Nuclear Moon Power, Mars Ocean Evidence, and Brains in Space
Astronomy Daily - January 14, 2026 Episode Nuclear Moon Power, Mars Ocean Evidence, and Brains in Space Episode Description Join hosts Anna and Avery for an action-packed episode covering six major space stories! We explore NASA's ambitious plan to put a nuclear reactor on the Moon by 2030, get the latest on tomorrow's historic ISS medical evacuation, examine compelling new evidence for an ancient Martian ocean, discover how spaceflight literally shifts astronauts' brains, learn about a revolutionary privately-funded space telescope, and find out how scientists finally solved the mystery of the Moon's two faces. Episode Duration: 17 minutes Episode Highlights ⚛️ NASA Commits to Lunar Nuclear Reactor by 2030
NASA and DOE sign memorandum of understanding
President Trump's executive order drives ambitious timeline
Nuclear power essential for permanent lunar bases
Building on 50+ years of space nuclear collaboration
🚀 Crew-11 Cleared for Wednesday Departure
First-ever medical evacuation from ISS proceeds on schedule
Undocking set for 5:05 PM EST Wednesday, January 15
Splashdown off California coast at 3:41 AM Thursday
Station will operate with skeleton crew of three
🌊 Ancient Martian Ocean Evidence Discovered
River delta features identified in Valles Marineris
Ocean covered half of Mars 3+ billion years ago
High-resolution orbital imagery reveals ancient coastline
Major implications for Mars' past habitability
🧠 Spaceflight Shifts Astronaut Brains Inside Skulls
MIT study reveals brains move "backward, upward and tilted"
Changes persist up to 6 months after return to Earth
Brain displacement linked to post-flight balance issues
Critical for planning longer Moon and Mars missions
🔭 $500M Private Space Telescope to Launch in 3-5 Years
Eric Schmidt funds Lazuli Space Observatory
"Move fast" philosophy applied to flagship telescope
Designed to catch transient events like gravitational waves
Will test technology for future NASA missions
🌙 Moon's Two-Faced Mystery Finally Solved
Chang'e-6 samples reveal impact chemistry differences
Ancient collision reshaped Moon's internal structure
Evidence of hemisphere-wide mantle convection
First hard evidence from lunar far side
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Episode link: https://play.headliner.app/episode/31114183?utm_source=youtube
Kind: captions
Language: en
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Hello everyone and welcome to Astronomy
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Daily. I'm Anna
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>> and I'm Avery. Thanks for joining us
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this Tuesday, January 14th, 2026. We've
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got a fantastic lineup of space news for
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you today.
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>> We really do. We're covering everything
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from nuclear reactors on the moon to
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ancient Martian oceans, plus some
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fascinating discoveries about how space
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flight affects astronaut brains. And
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we'll be talking about a major ISS
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update, a new privately funded space
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telescope, and scientists finally
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solving a six decade old mystery about
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the moon's two faces.
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>> It's going to be an exciting episode.
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So, let's dive right in.
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>> Anna, let's start with some big news
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from NASA and the Department of Energy.
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The United States is getting serious
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about putting a nuclear reactor on the
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moon by 2030.
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>> That's right, Avery. This isn't just
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talk anymore. Last week, NASA
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Administrator Jared Isaacman and US
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Secretary of Energy Chris Wright signed
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a memorandum of understanding that
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reaffirms their commitment to meet that
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ambitious deadline.
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>> And this comes on the heels of President
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Trump's executive order from December
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calling for construction to begin on a
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lunar base by 2030 with a nuclear
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reactor ready to launch by that same
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year. Isacman said something really
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interesting in the announcement. He
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said, "Achieving this future requires
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harnessing nuclear power. This agreement
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enables closer collaboration between
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NASA and the Department of Energy to
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deliver the capabilities necessary to
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usher in the golden age of space
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exploration and discovery.
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>> It makes sense when you think about it.
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Nuclear power can generate electricity
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continuously for years without
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refueling. And it's not affected by the
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moon's two week long nights or changing
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weather conditions like solar panels
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would be. And this isn't the first time
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NASA and the Department of Energy have
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worked together on space nuclear
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systems. They've been collaborating for
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more than half a century.
