April 12, 2026
Relativistic Beaming, Martian Waters & Cosmic Trash: The Space Nuts Q&A
Relativistic Doppler Beaming, Martian Water, and Fusion Confusion In this engaging Q&A edition of Space Nuts, hosts Andrew Dunkley and Professor Fred Watson dive into a variety of thought-provoking listener questions that explore the depths of...
Relativistic Doppler Beaming, Martian Water, and Fusion Confusion
In this engaging Q&A edition of Space Nuts, hosts Andrew Dunkley and Professor Fred Watson dive into a variety of thought-provoking listener questions that explore the depths of astronomy and space science. From the complexities of relativistic Doppler beaming in black holes to the intriguing evidence of water on Mars and the mysteries of nuclear fusion in the sun, this episode is brimming with cosmic insights and scientific clarity.
Episode Highlights:
- Relativistic Doppler Beaming: Ron from New York asks about the brightness differences in black hole accretion disks. Andrew and Fred explain how relativistic speeds affect light emission, leading to the phenomenon known as Doppler beaming and why we don't see the expected color shifts.
- Water on Mars: Sunny from California questions the geological evidence for water on Mars. The hosts discuss the findings from the Phoenix lander and the implications of briny water on the Martian surface, confirming that it was indeed water, albeit potentially different from what we know on Earth.
- Earth's Mass and Space Junk: Holt raises a fascinating question about how much material we can send into space before it impacts Earth's orbit. Andrew and Fred provide insights into the negligible mass we've launched compared to the Earth's total mass, reassuring listeners that our planet remains unaffected.
- Fusion Reactions in the Sun: Ken from Maroochydore seeks clarification on the fusion process in the sun, specifically regarding mass loss and binding energy. The hosts unravel the complexities of fusion, explaining how energy is produced and the significance of mass defects in nuclear reactions.
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WEBVTT
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Hi there, Thanks for joining us.
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This is a Q and A edition of Space Nuts
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where we talk astronomy and space science and we answer
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audience questions or we just say a lot of words
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that sound like answers, but then they'll check it later
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on the internet and realized we were just giving them
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an absolute.
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Loaded cod swallop.
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Coming up today, relative lp, you're not supposed to be
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talking yet. Relativistic relativistic Doppler beaming. What on Earth is
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that we're about to find out? Sunny has sent us
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an audio question about Mars water.
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Is it water? Was it water? Could it have been
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something else?
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Holt is asking how much stuff we can send off
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the planet before the planet sort of you know, starts
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to fall off itself and fusion reaction in the sun.
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We will dispel that confusion very very soon. On this
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episode of Space Nuts.
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Fifteen, Channel ten nine ignition Space Nuts or three two.
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Space Nurse and I reported Neil Good.
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Professor Fred Watson, a storm at large's here. You've already
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heard his voice. Hello Fred, Nice.
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To see you. Andrew. I'm always reminded of and you
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might know about this as well, even though our listeners
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are all too young to remember. But on the Goon
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Show there was once an episode where Eccles came on
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before he was supposed to. I had to make the
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comment do.
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I remember that? Yes, I'm.
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Which reminds me of a famous incident on ABC Radio
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where I worked for twenty two years, where a news
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reader was trying to do the bulletin but they were
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halfway through a live interview with Spike Milligan. Spike kept
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interrupting at the end of every sentence with and Spike
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Milligan and Spike Milligans. And so when the story finished,
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the newsreader said, Da Da Da Da da and Spike Milligan.
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He got He got fired for that. He got fired
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for that. It's one of the funniest pieces of radio
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you will ever hear. Look it up online. But he
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got canned.
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Probably yeah, old BBC days, probably, Oh well yeah, probably, well, yeah,
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the times have changed. Yes, Rather, let's get into some questions, Fred,
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and I've got our first one here from Ron, who
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is in upstate New York. He says, springs just around
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the corner. He says, hope all is well down under? Well,
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if you like wind, yeah it is, it's going great,
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and it's been pretty windy here lately. I have a
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question about relativistic Doppler beaming that we see on a
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black hole s accretion disc which causes the side moving
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towards us to be brighter than the side moving away
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from us. Why are we not seeing blue and red
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Doppler shifts in the color of the light in those
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respective regions. There's so much, and thanks so much for
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the great podcast. It is our pleasure. It is our pleasure.
