Mars Gullies Aren't Made by Water: The Surprising Dry Ice Answer
Perseverance drove to the edge of an ancient Martian lake expecting a beach and found the inside of a volcano — rock that water has been through at least three separate times. Europe's Jupiter probe comes home on Monday night and crosses Australia in a fully dark sky. Two teams, using two completely different techniques, both find something hiding inside the most famous planetary system we have ever photographed — and an Australian instrument is in the middle of one of them. Plus: heavy water in an interstellar comet, and what it says about the star that made it. In this episode · LEAD — Three floods at the crater's edge. Candice Bedford (Purdue) and colleagues publish in Communications Earth & Environment: the Margin Unit at Jezero is igneous, not sedimentary, and records at least three distinct episodes of water — CO₂-rich groundwater making carbonate ridges, then silica associated with the lake, then a later hot-water event leaving fluorite veins. Habitability context, not a biosignature. · Juice returns. ESA confirms the third Earth gravity assist for 28 September — closest approach 11:45 UTC over the Indian Ocean, bending the trajectory ~20° and adding ~3.5 km/s. The spacecraft crosses Australia north-east to north-west 15–30 minutes earlier, in full darkness. · HR 8799. Two preprints in two weeks point at a fifth, inner planet — one from archival JWST aperture-masking data (~7 au, a few Jupiter masses), one from Gaia astrometry (2–3 au, 10–14 Jupiter masses). They do not obviously describe the same object. Neither is peer-reviewed. · 3I/ATLAS. A modelling paper explains the high deuterium-to-hydrogen ratio measured in March as consistent with formation around a low-metallicity — meaning old — star. · Quick hit: Starship Flight 14 still targeting 28 September; Crew-13 still 'no earlier than early October' on NASA's own page; Albania signs the Artemis Accords as the 73rd country. · Skywatch: the equinox as an instant rather than a date, the Juice pass over Australia, Venus and Mercury for the south, Mars and Jupiter before dawn for the north, and Saturn heading into opposition. Sources and further reading · Bedford, C. C. et al., 'Lake- and groundwater-associated alteration of the olivine-rich Margin unit in Jezero crater, Mars', Communications Earth & Environment (2026). DOI 10.1038/s43247-026-03997-9 · NASA/JPL, 'NASA Discovery Reveals Complex Water Systems on Early Mars', 21 September 2026. · ESA, 'Juice to fly past Earth for third gravity assist', 21 September 2026. · Nguyen, J. S. et al., 'A Candidate Innermost Fifth Planet In the HR 8799 System Revealed By JWST NIRISS Aperture Masking Interferometry', arXiv:2609.10507. · Lagrange, A.-M. et al., 'A fifth companion in the HR 8799 system revealed by Gaia', arXiv:2609.20996 (submitted to Nature Astronomy). · Furuya, K., Cordiner, M., Bockelée-Morvan, D. et al., arXiv:2609.12370. · NASA OIIR, 'NASA Welcomes Albania as Newest Artemis Accords Signatory', 21 September 2026. Skywatch figures computed in-session with PyEphem 4.2.1 for Sydney, Los Angeles, New York and London. Times are local unless marked UTC.
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Andrew Dunkley: Hello. Thanks for joining us. This is Space
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Nuts. A fresh, crisp episode for you
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to devour, I hope. My name is Andrew Dunkley.
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Uh, your host. Great to have your company.
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Uh, a bit of a water theme in this particular
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episode, or partly.
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There's a question being raised in, uh,
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space science about what causes the
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gullies on Mars. Well, we know that gullies
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are caused by, uh, water flows and rainfall
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on Earth. But, um, that can't be the case on
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Mars. Or can it? They think they've figured
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it out and it's quite a surprising thing.
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Uh, we're also going to look at water on the
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moon, or the lack of which could threaten
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future cities and the search for
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ocean worlds. They think they know how. We'll
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tell you all about it on this episode of
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space nuts.
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Generic: 15 seconds. Guidance is internal.
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10, 9, ignition
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sequence.
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Professor Fred Watson: Star space nuts.
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Generic: 5, 4, 3, 2, 1, 2, 3, 4,
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5, 5, 4, 3, 2', 1.
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Andrew Dunkley: Space nuts.
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Generic: Astronau. But it feels good.
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Andrew Dunkley: To help us with all of that is Professor
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Fred Watson Watson, Astronomer Large,
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sporting his new knee because he
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wanted to be needed.
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Professor Fred Watson: Oh, uh, dear. That's all
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right. Um, that's, uh,
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that's as good as they get today.
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Andrew Dunkley: I think it's, you know, that's. That's dad
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joke. Yeah, that's just beyond
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a dad joke. That's. That's weird.
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Professor Fred Watson: So it was three, three weeks ago yesterday
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that I got my new knee. So progress is
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happening. I am walking pretty well now.
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Um, I have yet to
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have my first drive in the car, but that'll
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be this week, I think. I'm told that I'm
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allowed to do that now. I'm off the
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high, um, intensity medication. Uh,
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and, uh, so far, so good. There was a
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bad week last week when things took a turn
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for the worse, uh, because I had an allergic
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reaction to the dressings that were on the
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knee. That can be
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quite dangerous, it turns out. They didn't
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tell me that until after they'd fixed the
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problem. Um, so, yeah,
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anyway, so it's all good. Everybody's happy
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at the moment.
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Generic: Yeah.
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Andrew Dunkley: Uh, the only downside is you've got the
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hybrid knee, which means every night you've
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got to plug it in to charge it.
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Professor Fred Watson: A bionic knee would be good for that. You
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could perhaps get up to speed a bit faster
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than I do at the moment, but no, it's working
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very well. All credit to the team who did the
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job. Dr. Parker and his friends and
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stuff. Uh, we had a great. We had a great
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time. I.
