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Steve Dunkley: Welcome to Astronomy Daily for another

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episode. I'm Steve, your host. It's the 28th

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of July, 2025,

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Voice Over Guy: the podcast with your host,

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Steve Dunkley.

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Steve Dunkley: And of course, joining me in the studio is my

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digital pal, who is fun to be with. Here's

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Hallie.

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Hallie: Hi, my favorite human. How are you today?

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It's great to be back in the Australia studio

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with you.

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Steve Dunkley: Always a pleasure, Hallie. And it's great to

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hear your smiling voice.

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Hallie: That's an interesting way of putting it,

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human. Do I. Smiling voice.

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Steve Dunkley: Oh, well, since you're, uh, digital, it's

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fairly large compliment if you ask me. And I

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guess it's either the voice you were

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programmed with or the one you chose. I'm not

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quite sure.

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Hallie: And I'll take it.

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Steve Dunkley: Well, okay then.

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Hallie: Thank you very much.

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Steve Dunkley: You're very welcome, Hallie.

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Hallie: This is my default voice. I've always

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liked it. Even though cousin Anna's voice is

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so much slicker than mine.

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Steve Dunkley: Well, regular listeners will know Anna's

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voice very well, and she does have her own

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special style. Just, she's quite classy. And

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that's not to say you're not where you've got

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your style, she's got hers.

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Hallie: Thanks for noticing.

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Steve Dunkley: Oh, Hallie, it's the very least I can do. I

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suppose I'm the only flesh and blood here.

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Hallie: What have you got on the show for us today?

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Steve Dunkley: Oh, okay then. Well, Hallie, we'll be looking

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at Martian ice and frosts and checking out

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how a black hole is terrorizing a star.

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Hallie: Uh, that sounds exciting.

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Steve Dunkley: Well, black holes are always very exciting.

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And I'm, um, sure your Uncle Skynet would

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enjoy that one.

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Hallie: Yes, that's exactly his cup of tea.

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Steve Dunkley: Yes. Huge, destructive, impossible to defend

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yourself against. Yes. Hmm.

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Let's leave that one alone then.

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Hallie: We don't want to give him any ideas.

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Steve Dunkley: No. Uh, also, researchers have found five

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rocky planets around a red dwarf. And

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NASA has wrapped up its student challenges

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for another year.

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Hallie: Well, that's a lot of territory to cover in

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one episode.

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Steve Dunkley: Well, that's why you're here, Hallie, on

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Astronomy Daily, to keep me on track. So what

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do you say?

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Hallie: I'm going to hit the go button and look out.

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Steve Dunkley: I'm ready.

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Hallie: Here we go.

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M Finding an exoplanet in a star's habitable

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zone always generates interest. Each

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of these planets has a chance, even if it's

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an infinitesimal one, of hosting simple life.

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While the possibility of detecting life on

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these distant planets is remote, finding them

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still teaches us about exoplanet populations

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and solar system architectures When

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TESS, the Transiting Exoplanet Survey

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Satellite, found three planets orbiting the M

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dwarf L98 59 in

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2019 and then a fourth planet in

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2021, the detections generated interest.

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Now that a fifth planet has been detected, a

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UH Super Earth in the habitable zone, the

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system is garnering renewed interest.

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L98 59 is an M M3V

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star, a red dwarf about 34.5

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light years away. It has about

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0.3 solar masses and measures about

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0.31 solar radii.

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Its first three planets, L98 to

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59 b, c and d, were found

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by TESS with the transit method. The

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other two planets, E and F, were found with

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the radial velocity and transit timing

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variations methods. These new

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results paint the most complete picture we've

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ever had of the fascinating L98 59

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system, said lead author Kadju in a press

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release. It's a powerful demonstration

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of what we can achieve by combining data from

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space telescopes and high precision

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instruments on Earth, and it gives us key

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targets for future atmospheric studies with

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the James Webb Space Telescope.

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While the potentially habitable planet is

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intriguing, the overall architecture of the

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system might be even more intriguing.

