Artemis 2 Success, ESO Fallout & The Intriguing World of X-Ray Binaries | Space Nuts: Astronomy...
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Artemis 2 Launch, Australian Astronomy Setbacks, and the Mystery of X-Ray Binaries
In this thrilling episode of Space Nuts , hosts Andrew Dunkley and Professor Fred Watson dive into the latest advancements in space exploration and the challenges faced by the Australian astronomy community. The successful launch of Artemis 2 marks a significant milestone for humanity's return to the Moon, while a recent government decision leaves Australian astronomers concerned about their future access to critical telescopes. The episode also explores the intriguing discovery of an X-ray binary that defies conventional understanding, revealing new mysteries in the cosmos.
Episode Highlights:
- Artemis 2 Launch: Andrew and Fred share their excitement over the successful launch of Artemis 2, discussing the mission's significance and the historic achievements of the crew as they become the first humans to travel further than Apollo 13.
- Australian Astronomy Challenges: The hosts delve into the Australian government's decision to discontinue its partnership with the European Southern Observatory, examining the potential impact on local astronomers and the future of optical astronomy in Australia.
- X-Ray Binary Discovery: A fascinating conversation unfolds around the discovery of two peculiar X-ray binaries that challenge existing theories, leading to discussions about the nature of these celestial objects and what they reveal about stellar evolution.
- Future of Astronomy: Andrew and Fred reflect on the implications of these developments for the broader astronomy community, contemplating the balance between funding, scientific advancement, and international collaboration.
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/32650573?utm_source=youtube
Kind: captions
Language: en
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Hello again. Thanks for joining us on
00:00:02.399 --> 00:00:06.070
this yet another edition of Space Nuts,
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where we talk astronomy and space
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science. My name is Andrew Dunley, your
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host. Great to have your company. Coming
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up on a fresh episode, Arteimus 2 making
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headlines for all the right reasons.
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What a sigh of relief that was. Did you
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watch the launch? I sure did. Uh, but
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some bad news for the Australia ESO
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deal, which has got astronomers upset.
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One in particular I can think of. what's
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his name again? And the discovery of an
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X-ray binary. That's all coming up in
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this edition of Space Nuts.
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>> 15 seconds. Guidance is internal. 10 9
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Ignition sequence start.
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>> Space Nuts.
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>> 5 4 3 2
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>> 1 2 3 4 5 5 4 3 2 1
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>> Space Nuts.
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>> Astronauts report. It feels good.
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>> Just wondering what an X-ray binary is.
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It sounds like something you could get
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arrested for. And joining us to talk
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about all of that is Professor Fred
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Watson, astronomer at large. Hello,
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Fred.
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>> Hello, Andrew. And uh I I pick you up on
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that because I nearly got arrested once
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for doing astronomy with a an old brass
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telescope in the front garden, which the
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neighbors thought was a bazooka. Uh and
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so I had a visit from a very large
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policeman. I think I was uh 16 or 17 at
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the time
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>> cuz these these days you'd get accused
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of of being a peeping tom or something,
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>> but back back then they thought it was a
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weapon.
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>> The reason why they do have weaponike,
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>> you know, looks them, don't they?
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>> Yeah, they look like a gun. That's
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right. The reason why I didn't um I
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didn't get uh any complaints about being
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a peeping tom was that our front garden
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overlooked the cemetery uh and there
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wasn't anybody around to complain.
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>> That's Yeah. Okay. Lots of things come
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to mind, but I'll I'll just I won't go
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there. Won't go there.
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>> No. But yes, like Yeah. When when was
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that?
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>> The early 1960s. Yeah. Uh-huh.
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>> Long after the Second World War, which
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is where why bazookas were on people's
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minds.
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>> Yeah. Yeah. Everyone was still super
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sensitive, I guess.
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>> Fred, it's been an exciting week. I know
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this is podcast, so some people will
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hear this well after the fact. But, uh,
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the other day, Artemis 2 lifted off very
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successfully, which was very, very
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exciting. And I watched it live on NASA
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live, which a lot of people did. There
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were tens of thousands of people logged
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on and the system held up and I just
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watched the whole thing. I had it on my
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computer. I sat there and I just I
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watched the whole hour build up to the
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to the launch and and watched it all
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unfold. And it went something like this.
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10 9 8 7 RS25 engines. 8 4 3 2 1 booster
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ignition and liftoff.
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The crew of Artemis 2 now bound for the
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moon. Humanity's next great voyage
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begins.
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>> How cool is that? How cool. And and
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those engines, the the sound of those
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engines, even over the over the internet
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on a on a shony microphone cuz NASA
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can't really afford good stuff. Um, no,
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that it sounded You want to hear that
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again? That that that that just the
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sound of the engines. Okay. All right.
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>> No, that was just me blowing into the
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microphone, but um yeah, fantastic
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stuff. Uh it was so exciting to watch. I
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um I really got a big kick out of it and
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uh you could hear the crowd cheering at
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one stage. It was so loud that the
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microphones picked up the crowd and um
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yeah it was an amazing moment and of
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course as we speak today they have
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reached the moon and done their lap.
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They went onto the dark side and uh all
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that loss talk was being spoken of with
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loss of signal. I mean, they were
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blocked out by a big rock and um and
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they achieved so much. I think uh yeah,
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it's been a pretty exciting week, hasn't
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it, Fred?
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>> You can say that again. And that um that
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live broadcast that you're talking
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about, um I've still got it on in
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this afternoon.
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>> Yeah, we're we're getting updates uh uh
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all the time. And you know, this is kind
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of NASA at his best, isn't it really?
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It's just uh such a fantastic
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achievement for us to see this mission
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uh going so profoundly well. Um uh you
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said the uh the trans traverse behind
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the moon has taken place. Uh now um
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there was a 40-minute loss of signal
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which you'd expect for exactly the
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reason that you mentioned. Uh the moon
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is a big rock and gets in the way of
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sign of radio signals. But also what the
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astronauts on board Arteimus saw was an
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eclipse of the sun. So the moon's disc
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actually covered the sun. Now from our
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vantage point on Earth, the sun and the
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moon look to be the same size. It's one
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of the most curious cosmic coincidences
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that we've got our satellite and the and
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our star which have the same angular
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size half a degree in the sky. But of
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course from the vantage point of the u
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of the Arteimus astronauts uh who are
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roughly 6,000 kilometers from the moon's
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surface at the moment uh the moon is is
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a lot bigger and so yes they did see an
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eclipse uh and as the moon covered the
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disc of the sun they would see first of
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all the inner atmosphere of the sun what
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we call the chromosphere which often has
00:05:39.520 --> 00:05:42.469
pink uh glowing clouds of hydrogen on it
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but more especially they would have seen
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the corona the sun's outer atmosphere,
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which is what uh captivates eclipse
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goers whenever they go and see a total
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eclipse of the sun. And I can't resist
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there a plug for 22nd of July, 2028 when
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a total eclipse of the sun uh will see
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the moon shadow passing over both where
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you're sitting at the moment in do and
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where I'm sitting at the moment in
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Sydney. That's going to be a huge event.