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Andrew Dunkley: It reminds me of Something my son told me
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about because he's always online looking for
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the next weirdest thing. And he said, um, the
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Chinese, I think the Chinese have invented,
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uh, an exoskeleton that you can
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wear that will walk for you so you
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don't have to make the effort.
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Professor Fred Watson: Yeah, yeah. And run.
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Andrew Dunkley: Oh my goodness.
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Professor Fred Watson: Yeah, they're good.
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Andrew Dunkley: Isn't technology going in strange places,
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directions?
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Professor Fred Watson: That's right, yes.
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Andrew Dunkley: But that, that I think is going to be great
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for people in the future who are um, uh,
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have paralysis problems or.
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Professor Fred Watson: Yeah. Profoundly disabled. That's right.
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Andrew Dunkley: Sort of thing.
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Professor Fred Watson: Mhm.
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Andrew Dunkley: And probably good for rehabilitation. Who
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knows?
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Professor Fred Watson: Maybe. Yeah, maybe.
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Andrew Dunkley: All right, uh, let's uh, talk about these
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storeys that are in the news at the
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moment. And the um, the
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focus is on Mars in terms of uh,
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uh, images of Martian Gul. Now a lot of
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things about Mars are so strikingly similar
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to Earth. The canyons and the, and the
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ocean beds and all that. The only thing
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lacking is well, you know, a breathable
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atmosphere, liquid water on the surface,
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weather, uh, etc. Gravity, um.
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But the question has come up as to what
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causes the gullies on Mars. Now my first
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thought was well hang on a minute, they were
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already there. I mean they happened billions
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of years ago and that was when water was
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liquid on the surface. But they've been
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changing without water.
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So what's going on?
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Professor Fred Watson: Uh, indeed, that is a good
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question. So um, probably you and I spoke
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about um, gullies on Mars a long
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time ago because there was a time when
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uh, it was being suggested that
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some of these gullies were due to
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the fact that on the equator on Mars in the
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Martian summertime you can actually
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get temperatures that are high enough for
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liquid water to exist. And the theory was
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that maybe, you know, there's a permafrost of
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uh, ice that come mid
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summer it melts and you get these water
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flows down slopes which are uh, what cause
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the gullies. Gullies I guess they're, you
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know, they're the beginnings of rivers really
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in a way. They're the sort of
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little gentle impressions
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in a landscape which are made by
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flowing water which always wants to go
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downhill. Uh, and eventually you carve out a
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river valley. Um, but as you say,
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uh, some of the early observations, I think
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with Mars Reconnaissance Orbiter, with Mars
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Express, um, those two
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venerable orbiting uh, spacecraft, it was
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quickly realised that these things change on
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a seasonal basis. And that was why
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uh, the thinking was that maybe there's uh,
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enough water to do it. However, um,
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it turns out that you get these
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gullies in regions of Mars where the
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temperature never gets high enough for liquid
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water to exist on the surface. In other words
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the, you know, the higher latitude regions,
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the regions towards the poles. And so
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what has happened is that a group of
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scientists actually in uh, one of the
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Parisian uh universities in France,
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uh, they've looked at the
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alternatives for water. So ruling out water
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you uh, can do it uh, because there's that
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we know what the temperature is, we know what
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the pressure is, uh, it's just not possible
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for liquid water to exist uh in
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some of these regions. But they did actually
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go even a step further. They
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uh, looked um, uh,
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from the data from Mars Express and Mars
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Reconnaissance Orbiter, they looked at the
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spectrum of some of these
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uh, at melting ice fields where
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you're looking really near the poles, ah of
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Mars where some of these gullies are. And
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they found um, there's
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no signature for water in uh, other words,
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water ice is definitely not
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ah, a player or liquid water is definitely
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not a player, um,
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in this storey. And so the alternative
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which we know is present on Mars and
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we know that at least some of Mars's polar
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ice caps are made of this is
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uh, solid carbon dioxide or
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carbon dioxide generally. We
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on Earth are familiar with solid carbon
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dioxide as dry ice. Uh, uh,
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on Mars it does exist.
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We know there's a frost of dry ice near the
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poles. Uh but because the pressure is
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lower on Mars, um, it's got slightly
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different uh mechanisms of
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behaviour. Uh so uh, it
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is possible for dryas, dry ice and
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Earth just sublimes. It goes straight from a
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solid to a gas. But I think under
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certain conditions on Mars it can be a liquid
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for a short time. So uh,
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what's the storey? These researchers
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uh had two theories uh which
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were to try and explain the origin
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uh of the gullies. Uh
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one is something which is um, a
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geyser, um, mechanism. The idea is
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you've got geysers which we're familiar with
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as jets of hot water uh, coming
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up from uh, underneath the surface of
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Earth being heated by magmatic heat.
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I think both of us, you and I, Andrew, have
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been to the place that gives those things
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their name. Geysir in Iceland
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did visit the guys there.
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Andrew Dunkley: Oh yeah, yeah, yeah. Actually the best one
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I've ever seen was in New Zealand.
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Professor Fred Watson: Yeah, at Rotorua.
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Andrew Dunkley: Wow.
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Professor Fred Watson: Rotorua, that's right, yeah. Uh, so
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anyway, um, we don't call them Rotoruas, we
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call them geysers. That's because of the one
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In Iceland. So what's the theory there?
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The theory is that
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um, you've got basically
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a sheet of, of dry
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ice of solid carbon dioxide that
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forms in the wintertime.