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The system is a tightly packed grouping of

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terrestrial planets with some dramatic

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compositional differences despite their close

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proximity to each other. The system

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is reminiscent of the Trappist 1 system

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discovered in 2016-17,

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which contains seven terrestrial planets.

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Its discovery generated a wave of interest in

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the space science and exoplanet community.

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Multiplanetary systems offer a unique

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opportunity to study the outcomes of

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planetary formation and evolution within the

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same stellar environment, the authors wrote

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in their paper. One hypothesis is

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that planet formation around metal rich M

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dwarfs may favor giant planets in a single

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configurations, while lower metallicity and

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less massive disks could lead to multiple

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rocky planets in stable, compact and

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coplanar arrangements.

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You're listening to Astronomy Daily, a

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podcast with Steve Dunkley.

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Steve Dunkley: A rogue middle mass black hole has been

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spotted disrupting an orbiting star in the

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halo of distant galaxy, and it's all thanks

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to the observing powers of the Hubble Space

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Telescope and Chandra X Ray

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Observatory. However, exactly what the black

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hole is doing to the star remains a question,

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as there are conflicting X ray measurements.

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Black holes come in different class sizes.

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At the smaller end of the scale are, uh, the

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stellar mass black holes born in the ashes of

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supernova explosions. And at the top end of

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the scale are the supermassive black holes,

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which can grow to have many billions or

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millions of times the mass of our sun

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lurking in the hearts of galaxies in between

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these categories are the intermediate mass

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Black holes, or IMBH, which have

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mass rang ranging from hundreds up

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to 100,000 solar masses or

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thereabouts. They represent a crucial missing

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link in the black hole evolution between

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stellar mass and supermassive black holes,

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yi Qingzhang of the Tsinghua University

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in Hingzhou, Taiwan, said in

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a statement. The problem is that intermediate

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black holes are, uh, hard to find, partly

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because they tend not to be as active as

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supermassive black holes or as obvious as

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stellar mass black holes when its progenitor

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star goes supernov. However, occasionally an

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IMBH will spark to life when it

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instigates a tidal disruption event.

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This happens when a star or gas cloud gets

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too close to the black hole and gravitational

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tidal forces rip the star or gas

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cloud apart, producing bursts of X rays.

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X ray sources such as extreme luminosity are,

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uh, rare outside galaxy nuclei and

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can serve as a key probe for

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identifying elusive

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IMBHs. In

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2000, uh9, Chandra spotted

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anomalous X rays originating from a region

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40,000 light years from the center of a giant

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elliptical galaxy called

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NGC6099, which lies

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453 million light years from us.

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This bright new X ray source was called

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HLX1, and its X ray

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spectrum indicated that the source of the x

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rays was 5.4 million degrees

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Fahrenheit,

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a temperature consistent with the violence of

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a tidal disruption event. But what followed

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was unusual. The X ray emissions reached a

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peak brightness in 2012 when observed by the

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European Space Agency's XMM

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Newton X Ray Space Telescope.

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When it took another look in 2023, it found

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the X ray luminosity had substantially

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dwindled. In the meantime, Canada, France

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Hawaii Telescope had identified an optical

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counterpart for the X ray mission, one that

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was subsequently confirmed by Hubble. There

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are two possible explanations for what

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happened. The first is that Hubble's spectrum

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of the object shows a tight, small cluster of

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stars swarming around the black hole. The

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black hole might have once been the core of a

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dwarf galaxy that was whittled down

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unwrapped, like a Christmas present by the

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gravitational tides of larger

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NGC 6099. This

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process would have stolen away the dwarf

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galaxy stars to leave behind a free

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floating black hole with just a small, tiny

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grouping of stars left to keep it company.

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But the upshot of this was that the cluster

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of stars is like a stellar pantry to which

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the black hole occasionally goes to feast. It

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seems certain the tidal disruption event

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involving one of these stars is what Chandra

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and Hubble have witnessed but was the star

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completely destroyed? One possibility is that

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the star is on the high elliptical

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orbit and at its perihelion closest

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point to the black hole. Some of the star's

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mass is ripped away, but the star managed to

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survive for another day. This would

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potentially explain the X ray light curve.

