Asteroids, Comets & the Latest from the DART Mission: A Cosmic Update | Space Nuts: Astronomy...


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Asteroid Updates, DART Mission Insights, and the Chris Case of 3I ATLAS
In this exciting episode of Space Nuts , hosts Andrew Dunkley and Professor Fred Watson delve into the fascinating world of comets and asteroids. From the latest updates on asteroid 2024 YR4's potential impact with the Moon to groundbreaking findings from the DART mission, this episode is packed with cosmic discoveries and intriguing discussions.
Episode Highlights:
- Asteroid 2024 YR4 Update: The hosts discuss the recent observations made using the James Webb Space Telescope, which have ruled out the possibility of asteroid 2024 YR4 hitting the Moon in 2032. They explore the significance of these findings and the implications for future lunar missions.
- DART Mission Success: Andrew and Fred revisit the DART mission, highlighting how the impact on the asteroid moon Dimorphos not only changed its orbit but also altered the orbit of the entire Didymos system around the Sun. This marks a historic achievement in planetary defense and asteroid science.
- The Mystery of 3I ATLAS: The episode concludes with a discussion on comet 3I ATLAS, which has been found to have an unusual chemical composition, particularly a high ratio of methanol to hydrogen cyanide. The hosts ponder what this could mean for our understanding of other solar systems and the chemistry of celestial bodies.
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.
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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/32168323?utm_source=youtube
Kind: captions
Language: en
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Hello again and thank you for joining us
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on Space Nuts, the astronomy and space
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science podcast and radio show on
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community radio across Australia. My
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name's Andrew Dunley. Great to have your
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company in this the 607th episode of our
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program. Can you believe it? And this
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one is 100% dedicated to comets and
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asteroids in one way or another. We've
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got an update on the potential impact of
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asteroid Y4 with the moon. And they've
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been keeping an eye on this and they've
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come up with an answer and it's uh it's
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really clever the way they've done it.
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Uh more news out of the Dart mission.
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Something else has happened there. Yes,
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it's on a collision course with nothing.
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Had you worried there for a moment and
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three Atlas is chemically unstable. In
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fact, it's falling down drunk. We'll
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tell you why on this episode of Space
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Nuts.
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>> 15 seconds. Guidance is internal. 10 9
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Ignition sequence start. 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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>> Joining us again for another stint on
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this little podcast of ours is Professor
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Fred Watson, astronomer at large. Hello,
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Fred.
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>> Hello, Andrew. And uh it's nice to talk
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to you. What a surprise.
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>> Good to see you.
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And we have got um a um a real rocking
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program today.
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>> Oh, I love it. Love it.
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>> It's all about rocks and ice and
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asteroids and something else which we'll
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get to later that's not rock and ice. Uh
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but um first an update on the potential
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impact of asteroid Y R4 with the moon.
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were a little bit worried that its
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chances of hitting the moon were well I
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think I heard in the early stages of its
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discovery that people were quoting 20 or
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30% chance of it hitting the moon that
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kind of got wound back to a more
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reasonable number. Uh but now they've
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got some definitive
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evidence of what's going to happen
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that that's correct. Um, I mean, uh,
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it's not just the moon that worried us
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for a while with asteroid 2024 YR4.
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uh because when it was discovered back
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in 2024, as you might guess, uh Y4
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um when its trajectory was analyzed and
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you got to remember that an object is
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only 60 mters across um which is flying
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through space, you make observations of
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its position. uh and if you've only
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observed it over a short period of
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period of time, the uncertainties in its
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well both its past orbit and its future
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orbit are very large. So it's what we
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call the arc uh the arc of observation.
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The the wider the arc of observations
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that you can make, the more accurate is
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going to be your assessment of where
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it's come from and where it's going. Um
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and so those early assessments uh
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actually they were in early in 25 2025
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when these calculations were made. Um
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but it's it did suggest a small chance
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that it might hit the earth.
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>> Uh and that was very quickly I think I'm
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sure you and I talked about this on
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space.
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>> Yeah, we did.
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>> It was very quickly ruled out. Uh and
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but as it sort of wandered on its way uh
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early in 2025, uh there was still a
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possibility that it might hit the moon.
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Uh and the time that it would happen
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would be uh 2035
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uh was the uh basically the the targeted
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time for sorry no is that right? 2032
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>> 2032.
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Yeah. Yeah, that's correct. Sorry, I'm
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mixing up my numbers. You deserve when
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you get to a certain age.
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Uh 2032
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um that there was a non-zero chance that
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it would hit the moon. And the the story
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what happened then was of course this
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object is it's what we call a near-Earth
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asteroid because it approaches near the
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Earth, but it's not near the Earth all
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the time.
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>> Most of the time it's a long way away as
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it goes around in its orbit around the
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sun. and it sort of disappeared from
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view essentially certainly from the uh
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from the purview of groundbased
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telescopes. There was not going to be
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any way we thought of observing it again
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until 2028 when it would make another
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close approach, not one that had any
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risk attached to it. But we didn't
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expect uh to be able to see its position
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in any detail until 2028, which we would
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need in order to predict where it might
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be in 2032, whether it's going to hit
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the moon or not. Um but um there are
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some scientists at uh who use the James
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Web Space Telescope who tend not to let
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uh faintness stand in their way because
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that's why you couldn't observe this
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object. It was just too faint. And sure
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enough, uh early this year, last month
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in fact, they've made two sets of
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observations where they've actually
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picked up uh the image, a tiny faint
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image of uh 2024 YR4. Uh they've picked
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it up and uh allowed um them the
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calculations in uh to basically take
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those new positions, the 2026 positions
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into the orbit calculation. Uh, and what
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they've done is they've ruled out any
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possibility of it hitting the moon. So,
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that's an unexpected story for us. I
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didn't think we'll be talking about this
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again until 2028. Uh, but no, we've
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talked about it in 2026 and the web
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telescope has come to the rescue. Um,
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some people are disappointed, Andrew,
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because um,
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>> an asteroid hitting the moon uh,
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especially if you know when it's going
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to happen and you would know where it
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was going to happen as well. Uh, could
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have produced some um quite interesting
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pyrochnics. It would allow spectroscopy
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uh, which would tell you a little bit
00:06:05.919 --> 00:06:07.590
about the asteroid's makeup as well as
00:06:07.600 --> 00:06:09.590
the the makeup of the lunar regalith and
00:06:09.600 --> 00:06:12.230
the lunar lunar um, terrain that it
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smashed into. But that's not going to
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happen. Uh and so for anybody like
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astronauts who might happen to be
00:06:17.919 --> 00:06:20.790
hanging about on the moon in 2032 and
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there may well be both uh Chinese
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tyonauts and uh western astronauts on
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the moon by then. We'll um that that
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will be a great relief I'm sure.
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>> Yes. Yes. You don't really want a
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mission interrupted by a piece of an
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ice. Uh what would could you if if it
00:06:38.720 --> 00:06:40.870
did hit the moon? Let's just play that
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card for the moment. uh and you were
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looking at it at the time, would would
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you actually see it with the naked eye
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or with a telescope?