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>> Right. Many of NASA's deep space robotic
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explorers have used radioisotope
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thermmoelect electric generators or RTGs
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as a power source. We're talking about
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missions like the Cassini Saturn orbiter
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and the Curiosity and Perseverance Mars
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rovers.
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>> But this lunar reactor would be
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something different entirely. It would
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be designed to power one or more bases
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on the lunar surface as part of NASA's
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Aremis program. Secretary Wright made a
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connection to America's historic
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achievements. He said, "History shows
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that when American science and
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innovation come together, from the
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Manhattan Project to the Apollo mission,
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our nation leads the world to reach new
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frontiers once thought impossible. This
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agreement continues that legacy." For
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NASA's Aremis program, having a
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reliable, long-term power source on the
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moon is absolutely critical. If we're
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going to establish a permanent presence
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there and use it as a stepping stone to
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Mars, we need infrastructure that can
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operate reliably for years.
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>> And the 2030 timeline is really
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aggressive. We're talking about just
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over 4 years from now. That's incredibly
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fast for a project of this magnitude.
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>> It is. But with the renewed focus on
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lunar exploration and the competition
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with other space fairing nations,
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particularly China, there's definitely
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motivation to move quickly.
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>> Speaking of space developments, we have
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an important update on the crew 11
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situation at the International Space
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Station. Mission managers have
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officially given the go for the crew's
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return to Earth tomorrow.
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>> That's right. NASA astronauts Zena
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Cardman and Mike Fininky along with Jaxa
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astronaut Kimya Yu and Ross Cosmos
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cosminaut Oleg Platonov are scheduled to
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undock from the Harmony module at 5:05
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p.m. Eastern time on Wednesday.
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>> And they're coming home aboard the
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SpaceX Dragon crew spacecraft with
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Cardman commanding and finy piloting.
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The weather forecast is looking
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excellent for their parachute assisted
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splashdown off the coast of California,
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which is scheduled for 3:41 a.m. on
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Thursday. Yesterday, the crew spent most
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of their time preparing for departure.
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They packed cargo, reviewed return to
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Earth procedures, and transferred
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hardware. Hardman and her crew mates
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also trained on how to use respirators
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during unlikely emergency events like
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anemmonially. NASA is planning extensive
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coverage of the event. NASA Plus will
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begin live coverage at 3 p.m. on
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Wednesday when the crew enters the
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Dragon spacecraft and says goodbye to
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the remaining crew on the station.
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>> Coverage continues at 4:45 p.m. for the
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actual undocking, then returns at 2:15
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a.m. Thursday for the descent, and
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finally at 5:45 a.m. for the post
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splashdown news conference. You can
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watch all of this on NASA Plus, Amazon
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Prime, or NASA's YouTube channel.
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>> As we discussed yesterday, this is the
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first medical evacuation in ISS history.
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The crew was originally scheduled to
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stay until after crew 12 arrived in
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midFebruary, but an undisclosed medical
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condition affecting one of the four crew
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members prompted NASA to bring them home
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early. After crew 11 leaves, expedition
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74 will be commanded by Rosscosmos
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cosminaut Sergey Kuds Ferkov, leading
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flight engineers Sergey Mikv and NASA's
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Chris Williams. That's a skeleton crew
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of just three people running the entire
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station. Yesterday, Kutz Virkoff and
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Mikv participated in a study assessing
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how crews make decisions and work
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together in space, which is especially
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relevant given they'll be operating with
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a reduced crew for a while.
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>> BASA is still evaluating whether they
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can move up the crew 12 launch date to
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replenish the station crew sooner than
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originally planned.
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>> Now, let's talk about Mars. Anna,
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there's exciting new evidence that an
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ancient ocean once covered half the
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planet. This is really fascinating
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research, Avery. A team led by Ignatius
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Argadestia, a PhD student at the
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University of Burn, has identified
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features in Mars' Val Marinys that look
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remarkably similar to river deltas here
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on Earth.
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>> Val Marinys is that massive canyon
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system on Mars. Right. The largest in
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the solar system.