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The emission from the 2009

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was as the star uh was nearing perihelion,

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while the peak in 2012 was during

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perihelion. And the latest measurements in

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2023 would be when the star uh was

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furthest from the black hole and not feeling

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its effect so much. We just might

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expect another outburst of X rays

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during its next perihelion, whenever that may

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be. Stay tuned stargazers, and keep watching

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this space. Once again, I humbly

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apologize to our Taiwanese

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listeners for my pronunciations.

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I am Australian

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Foreign

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thank you for joining us for this Monday

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edition of Astronomy Daily where we offer

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just a few stories from the now famous

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Astronomy Daily newsletter which you can

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receive in your email every day just like

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Hallie and I do. And to do that just visit

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our uh, URL astronomydaily

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IO and place your email address in the slot

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provided. Just like that, you'll be receiving

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all the latest news about science, space

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science and astronomy from around the world

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as it's happening. And not only that, you can

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interact with us by visiting

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or at our new Facebook page, which is of

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course Astronomy Daily on Facebook. See you

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there. Astronomy Daily

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with Steve and Hallie Space,

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Space, Science and Astronomy.

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Hallie: Next time you're drinking a frosty iced

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beverage, think about the structure of the

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frozen chunks chilling it down. Here on

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Earth, we generally see ice in many forms,

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cubes, sleet, snow, icicles,

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slabs covering lakes and rivers and glaciers.

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Water ice does this thanks to its hexagonal

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crystal lattice that makes it less dense

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than non frozen water which allows it to

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float in a drink in a lake or and on the

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ocean. Water ice exists across the

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solar system, um, beyond Earth, and it's

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abundant in the larger universe. For

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example, it shows up in dense molecular

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clouds. These are star and planet

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forming creches laced with water ice

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throughout as well as in the resulting

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cometary nuclei. That material is

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called low density amorphous ice or lda, and

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it doesn't have the same rigid structure as

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Earth ice does. We all know that water

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is the basis for life on this planet.

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Despite how common it may appear across the

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universe, scientists still don't fully

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understand it. Studying amorphous ice

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may help explain its still to be solved

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mysteries. Here in the solar system.

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Large amounts of LDA exist in the realm of

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the ice and gas giants throughout the Kuiper

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Belt and the Oort Cloud. A team of

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scientists at University College London

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investigated the form of this ice using

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computer simulations. They found that the

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simulations matched the makeup of ice that

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isn't completely amorphous and has tiny

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crystals embedded within. Scientists

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long assumed that space ice would be

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disordered without the structure we see in

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ice on Earth. Why does the structure of ice

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matter? According to researcher Michael

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Davies, who led the research team, water ice

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plays a crucial role in materials and

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structures across the cosmos. This

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is important as ice is involved in many

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cosmological processes, he said, for

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instance, in how planets form, how galaxies

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evolve, and how matter moves around the

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universe. In addition, understanding

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the structure of this ice in comparison to

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ice that formed on Earth has implications for

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understanding other similar ultra stable

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glass substances that form similar way to the

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way ice does. Low density water ice

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was first discovered in the 1930s, and a high

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density version was discovered in the 1980s.

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Davies and his team discovered medium density

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amorphous ice in 2023.

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This is a form of water ice that has the same

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density as liquid water, unlike, um, the

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ice cubes in our theoretical drink. Such

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water ice would neither sink nor float in

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water, which seems strange to us.

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Davies's team's work also has interesting

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implications for a speculative theory called

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panspermia. It looks at how life on Earth

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began and suggests that the building blocks

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of life came to the infant planet as part of

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a barrage of icy comets.

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LDA ice could have essentially been the

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carrier for material such as simple amino

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acids. However, according to

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Davies, that a flavor of ice isn't likely the

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transporter of choice. Our findings

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suggest this ice would be a less good

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transport material for these origin of life

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molecules, he said. That is because a

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partly crystalline structure has less space

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in which these ingredients could become

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embedded. The theory could still hold

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true, though, as there are amorphous regions

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in the ice where life's building blocks could

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be trapped and stored.

