Space Light, Cosmic Shields & Moon Mysteries | Space Nuts: Astronomy Insights & Cosmic Discoveries
Cosmic Q&A: Light in Space, Astronaut Shielding, and Ice Giants
In this engaging Q&A edition of Space Nuts , hosts Andrew Dunkley and Professor Fred Watson tackle intriguing listener questions that delve into the mysteries of space. From the visibility of Voyager 1 in the depths of the solar system to the challenges of shielding astronauts from cosmic radiation, this episode is a treasure trove of cosmic knowledge.
Episode Highlights:
- Light in Space: Lee from New York City poses a thought-provoking question about how much light exists in space. Andrew and Fred explore the visibility of Voyager 1 and the implications of being far from the Sun, shedding light on human eye sensitivity and the ambient light from stars.
- Shielding Astronauts: Fenton from St. Paul, Minnesota, raises an important question about protecting astronauts from radiation beyond the Van Allen Belt. The hosts discuss potential technologies, including superconducting electromagnets and the surprising effectiveness of hydrogen-rich materials like water as radiation shields.
- Moon Comparisons: Robert from Vienna, Austria, wonders how our understanding of the solar system would differ if Earth had a moon like Europa or Titan, rather than our heavily cratered moon. The discussion highlights the significance of craters in understanding planetary history and the feasibility of landing on such moons.
- Ice Giants Explained: Duncan from Weymouth, UK, questions why Uranus and Neptune are termed "ice giants" instead of "rock giants." Andrew and Fred clarify the definitions and characteristics that distinguish these planets from their gas giant counterparts, emphasizing the unique atmospheric compositions.
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Stay curious, keep looking up, and join us next time for more stellar insights and cosmic wonders. Until then, clear skies and happy stargazing.
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Episode link: https://play.headliner.app/episode/30869022?utm_source=youtube
Kind: captions
Language: en
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Space Nuts is taking a bit of a break at
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the moment. Uh Fred and I will be back
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uh in the not too distant future with
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fresh episodes. In the meantime, enjoy
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some of uh the key episodes that we have
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presented over the years, major events
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in astronomy and space science and we'll
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see you real soon.
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>> Space Nuts.
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>> Hi there. Thanks for joining us on a Q&A
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edition of Space Nuts. I'm Andrew
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Dunley, your host. Once again, uh,
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thanks for joining us and, um, good to
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have your company. On this edition,
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we're answering some questions about
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light in space. Um, this one comes from
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Lee. He's he's asked a very interesting
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question. I've never actually thought
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about this particular uh, concept, but
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uh, it's it's a question that I think is
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worth answering for sure. It's why we
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included it. Fenton wants to know about
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um shielding astronauts in the outer
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reaches of the solar system and he's got
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an idea on how to do that. Uh Robert
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wants to talk about things we learn from
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the moon and what if our moon wasn't the
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same as the moon is now. Would our
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learnings be different? That's a really
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interesting question. And Duncan wants
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to talk about ice giants and why are
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they ice giants? Why don't we call them
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something else? That's all coming up
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shortly on this edition of Space Nuts.
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15 seconds. Guidance is internal. 10 9
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Ignition sequence start.
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>> Space nuts.
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>> 5 4 3 2
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>> 1 2 3 4 5 5 4 3 2 1
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>> Space Nuts.
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>> Astronauts report. It feels good.
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>> Once again, we welcome the one and only
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Fred Watson, astronomer at large. Hello,
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Fred.
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>> Hello, Andrew. How have you been since
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we lost B?
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>> Um, I haven't moved from this seat in
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all that time.
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Well, it's I know it's I can see you're
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glued to your chair there at home.
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>> Very much so.
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>> Yes. Uh shall we get um straight into it
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and answer some questions from our
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audience?
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>> Uh we will.
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>> That's a good idea. Yeah,
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>> it is. That's it's what we're here for.
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This first one, Fred, comes from Lee. He
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lives in New York City. Uh he's he's
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asking how much light is in space. He'll
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qualify that question. For example, if
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you were to visit Voyager 1, where
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Voyager 1 is today, would you be able to
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see it? Would you see just a silhouette?
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Would you be able to make out details
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and colors if there if there are any
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colors on it? Uh what about if you and
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Voyager were midway between the sun and
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Alpha Centuri? Uh can we know a
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reasonably accurate answer or is it pure
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speculation? Thanks. Love the show, Lee
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from New York. I I've never thought
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about that. I mean, we take for granted
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light on Earth because it's, you know,
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we're illuminated by the sun, but it's
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it's a bit different in other parts of
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the solar system and the universe in
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general. So, yeah, if we could just go,
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"Snap, we're out there next to Voyager
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One, could we actually see it? Is it
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illuminated in any way? Is it being
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illuminated by something? What would it
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be like?"
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>> Uh, the answer is yes, you'd see it. Um
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and um so we're talking really now about
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the sensitivity of the human eye
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>> u because uh with a with a camera uh you
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know um with long exposure settings and
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things you'd be able to see in great
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detail but thinking about the human eye.