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>> Exactly. Along with Olympus Mons, it's
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one of Mars' most defining features.
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This research focused specifically on
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the southeast part of a subc canyon
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called Capradus Chazma.
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>> The researchers used images from
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multiple orbital cameras, CTX and
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high-rise on NASA's Mars Reconnaissance
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Orbiter and CASSIS
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on the ESA/ Rosscosmos trace gas
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orbiter. They also worked with digital
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elevation models to examine what they
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call scarp fronted deposits.
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>> These scarp fronted deposits or SFDs are
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fan-shaped sediment deposits that form
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where a river empties into a body of
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standing water. The team identified
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three of these features in Capraatus
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Chazma and they're almost identical to
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river deltas we see on Earth.
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>> Professor Fritz Schlunger put it really
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clearly. He said, "The structures that
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we were able to identify in the images
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are clearly the mouth of a river into an
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ocean.
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>> What's particularly compelling is that
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all three SFDs are at the same
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elevation. That suggests they were all
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deposited at the same water level,
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essentially marking an ancient
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coastline." The researchers believe
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these deposits were formed sometime
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between the late Hisperian period and
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the early Amazonian period. That's
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roughly between 3.7 billion and 3
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billion years ago.
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>> Reed author Argodestia said something
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interesting in the press release. He
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said, "When measuring and mapping the
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Martian images, I was able to recognize
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mountains and valleys that resemble a
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mountainous landscape on Earth. However,
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I was particularly impressed with the
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deltas that I discovered at the edge of
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one of the mountains." Previous research
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had suggested Mars had a large ocean,
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but this study provides much more
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concrete evidence. Slungjugger noted
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that earlier claims were based on less
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precise data and sometimes indirect
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arguments.
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>> But their reconstruction of the sea
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level is based on clear evidence of an
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actual coastline thanks to these
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highresolution images. The paleo
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shoreline they identified extends from
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Val Marinus all the way to the northern
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lowlands. Argadestia summed it up
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nicely. With our study, we were able to
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provide evidence for the deepest and
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largest former ocean on Mars to date. An
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ocean that stretched across the northern
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hemisphere of the planet. This has huge
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implications for Mars's past
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habitability. As the authors write,
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their findings will impact research on
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the evidence for potential life on Mars.
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Since this represents a period when Mars
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had the highest water availability,
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>> it's amazing to think that billions of
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years ago, Mars might have looked very
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different from the cold, dry desert we
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see today.
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>> Speaking of things changing, Avery,
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let's talk about a fascinating new study
00:09:34.720 --> 00:09:37.430
on how spaceflight literally changes
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astronauts brains.
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>> This is wild, Anna. A team led by Rachel
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Sidler at MIT took MRI scans of 26
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astronauts and 24 non-stronaut
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participants and they found that
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spaceflight causes astronauts brains to
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shift position inside their skull. The
00:09:54.959 --> 00:09:57.590
study was published just yesterday. The
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researchers found a consistent pattern
00:09:59.839 --> 00:10:01.910
of the brain shifting backward and
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upward and rotating upward after time in
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microgravity. And here's the kicker.
00:10:07.680 --> 00:10:09.829
Some of these positional changes were
00:10:09.839 --> 00:10:12.470
still detectable months after astronauts
00:10:12.480 --> 00:10:13.990
returned to Earth.
00:10:14.000 --> 00:10:15.829
>> Instead of looking at the brain as one
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whole unit, they divided it into 130
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separate regions and examined each one
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individually. This regional analysis
00:10:24.079 --> 00:10:26.069
showed many areas with significant
00:10:26.079 --> 00:10:29.030
displacement across two spatial axes.
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>> The data set included astronauts with
00:10:31.519 --> 00:10:33.829
different mission lengths, roughly 2
00:10:33.839 --> 00:10:36.710
weeks, 6 months, and one year. They
00:10:36.720 --> 00:10:38.870
found significant positional shifts
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across large portions of the brain with
00:10:41.680 --> 00:10:44.389
some displacements measured as high as
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2.52 mm in subjects with the most time
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in space.