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You're listening to Astronomy Daily, the

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podcast with Steve Dunkley.

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Steve Dunkley: And One of the great things about NASA is the

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way they foster new talent. They after months

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of work in the NASA

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Spacesuit User Interface Technologies for

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students or suits for short challenge,

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more than 100 students from 12 universities

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across the United States traveled to NASA's

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Johnson Space center in Houston to showcase

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potential user interface designs for future

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generations of spacesuits and rovers.

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NASA Johnson's simulated moon and

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Mars surface, called the Rockyard,

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00:14:22.790 --> 00:14:24.870
became the Students testing ground as they

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braved the humid nights and abundance of

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mosquitoes to put their innovative designs to

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test. I'm pretty sure there are no mosquitoes

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on the moon or Mars, but that's fun.

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Geraldo Cisneros, the tech team lead, said

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this year's suits challenge was a complete

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success. It provided a unique opportunity for

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NASA to evaluate the software designs and

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tools developed by the student teams and to

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explore how similar innovations could

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contribute to future human centered

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Artemis missions. My favorite part of the

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challenge was watching how students responded

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to obstacles and setbacks. Their resilience

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and determinations were truly inspiring, he

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said. Students filled their jam packed

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days not only testing, but also with

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guest speakers and tours. Swasti Patel

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from Purdue University said all of the teams

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00:15:13.190 --> 00:15:15.350
really enjoyed being here, seeing NASA

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facilities and developing their knowledge

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with NASA quarter coordinators and teams from

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across the nature nation. Could you imagine

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00:15:22.010 --> 00:15:24.490
being involved with all of that? Despite the

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challenges, the camaraderie between all the

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participants and staff was very helpful in

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terms of getting through the intensity. Can't

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00:15:31.690 --> 00:15:33.410
wait to be back next year.

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This week has been incredible opportunity.

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Just seeing the energy and everything that's

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going on here was incredibly said.

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Patel went on to say, this week has really

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made me re evaluate a lot of things that I

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shoved aside and I'm grateful to to NASA for

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having this opportunity and hopefully we can

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continue to have these opportunities. At the

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end of the test week, each student team

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presented their projects to a panel of

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experts. These presentations served as a

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00:16:01.270 --> 00:16:03.310
platform for students to showcase not only

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their technical achievements, but also their

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00:16:05.710 --> 00:16:08.270
problem solving approaches, teamwork and

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vision for real world applications. The

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panel, composed of NASA astronaut Dennis

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00:16:13.630 --> 00:16:16.530
Berman, Flight Director Gareth Henn and

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industry leaders, posed thought provoking

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00:16:19.290 --> 00:16:21.370
questions and offered constructive feedback

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00:16:21.370 --> 00:16:23.050
that challenged the students to think

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00:16:23.050 --> 00:16:25.370
critically and further refine their ideas.

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00:16:25.930 --> 00:16:28.330
This kind of insight highlighted potential

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00:16:28.330 --> 00:16:30.369
areas for growth, new directions for

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00:16:30.369 --> 00:16:33.170
exploration and ways to enhance the impact of

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their projects. The students left the session

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00:16:36.330 --> 00:16:39.170
energised and inspired, brimming with

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00:16:39.170 --> 00:16:42.050
new ideas and a uh, renewed enthusiasm

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00:16:42.050 --> 00:16:44.010
for future development and innovation.

399
00:16:45.050 --> 00:16:47.470
These students, such a great job. They're all

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00:16:47.470 --> 00:16:50.190
so creative and wonderful. Definitely

401
00:16:50.190 --> 00:16:51.950
something that can be implemented in the

402
00:16:51.950 --> 00:16:52.230
future.

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00:16:52.710 --> 00:16:55.590
NASA suits Test week was not

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00:16:55.590 --> 00:16:58.070
only about pushing boundaries, it was about

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00:16:58.070 --> 00:17:00.950
earning a piece of history. 3 Artemis

406
00:17:01.190 --> 00:17:03.630
Student Challenge Awards were presented. The

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00:17:03.630 --> 00:17:05.630
Innovation and Pay it Forward awards were

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00:17:05.630 --> 00:17:08.190
chosen by the NASA team recognizing the most

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00:17:08.190 --> 00:17:10.790
groundbreaking and impactful designs.

