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Anna: Welcome back to Astronomy Daily, your go to

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podcast for all the latest happenings in our

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incredible universe. I'm Anna.

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Avery: And I'm Avery. We've got a big episode lined

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up for you today, packed with some truly

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fascinating cosmic updates.

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Anna: That's right, Avery. We'll be diving into new

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research about lunar seismic activity

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and what moonquakes could mean for future

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bases on our nearest celestial neighbour.

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Turns out the Moon is a lot shakier than you

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might think.

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Avery: And speaking of drama, we'll also explore the

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explosive end of a massive star that had a

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very close encounter with a black hole. It's

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a story straight out of a sci fi movie, but

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it's real.

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Anna: Plus, we're tackling some long standing

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cosmic mysteries, from the curious case of

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the universe's missing sulphur to

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groundbreaking new insights about Vesta, one

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of the largest objects in the asteroid belt.

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Which might be more than just an.

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Avery: Asteroid, but so buckle up because

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we're about to take a tour through the latest

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and greatest in space and astronomy news.

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Anna: Alright, let's kick things off with some big

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news about our own Moon. We often think

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of it as a quiet, unchanging place, but

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new research is challenging that idea,

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especially when we consider building long

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term bases there.

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Avery: That's right, Anna. It turns out our lunar

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neighbour is more seismically active than

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many might assume. A recent study focusing

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on the Lee Lincoln Fault in the Taurus

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Littrell Valley, where the Apollo 17

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astronauts landed in 1972,

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highlights that these moonquakes could pose

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significant risks to future permanent lunar

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structures.

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Anna: This research, led by Smithsonian Senior

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Scientist Emeritus Thomas R. Waters,

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emphasises that the global distribution of

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these young thrust faults and their potential

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to still be active needs to be seriously

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considered. We're talking about planning

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locations and assessing the stability of any

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permanent outposts on the Moon.

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Avery: And, um, the evidence isn't new. It's based

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on moonquakes in the region over the past 90

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million years. Much of this evidence comes

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from material gathered by the Apollo

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astronauts themselves. Things like chunks of

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rocks and landslides are silent. But clear

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proof of the power of even magnitude

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3.0 quakes to shift surface

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materials around it really points to the Moon

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still being geologically active.

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Anna: It makes you wonder, why does the Moon even

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have quakes here on Earth? We're very

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familiar with earthquakes, primarily caused

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by plate tectonics and volcanic activity.

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Think of the San Andreas Fault or the Ring of

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Fire. Magma movement also causes tremors,

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like the recent events in Hawaii and Iceland.

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Avery: But the Moon operates differently. Its quakes

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are most Likely caused by two main

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Earth's tidal pulling and the Moon's

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continuous cooling and shrinking. The deep

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moonquakes occurring hundreds of miles inside

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are due to Earth's gravity pulling on her

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satellite.

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Anna: And the weaker quakes closer to the surface

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are generally attributed to the Moon's

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gradual cooling and shrinking. Since its

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formation billions of years ago, the Moon has

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actually lost about 150ft of

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its diameter. There are also minor tremors

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from meteoroid impacts or surface rocks

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reacting to heating and cooling from the sun.

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So it's a world that's constantly shaking.

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Avery: When we talk about the risks to future bases,

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it becomes quite significant. Short term

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missions like the Apollo landings, where

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astronauts were on the Moon for less than two

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weeks, didn't face much danger. But for

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permanent bases, the chances of damage during

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a quake go up simply due to the extended

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exposure.

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Anna: Nicholas Schmer put it into perspective. He

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said if astronauts are there for a day,

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they'd just have very bad luck. If there was

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a damaging event, they. But if you have a

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habitat or crewed mission up on the Moon for

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a whole decade, that's

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3,650 days times 1

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in 20 million. Or the risk of a hazardous

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moonquake becoming about 1 in 5,500.

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Avery: He likened it to, uh, going from the

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extremely low odds of winning a lottery

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to the much higher odds of being dealt a four

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of a kind poker hand. It really illustrates

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how much the probability increases over time.

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Anna: And it's not just habitats. Countries like

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Russia, China and the US are planning to put

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nuclear power plants on the Moon. These

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facilities would supply massive amounts of

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power, but they'd also be susceptible to

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quake damage. This means any construction

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will need tough safety margins and shouldn't

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be located near active fault lines.

