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This Is Spacetime Series twenty eight, Episode one hundred and
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twelve were broadcast on the seventeenth of September twenty twenty five.
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Coming up on Space Time, ancient rocks revealing how a
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super continent broke apart, scientists confirm water once flowed on
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the asteroid Ryugu, and a new study trying to pin
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down the origins of globular clusters. All that and more
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coming up on space Time.
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Welcome to space Time with Stuart Gary.
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Scientists examining rare minerals found in outback Australia have shown
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how huge tectonic forces so we are apart the super
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continent of Rdinia more than eight hundred million years ago.
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The findings were reported in the journal Geological Magazine, are
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shedding new light on how rare metal rich magmas reached
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the planet's surface. The authors show that niobian rich carbonatites
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rose up from deep within the planet through pre existing
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full zones during a tectonic rifting event between eight hundred
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and thirty and eight hundred and twenty million years ago,
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and that ultimately broke up the super continent Redinia. Carbonatites
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are rare igneous rocks known to host major global deposits
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of critical metals such as niobium and rare earth elements.
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Niobium is a strategic metal vital for producing light, high
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strength steel used in aircraft construction, as well as pipelines,
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electric vehicles, and as a key component in some next
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generation batteries, in superconducting technologies and clean energy production. One
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of the studies authors, Chris Kirklan from Curtain University, says
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these carbonatites are unlike anything previously known in the Aileron
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Province and they contain important concentrations of niobium, but by
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detecting when and how they formed has historically been difficult
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due to their complex geological histories. The Aleron Province is
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located near Alice Springs in the Northern Territory. Kirkland and
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colleagues used multiple isotobe dating techniques and drill call carbonatite
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samples that had been in place during a period of
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continental rifting which preceded the breakup of Rhdinia. By analyzing
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isotopes and using higher resolution imaging, they were able to
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reconstruct more than five hundred million years of geological events
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the rocks had experienced. They found the tectonic setting allowed
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carbonatite magmas to rise through the fault zones. These fault
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zones had remained open and active for hundreds of millions
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of years, delivering metal rich melts from deep within the
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planet's mantle up into its crust. Kirkland says this approach
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allowed him and his colleagues to pinpoint where the carbonatites
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formed and separate those original magnetic events from changes that
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happened later in the rocks.
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Rudineas what's known as a super continent. So that's a
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period of time when all the continental fragments of Earth
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were really all joined together and stop together. So you
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can think, you know, at the minute, we've got Africa
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and America. You can see, you know, the outline of
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those continents kind of looked like they're pretty similar. So
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if we rule back time, those continental fragments would have
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come together. So Rodinia is a super continent about one
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billion years ago. So one billion years ago we had
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the super continent, this aggregation of all these fragments of
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crust on our planet, and it's quite important geologically.
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And as continental drift happened, tectonics took over and Redinea
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split apart about eight hundred and thirty eight hundred and
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twenty million years ago and there's some interesting evidence of that.
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Yeah, that's exactly right. So three time, you know, super
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continents come together and then they break up. But when
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they break up, interesting things happen with the rocks. You know,
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we get more manful material rising through the crassons that
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ass and it brings with it metals and that's kind
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of important for us going exploring to look for certain resources.
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So specific types of rocks. One specific type of rocks
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known as a carbonotype because it's a carbonet magma typically
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is associated with breakup. So Rodinia was breaking up about
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eight hundred and thirty million years ago and that breakup
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event brought metals up from the mantle. And that's a
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pretty interesting process because it helps us go and explore
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for rocks and metals. So we looked at these carbonotypes,
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the rocks from right at the center of Australia. But
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they've previously been looked at, but they're actually really challenging
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to understand their age. But using a range of different
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minerals and isotopic technique, we managed to get an age
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out of them at eight hundred and thirty million years,
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and as we said, that's an important time in Earth
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history because it tells us about the breakup of Rudinia.
