Solar Secrets, Cosmic Siblings & the Quest for Breathable Exoplanets | Space Nuts: Astronomy...


Solar Curiosities, Stellar Siblings, and the Quest for Sun Missions
In this enlightening episode of Space Nuts , hosts Andrew Dunkley and Professor Fred Watson dive into a plethora of solar-themed questions submitted by their curious audience. From the intriguing arc of the sun across the sky to the search for the sun's long-lost siblings, this episode is packed with cosmic insights that will leave you pondering the mysteries of our solar system.
Episode Highlights:
- The Sun's Arc: Andrew kicks off the episode with a question about the sun's arc as observed from the French Alps. Fred explains the celestial mechanics behind this phenomenon, illustrating how our perspective from Earth creates the illusion of an arc due to the spherical nature of the celestial sphere.
- Searching for Solar Siblings: Ernie's inquiry about the sun's siblings leads to a fascinating discussion on galactic archaeology. The hosts explore ongoing research aimed at identifying stars with similar chemical compositions to the sun, potentially revealing our sun's stellar family tree.
- Close Encounters with the Sun: Mark's question about missions to the sun sparks an exploration of the Parker Solar Probe, which has been gathering invaluable data by flying close to the sun. Andrew and Fred discuss the probe's findings and the various other missions dedicated to studying our star.
- Exoplanetary Possibilities: Martin shares his sci-fi aspirations and questions the potential for breathable atmospheres on exoplanets. The hosts reflect on recent discoveries of Earth-sized exoplanets and the challenges of confirming their atmospheres, while also encouraging Martin's creative writing endeavors.
For more Space Nuts, including our continuously updating newsfeed and to listen to all our episodes, visit our website. (https://www.spacenutspodcast.com/) Follow us on social media at SpaceNutsPod on Facebook, Instagram, and more. 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 (https://www.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.
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Episode link: https://play.headliner.app/episode/31442835?utm_source=youtube
Kind: captions
Language: en
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Hello again. Thank you for joining us on
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Space Nuts. This is our weekly Q&A
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edition where we take questions from the
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audience. We go and find someone who can
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tell us the answer and then we pretend
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we're doing it. Um, my name's Andrew
00:00:13.599 --> 00:00:16.070
Dunley, your host. Fred's Fred's face
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went, "Oh, we don't." [laughter]
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Uh, coming up on this episode, uh, we've
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got a lot of, uh, solar questions. We've
00:00:23.600 --> 00:00:25.029
got a question from Andrew about the
00:00:25.039 --> 00:00:27.029
sun's arc. Ernie wants to know about the
00:00:27.039 --> 00:00:28.870
sun's siblings and Mark wants to know
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about missions to the sun. You go, Mark.
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I'm not setting foot on it. It's hot
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enough here already. And we're going to
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finish off with a question about
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Earthlike planets. That's all coming up
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on this episode of Space Nuts.
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>> 15 seconds. Guidance is internal. 10 9g
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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 4 3 2 1
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>> Space Nuts. Astronauts report. It feels
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good.
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>> Back again for more. His name is
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Professor Fred Watson, astronomer at
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large. Hello, Fred.
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>> Hello. Hello, Andrew. Um, fancy seeing
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you here.
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>> Yes, it's quite unusual. Quite unusual.
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And we're all decked out in blue today.
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You've got the gun barrel blue. I've got
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the sky blue of New South Wales on.
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>> That's the um official sporting color of
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my state.
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>> I didn't know that.
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>> Yeah. Yeah.
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>> Didn't even know there was
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>> sky blue. Yeah. Oh, look. Um, the the
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the official Australian sporting colors
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are green and gold.
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>> Green and gold. That's right.
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>> But that that wasn't actually uh
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official until the 80s. Before that,
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they just used to wear a pair of thongs
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and a cut off jeans and go to the
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Olympics, I think.
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>> She'll be right.
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>> Yeah, mate. No worries. Yes. Um, we got
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a bunch of questions to deal with, so we
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might as well hit the ground running in
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our thongs. I know there's some people
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laughing at that because thong means
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something else in other countries, but
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it does. That's right.
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>> It's it's a pair of flip-flops or
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jandles or whatever you call them,
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wherever you're from. Uh, first question
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comes from Andrew. It's about the Sun's
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Ark. I'm sitting here in the French Alps
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on Boxing Day. You lucky duck. uh
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slightly hung over thanks to uh an
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excess of a prey ski uh last night and
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watching the sun trace an arc across the
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sky measured from mountain peak to
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mountain peak. But why an arc the shape
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of which varies uh by the time of year
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given the earth itself is rotating uh on
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only one axis. Uh, I know the Earth's uh
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tilted from um from the vertical, but
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how does that explain the arc uh with
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only one axis of rotation? Shouldn't it
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be a straight line? That comes from
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Andrew Jones. Hope you had a nice
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Christmas, Andrew. Sounds like it. What
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a what a horrible place to be. The
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French Alps for Christmas.
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>> Oh, yeah. Sounds great, doesn't it?
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>> Yeah. But he brings up an interesting
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point. Uh sitting there sipping on
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whatever it is he was drinking and uh
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and and watching the sun and going,
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"Hang on a minute. What's going on here?
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There's an arc and it's not Noah's.
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It's not. That's right. Uh it's a
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different sort of arc. Uh because it's
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spelled differently. It's got a C
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instead of a K. [laughter]
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[snorts] Uh it uh and in fact so so uh
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you know Andrew's question is uh with
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only one axis of rotation shouldn't it
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be a straight line? And the answer is it
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is a straight line.
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>> Yeah. Uh but it's a straight line on a
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sphere. Uh because we are our vantage
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point uh from Earth. Uh we look out into
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space. We imagine something called the
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celestial sphere. It's a great way of uh
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you know working out the way things move
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in space and how the motion of the sun
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and planets all fits together. You what
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you imagine is a sphere of infinite
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dimensions and we're sitting at the
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middle of it. We only see half of it
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because the other half is below the
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horizon. It's still there. The celestial
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sphere goes on below the earth, this
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hypothesized sphere. Um but um it's very
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useful uh a useful device for
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understanding how things move in the
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sky. And if you imagine yourself uh
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sitting in the French Alps uh with the
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celestial sphere above you uh you uh
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would certainly in the northern
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hemisphere be able to see uh the thing
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that we call the north pole star polar
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star Polaris. Uh the pole star faint
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star that um I nearly always look for
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whenever I'm in the northern hemisphere
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just to reconnect with it. It's at the
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end of the the little bear's tail. uh if
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you know your northern constellations
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but that
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would come with us sometime.