00:10:49.680 --> 00:10:51.670
>> To put that in perspective, that's about
00:10:51.680 --> 00:10:53.910
a tenth of an inch. It might not sound
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like much, but when we're talking about
00:10:55.680 --> 00:10:57.590
the brain inside your skull, that's
00:10:57.600 --> 00:10:59.750
actually quite significant. The
00:10:59.760 --> 00:11:02.230
researchers also compared astronauts
00:11:02.240 --> 00:11:04.630
with people who participated in a long
00:11:04.640 --> 00:11:07.110
duration headdown tilt bed rest
00:11:07.120 --> 00:11:09.509
experiment which is used to simulate
00:11:09.519 --> 00:11:12.630
some effects of microgravity on Earth.
00:11:12.640 --> 00:11:13.990
>> And they found some interesting
00:11:14.000 --> 00:11:16.470
differences. Astronauts showed stronger
00:11:16.480 --> 00:11:18.389
upward movement while the bed rest
00:11:18.399 --> 00:11:20.790
participants showed stronger backward
00:11:20.800 --> 00:11:22.949
movement. Only some of the brain shape
00:11:22.959 --> 00:11:24.870
changes observed after space flight
00:11:24.880 --> 00:11:27.350
appeared in the bed rest group. This
00:11:27.360 --> 00:11:29.990
tells us that head down bed rest, while
00:11:30.000 --> 00:11:32.790
useful, doesn't perfectly replicate what
00:11:32.800 --> 00:11:34.710
happens to the brain in actual
00:11:34.720 --> 00:11:37.350
microgravity, there are unique effects
00:11:37.360 --> 00:11:40.470
that only real space flight produces.
00:11:40.480 --> 00:11:42.230
>> One of the most important findings was
00:11:42.240 --> 00:11:44.470
the connection to balance problems. The
00:11:44.480 --> 00:11:46.470
study found that displacement affecting
00:11:46.480 --> 00:11:48.949
sensory related brain regions correlated
00:11:48.959 --> 00:11:50.949
with larger declines in astronauts
00:11:50.959 --> 00:11:53.110
balance after space flight.
00:11:53.120 --> 00:11:55.350
>> Right? We know that when astronauts
00:11:55.360 --> 00:11:57.829
return from space, they often experience
00:11:57.839 --> 00:12:00.470
balance issues because their inner ears
00:12:00.480 --> 00:12:02.710
sense of direction isn't immediately
00:12:02.720 --> 00:12:05.590
restored. This study helps explain why
00:12:05.600 --> 00:12:06.949
that happens.
00:12:06.959 --> 00:12:08.949
>> And while astronauts normally find their
00:12:08.959 --> 00:12:10.710
footing within a week or so, the
00:12:10.720 --> 00:12:12.470
physical shifts in their brains
00:12:12.480 --> 00:12:15.110
persisted for up to 6 months post space
00:12:15.120 --> 00:12:17.910
flight. That's quite remarkable. The
00:12:17.920 --> 00:12:20.389
authors note that this underscores the
00:12:20.399 --> 00:12:22.790
longlasting effects of spaceflight on
00:12:22.800 --> 00:12:25.590
neuroanatomy. They recommend future
00:12:25.600 --> 00:12:28.550
studies with larger astronaut crews on a
00:12:28.560 --> 00:12:30.790
broad range of mission lengths to better
00:12:30.800 --> 00:12:32.949
understand how quickly these shifts
00:12:32.959 --> 00:12:35.350
begin and how they evolve.