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Avery: Which is a tall order considering how many

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fault lines thread through the Moon. That's

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why this study of lunar paleoseismology

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looking at evidence of past quakes is so

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crucial. It will help us chart the safest

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places to build these long term habitats and

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power plants. It's all about understanding

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our cosmic neighbourhood.

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Before we make ourselves at home from

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lunar shaking, let's zoom out to something

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truly dramatic happening in the cosmos.

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Scientists have captured the explosive end of

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a massive star in a scenario unlike

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anything they've seen before.

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Anna: That's right, Avery. This event, more than

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700 million light years away, began as

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a faint flicker. Within days, the light

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flared, faded, and then, surprisingly,

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flared again. It was completely

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unlike the standard playbook for dying stars.

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Avery: What makes this even more incredible is that

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an artificial intelligence System flagged the

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event in real time. This allowed scientists

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to capture every phase of what may be the

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first recorded case of a massive star

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exploding as it tried to devour a black

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hole companion. Talk about cosmic drama.

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This supernova, named

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SN2023ZKD, was

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first spotted in July 2023 by the Zwicky

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Transient Facility and then analysed by a

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team from the Centre for Astrophysics at

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Harvard and Smithsonian mit. Their

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findings, published in the Astrophysical

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Journal, provide the clearest evidence yet

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that such extreme binary interactions can

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actually trigger a stellar detonation. It

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was part of the Young Supernova Experiment, a

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project designed to catch these exploding

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stars in their earliest stages. The AI system

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gave astronomers a crucial head start,

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allowing them to follow the explosion in near

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real time from both ground and space

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observatories.

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Anna: Alexander Agliano, the lead author of

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the study, stated that their analysis shows

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the blast was sparked by a catastrophic

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encounter with a black hole companion,

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providing the strongest evidence to date that

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such close interactions can indeed

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detonate a star.

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Avery: The leading explanation is that this massive

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star and black hole were locked in a decaying

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orbit. As they drew closer, the black hole's

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immense gravity pulled gas from the star into

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a surrounding disc. This intense stress is

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believed to have triggered the explosion

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before the star could fully engulf the black

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hole.

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Anna: Another possibility is that the black hole

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completely shredded the star, with the

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debris's collisions then powering the

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supernova's light. In either scenario,

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the aftermath left behind a heavier black

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hole.

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Avery: What really stood out to astronomers were the

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unusual light patterns from Earth.

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SN2023ZKD initially

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looked like a normal supernova. A single

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burst of light followed by a gradual fade.

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But then, months later, it did something

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truly extraordinary. It brightened again.

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Anna: Archival records showed that the system had

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actually been slowly brightening for more

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than four years before the explosion,

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a rare and telling sign of pre death

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instability. The analysis revealed that the

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supernova's light was shaped by layers of gas

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shed by the star in its final years.

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Avery: The first brightening came from the blast

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wave colliding with diffused gas, while while

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that second peak was fueled by a slower

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collision with a dense disc shaped cloud.

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The structure and timing of these events

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strongly point to extreme gravitational

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forces from a nearby compact object.

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Anna: It's clear that AI played a crucial role

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here. As Gagliano mentioned, their machine

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Learning system flagged

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SN2023SKD months

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before its most unusual behaviour, which gave

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them ample time to secure the critical

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observations needed to unravel this

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extraordinary explosion V. Ashley Villar,

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a.

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Avery: AH co author and assistant professor of

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astronomy at cfa, added that this event shows

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some of the clearest signs they've seen of a

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massive star interacting with the companion

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in the years before an explosion. They

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believe this might be part of a whole class

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of hidden explosions that AI will help them

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discover in the future.

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Anna: With new observatories like the veracy Rubin

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Observatory soon scanning the entire sky

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every few nights and projects like the Young

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Supernova Experiment continuing to identify

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new events quickly, astronomers expect expect

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to catch more of these rare and complex

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explosions in action. It's truly

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a new era for observing the most extreme

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cosmic events. That's an incredible story

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of cosmic violence and detection.

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Now let's shift gears a bit and delve into a

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long standing cosmic mystery. The case of

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the universe's missing sulphur.