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So um
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I used to work as you know at Siding
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Spring Observatory. Uh I spent many
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hours uh outside at night there. It is a
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place that is truly dark. There's no
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interference from street lights. Uh
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there are few blobs of light on the
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horizon but nothing that affects the
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pristine darkness of the night sky. And
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on a starry night with the sun not in
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the sky, you can see quite clearly. Um
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there's enough light from the stars
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themselves to let you see where you're
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going. Uh let you, you know, walk around
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and be quite confident that you're not
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going to fall off the mountain as I
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nearly did one night when it was uh
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cloudy. I went out without my torch. I
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thought, "Oh yeah, I'll see by the
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stars." But fortunately unfortunately
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the cloud had come in. I couldn't see
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anything and I nearly fell fell off the
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mountain.
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>> I didn't in the end, but um
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>> that's a that's a long drop free.
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>> Yes, it is. Yes, it's quite a long drop.
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Anyway, uh if you uh you know, normally
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on a starry night you will see um by the
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light of the stars. Now, where Voyager
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is, Voyager 1, uh I just looked it up.
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uh it is uh at a distance from the sun
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in astronomical units which is 163
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astronomical units. That's 163 times the
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number of uh times the distance between
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the earth and the sun. So that's 150
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million kilometers. Multiply that by 163
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and you will get
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uh what do you get? Uh I was looking for
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it in kilometers but it's not there.
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I'll have to do the numbers. Anyway, it
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doesn't matter. The main thing is um its
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distance is 22.55 light hours away. Uh
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that's how long it takes uh the signal
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to get from Voyager to Earth. It's
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almost a day. It's almost a light day
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away. Um, so at that distance from the
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sun, 160 odd astronomical units, uh,
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there's still significant light coming
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from the sun, not to mention Venus,
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uh, and, um, you know, Jupiter and, uh,
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the other planets, mostly the sun,
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though, you you're being illuminated by
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the sun. So that certainly ups it, uh,
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as compared with just being illuminated
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by the starry sky, which is what I was
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just talking about. So you'd see it
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really clearly. Uh you wouldn't have any
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problem making it out assuming your eye
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was dark adapted.
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>> So [clears throat] it's um it's fairly
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bright out there. I we talked about the
00:06:07.840 --> 00:06:10.390
sensitivity of the human eye as uh you
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you referred to. How how small amount of
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light can we see as human beings?
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>> Um I think there were some experiments.
00:06:20.479 --> 00:06:23.510
Let me think. Was it was it one photon
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or one pixel like that?
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>> There was that's right. We might have
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talked about this. There were
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experiments done that showed that the
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human eye is capable of detecting single
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photons. Uh it was under special
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circumstances but uh and that is just
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extraordinary. Um when you think that
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the human eye can also cope with broad
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daylight that's the amazing thing about
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the human eye. It can, you know, it's
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quite happy uh to see light uh at one
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brightness and then a light that's only
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a millionth of as bright. Um it's fine.
00:07:00.160 --> 00:07:01.909
You can deal with that. And that's a
00:07:01.919 --> 00:07:03.909
combination of what's called retinal
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bleaching and the the iris of your eye
00:07:06.880 --> 00:07:08.550
opening and closing. It's all those
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things come together to give you this
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unbelievably versatile and sensitive
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tool with which we can look at the our
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surroundings. Whether it's uh the the
00:07:19.280 --> 00:07:20.950
rock face I'm looking at now because
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that's what our backyard consists of or
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whether it's uh you know the night sky
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where you're looking at faint objects uh
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in the sky. It's quite amazing.
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>> So even if you went deeper into space
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way beyond our solar system you you
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would probably still see objects that
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you were near.
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>> There'd be enough light from the stars.
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The Milky Way uh is is bright. Uh it
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would it would you know even if as as uh
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as Lee says even even if you were
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halfway between the sun and Alpha
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Centuri you'd still see it because of
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the ambient light u that's coming from
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from the stars.
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>> Yeah. And you'd still see color because
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that's well if it's dark enough it might
00:08:03.199 --> 00:08:05.029
turn into the grays which happen to
00:08:05.039 --> 00:08:06.550
>> That's right. Yeah. And I think that's
00:08:06.560 --> 00:08:08.150
likely I think it I don't think you
00:08:08.160 --> 00:08:10.469
would see color. um you would you would
00:08:10.479 --> 00:08:11.830
where it is now there's enough light
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coming from the sun that you'd see color
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but I think uh when you got further out
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you would start to just see the you know
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the as you said the that fit that sort
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of pale gray appearance where you're
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looking at very low light low light
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levels indeed where the color cells
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aren't receptive.
00:08:29.280 --> 00:08:31.029
>> There you go Lee. Uh the answer to your
00:08:31.039 --> 00:08:33.029
question is yes to all of the above
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basically. [clears throat]
00:08:35.200 --> 00:08:37.750
>> Great question. Excellent question. All
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right, let's move on. This is from
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Fenton.