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And that's interesting because at that time we also note
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that there's nilobium bearing rocks. So these carbonotypes are bringing
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metals with them, and those metals, we think are being
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formed at the same time, so they're being brought out
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of the mantle and placed into the crust. And that
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that's useful knife because we've got a recipe, if you like,
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for a mineral system, so it helps us to go
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and explore for these other niobium bearing rocks, which is
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an important metal for you know, high strength schemes advanced
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down in green technology like that electric vehicle batteries and
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wind turbines for example, they all the lion niobium. So
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having this recipe for this metal is kind of important
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to help us find more of it.
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Do we know how the metals may deep underground?
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Most metals sink, right, you know, we've got a magnum
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that creates a process where you've got fractionate material, so
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white material will rise up and heavy material will sink die,
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so the mantle becomes more concentrated in metals than one
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of them is niobium. So when you have rifting events
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and that's when magmas are rising up from the mantil,
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it actually provides a mechanism for transferring some of these
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concentrated metals deep in our planets upwards into the crust
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where we can access them. And what specifically interesting is
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these urbonotype melt are very reactive. They're chemically strange rocks,
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so they react quite strongly. They dissolve crystals, but then
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they re precipitate them or redrow them again and in
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that process they drop out the metal into a range
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of different minerals, including one that's named a pyrochlore, and
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that's part of the process that enriches the rocks in metal.
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The entire Western Australian region is an absolute playground or
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new metals and unique geology, isn't it.
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Yeah, that's exactly right. I think there's a number of
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different reasons for that. So one is that through time,
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you know, you get different types of metal deposits forming,
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So gold, for example, tends to be concentrated in really
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old blocks of crust, and then you might get events
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that circulate water and fluid through those rocks when they
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tend to enrich things like gold. But then we have
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other mineral systems which are formed in a different way.
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For example, when we're getting mantle upwelling events like we've
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just been talking about it, like rifting, and those sorts
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of events would happen away from the older blocks. They
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can to occur in slightly younger rocks. I play slightly younger, right,
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We're talking about a process eight hundred and thirty million
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years ago. That's actually quite young for West Australia, where
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we've got these really truly ancient it is across most
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of the yields aren't. For example, is about two point
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six billion years old. That's much much older. But it's
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about having this huge amount of time and this ability
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for and then fluids to interact with each other that
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allows us to have these enrichment events creating all these
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metals that we need for our society at different points
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in time.
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We see this on the surface in the jagged remains
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of these giant cratons.
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Yeah, we do, We absolutely do. So you can find
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lots of interesting rocks on the surface. But of course,
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when you want to fight a mind, you need to
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look at things in three dimensions. So that's when you
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start to think about drill core and exploring for rocks
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deeper under the cover, and that's where we use drill core,
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and we look at those drill courts to understand the
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size and the volumes of rocks that are carrying these metals.
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So it's not just about the exposed rock, it's about
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predicting in if you like three dimensions where these volumes
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of rock occur.
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The size of these features is incredible.
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Yeah, that's exactly right. Yeah, there's these fantastic geophysical maps
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that alliaus to kind of image through the subsurface, and
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there's geological structures that run all the way through our continent.
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It's quite remarkable. There's even one actually very close to
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where you're talking about that runs almost north Spout and
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it looks as if it's a massive, big crack through
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our entire confidence and the reality of that is, well,
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it kind of was. You know, we have these big
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structures that are where the crack arms broke apart and
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came back together again, and those cracks are the exact
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places we have fluid. When geologists talk about fluids, they
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mean magmas, but they also need water circulation as well.
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But they mean silica rock circulation, so magmas and they
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were pumping up along these long lived deep fracture systems.
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These fracture systems can be so huge they tap all
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the way to the mantle. So they're not just surface features.
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These are deep features that really tell us about heart
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planet was put together, and they're the exact places we
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might get metals enrich so planet it's very important for
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carrying out exploration.
