Feb. 10, 2025
Cosmic Queries, Jovian Mysteries & Martian Quakes: #494 - The Great Space Q&A
Space Nuts Episode 494: Radiation Around Jupiter, Light Refraction, and Brown Dwarfs
Join Andrew Dunkley and Professor Jonti Horner in this thought-provoking Q&A edition of Space Nuts, where they tackle a variety of intriguing questions from our...
Space Nuts Episode 494: Radiation Around Jupiter, Light Refraction, and Brown Dwarfs
Join Andrew Dunkley and Professor Jonti Horner in this thought-provoking Q&A edition of Space Nuts, where they tackle a variety of intriguing questions from our listeners. From the complexities of radiation surrounding Jupiter to the effects of light refraction in space, and the mysteries of brown dwarfs, this episode is packed with insights that will expand your understanding of the cosmos.
Episode Highlights:
- Radiation Around Jupiter: Fenton from Minnesota dives deep into the types of radiation emitted by Jupiter and the charged particles from its volcanic moon Io. Jonti explains the implications for spacecraft navigating this hazardous environment and how these particles interact with Jupiter's magnetic field.
- Light Refraction and Redshift: Kerry from Mount Gambier wonders about the impact of gas clouds on light refraction and redshift. Jonti clarifies how light behaves when passing through these clouds and reassures listeners that the redshift measurements remain largely unaffected.
- Brown Dwarfs and Binary Systems: Nigel from Brisbane asks whether binary brown dwarfs are destined to collide. Jonti discusses the dynamics of binary systems and the various factors that could lead to such an event, while also exploring the potential for merging to create a star.
- Marsquakes and Planetary Structure: Buddy poses a fascinating question about the origins of marsquakes and whether Mars could eventually break apart. Jonti unpacks the geological processes at play on Mars and the role of Jupiter in shaping the asteroid belt.
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 radiation around Jupiter and its implications
10:30 - Light refraction and its impact on redshift
18:00 - Insights into binary brown dwarfs and potential collisions
26:45 - Marsquakes and the internal structure of Mars
30:00 - Closing thoughts and listener engagement
✍️ Episode References
Jupiter's Magnetosphere
https://en.wikipedia.org/wiki/Magnetosphere_of_Jupiter
Marsquakes Research
https://mars.nasa.gov/marsquake/
Brown Dwarfs and Binary Systems
https://en.wikipedia.org/wiki/Brown_dwarf
Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts--2631155/support.
Join Andrew Dunkley and Professor Jonti Horner in this thought-provoking Q&A edition of Space Nuts, where they tackle a variety of intriguing questions from our listeners. From the complexities of radiation surrounding Jupiter to the effects of light refraction in space, and the mysteries of brown dwarfs, this episode is packed with insights that will expand your understanding of the cosmos.
Episode Highlights:
- Radiation Around Jupiter: Fenton from Minnesota dives deep into the types of radiation emitted by Jupiter and the charged particles from its volcanic moon Io. Jonti explains the implications for spacecraft navigating this hazardous environment and how these particles interact with Jupiter's magnetic field.
- Light Refraction and Redshift: Kerry from Mount Gambier wonders about the impact of gas clouds on light refraction and redshift. Jonti clarifies how light behaves when passing through these clouds and reassures listeners that the redshift measurements remain largely unaffected.
- Brown Dwarfs and Binary Systems: Nigel from Brisbane asks whether binary brown dwarfs are destined to collide. Jonti discusses the dynamics of binary systems and the various factors that could lead to such an event, while also exploring the potential for merging to create a star.
- Marsquakes and Planetary Structure: Buddy poses a fascinating question about the origins of marsquakes and whether Mars could eventually break apart. Jonti unpacks the geological processes at play on Mars and the role of Jupiter in shaping the asteroid belt.