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>> Yeah. Hello, Fred and Andrew. This is
00:08:43.440 --> 00:08:46.550
Fenton contacting you from St. Paul,
00:08:46.560 --> 00:08:51.190
Minnesota in the US. Um, I sort of have
00:08:51.200 --> 00:08:53.750
a different type of astrophysical
00:08:53.760 --> 00:08:58.150
question for you and this is on how to
00:08:58.160 --> 00:09:02.150
shield astronauts from radiation outside
00:09:02.160 --> 00:09:05.670
of the Van Allen belt. Um, I was curious
00:09:05.680 --> 00:09:08.949
if you know of any pending technologies
00:09:08.959 --> 00:09:11.750
that would allow this. Obvious choice
00:09:11.760 --> 00:09:14.070
would some people would say is lead, but
00:09:14.080 --> 00:09:16.230
I can think of several reasons why this
00:09:16.240 --> 00:09:19.590
is not a good idea. How about a
00:09:19.600 --> 00:09:22.949
miniature Van Allen belt which could
00:09:22.959 --> 00:09:26.310
surround a spacecraft? How does that
00:09:26.320 --> 00:09:29.350
sound? How could this become
00:09:29.360 --> 00:09:31.990
reality? Thank you very much. I hope you
00:09:32.000 --> 00:09:34.870
like the question. Bye now.
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>> Thanks, Fenton. Fenton always has these
00:09:36.800 --> 00:09:38.949
intriguing thoughts. I I've noticed in
00:09:38.959 --> 00:09:41.110
the times that we've heard from him. Um
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maybe we should start by explaining what
00:09:42.880 --> 00:09:44.870
the Van Allen belt is for those of us
00:09:44.880 --> 00:09:48.710
who just can't remember like me.
00:09:48.720 --> 00:09:54.870
Um it's uh so the van element bel
00:09:54.880 --> 00:09:57.030
you know the magnetic shielding around
00:09:57.040 --> 00:10:01.590
the earth uh which is uh
00:10:01.600 --> 00:10:03.829
caused by the the magnetism of the
00:10:03.839 --> 00:10:05.910
earth. It's caused by the uh the fact
00:10:05.920 --> 00:10:10.070
that we've got an iron core and uh
00:10:10.080 --> 00:10:11.910
basically it's in two parts. It's solid
00:10:11.920 --> 00:10:13.750
and liquid. So it acts like a dynamo.
00:10:13.760 --> 00:10:16.630
it's rotating and that gives us this uh
00:10:16.640 --> 00:10:20.069
exactly the protection that um that um
00:10:20.079 --> 00:10:23.110
um Fenton is talking about. Um yeah,
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>> I was going to refer I'm a bit annoyed
00:10:26.800 --> 00:10:29.030
actually because I've lost it. Uh there
00:10:29.040 --> 00:10:34.069
is a very nice article on uh it's
00:10:34.079 --> 00:10:38.790
actually on the um BBC's website uh
00:10:38.800 --> 00:10:41.269
their Sky at Night website. There's a
00:10:41.279 --> 00:10:43.670
lovely article on exactly this. Here it
00:10:43.680 --> 00:10:45.990
is. I found it. I hadn't lost it. How
00:10:46.000 --> 00:10:47.990
astronauts can hide from radiation on
00:10:48.000 --> 00:10:52.949
Mars and it goes into uh the exactly the
00:10:52.959 --> 00:10:54.710
problem that uh that Fenton's talking
00:10:54.720 --> 00:10:56.550
about. How do you present how do you
00:10:56.560 --> 00:11:00.710
prevent u astronauts basically becoming
00:11:00.720 --> 00:11:02.310
irradiated
00:11:02.320 --> 00:11:06.949
uh and over time it's basically lethal
00:11:06.959 --> 00:11:08.949
uh because because of the cosmic
00:11:08.959 --> 00:11:11.269
radiation that's coming down through
00:11:11.279 --> 00:11:16.550
space uh and it it does cell damage uh
00:11:16.560 --> 00:11:19.030
in your body uh and it can actually
00:11:19.040 --> 00:11:22.389
trigger cancer. So um the the whole
00:11:22.399 --> 00:11:27.269
study of this is uh or sorry the the
00:11:27.279 --> 00:11:29.590
thrust of this article BBC Sky at Night
00:11:29.600 --> 00:11:33.430
magazine uh is to discuss how you might
00:11:33.440 --> 00:11:35.829
protect astronauts uh from the
00:11:35.839 --> 00:11:38.230
radiation. Uh and that's not just on
00:11:38.240 --> 00:11:42.069
Mars but on route. Uh okay.
