was life
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here or Conversely, if we were to observe an exoplanet
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that's exactly like Earth, teeming with carbon based life and
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perhaps with an advanced civilization modifying their atmosphere, which we
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talked about in the last could we tell that there's
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life there? Thanks? Ron, great question, Ron, We've had questions
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like it before, but I just love this topic, so yeah,
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we'll do it again. And Johnty hasn't had to answer
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this one before, so I thought it'd be interesting to
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get his take on it.
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Well, it's a fabulous question, and I mean, the sad
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answer is we're not quite there yet. So if we
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were looking at the Solar System from around another star,
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depending on which method we use, we'd be able to
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find Jupterum, probably Saturn, but we'd have to observe for
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a very long time to measure the wobbles for them.
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So we need to observe the Sun for a decade
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or two to pick up DUP from Saturn. Everything else
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we wouldn't be able to find. Now, if we have
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something like tests the Transit eight Planet Service that'llite looking
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at our Solar system, there's a very small chance it
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might pick up the Earth, our venus but test typically
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it starts for twenty seven days. The Earth takes three
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hundred and sixty five days to around and would take
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over sixteen hours to transit, so the old of catching
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a transit a pretty much nil. So we're not there yet.
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We are getting better, and as we talked about in
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the other episode, we're getting to the point where we
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can find planets that are a bit bigger than the Earth,
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but on all bits that are comparable to the Earth.
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Around stars like the Sun. We can find planets smaller
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than the Earth around dim little red dwarf stars using
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the transit method, but that's partly because as planets are
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so close they're stars, they're going around really quickly. So
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the upshot of all that is, if we were orbiting
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another star looking back at the Solar System, I think
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we could only confidently detect one or two planets. The
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Earth would probably be the third planet that would be
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discovered as a technology got better, because it's the biggest
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of the terrestrial planets. But it would depend a little
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bit on your line of sight because the treasural planets
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are all slightly tilted to each other, So if you're
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going to find them through the transit method, the likelihood
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is only one of them will transit and the others won't.
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In the radial velossy method, you'd pick out Jupter and Saturn,
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but you'd struggle for anything else. Eventually you get there,
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but you'd need technology a bit better than ours. So
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we're not at the point of finding the planets yet,
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never mind finding the life on them. But that's like
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the next step in the journey. We've only had thirty
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years of the exoplanet ere we're only in the first
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few decades have been able to do this at all,
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and the progress we've made is ugly astonishing, and I
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think within the next decade or two will routinely start
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being able to find planets that are Earth sized on
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Earth like orbits and to start looking for evidence of
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life on them. But that is going to be the
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hardest observations we've ever to carry out in terms of
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detecting life like us, so it's a slightly different proposition.
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So finding any evidence of life is going to be challenging.
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So people often talk about biomarkers, which is this concept
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that there are certain things you could look for that
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will be indicative of life. And we've talked about the
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possible detection of phosphene and venus atmosphere before. We've talked
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about stuff like the chicken soup experiment the Viking land
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did on Mars in the nineteen seventies, where they dug
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up some soil and put some soup on it, and
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so if it gave off gases, because they can be life,
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they use of nutrients. When you're looking at planets arounder
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the stars, there is no guarantee that life on those
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planets would have followed the same evolitary pathways as life
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on Earth. So a lot of the very specific biomarkers
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people propose there best on our knowledge of life on
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Earth because it's the only planet we know does have life,
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and it's the only example of life we've got. One
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of the examples here is something called the red edge,
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which is when you look at the spectrum of light
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from a planet, if the planet has a lot of
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plants on board that are using chlorophyll, chlorophyll absorbs incredibly
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strongly in the red, so you might see a feature
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in the red that is the signature of chlorophyll, and
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that will be an indication of plant life. The problem is,
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and again I'm not a biologist, so there's probably more
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to this than I'm going to say. In my simple
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version is that chlorophyll is an incredibly efficient compound for
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allowing plants to utilize the light like the light from
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our suck. But there are many other compounds that could
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do a similar job for stars of different temperatures that
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are there for different colors, so they put out the
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bulk of their light at slightly different wavelengths, And there's
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no guarantee that life on another planet would use chlorophyll,
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especially if that star was significantly different to the Sun,
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So the specific bymarker of the red edge from chlorophyll
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wouldn't work very well. Necessarily, it wouldn't be guaranteed to work,
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especially because it's also mimicked by the spectrum of olivine,
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which is a very common mineral, has a very similar appearance.
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But looking more generally for that kind of absorption feature
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in the spectrum that you can't explain any other way
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is one of the size people have looked for. So
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it's not so much case of looking for a specific thing,
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but rather for looking for something that is out of place,
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trying to explain it, and finding that the only explanation
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left is life. You're looking for something out of balance.
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So another good example is on Earth, we have oxygen,
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we have methane. Now, there's a lot of oxygen in
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the atmosphere, but that doesn't necessarily mean life, because there
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are chemical processes that can produce oxygen without life being involved.
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Similarly with a lot of methane in the atmosphere. And
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methane is a natural product of animal life. I my
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dog line next to me has been quite happily producing
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methae through the podcast because we've fed at some broccoli
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I think in a puppy food last night. So methane
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is produced by life, but there are also lots of
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natural ways it can produce. And you know, there's huge
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amounts of methane in the atmospheres of Urinus and Neptune,
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for example. So finding oxygen or finding methane doesn't necessarily
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mean life. There's a lot of other explanations, but the
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oddity with Earth is that we've got oxygen and methen together. Now,
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when you put oxygen and methne together, they react with
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each other a lot, and they react until all of
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one of them is gone. So the methane in this
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atmosphere has a really short residence time of only a
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century or a few centuries I think four hundred year
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before it's all gone. So you look at the Earth
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and it's got oxygen and methen together, which means something
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has to be producing new methane to replace the methen
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that's lost. Now, even that doesn't mean it's life, because
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volcanoes perished me fed. So what you then have to
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do is say, well, this is interesting. It could be life,
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it could be something else. Let's measure the methane over time,
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and if it's volcanoes, you'll get the methane falling off
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and a random time of volcano ups and there's a
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spike of methane and then it falls off again, and
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a random time later you get another spike. But when
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you look at methane in the Earth's atmosphere, it varies
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with the seasons. Volcanoes don't do that, so therefore that's
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an indication of life. So it's looking for that oddity
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that's out of place. There are a couple of things
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that would give away arguably technologically developed life, which doesn't
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necessarily mean intelligent life, as we're seeing in the political sphere,
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at the minute, but technologically developed life. One of them
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is chlorophylor of carbons, So the things that we were
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putting up into the atmosphere that devastated the layer. Yeah,
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we only know of those being produced by technology if
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there is no natural process that seems to produce them.
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Another is radio broadcasts. So any intelligent aliens within about
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eighty light years of us ninety light years of us
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now would see our broadcast. Now. The exact date of
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the first broadcast that we sent out that was strong
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enough to be detected from around the stars depends w
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you talked. It could have been the Berlin Olympics in
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nineteen thirty six, I think, or the coronation of Queen
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Elizabeth in nineteen fifty two. I think with it it was,
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and they usually held has been the first big broadcast
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that would have been detectable on an interstellar distance. What
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that means is that within a certain distance of the
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