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>> I don't think you would with the naked
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eye, but you certainly would with
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telescopes and even maybe a relatively
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small telescope. We've known I mean
00:06:55.919 --> 00:06:58.469
certainly since the 1950s,
00:06:58.479 --> 00:07:02.550
uh that rocks do hit the moon. Um and
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often these are ones that are much
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smaller than the 60 m of Y4. Um it's for
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a long time I remember you know when I
00:07:12.720 --> 00:07:14.710
was first getting into astronomy in the
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1950s uh that um people talked and in
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particular Patrick Moore talked about
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these what what were called TLE's uh
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transient lunar events uh and there were
00:07:26.240 --> 00:07:28.070
flashes basically that amateur
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astronomers kept reporting said every so
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often there'd be something you know
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they'd be looking at the moon through a
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telescope and suddenly there'd be a
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flash. uh and for a long time it was not
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show not known really whether this was
00:07:41.599 --> 00:07:44.150
due to some sort of residual volcanic
00:07:44.160 --> 00:07:46.230
activity on the moon or whether it was
00:07:46.240 --> 00:07:49.270
impact of asteroids and and large meteor
00:07:49.280 --> 00:07:53.110
meteorites. Uh and um it was really once
00:07:53.120 --> 00:07:55.990
we seen the Apollo results and got to
00:07:56.000 --> 00:07:57.749
know the moon a lot better because of
00:07:57.759 --> 00:08:00.150
the Apollo missions that it it was
00:08:00.160 --> 00:08:02.390
deemed to be impacts that caused these
00:08:02.400 --> 00:08:05.749
transient lunar events. uh and so uh it
00:08:05.759 --> 00:08:08.070
would certainly be a 60 meter object
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hitting the moon is quite significant uh
00:08:10.560 --> 00:08:12.950
and that I don't think it would be naked
00:08:12.960 --> 00:08:15.909
eye visibility but I you probably
00:08:15.919 --> 00:08:17.430
wouldn't need that big a telescope to be
00:08:17.440 --> 00:08:18.550
able to see it.
00:08:18.560 --> 00:08:18.950
>> Wow.
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>> And so yes so yeah interesting
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>> and especially you know sorry especially
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if you could predict when and where it
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was going to happen you'd have all the
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amateur astronomers in the world of that
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side of the earth facing the moon. Yeah
00:08:31.280 --> 00:08:33.909
with eyes glued to your telescope. Yeah.
00:08:33.919 --> 00:08:37.670
Um, now just need you probably to
00:08:37.680 --> 00:08:41.190
explain how this works. But, uh, the
00:08:41.200 --> 00:08:43.110
scientists using the James Web took
00:08:43.120 --> 00:08:47.590
images 8 days apart. Is that that's
00:08:47.600 --> 00:08:49.350
obviously significant because then they
00:08:49.360 --> 00:08:52.470
get a straight line uh, observation. Is
00:08:52.480 --> 00:08:54.310
that how it works?
00:08:54.320 --> 00:08:57.750
>> No. What what happens is um, uh, in fact
00:08:57.760 --> 00:09:00.070
what even just one of those observations
00:09:00.080 --> 00:09:03.190
would have been invaluable. two is
00:09:03.200 --> 00:09:05.350
devastatingly invaluable. It makes it,
00:09:05.360 --> 00:09:07.350
you know, it increases your accuracy
00:09:07.360 --> 00:09:10.230
even more. Uh because what they do, they
00:09:10.240 --> 00:09:13.990
combine those new observations with what
00:09:14.000 --> 00:09:17.350
we knew from its orbit the last where
00:09:17.360 --> 00:09:21.350
when we observed it in 2024 25. So what
00:09:21.360 --> 00:09:23.430
you've suddenly got is you've you know
00:09:23.440 --> 00:09:25.430
the arc of observation might just have
00:09:25.440 --> 00:09:27.670
been a few months at the end of 2024
00:09:27.680 --> 00:09:30.470
early 2025. Now what you've done is
00:09:30.480 --> 00:09:33.990
you've extended that arc by a year
00:09:34.000 --> 00:09:36.550
effectively. Uh and that gives you a
00:09:36.560 --> 00:09:41.829
much much more accurate uh value of of
00:09:41.839 --> 00:09:43.750
uh what we call its orbital elements.
00:09:43.760 --> 00:09:47.829
The the asteroid um is its orbit is
00:09:47.839 --> 00:09:51.350
actually delineated by six numbers. Uh
00:09:51.360 --> 00:09:53.269
and those are the orbital elements as
00:09:53.279 --> 00:09:56.230
they're called. uh those numbers uh get
00:09:56.240 --> 00:09:59.269
more accurate the more uh the longer you
00:09:59.279 --> 00:10:01.590
can observe it for. So and and it's not
00:10:01.600 --> 00:10:03.269
just the how long you can observe it
00:10:03.279 --> 00:10:05.910
for. It's the interval between you know
00:10:05.920 --> 00:10:07.430
what's the interval of time between the
00:10:07.440 --> 00:10:08.949
observations which is what we've got
00:10:08.959 --> 00:10:11.269
here. We've suddenly got observations
00:10:11.279 --> 00:10:13.990
made a year later. It's it's absolutely
00:10:14.000 --> 00:10:15.910
narrowed down the uncertainties in the
00:10:15.920 --> 00:10:18.790
in the orbital elements. And so what we
00:10:18.800 --> 00:10:21.509
can then do is another great word from
00:10:21.519 --> 00:10:23.269
those orbital elements we can generate
00:10:23.279 --> 00:10:25.590
what's called an ephemeris and ephemeris
00:10:25.600 --> 00:10:27.190
tells you where the asteroid is going to
00:10:27.200 --> 00:10:29.190
be. It's a future predictions.
00:10:29.200 --> 00:10:32.630
>> That was what my MSE was on uh making
00:10:32.640 --> 00:10:36.230
orbital elements and uh fem
00:10:36.240 --> 00:10:39.030
of asteroids with a really new invention
00:10:39.040 --> 00:10:41.509
called computers.
00:10:41.519 --> 00:10:43.829
Yes. Yes. That I think that'll be a big
00:10:43.839 --> 00:10:45.670
hit.
00:10:45.680 --> 00:10:48.150
Well, it might be, hopefully not
00:10:48.160 --> 00:10:50.470
depending on where you're standing. It
00:10:50.480 --> 00:10:51.910
was certainly I'll tell you it was a big
00:10:51.920 --> 00:10:53.670
hit with the um with the external
00:10:53.680 --> 00:10:55.509
examiner, a gentleman in Glasgow
00:10:55.519 --> 00:10:57.590
University by the name of Archie Roy. He
00:10:57.600 --> 00:10:59.910
said, "Oh, this this work should be
00:10:59.920 --> 00:11:01.829
published. People should be able to read
00:11:01.839 --> 00:11:04.949
about this." Uh it never was, but uh the
00:11:04.959 --> 00:11:08.870
one copy is actually behind me.
00:11:08.880 --> 00:11:10.790
>> Yeah, it's one of the two thick volumes
00:11:10.800 --> 00:11:13.670
at the end. The other's my PhD thesis.
00:11:13.680 --> 00:11:15.590
I keep thinking of questions while we
00:11:15.600 --> 00:11:18.069
talk about this. Um, but what I what I
00:11:18.079 --> 00:11:20.230
find extraordinary is that the James Web
00:11:20.240 --> 00:11:22.470
Space Telescope was trying to find
00:11:22.480 --> 00:11:26.310
something 60 m in size from a distance
00:11:26.320 --> 00:11:29.190
of 48 million kilometers, 30 million
00:11:29.200 --> 00:11:29.910
miles.