00:11:42.079 --> 00:11:46.069
Uh the solution that that Fenton has
00:11:46.079 --> 00:11:48.550
suggested is covered in a paragraph. I'm
00:11:48.560 --> 00:11:49.910
going to read it because we've quoted
00:11:49.920 --> 00:11:53.990
where the source is. Uh, for example,
00:11:54.000 --> 00:11:55.750
all right, let me no, let me go back a
00:11:55.760 --> 00:11:57.509
paragraph. One, one method of helping
00:11:57.519 --> 00:11:59.509
astronauts to avoid the radiation on
00:11:59.519 --> 00:12:03.190
Mars is active shielding. For example,
00:12:03.200 --> 00:12:05.590
superconducting electromagnets could be
00:12:05.600 --> 00:12:08.150
used to create a powerful magnetic field
00:12:08.160 --> 00:12:09.829
to deflect the incoming charged
00:12:09.839 --> 00:12:11.910
radiation particles away just as the
00:12:11.920 --> 00:12:13.990
Earth's field does. That's the lanel
00:12:14.000 --> 00:12:16.710
belt. The problem is that such solutions
00:12:16.720 --> 00:12:19.430
can demand a lot of power to run and the
00:12:19.440 --> 00:12:21.430
technology is a long way from being
00:12:21.440 --> 00:12:24.310
fully developed. An easier alternative
00:12:24.320 --> 00:12:26.470
is passive shielding. Simply placing a
00:12:26.480 --> 00:12:28.949
thick bulk of shielding material between
00:12:28.959 --> 00:12:32.389
the crew habitat and the sky. Uh and
00:12:32.399 --> 00:12:34.629
then they go on to consider different
00:12:34.639 --> 00:12:38.790
materials. Aluminium aka aluminum. Uh
00:12:38.800 --> 00:12:40.389
the metal that spacecraft are
00:12:40.399 --> 00:12:42.069
constructed from is actually a pretty
00:12:42.079 --> 00:12:45.750
bad radiation shield. Um, and they say
00:12:45.760 --> 00:12:48.550
when hit by an energetic cosmic ray, its
00:12:48.560 --> 00:12:50.470
atoms can shatter and fly onwards to
00:12:50.480 --> 00:12:53.269
create even more radiation particles.
00:12:53.279 --> 00:12:55.509
And Martian soil, the regalith, uh,
00:12:55.519 --> 00:12:57.190
which if you're on Mars, you might think
00:12:57.200 --> 00:12:59.990
about digging a hole there. Uh, it's got
00:13:00.000 --> 00:13:02.710
the same problem, but it's it's actually
00:13:02.720 --> 00:13:06.230
uh, you know, abundant. Um, and so you
00:13:06.240 --> 00:13:09.269
could use that to dig a pole. If you put
00:13:09.279 --> 00:13:12.069
a two to three meter layer on top of
00:13:12.079 --> 00:13:15.430
your habitat, uh then you'll you'll get
00:13:15.440 --> 00:13:17.990
some protection. But uh the thing that
00:13:18.000 --> 00:13:20.790
surprised me, Andrew, uh is once again
00:13:20.800 --> 00:13:23.430
it comes from this same article. Uh
00:13:23.440 --> 00:13:26.230
hydrogen is the best shielding material
00:13:26.240 --> 00:13:28.949
as it's light atoms. Yeah. It's light
00:13:28.959 --> 00:13:32.069
atoms. Uh and by light, I mean not
00:13:32.079 --> 00:13:34.389
heavy. Its light atoms don't create as
00:13:34.399 --> 00:13:37.110
much secondary radiation. And so tanks
00:13:37.120 --> 00:13:40.310
of rocket fuel or water, which is rich
00:13:40.320 --> 00:13:42.629
in hydrogen, placed over crew quarters
00:13:42.639 --> 00:13:44.470
could double up as effective radiation
00:13:44.480 --> 00:13:47.350
shields. I've heard that before that um
00:13:47.360 --> 00:13:49.190
you know, one way of protecting your
00:13:49.200 --> 00:13:51.190
spacecraft as it flies to Mars is put it
00:13:51.200 --> 00:13:53.590
put it in a tank of water. Uh it's the
00:13:53.600 --> 00:13:56.069
last thing you'd expect to do, but uh
00:13:56.079 --> 00:13:58.470
water is a good shielding material. And
00:13:58.480 --> 00:14:01.829
they also uh point out the alternative
00:14:01.839 --> 00:14:03.590
of hydrogen-rich plastics like
00:14:03.600 --> 00:14:06.310
polyethylene could be used to cement
00:14:06.320 --> 00:14:08.069
regalith grains together. This is on
00:14:08.079 --> 00:14:10.949
Mars and improve their shielding effect.
00:14:10.959 --> 00:14:13.590
Um so uh if you want to read more about
00:14:13.600 --> 00:14:15.430
this, it's an article that originally
00:14:15.440 --> 00:14:18.710
appeared in the August 22 2022 issue of
00:14:18.720 --> 00:14:21.269
BBC Skylight magazine and it covers
00:14:21.279 --> 00:14:23.350
pretty well most of the ideas uh that
00:14:23.360 --> 00:14:25.590
have been that have been suggested for
00:14:25.600 --> 00:14:27.670
this radiation issue. It's one that's
00:14:27.680 --> 00:14:29.269
got to, you know, it's got to find an
00:14:29.279 --> 00:14:32.790
answer soon because uh good old Elon and
00:14:32.800 --> 00:14:35.670
his Starship uh is getting nearer to
00:14:35.680 --> 00:14:36.949
thinking about going to Mars. I don't
00:14:36.959 --> 00:14:38.550
think it's ever going to happen, but um
00:14:38.560 --> 00:14:40.710
that's uh uh that's something he'll
00:14:40.720 --> 00:14:42.710
definitely be thinking about.
00:14:42.720 --> 00:14:44.629
>> Yes, indeed. Well, he's he's too busy
00:14:44.639 --> 00:14:45.829
dealing with the Australian government
00:14:45.839 --> 00:14:46.629
at the moment.
00:14:46.639 --> 00:14:48.790
>> Yes, indeed. That's that's right.