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>> Yeah, they they're great. The northern
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constellations of they've got great
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charm. Anyway, that's another story. So,
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um that is the point about which the
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whole celestial sphere seems to rotate.
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And so, uh, the height of the pole star
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above your horizon, uh, is the same as
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your latitude. So, if you're at latitude
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French Alps is probably 45 or
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thereabouts, maybe a bit more than that,
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45, uh, it means your pole star is going
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to be 45 degrees above the horizon. And
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this entire sphere rotates around that
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point. And so uh that's why on on a
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sphere the sun's motion is a straight
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line. It goes from the east eastern side
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of the sky depends on the time of year
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as to exactly where it rises and sets.
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Uh but it sets on the western side. And
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so um uh what looks like an arc to you
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is really a straight line bent by the
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celestial sphere. this apparent uh you
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know it's it's a just a great way of
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imagining the sky because it doesn't you
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don't have to worry about the distances
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of anything. You're just imagining
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everything projected onto this infinite
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sphere. And when you do that as the
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earth's rotating the sun rises in
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towards the east and sets towards the
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west. Um and uh it follows basically an
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arc as we see it from our position. But
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in terms of the sphere itself, it's just
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going from one side to the other in a
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straight line.
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>> There you go. Sounds like putting in
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golf. Like every putt they say every
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putt's a straight putt except
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that the um the green isn't dead flat
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and straight, so the ball will move
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accordingly.
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>> Yes, that's right. Yeah. In fact, that's
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um that's that almost puts you into a
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different uh regime because that's
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effectively what geodessics are, which
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are
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>> uh the way light behaves uh in general
00:06:53.360 --> 00:06:56.629
relativity. Uh so light travels what it
00:06:56.639 --> 00:06:58.870
in what it thinks is a straight line,
00:06:58.880 --> 00:07:00.710
but it's going through different
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gravitational fields and gravitational
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wells. And so like you know like your
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your golf ball when you're put putting
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it uh it it's it it's moving around.
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It's wandering around.
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>> Yeah. Uh we we have a quirk at um do
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golf club where um if you want to figure
00:07:19.199 --> 00:07:21.350
out where the putt goes work out which
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direction the river is.
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>> Yes.
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>> They they always fall towards the river.
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>> Always remember Andrew that five irons
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don't flow.
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>> They do not. It's a good book that I
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don't know who wrote it, but it's a
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ripper.
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>> I should read this.
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>> It's a ripper.
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>> Well, it's got swearing in it. Don't
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know how that happened.
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>> Yeah. Gosh. Disgraceful. Disgraceful.
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And by the way, the French Alps are at
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45.8345
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degrees north.
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>> So, you did very well.
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>> Yeah.
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>> And 6.85
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uh 6.8655 degrees east.
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>> That's right.
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>> Yeah. Uh, thank you for the question,
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Andrew. Great to hear from you. Hope you
00:08:00.080 --> 00:08:03.430
survived the u the French Alps um
00:08:03.440 --> 00:08:06.469
adventure. Uh our next question comes
00:08:06.479 --> 00:08:10.550
from a a new contributor. Hello Ernie.
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>> Hello Andrew and Fred. My name is Ernie
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and I'm reaching out to you from a small
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town near Buffalo, New York. I'm a
00:08:16.960 --> 00:08:18.950
longtime listener and this is the first
00:08:18.960 --> 00:08:21.909
time I'm submitting a question. In a
00:08:21.919 --> 00:08:23.990
recent episode, a listener asked if
00:08:24.000 --> 00:08:26.469
astronomers have ever identified the
00:08:26.479 --> 00:08:29.589
star or stars that went supernova,
00:08:29.599 --> 00:08:32.310
seating the nebula our sun formed in
00:08:32.320 --> 00:08:34.949
with heavy elements. This got me to
00:08:34.959 --> 00:08:37.269
thinking, stars typically form in
00:08:37.279 --> 00:08:41.909
clusters. And I assume our sun isn't any
00:08:41.919 --> 00:08:45.190
different. Has there ever been or is
00:08:45.200 --> 00:08:47.990
there any active research that is
00:08:48.000 --> 00:08:51.350
looking for any of the son's siblings?
00:08:51.360 --> 00:08:54.310
Thank you so much um for doing this
00:08:54.320 --> 00:08:56.870
podcast. Really enjoy it. Always look
00:08:56.880 --> 00:08:59.670
forward when new episodes drop. Wishing
00:08:59.680 --> 00:09:02.070
you the best for the holidays. Thank
00:09:02.080 --> 00:09:03.990
you, Ernie. Great to hear from you, a
00:09:04.000 --> 00:09:06.870
first time callerina. And uh great
00:09:06.880 --> 00:09:08.790
question, too. Great question. Sorry to
00:09:08.800 --> 00:09:10.389
hear about the Buffalo Bills. I don't
00:09:10.399 --> 00:09:12.310
know if you're into the uh American
00:09:12.320 --> 00:09:16.470
football um Ernie, but um we visited
00:09:16.480 --> 00:09:19.030
Buffalo um late last year and they were
00:09:19.040 --> 00:09:21.670
very very hopeful that the the Bills
00:09:21.680 --> 00:09:23.430
would come through, but they've been
00:09:23.440 --> 00:09:25.750
knocked out in the playoffs. So, um very
00:09:25.760 --> 00:09:27.910
unfortunate, but maybe maybe next year.
00:09:27.920 --> 00:09:29.350
They're certainly starting to look like
00:09:29.360 --> 00:09:33.110
a pretty solid outfit. So, um yeah, any
00:09:33.120 --> 00:09:35.190
work going into finding the Sun's
00:09:35.200 --> 00:09:36.870
siblings? Now, I remember us talking
00:09:36.880 --> 00:09:40.150
some time back about the possibility
00:09:40.160 --> 00:09:43.269
that the son had a twin [clears throat]
00:09:43.279 --> 00:09:45.350
>> and they got separated at birth and they
00:09:45.360 --> 00:09:46.710
can't find each other, but they're
00:09:46.720 --> 00:09:48.470
they're going through the archives to
00:09:48.480 --> 00:09:50.710
see if there's any family history that
00:09:50.720 --> 00:09:55.030
can connect them. Um that Yeah, but the
00:09:55.040 --> 00:09:57.910
the sun would have been part of um I I
00:09:57.920 --> 00:10:00.470
imagine a whole bunch of stars that were
00:10:00.480 --> 00:10:04.230
born in that um that um supernova
00:10:04.240 --> 00:10:05.670
situation. Is that what he was talking
00:10:05.680 --> 00:10:06.790
about?