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That's Professor Chris Kirkland from Curtain University. And this is
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space time. Still the CAM siders confirmed that water once
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flowed across the asteroid Ryegu, and we look at the
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possible origins of popular clusters. All that and more still
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to come on space time, scientists have shown that liquid
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water once flowed on the parent body which spawned the
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nearest astroid Ryuga, more than a billion years after it
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first formed. The findings, reported in the journal Nature, could
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impact current models of planetary formation, including those describing the
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birth of the Earth, and the study also overturned some
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long held assumptions that water activity on asteroids only occur
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during the earliest moments of the Solar System's history. And
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your results are based on tiny rock fragments of asteroid
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returned by the Japanese Aerospace Exploration agencies hya BUSA two spacecraft,
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which visited Ryugo on a sample return mission back in
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twenty eighteen. The studies lead author so Yoshi Izuka from
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the University of Tokyo. Astronomers already have a relatively good
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understanding of how our solar system formed, but there are
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still gaps, including knowledge of how the Earth can to
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possessed so much water. Now, it's long been hypothesized the
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carbonaceous asteroids like Ryugu, which formed from ISOs and dust
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in the art of solar system, could be one potential
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source of Earth's water. A zuclin colleagues found that Rayugu
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preserved a pristine record of water activity, evidence that fluids
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were moving through its rocks far later than expected, and
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this changes how astronomers think about the long term fate
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of water in asteroids. The heart of the discovery comes
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from an analysis of isotopes of lutetium and hafnium. Is
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radioactive decay from the tetium one seventy six into hafnium
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one seventy six can serve as a sort of clock
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for measuring geological processes. Their presence in specific quantities in
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the sample studied were expected to relate to the age
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of the asteroid in a fairly predictable way, but the
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ratio of the tetium one seventy six to happenium one
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seventy six was farhigher than expected, and this strongly implied
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that some sort of fluid, probably water, was essentially washing
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out the the tetium from the rocks containing it. Now
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the most likely trigger for all of this was an
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impact on the larger parent asteroid of Ryugu, which fractured
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the rock, generating heat and melting the buried ice. This
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allowed the liquid water to percolate through the body, and
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the same impact may well have been responsible for creating
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Rayugu out of its parent asteroid in the first place.
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One of the most important implications for all this is
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that carbon riche asteroids may have contained and delivered much
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more of Earth's water previously thought. It seems Roheugue's parent
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body retained ice for more than a billion years, meaning
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similar bodies striking a young Earth they will have carried
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an estimated two to three times more water than what
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standard models currently account for, significantly affecting Earth's early oceans
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and atmosphere. It suggests that the building blocks of Earth
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were far wetter than previously imagined, and it forced the
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scientists to rethink this starting conditions for Earth's water system
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and how and when our planet first became habitable. This
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is space time still to come. We look at the
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possible origins of those mysterious objects called globular clusters, and
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later in the Science report and you study finds that
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the more psychiatric disorders you have in later life, the
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more likely you are to develop dementia. All that and
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more still to come on space time. For centuries, astronomers
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have puzzled over the origins of some of the universe's
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oldest and dens estellar systems, known as globular clusters, and
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now they may finally have an answer. Globular clusters are
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stellar spheres containing thousands to millions of densely packed, gravitationally
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bound stars. The stars in globular clusters all have a
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similar chemical composition that suggests they were all originally born
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at the same time in the same stellar nursery of
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molecular gas and dust clouds. Most galaxies have large collections
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of globular clusters, orbiting them. Our own galaxy, the Milky Way,
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has at least one hundred and fifty, and a neighboring
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big galaxy, Andromeda, has more than two hundred. But that
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also opens the possibility that at least some globular clusters
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I in fact the stellar cause of satellite dwarf galaxies,
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which were stripped of their outer stars during mergers with
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host galaxies in a process called galactic cannibalism. Now a