00:14:48.800 --> 00:14:50.470
>> Some of the content on Twitter that the
00:14:50.480 --> 00:14:53.030
government wants to get rid of simply
00:14:53.040 --> 00:14:55.030
because of its um volatility. But
00:14:55.040 --> 00:14:56.870
anyway, that's a different story. Uh but
00:14:56.880 --> 00:14:59.110
there plenty of water on Mars. So maybe
00:14:59.120 --> 00:15:01.509
maybe creating those water barriers is
00:15:01.519 --> 00:15:03.590
is probably the simplest thing to do.
00:15:03.600 --> 00:15:05.430
You've already got the material there
00:15:05.440 --> 00:15:07.110
>> if you've if you've landed in the right
00:15:07.120 --> 00:15:09.509
spot where you've got or whatever.
00:15:09.519 --> 00:15:11.750
>> That's the question. Yes, indeed. Well
00:15:11.760 --> 00:15:13.509
done, Fent Fenton. You you actually
00:15:13.519 --> 00:15:15.110
happened across some of the uh the
00:15:15.120 --> 00:15:18.150
answers too in uh asking your question.
00:15:18.160 --> 00:15:20.629
>> Uh this is Space Nuts. Andrew Dunley
00:15:20.639 --> 00:15:25.670
here with Professor Fred Watson.
00:15:25.680 --> 00:15:28.470
3 2 1
00:15:28.480 --> 00:15:31.269
>> space nuts. Now Fred, uh, our next
00:15:31.279 --> 00:15:33.509
question comes from Robert. Hi guys,
00:15:33.519 --> 00:15:35.269
love your show. Sorry for the long
00:15:35.279 --> 00:15:37.829
question, but feel free to paraphrase uh
00:15:37.839 --> 00:15:40.710
or shorten it. Our moon is heavily
00:15:40.720 --> 00:15:42.870
created and has given us a lot of
00:15:42.880 --> 00:15:44.470
insight into the history of the solar
00:15:44.480 --> 00:15:46.230
system and perhaps how the planets
00:15:46.240 --> 00:15:49.350
formed. But what if we had a moon like
00:15:49.360 --> 00:15:52.629
the icy moon Europa or the shrouded in
00:15:52.639 --> 00:15:55.749
haze Titan, both of which don't show
00:15:55.759 --> 00:15:58.069
immediate evidence of cratering? Would
00:15:58.079 --> 00:16:00.629
our theory about how the planets
00:16:00.639 --> 00:16:03.430
developed would be different? What other
00:16:03.440 --> 00:16:05.829
insights about our solar system would be
00:16:05.839 --> 00:16:08.389
missing or or would we be missing? And
00:16:08.399 --> 00:16:11.110
lastly, uh would we have spent uh or
00:16:11.120 --> 00:16:13.189
would we have sent people to land on
00:16:13.199 --> 00:16:17.749
such moons? I.e. Uh, would they be more
00:16:17.759 --> 00:16:19.990
dangerous for astronauts? Uh, cheers,
00:16:20.000 --> 00:16:22.470
Robert in Vienna, Austria. Wow. I don't
00:16:22.480 --> 00:16:23.829
think we've had a question from Vienna
00:16:23.839 --> 00:16:25.269
before, have we?
00:16:25.279 --> 00:16:27.189
>> Lovely to hear from you, Robert.
00:16:27.199 --> 00:16:28.710
>> I think I think Robert might have been
00:16:28.720 --> 00:16:30.069
in touch once before. I can't
00:16:30.079 --> 00:16:32.470
>> Oh, I might have been too.
00:16:32.480 --> 00:16:34.710
And here from Vienna. Yeah, I was in
00:16:34.720 --> 00:16:36.150
Vienna at the beginning of last year and
00:16:36.160 --> 00:16:37.910
I think I think we got something around
00:16:37.920 --> 00:16:40.069
about the same time and I was waxing
00:16:40.079 --> 00:16:42.389
lyrical about being in Vienna at the UN
00:16:42.399 --> 00:16:45.269
when I was at the Copas meeting. Anyway,
00:16:45.279 --> 00:16:47.990
uh that's another another issue. Uh what
00:16:48.000 --> 00:16:49.670
if we had a Yeah, it's a really
00:16:49.680 --> 00:16:53.670
interesting question. Um, what would we
00:16:53.680 --> 00:16:57.350
not know about the solar system if our
00:16:57.360 --> 00:17:01.749
moon was basically uh one that had been
00:17:01.759 --> 00:17:05.829
resurfaced in recent years or millennia
00:17:05.839 --> 00:17:07.429
because that's what makes a surface
00:17:07.439 --> 00:17:10.949
smooth. That's how we recognize
00:17:10.959 --> 00:17:13.909
um the fact that the universe sorry that
00:17:13.919 --> 00:17:15.429
the
00:17:15.439 --> 00:17:17.350
it's how we recognize the age of a
00:17:17.360 --> 00:17:19.669
surface is by how many craters it's got.