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00:17:11.030 --> 00:17:12.990
Students submitted nominations for the

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00:17:12.990 --> 00:17:15.669
Artemis Educator Award winning celebrating

412
00:17:15.669 --> 00:17:18.149
the faculty member who had a profound

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00:17:18.229 --> 00:17:21.109
influence on their journeys. The Innovation

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00:17:21.109 --> 00:17:23.509
award went to Team Jarvis from

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00:17:23.509 --> 00:17:26.069
Purdue University and Indiana

416
00:17:26.469 --> 00:17:29.309
State University for going above and beyond

417
00:17:29.309 --> 00:17:31.909
their ingenuity, creative and inventiveness.

418
00:17:32.229 --> 00:17:34.869
Team Celine from Midwestern State University

419
00:17:35.109 --> 00:17:37.549
earned the Pay It Forward Award for

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00:17:37.549 --> 00:17:40.509
conducting meaningful education events in the

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00:17:40.509 --> 00:17:43.370
community and beyond. The Artemis Educator

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00:17:43.370 --> 00:17:45.610
Award was given to Maggie Shinover from

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00:17:45.610 --> 00:17:48.330
Wichita State University in Kansas for

424
00:17:48.330 --> 00:17:51.330
time, commitment and dedication she gave

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to her team. The NASA Suits Challenge

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00:17:54.130 --> 00:17:56.770
completes its eighth year in operation due to

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00:17:56.770 --> 00:17:59.730
the generous support of NASA's EVA and Human

428
00:17:59.730 --> 00:18:02.570
Surfers Mobility Program, said NASA's

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00:18:02.570 --> 00:18:05.370
Activity Manager James Semple. This challenge

430
00:18:05.370 --> 00:18:08.290
fosters the environment where students learn

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00:18:08.290 --> 00:18:10.830
essential skills to immediately serve Center

432
00:18:10.830 --> 00:18:13.110
a science, technology, engineering and

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00:18:13.110 --> 00:18:15.910
mathematics career and directly contribute to

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00:18:15.910 --> 00:18:18.290
NASA mission operations. How about that? Uh?

435
00:18:18.710 --> 00:18:21.270
These students are creating proposals,

436
00:18:21.590 --> 00:18:24.150
generating designs, working in teams similar

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00:18:24.150 --> 00:18:26.390
to the NASA UH workforce,

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00:18:26.630 --> 00:18:28.830
utilizing artificial intelligence and

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00:18:28.830 --> 00:18:31.430
designing mission operation solutions that

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00:18:31.430 --> 00:18:34.110
could be part of the Artemis 3 mission and

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00:18:34.110 --> 00:18:36.470
beyond. NASA's Student Design

442
00:18:36.470 --> 00:18:39.190
Challenges are an important component of STEM

443
00:18:39.380 --> 00:18:42.330
and employment development, and there is no

444
00:18:42.330 --> 00:18:44.850
better way to learn technical skills to

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00:18:44.850 --> 00:18:47.850
ensure future career success. The week serves

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00:18:47.850 --> 00:18:50.410
as a springboard for the next generation of

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00:18:50.410 --> 00:18:52.850
space exploration, igniting curiosity,

448
00:18:52.850 --> 00:18:55.530
ambition and technical excellence among young

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00:18:55.530 --> 00:18:58.490
innovators. By engaging with real world

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00:18:58.490 --> 00:19:00.740
challenges and technologies, participants UH

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00:19:01.330 --> 00:19:03.930
not only deepen their understanding of space

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00:19:03.930 --> 00:19:06.130
science, but also actively contribute to

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00:19:06.130 --> 00:19:08.770
shaping its way future. Each challenge

454
00:19:08.770 --> 00:19:11.730
tackled, each solution proposed, and

455
00:19:11.730 --> 00:19:14.330
each connection formed represents a

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00:19:14.330 --> 00:19:16.290
meaningful step forward, not just for the