00:12:35.360 --> 00:12:37.269
>> This research is crucial as we plan
00:12:37.279 --> 00:12:38.790
longer missions to the moon and
00:12:38.800 --> 00:12:41.190
eventually to Mars. Understanding how
00:12:41.200 --> 00:12:43.269
extended space flight affects the brain
00:12:43.279 --> 00:12:45.110
will help us better prepare astronauts
00:12:45.120 --> 00:12:47.509
and develop countermeasures. Avery,
00:12:47.519 --> 00:12:49.590
let's shift gears and talk about a
00:12:49.600 --> 00:12:51.829
really exciting development in space
00:12:51.839 --> 00:12:54.310
telescope technology. There's a new
00:12:54.320 --> 00:12:56.470
privately funded observatory called
00:12:56.480 --> 00:12:58.629
Lazuli that could change how we build
00:12:58.639 --> 00:13:01.190
flagship class telescopes. This is
00:13:01.200 --> 00:13:03.750
fascinating, Anna. The Lazuli Space
00:13:03.760 --> 00:13:05.910
Observatory is being funded by Eric
00:13:05.920 --> 00:13:08.310
Schmidt, the former CEO of Google, and
00:13:08.320 --> 00:13:09.670
his wife Wendy through their
00:13:09.680 --> 00:13:11.750
philanthropic organization Schmidt
00:13:11.760 --> 00:13:14.470
Sciences. We're talking about a $500
00:13:14.480 --> 00:13:17.190
million investment. The whole premise is
00:13:17.200 --> 00:13:19.509
applying the new space philosophy to
00:13:19.519 --> 00:13:22.069
space telescopes. You know that Silicon
00:13:22.079 --> 00:13:24.870
Valley mindset of move fast and don't
00:13:24.880 --> 00:13:27.269
break things. The idea is to prove that
00:13:27.279 --> 00:13:29.430
you don't need decades and billions of
00:13:29.440 --> 00:13:31.910
dollars to build a flagship level space
00:13:31.920 --> 00:13:33.030
observatory.
00:13:33.040 --> 00:13:35.430
>> Right? Compare this to the James Webb
00:13:35.440 --> 00:13:38.389
Space Telescope which cost 10 billion or
00:13:38.399 --> 00:13:40.629
the upcoming Nancy Grace Roman Space
00:13:40.639 --> 00:13:42.550
Telescope which is on track for $3
00:13:42.560 --> 00:13:45.110
billion. These huge costs come from
00:13:45.120 --> 00:13:47.590
using completely derisked flight proven
00:13:47.600 --> 00:13:49.990
technology to ensure taxpayer dollars
00:13:50.000 --> 00:13:52.230
don't literally go up in flames. But
00:13:52.240 --> 00:13:55.829
Schmidt has a $ 36 billion fortune. So
00:13:55.839 --> 00:13:58.230
even if Lzulli fails, he can afford the
00:13:58.240 --> 00:14:01.110
loss. And that's kind of the point. This
00:14:01.120 --> 00:14:03.269
is an experiment to see if the approach
00:14:03.279 --> 00:14:05.910
even works for expensive flagship level
00:14:05.920 --> 00:14:07.110
observatories.
00:14:07.120 --> 00:14:09.590
>> To keep costs down, up to 80% of the
00:14:09.600 --> 00:14:11.269
telescope will use off-the-shelf
00:14:11.279 --> 00:14:13.509
components. and operating under Schmidt
00:14:13.519 --> 00:14:15.430
Sciences alleviates a lot of the
00:14:15.440 --> 00:14:16.790
bureaucratic and political
00:14:16.800 --> 00:14:18.949
decision-making that inevitably delays
00:14:18.959 --> 00:14:20.790
government- funded programs.
00:14:20.800 --> 00:14:23.030
>> So, where does Lazuli fit in the bigger
00:14:23.040 --> 00:14:25.430
picture? Web is obviously already
00:14:25.440 --> 00:14:27.829
operational, sending back spectacular
00:14:27.839 --> 00:14:30.470
images. Roman is next, scheduled to
00:14:30.480 --> 00:14:33.269
launch in May 2027, but both have
00:14:33.279 --> 00:14:35.509
weaknesses when tracking transient
00:14:35.519 --> 00:14:36.550
phenomena.
00:14:36.560 --> 00:14:39.189
>> Exactly. Events like kilon nove or
00:14:39.199 --> 00:14:41.350
gravitational wave producing black hole
00:14:41.360 --> 00:14:43.750
mergers happen on time scales of hours
00:14:43.760 --> 00:14:46.550
not days. They require almost immediate
00:14:46.560 --> 00:14:48.310
response from observatories to catch
00:14:48.320 --> 00:14:49.670
them before they end.