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Perhaps not quite as momentous as seeing
00:06:10.400 --> 00:06:12.469
it from a spacecraft on the far side of
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the moon, but still pretty good. uh and
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uh you know the the astronauts are
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indeed now on their way home. They in a
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sense they've been on their way home
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ever since they left Earth orbit because
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the trajectory that um that the rocket
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was inserted into the the Trans Luna
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insertion move uh which took place above
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the Earth's surface that that really
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placed them on on a path that inevitably
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would take them in a figure of eight uh
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loop around the moon and bring them back
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to Earth. Uh now there are midcourse
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connection sorry corrections. I think
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there is one planned for later today uh
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uh after which I think the um the
00:06:56.160 --> 00:06:58.230
astronauts are going to be given some
00:06:58.240 --> 00:07:00.230
time to themselves because they've been
00:07:00.240 --> 00:07:02.230
pretty hard at work in the last 24 hours
00:07:02.240 --> 00:07:04.950
with the with the lunar far side flyby.
00:07:04.960 --> 00:07:07.270
>> Absolutely. Uh they've achieved so much
00:07:07.280 --> 00:07:10.309
today. Um the four astronauts Reed
00:07:10.319 --> 00:07:13.749
Weisman, Victor Glover, Christina Ko or
00:07:13.759 --> 00:07:15.270
Kosh depending on how you want to
00:07:15.280 --> 00:07:17.350
pronounce it, Jeremy Hansen uh have
00:07:17.360 --> 00:07:21.189
become the um the first humans to go
00:07:21.199 --> 00:07:24.390
beyond where Apollo 13 set the record
00:07:24.400 --> 00:07:26.629
for the first furthest distance for
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humans from Earth. So they are now world
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record holders. Is it a world record
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when you're not on the world?
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>> I don't
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It's a solar system record. Yes, the um
00:07:39.599 --> 00:07:42.629
yes indeed the distance 47,000
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kilometers from Earth
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>> uh which uh and I think it was about
00:07:47.599 --> 00:07:50.790
400,000 that the Apollo 13 astronauts
00:07:50.800 --> 00:07:53.270
flew out. So it's a significant increase
00:07:53.280 --> 00:07:55.189
from that more than 6,000 km.
00:07:55.199 --> 00:07:57.909
>> So the most isolated humans in history
00:07:57.919 --> 00:07:59.029
in real terms.
00:07:59.039 --> 00:08:01.270
>> Yes, in a that's right in a sense. Um
00:08:01.280 --> 00:08:03.110
and they probably felt like that when
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they were out of communication for that
00:08:04.560 --> 00:08:06.550
40 minutes when they were in the moon
00:08:06.560 --> 00:08:08.790
shadow from radio signals from Earth.
00:08:08.800 --> 00:08:12.390
>> M yeah and uh one while I was listening
00:08:12.400 --> 00:08:15.909
to the live broadcast uh this afternoon
00:08:15.919 --> 00:08:19.110
our time uh I heard them talking about
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seeing uh meteorite flashes on the
00:08:21.919 --> 00:08:24.309
surface of the moon. They they spotted
00:08:24.319 --> 00:08:28.150
uh three four impacts while they were um
00:08:28.160 --> 00:08:29.909
rounding the moon which I I find
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astounding and it was really exciting
00:08:31.440 --> 00:08:33.430
for everybody especially the science
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team that were talking to them at that
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moment.
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>> Now that I didn't hear so that's great.
00:08:39.360 --> 00:08:39.829
That's great.
00:08:39.839 --> 00:08:42.070
>> Yeah. Quite incredible. Yeah. So, you
00:08:42.080 --> 00:08:43.670
know, things are happening that you just
00:08:43.680 --> 00:08:46.389
you wouldn't. And and apparently where
00:08:46.399 --> 00:08:49.110
the where these impacts happened, people
00:08:49.120 --> 00:08:50.949
on Earth who were observing the moon at
00:08:50.959 --> 00:08:53.509
the time may well have seen them, too.
00:08:53.519 --> 00:08:56.630
>> So, um I don't know if it's just a
00:08:56.640 --> 00:08:58.150
coincidence. We just happen to have a
00:08:58.160 --> 00:09:00.070
spaceship right there at the time or
00:09:00.080 --> 00:09:01.590
this happens a lot.
00:09:01.600 --> 00:09:03.190
>> I think it's happening a lot. I think
00:09:03.200 --> 00:09:06.230
that's the bottom line. It's um um you
00:09:06.240 --> 00:09:08.150
know these things have been observed
00:09:08.160 --> 00:09:10.070
actually since the 1950s when they were
00:09:10.080 --> 00:09:12.550
called transient lunar events which we
00:09:12.560 --> 00:09:14.949
now know are as you said meteorite
00:09:14.959 --> 00:09:19.110
impacts. Um I also noted that uh two
00:09:19.120 --> 00:09:22.150
relatively fresh and unnamed craters
00:09:22.160 --> 00:09:25.430
have been uh given a name by the uh
00:09:25.440 --> 00:09:28.550
astronauts. One is is integrity which is
00:09:28.560 --> 00:09:30.550
the name of the spacecraft and the other
00:09:30.560 --> 00:09:32.470
is Carol which is the name of Reed
00:09:32.480 --> 00:09:34.870
Wiseman's late wife who died a few years
00:09:34.880 --> 00:09:35.910
ago.
00:09:35.920 --> 00:09:39.430
>> Yeah. Lovely lovely stuff. Yeah.