00:10:06.800 --> 00:10:09.590
>> Well, that's part of the issue. The the
00:10:09.600 --> 00:10:12.230
fact that the you know the the gas cloud
00:10:12.240 --> 00:10:15.269
in which the sun and the rest of the
00:10:15.279 --> 00:10:17.110
cluster that was formed at the same time
00:10:17.120 --> 00:10:21.750
as the sun um that that was uh seeded by
00:10:21.760 --> 00:10:24.230
gases from a supernova explosion which
00:10:24.240 --> 00:10:26.710
we have no knowledge of but we you know
00:10:26.720 --> 00:10:28.710
it's just the background interstellar
00:10:28.720 --> 00:10:31.509
medium is enriched by the elements that
00:10:31.519 --> 00:10:33.750
come from a supernova explosion. But um
00:10:33.760 --> 00:10:35.990
no Ernie's question is on the money and
00:10:36.000 --> 00:10:40.389
the answer is yes. Uh that's um
00:10:40.399 --> 00:10:43.190
to try and find the sun's siblings is
00:10:43.200 --> 00:10:46.150
actually uh ongoing research and it's
00:10:46.160 --> 00:10:48.710
part of the subject that we usually call
00:10:48.720 --> 00:10:50.790
galactic archaeology. is looking at the
00:10:50.800 --> 00:10:54.470
way our galaxy has evolved uh by
00:10:54.480 --> 00:10:57.269
studying in detail the chemical
00:10:57.279 --> 00:11:00.630
composition of the stars within uh the
00:11:00.640 --> 00:11:02.310
sun's neighborhood within a few thousand
00:11:02.320 --> 00:11:03.990
light years. I was involved with all
00:11:04.000 --> 00:11:05.829
that with the rave project a few years
00:11:05.839 --> 00:11:09.030
ago. And so one of the uh not the holy
00:11:09.040 --> 00:11:10.550
grails of that but certainly one of the
00:11:10.560 --> 00:11:13.829
interesting aspects is to find stars
00:11:13.839 --> 00:11:17.829
that have identical chemical mixes to
00:11:17.839 --> 00:11:21.910
the sun. Uh and um if you can do that,
00:11:21.920 --> 00:11:24.310
if you can find them, uh there's a good
00:11:24.320 --> 00:11:26.630
chance that they were born from the same
00:11:26.640 --> 00:11:29.829
dust cloud as the sun was. Uh and so
00:11:29.839 --> 00:11:32.630
they might very well be solar siblings.
00:11:32.640 --> 00:11:35.590
Um it may even be possible that, you
00:11:35.600 --> 00:11:37.350
know, we know that the sun's four four
00:11:37.360 --> 00:11:39.590
and a half billion years old, about 4.6
00:11:39.600 --> 00:11:43.590
4.7 billion years old. Um if you could
00:11:43.600 --> 00:11:46.230
look at the motion of stars that have
00:11:46.240 --> 00:11:49.910
the identical uh constituents to the sun
00:11:49.920 --> 00:11:51.590
and you will be able to certainly me
00:11:51.600 --> 00:11:54.069
measure their velocities quite easily
00:11:54.079 --> 00:11:57.030
then you might be able to almost rewind
00:11:57.040 --> 00:11:59.829
back to a time uh when you could prove
00:11:59.839 --> 00:12:01.350
that they were all in the same place at
00:12:01.360 --> 00:12:04.230
the same time.
00:12:04.240 --> 00:12:06.310
>> Okay. Yeah. All right. Um
00:12:06.320 --> 00:12:09.509
>> so so the answer is yes. We are there is
00:12:09.519 --> 00:12:11.269
interest there is certainly research on
00:12:11.279 --> 00:12:13.110
all that and yes I had a couple of weeks
00:12:13.120 --> 00:12:15.030
in Buffalo once I was a guest lecturer
00:12:15.040 --> 00:12:17.430
at the Canius College there and it's
00:12:17.440 --> 00:12:19.670
very cold
00:12:19.680 --> 00:12:21.509
>> uh wasn't cold while we were there I
00:12:21.519 --> 00:12:23.110
mean it's it's a stones throw from
00:12:23.120 --> 00:12:25.190
Niagara Falls which is
00:12:25.200 --> 00:12:27.269
>> yeah like you could almost walk it
00:12:27.279 --> 00:12:29.350
>> they were pretty icy when we were there.
00:12:29.360 --> 00:12:31.990
>> Yeah. Um, but I I really enjoyed
00:12:32.000 --> 00:12:33.590
spending some time there and and
00:12:33.600 --> 00:12:35.350
learning like they they they had a big
00:12:35.360 --> 00:12:37.350
big exhibition on while we were there
00:12:37.360 --> 00:12:40.870
about the um one of the great canals
00:12:40.880 --> 00:12:44.870
that was built 150 odd years ago now I
00:12:44.880 --> 00:12:47.990
think. Um and and how it changed the
00:12:48.000 --> 00:12:49.509
entire region
00:12:49.519 --> 00:12:51.910
>> forever um in terms of trade and
00:12:51.920 --> 00:12:55.430
movement of materials and uh fascinating
00:12:55.440 --> 00:12:58.870
place really quite fascinating. Um,
00:12:58.880 --> 00:13:01.030
yeah. I suppose the the the problem with
00:13:01.040 --> 00:13:03.670
trying to find the sun's siblings is is
00:13:03.680 --> 00:13:05.750
the amount of time that's passed. It's
00:13:05.760 --> 00:13:06.949
not like you're looking back through
00:13:06.959 --> 00:13:08.629
your family tree a couple of
00:13:08.639 --> 00:13:10.629
generations, which we're talking
00:13:10.639 --> 00:13:13.110
billions of years of movement.
00:13:13.120 --> 00:13:15.269
>> That's right. Yes. But but as I said,
00:13:15.279 --> 00:13:17.910
you you know, the way you identify them
00:13:17.920 --> 00:13:20.550
is not because they're close or anything
00:13:20.560 --> 00:13:22.310
like that. It's by their chemical
00:13:22.320 --> 00:13:23.829
composition.