00:14:49.680 --> 00:14:52.550
>> And web just can't slew. That's the term
00:14:52.560 --> 00:14:54.790
for rotating to a new target fast
00:14:54.800 --> 00:14:56.949
enough. It captures extremely
00:14:56.959 --> 00:14:59.430
highresolution images, but it takes too
00:14:59.440 --> 00:15:01.590
long to get into position. On the other
00:15:01.600 --> 00:15:04.069
hand, Roman is a survey telescope that
00:15:04.079 --> 00:15:06.629
looks at white swaps of sky, but doesn't
00:15:06.639 --> 00:15:08.389
have the resolution to examine
00:15:08.399 --> 00:15:10.949
individual systems like Lazuli will.
00:15:10.959 --> 00:15:13.990
>> So, Lazil's sweet spot is target of
00:15:14.000 --> 00:15:16.389
opportunity tracking. It's designed to
00:15:16.399 --> 00:15:18.470
slew within an hour and a half to
00:15:18.480 --> 00:15:20.870
observe short-lived events. It'll work
00:15:20.880 --> 00:15:22.550
in concert with groundbased
00:15:22.560 --> 00:15:24.790
observatories like LIGO, the
00:15:24.800 --> 00:15:27.269
gravitational wave detector. But it has
00:15:27.279 --> 00:15:29.910
the advantage of being in space, so no
00:15:29.920 --> 00:15:32.389
cloud cover or daylight to worry about.
00:15:32.399 --> 00:15:34.550
Lazuli will also have a wild field
00:15:34.560 --> 00:15:37.110
context camera with 23 separate SEMOS
00:15:37.120 --> 00:15:39.670
sensors, kind of like Roman, to detect
00:15:39.680 --> 00:15:41.910
things like exoplanet transits.
00:15:41.920 --> 00:15:44.150
>> And here's something really cool. It
00:15:44.160 --> 00:15:45.990
should be able to directly image
00:15:46.000 --> 00:15:48.389
exoplanets using a vector vortex
00:15:48.399 --> 00:15:50.629
coronagraph along with deformable
00:15:50.639 --> 00:15:52.949
mirrors to suppress starlight by up to
00:15:52.959 --> 00:15:55.829
10 million times. This same technology
00:15:55.839 --> 00:15:57.990
is planned for NASA's Habitable Worlds
00:15:58.000 --> 00:15:59.749
Observatory, which won't launch for
00:15:59.759 --> 00:16:02.310
decades. So, Lazuli will actually serve
00:16:02.320 --> 00:16:04.629
as a technology demonstration platform
00:16:04.639 --> 00:16:07.030
well before the taxpayer funded mission.
00:16:07.040 --> 00:16:09.269
Perhaps the most impressive aspect is
00:16:09.279 --> 00:16:11.509
the timeline. Schmidt Sciences is
00:16:11.519 --> 00:16:14.069
planning a 3 to 5ear development cycle
00:16:14.079 --> 00:16:16.550
for this massive space observatory.
00:16:16.560 --> 00:16:18.790
That's exponentially faster than any
00:16:18.800 --> 00:16:21.350
comparable government-led system. Though
00:16:21.360 --> 00:16:23.910
to be fair, new space leaders do have a
00:16:23.920 --> 00:16:26.230
tendency to underestimate timelines.
00:16:26.240 --> 00:16:28.150
Even if it takes twice as long, though,
00:16:28.160 --> 00:16:30.069
we'd still get another flagship level
00:16:30.079 --> 00:16:32.069
observatory within a decade.
00:16:32.079 --> 00:16:34.629
>> And here's something amusing. If Schmidt
00:16:34.639 --> 00:16:37.350
just leaves his remaining $ 36 billion
00:16:37.360 --> 00:16:40.790
in an S&P 500 index fund, he'd make back
00:16:40.800 --> 00:16:43.269
around 40 times what the entire project
00:16:43.279 --> 00:16:45.749
cost over a 5-year period. So,
00:16:45.759 --> 00:16:47.829
financially, this is barely a blip for
00:16:47.839 --> 00:16:50.389
him. Either we get an amazing new space
00:16:50.399 --> 00:16:52.870
telescope or we get a $500 million
00:16:52.880 --> 00:16:54.629
lesson in what can go wrong when
00:16:54.639 --> 00:16:56.230
applying speed to large-scale
00:16:56.240 --> 00:16:58.710
astrophysics projects. Either way, the
00:16:58.720 --> 00:17:00.230
scientific community learned something
00:17:00.240 --> 00:17:01.030
valuable.