00:09:39.440 --> 00:09:42.070
>> Yeah. And more more to be written I
00:09:42.080 --> 00:09:45.030
suppose as this mission unfolds. Um and
00:09:45.040 --> 00:09:48.389
and so far so good. um and a whole new
00:09:48.399 --> 00:09:50.630
generation um feeling the same
00:09:50.640 --> 00:09:53.670
excitement we did back in the 60s and
00:09:53.680 --> 00:09:56.310
70s when the Apollo missions did exactly
00:09:56.320 --> 00:09:58.949
the same thing. This this flyby is
00:09:58.959 --> 00:10:01.430
probably a replication of what Apollo 8
00:10:01.440 --> 00:10:02.630
I think
00:10:02.640 --> 00:10:04.870
>> very much. Yeah, very similar to Apollo
00:10:04.880 --> 00:10:07.750
8. December 1968 I remember it well.
00:10:07.760 --> 00:10:09.670
>> Christmas was
00:10:09.680 --> 00:10:11.750
>> it was Yeah, that's right. Christmas Eve
00:10:11.760 --> 00:10:12.949
I think it might have been but it
00:10:12.959 --> 00:10:15.670
depends on your time zone. It's sort of
00:10:15.680 --> 00:10:17.670
um occurred to me a couple of times. I'm
00:10:17.680 --> 00:10:22.389
kind of rambling a bit now, but um in a
00:10:22.399 --> 00:10:25.269
perhaps a quai Trumpian manner. Uh but
00:10:25.279 --> 00:10:27.990
um I think it's really interesting to me
00:10:28.000 --> 00:10:30.710
because my career in astronomy, my
00:10:30.720 --> 00:10:32.310
working career in astronomy is kind of
00:10:32.320 --> 00:10:36.230
bookended by lunar missions. Um because
00:10:36.240 --> 00:10:37.990
it was early in my career that we were
00:10:38.000 --> 00:10:39.990
watching all the Apollo flights and I
00:10:40.000 --> 00:10:41.750
don't think anyone even with the best
00:10:41.760 --> 00:10:43.509
will in the world would deny that I'm
00:10:43.519 --> 00:10:46.150
now late in my career and we've got the
00:10:46.160 --> 00:10:48.310
Optimus excitement coming as well. It's
00:10:48.320 --> 00:10:50.710
just great stuff. It is fabulous stuff
00:10:50.720 --> 00:10:52.710
and you can read all about it or even
00:10:52.720 --> 00:10:55.750
watch it live as it happens which we
00:10:55.760 --> 00:10:57.590
really couldn't do back in the 60s and
00:10:57.600 --> 00:10:59.430
70s. Not like this. We had to rely on
00:10:59.440 --> 00:11:01.590
television but now you can just log on
00:11:01.600 --> 00:11:04.230
to NASA live and watch it all happen in
00:11:04.240 --> 00:11:07.350
real time. s. Fantastic stuff. Yeah. Uh,
00:11:07.360 --> 00:11:09.030
so more more to talk about down the
00:11:09.040 --> 00:11:10.949
track, I'm sure, but uh, if you've been
00:11:10.959 --> 00:11:12.550
following it, well, you probably know
00:11:12.560 --> 00:11:14.790
more than we do. This is Space Nuts with
00:11:14.800 --> 00:11:18.949
Andrew Dunley and Professor Fred Watson.
00:11:18.959 --> 00:11:21.430
Let's take a short break from Space Nuts
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>> The crew of Artemis 2 now bound for the
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moon. Humanity's next great voyage
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begins.
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>> Space nuts. Now Fred, we go from
00:13:00.720 --> 00:13:04.150
excitement to something um quite uh
00:13:04.160 --> 00:13:06.629
upsetting for Australian astronomers,
00:13:06.639 --> 00:13:09.190
including yourself, and that is an
00:13:09.200 --> 00:13:10.710
announcement by the Australian
00:13:10.720 --> 00:13:14.470
government to um discontinue
00:13:14.480 --> 00:13:18.230
uh the the deal with um the European
00:13:18.240 --> 00:13:20.389
Southern Observatory. It's uh all over
00:13:20.399 --> 00:13:22.949
Red Rover by the sound of it.
00:13:22.959 --> 00:13:28.629
>> Uh yes. Yes, we still hope for um
00:13:28.639 --> 00:13:31.190
something to come out of all this, but
00:13:31.200 --> 00:13:33.590
the backstory here is that Australian
00:13:33.600 --> 00:13:37.750
astronomers uh since 2017 have had
00:13:37.760 --> 00:13:40.710
access to the best telescopes in the
00:13:40.720 --> 00:13:42.230
southern hemisphere without question,
00:13:42.240 --> 00:13:43.910
the best optical telescopes anyway,
00:13:43.920 --> 00:13:45.750
visible light telescopes, which are
00:13:45.760 --> 00:13:47.110
operated by the European Southern
00:13:47.120 --> 00:13:48.629
Observatory, whose headquarters are in
00:13:48.639 --> 00:13:51.910
Munich uh and whose telescopes are in
00:13:51.920 --> 00:13:55.990
northern Chile. uh and um those
00:13:56.000 --> 00:13:57.829
principally the the biggest uh
00:13:57.839 --> 00:14:01.110
telescopes are the four 8.2 2 meter
00:14:01.120 --> 00:14:03.509
components of what's called the VT the
00:14:03.519 --> 00:14:07.269
very large telescope uh which have been
00:14:07.279 --> 00:14:09.110
you know so which um Australian
00:14:09.120 --> 00:14:10.870
astronomers have have had access to
00:14:10.880 --> 00:14:14.710
since 2017 uh and has been a highly
00:14:14.720 --> 00:14:16.710
productive arrangement not just for the
00:14:16.720 --> 00:14:18.790
astronomers but also because our
00:14:18.800 --> 00:14:20.629
instrument builders here in Australia
00:14:20.639 --> 00:14:21.750
the people who build the fancy
00:14:21.760 --> 00:14:23.509
instruments that go on the back of
00:14:23.519 --> 00:14:28.230
telescopes um are um they are have have
00:14:28.240 --> 00:14:29.990
excelled themselves with what they've
00:14:30.000 --> 00:14:33.189
achieved uh because of the you know the
00:14:33.199 --> 00:14:35.590
opportunities to build a kit for these
00:14:35.600 --> 00:14:39.030
giant telescopes. So and plus all the
00:14:39.040 --> 00:14:41.750
spin-offs in terms of education and STEM
00:14:41.760 --> 00:14:43.590
and outreach and all the rest of it
00:14:43.600 --> 00:14:46.870
which we've tried to capitalize on. Um
00:14:46.880 --> 00:14:49.990
but that partnership was always going to
00:14:50.000 --> 00:14:54.069
be a 10-year deal. So 2017 to 2027, it
00:14:54.079 --> 00:14:56.790
comes to an end in December next year.