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 radiation around Jupiter and its implications
10:30 - Light refraction and its impact on redshift
18:00 - Insights into binary brown dwarfs and potential collisions
26:45 - Marsquakes and the internal structure of Mars
30:00 - Closing thoughts and listener engagement
✍️ Episode References
Jupiter's Magnetosphere
https://en.wikipedia.org/wiki/Magnetosphere_of_Jupiter
Marsquakes Research
https://mars.nasa.gov/marsquake/
Brown Dwarfs and Binary Systems
https://en.wikipedia.org/wiki/Brown_dwarf
Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts--2631155/support.
WEBVTT
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Hi there, thanks for joining us.
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This is a Q and a episode of Space Nuts.
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That's me.
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That means says questions that people ask and there are
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answers that I do not give. Someone else will do that.
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But coming up we're going to We're going to get
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to something we planned to do last week, but it
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just it was a big question which required a lot
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of effort and a lot of answers and a lot
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of research. We just sort of ran out of time.
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So we'll get that one done today. From Fenton, Kerry
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is asking about the effects of light by dust clouds
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or the effects on light. Nigel is talking brown dwarfs
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and Paddy mars quakes. That's all coming up in this
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edition of Space Nuts fifteen in Channel ten nine ignition.
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Squench Space Nuts or three.
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Two Space nuts as and I report it Neils Good.
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Joining us again is Professor John D. Horner, who is
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a professor of astrophysics at the University of Southern Queensland.
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A horrible part of the world, but somebody's got to
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live there, haven't they.
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Johnny.
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Absolutely, it's drudged. It's glorious here at the minute, but
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we could do with a bit of rand that said,
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giving the amount of rent, that's something elsewhere in Australia.
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I'm probably gloved that we're not getting that. Yes, much
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much further north than you are.
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Up around the North Queensland Townsville area, it's been bucketing
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down and they've had some big floods.
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Big flood that my head around the concept of getting
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two meters of ren in a couple of days.
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Yeah, I can't. Yeah, I mean a big rain for
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us is eighty millimeters in an hour. Yeah, that's a
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big rain. I think the biggest I've ever experienced here
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was two hundred millimeters over a weekend. Yeah, that was
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some years ago and that caused big floods across the area.
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But yeah, the numbers they're talking up there are astronomical
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and your power thoughts go out.
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To everybody affected.
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Now we should get straight into Fenton's question because it's
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a big one, and we'll be back in about two
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or three als once he's finished.
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Hey, fer Andrew, this is Fenton speaking to you from
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Saint Paul, Minnesota, and you're asked on the other side
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of the planet. I got some questions for you today
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about radiation. Now, right now, we have spacecraft that are
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underway to Jupiter, and there's a lot of fretting about
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what's going to happen and how to get them to
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avoid radiation blasting off Jupiter. Well, we have three types
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of radiation alpha, beta, and gamma. If you wish, I'll
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leave that up to you to explain that to the audience.
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My question to you here is what type of radiation
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is that that's coming off of Jupiter.
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Is it just the alpha particles? In other words, just
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protons hydrogen atoms. Now here we go on to ion.
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Io is also blasting off particles from its surface as
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a result of it being volcanic. So I guess that
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means we have these charged particles coming off. Do you
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want to also include them in the term of radiation?
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Now I was also interested in what types of particles
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they have. These are metals apparently, for example, if it
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were iron then and if it were charged, then iron
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can be magnetic and that means it could possibly be
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interactive with the magnetic field of Jupiter. So where's that
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stuff going? Is it sticking along Jupiter? Is it heading
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off beyond Jupiter? Is it landing on some moons? And lastly,
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I want to ask you about a practical application for
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this now here back on Earth, we can deposit metal
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ions from the gas phase onto substrates and that has
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a lot of very useful applications. It's pretty expensive too,
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So what happens when we put a substrate in a
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way in blocking those metal ions or metal metal particles
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they are coming off of aio? Could we use that
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to deposit metals onto a surface? Just a thought. I'd
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love to hear what you think about it and what
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where you take my questions?
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Oh a great week? Why no?
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Thank you? Fenton? Always always thinking deeply?
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Is Fenton?
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These questions are always multifaceted, and that one is no exception.