00:11:29.920 --> 00:11:30.230
>> Yep.
00:11:30.240 --> 00:11:31.750
>> And it found it twice.
00:11:31.760 --> 00:11:33.910
>> It's pretty fantastic, isn't it?
00:11:33.920 --> 00:11:36.069
>> It would just pop above the the
00:11:36.079 --> 00:11:37.670
background noise. you know, when you
00:11:37.680 --> 00:11:39.110
when you're doing these observations,
00:11:39.120 --> 00:11:41.990
you've got various sources of what we
00:11:42.000 --> 00:11:43.350
call noise, which is basically
00:11:43.360 --> 00:11:46.310
uncertainty. Uh, and um, these are
00:11:46.320 --> 00:11:47.829
probably
00:11:47.839 --> 00:11:50.389
very close to that noise level, but it's
00:11:50.399 --> 00:11:52.550
just shown up enough that gives them
00:11:52.560 --> 00:11:53.990
what they call what we call a three
00:11:54.000 --> 00:11:56.069
sigma certainty. It's, you know, that's
00:11:56.079 --> 00:11:57.590
the level of certainty that you need.
00:11:57.600 --> 00:11:59.110
It's just a technical term for the
00:11:59.120 --> 00:12:01.910
statistical analysis that's being used.
00:12:01.920 --> 00:12:04.310
>> Um, I maybe they got help from AI as
00:12:04.320 --> 00:12:05.110
well. I don't know.
00:12:05.120 --> 00:12:08.230
>> Maybe. Yeah, it's possible. Um, I have a
00:12:08.240 --> 00:12:10.150
doomsday question though.
00:12:10.160 --> 00:12:11.190
>> Great.
00:12:11.200 --> 00:12:12.949
>> When, and we're going to talk about the
00:12:12.959 --> 00:12:14.790
dart mission next because there's new
00:12:14.800 --> 00:12:16.790
information about that uh, deflection
00:12:16.800 --> 00:12:20.150
test. But when do you intervene? Like if
00:12:20.160 --> 00:12:24.710
if we left it a couple of years because
00:12:24.720 --> 00:12:26.949
James Webb couldn't find it and then we
00:12:26.959 --> 00:12:28.629
realized it was going to hit Earth or
00:12:28.639 --> 00:12:31.110
something to that effect. When is it too
00:12:31.120 --> 00:12:34.550
late to intervene? it it's um with an
00:12:34.560 --> 00:12:37.030
asteroid like that it's almost too late
00:12:37.040 --> 00:12:40.150
already uh because you've only got so if
00:12:40.160 --> 00:12:42.710
we'd observed this in 2028 and the
00:12:42.720 --> 00:12:44.550
probability of an impact with Earth had
00:12:44.560 --> 00:12:47.190
gone up I mean it that had disappeared
00:12:47.200 --> 00:12:49.190
long ago so it's it's not a problem but
00:12:49.200 --> 00:12:52.230
if that happened you've only got four
00:12:52.240 --> 00:12:57.509
years uh and we're not ready quite yet
00:12:57.519 --> 00:13:00.150
to mount an emergency mission I think
00:13:00.160 --> 00:13:02.310
down the track we will be Having seen
00:13:02.320 --> 00:13:04.069
what come out of the story we're going
00:13:04.079 --> 00:13:05.910
to do next and
00:13:05.920 --> 00:13:08.949
>> um I think down the track we will have
00:13:08.959 --> 00:13:12.069
uh probably planetary defense uh rockets
00:13:12.079 --> 00:13:14.949
and spacecraft almost ready to go uh so
00:13:14.959 --> 00:13:17.190
that you could think about deflecting an
00:13:17.200 --> 00:13:18.870
object if it looked as though it was
00:13:18.880 --> 00:13:21.190
going to impact the earth but I suspect
00:13:21.200 --> 00:13:24.150
with four years that's not very long for
00:13:24.160 --> 00:13:26.470
a modified orbit to evolve into one that
00:13:26.480 --> 00:13:29.990
will miss the planet altogether. Um, uh,
00:13:30.000 --> 00:13:32.870
I think what would happen would be you'd
00:13:32.880 --> 00:13:36.230
you'd mobilize a civil defense, uh,
00:13:36.240 --> 00:13:38.629
resources because you'd probably quite
00:13:38.639 --> 00:13:40.870
quickly get an idea where the collision
00:13:40.880 --> 00:13:42.870
was going to be. You'd have a a circle
00:13:42.880 --> 00:13:44.870
of uncertainty, but you would know
00:13:44.880 --> 00:13:46.710
roughly where it was, which which side
00:13:46.720 --> 00:13:49.430
of the planet was going to be facing it.
00:13:49.440 --> 00:13:53.190
uh and a 60 m object. I mean, it's
00:13:53.200 --> 00:13:55.829
probably twice the size of what exploded
00:13:55.839 --> 00:13:59.670
over Chelabinsk uh in 2013. And we know
00:13:59.680 --> 00:14:03.030
that that caused structural damage when
00:14:03.040 --> 00:14:05.430
the shock wave hit the ground from 30
00:14:05.440 --> 00:14:08.310
kilometers high and it was the broken
00:14:08.320 --> 00:14:09.829
glass that caused all the injuries.
00:14:09.839 --> 00:14:12.629
Nobody died. Uh but but people did get
00:14:12.639 --> 00:14:14.870
injured. Um, and if you knew something
00:14:14.880 --> 00:14:17.030
like that was going to happen, uh, then
00:14:17.040 --> 00:14:19.030
you'd get the people out or get them in
00:14:19.040 --> 00:14:21.910
bunkers or whatever. Um, because it that
00:14:21.920 --> 00:14:23.430
that would be the most likely scenario,
00:14:23.440 --> 00:14:25.670
an air burst. It may be what happened at
00:14:25.680 --> 00:14:26.949
Tangaska actually.
00:14:26.959 --> 00:14:29.750
>> Yes.
00:14:29.760 --> 00:14:32.629
>> Yeah. I think the latest theory is it
00:14:32.639 --> 00:14:35.350
was actually a atmospheric graze rather
00:14:35.360 --> 00:14:37.910
than impact and caused
00:14:37.920 --> 00:14:40.150
>> explosion downwards. Yeah.
00:14:40.160 --> 00:14:42.949
>> Rading radiating out. Um the images from
00:14:42.959 --> 00:14:44.310
that are incredible. You can look them
00:14:44.320 --> 00:14:44.949
up on
00:14:44.959 --> 00:14:45.990
>> all the trees.
00:14:46.000 --> 00:14:48.310
>> Yeah. Just flattened. Unbelievable.
00:14:48.320 --> 00:14:49.030
Yeah.
00:14:49.040 --> 00:14:51.030
>> If you would like to read about the the
00:14:51.040 --> 00:14:53.430
latest observations uh regarding
00:14:53.440 --> 00:14:56.389
asteroid 2024 YR2, you can go to the
00:14:56.399 --> 00:14:58.790
scienceblog.com website or you can go to
00:14:58.800 --> 00:15:00.949
the issa website where they've published
00:15:00.959 --> 00:15:03.509
the findings. This is space nuts with
00:15:03.519 --> 00:15:06.710
Andrew Dunley and Professor Fred Watson.