00:14:56.800 --> 00:15:00.389
>> And uh we in the astronomy community uh
00:15:00.399 --> 00:15:01.990
I started worrying about this actually
00:15:02.000 --> 00:15:04.870
in 2018. Uh what was going to happen
00:15:04.880 --> 00:15:08.069
next uh and to to make a case for the
00:15:08.079 --> 00:15:10.470
next step which would have to be
00:15:10.480 --> 00:15:12.550
according to the rules of the European
00:15:12.560 --> 00:15:14.389
Southern Observatory would have to be
00:15:14.399 --> 00:15:17.910
full membership. Um and that is the
00:15:17.920 --> 00:15:22.790
stumbling block because whilst um whilst
00:15:22.800 --> 00:15:25.350
10 years of strategic partnership were
00:15:25.360 --> 00:15:28.870
valued at 129 million Australian
00:15:28.880 --> 00:15:32.550
dollars, 10 years of full membership is
00:15:32.560 --> 00:15:36.389
$400 million uh nearly half a billion
00:15:36.399 --> 00:15:38.389
and that is something that governments
00:15:38.399 --> 00:15:41.829
don't like big numbers like that. uh and
00:15:41.839 --> 00:15:43.910
especially in times of financial
00:15:43.920 --> 00:15:46.550
stringent which we understand. Um
00:15:46.560 --> 00:15:49.110
however we do think that the government
00:15:49.120 --> 00:15:50.790
could have looked rather more
00:15:50.800 --> 00:15:52.870
constructively at other possible
00:15:52.880 --> 00:15:55.829
opportunities uh before making this
00:15:55.839 --> 00:15:58.150
announcement. Uh and there may be still
00:15:58.160 --> 00:16:00.629
scope for that. Um we've you know we've
00:16:00.639 --> 00:16:03.269
discussed things like uh Australian
00:16:03.279 --> 00:16:05.749
astronomers making inind contributions
00:16:05.759 --> 00:16:08.710
to ESO European Southern Observatory by
00:16:08.720 --> 00:16:11.670
for example building uh instruments in
00:16:11.680 --> 00:16:13.189
including the possibility of a new
00:16:13.199 --> 00:16:15.990
telescope here in Australia that could
00:16:16.000 --> 00:16:21.509
be uh actually um installed in the site
00:16:21.519 --> 00:16:24.470
near the site where the VT very large
00:16:24.480 --> 00:16:26.790
telescope uh unit instruments are
00:16:26.800 --> 00:16:28.710
situated at place called Sarah for
00:16:28.720 --> 00:16:30.790
paranal. Perhaps the most glawing thing
00:16:30.800 --> 00:16:33.189
about this though, Andrew, is that we
00:16:33.199 --> 00:16:35.910
have uh
00:16:35.920 --> 00:16:39.030
our membership, if we were to become
00:16:39.040 --> 00:16:41.829
members of ESO, would give us access to
00:16:41.839 --> 00:16:45.269
what is going to be the most stupendous
00:16:45.279 --> 00:16:47.269
telescope in the world when it comes on
00:16:47.279 --> 00:16:49.910
stream early in 2029. That is the
00:16:49.920 --> 00:16:52.389
European Southern Observatory's ELT or
00:16:52.399 --> 00:16:55.509
extremely large telescope. Sorry, one
00:16:55.519 --> 00:16:57.749
>> that's the one that that's as good a
00:16:57.759 --> 00:16:59.110
title because that's what it's going to
00:16:59.120 --> 00:17:03.269
be. Uh 39 meter diameter mirror. The the
00:17:03.279 --> 00:17:06.309
mirror diameter is 10 times that of the
00:17:06.319 --> 00:17:07.750
biggest telescope in Australia, the
00:17:07.760 --> 00:17:09.189
Anglo Australian telescope that I used
00:17:09.199 --> 00:17:11.029
to be astronomer in charge of. It's 10
00:17:11.039 --> 00:17:13.029
times bigger, which gives you a 100
00:17:13.039 --> 00:17:15.110
times the the sensitivity in terms of
00:17:15.120 --> 00:17:17.110
light gathering power and plus many
00:17:17.120 --> 00:17:19.270
other benefits. That will come on stream
00:17:19.280 --> 00:17:22.549
2029. Um it is sure to generate Nobel
00:17:22.559 --> 00:17:25.110
prizes. uh Australian astronomers will
00:17:25.120 --> 00:17:26.949
be barred from that and the great pity
00:17:26.959 --> 00:17:29.270
of that is uh that Australian
00:17:29.280 --> 00:17:32.710
astronomers have access uh to the square
00:17:32.720 --> 00:17:34.710
kilometer array which will come online
00:17:34.720 --> 00:17:37.270
at about the same time. Uh and to have
00:17:37.280 --> 00:17:39.990
those two things together under the you
00:17:40.000 --> 00:17:42.230
know the opaces of Australian astronomy
00:17:42.240 --> 00:17:44.150
would have given them a head start over
00:17:44.160 --> 00:17:46.630
the whole world in terms of discoveries.
00:17:46.640 --> 00:17:48.470
uh because the two things absolutely
00:17:48.480 --> 00:17:52.150
dovetail together the SKA and the uh ESO
00:17:52.160 --> 00:17:55.029
ELT that is not now going to happen and
00:17:55.039 --> 00:17:57.270
we feel that's a wasted opportunity and
00:17:57.280 --> 00:18:00.390
I might just add one more thing if I may
00:18:00.400 --> 00:18:03.510
because this is um this is a you know uh
00:18:03.520 --> 00:18:05.510
it is something very close to my heart
00:18:05.520 --> 00:18:07.029
I've worked very hard on this for the
00:18:07.039 --> 00:18:10.230
last almost decade um there is a there
00:18:10.240 --> 00:18:14.070
was a report that came out uh last month
00:18:14.080 --> 00:18:17.270
written by one of the country's senior
00:18:17.280 --> 00:18:18.789
economists
00:18:18.799 --> 00:18:21.430
uh a man named Professor Richard Holden
00:18:21.440 --> 00:18:23.430
and uh he's at the University of New
00:18:23.440 --> 00:18:25.990
South Wales here in Australia. He has
00:18:26.000 --> 00:18:28.630
done an analysis of the economic
00:18:28.640 --> 00:18:32.630
benefits of astronomy. Not just about,
00:18:32.640 --> 00:18:34.549
you know, the deals that you can do
00:18:34.559 --> 00:18:36.150
where you get money to build instruments
00:18:36.160 --> 00:18:37.830
and things of that sort. It's about the
00:18:37.840 --> 00:18:40.549
value of ideas, the the spin-offs that
00:18:40.559 --> 00:18:44.470
we have. All of those things um are
00:18:44.480 --> 00:18:46.710
taken into account in a report he wrote
00:18:46.720 --> 00:18:50.150
and he makes the point uh in conclusion
00:18:50.160 --> 00:18:52.630
in that report that Australian astronomy
00:18:52.640 --> 00:18:57.029
adds about $330 million per year to the
00:18:57.039 --> 00:19:00.070
country's economy. Uh which makes $40
00:19:00.080 --> 00:19:03.110
million a year for the ESO deal seem
00:19:03.120 --> 00:19:05.110
really quite proportionate. uh there
00:19:05.120 --> 00:19:07.029
would be a huge return on that $40
00:19:07.039 --> 00:19:09.909
million uh in terms of other benefits
00:19:09.919 --> 00:19:11.510
and that's what the government's missing
00:19:11.520 --> 00:19:12.390
out on. Yeah.