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Avery: It sounds like something out of a detective

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novel. For years, scientists have been

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puzzled because there simply isn't as much

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sulphur floating around in deep space as they

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expected. This is quite an enigma,

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considering Sulphur is the 10th most abundant

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element in the universe and crucial for both

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planets and life.

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Anna: Exactly. But a, uh, new international study

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might have finally found its hiding place.

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Researchers from the University of

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Mississippi, the University of Hawaii at

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Manoa and Georgia State University teamed

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up to search for answers, publishing their

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findings in Nature Communication.

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Avery: So where has all the sulphur been? The team's

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results suggest that it's not actually

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missing at all. Instead, it's locked away in

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solid forms, bound within icy grains of

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interstellar dust.

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Anna: In these frigid environments, sulphur atoms

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can arrange themselves in two main

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neat eight atom rings called

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octasulfur crowns and chains of

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sulphur atoms connected by hydrogen, known

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as polysulfons. These structures

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literally stick to icy dust grains,

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essentially freezing the sulphur out of view.

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Avery: It's fascinating how a common element on

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Earth found in volcanoes and power plants

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can be so elusive in space. Ralph

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Kaiser, one of the lead researchers,

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explained that the observed amount of sulphur

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in dense molecular clouds is three orders of

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magnitude less than predicted gas phase

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abundances. That's a huge difference.

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Anna: Astronomers typically identify elements in

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space by detecting the unique patterns of

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light they emit or absorb. While tools

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like James Webb Space Telescope can easily

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pick out oxygen, carbon and nitrogen,

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sulphur just doesn't follow the rules in the

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same way. As researcher uh, Ryan Fortenberry

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noted, when you do that for sulphur, it's out

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of whack.

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Avery: Another challenge is sulfur's shape. Shifting

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nature. Fortenberry likened it to a virus

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always changing shape as it moves, making it

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incredibly difficult to track. But this new

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research points to stable molecular forms

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that astronomers can now specifically hunt

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for using advanced radio telescopes.

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Anna: By recreating the conditions of deep space in

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laboratory experiments, the researchers

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confirmed that these solid sulphur compounds

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could indeed form on icy surfaces.

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And here's the Once these icy grains are

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heated in young star systems, the sulphur can

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sublime, meaning it transforms directly from

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a solid to a gas, making it finally

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detectable from Earth.

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Avery: This work could finally help astronomers

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piece together sulfur's role in both the

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formation of planets and the very chemistry

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that supports life. If they can pinpoint

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exactly where sulphur is stored, it could

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deepen our understanding of how essential

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life building elements are distributed across

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the cosmos. And, um, even improve models of

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planetary atmospheres, especially for

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exoplanets.

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Anna: It's a perfect example of astrochemistry

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forcing hard questions and leading to

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creative solutions. As Fortenberry put it,

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this kind of foundational research has the

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potential for significant unintended positive

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consequences for our broader understanding of

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the universe.

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Avery: That's a great point, Anna.

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Speaking of profound insights into how

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celestial bodies form, our next story

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completely redefines what we thought we knew

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about Vesta, one of the largest objects in

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the asteroid belt. For years, astronomers

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viewed Vesta as almost a miniature version of

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Earth, something between a rock in space and

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a full fledged planet due to its rocky

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surface, distinct layers, and volcanic

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history.

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Anna: But new research is truly shaking up that

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view. Data collected from NASA's dawn

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spacecraft, reanalyzed years later,

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is rewriting our understanding of how early

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planets may have formed and what might have

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gone wrong in Vesta's case.

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Avery: M the Dante spacecraft orbited Vesta from

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2011 to 2012, meticulously

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mapping its surface and measuring its

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gravity. Initially, this data suggested

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Vesta had undergone planetary

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differentiation, the process where dense

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materials sink to form a core and

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lighter materials create a mantle and crust.

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The Just like Earth or Mars, Vesta's

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volcanic surface seemed to confirm this.

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Anna: However, a decade after Dawn's mission ended

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in 2018, researchers at NASA's Jet

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Propulsion Lab, or JPL, decided to take

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a fresh look at the data, using better

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calibration and updated processing tools.

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And what they found completely challenged

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that long held Vesta may not have

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a core at all.

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Avery: That's a huge revelation. Ryan Park, a

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senior research scientist and principal

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engineer at jpl, expressed excitement,

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saying they were thrilled to confirm the

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data's strength in revealing Vesta's deep

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interior. By reanalyzing the dawn data,

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the team made a more precise estimate of, uh,

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Vesta's moment of inertia.