00:13:23.839 --> 00:13:28.550
uh which we can do out to many several
00:13:28.560 --> 00:13:30.389
thousands light years depending how how
00:13:30.399 --> 00:13:33.030
precise you want it to be. Um in fact
00:13:33.040 --> 00:13:34.150
there's an instrument on the Anglo
00:13:34.160 --> 00:13:35.750
Australian telescope which is called
00:13:35.760 --> 00:13:38.870
Hermes uh which is designed exactly for
00:13:38.880 --> 00:13:41.269
doing that job. It looks at very limited
00:13:41.279 --> 00:13:44.550
areas uh regions of the spectrum of
00:13:44.560 --> 00:13:47.269
stars uh to look for [clears throat]
00:13:47.279 --> 00:13:49.030
exactly the amount of chemicals that
00:13:49.040 --> 00:13:51.110
that are in those atmospheres of those
00:13:51.120 --> 00:13:53.350
stars. And that's the kind of instrument
00:13:53.360 --> 00:13:55.509
that you use to try and find the sun
00:13:55.519 --> 00:13:57.430
siblings. What I haven't said is whether
00:13:57.440 --> 00:13:59.590
there's been any success on that.
00:13:59.600 --> 00:14:00.710
>> I was bad to ask.
00:14:00.720 --> 00:14:01.670
>> Yeah. [laughter]
00:14:01.680 --> 00:14:04.230
And um uh I can't remember the answer. I
00:14:04.240 --> 00:14:06.230
I mean there are certainly stars which
00:14:06.240 --> 00:14:08.230
have got very similar chemical
00:14:08.240 --> 00:14:12.069
composition and ages to the sun. Uh, I'm
00:14:12.079 --> 00:14:14.150
not sure just how near we are to to
00:14:14.160 --> 00:14:15.829
being able to identify them as
00:14:15.839 --> 00:14:17.990
definitely coming from the same gas
00:14:18.000 --> 00:14:20.150
cloud and being born in the same cluster
00:14:20.160 --> 00:14:21.829
as the sun was.
00:14:21.839 --> 00:14:24.629
>> Well, according to a quick search I've
00:14:24.639 --> 00:14:28.069
just done, and this is an AI response,
00:14:28.079 --> 00:14:29.910
uh, yes, astronomers have identified
00:14:29.920 --> 00:14:31.590
several candidates. Yeah.
00:14:31.600 --> 00:14:33.509
>> The solar siblings, stars formed from
00:14:33.519 --> 00:14:36.790
the same gas cloud as our sun 4.5
00:14:36.800 --> 00:14:38.870
billion years ago, but none are
00:14:38.880 --> 00:14:42.710
definitely confirmed. There you go.
00:14:42.720 --> 00:14:45.269
>> Um they maybe they don't want to be
00:14:45.279 --> 00:14:47.990
found. Maybe maybe our our son was, you
00:14:48.000 --> 00:14:49.670
know, the black sheep of the family and
00:14:49.680 --> 00:14:51.509
they all went, "No, we're out of here.
00:14:51.519 --> 00:14:52.790
We know what's going to happen around
00:14:52.800 --> 00:14:55.189
this place. It's going to fall planets
00:14:55.199 --> 00:14:56.870
and then where will we be?" And then
00:14:56.880 --> 00:14:58.230
there'll be humans and then
00:14:58.240 --> 00:14:59.350
>> Yes, that's right. Exactly.
00:14:59.360 --> 00:15:01.509
>> You know, they'll want us they'll want
00:15:01.519 --> 00:15:03.350
us to pay them money or something. Yeah.
00:15:03.360 --> 00:15:05.590
I don't know. Um but it was a great
00:15:05.600 --> 00:15:06.949
question, Ernie. Thanks for sending it
00:15:06.959 --> 00:15:09.829
in and please do so again. This is Space
00:15:09.839 --> 00:15:12.310
Nuts with Andrew Dunley and Professor
00:15:12.320 --> 00:15:15.189
Fred Watson.
00:15:15.199 --> 00:15:17.110
>> Hey, that's one of the better sims.
00:15:17.120 --> 00:15:18.949
Believe me, we've had a couple of
00:15:18.959 --> 00:15:20.389
cardiac [music] arrest down here too,
00:15:20.399 --> 00:15:20.870
Pete.
00:15:20.880 --> 00:15:23.030
>> There weren't any time for that up here.
00:15:23.040 --> 00:15:24.949
>> Space nuts.
00:15:24.959 --> 00:15:27.590
>> I love that one. No time for a cardiac
00:15:27.600 --> 00:15:32.389
arrest. Uh let's uh carry on to our next
00:15:32.399 --> 00:15:34.230
question that comes from Mark. It's
00:15:34.240 --> 00:15:36.389
another story about this uh question
00:15:36.399 --> 00:15:38.150
about the sun. Hi Andrew and Fred. Are
00:15:38.160 --> 00:15:40.310
there any plans to send a spacecraft to
00:15:40.320 --> 00:15:42.389
the sun? And I mean up close and
00:15:42.399 --> 00:15:45.030
personal. Uh the data they could get
00:15:45.040 --> 00:15:47.430
would be invaluable and could really
00:15:47.440 --> 00:15:50.150
tighten up uh some loose ends on what we
00:15:50.160 --> 00:15:52.550
think we know. Uh keep up the great
00:15:52.560 --> 00:15:56.230
work. Uh that's Mark from Sussex. Sussex
00:15:56.240 --> 00:15:58.710
in England. I assume England. Uh I'm
00:15:58.720 --> 00:16:00.389
pretty sure that'd be right.
00:16:00.399 --> 00:16:02.389
>> So you s I used to live in Sussex as
00:16:02.399 --> 00:16:03.189
well.
00:16:03.199 --> 00:16:04.790
>> Yes. Yeah. I think we mentioned that a
00:16:04.800 --> 00:16:06.389
week or two ago. So we've had a few
00:16:06.399 --> 00:16:08.389
>> where the royals from Sussex of late
00:16:08.399 --> 00:16:10.710
>> the the Royal Greenwich Observatory used
00:16:10.720 --> 00:16:13.986
to be a place called Hmansu. Yeah.
00:16:13.996 --> 00:16:15.269
[clears throat and cough] Not far from
00:16:15.279 --> 00:16:17.189
where William the Conqueror landed in
00:16:17.199 --> 00:16:18.710
1066.
00:16:18.720 --> 00:16:19.110
>> Okay.
00:16:19.120 --> 00:16:22.069
>> It was all very historic place. Um and
00:16:22.079 --> 00:16:23.430
the Royal Observatory was actually
00:16:23.440 --> 00:16:25.910
>> he defeated he did he defeated King
00:16:25.920 --> 00:16:27.189
>> Henry was it?