00:19:12.400 --> 00:19:13.830
>> Yeah. I think when we talked about this
00:19:13.840 --> 00:19:17.270
a few episodes ago u because we knew
00:19:17.280 --> 00:19:19.029
which was coming up
00:19:19.039 --> 00:19:21.190
>> um
00:19:21.200 --> 00:19:23.110
I I said something flippant like you
00:19:23.120 --> 00:19:24.630
know the left hand probably won't know
00:19:24.640 --> 00:19:27.029
what what the right hand's doing. So the
00:19:27.039 --> 00:19:29.990
the cost benefit versus cost, you know,
00:19:30.000 --> 00:19:32.390
the the benefit versus cost analysis may
00:19:32.400 --> 00:19:35.029
not get on the right desk and the
00:19:35.039 --> 00:19:37.190
decision could go against you. And I I
00:19:37.200 --> 00:19:40.310
was being a a smarty pants, but kind of
00:19:40.320 --> 00:19:41.830
looks like that's what's happened.
00:19:41.840 --> 00:19:45.590
>> Yeah. I don't actually I think it's uh
00:19:45.600 --> 00:19:47.990
different from that because um we made
00:19:48.000 --> 00:19:50.070
sure that the people who are making the
00:19:50.080 --> 00:19:52.710
decisions um and it's not Jordi by the
00:19:52.720 --> 00:19:54.549
way, but he makes his own decisions. I
00:19:54.559 --> 00:19:56.070
don't know whether you heard that.
00:19:56.080 --> 00:19:56.630
>> I did.
00:19:56.640 --> 00:19:58.150
>> The people Yeah. the people who were
00:19:58.160 --> 00:20:01.190
making the decisions um had access to
00:20:01.200 --> 00:20:03.190
that report. We made that very clear as
00:20:03.200 --> 00:20:06.789
soon as it came out. Um now um I'm
00:20:06.799 --> 00:20:09.029
suspect that the minister and his
00:20:09.039 --> 00:20:10.950
science advisers would also have had
00:20:10.960 --> 00:20:13.350
access to it. Uh so what they've done is
00:20:13.360 --> 00:20:14.870
they've turned their backs on that and
00:20:14.880 --> 00:20:17.430
they've turned their backs on on
00:20:17.440 --> 00:20:20.710
something that is very exciting in
00:20:20.720 --> 00:20:22.230
relation to our exploration of the
00:20:22.240 --> 00:20:24.549
universe at the very time when everybody
00:20:24.559 --> 00:20:26.150
else is looking skyward because of
00:20:26.160 --> 00:20:30.549
Arteimus. We we had this news on the day
00:20:30.559 --> 00:20:33.750
of the Arteimus 2 launch. Uh couldn't
00:20:33.760 --> 00:20:35.909
have been a bigger contrast between the
00:20:35.919 --> 00:20:37.590
two stories. And and where does this
00:20:37.600 --> 00:20:40.390
leave the likes of um the Australian
00:20:40.400 --> 00:20:42.310
Space Agency for example? I mean the
00:20:42.320 --> 00:20:45.190
government's established that or a
00:20:45.200 --> 00:20:46.630
former government did and they've been
00:20:46.640 --> 00:20:48.870
pouring money into it. Now now they've
00:20:48.880 --> 00:20:50.870
sort of shot the door in your face in
00:20:50.880 --> 00:20:54.149
regard to um
00:20:54.159 --> 00:20:57.669
the Europe the the um the work
00:20:57.679 --> 00:20:58.470
observatory.
00:20:58.480 --> 00:21:02.070
>> Yes, exactly. ESO um you know where does
00:21:02.080 --> 00:21:04.710
this put everything? Are we kind of
00:21:04.720 --> 00:21:06.950
going back to the dark ages?
00:21:06.960 --> 00:21:09.029
>> Um, no, no pun intended.
00:21:09.039 --> 00:21:10.789
>> No, no pun intended. No, we are going
00:21:10.799 --> 00:21:13.190
back probably several decades for
00:21:13.200 --> 00:21:15.750
Australian optical astronomy. But
00:21:15.760 --> 00:21:19.750
>> um the space agency has been likewise
00:21:19.760 --> 00:21:22.230
um chastised, if I can put it that way.
00:21:22.240 --> 00:21:26.230
They had large budget taken off them by
00:21:26.240 --> 00:21:28.950
the present government about three two
00:21:28.960 --> 00:21:31.590
three years ago. Uh, and I actually
00:21:31.600 --> 00:21:33.669
wonder if some of this is political
00:21:33.679 --> 00:21:36.870
because the space agency was was uh
00:21:36.880 --> 00:21:39.669
initiated by a previous government. Uh,
00:21:39.679 --> 00:21:42.390
and the ESO strategic partnership was
00:21:42.400 --> 00:21:44.549
initiated by a previous government of
00:21:44.559 --> 00:21:47.110
opposite flavor to what we have now.
00:21:47.120 --> 00:21:49.270
>> Um, so there might be a political side
00:21:49.280 --> 00:21:51.110
to it. I'm sure the minister would deny
00:21:51.120 --> 00:21:54.149
that. It takes all of
00:21:54.159 --> 00:21:57.270
>> course he would. that um I've seen
00:21:57.280 --> 00:21:59.270
politics in action and I I I can tell
00:21:59.280 --> 00:22:01.350
you quite clearly we I'll give you an
00:22:01.360 --> 00:22:03.270
example. We we were going to get a big
00:22:03.280 --> 00:22:05.510
sports hub in do
00:22:05.520 --> 00:22:08.070
and uh it was announced by our local
00:22:08.080 --> 00:22:11.510
member who was also the leader of um his
00:22:11.520 --> 00:22:14.950
party at the time and when they lost the
00:22:14.960 --> 00:22:18.549
next election the new premier of the
00:22:18.559 --> 00:22:21.270
opponent party took the money away and
00:22:21.280 --> 00:22:23.350
said no you can't have it.
00:22:23.360 --> 00:22:26.390
>> Yeah. and that that was purely political
00:22:26.400 --> 00:22:28.390
to you just basically to slap an
00:22:28.400 --> 00:22:31.510
opposition leader in the face and yes
00:22:31.520 --> 00:22:33.669
they would deny it but it's absolutely
00:22:33.679 --> 00:22:35.270
that's just the way the game is played
00:22:35.280 --> 00:22:37.750
all over the world. Um this is really
00:22:37.760 --> 00:22:40.710
sad really really sad that it's it's
00:22:40.720 --> 00:22:43.750
come to this any any hope Fred of some
00:22:43.760 --> 00:22:45.830
turnaround some chance of
00:22:45.840 --> 00:22:47.830
>> there's always there's always hope um I
00:22:47.840 --> 00:22:48.789
I
00:22:48.799 --> 00:22:51.190
>> maybe not after what I just said but you
00:22:51.200 --> 00:22:51.510
know
00:22:51.520 --> 00:22:51.990
>> it's okay
00:22:52.000 --> 00:22:54.149
>> I'm not an astronomer. No, no, no,
00:22:54.159 --> 00:22:56.070
nobody nobody listens to this. It's
00:22:56.080 --> 00:22:58.230
okay.