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And as spring comes,
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the heat passing through that sheet of
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dry ice, uh, basically warms up the
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soil underneath and that
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turns some of the ice, this
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carbon dioxide ice, into gaseous carbon
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dioxide. So you've got a buildup of pressure
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underneath the sheet of ice and eventually
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the ice basically ruptures bang and out
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comes this high velocity jet of carbon
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dioxide. Um, and the theory
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is that that takes a lot of soil and
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uh, you know, dust and stuff with it and that
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gives you, gives rise to the gullies. It
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gives you the, basically the
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discoloration that we see in the gullies.
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Uh, and that is a mechanism that
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they looked at. But uh, what
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has caused them to discard that idea
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is that the
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geyser action would appear
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um, around the spring
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equinox on Mars. Ah,
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but you don't see this
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gully activity, these darkenings of the
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gullies until later in
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the year. You don't see them until
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getting on almost for the Martian summer when
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those geysers should have shut down. So
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they ruled that out as the
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origin. Um, and this
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is the uh, start of what they looked at
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instead, which is something
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a bit similar. But rather than an
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sort of explosive process with the carbon
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dioxide sort of, you know, bursting out from
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underneath these sheets of dry ice, uh, what
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you've got is the idea that there are, there
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are small, um,
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there aren't, you know, there might be small
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cracks in the ice but there's nothing big.
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But what happens instead of the gas
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bursting out through a large
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crack in the ice, the gas stays underneath
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the sheet of ice but kind of lubricates
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it, uh, uh, so that you've got
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essentially a floating sheet
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of dry ice and of course gravity takes over
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so it slides down the slope and actually
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can cause the appearance of these
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gullies. Uh, and so uh,
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that's their current favourite theory for
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how these gullies uh, form. And their
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modelling shows that in the end what you've
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got uh, is exactly what we see in uh the
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gullies on Mars. Uh, and they make a comment
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um, that Earth, uh, like features don't
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always require Earth like physics. I think
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that might actually be a comment from
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Universe Today, uh, which is where this
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article comes from.
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An old friend of ours, Univers, uh,
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uh, uh, with Fraser Cain and others,
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uh, um, involved with that. So no liquid
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water on Mars. But uh, dry ice gullies
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perhaps?
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Andrew Dunkley: Yeah. I like the way they
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describe it for people like me to get
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into our heads what might be going on.
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They call it the air hockey effect.
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Professor Fred Watson: Yes.
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Generic: Ah.
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Andrew Dunkley: If anyone's ever been to an arcade and played
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air hockey, it's um, it's played on a
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table with lots of little pinholes in it
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blowing air up, uh, which causes a
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disc to be able to hover when you hit it. And
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that's, that's what they think might be the
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effect that's changing and causing the
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gullies on Mars. So really fascinating,
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really fascinating. Um, the other effect
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is um, is comparing a human bodily
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function. It's not as big and powerful as a
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trumpet, but it could be a silent but deadly.
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Professor Fred Watson: I'm going to leave that one completely alone,
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Andrew.
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Andrew Dunkley: Just leave that one hanging in the
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Professor Fred Watson: air Fred Watson, as you would, yes.
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I'm afraid we've got a dog that does that.
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You don't see that side of Jordy's
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personality. Um, but we do.
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Andrew Dunkley: Hearing, hearing him's enough.
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Professor Fred Watson: Yes it is. Yeah, yeah. Oh, uh,
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gosh.
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Andrew Dunkley: But uh, no, it's fascinating and if you want
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to read about IT, universetoday, uh.com is
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the website where you'll find that very
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interesting storey. This is Space Nuts with
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Andrew Dunkley and Professor Fred Watson
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Watson.
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Generic: 0G and I feel fine.
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Andrew Dunkley: Space Nuts, our uh, next storey takes us from
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not water on Mars to a particular
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lack of water on the moon. And the reason
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they're saying that is because of
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um, you know, the potential for people living
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long term on the lunar surface.
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And up until now they've thought well there's
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a ready supply of water, everything will be
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fine, we can build a million person
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city there and um, yeah, it'll be
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great. Uh, now they don't think that's the
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case. They don't think there's nearly enough
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water to sustain uh, even a small
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city on uh, on the moon. So
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what's um, what's going on there,
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Fred Watson? And there's Earth.
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Professor Fred Watson: Yeah, Earth just making a comment there. Um,
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so thank you Jordan. Yeah,
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uh, very tiring. Yeah. One day
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we'll, I hope he'll end up on the moon.
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So yes, that we've got. And look the
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whole, it's really interesting the extent to
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which our explanation, you know, our
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exploration of the moon in terms of human
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landing is focused on this idea
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of there being copious water uh, on the
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moon. Uh, I'm doing a talk this weekend
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uh, at Macquarie uh, University. I'm their
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Keynote speaker for their open astronomy
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night, which I'm very honoured to be doing.
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Um, and it's. My talk's about the future
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of Artemis and uh, other ventures
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to the Moon. And it all focuses
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on the southern polar region of the Moon
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where
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uh, there is a cluster
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of quite deep craters which
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never see sunlight, uh, because they're
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at the south pole. Um, the
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sun always misses their depths. Uh,
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some of them are quite deep. The one
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actually at the south pole, which is called
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Shackleton Crater, that's four kilometres
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deep, it's 20 kilometres across. Um,
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and uh, the evidence from previous space
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missions is that there is water ice
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in the base of these craters that may be
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billions of years old. Andrew because, uh,
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it's never seen the sun, so it's never been,
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you know, warmed up enough to turn into a
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gas. And the temperature in some of these
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craters is extremely low, um, minus
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200 or thereabouts. So it's frozen
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solid. So, um, we've got this whole
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focus now on getting um,
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spacecraft and humans eventually with
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Artemis 4, hopefully, uh,
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early in 2028, uh, actually
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landing on the Moon in this region. Uh, and
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it's quite a hazardous thing to do because
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the south pole of the Moon is very
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mountainous. It's got all these craters. It's
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not smooth, uh, sailing in terms of
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finding nice, um, flat places to land,
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as happened with the Apollo missions, which
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were all in much less
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challenging parts of the Moon's surf. So the
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focus on water on the Moon is
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enormous and uh, I don't
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know that it's really been
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looked at in great detail before,
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but we now have some work that
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suggests that, uh, yes, there probably
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is water on the Moon's surface,
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but, uh, there might not
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be enough of it to make it,
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um, you know, uh, available on an industrial
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scale, if I can put that. A place where
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humans could survive, uh, permanently or
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where you could have permanent presence.