00:16:27.199 --> 00:16:28.629
>> Harold. Harold. I knew it started with
00:16:28.639 --> 00:16:29.430
an H.
00:16:29.440 --> 00:16:34.230
>> Yeah. H um so yeah look I I I I know
00:16:34.240 --> 00:16:37.670
there are probes that are um gathering
00:16:37.680 --> 00:16:39.110
information about the sun all the time
00:16:39.120 --> 00:16:41.030
and in fact we had a recent probe that's
00:16:41.040 --> 00:16:43.269
name escapes me that actually touched
00:16:43.279 --> 00:16:45.350
the sun which was uh a pretty
00:16:45.360 --> 00:16:47.430
extraordinary thing and
00:16:47.440 --> 00:16:49.829
>> in fact that's the one that um that
00:16:49.839 --> 00:16:52.710
really Mark is asking about uh uh are
00:16:52.720 --> 00:16:54.629
there any plans to sp send a spacecraft
00:16:54.639 --> 00:16:56.949
to the sun uh and I mean up close and
00:16:56.959 --> 00:16:59.749
personal it is already there Uh it's
00:16:59.759 --> 00:17:02.629
called the Parker Solar Probe. Uh it's
00:17:02.639 --> 00:17:04.949
um flown through the inner or the outer
00:17:04.959 --> 00:17:08.069
corona of the sun uh experiencing those
00:17:08.079 --> 00:17:09.829
very high temperatures. It's got a heat
00:17:09.839 --> 00:17:12.150
shield. It's in a or an orbit that is
00:17:12.160 --> 00:17:16.211
highly elliptical, very elongated. So
00:17:16.221 --> 00:17:17.669
[clears throat] it it spends some of its
00:17:17.679 --> 00:17:20.230
time close to the sun and some of its
00:17:20.240 --> 00:17:22.549
time quite a long way away. I'm not
00:17:22.559 --> 00:17:23.990
actually sure whether it is still
00:17:24.000 --> 00:17:27.510
active. uh but what it's done is it has
00:17:27.520 --> 00:17:31.750
enhanced our understanding of the uh of
00:17:31.760 --> 00:17:34.549
the way the corona is heated. The sun's
00:17:34.559 --> 00:17:37.750
corona is at so several tens of millions
00:17:37.760 --> 00:17:41.430
of degrees uh and the surface of the sun
00:17:41.440 --> 00:17:43.350
the photosphere this bit that we see is
00:17:43.360 --> 00:17:45.909
about 5 a half thousand degrees. How
00:17:45.919 --> 00:17:48.150
does the outer atmosphere get so hot
00:17:48.160 --> 00:17:49.669
when you've got something relatively
00:17:49.679 --> 00:17:53.110
cool inside? And the Parker Solar Probe
00:17:53.120 --> 00:17:55.590
has revealed that it's almost certainly
00:17:55.600 --> 00:17:57.110
magnetism that does that, the
00:17:57.120 --> 00:17:59.350
transportation of energy via magnetic
00:17:59.360 --> 00:18:01.350
fields. You're about to tell me whether
00:18:01.360 --> 00:18:02.549
it's still going or not.
00:18:02.559 --> 00:18:05.990
>> It is. It is actually uh the uh is fully
00:18:06.000 --> 00:18:07.990
active. It's healthy. It's operating
00:18:08.000 --> 00:18:12.789
normally as at early 2026. It's done 26
00:18:12.799 --> 00:18:14.549
close approach
00:18:14.559 --> 00:18:18.150
>> uh approaches to the sun. Um, and that
00:18:18.160 --> 00:18:21.190
was up to December of of last year. And
00:18:21.200 --> 00:18:23.350
it uh will continue to orbit the sun.
00:18:23.360 --> 00:18:25.510
It'll set speed records while it's doing
00:18:25.520 --> 00:18:27.270
it. Uh, it's it's been doing some
00:18:27.280 --> 00:18:29.990
extraordinary things. Uh, what I find
00:18:30.000 --> 00:18:31.909
extraordinary is that it can survive
00:18:31.919 --> 00:18:33.510
temperatures around 2 and a half
00:18:33.520 --> 00:18:36.789
thousand degrees Fahrenheit. That's um
00:18:36.799 --> 00:18:39.510
that's that's mighty warm.
00:18:39.520 --> 00:18:41.590
>> Yep. With a with a clever cleverly
00:18:41.600 --> 00:18:43.350
designed heat shield. I think that's
00:18:43.360 --> 00:18:46.150
whath keeps the spacecraft cool and lets
00:18:46.160 --> 00:18:48.230
it continue its work. It's a very
00:18:48.240 --> 00:18:50.150
successful mission.
00:18:50.160 --> 00:18:52.470
>> Are there any other probes working out
00:18:52.480 --> 00:18:55.029
there? I mean, there are observer
00:18:55.039 --> 00:18:56.870
probes. I believe they're not designed
00:18:56.880 --> 00:18:59.270
to go in and out of the sun's corona,
00:18:59.280 --> 00:19:01.029
but they're they're sort of keeping a
00:19:01.039 --> 00:19:03.029
close eye on it.
00:19:03.039 --> 00:19:05.190
>> Yeah, that's right. There's uh so so the
00:19:05.200 --> 00:19:08.549
sun's observed from a safer distance uh
00:19:08.559 --> 00:19:10.789
up close and personal uh compared with
00:19:10.799 --> 00:19:12.470
where we are on Earth. uh there's a
00:19:12.480 --> 00:19:15.029
there's a flatilla of uh of
00:19:15.039 --> 00:19:17.190
observatories looking at the various
00:19:17.200 --> 00:19:20.950
aspects of the sun. We also now have um
00:19:20.960 --> 00:19:23.909
a very large groundbased telescope that
00:19:23.919 --> 00:19:26.710
is set providing the most amazing images
00:19:26.720 --> 00:19:28.870
of the sun's photosphere. That's the the
00:19:28.880 --> 00:19:31.590
visible sphere of the sun. Uh it's the
00:19:31.600 --> 00:19:34.549
Daniel K. Anui solar telescope. It's on
00:19:34.559 --> 00:19:38.070
top of Halakala on the island of Maui uh
00:19:38.080 --> 00:19:41.990
in the Hawaiian islands. Money and I got
00:19:42.000 --> 00:19:43.510
married in front of it.
00:19:43.520 --> 00:19:47.029
>> Yeah, I remember. Yeah. Um they have
00:19:47.039 --> 00:19:48.950
great names for stuff in Hawaii, don't
00:19:48.960 --> 00:19:50.070
they?