00:15:06.720 --> 00:15:08.230
Let's take a break from the show to tell
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I believe that this nation should commit
00:16:41.920 --> 00:16:45.509
itself to achieving the goal before this
00:16:45.519 --> 00:16:48.230
decade is out of landing a man on the
00:16:48.240 --> 00:16:50.310
moon and returning him safely to the
00:16:50.320 --> 00:16:50.710
earth.
00:16:50.720 --> 00:16:52.150
>> These nuts.
00:16:52.160 --> 00:16:53.829
>> Well, we said we'd talk about it and we
00:16:53.839 --> 00:16:56.230
got to talk about it. The Dart mission.
00:16:56.240 --> 00:16:58.870
I think we should start by kind of just
00:16:58.880 --> 00:17:00.870
revisiting what that mission was all
00:17:00.880 --> 00:17:03.509
about and why. Well, we know why. to see
00:17:03.519 --> 00:17:06.069
if we could move something that may hit
00:17:06.079 --> 00:17:08.630
Earth one day off a bit so that it
00:17:08.640 --> 00:17:11.270
missed us. Uh I probably just explained
00:17:11.280 --> 00:17:13.350
it, but um yeah, this was four years
00:17:13.360 --> 00:17:14.870
ago, wasn't it, Fred?
00:17:14.880 --> 00:17:17.750
>> Uh indeed it was. That's right. 2022. Um
00:17:17.760 --> 00:17:20.870
it was I think it was it September. Uh I
00:17:20.880 --> 00:17:21.350
can't remember.
00:17:21.360 --> 00:17:22.150
>> Good question.
00:17:22.160 --> 00:17:25.510
>> About I think it was about then. Um the
00:17:25.520 --> 00:17:29.909
so a really really clever experiment uh
00:17:29.919 --> 00:17:33.029
conducted by NASA and a team of project
00:17:33.039 --> 00:17:35.990
scientists. Uh what do you do to test
00:17:36.000 --> 00:17:39.029
whether you can move an asteroid? What
00:17:39.039 --> 00:17:42.150
you don't do is slap something into an
00:17:42.160 --> 00:17:44.390
asteroid and see whether you can change
00:17:44.400 --> 00:17:46.710
its orbit around the sun. And that's
00:17:46.720 --> 00:17:49.110
because uh the orbits of planets,
00:17:49.120 --> 00:17:52.710
asteroids um and comets actually as well
00:17:52.720 --> 00:17:54.870
are very very stable. It's quite hard to
00:17:54.880 --> 00:17:56.789
change them. Uh because you're talking
00:17:56.799 --> 00:18:00.789
about, you know, lots of rather large
00:18:00.799 --> 00:18:02.630
forces, gravitational forces and things
00:18:02.640 --> 00:18:04.470
like that. So what they did was they
00:18:04.480 --> 00:18:06.390
said, "Okay, we won't do that. What
00:18:06.400 --> 00:18:07.909
we'll do is we'll find an asteroid with
00:18:07.919 --> 00:18:10.470
a a moon." Uh and we now know there are
00:18:10.480 --> 00:18:12.310
a lot of those. And they chose an
00:18:12.320 --> 00:18:15.350
asteroid called Ditimos. Uh if I
00:18:15.360 --> 00:18:16.950
remember rightly about half a kilometer
00:18:16.960 --> 00:18:19.669
across uh which had a little moon called
00:18:19.679 --> 00:18:24.230
Dorphos which is about I think 170 m is
00:18:24.240 --> 00:18:26.070
the figure that comes to mind. This
00:18:26.080 --> 00:18:28.230
little moon that goes around Diddimos
00:18:28.240 --> 00:18:30.390
once in I've got a feeling remembering
00:18:30.400 --> 00:18:32.230
it was about 11 hours its orbital
00:18:32.240 --> 00:18:34.630
period. So you smash something into the
00:18:34.640 --> 00:18:38.470
little asteroid moon. Uh, and what you
00:18:38.480 --> 00:18:41.350
then look for is how the orbit of the
00:18:41.360 --> 00:18:43.430
moon around its parent body, in other
00:18:43.440 --> 00:18:45.909
words, the moon, the orbit of Demorphos
00:18:45.919 --> 00:18:48.549
around Ditimos, how that changes because
00:18:48.559 --> 00:18:50.789
something on that scale is much easier
00:18:50.799 --> 00:18:53.110
to change than the orbit of an asteroid
00:18:53.120 --> 00:18:56.950
around the sun. Uh, and as we all know,
00:18:56.960 --> 00:18:59.190
it was incredibly successful. the orbit
00:18:59.200 --> 00:19:03.029
of the orbital period of um Demorphus I
00:19:03.039 --> 00:19:04.950
think it was reduced by was it 33
00:19:04.960 --> 00:19:08.070
minutes I think was the the figure um if
00:19:08.080 --> 00:19:11.029
I remember rightly the Dart spacecraft
00:19:11.039 --> 00:19:13.110
I'm remembering these numbers from the
00:19:13.120 --> 00:19:15.669
last time we talked about it I think it
00:19:15.679 --> 00:19:20.390
was um uh three tons I think thereabouts
00:19:20.400 --> 00:19:24.390
hit Demorphos at 6 kilometers/s
00:19:24.400 --> 00:19:27.510
caused a huge plume of data sorry a huge
00:19:27.520 --> 00:19:29.909
plume of debris not data, lots of data
00:19:29.919 --> 00:19:33.270
as well, but debris too. Um, and that
00:19:33.280 --> 00:19:35.510
was all in fact visible from Earth as
00:19:35.520 --> 00:19:37.669
well as from uh things like the Hubble
00:19:37.679 --> 00:19:40.390
Space Telescope. Uh, so it was a
00:19:40.400 --> 00:19:43.990
experiment that was well uh devised,
00:19:44.000 --> 00:19:46.710
well set up and had excellent results.
00:19:46.720 --> 00:19:49.830
It did exactly it did better than what
00:19:49.840 --> 00:19:51.750
um the mission scientists hoped. And the
00:19:51.760 --> 00:19:53.669
reason why it did better was because
00:19:53.679 --> 00:19:55.669
they there was a much bigger effect.
00:19:55.679 --> 00:19:57.909
It's when you hit something at 6
00:19:57.919 --> 00:20:00.470
kilometers/s, everything's vaporized.
00:20:00.480 --> 00:20:02.630
The the surface that you hit, which is
00:20:02.640 --> 00:20:04.150
actually a rubble pile, but the surface
00:20:04.160 --> 00:20:06.230
you hit vaporized, as is the spacecraft
00:20:06.240 --> 00:20:09.190
itself, and that vapor acts like a
00:20:09.200 --> 00:20:11.029
rocket exhaust. So, it's not just the
00:20:11.039 --> 00:20:13.190
nudge that you get from knocking
00:20:13.200 --> 00:20:15.110
something weighing three tons into an
00:20:15.120 --> 00:20:17.510
asteroid. Uh, it's also the sort of
00:20:17.520 --> 00:20:20.070
exhaust effect that comes from that uh
00:20:20.080 --> 00:20:25.110
as well. Um, so it uh and that that was
00:20:25.120 --> 00:20:27.029
what was very hard to quantify. We
00:20:27.039 --> 00:20:28.549
didn't really know what that would be,
00:20:28.559 --> 00:20:30.549
but it was enough to make a significant
00:20:30.559 --> 00:20:32.390
difference. So that's the backstory,
00:20:32.400 --> 00:20:33.110
Andrew.