00:22:58.240 --> 00:23:02.549
Um, look, I I am hopeful. We have some
00:23:02.559 --> 00:23:06.630
discussions coming up that I hope might
00:23:06.640 --> 00:23:09.190
emerge from which might emerge some
00:23:09.200 --> 00:23:10.549
perhaps what you might call more
00:23:10.559 --> 00:23:14.070
affordable options uh which might still
00:23:14.080 --> 00:23:16.310
involve ESO. The problem is ESO has its
00:23:16.320 --> 00:23:17.510
own rules
00:23:17.520 --> 00:23:21.510
>> and ESO is I think it's 17 uh member
00:23:21.520 --> 00:23:24.789
countries and if you do a special deal
00:23:24.799 --> 00:23:26.470
for Australia they're all going to say
00:23:26.480 --> 00:23:27.990
well why don't we get a special deal
00:23:28.000 --> 00:23:30.789
like that as well. Um and that's
00:23:30.799 --> 00:23:33.029
understandable. So ISO has to tread very
00:23:33.039 --> 00:23:34.950
carefully in this kind of thing.
00:23:34.960 --> 00:23:36.870
>> Yeah, that makes sense. All right. Well,
00:23:36.880 --> 00:23:38.710
hopefully common sense will prevail
00:23:38.720 --> 00:23:42.390
sometime in the next uh two years and
00:23:42.400 --> 00:23:44.870
somebody changes their mind and sees the
00:23:44.880 --> 00:23:47.669
the benefits rather than just looking at
00:23:47.679 --> 00:23:48.630
the dollar signs.
00:23:48.640 --> 00:23:50.630
>> Looking at the dollars. That's right.
00:23:50.640 --> 00:23:53.270
>> Okay. This is Space Nuts. Andrew Dunley
00:23:53.280 --> 00:23:57.590
with Professor Fred Watson.
00:23:57.600 --> 00:23:59.430
>> Hey, that's one of the better sims.
00:23:59.440 --> 00:24:00.470
Believe me,
00:24:00.480 --> 00:24:02.070
>> we've had a couple of cardiac arrests
00:24:02.080 --> 00:24:03.270
down here too, peeps.
00:24:03.280 --> 00:24:05.430
>> There weren't any time for that up here.
00:24:05.440 --> 00:24:08.070
Space nuts.
00:24:08.080 --> 00:24:11.110
>> All right. Uh, our final story takes us
00:24:11.120 --> 00:24:13.990
um quite a way away from the planet, a
00:24:14.000 --> 00:24:15.990
little bit further than Artemus 2 has
00:24:16.000 --> 00:24:17.669
traveled, in fact. Uh, the discovery of
00:24:17.679 --> 00:24:22.149
an X-ray binary, Fred. Now, I'm not sure
00:24:22.159 --> 00:24:26.390
what this is. Um, but yes, I I know
00:24:26.400 --> 00:24:29.350
there's all sorts of um, you know, radio
00:24:29.360 --> 00:24:31.669
wave type signals flying around the
00:24:31.679 --> 00:24:35.830
universe. X-rays, gamma rays, um, AC/DC,
00:24:35.840 --> 00:24:39.029
you name it. Um, but it's all out there.
00:24:39.039 --> 00:24:42.390
Uh, what is an X-ray binary?
00:24:42.400 --> 00:24:44.870
>> Um, that's a great question because this
00:24:44.880 --> 00:24:47.750
is this is a story about an X-ray binary
00:24:47.760 --> 00:24:50.549
that isn't a binary.
00:24:50.559 --> 00:24:52.470
>> So, just to complicate things further.
00:24:52.480 --> 00:24:54.870
So what's an X-ray binary? Uh if you've
00:24:54.880 --> 00:24:58.710
got a star which has got a star a bit
00:24:58.720 --> 00:25:00.470
like the sun actually these are normal
00:25:00.480 --> 00:25:03.029
stars like the sun uh gets to the end of
00:25:03.039 --> 00:25:07.269
its life uh and after usually something
00:25:07.279 --> 00:25:09.990
in the region of 10 billion years. Um
00:25:10.000 --> 00:25:12.630
what it what happens is it it puffs off
00:25:12.640 --> 00:25:14.470
its outer layers because the nuclear
00:25:14.480 --> 00:25:16.789
reactions change in its interior and
00:25:16.799 --> 00:25:19.350
eventually its core collapses to become
00:25:19.360 --> 00:25:21.029
something we call a white dwarf star.
00:25:21.039 --> 00:25:22.390
We've talked about them before. They're
00:25:22.400 --> 00:25:24.310
about the size of the Earth with about
00:25:24.320 --> 00:25:27.350
the mass of a star. Uh and they've
00:25:27.360 --> 00:25:29.830
basically exhausted their fuel. They're
00:25:29.840 --> 00:25:31.990
still shining because they're very hot.
00:25:32.000 --> 00:25:36.470
Uh so, um that's an a white dwarf star.
00:25:36.480 --> 00:25:40.710
Now, often that will happen in what's
00:25:40.720 --> 00:25:42.630
called a binary system. Two stars
00:25:42.640 --> 00:25:44.710
orbiting around their common center of
00:25:44.720 --> 00:25:49.350
gravity. And a binary is actually almost
00:25:49.360 --> 00:25:52.149
the most common form of stars in the
00:25:52.159 --> 00:25:55.190
galaxy. Many many stars that we observe,
00:25:55.200 --> 00:25:57.990
almost 50% are actually part of a binary
00:25:58.000 --> 00:26:00.470
pair. They're part of a duo. So, if
00:26:00.480 --> 00:26:02.789
you've got a star that's collapsed into
00:26:02.799 --> 00:26:05.669
a white dwarf star, um, which has
00:26:05.679 --> 00:26:07.669
intense gravity, not quite as intense as
00:26:07.679 --> 00:26:09.750
a black hole, but pretty intense, and
00:26:09.760 --> 00:26:11.909
it's being orbited by another star that
00:26:11.919 --> 00:26:13.590
hasn't got to that stage in its
00:26:13.600 --> 00:26:15.750
evolution, then what you get is the
00:26:15.760 --> 00:26:18.630
white dwarf is sucking matter off the
00:26:18.640 --> 00:26:21.510
other star and spiraling it inwards. The
00:26:21.520 --> 00:26:23.510
white dwarf's eating it up. Uh, and
00:26:23.520 --> 00:26:25.350
eventually if the white dwarf has enough
00:26:25.360 --> 00:26:27.029
of that stuff, it becomes unstable and
00:26:27.039 --> 00:26:28.950
turns into what we call a type 1A
00:26:28.960 --> 00:26:33.110
supernova, an exploding star. Um but
00:26:33.120 --> 00:26:35.669
during that process while your your
00:26:35.679 --> 00:26:38.149
white dwarf and your normal star are in
00:26:38.159 --> 00:26:40.630
this dance around each other with stuff
00:26:40.640 --> 00:26:42.789
being pulled off the normal star that
00:26:42.799 --> 00:26:44.710
stuff will be accelerated by the gravity
00:26:44.720 --> 00:26:47.110
of the white dwarf and it will emit
00:26:47.120 --> 00:26:50.470
x-rays because it is being so uh so
00:26:50.480 --> 00:26:54.870
highly excited uh by the energy that's
00:26:54.880 --> 00:26:56.549
basically being imparted to it as it
00:26:56.559 --> 00:26:57.750
gets pulled in. It's a bit like the
00:26:57.760 --> 00:26:59.990
accretion disc of a black hole. It's a
00:27:00.000 --> 00:27:02.390
kind of calm down version of that.