00:19:50.080 --> 00:19:51.669
>> Yeah, they do.
00:19:51.679 --> 00:19:52.470
>> They do.
00:19:52.480 --> 00:19:54.549
>> Just rolls off the tongue, that one. Uh
00:19:54.559 --> 00:19:57.430
there are plenty of probes actually um
00:19:57.440 --> 00:19:59.590
Mark that are that are wandering around
00:19:59.600 --> 00:20:01.270
the sun. There's the Solar Orbiter,
00:20:01.280 --> 00:20:05.750
which is an ISSa NASA mission um taking
00:20:05.760 --> 00:20:07.510
high resolution imagery and and
00:20:07.520 --> 00:20:09.029
gathering data about the sun. There's
00:20:09.039 --> 00:20:11.990
another one that was launched in 2023
00:20:12.000 --> 00:20:14.230
uh an Indian mission uh which is
00:20:14.240 --> 00:20:17.510
dedicated to observing the solar corona
00:20:17.520 --> 00:20:22.150
and it's the Adita L1 mission and
00:20:22.160 --> 00:20:26.230
there's a there's a a whole fleet of uh
00:20:26.240 --> 00:20:28.549
probes that are that are monitoring the
00:20:28.559 --> 00:20:30.549
solar winds. So the Solar Dynamics
00:20:30.559 --> 00:20:33.590
Observatory SOHO that's a famous one. Uh
00:20:33.600 --> 00:20:36.070
the STEREO mission because there are
00:20:36.080 --> 00:20:37.909
twin satellites doing that. I think we
00:20:37.919 --> 00:20:40.390
talked about that one. Uh Hinade, which
00:20:40.400 --> 00:20:43.590
is a a JAXA mission. Uh the GO solar
00:20:43.600 --> 00:20:45.830
ultraviolet imager and the advanced
00:20:45.840 --> 00:20:49.270
composition explorer or ACE uh which is
00:20:49.280 --> 00:20:51.350
looking at the solar winds which have um
00:20:51.360 --> 00:20:54.230
been very busy of late. We've seen some
00:20:54.240 --> 00:20:56.950
incredible activity. The sun's sort of
00:20:56.960 --> 00:20:59.430
reaching the end of its most active
00:20:59.440 --> 00:21:02.230
phase, isn't it Fred? Yeah, it's it's
00:21:02.240 --> 00:21:04.070
sort of still at solar maximum, but it
00:21:04.080 --> 00:21:08.070
gradually uh dies away to solar minimum.
00:21:08.080 --> 00:21:10.549
>> Yeah. And from what I understand, you've
00:21:10.559 --> 00:21:12.310
you've really only got a short period of
00:21:12.320 --> 00:21:15.669
time to enjoy the the the current level
00:21:15.679 --> 00:21:17.830
of activity before things start to ease
00:21:17.840 --> 00:21:23.029
off and um we see less um less
00:21:23.039 --> 00:21:24.549
spectacular
00:21:24.559 --> 00:21:26.230
light shows. Would that be the way to
00:21:26.240 --> 00:21:26.789
describe?
00:21:26.799 --> 00:21:28.390
>> Yeah. And and certainly as the sun's
00:21:28.400 --> 00:21:31.029
activity declines, the aurora that we
00:21:31.039 --> 00:21:33.029
see get further and further away from
00:21:33.039 --> 00:21:35.669
the equator, if I put it that way. The
00:21:35.679 --> 00:21:38.470
more active the sun is, the the the
00:21:38.480 --> 00:21:40.470
lower latitude you can you can see it
00:21:40.480 --> 00:21:41.830
at.
00:21:41.840 --> 00:21:44.310
>> Well, it's um it's certainly uh been
00:21:44.320 --> 00:21:47.029
spectacular lately. Uh thanks for the
00:21:47.039 --> 00:21:50.950
question, Mark.
00:21:50.960 --> 00:21:52.390
>> You're here also.
00:21:52.400 --> 00:21:53.510
>> Space nuts.
00:21:53.520 --> 00:21:55.750
>> Our final question, or is it a sermon?
00:21:55.760 --> 00:21:58.950
comes from Martin. Sit back, relax, grab
00:21:58.960 --> 00:22:00.710
a cup of tea. This is going to take a
00:22:00.720 --> 00:22:05.590
while. Hello, space nuts. Margin Burman
00:22:05.600 --> 00:22:09.029
Gorvine here, writer extraordinaire in
00:22:09.039 --> 00:22:11.110
many genres
00:22:11.120 --> 00:22:16.470
with a question for my work in progress.
00:22:16.480 --> 00:22:21.110
uh my science fiction novel involving a
00:22:21.120 --> 00:22:23.350
certain unpleasant
00:22:23.360 --> 00:22:29.430
very rich dude called Egon Rusk who
00:22:29.440 --> 00:22:32.549
wishes to see the stars with what he
00:22:32.559 --> 00:22:36.549
imagines is the master race and comes to
00:22:36.559 --> 00:22:41.830
a rather unfortunate end. Um,
00:22:41.840 --> 00:22:47.190
as I've been writing this, the uh their
00:22:47.200 --> 00:22:52.070
supposed destination is Trappist 1E.
00:22:52.080 --> 00:22:54.870
Now,
00:22:54.880 --> 00:22:57.830
Professor John T. Hero mentioned on a
00:22:57.840 --> 00:23:01.270
recent podcast that all the star, all
00:23:01.280 --> 00:23:04.789
the planets in the Trappist one system
00:23:04.799 --> 00:23:07.270
lack an atmosphere.