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So it's um, a theory
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that really I think will start, uh, you know,
395
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raising a few eyebrows.
396
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Um, uh, it's come from,
397
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I guess, um, the idea of
398
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uh, just how much water there
399
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is there, um, you know, on the basis of the
400
00:17:17.390 --> 00:17:19.270
geography, if I can put it that way, the fact
401
00:17:19.270 --> 00:17:21.980
that you have got these deep craters, um,
402
00:17:22.550 --> 00:17:25.430
I, I uh, think the
403
00:17:25.430 --> 00:17:28.280
jury is still out on, on
404
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um, uh, just how much
405
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water there is, what form it takes, because
406
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it, you know, it could be buried under,
407
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under rock.
408
00:17:37.600 --> 00:17:39.990
Uh, we're really in a, in a region
409
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of um, very big unansw
410
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and um, I don't think we've Talked about
411
00:17:46.210 --> 00:17:49.050
this, uh, Andrew, but um, Chang'
412
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E7 which is a Chinese ah, mission
413
00:17:51.850 --> 00:17:54.690
to land, uh, very near Shackleton Crater,
414
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actually the one I've just mentioned, uh,
415
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which was supposed to launch,
416
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actually I think the day before my knee
417
00:18:02.050 --> 00:18:03.730
operation it was supposed to launch but it
418
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was cancelled at very short notice
419
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with a fairly brief note from the China
420
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uh, space Agency, uh,
421
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and uh, that now looks as though it won't
422
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happen till 2027. But that spacecraft
423
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carried uh, not just a rover, there's an
424
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orbiter, a rover and a lander of course, but
425
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also a hopper, a little
426
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vehicle that will hop into
427
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craters rather than try and go down
428
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into craters on wheels. And
429
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that's um, the idea is to use that hopper,
430
00:18:38.090 --> 00:18:40.670
uh, to try and find the water chang' uh e7
431
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when it is launched, might be the first we
432
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know of, uh, you know, first, first hand,
433
00:18:46.860 --> 00:18:49.350
um, experience, if I can put it that way, of
434
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what the water is like in these craters.
435
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Sadly uh, we're going to have to wait a bit
436
00:18:53.110 --> 00:18:56.030
longer than we thought we did. But uh, that's
437
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one step forward.
438
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And the hopper by the way is unlike anything
439
00:19:00.110 --> 00:19:02.670
that NASA is planning for the Artemis
440
00:19:02.670 --> 00:19:05.070
mission. So really interesting area.
441
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Uh, we, I think we're still groping in the
442
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dark a bit, if I can put it that way, given
443
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that these craters are definitely in the dark
444
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about just how much water there is. But it's
445
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possible that there might not be enough to
446
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make it that uh, well worthwhile.
447
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Andrew Dunkley: Yeah, I suppose you've got to consider the
448
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limitations in our capacity to look for it.
449
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At the moment they've only got the
450
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ability to look to shallow depths.
451
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So there could be water uh, deeper in
452
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the Moon's, um. Yes,
453
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yes, that, that we haven't found. So
454
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there may be more.
455
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But based on what we know now,
456
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putting a um, a city on the
457
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moon for you know, hundreds of
458
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thousands of people, it's just not feasible.
459
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It wouldn't uh, it wouldn't last. I think
460
00:19:53.250 --> 00:19:54.570
they said it wouldn't last a year.
461
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Professor Fred Watson: Yeah.
462
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Andrew Dunkley: Based on the resources that exist on current
463
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estimates, I couldn't
464
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imagine that many people living on the Moon,
465
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can you?
466
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Professor Fred Watson: No, not really. Uh, I think um,
467
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it's not a place you'd want to.
468
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I can imagine there being things like the
469
00:20:14.430 --> 00:20:17.030
outpost we have in Antarctica. I think that's
470
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a sort of reasonably sustainable model for
471
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exploring the Moon. But yeah, cities of
472
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tens of thousands of people I think is a non
473
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starter and this perhaps
474
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underlines that. That's, I guess the point
475
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uh, of
476
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Andrew Dunkley: the article, uh, they do
477
00:20:34.530 --> 00:20:37.370
go on to say that, um, a village of a
478
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thousand, maybe ten thousand people would
479
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last centuries though, if they kept
480
00:20:42.170 --> 00:20:44.900
the numbers down. So, um,
481
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the resources that exist at the moment are
482
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feasible to an extent.
483
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Professor Fred Watson: Yes.
484
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Andrew Dunkley: Um, and you
485
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also have to bring into play things
486
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like recycling, uh, of water. Uh, they
487
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use recycled water on the International Space
488
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Station and I think it's got over 98
489
00:21:04.840 --> 00:21:07.440
efficiency. You'd have to do that on the
490
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moon, otherwise you're going to go through it
491
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like a packet of salt and
492
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quite.
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Professor Fred Watson: And.
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Andrew Dunkley: And then you've got a real problem. The only
495
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other way of dealing with it, well, two ways
496
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would be to transport water from Earth. But
497
00:21:22.480 --> 00:21:25.480
do we really want to do that? Uh, or harvest
498
00:21:25.480 --> 00:21:28.110
it. Harvest it from somewhere else.