00:20:33.120 --> 00:20:34.870
>> Yes. And you were right. It was the 26th
00:20:34.880 --> 00:20:37.190
of September, 2022.
00:20:37.200 --> 00:20:37.669
>> Okay.
00:20:37.679 --> 00:20:38.470
>> Great. Yeah.
00:20:38.480 --> 00:20:40.070
>> Yeah.
00:20:40.080 --> 00:20:41.990
Do you want to just check the mass of of
00:20:42.000 --> 00:20:44.070
the dart impactor while you're looking
00:20:44.080 --> 00:20:45.510
there? So
00:20:45.520 --> 00:20:47.510
>> correct if I've said it wrong. I said
00:20:47.520 --> 00:20:49.029
three tons, but I might be wrong. I
00:20:49.039 --> 00:20:51.669
can't remember. Okay, I'll do that. Um,
00:20:51.679 --> 00:20:53.990
but I guess we could uh move on to
00:20:54.000 --> 00:20:55.590
what's actually happened now. They've
00:20:55.600 --> 00:20:57.990
done more analysis and and something
00:20:58.000 --> 00:20:59.750
spectacular has happened as a
00:20:59.760 --> 00:21:01.750
consequence of that event three and a
00:21:01.760 --> 00:21:02.870
half years ago.
00:21:02.880 --> 00:21:05.270
>> And the way it's happened is neat as
00:21:05.280 --> 00:21:08.950
well because uh what you're looking for
00:21:08.960 --> 00:21:11.029
um if you're looking at the way an
00:21:11.039 --> 00:21:13.190
asteroid change an asteroid orbit
00:21:13.200 --> 00:21:16.070
changes, you're looking for incredible
00:21:16.080 --> 00:21:19.510
precision in space. uh and there are
00:21:19.520 --> 00:21:22.470
limits as to how precise we can get uh
00:21:22.480 --> 00:21:25.029
those measurements using telescopes.
00:21:25.039 --> 00:21:26.950
It's all about the position in space of
00:21:26.960 --> 00:21:29.430
the object. Telescopes are great at that
00:21:29.440 --> 00:21:33.190
of course but there is a better way uh
00:21:33.200 --> 00:21:35.590
for asteroids and that is to use
00:21:35.600 --> 00:21:38.789
occultations and an occultation is when
00:21:38.799 --> 00:21:41.510
an object like an asteroid passes in
00:21:41.520 --> 00:21:45.029
front of a star and you can predict this
00:21:45.039 --> 00:21:48.710
is going to happen. So what you do is
00:21:48.720 --> 00:21:52.630
for an object that's only 170 m across
00:21:52.640 --> 00:21:56.310
uh which is the size of demorphos um you
00:21:56.320 --> 00:21:59.190
you you've got what you do is you space
00:21:59.200 --> 00:22:02.310
astronomers along a line uh who are
00:22:02.320 --> 00:22:05.110
observing and because you you're not
00:22:05.120 --> 00:22:07.830
quite sure where the shadow of the
00:22:07.840 --> 00:22:10.470
asteroid casting the light of the star
00:22:10.480 --> 00:22:12.630
is going to fall. But with telescopes,
00:22:12.640 --> 00:22:14.470
what you can do is you can see the dip
00:22:14.480 --> 00:22:17.270
in a star's light as the asteroid passes
00:22:17.280 --> 00:22:18.470
in front of it. It's what we call
00:22:18.480 --> 00:22:20.710
noultation. And if you've got enough
00:22:20.720 --> 00:22:23.350
observers on the ground, it gives you a
00:22:23.360 --> 00:22:25.750
much higher level of precision as to
00:22:25.760 --> 00:22:28.230
where in the sky that asteroid is. And
00:22:28.240 --> 00:22:31.430
so that process was carried out um I
00:22:31.440 --> 00:22:35.430
think last year. Um and uh so that means
00:22:35.440 --> 00:22:37.750
that you've suddenly got very very
00:22:37.760 --> 00:22:40.070
accurate measurements of the position
00:22:40.080 --> 00:22:42.710
not just of of Dimorphus itself but also
00:22:42.720 --> 00:22:45.190
the parent asteroid Ditimos. In fact, I
00:22:45.200 --> 00:22:48.230
think it might be Ditimos um that was
00:22:48.240 --> 00:22:50.870
used for the occultation. And so the
00:22:50.880 --> 00:22:56.230
bottom line is uh that uh lo and behold
00:22:56.240 --> 00:22:58.549
it didn't just the impact didn't just
00:22:58.559 --> 00:23:01.270
change the orbit of Demorphos around
00:23:01.280 --> 00:23:03.830
Dillimos. It changed the orbit of the
00:23:03.840 --> 00:23:06.310
whole system, the pair of them around
00:23:06.320 --> 00:23:10.230
the sun. And that is the first time, one
00:23:10.240 --> 00:23:11.590
of the nice quotes in one of these
00:23:11.600 --> 00:23:13.590
articles, it's the first time a
00:23:13.600 --> 00:23:15.750
humanmade object has measurably altered
00:23:15.760 --> 00:23:17.750
the path of a celestial body around the
00:23:17.760 --> 00:23:20.390
sun. That's in a NASA statement.
00:23:20.400 --> 00:23:23.430
>> That is incredible. And of course, the
00:23:23.440 --> 00:23:25.430
obvious question is now, will we be able
00:23:25.440 --> 00:23:27.750
to track where it will go versus where
00:23:27.760 --> 00:23:29.430
it would have gone?
00:23:29.440 --> 00:23:31.909
>> Yes. And and indeed that's already sort
00:23:31.919 --> 00:23:34.070
of already happening because there'll be
00:23:34.080 --> 00:23:36.149
further observations and it's the same
00:23:36.159 --> 00:23:37.830
as we were just talking about in regard
00:23:37.840 --> 00:23:40.230
to Y4. The longer the arc of
00:23:40.240 --> 00:23:41.590
observations you've got, the more
00:23:41.600 --> 00:23:44.390
accurate uh your knowledge of its orbit.
00:23:44.400 --> 00:23:47.909
Now um the change in orbit is not much.
00:23:47.919 --> 00:23:52.549
Um I can't remember how many days um
00:23:52.559 --> 00:23:54.710
I've got the paper in front of me
00:23:54.720 --> 00:23:58.310
actually the the main paper. um it
00:23:58.320 --> 00:24:00.310
doesn't actually give us the the orbital
00:24:00.320 --> 00:24:02.870
period of the pair around the sun but
00:24:02.880 --> 00:24:05.510
they've changed that orbital period by
00:24:05.520 --> 00:24:09.830
wait for it it's.15 of a second so it's
00:24:09.840 --> 00:24:11.830
very I mean it's a matter of um you know
00:24:11.840 --> 00:24:15.110
it's it's these two orbit between the
00:24:15.120 --> 00:24:17.029
between the um orbits of Mars and
00:24:17.039 --> 00:24:18.070
Jupiter they're part of the main
00:24:18.080 --> 00:24:21.029
asteroid belt so they're their orbital
00:24:21.039 --> 00:24:23.590
periods are probably measured in sort of
00:24:23.600 --> 00:24:25.669
thousands of days or at least high
00:24:25.679 --> 00:24:28.310
numbers of hundreds of days uh and to
00:24:28.320 --> 00:24:31.510
change that by 0.15 of a second is not
00:24:31.520 --> 00:24:34.070
very much. It speaks wonders for the
00:24:34.080 --> 00:24:36.310
volumes for the uh accuracy with which
00:24:36.320 --> 00:24:39.110
the orbit has been determined. But uh
00:24:39.120 --> 00:24:41.830
it's look it it's it's it happened. It
00:24:41.840 --> 00:24:43.990
has actually happened that we've changed
00:24:44.000 --> 00:24:47.110
the orbit of an asteroid by hitting it
00:24:47.120 --> 00:24:50.470
or hitting its little moon in fact by uh
00:24:50.480 --> 00:24:52.549
with with a with a massive object. Did
00:24:52.559 --> 00:24:53.830
you manage to find out how much it
00:24:53.840 --> 00:24:56.630
weighed? 610 kg.