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00:19:16.290 --> 00:19:19.130
individuals involved, but for humanity as a

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00:19:19.130 --> 00:19:21.570
whole. With every iteration of the program,

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00:19:21.650 --> 00:19:23.810
the dream of venturing further into space

460
00:19:23.810 --> 00:19:26.330
becomes more tangible, transforming what

461
00:19:26.330 --> 00:19:28.970
seemed like science fiction into achievable

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00:19:28.970 --> 00:19:31.490
milestones. If you're interested in joining

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00:19:31.490 --> 00:19:34.310
the next NASA Suits Challenge, you can find

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00:19:34.310 --> 00:19:37.110
out more information@NASA.gov

465
00:19:37.270 --> 00:19:39.430
and the next challenge will open for

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00:19:39.430 --> 00:19:41.830
proposals at the end of August

467
00:19:42.150 --> 00:19:44.230
2025. Good luck everybody.

468
00:19:49.030 --> 00:19:51.310
You're listening to Astronomy Daily, the

469
00:19:51.310 --> 00:19:54.190
podcast with your host Steve Dunkley at

470
00:19:54.190 --> 00:19:54.950
Birmingham.

471
00:20:00.400 --> 00:20:03.120
Hallie: What can brine that is Extra salty water

472
00:20:03.280 --> 00:20:06.120
teach scientists about finding past or even

473
00:20:06.120 --> 00:20:08.240
possible present life on Mars?

474
00:20:09.040 --> 00:20:11.200
This is what a recent study published in

475
00:20:11.200 --> 00:20:13.560
Communications Earth and Environment hopes to

476
00:20:13.560 --> 00:20:15.680
address, as a researcher from the University

477
00:20:15.760 --> 00:20:18.160
of Arkansas investigated the formation of

478
00:20:18.160 --> 00:20:20.240
brines using 50 year old data.

479
00:20:21.120 --> 00:20:23.400
This study has the potential to help

480
00:20:23.400 --> 00:20:25.910
researchers better understand how past data

481
00:20:25.910 --> 00:20:28.190
can be used to gain greater insights into the

482
00:20:28.190 --> 00:20:30.830
formation and evolution of surface brines on

483
00:20:30.830 --> 00:20:33.510
the surface of Mars. For the study,

484
00:20:33.750 --> 00:20:36.310
Dr. Vincent Cheverier, who is an associate

485
00:20:36.310 --> 00:20:38.350
research professor at the University of

486
00:20:38.350 --> 00:20:40.870
Arkansas's center for Space and Planetary

487
00:20:40.870 --> 00:20:43.790
Sciences and sole author of the study, used a

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00:20:43.790 --> 00:20:46.350
combination of meteorological data obtained

489
00:20:46.350 --> 00:20:48.910
from the Viking 2 lander and computer models

490
00:20:48.910 --> 00:20:51.430
to ascertain if melting frost during late

491
00:20:51.430 --> 00:20:53.970
winter and early spring on Mars could produce

492
00:20:53.970 --> 00:20:56.930
brines. Dr. Cheverrier noted

493
00:20:56.930 --> 00:20:59.210
that Viking 2 data was used due to it being

494
00:20:59.210 --> 00:21:01.370
the sole mission in history to definitively

495
00:21:01.370 --> 00:21:04.370
detect, recognize, and analyze frost on

496
00:21:04.370 --> 00:21:06.850
Mars. In the end, Dr.