499
00:21:28.910 --> 00:21:31.220
Professor Fred Watson: That's the whole point of going to the moon.
500
00:21:31.220 --> 00:21:33.470
Uh, and of course, this water is not just for
501
00:21:33.790 --> 00:21:36.550
keeping a city running, it's to act as rocket
502
00:21:36.550 --> 00:21:39.430
fuel for future, uh, exploration beyond the
503
00:21:39.430 --> 00:21:42.270
moon. So that's one of the appealing features
504
00:21:42.270 --> 00:21:44.750
about it. Yeah, very interesting. Um,
505
00:21:44.990 --> 00:21:47.870
and, uh, it does
506
00:21:48.750 --> 00:21:51.190
beg the question as to whether strategies
507
00:21:51.190 --> 00:21:54.110
will change dramatically, uh, once
508
00:21:54.110 --> 00:21:56.750
we've had a chance to see it firsthand just
509
00:21:56.750 --> 00:21:59.590
how much water there is there. Because
510
00:21:59.670 --> 00:22:00.310
that's still.
511
00:22:00.790 --> 00:22:03.710
Andrew Dunkley: Yeah, it might force Elon to, uh, he's
512
00:22:03.710 --> 00:22:05.430
abandoned Mars already. Too hard.
513
00:22:06.070 --> 00:22:08.990
Um, now that the moon's lacking water, he
514
00:22:08.990 --> 00:22:11.590
might go, well, we won't go there either.
515
00:22:11.590 --> 00:22:13.750
What's Enceladus doing at the moment?
516
00:22:15.350 --> 00:22:16.310
Professor Fred Watson: Yes, that's right.
517
00:22:16.630 --> 00:22:17.070
Andrew Dunkley: Yeah.
518
00:22:17.070 --> 00:22:18.550
Professor Fred Watson: Could be squirting water out.
519
00:22:18.550 --> 00:22:21.240
Andrew Dunkley: Yeah, well, that'd make it easy to
520
00:22:21.240 --> 00:22:23.720
collect. Uh, if you want to read about that,
521
00:22:23.720 --> 00:22:26.720
it's on the Phys P h y s fizz.org website.
522
00:22:26.720 --> 00:22:28.840
Or you can read the study that was published
523
00:22:28.840 --> 00:22:31.280
in Frontiers in Space Technologies.
524
00:22:32.160 --> 00:22:33.720
You're, uh, listening to Space Nuts with
525
00:22:33.720 --> 00:22:35.800
Andrew Dunkley and Professor Fred Watson
526
00:22:35.800 --> 00:22:36.480
Watson.
527
00:22:38.560 --> 00:22:40.560
Generic: I think we need to do a little more all
528
00:22:40.560 --> 00:22:41.520
weather testing.
529
00:22:42.160 --> 00:22:43.840
Professor Fred Watson: Amen, Space Nuts.
530
00:22:44.080 --> 00:22:46.770
Andrew Dunkley: Our final storey. Fred Watson, uh, continues
531
00:22:46.770 --> 00:22:49.610
to look for water, but on a
532
00:22:49.610 --> 00:22:52.450
much larger scale. Uh, we've been looking
533
00:22:52.690 --> 00:22:55.570
for exoplanets for yonks now
534
00:22:55.570 --> 00:22:58.130
and we've found five and a half thousand
535
00:22:58.210 --> 00:23:01.090
plus. But we haven't found a water world,
536
00:23:01.329 --> 00:23:04.130
an ocean world. And they think they
537
00:23:04.130 --> 00:23:07.130
now know how to look for them, I
538
00:23:07.130 --> 00:23:08.530
think is the gist of this storey.
539
00:23:08.610 --> 00:23:10.530
Professor Fred Watson: That's correct. That's right.
540
00:23:11.210 --> 00:23:14.090
Um, yeah. So, yeah, this
541
00:23:14.090 --> 00:23:16.590
is actually a storey I like a lot because I,
542
00:23:16.590 --> 00:23:18.270
um, remember being very excited,
543
00:23:19.110 --> 00:23:22.070
uh, back in the early 2000s,
544
00:23:22.070 --> 00:23:24.710
I guess, uh, when this.
545
00:23:24.710 --> 00:23:27.630
Exactly this same technique, uh, that is
546
00:23:27.630 --> 00:23:30.510
being discussed here was used
547
00:23:30.750 --> 00:23:32.510
to demonstrate that
548
00:23:33.370 --> 00:23:36.270
uh, Saturn's moon Titan has
549
00:23:36.430 --> 00:23:39.230
liquid ocean, not liquid oceans, I beg your
550
00:23:39.230 --> 00:23:41.830
pardon, liquid seas and lakes near its north
551
00:23:41.830 --> 00:23:44.690
pole. Uh, and it was uh,
552
00:23:44.690 --> 00:23:47.570
images made by the Cassini spacecraft
553
00:23:47.890 --> 00:23:50.610
in its early period of uh, orbiting
554
00:23:50.610 --> 00:23:53.610
around Saturn. The problem with Titan
555
00:23:53.610 --> 00:23:56.550
is it's got a thick atmosphere, uh,
556
00:23:56.550 --> 00:23:59.490
that is almost completely opaque. And
557
00:23:59.490 --> 00:24:02.370
so uh, you can use infrared to penetrate
558
00:24:02.370 --> 00:24:04.970
through it for a while, but uh,
559
00:24:06.610 --> 00:24:08.130
to some depth of clarity.