00:24:56.640 --> 00:24:59.510
>> Okay. That's 840 pounds.
00:24:59.520 --> 00:25:01.350
>> Yeah. So, it's less than a ton. Half a
00:25:01.360 --> 00:25:04.390
ton. Yeah. I apologize for three tons.
00:25:04.400 --> 00:25:06.710
That was the number from something else.
00:25:06.720 --> 00:25:08.149
>> I reckon if they if they could have got
00:25:08.159 --> 00:25:09.350
three tons up there, they would have
00:25:09.360 --> 00:25:09.750
used it.
00:25:09.760 --> 00:25:11.430
>> They would have done. Yeah. But but that
00:25:11.440 --> 00:25:13.190
makes it even more spectacular. You
00:25:13.200 --> 00:25:16.470
know, something weighing less than a car
00:25:16.480 --> 00:25:19.029
clouting a the moon of an asteroid can
00:25:19.039 --> 00:25:21.029
change the orbit of that asteroid and
00:25:21.039 --> 00:25:25.510
its parent body. Um just to very quickly
00:25:25.520 --> 00:25:27.669
since we're talking to a educated and
00:25:27.679 --> 00:25:30.070
erodendite audience here the mechanism
00:25:30.080 --> 00:25:33.029
by which that changed is so you think
00:25:33.039 --> 00:25:35.110
well you've hit the you've hit the moon
00:25:35.120 --> 00:25:37.750
asteroid how does that change the orbit
00:25:37.760 --> 00:25:40.390
of the parent asteroid and what it does
00:25:40.400 --> 00:25:42.789
hitting the moon asteroid gives you a
00:25:42.799 --> 00:25:44.950
slight change in the position of the
00:25:44.960 --> 00:25:47.350
barry center that's the center of mass
00:25:47.360 --> 00:25:49.350
of the two objects their center of
00:25:49.360 --> 00:25:53.110
gravity combined and it's that that has
00:25:53.120 --> 00:25:55.510
changed its orbit. It's the Barry center
00:25:55.520 --> 00:25:57.269
which of course includes both of the
00:25:57.279 --> 00:25:58.950
objects. The Barry center is
00:25:58.960 --> 00:26:00.950
representative of both Ditimos and
00:26:00.960 --> 00:26:02.950
Dimorphus because it's the center of
00:26:02.960 --> 00:26:04.870
mass between them. So changing the
00:26:04.880 --> 00:26:06.310
position of the Barry center or the
00:26:06.320 --> 00:26:08.470
orbit of the Barry center essentially
00:26:08.480 --> 00:26:10.470
changes the orbit of the asteroid which
00:26:10.480 --> 00:26:13.669
means that would something like that
00:26:13.679 --> 00:26:15.830
threatening the earth and you had enough
00:26:15.840 --> 00:26:17.990
enough years down the track for its
00:26:18.000 --> 00:26:19.750
orbit to evolve so that it would miss
00:26:19.760 --> 00:26:21.990
the earth. Uh, that might be a way to do
00:26:22.000 --> 00:26:22.549
it.
00:26:22.559 --> 00:26:24.310
>> Yeah, I know a few people named Barry
00:26:24.320 --> 00:26:25.750
and they're always wanting to be the
00:26:25.760 --> 00:26:29.590
center of attentive.
00:26:29.600 --> 00:26:31.350
>> It had to cut, didn't it? Yeah, it did.
00:26:31.360 --> 00:26:34.470
It did. Uh, it's a it's a great story.
00:26:34.480 --> 00:26:36.070
It's a great read. Uh, you can pick it
00:26:36.080 --> 00:26:38.789
up on the NASA website or you can go to
00:26:38.799 --> 00:26:40.549
fizz.org.
00:26:40.559 --> 00:26:42.149
Phys.
00:26:42.159 --> 00:26:43.909
I got to do that from now on because
00:26:43.919 --> 00:26:47.269
somebody came to us one day and said, "I
00:26:47.279 --> 00:26:49.750
can't find this fi.org
00:26:49.760 --> 00:26:50.789
thing
00:26:50.799 --> 00:26:55.350
>> cuz it's not it's fizz phys uh yes but
00:26:55.360 --> 00:26:56.870
uh it's great news out of that
00:26:56.880 --> 00:26:59.510
experiment three and a half years post
00:26:59.520 --> 00:27:02.310
event this is space nuts dunley with
00:27:02.320 --> 00:27:08.549
professor Fred Watson
00:27:08.559 --> 00:27:10.789
>> base here the angle has landed
00:27:10.799 --> 00:27:12.070
>> space nuts
00:27:12.080 --> 00:27:16.470
>> now to another piece of rock that has
00:27:16.480 --> 00:27:18.149
been getting a lot of attention in
00:27:18.159 --> 00:27:21.750
recent times I Atlas, the exo comet or
00:27:21.760 --> 00:27:23.350
exoaststeroid. Is it a comet or an
00:27:23.360 --> 00:27:24.390
asteroid? Fred,
00:27:24.400 --> 00:27:25.350
>> comet. Comet.
00:27:25.360 --> 00:27:27.669
>> Comet. Yeah. Uh, yeah. It appears that
00:27:27.679 --> 00:27:29.590
it's um it's very different from
00:27:29.600 --> 00:27:31.590
anything we've seen before to the point
00:27:31.600 --> 00:27:33.750
where it's uh raging through our solar
00:27:33.760 --> 00:27:38.149
system, stone drunk off its face.
00:27:38.159 --> 00:27:40.630
Not quite, but uh its chemical makeup is
00:27:40.640 --> 00:27:42.950
just way out of kilter with what we
00:27:42.960 --> 00:27:45.029
would have expected.
00:27:45.039 --> 00:27:47.430
>> Uh that's right. So, you know, this is
00:27:47.440 --> 00:27:49.510
uh three eyeatlas is definitely the gift
00:27:49.520 --> 00:27:53.350
that keeps on giving um because um what
00:27:53.360 --> 00:27:55.510
we've got is a free sample from another
00:27:55.520 --> 00:27:57.830
solar system that is careering through
00:27:57.840 --> 00:28:00.549
our own solar system and near enough for
00:28:00.559 --> 00:28:02.630
our telescopes to get details of it.
00:28:02.640 --> 00:28:05.990
It's now actually receding from Earth um
00:28:06.000 --> 00:28:09.830
and from the sun, but it's still
00:28:09.840 --> 00:28:13.750
producing um gases from its icy surface.