00:27:02.400 --> 00:27:05.510
>> Um, so that all makes sense.
00:27:05.520 --> 00:27:07.830
>> I'm glad it does. That's that's where
00:27:07.840 --> 00:27:09.909
the X-ray bit comes from. So an X-ray
00:27:09.919 --> 00:27:12.789
binary is two stars. One's a normal star
00:27:12.799 --> 00:27:14.950
having its surface sucked away by a
00:27:14.960 --> 00:27:17.350
white dwarf and that sucking away of
00:27:17.360 --> 00:27:19.510
material causes the X-rays. So that's
00:27:19.520 --> 00:27:21.510
how you discover it. So what has
00:27:21.520 --> 00:27:23.430
happened? But this isn't what's
00:27:23.440 --> 00:27:24.950
happening now, is it? With this
00:27:24.960 --> 00:27:27.990
discovery. No, no, but that's the that's
00:27:28.000 --> 00:27:30.310
the backstory if I can put it that way.
00:27:30.320 --> 00:27:34.630
>> Um what has happened now is um there are
00:27:34.640 --> 00:27:37.510
two of them actually two stars that have
00:27:37.520 --> 00:27:40.310
been uh discovered
00:27:40.320 --> 00:27:43.990
>> which show all the signs of being an
00:27:44.000 --> 00:27:46.950
X-ray binary in terms of the X-rays that
00:27:46.960 --> 00:27:49.909
they emit. But there's no other star
00:27:49.919 --> 00:27:52.390
there. There's there's no, you know,
00:27:52.400 --> 00:27:53.990
there's there's there's only the white
00:27:54.000 --> 00:27:56.310
dwarf. there's there's nothing else.
00:27:56.320 --> 00:27:56.630
>> Okay.
00:27:56.640 --> 00:27:59.590
>> Um and that means it's an X-ray binary
00:27:59.600 --> 00:28:02.470
that isn't a binary. Uh and two of these
00:28:02.480 --> 00:28:06.389
things have been discovered um by a
00:28:06.399 --> 00:28:08.230
group of scientists who actually look
00:28:08.240 --> 00:28:10.630
for these things. Uh they've got
00:28:10.640 --> 00:28:12.310
interesting names, perhaps a bit more
00:28:12.320 --> 00:28:14.310
imaginative than the usual astronomical
00:28:14.320 --> 00:28:17.830
names. One is called Gandalf. Uh and the
00:28:17.840 --> 00:28:20.549
and the other is called Moonsized. uh
00:28:20.559 --> 00:28:22.149
they were discovered at different times
00:28:22.159 --> 00:28:25.029
but they're basically um you know they
00:28:25.039 --> 00:28:28.389
are um part of the same survey. So
00:28:28.399 --> 00:28:31.830
they've got this signature of X-rays but
00:28:31.840 --> 00:28:37.029
um no companion object that is basically
00:28:37.039 --> 00:28:39.669
telling you that it's a normal B X-ray
00:28:39.679 --> 00:28:40.470
binary.
00:28:40.480 --> 00:28:42.070
>> So
00:28:42.080 --> 00:28:43.830
does that mean there's something else
00:28:43.840 --> 00:28:46.310
there that it's feeding off or
00:28:46.320 --> 00:28:50.070
>> That's correct. It looks as though that
00:28:50.080 --> 00:28:55.909
what what they have is a a half ring of
00:28:55.919 --> 00:28:59.590
material actually circulating around the
00:28:59.600 --> 00:29:01.269
white dwarf.
00:29:01.279 --> 00:29:06.310
>> So, and that this is the debris from
00:29:06.320 --> 00:29:08.389
basically a star being swallowed up,
00:29:08.399 --> 00:29:10.470
another star being swallowed up by the
00:29:10.480 --> 00:29:13.669
by the white dwarf. Uh it's very very
00:29:13.679 --> 00:29:15.909
odd and very unusual and quite hard to
00:29:15.919 --> 00:29:18.389
get your head around. This uh this this
00:29:18.399 --> 00:29:22.149
moving ring um which uh as the white
00:29:22.159 --> 00:29:24.310
dwarf itself spins and generates a
00:29:24.320 --> 00:29:26.549
magnetic field is not actually aligned
00:29:26.559 --> 00:29:28.630
with where we think the magnetic field
00:29:28.640 --> 00:29:34.870
is. Um so it's it's um it's a puzzle.
00:29:34.880 --> 00:29:37.350
I'm going to quote one of the authors of
00:29:37.360 --> 00:29:41.350
one of these papers who says to to note
00:29:41.360 --> 00:29:43.990
white dwarfs of similar age and
00:29:44.000 --> 00:29:46.470
evolutionary stage are typically
00:29:46.480 --> 00:29:48.789
non-magnetic
00:29:48.799 --> 00:29:50.950
while highly magnetic white dwarf
00:29:50.960 --> 00:29:53.430
remnants are already an exception.
00:29:53.440 --> 00:29:57.430
Gandalf is now only one one of only two
00:29:57.440 --> 00:29:59.990
known merger remnants to feature
00:30:00.000 --> 00:30:02.310
asymmetric magnetization.
00:30:02.320 --> 00:30:04.230
That's all gobbledygook for saying this
00:30:04.240 --> 00:30:06.870
is a very very peculiar pair of objects
00:30:06.880 --> 00:30:08.870
that we uh that we see and they're in
00:30:08.880 --> 00:30:10.149
different parts of the universe. They're
00:30:10.159 --> 00:30:11.909
not related to each other. They are
00:30:11.919 --> 00:30:15.110
different parts. So this is a really
00:30:15.120 --> 00:30:18.549
interesting um episode because it looks
00:30:18.559 --> 00:30:20.310
as though a completely new class of
00:30:20.320 --> 00:30:22.070
stars has been discovered here.