00:17:19.679 --> 00:17:21.829
The old the older the surface, the more
00:17:21.839 --> 00:17:24.710
craters it has. And so the moon's south
00:17:24.720 --> 00:17:26.309
southern region, which is heavily
00:17:26.319 --> 00:17:29.190
cratered, as is the backside, uh tell us
00:17:29.200 --> 00:17:31.510
that uh early on in the solar systems
00:17:31.520 --> 00:17:34.150
history, it was a very wild and woolly
00:17:34.160 --> 00:17:36.070
place with things charging about all
00:17:36.080 --> 00:17:38.789
over and causing these craters. Now, if
00:17:38.799 --> 00:17:40.950
we had a moon that was like Europa that
00:17:40.960 --> 00:17:45.270
um had, you know, icy geysers on it that
00:17:45.280 --> 00:17:47.430
basically covered up the craters, would
00:17:47.440 --> 00:17:50.470
we have known about that? My guess is
00:17:50.480 --> 00:17:52.789
yes, we would because we'd see other
00:17:52.799 --> 00:17:55.669
bodies within the solar system uh like
00:17:55.679 --> 00:17:59.430
you know other moons like um places like
00:17:59.440 --> 00:18:02.630
um um series the the biggest of the
00:18:02.640 --> 00:18:03.990
asteroids the dwarf planet that
00:18:04.000 --> 00:18:05.909
dominates the asteroid belt that's
00:18:05.919 --> 00:18:08.789
heavily created. Uh parts of Pluto are
00:18:08.799 --> 00:18:12.310
heavily crated. Um
00:18:12.320 --> 00:18:15.669
Mimas uh one of Saturn's moon is moons
00:18:15.679 --> 00:18:18.150
is heavily created too. So, so we we'd
00:18:18.160 --> 00:18:19.830
know about it by looking at other
00:18:19.840 --> 00:18:23.029
objects even if our own moon was uh
00:18:23.039 --> 00:18:26.710
smoothly surfaced. Um it's it's a but
00:18:26.720 --> 00:18:30.950
the Robert's last point uh on this uh
00:18:30.960 --> 00:18:33.190
would we have sent people to land on
00:18:33.200 --> 00:18:37.110
such a moon? Uh I think um I don't know
00:18:37.120 --> 00:18:38.950
that's a really good question. I mean we
00:18:38.960 --> 00:18:40.950
have sent people to land on our moon as
00:18:40.960 --> 00:18:44.230
it stands uh with an ancient surface. In
00:18:44.240 --> 00:18:47.110
fact, where they landed were more recent
00:18:47.120 --> 00:18:49.029
uh than the heavily cratered surfaces
00:18:49.039 --> 00:18:50.150
because they were principally in the
00:18:50.160 --> 00:18:52.710
Maria, the the basalt planes.
00:18:52.720 --> 00:18:53.669
>> Yeah.
00:18:53.679 --> 00:18:57.029
>> So maybe that suggests that we would
00:18:57.039 --> 00:18:59.750
have landed people on Europa as well. Uh
00:18:59.760 --> 00:19:00.150
because
00:19:00.160 --> 00:19:02.549
>> I think we pro Yeah, we probably would
00:19:02.559 --> 00:19:05.029
because it would have a solid surface.
00:19:05.039 --> 00:19:07.350
There'd be places because it would be so
00:19:07.360 --> 00:19:09.110
close to us, we'd be able to examine and
00:19:09.120 --> 00:19:12.230
and find the the right landing points.
00:19:12.240 --> 00:19:14.710
might be a bit more difficult with a
00:19:14.720 --> 00:19:18.070
moon that's shrouded in land gas.
00:19:18.080 --> 00:19:19.270
>> Yeah. Yeah.
00:19:19.280 --> 00:19:21.750
>> Yeah, that's right. Uh and especially um
00:19:21.760 --> 00:19:25.110
place like Titan. Uh
00:19:25.120 --> 00:19:27.110
I I still think we'd have done it.
00:19:27.120 --> 00:19:30.950
Actually, I think um you know the JFK's
00:19:30.960 --> 00:19:33.190
uh promise to put astronauts on the moon
00:19:33.200 --> 00:19:35.110
would have still held good even if it
00:19:35.120 --> 00:19:36.789
had been a very different place. If it
00:19:36.799 --> 00:19:39.510
had been like Io, uh, it might have been
00:19:39.520 --> 00:19:41.270
a different story where, you know,
00:19:41.280 --> 00:19:43.270
you've got the most volcanically active
00:19:43.280 --> 00:19:45.270
body in the entire solar system with
00:19:45.280 --> 00:19:47.190
stuff going off all over the place. I
00:19:47.200 --> 00:19:48.230
think we might have been a bit more
00:19:48.240 --> 00:19:51.830
reluctant to to land on a Yes, possibly.
00:19:51.840 --> 00:19:54.230
So, uh, it would be interesting to have
00:19:54.240 --> 00:19:55.590
something different, but then if we'd
00:19:55.600 --> 00:19:57.990
always had if if we'd always had an ice
00:19:58.000 --> 00:20:00.390
moon, we probably would have caught a
00:20:00.400 --> 00:20:03.190
question from Robert asking, "What if we
00:20:03.200 --> 00:20:07.590
had a rocky moon?" Now, would we Would
00:20:07.600 --> 00:20:09.510
we have a different interpretation of
00:20:09.520 --> 00:20:11.110
four masses of planets if there was a
00:20:11.120 --> 00:20:12.870
rocky moon next to us instead of an ice
00:20:12.880 --> 00:20:15.430
moon? Yes. Um, in an alternative
00:20:15.440 --> 00:20:16.950
universe, Robert, you would have flipped
00:20:16.960 --> 00:20:18.789
your question. Good to hear from you.