00:17:01.040 --> 00:17:04.069
>> For our final story today, Avery,
00:17:04.079 --> 00:17:06.470
scientists may have finally solved a
00:17:06.480 --> 00:17:09.429
mystery that's puzzled them for over 60
00:17:09.439 --> 00:17:12.309
years. Why does the moon look so
00:17:12.319 --> 00:17:15.350
different on its near and far sides?
00:17:15.360 --> 00:17:17.270
This is based on analysis of dust
00:17:17.280 --> 00:17:19.270
collected from the lunar far side by
00:17:19.280 --> 00:17:22.150
China's Chong A6 mission which returned
00:17:22.160 --> 00:17:24.150
the first ever samples from the moon's
00:17:24.160 --> 00:17:26.710
hidden hemisphere in 2024.
00:17:26.720 --> 00:17:29.270
>> The material came from the south pole
00:17:29.280 --> 00:17:32.150
8kin basin which is believed to be the
00:17:32.160 --> 00:17:34.789
site of the largest impact in the solar
00:17:34.799 --> 00:17:37.909
system. This colossal crater spans
00:17:37.919 --> 00:17:41.110
nearly a quarter of the lunar surface. A
00:17:41.120 --> 00:17:43.430
team letter by Hangi Tan from the
00:17:43.440 --> 00:17:45.909
Chinese Academy of Sciences conducted
00:17:45.919 --> 00:17:48.789
isotopic analysis of potassium and iron
00:17:48.799 --> 00:17:51.270
found in the farside dust and compared
00:17:51.280 --> 00:17:53.190
it with samples from the moon's near
00:17:53.200 --> 00:17:54.950
side collected during the Apollo
00:17:54.960 --> 00:17:57.510
missions and by China's Chang A5
00:17:57.520 --> 00:17:58.630
spacecraft.
00:17:58.640 --> 00:18:00.950
>> The results showed a significant
00:18:00.960 --> 00:18:03.909
difference. Nearside samples contained
00:18:03.919 --> 00:18:06.870
more light isotopes while the far side
00:18:06.880 --> 00:18:10.150
material was richer in heavier isotopes.
00:18:10.160 --> 00:18:12.549
particularly of potassium.
00:18:12.559 --> 00:18:14.470
>> This type of isotopic separation
00:18:14.480 --> 00:18:16.789
couldn't be explained by normal volcanic
00:18:16.799 --> 00:18:19.110
activity. Instead, the researcher
00:18:19.120 --> 00:18:22.070
suggest the south pole akin impactor
00:18:22.080 --> 00:18:24.710
generated such extreme heat that lighter
00:18:24.720 --> 00:18:27.270
isotopes were vaporized and lost,
00:18:27.280 --> 00:18:29.350
leaving behind a heavier chemical
00:18:29.360 --> 00:18:32.230
fingerprint. The researchers wrote,
00:18:32.240 --> 00:18:35.110
"This feature most likely resulted from
00:18:35.120 --> 00:18:37.750
potassium evaporation caused by the
00:18:37.760 --> 00:18:41.270
South Pole 8kin basin forming impactor,
00:18:41.280 --> 00:18:43.830
demonstrating the profound influence of
00:18:43.840 --> 00:18:47.430
this event on the moon's deep interior.