00:23:07.280 --> 00:23:09.830
So, I was very concerned about that
00:23:09.840 --> 00:23:12.789
because uh I don't want my characters
00:23:12.799 --> 00:23:17.830
all choking and dying. So, I had a look
00:23:17.840 --> 00:23:21.830
and it seems according to NASA that it's
00:23:21.840 --> 00:23:24.950
Trappist 1D
00:23:24.960 --> 00:23:28.470
as in David that has been shown to lack
00:23:28.480 --> 00:23:30.630
an atmosphere. But they're still trying
00:23:30.640 --> 00:23:35.590
to figure out whether Travis 1E has one
00:23:35.600 --> 00:23:40.230
or not. Um, in any case, I was just
00:23:40.240 --> 00:23:44.149
wondering if there are any other
00:23:44.159 --> 00:23:48.950
uh stars with with exoplanets
00:23:48.960 --> 00:23:53.029
within say 20, 30, 40 light years of
00:23:53.039 --> 00:23:57.350
Earth that might conceivably be roughly
00:23:57.360 --> 00:24:00.950
the mass of Earth and might conceivably
00:24:00.960 --> 00:24:04.310
have a breathable atmosphere. I mean,
00:24:04.320 --> 00:24:06.230
this is all
00:24:06.240 --> 00:24:09.350
kind of off-the-wall satirical se uh
00:24:09.360 --> 00:24:11.750
sci-fi, so it doesn't matter that much,
00:24:11.760 --> 00:24:13.590
but I was just wondering about your
00:24:13.600 --> 00:24:18.470
thoughts, and I don't mean to uh
00:24:18.480 --> 00:24:24.470
disparage Professor her. Um I I I but I
00:24:24.480 --> 00:24:26.950
I you know I just suspect that he did
00:24:26.960 --> 00:24:30.630
see that Trappist one D lacks an
00:24:30.640 --> 00:24:32.549
atmosphere and sort of thought well
00:24:32.559 --> 00:24:35.430
maybe that's all the planets in that
00:24:35.440 --> 00:24:38.549
system. And also
00:24:38.559 --> 00:24:42.630
um I would like to conclude by reading a
00:24:42.640 --> 00:24:45.990
poem on that I've just written that is a
00:24:46.000 --> 00:24:49.830
riff on
00:24:49.840 --> 00:24:53.990
uh Robert Frost's famous uh fire and ice
00:24:54.000 --> 00:24:57.350
about the back and forth debate over the
00:24:57.360 --> 00:25:00.710
big bang versus the big crunch also
00:25:00.720 --> 00:25:03.510
known as the ganab gibb although I don't
00:25:03.520 --> 00:25:05.750
love that term because it sort of sounds
00:25:05.760 --> 00:25:08.630
like A lost BG.
00:25:08.640 --> 00:25:11.269
So
00:25:11.279 --> 00:25:14.230
swell or crunch.
00:25:14.240 --> 00:25:18.070
Some think the cosmos swells for I. Some
00:25:18.080 --> 00:25:22.149
see a crunch of aging bones I know and
00:25:22.159 --> 00:25:26.149
sigh. So might the cold get worse for I.
00:25:26.159 --> 00:25:29.029
But pressure hits you like a punch. You
00:25:29.039 --> 00:25:33.669
feel your skin begin to burn. And so I
00:25:33.679 --> 00:25:37.190
have a dreadful hunch. We may all learn.
00:25:37.200 --> 00:25:40.470
We must all bunch.
00:25:40.480 --> 00:25:44.950
Burman Gorvine. Over and out.
00:25:44.960 --> 00:25:48.710
Never leaves you wondering, Martin. Uh,
00:25:48.720 --> 00:25:51.350
thanks for the question. Um, I'm going
00:25:51.360 --> 00:25:53.190
to go first here, Fred, because only
00:25:53.200 --> 00:25:55.510
this morning by coincidence did I read a
00:25:55.520 --> 00:25:57.830
story and it's a little bit of an irony
00:25:57.840 --> 00:25:59.590
in this because it comes from the
00:25:59.600 --> 00:26:01.669
University of Southern Queensland where
00:26:01.679 --> 00:26:05.990
Professor Jonty her works and it's uh
00:26:06.000 --> 00:26:08.310
this has been published on the ABC uh
00:26:08.320 --> 00:26:11.590
science website. Uh so it it basically
00:26:11.600 --> 00:26:13.510
says that the that astronomers at the
00:26:13.520 --> 00:26:15.990
University of Southern Queensland have
00:26:16.000 --> 00:26:19.029
discovered a potential candidate for an
00:26:19.039 --> 00:26:21.269
Earth-sized planet. It's uh planet
00:26:21.279 --> 00:26:24.950
HD137030B.
00:26:24.960 --> 00:26:26.630
It's a bit further away than Martin
00:26:26.640 --> 00:26:29.190
would like, 150 light years from Earth,
00:26:29.200 --> 00:26:33.190
but it orbits a sunlike star and they're
00:26:33.200 --> 00:26:36.070
referring to it as a planet candidate.
00:26:36.080 --> 00:26:39.110
Um the p paper needs uh one more
00:26:39.120 --> 00:26:42.390
observation to confirm the uh status of
00:26:42.400 --> 00:26:46.390
planet but this one is only slightly
00:26:46.400 --> 00:26:49.590
bigger than earth if it is uh indeed a
00:26:49.600 --> 00:26:53.750
um a a a planet. They think they think
00:26:53.760 --> 00:26:57.430
so. Uh an earth almost earthsized planet
00:26:57.440 --> 00:27:00.310
orbiting a sunlike star sounds like it's
00:27:00.320 --> 00:27:02.950
got some some potential there coming out
00:27:02.960 --> 00:27:04.070
of the University of Southern
00:27:04.080 --> 00:27:05.909
Queensland. So that's uh interesting
00:27:05.919 --> 00:27:08.149
news, very interesting timing based on
00:27:08.159 --> 00:27:10.390
um receiving Martin's question.
00:27:10.400 --> 00:27:10.710
>> Yeah.
00:27:10.720 --> 00:27:12.870
>> Um just before the uh the publication of
00:27:12.880 --> 00:27:14.630
that story.
00:27:14.640 --> 00:27:17.269
>> Yeah. Um and uh Luke, Martin's as
00:27:17.279 --> 00:27:20.310
capable as I am of looking all these up.