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Thanks for the question, Ron, It's.
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A good question, and there's the answer, Jordy. Yeah, so
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we do. We do see the Doppler shift. But the
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reason why we don't talk about that is because this
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radiation that's being beamed out is a continuum radiation. By that,
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I mean it's at all wavelengths. So to make Doppler work,
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just the backstory here. If you've got something coming towards you,
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it's light is shifted to the blue. If it's moving
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away from you, it's light it's shifted to the red.
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But you need a feature in order to detect that.
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And some sources of light, for example, it actually even
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works with LEDs does this. But if you think of
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the old orange sodium lights which we used to see
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the low pressure sodium lights. They emit all their light
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at one wavelength, which is called the sodium D line
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for historical reasons. And so if you had a sodium
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lamp coming towards you, then that peak of wavelength would
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be moved to the blue end of the spectrum. If
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it was going away from you, it be moved to
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the red end of the spectrum, the sodium line. But
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in order to so that happens for all moving objects.
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But in order for you to be able to detect
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that it's moving, you need a discrete peak of lights
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or radiation, And in the case of a moving sodium lamp,
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that's it the peak of the sodium sodium emission line.
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If you've got a continuum a spectrum that was all
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the way from blue to red or violet to red, yes,
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it can be moved by the Doppler shift, but you
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don't see it, you don't detect it. And so in
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the case of the material swirling around a black hole
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in the accretion disc, exactly as Ron says, it actually
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undergoes something called relativistic Doppler beaming. And because this stuff
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is moving so fast, it's really not far short of
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the speed of light, the path of the photons is altered,
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and they tend to cluster around the direction in which
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the movement is taking place. And that's why an accretion
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disc is brighter on one side than it is on
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the other. It's brighter in the side that's coming towards
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you because of this relativistic Doppler beaming. It's quite an
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esoteric topic. I'm quite amazed that we're covering this on
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Space nuts, but it's really good stuff. Thank you, Ron,
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because you're clearly very very well versed in this stuff
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as well.
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I mean, when you look at the images of black
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holes that we now have, you're looking at an orange
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frosted doughnut. Basically, that's that's the primary color, the orange,
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but it is brighter on one side.
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This is there are.
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Blight spots in it, that's correct. Yeah, and some of
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that will be due to relativistic beaming.
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Yeah, okay, And how many have they taken now? I
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think there's been maybe three through.
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Yes, so we've got M fifty two was the first,
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is that right?
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Yeah?
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Fifty two the center of our galaxy, Sagittaria s a star.
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But also M fifty two done again with polarization, so
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we could see the magnetism in it. I think that's
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the way it worked. Okay, these we were with the
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event horizon telescope.
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Because I've got another one here that's of M eighty seven.
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Okay, that's there is another object that's.
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Yeah, that's the third one I was thinking of. I
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didn't know they've done in fifty two. Again, but the
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technology has reached a point now where we can actually
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image these things. They're not photos, so are they? These
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are gathered through radio spectrometry of Yeah.
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It's basically a planet sized array of radio telescopes that
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conspire together in very cunning ways to make these images,
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to synthesize the images.
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Fantastic stuff. Ron Thanks so much for the question.
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Really enjoyed that one, and hopefully hopefully we'll hear from
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you again. Our next question comes from Sunny What a
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great name for somebody who listens to an astronomy podcast.
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Hello, Spacenuts, This is Sunny Skies from southern California, Long Beach.
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In fact, my question for you today is regarding geological
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formations on Mars, which indicate there was large quantities of
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water for a long period of time. Similar to something
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we'd see on Earth. Is there any other corroborative information
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or data to support that it actually was water and
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not some other crazy liquid that we don't have here,
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possibly on Earth?
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Love the podcast the sunny.
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We're trying to it's coming into winter here, so it
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won't be sunny for long, Sonny Lovely to hear from you.
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That's a good question, because we've got a lot of
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evidence that shows there was water, rivers, oceans, streams, you know, cestpits,
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whatever you want to call them, on Mars. But that's
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all gone, but we are, you know, the telltale signs
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are there. Sonny's question is was it really water or
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could it have been something else?