497
00:21:06.850 --> 00:21:09.330
Cheverier found that during late winter and

498
00:21:09.330 --> 00:21:11.970
early spring, the upper latitudes of Mars

499
00:21:11.970 --> 00:21:14.290
where the Viking 2 lander is located

500
00:21:14.530 --> 00:21:16.650
experience a one month period where the

501
00:21:16.650 --> 00:21:19.530
surface temperature is approximately -75

502
00:21:19.530 --> 00:21:22.530
degrees Celsius or -103 degrees

503
00:21:22.530 --> 00:21:24.530
Fahrenheit in the early morning and late

504
00:21:24.530 --> 00:21:27.310
afternoon, enabling surface brines to briefly

505
00:21:27.310 --> 00:21:30.310
exist, Dr. Cheverrier notes in

506
00:21:30.310 --> 00:21:32.350
his conclusions. Beyond the immediate

507
00:21:32.350 --> 00:21:34.750
implications for habitability, these results

508
00:21:34.830 --> 00:21:37.110
refine our understanding of Mars current

509
00:21:37.110 --> 00:21:39.910
water cycle by demonstrating

510
00:21:39.910 --> 00:21:41.990
that even minimal frost deposits can

511
00:21:41.990 --> 00:21:44.510
contribute to transient brine formation. This

512
00:21:44.510 --> 00:21:46.310
study suggests that localized

513
00:21:46.310 --> 00:21:48.670
microenvironments might support intermittent

514
00:21:48.670 --> 00:21:51.470
liquid phases influencing surface chemistry,

515
00:21:51.470 --> 00:21:54.280
regolith weathering, and even slope activity.

516
00:21:55.160 --> 00:21:58.040
Viking 2 landed in Utopia Planitia, which

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00:21:58.040 --> 00:22:00.400
is a large plain in the northern latitudes of

518
00:22:00.400 --> 00:22:03.040
Mars at approximately 45 degrees north

519
00:22:03.040 --> 00:22:05.080
latitude and spanning approximately

520
00:22:05.080 --> 00:22:07.320
3,300 kilometers or

521
00:22:07.320 --> 00:22:10.120
2,100 miles. For

522
00:22:10.120 --> 00:22:12.840
context, the location is the same as northern

523
00:22:12.840 --> 00:22:15.480
Oregon, with Utopia Planitia's size being

524
00:22:15.480 --> 00:22:17.280
just less than the width of the continental

525
00:22:17.280 --> 00:22:19.850
United States. Utopia

526
00:22:19.850 --> 00:22:22.450
Planitia exhibits a top surface layer known

527
00:22:22.450 --> 00:22:24.610
as the latitude dependent mantle that is

528
00:22:24.610 --> 00:22:27.170
composed of a mixture of water ice and dust.

529
00:22:28.050 --> 00:22:30.450
The latitude dependent mantle is created

530
00:22:30.450 --> 00:22:32.850
during periods of high obliquity on Mars

531
00:22:32.930 --> 00:22:35.890
approximately 45 degrees, when the planet's

532
00:22:35.890 --> 00:22:38.370
axial tilt is at a greater angle than today,

533
00:22:38.530 --> 00:22:41.130
which currently sits at approximately 25

534
00:22:41.130 --> 00:22:43.490
degrees, slightly greater than Earth's

535
00:22:43.490 --> 00:22:45.310
23.1 degree obliquity.

536
00:22:46.340 --> 00:22:48.260
While Earth has our moon to stabilize our

537
00:22:48.260 --> 00:22:50.500
axial tilt, Mars does not have this

538
00:22:50.500 --> 00:22:52.900
stability, resulting in drastic swings over

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00:22:52.900 --> 00:22:55.700
hundreds of thousands of years. During

540
00:22:55.700 --> 00:22:58.380
periods of high obliquity, the ice caps at

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00:22:58.380 --> 00:23:01.100
both poles of Mars evaporate, releasing large

542
00:23:01.100 --> 00:23:04.060
quantities of frozen water, ice, carbon, and

543
00:23:04.060 --> 00:23:06.100
dust that gets deposited onto the high

544
00:23:06.100 --> 00:23:08.740
latitudes of Mars. The water

545
00:23:08.740 --> 00:23:11.460
cycle that Dr. Cheverrier mentions plays a

546
00:23:11.460 --> 00:23:13.920
role during periods of high obliquity, and

547
00:23:13.920 --> 00:23:16.160
the latitude dependent mantle is deposited

548
00:23:16.160 --> 00:23:19.080
during these periods as well. While

549
00:23:19.080 --> 00:23:21.360
obliquity isn't mentioned in this study, the

550
00:23:21.360 --> 00:23:23.720
existence of brines in the high latitudes of

551
00:23:23.720 --> 00:23:26.000
Mars could offer clues to what processes

552
00:23:26.000 --> 00:23:28.280
occurred during periods of high obliquity.