00:28:13.760 --> 00:28:16.310
It behaves exactly like a comet would
00:28:16.320 --> 00:28:19.110
from our own solar system. Gets near the
00:28:19.120 --> 00:28:22.789
sun. Uh the ice is basically turn into
00:28:22.799 --> 00:28:26.310
gas directly. They sublimate and uh what
00:28:26.320 --> 00:28:29.430
then happens is um we can sense what
00:28:29.440 --> 00:28:31.990
gases are there, what what chemical
00:28:32.000 --> 00:28:33.909
compounds are there by looking at the
00:28:33.919 --> 00:28:36.630
spectrum of the what we call the coma of
00:28:36.640 --> 00:28:38.549
the comet. That's the fuzzy area around
00:28:38.559 --> 00:28:40.710
it that's caused by all this outging
00:28:40.720 --> 00:28:44.470
material. And so, um, comet 3i Atlas has
00:28:44.480 --> 00:28:47.269
recently been the subject of pro
00:28:47.279 --> 00:28:49.830
probably the world's most powerful,
00:28:49.840 --> 00:28:51.029
well, certainly the world's most
00:28:51.039 --> 00:28:52.470
powerful millimeter wave radio
00:28:52.480 --> 00:28:55.590
telescope. Uh, the array in the high
00:28:55.600 --> 00:28:58.549
country of the Atakama, uh, the Alma
00:28:58.559 --> 00:29:00.630
telescope, the Atakama large millimeter
00:29:00.640 --> 00:29:04.710
submill array. Um, at about 5,000 mters
00:29:04.720 --> 00:29:06.870
high, not very far from San Pedro de
00:29:06.880 --> 00:29:10.070
Atakama. Uh, and when I went to try and
00:29:10.080 --> 00:29:11.830
get in their back door one time, I
00:29:11.840 --> 00:29:14.549
nearly um died because the air was so
00:29:14.559 --> 00:29:16.630
thin and we didn't get in the back door
00:29:16.640 --> 00:29:18.470
either.
00:29:18.480 --> 00:29:21.990
So, uh, never mind. Uh, ALMA is fabulous
00:29:22.000 --> 00:29:24.870
telescope. So, what's the story? Uh,
00:29:24.880 --> 00:29:29.430
ALMA uh, which is run by various
00:29:29.440 --> 00:29:31.750
different organizations. uh but the
00:29:31.760 --> 00:29:33.430
scientists who have been observing a
00:29:33.440 --> 00:29:36.630
three-ey atlas with it have looked at
00:29:36.640 --> 00:29:39.190
the fingerprints the spectral
00:29:39.200 --> 00:29:42.149
fingerprints of two molecules. One is
00:29:42.159 --> 00:29:45.190
methanol which is a type of alcohol and
00:29:45.200 --> 00:29:49.029
the other is hydrogen cyanide uh HCN.
00:29:49.039 --> 00:29:51.510
It's a an organic molecule very common
00:29:51.520 --> 00:29:55.350
in comets. Uh so both of those are found
00:29:55.360 --> 00:29:58.389
in comets in the solar system. But what
00:29:58.399 --> 00:30:00.710
is the surprise is the amount of
00:30:00.720 --> 00:30:05.990
methanol. Uh it's as the um NRO
00:30:06.000 --> 00:30:08.070
National Radio Astronomy Observatory
00:30:08.080 --> 00:30:11.669
press release says uh ThreeI Atlas is
00:30:11.679 --> 00:30:14.470
heavily enriched in methanol compared to
00:30:14.480 --> 00:30:17.190
hydrogen cyanide. Far beyond what is
00:30:17.200 --> 00:30:19.350
typically seen in comets born in our own
00:30:19.360 --> 00:30:20.389
solar system.
00:30:20.399 --> 00:30:23.430
>> You know, you know what it is, Fred?
00:30:23.440 --> 00:30:25.830
>> Wait for it. You're gonna love this one.
00:30:25.840 --> 00:30:28.470
It's inroxinated.
00:30:28.480 --> 00:30:31.990
>> Oh
00:30:32.000 --> 00:30:35.669
yes, I'll go with that. I um I know I
00:30:35.679 --> 00:30:37.750
can just invented a new word. Well, he
00:30:37.760 --> 00:30:39.430
did. Yes. And you probably need to be
00:30:39.440 --> 00:30:41.350
reasonably in Roxinating in order to
00:30:41.360 --> 00:30:42.389
invent it.
00:30:42.399 --> 00:30:45.190
>> Yeah, I suppose so. And it's so early
00:30:45.200 --> 00:30:45.510
anyway.
00:30:45.520 --> 00:30:47.909
>> Yes. So early in the day. That's right.
00:30:47.919 --> 00:30:50.070
>> Anyway, um the observing team just
00:30:50.080 --> 00:30:52.549
coming back to a state of back perfect
00:30:52.559 --> 00:30:55.830
back to reality, perfect sobriety. Um
00:30:55.840 --> 00:30:59.830
it's um methanol to hydrogen cyanide
00:30:59.840 --> 00:31:05.830
ratios of between 70 and 120 uh which
00:31:05.840 --> 00:31:09.750
means it's among the most methanol rich
00:31:09.760 --> 00:31:11.830
uh comets ever discovered. There's been
00:31:11.840 --> 00:31:14.389
a few in the solar system that have got
00:31:14.399 --> 00:31:17.510
high levels of methanol, but this is,
00:31:17.520 --> 00:31:19.990
you know, it's up there on the extreme
00:31:20.000 --> 00:31:23.590
end of this distribution. Um and and if
00:31:23.600 --> 00:31:25.430
I may, I'll just read from there's a
00:31:25.440 --> 00:31:27.830
very nice uh National Radio Astronomy
00:31:27.840 --> 00:31:30.470
Observatory press release on this uh
00:31:30.480 --> 00:31:32.950
which says these measurements imply that
00:31:32.960 --> 00:31:35.909
the icy material from three Atlas was
00:31:35.919 --> 00:31:39.750
formed by or experienced very different
00:31:39.760 --> 00:31:42.549
conditions uh from those that shape most
00:31:42.559 --> 00:31:45.190
comets in our own solar system. Previous
00:31:45.200 --> 00:31:46.950
work with the James Webb Space Telescope
00:31:46.960 --> 00:31:49.669
has shown that ThreeI Atlas had a coma
00:31:49.679 --> 00:31:52.070
dominated by carbon dioxide when it was
00:31:52.080 --> 00:31:54.389
far from the sun. And these new ALMA
00:31:54.399 --> 00:31:57.430
results add methanol as another unusual
00:31:57.440 --> 00:31:59.909
detail in its chemical inventory. It's a
00:31:59.919 --> 00:32:03.110
very nice paragraph. So, it is unusual.
00:32:03.120 --> 00:32:06.149
It's an object that shows all the
00:32:06.159 --> 00:32:07.909
characteristics of a comet, but we're
00:32:07.919 --> 00:32:10.710
seeing all the extremes. And and maybe
00:32:10.720 --> 00:32:12.710
that shouldn't surprise us because it we
00:32:12.720 --> 00:32:14.950
do know it has come from somewhere else,
00:32:14.960 --> 00:32:16.070
not our own.
00:32:16.080 --> 00:32:18.070
>> Prompts the question, does that mean
00:32:18.080 --> 00:32:19.990
where it's come from might be quite
00:32:20.000 --> 00:32:22.070
different to our system?