00:20:18.799 --> 00:20:21.430
Hope all all is well in Austria. Our
00:20:21.440 --> 00:20:23.430
final question for this episode comes
00:20:23.440 --> 00:20:25.350
from Duncan.
00:20:25.360 --> 00:20:29.270
>> Hello. Duncan here from Wayouth in the
00:20:29.280 --> 00:20:34.390
UK. Again, a quick question.
00:20:34.400 --> 00:20:36.710
just looking was just doing some reading
00:20:36.720 --> 00:20:39.909
and I noticed that Uranus and Neptune
00:20:39.919 --> 00:20:44.070
are often referred to as ice giants.
00:20:44.080 --> 00:20:48.870
Now, given that ice is basically just
00:20:48.880 --> 00:20:53.510
sort of like a rock form of water or CO2
00:20:53.520 --> 00:20:56.630
or whatever else, but basically just a
00:20:56.640 --> 00:20:59.110
solid form of it. Why are they not just
00:20:59.120 --> 00:21:03.270
called rock giants? Why do we make the
00:21:03.280 --> 00:21:05.750
definition of ice rather than just
00:21:05.760 --> 00:21:08.630
calling them rock? It just seems odd
00:21:08.640 --> 00:21:11.669
because the little planets in the inner
00:21:11.679 --> 00:21:13.830
solar system are referred to as rocky
00:21:13.840 --> 00:21:17.430
planets. So given that they're also
00:21:17.440 --> 00:21:19.110
apparently rocky, why are they not
00:21:19.120 --> 00:21:21.669
called rocky giants?
00:21:21.679 --> 00:21:26.149
Okay, thank you. Bye. Thanks Duncan.
00:21:26.159 --> 00:21:28.630
Appreciate your questions as always. Uh
00:21:28.640 --> 00:21:30.789
yeah. Why do we call them ice giants
00:21:30.799 --> 00:21:32.870
just for the sake of the exercise? Cuz
00:21:32.880 --> 00:21:36.390
there's gas giants and ice giants.
00:21:36.400 --> 00:21:38.950
>> Yeah, except one is a subset of the
00:21:38.960 --> 00:21:42.149
other. And so all four of the outer
00:21:42.159 --> 00:21:44.390
planets, Jupiter, Saturn, Neptune,
00:21:44.400 --> 00:21:46.549
sorry, Uranus, and Neptune, they're all
00:21:46.559 --> 00:21:51.430
gas giants because they have uh eye mass
00:21:51.440 --> 00:21:55.590
uh um you know, much more in the case of
00:21:55.600 --> 00:21:57.909
Jupiter certainly than uh than our own
00:21:57.919 --> 00:22:01.110
planet. Um the they've got they're
00:22:01.120 --> 00:22:03.029
giants. They're big. They've got high
00:22:03.039 --> 00:22:07.350
mass. Uh and they don't have a visible
00:22:07.360 --> 00:22:09.510
surface, which is why they're called gas
00:22:09.520 --> 00:22:11.590
giants because all we see is a gasy
00:22:11.600 --> 00:22:15.510
envelope. Um just to go to the last of
00:22:15.520 --> 00:22:17.270
Duncan's questions there, we we wouldn't
00:22:17.280 --> 00:22:19.990
call the inner planets rocky giants
00:22:20.000 --> 00:22:21.909
because they're not giants. They're kind
00:22:21.919 --> 00:22:23.510
of normal planet size. You know, if you
00:22:23.520 --> 00:22:25.110
if you think of the Earth as being your
00:22:25.120 --> 00:22:28.789
standard planet, then uh Mercury, Venus,
00:22:28.799 --> 00:22:32.070
and Mars are similar in size. They're
00:22:32.080 --> 00:22:33.990
all smaller. Venus is about the same
00:22:34.000 --> 00:22:35.590
size, but Mercury and Mars, of course,
00:22:35.600 --> 00:22:38.390
are smaller. So, uh so it's only when
00:22:38.400 --> 00:22:40.710
you compare with the size of Earth that
00:22:40.720 --> 00:22:42.470
you'd start talking about giants because
00:22:42.480 --> 00:22:44.470
they are much much bigger than Earth.
00:22:44.480 --> 00:22:47.430
And so, that's the gas giants. So, why
00:22:47.440 --> 00:22:50.149
are Uranus and Neptune called ice
00:22:50.159 --> 00:22:55.350
giants? because they have hazes of ice
00:22:55.360 --> 00:22:57.270
in their atmosphere.
00:22:57.280 --> 00:23:00.149
>> So, uh, and that's the the trick. It's
00:23:00.159 --> 00:23:02.710
not a solid surface. It's not rock.