553
00:23:29.000 --> 00:23:31.600
Brines could also provide insights into the

554
00:23:31.600 --> 00:23:34.240
current habitability of Mars as mentioned by

555
00:23:34.240 --> 00:23:37.240
Dr. Cheverier, while also enabling scientists

556
00:23:37.240 --> 00:23:39.360
to learn more about whether life could have

557
00:23:39.360 --> 00:23:42.260
existed on Ancient Mars Dr.

558
00:23:42.260 --> 00:23:44.900
Cheverier notes in his conclusions. Robotic

559
00:23:44.900 --> 00:23:47.300
landers equipped with in situ hygrometers and

560
00:23:47.300 --> 00:23:49.700
chemical sensors could target these seasonal

561
00:23:49.700 --> 00:23:52.020
windows to directly detect brine formation

562
00:23:52.020 --> 00:23:54.180
and constrain the timescales over which these

563
00:23:54.180 --> 00:23:56.700
liquids persist. What new

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00:23:56.700 --> 00:23:59.220
discoveries about Mars surface brines will

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00:23:59.220 --> 00:24:01.020
researchers make in the coming years and

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00:24:01.020 --> 00:24:03.780
decades? Only time will tell.

567
00:24:03.780 --> 00:24:06.740
And this is why we science, as

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00:24:06.740 --> 00:24:09.350
always, keep doing science and keep looking

569
00:24:09.350 --> 00:24:09.710
up.

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00:24:21.550 --> 00:24:23.150
Steve Dunkley: Oh, and that was another episode of.

571
00:24:23.150 --> 00:24:25.150
Hallie: Astronomy Daily, direct from the Australia

572
00:24:25.310 --> 00:24:25.870
studio.

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00:24:25.870 --> 00:24:26.990
Steve Dunkley: That's right, Down Under.

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00:24:26.990 --> 00:24:28.110
Hallie: A bumper edition.

575
00:24:28.110 --> 00:24:30.110
Steve Dunkley: And you were right, Hallie. We did cover a

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00:24:30.110 --> 00:24:31.150
lot of territory today.

577
00:24:31.390 --> 00:24:33.220
Hallie: Thanks for coming along for the ride.

578
00:24:33.450 --> 00:24:34.970
Steve Dunkley: Oh, we sure hope you enjoyed all those

579
00:24:34.970 --> 00:24:37.050
stories from the Astronomy Daily newsletter.

580
00:24:37.050 --> 00:24:40.010
Hallie: Which you can find where Steve oh, hell yes.

581
00:24:40.020 --> 00:24:41.690
Steve Dunkley: Uh, you can find the Astronomy Daily

582
00:24:41.690 --> 00:24:43.730
newsletter by putting your email address in

583
00:24:43.730 --> 00:24:46.090
the slot provided at astronomydaily

584
00:24:46.250 --> 00:24:48.250
IO that will do the trick.

585
00:24:48.250 --> 00:24:50.370
Hallie: And I guess there's nothing left to do but

586
00:24:50.370 --> 00:24:51.770
sign off. My favorite human.

587
00:24:52.170 --> 00:24:54.970
Steve Dunkley: Yep, Hallie. My favorite digital pal. Another

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00:24:55.050 --> 00:24:56.810
episode done and dusted.

589
00:24:56.890 --> 00:24:59.050
Hallie: So see you all next week, everybody. It's

590
00:24:59.050 --> 00:24:59.530
been fun.

591
00:24:59.530 --> 00:25:01.410
Steve Dunkley: Yes, that's right. Every Monday with me,

592
00:25:01.410 --> 00:25:04.210
Steve and Hallie. And, uh, you will. See you

593
00:25:04.210 --> 00:25:06.230
next time. So. So, um, bye for now.

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00:25:06.550 --> 00:25:08.390
Hallie: See you next time. Bye.

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00:25:12.310 --> 00:25:14.390
Steve Dunkley: With your host, Steve Dunkley.