00:27:20.320 --> 00:27:22.630
Uh the Wikipedia list of nearest
00:27:22.640 --> 00:27:24.549
terrestrial exoplanet candidates is
00:27:24.559 --> 00:27:26.950
probably the the neatest source to go to
00:27:26.960 --> 00:27:28.789
because it gives references to a lot of
00:27:28.799 --> 00:27:32.310
the original papers of these uh the in
00:27:32.320 --> 00:27:35.990
which the planets are described. Um it's
00:27:36.000 --> 00:27:40.789
uh uh currently got this is uh uh ones
00:27:40.799 --> 00:27:44.149
within 50 light years. uh I put in when
00:27:44.159 --> 00:27:46.950
I went through this the search 34
00:27:46.960 --> 00:27:49.909
exoplanets 11 of which probably lie
00:27:49.919 --> 00:27:52.470
inside their stars habitable zone. It's
00:27:52.480 --> 00:27:56.070
a bit more difficult to, as Martin was
00:27:56.080 --> 00:27:58.149
um kind of hinting there, it's a bit
00:27:58.159 --> 00:28:01.830
more difficult to confirm the atmosphere
00:28:01.840 --> 00:28:05.110
uh of a of a an exoplanet because what
00:28:05.120 --> 00:28:08.950
you what you're trying to do is um most
00:28:08.960 --> 00:28:10.630
of these are discovered by the transit
00:28:10.640 --> 00:28:12.630
method. You know, planets that go in
00:28:12.640 --> 00:28:14.070
front of their parent star, they dim the
00:28:14.080 --> 00:28:17.190
light slightly uh as they pass in front
00:28:17.200 --> 00:28:18.789
of the parent star, and you can measure
00:28:18.799 --> 00:28:22.149
that dimming. Uh but you can also um if
00:28:22.159 --> 00:28:24.789
you're if you've got very topline
00:28:24.799 --> 00:28:27.990
equipment like the web telescope uh you
00:28:28.000 --> 00:28:30.230
can also look at the spectrum uh change
00:28:30.240 --> 00:28:32.310
in the star as the planet passes in
00:28:32.320 --> 00:28:34.149
front of it and if that spectrum changes
00:28:34.159 --> 00:28:37.350
then uh you can be sure that the planet
00:28:37.360 --> 00:28:39.350
has an atmosphere and you can actually
00:28:39.360 --> 00:28:42.070
see what gases are are actually present
00:28:42.080 --> 00:28:44.870
in the atmosphere. So, um, that's a much
00:28:44.880 --> 00:28:46.470
more difficult observation and I think
00:28:46.480 --> 00:28:48.549
that's why, uh, it's a bit of a struggle
00:28:48.559 --> 00:28:51.510
for Martin to find to to identify with
00:28:51.520 --> 00:28:54.630
certainty, uh, which of these exoplanets
00:28:54.640 --> 00:28:56.630
might have an atmosphere. I might leave
00:28:56.640 --> 00:28:58.389
him to that and remind him that since
00:28:58.399 --> 00:28:59.909
he's writing fiction, he can do anything
00:28:59.919 --> 00:29:02.149
like with these planets, anything,
00:29:02.159 --> 00:29:04.149
anything he wants.
00:29:04.159 --> 00:29:06.870
>> I I'm um well into my trilogy, Fred.
00:29:06.880 --> 00:29:09.110
I've uh written the first book and I'm
00:29:09.120 --> 00:29:12.149
six chapters into the second book and
00:29:12.159 --> 00:29:13.990
>> still the the ideas are still coming.
00:29:14.000 --> 00:29:15.909
I'm I'm wondering when I'll hit the
00:29:15.919 --> 00:29:18.230
brick wall, but um yeah, it's it's going
00:29:18.240 --> 00:29:20.310
well at the moment. I'm enjoying it. So,
00:29:20.320 --> 00:29:22.149
I'm not going to give anything away, but
00:29:22.159 --> 00:29:22.710
um
00:29:22.720 --> 00:29:25.110
>> you're making it up as you go along.
00:29:25.120 --> 00:29:27.269
>> That's exactly how I'm
00:29:27.279 --> 00:29:28.710
>> I'll get to the next chapter and go,
00:29:28.720 --> 00:29:30.230
okay, where do I want this to go? And I
00:29:30.240 --> 00:29:33.269
just let my imagination run wild. So, um
00:29:33.279 --> 00:29:35.350
that's how I've always written. I don't,
00:29:35.360 --> 00:29:37.430
you know, started at school doing it
00:29:37.440 --> 00:29:38.950
that way when I won a composition
00:29:38.960 --> 00:29:39.909
contest.
00:29:39.919 --> 00:29:40.710
>> Very good.
00:29:40.720 --> 00:29:44.149
>> And that was that. Um, so yeah, we we
00:29:44.159 --> 00:29:45.990
covered Martin's question. Great poetry,
00:29:46.000 --> 00:29:48.470
by the way. The the big crunch. Yeah,
00:29:48.480 --> 00:29:50.230
nice work. Thanks, Martin. Good to hear
00:29:50.240 --> 00:29:52.149
from you as always. If you'd like to
00:29:52.159 --> 00:29:54.630
send questions into us, you can do so on
00:29:54.640 --> 00:29:56.950
our website, spacenutspodcast.com.
00:29:56.960 --> 00:29:58.789
Spacenuts.io.
00:29:58.799 --> 00:30:01.990
Choose your URL wisely and just click
00:30:02.000 --> 00:30:05.269
the uh AMA button which stands for ask
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00:30:08.240 --> 00:30:09.590
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our website as well. Uh one thing we do
00:30:16.799 --> 00:30:18.950
ask is if you um it doesn't matter what
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platform you're on, whether it's YouTube
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or Spreaker or uh Apple Podcasts, please
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leave a review. Uh the more the merrier.
00:30:27.760 --> 00:30:30.710
uh they do help apparently to um find
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more listeners and that's what we'd like
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to do. So if you could leave a review
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for us, we would appreciate it greatly
00:30:38.559 --> 00:30:40.549
and thank you Fred as always. It's been
00:30:40.559 --> 00:30:41.750
great fun.
00:30:41.760 --> 00:30:43.830
>> Um it's good fun or else we wouldn't do
00:30:43.840 --> 00:30:44.470
it.
00:30:44.480 --> 00:30:46.470
>> That's that's absolutely true. Certainly
00:30:46.480 --> 00:30:49.269
not doing it for the money. Um
00:30:49.279 --> 00:30:49.669
>> no,
00:30:49.679 --> 00:30:51.029
>> thanks Fred.
00:30:51.039 --> 00:30:53.350
>> We'll see you next week. Uh, Professor
00:30:53.360 --> 00:30:54.870
Fred Watson, astronomer at large. And
00:30:54.880 --> 00:30:56.789
thanks to Hugh in the studio, who
00:30:56.799 --> 00:30:58.630
couldn't be with us today because he's
00:30:58.640 --> 00:31:00.230
actually put his hand up for a mission
00:31:00.240 --> 00:31:02.549
to the sun because it's a lot cooler
00:31:02.559 --> 00:31:04.149
there than it is in Australia at the
00:31:04.159 --> 00:31:06.230
moment. Can't blame him for that. And
00:31:06.240 --> 00:31:07.750
from me, Andrew Dunley, thanks for your
00:31:07.760 --> 00:31:09.190
company. We'll catch you on the next
00:31:09.200 --> 00:31:11.190
episode of Space Nuts. Bye-bye.
00:31:11.200 --> 00:31:13.510
>> Space Nuts. You've been listening to the
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