00:23:02.720 --> 00:23:04.789
[snorts] It's it's a haze. It's kind of
00:23:04.799 --> 00:23:07.990
like a a dust of ice which permeates
00:23:08.000 --> 00:23:10.230
their atmosphere. And and and it's water
00:23:10.240 --> 00:23:14.310
ice in fact, uh, mostly. Uh so that's
00:23:14.320 --> 00:23:15.990
why they're called ice giants because
00:23:16.000 --> 00:23:19.029
unlike Saturn and Jupiter uh which don't
00:23:19.039 --> 00:23:21.669
have these hazes uh the the outer the
00:23:21.679 --> 00:23:25.110
rocky rock sorry the two outer planets
00:23:25.120 --> 00:23:27.750
Uranus and Neptune do they have ice
00:23:27.760 --> 00:23:29.350
hazes in their atmosphere hence the
00:23:29.360 --> 00:23:30.950
name.
00:23:30.960 --> 00:23:33.430
Okay. Yeah. And because last episode we
00:23:33.440 --> 00:23:35.750
learned there wasn't much water in
00:23:35.760 --> 00:23:37.830
Jupiter's
00:23:37.840 --> 00:23:41.430
>> in the in the two outer gas giants.
00:23:41.440 --> 00:23:42.789
Yeah. It sounds like there is. Is that
00:23:42.799 --> 00:23:46.390
why they're a different color? Yes. Yes,
00:23:46.400 --> 00:23:48.310
I think that's right. They're um and and
00:23:48.320 --> 00:23:49.830
also their their atmospheric
00:23:49.840 --> 00:23:51.990
constituents are are different. They
00:23:52.000 --> 00:23:53.750
don't have the same belt structure that
00:23:53.760 --> 00:23:56.549
Saturn and Jupiter do. Uh it may be that
00:23:56.559 --> 00:23:58.789
that's because any belts that exist are
00:23:58.799 --> 00:24:00.549
much lower in the atmosphere and so you
00:24:00.559 --> 00:24:03.669
don't see them. Um yeah, I mean uh
00:24:03.679 --> 00:24:08.070
there's there's a strong body of uh of
00:24:08.080 --> 00:24:11.909
advocacy within the space fraternity to
00:24:11.919 --> 00:24:16.710
get get more spacecraft out to Uranus
00:24:16.720 --> 00:24:19.510
and Neptune cuz they're the two planets
00:24:19.520 --> 00:24:22.549
about which we know least. Um and uh
00:24:22.559 --> 00:24:24.710
will be good to know more.
00:24:24.720 --> 00:24:27.510
>> Yeah. Well, if you sit down in snow for
00:24:27.520 --> 00:24:29.430
long enough, your Uranus turns into a
00:24:29.440 --> 00:24:32.149
nice giant sun.
00:24:32.159 --> 00:24:36.710
I couldn't help it. Sorry. Uh, yeah.
00:24:36.720 --> 00:24:38.549
>> Which is why we call it Uranus in
00:24:38.559 --> 00:24:39.590
politics.
00:24:39.600 --> 00:24:41.190
>> I know. I know.
00:24:41.200 --> 00:24:43.669
>> Yeah. But it's just a joke you've got to
00:24:43.679 --> 00:24:46.630
tell. It's just you have to.
00:24:46.640 --> 00:24:49.669
>> Yes. I blame Johannes Borda, who is the
00:24:49.679 --> 00:24:52.149
person who chose the name. It's fine in
00:24:52.159 --> 00:24:54.470
German. Uess. Uess. There's nothing
00:24:54.480 --> 00:24:57.430
wrong with that. It's great. Yeah. Ruins
00:24:57.440 --> 00:24:59.830
all the jokes, bro.
00:24:59.840 --> 00:25:01.830
>> All right. So, yes, they're ice giants
00:25:01.840 --> 00:25:03.269
for a very good reason, Duncan, because
00:25:03.279 --> 00:25:05.350
they've got ice in them uh in the
00:25:05.360 --> 00:25:07.110
atmosphere. But technically speaking,
00:25:07.120 --> 00:25:09.430
they are in fact gas giants. But
00:25:09.440 --> 00:25:11.590
>> yes, we differentiate them because of
00:25:11.600 --> 00:25:13.350
their substantially different
00:25:13.360 --> 00:25:15.430
atmospheres. There you are. Thanks,
00:25:15.440 --> 00:25:17.269
Duncan. Great to hear from you. Great to
00:25:17.279 --> 00:25:18.710
hear from everybody. Thanks for sending
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Send us your question. That's audio
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places. Uh Fred, as always, thank you so
00:25:57.520 --> 00:26:00.470
much. Pleasure, Andrew. See you soon.
00:26:00.480 --> 00:26:02.950
>> Okay, Fred Watson, astronomer at large.
00:26:02.960 --> 00:26:04.310
We'll catch him on the next episode of
00:26:04.320 --> 00:26:06.390
Space Nuts. might catch Hugh then as
00:26:06.400 --> 00:26:09.190
well because um
00:26:09.200 --> 00:26:11.430
not here today. Didn't even call in
00:26:11.440 --> 00:26:13.909
sick. I need a note. And from me, Andrew
00:26:13.919 --> 00:26:15.350
Dumprey, thanks very much for your
00:26:15.360 --> 00:26:17.190
company. We'll see you again soon on the
00:26:17.200 --> 00:26:19.750
next episode of Space Nuts. Bye-bye.
00:26:19.760 --> 00:26:20.710
>> Space Nuts.
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