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So we started off talking about the different types of
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radiation and which which kind is it's coming off Jupiter.
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Yeah, I'll dive through this set BA set, But what
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I will do initially is it's a fabulous question. There's
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a lot in here I'd recommend for the interested listener
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who wants to dig into Jupiter's.
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Environment a little bit more.
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It's a Wikipedia article about Jupiter's my magnetosphere, which is
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literally magnetosphere of Jupiter, which is incredibly thorough and detailed
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and goes into some of the things we're about to
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discuss in more detail than I will do. Now, Wikipedia's
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a fluid resource. It can be changed, so your experience
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may vary.
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But what we.
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Typically typically see is for astronomy and space subjects. They
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are not controversial, but there's enough people out there who
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are incredibly passionate about it that when an error creeps in.
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It gets fixed very quickly.
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So whilst it's not the most reliable resource, it can
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be very very good. So I do recommend looking into
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that if you want more details on some of the
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stuff we'll discuss, but I'll try and pick through the
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many things Fenton said there in turn, just to try
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and work through them if that makes sense, and hopefully
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that will be helpful. Fenton, if you're listening in. Firstly,
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when you mentioned three types of radiation, you're talking there
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about alpha, betre, and gamma, which are the kinds of
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radiation that people talk about being produced by radioactive decay.
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And they are three kinds of radiation, but they're not
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the entirety of what radiation is, and they're actually different
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kinds of thing anyway. So alpha radiation is essentially helium nuclei,
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so two protons and two neutrons stuck together coming outwards.
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That's fairly substantial particle. So that's radiation as a particle.
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So particle that's ejected in this case from a radioactive process,
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flung outwards with a certain speed, and it's carrying energy
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from one place to another in the form of the
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particle itself moving at that speed from A to B.
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Beta radiation is electrons essentially, so much less massive, typically
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traveling much faster, that are again produced by radioactivetycare quite
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often other processors. Alpha particles are positively charged because you've
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got protons in but no electrons. Beta radiation is negatively
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charged because it's got electrons in, and then gamma radiation
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is very high energy electromagnetic radiation. So that's the top
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end of the electromagnetic spectrum, which also features light that
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I'm using to look at Andrew whileye waffle away here
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and see him nodding unwisely. So there are different bits
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of radiation. Essentially, at the very simplest end, you talk
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about radiation just being energy being moved from one place
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to another, and that can be done by waves or particles.
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So a very extreme stretch, you could probably argue that
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when you go outside and you turn the hose pipe
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on and you have a jet, and that water is
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going from one pleasure another. That's form of radiation. It's
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energy being moved from one place to another. So there's
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a lot of different ways that energy can be transferred
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in this way, and light in its many forms is
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one of them. So that's everything from gamma rays at
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the high energy end to radio waves at low energy end,
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with optical and microwaven infrared in the middle somewhere. So
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there's a lot too radiation there. Now there's a couple
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of things happening with Jupiter. Firstly, you talk about the
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radiation coming off Jupiter. Now, if you think about jupe
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to the planet itself, it's sometimes said that Jupiter emits
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more energy than it receives from the Sun, and that's
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the leftover from Jupiter's form a from all the material
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coming into it, the gravitational relaxation of it. Essentially, that
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is energy emitted in the form of electromagnetic radiation. So
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light essentially of various wavelengths, it will emit as what
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we call a black body, so it'll have one particular
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color of light.
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That it emits.
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Happen most strongly, and whether you go blue or or
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reader of that color, it will emit more weakly as
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you go further away. So that's due to emitting energy,
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but it's also surrounded by an incredibly intense magnetic field,
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much stronger than the Earth's. So hop to the Earth briefly.
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One of the challenges that people face when the fly
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satellites around the Earth is that there are these radiation.
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Belts around the Earth called the Van Allen Belts, and.
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They were proposed just prior to the space age and
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then detected by the first satellites. What's going on there
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is that the Earth has a magnetic field around it
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that interacts with the magnetic field of the Sun and
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the rest of.