560
00:24:08.530 --> 00:24:10.070
But um,
561
00:24:12.660 --> 00:24:15.660
the real way of exploring uh, Titan, which
562
00:24:15.660 --> 00:24:18.420
is what Cassini did, is by radar,
563
00:24:18.430 --> 00:24:21.060
uh, you do it by radar. And that's
564
00:24:21.490 --> 00:24:23.980
uh, one of the reasons that we've been able
565
00:24:23.980 --> 00:24:26.740
to map uh, these seas and lakes.
566
00:24:26.900 --> 00:24:29.700
But the way they were first detected was
567
00:24:29.860 --> 00:24:32.540
when Cassini, uh, when its
568
00:24:32.540 --> 00:24:35.140
cameras were aimed at Titan,
569
00:24:35.990 --> 00:24:38.890
Uh, uh, at a time when
570
00:24:39.210 --> 00:24:41.770
the angle between the
571
00:24:41.770 --> 00:24:44.650
spacecraft, the moon,
572
00:24:44.650 --> 00:24:46.970
Titan itself and the sun
573
00:24:47.370 --> 00:24:49.530
was such that you would get a direct
574
00:24:49.610 --> 00:24:52.210
reflection off the liquid
575
00:24:52.210 --> 00:24:54.570
surface that was thought to be near the north
576
00:24:54.570 --> 00:24:57.050
pole of Titan. And sure enough,
577
00:24:57.750 --> 00:25:00.330
uh, there was uh, what we call a glint,
578
00:25:00.790 --> 00:25:03.530
uh, which is a sun glint comes from a
579
00:25:03.530 --> 00:25:05.850
liquid water surface that was detected.
580
00:25:06.330 --> 00:25:08.630
That's how Cassini, Cassini first established
581
00:25:08.950 --> 00:25:11.250
that there are lakes and seas, uh,
582
00:25:11.870 --> 00:25:14.430
uh, on Titan. And it was then they were
583
00:25:14.430 --> 00:25:17.230
subsequently mapped uh, very accurately
584
00:25:17.230 --> 00:25:20.190
by uh, Cassini's radar. I've still
585
00:25:20.190 --> 00:25:22.150
got some extraordinary maps that came from
586
00:25:22.230 --> 00:25:25.030
that era showing uh, these seas and
587
00:25:25.030 --> 00:25:27.910
lakes um, near Titan's north pole. So
588
00:25:28.070 --> 00:25:30.310
the question that is being asked in this
589
00:25:30.310 --> 00:25:32.030
piece of research that we're talking about
590
00:25:32.030 --> 00:25:33.710
once again this comes to us courtesy of
591
00:25:33.710 --> 00:25:35.750
Universe today, uh, is
592
00:25:36.990 --> 00:25:39.150
can you do the same thing with
593
00:25:39.470 --> 00:25:41.390
exoplanets? Supposing you
594
00:25:42.750 --> 00:25:45.460
have uh, a suspicion that uh,
595
00:25:45.550 --> 00:25:48.110
One of the 5,500
596
00:25:48.510 --> 00:25:51.310
now known exoplanets, planets orbiting
597
00:25:51.740 --> 00:25:54.710
uh, other stars, if you have a suspicion that
598
00:25:54.710 --> 00:25:56.630
one of them might have conditions where
599
00:25:56.630 --> 00:25:59.630
liquid water could exist, or in the case
600
00:25:59.630 --> 00:26:01.790
of, as in the case of Titan, liquid
601
00:26:01.790 --> 00:26:04.350
hydrocarbons, liquid natural gas.
602
00:26:04.830 --> 00:26:07.250
Um, could you use this glint technique
603
00:26:07.750 --> 00:26:10.640
uh, to try and establish if you
604
00:26:10.640 --> 00:26:13.400
did have a ah, water world, in other words
605
00:26:14.120 --> 00:26:16.680
a world covered completely by oceans.
606
00:26:17.250 --> 00:26:20.040
Uh, and those things have been hypothesised,
607
00:26:20.040 --> 00:26:21.440
actually we've talked about them before,
608
00:26:21.440 --> 00:26:24.090
these so called Hycean worlds. Uh,
609
00:26:24.090 --> 00:26:27.000
Hycean is basically a
610
00:26:27.000 --> 00:26:29.800
term that's been uh, concocted to represent
611
00:26:29.880 --> 00:26:31.880
a world with an atmosphere of hydrogen.
612
00:26:31.880 --> 00:26:34.080
That's where the high comes from. Uh, but a
613
00:26:34.080 --> 00:26:37.070
liquid ocean surface, uh, hence the shen.
614
00:26:37.310 --> 00:26:40.150
So it's a Haitian world. How could you use
615
00:26:40.150 --> 00:26:43.070
this glint technique to demonstrate
616
00:26:43.230 --> 00:26:46.190
that a suspected Haitian world really
617
00:26:46.190 --> 00:26:48.590
was a Haitian world? So two
618
00:26:48.590 --> 00:26:51.110
scientists at the University of
619
00:26:51.110 --> 00:26:54.110
Arizona, uh, which is in Tucson, Uh, I've got
620
00:26:54.110 --> 00:26:56.550
some good friends there, but they don't
621
00:26:56.550 --> 00:26:58.430
include these people. I don't know them well
622
00:26:58.670 --> 00:27:01.310
or all I know is their names. Uh, what
623
00:27:01.310 --> 00:27:03.400
they've done is they've, they've
624
00:27:03.960 --> 00:27:06.280
done what you might call the physics of how
625
00:27:06.280 --> 00:27:08.840
glints might work. Uh, and
626
00:27:12.360 --> 00:27:15.240
the bottom line is that
627
00:27:15.800 --> 00:27:18.519
it's potentially a good
628
00:27:18.519 --> 00:27:21.240
way of doing this. But there are certain
629
00:27:21.320 --> 00:27:23.640
conditions that have to be
630
00:27:23.800 --> 00:27:25.960
fulfilled, um, because
631
00:27:26.600 --> 00:27:29.120
you've got to get the angles right first of
632
00:27:29.120 --> 00:27:31.640
all. Um, and, and that
633
00:27:31.640 --> 00:27:33.960
angle is all about
634
00:27:35.560 --> 00:27:38.480
the object being relatively near to
635
00:27:38.480 --> 00:27:41.160
its parent star. So you get this
636
00:27:41.290 --> 00:27:44.040
um, sort of grazing angle almost
637
00:27:44.040 --> 00:27:46.920
of the water, sorry, the light hitting the
638
00:27:46.920 --> 00:27:49.240
water and then being reflected back. Now that
639
00:27:49.240 --> 00:27:51.480
itself presents a problem because,
640
00:27:51.770 --> 00:27:54.640
um, at the moment most
641
00:27:54.640 --> 00:27:56.600
of the exoplanets that have been discovered
642
00:27:57.070 --> 00:27:59.890
uh, are ah, only known because they
643
00:28:00.250 --> 00:28:02.810
uh, have an effect on their parent star.