00:32:22.080 --> 00:32:23.750
>> Yeah, that it's Yes, that's right. It
00:32:23.760 --> 00:32:26.149
could, you know, it it would certainly
00:32:26.159 --> 00:32:30.149
lead credibility to any idea that um
00:32:30.159 --> 00:32:32.950
chemical ratios within other solar
00:32:32.960 --> 00:32:35.590
systems are not necessarily what we find
00:32:35.600 --> 00:32:37.990
here in our own solar system. In other
00:32:38.000 --> 00:32:39.830
words, you know, there could be quite
00:32:39.840 --> 00:32:41.669
different chemistry going on
00:32:41.679 --> 00:32:43.509
particularly in the early history of
00:32:43.519 --> 00:32:45.190
those solar systems. We think a lot of
00:32:45.200 --> 00:32:47.909
these compounds like methanol and
00:32:47.919 --> 00:32:50.149
hydrogen cyanide. Uh we think a lot of
00:32:50.159 --> 00:32:52.630
these are formed very early in the
00:32:52.640 --> 00:32:55.350
history of a solar system in the cold of
00:32:55.360 --> 00:32:58.149
space. Molecules, atoms combine together
00:32:58.159 --> 00:33:00.389
to form molecules. And we know that
00:33:00.399 --> 00:33:03.029
there is a very very rich chemistry out
00:33:03.039 --> 00:33:06.310
there which was kind of unexpected
00:33:06.320 --> 00:33:07.909
really. I mean when I was a young
00:33:07.919 --> 00:33:10.389
astronomer we thought always in terms of
00:33:10.399 --> 00:33:12.630
just elements. The elements that we can
00:33:12.640 --> 00:33:14.310
see in the atmospheres of stars,
00:33:14.320 --> 00:33:17.669
hydrogen, carbon, calcium, uh iron, all
00:33:17.679 --> 00:33:20.070
of those. But now such a lot of what we
00:33:20.080 --> 00:33:24.230
do with the um you know with the arsenal
00:33:24.240 --> 00:33:26.310
of wonderful astronomical instruments
00:33:26.320 --> 00:33:28.070
that we have today. We can look at the
00:33:28.080 --> 00:33:30.149
chemistry of these things, the actual
00:33:30.159 --> 00:33:33.110
chemical reactions that uh go on in the
00:33:33.120 --> 00:33:35.029
laboratory of deep space.
00:33:35.039 --> 00:33:36.710
>> Yeah. Uh, some something you don't know
00:33:36.720 --> 00:33:38.710
about Fred is he's been in astronomy so
00:33:38.720 --> 00:33:40.310
long that he got in trouble at school
00:33:40.320 --> 00:33:41.990
once for throwing an apple at Isaac
00:33:42.000 --> 00:33:44.470
Newton. So,
00:33:44.480 --> 00:33:45.269
true story.
00:33:45.279 --> 00:33:47.029
>> Yeah. Yeah. Yeah. Yeah. Yeah. I got the
00:33:47.039 --> 00:33:48.870
cane for that. But
00:33:48.880 --> 00:33:50.470
>> yeah, I got the cane a lot at school,
00:33:50.480 --> 00:33:52.149
too, but not for throwing apples. I did
00:33:52.159 --> 00:33:54.389
throw a sandwich at a teacher once, but
00:33:54.399 --> 00:33:56.230
um yeah, I was egged on to do that and I
00:33:56.240 --> 00:33:57.110
fell for it.
00:33:57.120 --> 00:33:58.950
>> Was it silly?
00:33:58.960 --> 00:34:00.630
>> No, no, I can't remember what was on.
00:34:00.640 --> 00:34:02.389
Probably something hideous that I ate
00:34:02.399 --> 00:34:04.549
when I was a kid. If you ragged on, it
00:34:04.559 --> 00:34:05.590
must have been an
00:34:05.600 --> 00:34:08.470
>> Yeah, that was was a very silly move and
00:34:08.480 --> 00:34:11.669
I'll always regret it. Um, okay. So, if
00:34:11.679 --> 00:34:14.069
you want to read about that uh what u
00:34:14.079 --> 00:34:17.270
constitutes a um a rather drunk rock in
00:34:17.280 --> 00:34:19.430
space, you can go to the NA National
00:34:19.440 --> 00:34:21.669
Radio Observatory website where they've
00:34:21.679 --> 00:34:24.470
published their findings. And Fred, that
00:34:24.480 --> 00:34:26.230
brings us to the end. Thank you so very
00:34:26.240 --> 00:34:27.190
much.
00:34:27.200 --> 00:34:28.869
>> It's a great pleasure, Andrew. Always
00:34:28.879 --> 00:34:30.629
good to chat. And we'll see you again
00:34:30.639 --> 00:34:33.990
next time. We will on a Q&A edition. Uh
00:34:34.000 --> 00:34:35.750
Fred Watson, Professor Fred Watson,
00:34:35.760 --> 00:34:37.669
astronomer at large, joining us every
00:34:37.679 --> 00:34:39.990
week, twice a week in fact, for Space
00:34:40.000 --> 00:34:42.790
Nuts. And uh if you would like to visit
00:34:42.800 --> 00:34:44.950
our website, please do. Uh one thing we
00:34:44.960 --> 00:34:47.829
could use for our Q&A episodes, uh audio
00:34:47.839 --> 00:34:49.669
questions, we are desperately short of
00:34:49.679 --> 00:34:51.990
them. There's some weird quirk that at
00:34:52.000 --> 00:34:54.389
the beginning of every year they dry up,
00:34:54.399 --> 00:34:55.829
and we don't know why that is an
00:34:55.839 --> 00:34:59.349
anomaly, but it is a thing. Uh but if
00:34:59.359 --> 00:35:00.390
you go to our website
00:35:00.400 --> 00:35:01.990
spacenutspodcast.com
00:35:02.000 --> 00:35:04.069
and click on the ask me anything tab at
00:35:04.079 --> 00:35:06.069
the top, it's just labeled AMA. You can
00:35:06.079 --> 00:35:08.710
send us your questions or comments. We
00:35:08.720 --> 00:35:10.470
uh welcome them. Don't forget to tell us
00:35:10.480 --> 00:35:11.990
who you are and where you're from. And
00:35:12.000 --> 00:35:14.230
thanks to Hugh in the studio who
00:35:14.240 --> 00:35:15.910
couldn't be with us today because he
00:35:15.920 --> 00:35:17.829
went out on a bender last night and got
00:35:17.839 --> 00:35:21.109
inroxicated. Boom boom. And from me,
00:35:21.119 --> 00:35:23.109
from me, Andrew Dunley, thanks for your
00:35:23.119 --> 00:35:24.630
company. See you on the next episode of
00:35:24.640 --> 00:35:27.190
Space Nuts. Bye-bye. Space Nuts.
00:35:27.200 --> 00:35:29.349
>> You'll be listening to the Space Nuts
00:35:29.359 --> 00:35:31.589
podcast
00:35:31.599 --> 00:35:34.550
>> available at Apple Podcasts, Spotify,
00:35:34.560 --> 00:35:37.190
iHeart Radio, or your favorite podcast
00:35:37.200 --> 00:35:39.589
player. You can also stream on demand at
00:35:39.599 --> 00:35:42.550
byes.com. This has been another quality
00:35:42.560 --> 00:35:47.000
podcast production from byes.com.