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The Solar system.
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And we've got this area around the Earth called the magnetosphere,
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and the magnetosphere if sculptured and shaped by what's going
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on else.
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Now.
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In the case of the Earth, you've got solar radiation
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in the form of charged particles as part of the
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solar wind buffeting against our magnetosphere, penetrating in. And when
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you have particles that have charge, whether they're positively or
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negatively charged, they interact with magnetic fields, so they will
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follow the direction of the magnetic field lines. And now
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our magnetosphere shields us from a lot of the radiation
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like that because it goes around the Earth rather than
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hitting us. But some of the radiation, in the form
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of charge particles that penetrates the ath magnetic field then
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gets trapped in the magnetic field in these belts that
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we call the Vanalon belts, which are areas where you
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have a lot of charge particles moving around at high
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speed trapped in these belts around the Earth between a
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few hundred and a few tens of thousands kilometers above
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the Earth's service. Those are areas where if you fly
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a spacecraft through there, there's a lot of charge particles
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crashing into your spacecraft at high speed that can damage
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the electronics of circuitry in particular very sensitive to this
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and gradually damage your spacecraft and take it out of operation.
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So that's the radiation environment around the Earth, and they're
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try and avoid going through the viole and belts as
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a result. Jupiter's the same. Jupiter has a much more
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intense magnetic field, so it can have a much more
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significant area of radiation belts, and those radiation belts correspond
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roughly with the location of the large moons, particularly Europa
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and Io. So in that area, when you're a spacecraft
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moving through there, you're moving through a soup of high
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speed charged particles that are continually bombarding your spacecraft, degrading it,
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damaging it, and of course they're particularly damaging to the
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electrical component ry. So you want to spend as little
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time as you can there, and that's essentially what the
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concern is for the scientists who are sending spacecraft to Jupiter.
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So that's what's going on there. Added to that, though,
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you've got the volcanism from Io, which Fenton mentions, and
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Fentin's quite right, always erupting continuously volcanically into that radiation
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environment around Jupiter, adding I think some quotes say up
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to one thousand kilos per second of new material into
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that environment. Now, the atoms that are launched out of
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Io by this volcanism are things like sulfur, oxygen, sulfur dioxide,
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all these kind of things that initially are molecules and
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atoms but are very quickly ionized, so they have an
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electron knocked off colliding with the charge particles, which certainly
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means you've got sulfur ions, oxygen ions, sodium ions, all
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floating around in a magnetic field, so I always dumping
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even more charged particles into that radiation. Bell those charge
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particles from ioincidentally flow along Jupiter's magnetic field lines and
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crash into the Jovian poles, creating hot spots of aurora.
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So they are aurora on Jupiter that are directly linked
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to Io and to a lesser extent, Europa and Ganymat.
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You can see them if you look at aurora maps
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of Jupiter that are spacecraft to seven. So you get
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this flux Taurus connecting Io to the poles of Jupiter,
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which is the charged particles flowing along the magnetic fielands
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and crashing into Jupiter's poles. So that's how Io's chipping,
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and it's just adding more soup to the mix, essentially
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moving the metals.
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Being magnetic. I'm trying to get through all the points.
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Yeah, I just thought it was fascinating that that there's
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such an effect happening around Jupiter, and like the like,
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we see similar effects with the Aurora borealis and the
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Aurora stralla, but different reasons, same effect, So you'll have.
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Aurora on Jupiter that had caused the same way as
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the aurora on Earth. But you also have Io Europe
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and Ganymede cooking their own aurora as well, So it's complicated.
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I think.
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With the metals being magnetic, there's a couple of things
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there to mention. You're entirely right that metals like iron
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and nickel can become permanently magnetized, and this is something
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called ferromagnetism. Now I'm not a specialist on magnetism any means,
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And one of the common jokes in astronomy is if
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you want to ask a question at a conference, it's
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almost certainly have you considered magnetic fields? And the answer
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is almost certainly no, because it's just complicated. There's actually
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