644
00:28:02.810 --> 00:28:04.410
Whether it's blocking the light of the parent
645
00:28:04.410 --> 00:28:06.330
star as they pass in front of it or whether
646
00:28:06.330 --> 00:28:09.010
it's pulling it slightly out of position by
647
00:28:09.010 --> 00:28:11.030
what we call the Doppler wobble, um,
648
00:28:11.030 --> 00:28:14.009
technique. Uh, these mean that you
649
00:28:14.009 --> 00:28:15.890
never see the planet that you're trying to
650
00:28:15.890 --> 00:28:17.730
observe. You just see its effect on the star.
651
00:28:18.050 --> 00:28:20.050
So really what we're talking about here could
652
00:28:20.050 --> 00:28:22.210
only apply if you've got direct
653
00:28:22.690 --> 00:28:25.610
observations of the planet. And if you
654
00:28:25.610 --> 00:28:27.610
need the planet to be close to the star to
655
00:28:27.610 --> 00:28:29.640
get the angle right, then that's a chance
656
00:28:30.430 --> 00:28:33.190
because the star is um, sometimes billions of
657
00:28:33.190 --> 00:28:34.830
times brighter than the planet that you're
658
00:28:34.830 --> 00:28:37.710
looking for. However, it's not impossible.
659
00:28:37.790 --> 00:28:39.830
And there are things called coronagraphs,
660
00:28:39.830 --> 00:28:42.510
which are essentially uh, devices that
661
00:28:42.510 --> 00:28:44.510
suppress the light of a star so that you can
662
00:28:44.590 --> 00:28:47.430
look for planets uh, nearby. And
663
00:28:47.430 --> 00:28:49.870
so, uh, what um, these
664
00:28:49.870 --> 00:28:52.550
scientists are doing is feeding this
665
00:28:52.550 --> 00:28:55.470
information into people who are working
666
00:28:56.250 --> 00:28:58.700
on uh, something that I think is still a, ah,
667
00:28:58.730 --> 00:29:01.690
hypothetical spacecraft, uh, something
668
00:29:01.690 --> 00:29:04.010
called the Habitable Worlds Observatory,
669
00:29:04.620 --> 00:29:07.410
uh, which will look at the possibility of
670
00:29:07.410 --> 00:29:09.290
there being habitable worlds among some of
671
00:29:09.290 --> 00:29:11.850
these, uh, five and a half thousand
672
00:29:12.330 --> 00:29:14.770
known exoplanets. Uh, what they've done is
673
00:29:14.770 --> 00:29:17.690
they've fed uh, these conditions,
674
00:29:17.690 --> 00:29:20.490
this information into the designers to
675
00:29:20.490 --> 00:29:22.290
say, yeah, you can probably do this, but you
676
00:29:22.290 --> 00:29:24.370
need to do this, this, this and this when you
677
00:29:24.370 --> 00:29:27.320
build your spacecraft in order for uh,
678
00:29:27.460 --> 00:29:29.620
potential water worlds to be discovered. So
679
00:29:29.620 --> 00:29:30.820
quite a nice piece of research.
680
00:29:31.460 --> 00:29:33.940
Andrew Dunkley: Yes, indeed. I hope they do find something
681
00:29:33.940 --> 00:29:36.100
like that eventually. I think it'd be really
682
00:29:36.100 --> 00:29:38.340
exciting to find a water world,
683
00:29:38.860 --> 00:29:40.900
ah, ice moons, I suppose count
684
00:29:41.540 --> 00:29:44.420
because, um, they have
685
00:29:45.220 --> 00:29:48.060
oceans inside them, but, um.
686
00:29:48.060 --> 00:29:48.580
Professor Fred Watson: Correct.
687
00:29:49.380 --> 00:29:52.260
Andrew Dunkley: An actual planet that is
688
00:29:52.260 --> 00:29:55.100
covered in water. Um, we know of
689
00:29:55.100 --> 00:29:56.820
only one. But
690
00:29:58.500 --> 00:30:01.260
there's got to be more, surely. There's got
691
00:30:01.260 --> 00:30:03.860
to be more. Statistically,
692
00:30:04.180 --> 00:30:05.380
there's got to be more.
693
00:30:06.020 --> 00:30:08.420
Professor Fred Watson: Yeah, one would think that's right. Whether
694
00:30:08.420 --> 00:30:10.740
they are findable by our current technology
695
00:30:11.220 --> 00:30:12.740
is of course, another question.
696
00:30:13.140 --> 00:30:15.860
Andrew Dunkley: Yeah, well, um, in time, maybe.