00:30:22.080 --> 00:30:24.070
Something that really is not the norm.
00:30:24.080 --> 00:30:25.510
Stuff that we know about and are
00:30:25.520 --> 00:30:27.909
familiar and and love. It's just not
00:30:27.919 --> 00:30:31.110
part of that. It's something quite new.
00:30:31.120 --> 00:30:34.230
as you're explaining it, my thought just
00:30:34.240 --> 00:30:37.110
went to could this just be the end of
00:30:37.120 --> 00:30:40.310
the partnership? Like it's the the stars
00:30:40.320 --> 00:30:42.070
pretty well just, you know, there's
00:30:42.080 --> 00:30:43.830
hardly anything left. You're still
00:30:43.840 --> 00:30:46.230
getting that X-ray deal going on,
00:30:46.240 --> 00:30:49.110
>> but you know, um there's there's
00:30:49.120 --> 00:30:51.669
>> hardly any material left and see you
00:30:51.679 --> 00:30:53.190
later alligator
00:30:53.200 --> 00:30:55.029
>> and and what's what's there is spread
00:30:55.039 --> 00:30:57.269
into half a ring, which seems to be the
00:30:57.279 --> 00:30:59.110
case. Yeah, I think that's I think that
00:30:59.120 --> 00:31:01.750
is probably the the bottom line of this.
00:31:01.760 --> 00:31:03.430
Um, which is is boring.
00:31:03.440 --> 00:31:04.630
>> You figured something out. Perhaps
00:31:04.640 --> 00:31:05.990
>> you figured something out. Yep. Yep.
00:31:06.000 --> 00:31:08.230
>> Where's my Nobel Prize?
00:31:08.240 --> 00:31:09.750
>> Actually, it's I think I've got it here
00:31:09.760 --> 00:31:12.789
in this drawer. So, I put it away last
00:31:12.799 --> 00:31:15.510
week.
00:31:15.520 --> 00:31:18.630
Uh, yes, it's um, look, it's great uh
00:31:18.640 --> 00:31:20.630
that that we've got entirely new
00:31:20.640 --> 00:31:22.310
category of highly magnetized white
00:31:22.320 --> 00:31:24.630
dwarf, which is something that's not
00:31:24.640 --> 00:31:26.789
been seen before.
00:31:26.799 --> 00:31:28.870
Yes, indeed. Very exciting. Uh if you'd
00:31:28.880 --> 00:31:30.789
like to read about that, you can see it
00:31:30.799 --> 00:31:33.750
on uh one of the best websites around
00:31:33.760 --> 00:31:35.990
when it comes to uh science and
00:31:36.000 --> 00:31:39.750
astronomy. And that's f.org, not fi.
00:31:39.760 --> 00:31:41.830
It's phys.org.
00:31:41.840 --> 00:31:43.590
fizz.org.
00:31:43.600 --> 00:31:45.830
Great story. Uh we had a bit of a
00:31:45.840 --> 00:31:47.269
sandwich there. Good news, bad news,
00:31:47.279 --> 00:31:48.630
good news, I think.
00:31:48.640 --> 00:31:52.070
>> Yes. Yeah, that's right. We We do our
00:31:52.080 --> 00:31:53.590
best. We aim to please, don't we? I
00:31:53.600 --> 00:31:55.029
mean, we're we're only adequate, but we
00:31:55.039 --> 00:31:57.029
do aim to please at some level.
00:31:57.039 --> 00:31:59.350
>> We do. Yes. Although, you know, depends
00:31:59.360 --> 00:32:00.630
which part of it you were listening to
00:32:00.640 --> 00:32:02.789
as to what is pleasing and what wasn't.
00:32:02.799 --> 00:32:05.029
I think it was self-evident.
00:32:05.039 --> 00:32:06.950
>> Yes, indeed.
00:32:06.960 --> 00:32:08.710
>> We are all done, Fred. Thank you very
00:32:08.720 --> 00:32:09.750
much.
00:32:09.760 --> 00:32:11.590
>> Great pleasure, Andrew. Always good to
00:32:11.600 --> 00:32:14.230
air my grievances as well as talk about
00:32:14.240 --> 00:32:17.110
the latest in science news. We'll see
00:32:17.120 --> 00:32:18.070
you next time.
00:32:18.080 --> 00:32:19.430
>> Yes, we will catch you on the next
00:32:19.440 --> 00:32:21.830
episode, a Q&A episode coming your way
00:32:21.840 --> 00:32:23.830
very, very soon. And uh while you're
00:32:23.840 --> 00:32:26.470
online uh have a listen or have a look
00:32:26.480 --> 00:32:28.310
around on our website because uh we
00:32:28.320 --> 00:32:30.149
would uh we'd love you to do that. You
00:32:30.159 --> 00:32:32.789
can u sign up to the astronomy daily
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00:32:38.720 --> 00:32:40.710
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00:32:40.720 --> 00:32:42.710
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00:32:42.720 --> 00:32:47.110
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00:32:47.120 --> 00:32:50.070
um favorite podcasting platform. Um,
00:32:50.080 --> 00:32:52.630
they help us a lot and we really would
00:32:52.640 --> 00:32:56.470
appreciate it. Um, I I think we mostly
00:32:56.480 --> 00:32:57.990
get reasonably good ones, you know, two
00:32:58.000 --> 00:33:00.789
and a half, three stars. Woohoo. No,
00:33:00.799 --> 00:33:02.870
we've had a few bigger than that. Uh,
00:33:02.880 --> 00:33:05.029
and thanks to Hugh in the studio. Uh,
00:33:05.039 --> 00:33:06.549
we've just come out of a long weekend
00:33:06.559 --> 00:33:08.710
here in Australia and Hugh's been away
00:33:08.720 --> 00:33:10.630
and um he was running late because he
00:33:10.640 --> 00:33:13.590
was at a convention of white dwarfs. And
00:33:13.600 --> 00:33:15.830
from me, Andrew Dunley, thanks for your
00:33:15.840 --> 00:33:17.190
company. We'll see you on the next
00:33:17.200 --> 00:33:19.590
episode of Space Nuts. Bye-bye.
00:33:19.600 --> 00:33:20.549
>> Space nuts.
00:33:20.559 --> 00:33:22.630
>> You've been listening to the Space Nuts
00:33:22.640 --> 00:33:24.950
podcast
00:33:24.960 --> 00:33:27.909
>> available at Apple Podcasts, Spotify,
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