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We do know there are other liquid.
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Oceans in our Solar system that are not water. Yes,
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we do, that's right, and there's more than one kind
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of water, which is also a fact that it considers.
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So yeah, could he be onder something or we absolutely
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did set certain that Mars had water?
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I think we are water perhaps.
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Yes, and that's why for that reason we still we
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can still see it. So and I'll explain that in
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a second. Yes, I guess gives me. Sonny's point is
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we see evidence of liquid. Could it have been something
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peculiar that we don't know about, And.
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In a way it is because.
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We have seen evidence on Mars from principally from the
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Phoenix Lander, which was on the which is near the
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northern Polar regions, the Northern Arctic of Mars, which actually
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analyzed chemically some of these materials. So you might remember
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Andrew Phoenix had a little backo. It was didn't have
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any wheels, it was stationary, but it had a bacco
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with which it could scrape away the top surface of
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the soil of Mars. And it didn't have to scrape
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much before it got to solid ice. And the first
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hint that this was ice was in the color it
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was white. The second hint was that some scraps of
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this material that had been dug up by the backo
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basically disappeared after a few days. They had turned directly
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into vapor. They'd sublimed, and that's exactly what you'd expect
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for water ice to do. But more especially, that bacho
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wasn't just there to scrape things. It was to pour
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the things it had dug up into a chemical analysis.
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And that's the smoking gun, because the chemical analysis demonstrated
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that yes, this was water, water ice, solid ice, and
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that's there in large quantities under the surface of the
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Arctic regions of Mars. And we know it's there in
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the on the surface actually in the polar caps of Mars,
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and we know it's water ice from there because it's
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got the spectral signature of water ice. But the reason
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why I say it could be a bit different is
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that we believe that this water is very briny, that
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it's rich in what are called perchlorates, which actually lower
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the freezing point. And there's evidence that for a short
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time there were droplets of water actually on the legs
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of the Phoenix Lander, probably made of ice that have
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been melted during the descent, vaporized, condensed out onto the
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onto the legs of the lander, and stayed liquid for
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a little time while the heat was well that temperature
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was high enough. So all the all the evidence points
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to those oceans having been made of water. Although it
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might be very briny, it might be chemically different from
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from what we experience on Earth. But only to look
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at the different forms that water comes in on Earth.
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When you've got some of them where you've got cyanide
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dissolved in it, in some of these pools, you know,
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in Yosemite in places like that. So I think I
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think it's a good question. But I think basically H
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two O is what makes up the contents of those
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format oceans.
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I think what's interesting about Mars water is that it's
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it's heavier.
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Than Earth water.
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It's got a much higher ratio of isotopes, heavy isotopes
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of hydrogen. I think is which is which is heavy water?
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Not the stuff ever the nuclear reactors, but natural it
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is water.
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Yes, that's right. It's it's similar to what was used
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in the nuclear reactors. So it's it's hydrogen with an
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extra neutron. I guess, is that right to make deuterium?
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And and yes, you're right that the ratio of and
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once again this comes from analysis by machines like Phoenix.
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On the surface of Mars, there's a higher ratio of.
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I think that's the way around. It is a higher
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ratio of heavy water to normal water on Mars than
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there is on Earth. I think that's the case.
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Yeah.
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And the other thing sunny is you couldn't drink it
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in its current state. It would need to be cleaned
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up a bit.
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Yeah.
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Do you remember we want to talk about how much
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heavy water you could drink and still survive, and it's come.
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It's a fair bit. Actually it was a few percent, yes, but.
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If you drank it for long enough, it would start
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you'd start to basically fall apart, literally fall apart, because
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the deuterium wouldn't your bodies. We're not built for it, basically.
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Yes, exactly.
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Yeah, if we were to find a water world that
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was one hundred percent D two ozer rather than age,
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we couldn't live there.
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It would kill it.
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Even though it's water, it's just it's not our water,
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heavy water. Yes, yes, So your point is very very good, Sonny.
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There's a bit more to it than.
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Meets the eye.
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And yes it is water on Mars, but it's not
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the same as our water. It's close, but it's not
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quite the same. Thanks for the question, and hopefully hopefully
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we'll hear from you again, Sonny. Great question, that one.
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