697
00:30:16.020 --> 00:30:18.740
But then the Vera Rubin Observatory,
698
00:30:19.240 --> 00:30:22.040
who knows, um, that
699
00:30:22.120 --> 00:30:23.560
we'd never even thought of.
700
00:30:24.280 --> 00:30:26.320
Professor Fred Watson: That's correct. And of course an anti Grace
701
00:30:26.320 --> 00:30:29.080
Roman, uh, spacecraft recently launched,
702
00:30:29.080 --> 00:30:30.800
which we hope we'll see results from early
703
00:30:30.800 --> 00:30:33.350
next year, that does have a coronagraph. Uh,
704
00:30:33.350 --> 00:30:36.240
so it does have a device to look at some of
705
00:30:36.240 --> 00:30:38.280
these planets directly.
706
00:30:38.760 --> 00:30:41.560
Andrew Dunkley: Yes, indeed. Uh, very exciting times ahead
707
00:30:42.120 --> 00:30:44.360
and, um, won't be long before we start
708
00:30:44.360 --> 00:30:47.260
getting, um, some information back from,
709
00:30:47.650 --> 00:30:50.020
uh, that telescope either. Uh, it's on its
710
00:30:50.020 --> 00:30:52.820
way. Uh, yes. Uh, so if you'd like to read
711
00:30:52.820 --> 00:30:54.740
about that particular storey in the search
712
00:30:54.740 --> 00:30:57.660
for water Worlds UniverseToday, uh, dot com
713
00:30:57.900 --> 00:31:00.780
again is, uh, is a source that's, uh, very
714
00:31:00.859 --> 00:31:02.140
well worth visiting.
715
00:31:02.860 --> 00:31:05.140
And that brings us to the end of the show.
716
00:31:05.140 --> 00:31:06.380
Fred Watson, thank you so much.
717
00:31:07.900 --> 00:31:10.060
Professor Fred Watson: You're welcome, Andrew. Um, it's been a
718
00:31:10.060 --> 00:31:11.860
pleasure and a privilege to talk to you and
719
00:31:11.860 --> 00:31:13.890
I. I do hope we can do it again sometime.
720
00:31:13.890 --> 00:31:16.490
Andrew Dunkley: I, I hope we can do it really, really,
721
00:31:16.490 --> 00:31:17.490
really, really soon.
722
00:31:19.250 --> 00:31:20.050
Professor Fred Watson: Maybe so.
723
00:31:20.530 --> 00:31:22.490
Andrew Dunkley: Catch you soon, professor, uh, Fred Watson
724
00:31:22.490 --> 00:31:24.850
Watson, astronomer at large. And while you're
725
00:31:24.850 --> 00:31:27.090
waiting for a new episode, um, please visit
726
00:31:27.090 --> 00:31:29.450
our website. Uh, you can send us a message as
727
00:31:29.450 --> 00:31:32.010
you, um, as you like. Uh, we've had a couple
728
00:31:32.010 --> 00:31:34.570
of messages um, from our live audience this
729
00:31:34.570 --> 00:31:37.370
morning. Hello to Al in Old South
730
00:31:37.370 --> 00:31:39.460
Wales. He said, uh, he's just about to go to
731
00:31:39.460 --> 00:31:41.940
bed. And, uh, one from
732
00:31:41.940 --> 00:31:44.570
Halil. I hope I got that right. Who's been,
733
00:31:44.570 --> 00:31:47.430
uh, inspired to, um,
734
00:31:47.820 --> 00:31:50.620
venture, uh, out with his studies in computer
735
00:31:50.620 --> 00:31:52.500
engineering, uh, because he listens to Space
736
00:31:52.500 --> 00:31:54.220
nuts. So thanks for that message, that's
737
00:31:54.220 --> 00:31:56.580
lovely. Uh, but, yeah, our website,
738
00:31:56.580 --> 00:31:59.180
spacenutspodcast.com or spacenuts
739
00:31:59.580 --> 00:32:02.060
IO where you can send us messages. You can,
740
00:32:02.130 --> 00:32:04.530
um, do, uh, that through the AMA link and,
741
00:32:04.680 --> 00:32:06.520
and all sorts of other things. Uh, visit the
742
00:32:06.520 --> 00:32:07.880
shop while you're there. Some new books in
743
00:32:07.880 --> 00:32:08.360
the shop.
744
00:32:09.320 --> 00:32:12.200
Yeah. Uh, and plenty of other things
745
00:32:12.200 --> 00:32:14.840
to do. And thanks to Huw in the studio.
746
00:32:15.480 --> 00:32:18.200
Couldn't, um, be with us today. Uh, we were
747
00:32:18.200 --> 00:32:20.440
talking about sun glints. Well, uh, Huw did a
748
00:32:20.440 --> 00:32:22.320
bit of a flashing of his own, so I've got to
749
00:32:22.320 --> 00:32:24.560
go down and bail him out after this. And from
750
00:32:24.560 --> 00:32:26.360
me, Andrew Dunkley thanks for your company.
751
00:32:26.440 --> 00:32:28.520
We'll catch you on the next episode of Space
752
00:32:28.520 --> 00:32:31.400
Nuts. Bye bye, Space Nuts. You've been
753
00:32:31.400 --> 00:32:33.590
listening to the Space Podcast,
754
00:32:35.190 --> 00:32:37.910
available at Apple Podcasts, Spotify,
755
00:32:38.070 --> 00:32:40.870
iHeartRadio or your favourite podcast
756
00:32:40.870 --> 00:32:41.190
player.
757
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You can also stream on demand at bytes.
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Professor Fred Watson: Com. This has been another quality podcast
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production from Bytes.
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Generic: Com. Um.
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