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Anna: For those wondering, the moment of inertia is

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a physics concept that reveals how mass is

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distributed within a rotating body.

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Assistant Professor Seth Jacobson of Michigan

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State University explained it with a simple

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Think of a figure skater. When they pull

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their arms in, they spin faster. When they

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stretch their arms out, they slow down.

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Celestial bodies with dense cores behave like

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skaters with their arms in rotating

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differently.

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Avery: And Vesta's behaviour simply didn't match

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what scientists expected from a core bearing

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body. Its moment of inertia and calculated

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at only 6.6% lower than a

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perfectly uniform structure suggests its

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internal structure is. Surprisingly, even

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this value points to only a mild difference

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in density beneath its crust, not the

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deep layering we see in fully differentiated

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planets.

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Anna: This new perspective has forced scientists to

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rethink everything they thought they knew

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about Vesta's formation. They're now

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exploring two main ideas. The first

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is that Vesta began to differentiate. Its

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insides started to melt and separate into

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layers. But something interrupted the

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process. This could have been a late start in

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forming or limited exposure to heat producing

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elements like radioactive aluminium.

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Avery: 26 the second theory is even more

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dramatic. It suggests Vesta might be the

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shattered remnants of a much larger

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differentiated planet. That body could have

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been destroyed in a massive collision during

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the solar system's early years. And Vesta

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would then be just one of the reassembled

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pieces, essentially chunky space debris of,

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uh, a growing world that never quite made

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it. Seth Jacobson, who initially

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considered this idea a stretch years ago,

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now takes it seriously.

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Anna: The mystery deepens when you consider Vesta's

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meteorites. Researchers have collected

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thousands of space rocks on Earth believed to

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have come from Vesta. And these meteorites

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look like they formed in a molten environment

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showing signs of volcanic activity. However,

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they don't obviously suggest incomplete

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differentiation, which creates a problem for

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the first hypothesis of partial melting.

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Avery: That's quite the conundrum. The second idea,

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where Vesta is a remnant of a larger

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destroyed planet, might better explain the

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rocks by. But it also raises new questions

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about how such a colossal collision would

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occur. Jacobson's lab is actively

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modelling what those collisions m might have

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looked like and how debris like Vesta might

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have formed.

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Anna: Ultimately, Vesta's internal structure holds

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the key to understanding how planets grow

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or fail to. For a long time,

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Vesta seemed like a textbook

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protoplanet, an object that started forming

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but didn't quite make it. Now

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that picture has become much blurrier.

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Avery: Instead of being a failed planet, Vesta might

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be something even more intriguing. A, uh,

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survivor of cosmic violence. If it

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truly is a chunk of a planet destroyed in the

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early solar system, it could provide

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scientists with invaluable insights into the

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collisions and processes that shaped the

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worlds we see today.

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Anna: As Jacobsen puts it, no longer is the Vesta,

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um, meteorite collection a sample of a body

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in space that failed to make it as a planet.

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These could be pieces of an ancient planet

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before it grew to full completion. We just

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don't know which planet that is yet.

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Avery: This discovery is a powerful reminder that in

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science, answers often lead to more

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questions. This reanalysis of old

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data isn't just changing our understanding of

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one asteroid. It could reshape how

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researchers think about early planetary

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formation across the entire solar system.

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Anna: And that's it for this episode. What a

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journey we've had today. From the surprising

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seismic activity of our moon and the critical

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implications for future lunar bases, to the

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mind boggling explosion of a star trying to

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swallow a block whole, the universe

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certainly keeps us on our toes.

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Avery: Absolutely, Anna. Uh, and let's not forget

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the cosmic mystery of the missing sulphur,

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now believed to be hidden in icy dust, uh,

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grains. And the groundbreaking reanalysis of

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Vesta, which challenges its long held

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status as a protoplanet, suggesting it might

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be a fragment of a destroyed world.

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Anna: It's been a day packed with fascinating

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discoveries that push the boundaries of our

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understanding.

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Avery: Indeed. Thank you for joining us on Astronomy

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Daily. We hope you enjoyed diving into the

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latest space news with us.

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Anna: We look forward to having you back next time

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for more amazing insights from across the

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cosmos. Until then, keep looking up.