00:18:47.440 --> 00:18:49.270
>> What's particularly interesting is that
00:18:49.280 --> 00:18:51.350
the study suggests the impact may have
00:18:51.360 --> 00:18:53.350
punched through the crust and into the
00:18:53.360 --> 00:18:55.750
mantle, permanently changing the moon's
00:18:55.760 --> 00:18:58.870
inner composition. The sample analysis
00:18:58.880 --> 00:19:01.510
revealed that potassium isotopes on the
00:19:01.520 --> 00:19:04.230
far side appear to originate from a
00:19:04.240 --> 00:19:06.710
mantle source distinct from that of the
00:19:06.720 --> 00:19:09.750
near side. This implies widespread
00:19:09.760 --> 00:19:11.990
internal melting and chemical
00:19:12.000 --> 00:19:13.510
redistribution.
00:19:13.520 --> 00:19:15.590
>> The team even proposes that the impact
00:19:15.600 --> 00:19:17.590
might have triggered hemispherewide
00:19:17.600 --> 00:19:20.070
mantle convection, a process that could
00:19:20.080 --> 00:19:22.230
reshape a planet's crust and inner
00:19:22.240 --> 00:19:25.029
layers over time. As they noted in their
00:19:25.039 --> 00:19:28.150
study, this finding also implies that
00:19:28.160 --> 00:19:31.350
largecale impacts are key drivers in
00:19:31.360 --> 00:19:34.870
shaping mantle and crustal compositions.
00:19:34.880 --> 00:19:37.430
>> So, planetary impacts leave far more
00:19:37.440 --> 00:19:39.830
than just visible craters. They can set
00:19:39.840 --> 00:19:42.230
off longlasting internal transformations
00:19:42.240 --> 00:19:44.549
that remain detectable billions of years
00:19:44.559 --> 00:19:45.510
later.
00:19:45.520 --> 00:19:49.029
>> Hang Ton summed it up nicely. With our
00:19:49.039 --> 00:19:51.350
study, we were able to provide evidence
00:19:51.360 --> 00:19:54.310
for the deepest and largest former ocean
00:19:54.320 --> 00:19:57.510
on Mars to date. Wait, that's the wrong
00:19:57.520 --> 00:19:59.110
quote.
00:19:59.120 --> 00:20:00.549
>> Wrong planet, Anna.
00:20:00.559 --> 00:20:02.710
>> Oh my goodness. Let me get that right.
00:20:02.720 --> 00:20:06.310
Pan said, "With the Chang A6 samples,
00:20:06.320 --> 00:20:08.789
scientists now have their first hard
00:20:08.799 --> 00:20:11.430
evidence from the moon's far side, an
00:20:11.440 --> 00:20:14.789
area once entirely out of reach." This
00:20:14.799 --> 00:20:17.190
discovery is particularly timely as
00:20:17.200 --> 00:20:19.110
multiple nations gear up for lunar
00:20:19.120 --> 00:20:21.350
exploration missions, including NASA's
00:20:21.360 --> 00:20:23.830
Aremis program and China's continuing
00:20:23.840 --> 00:20:27.190
Chang missions. Understanding the moon's
00:20:27.200 --> 00:20:29.590
geological history and internal
00:20:29.600 --> 00:20:32.470
structure will be crucial as we plan to
00:20:32.480 --> 00:20:35.270
establish permanent bases there. Each
00:20:35.280 --> 00:20:38.070
new sample and discovery helps us piece
00:20:38.080 --> 00:20:40.710
together the story of how our nearest
00:20:40.720 --> 00:20:43.830
celestial neighbor formed and evolved.
00:20:43.840 --> 00:20:45.430
Well, that brings us to the end of
00:20:45.440 --> 00:20:47.830
today's episode of Astronomy Daily. What
00:20:47.840 --> 00:20:50.470
an incredible day of space news. From
00:20:50.480 --> 00:20:53.110
nuclear reactors on the moon and the
00:20:53.120 --> 00:20:56.630
Crew 11 undocking tomorrow to ancient
00:20:56.640 --> 00:20:59.430
Martian oceans and shifting astronaut
00:20:59.440 --> 00:21:02.390
brains, plus a privately funded space
00:21:02.400 --> 00:21:04.710
telescope and solving the moon's
00:21:04.720 --> 00:21:07.350
two-faced mystery. We've covered a lot
00:21:07.360 --> 00:21:09.750
of ground today. If you enjoyed today's
00:21:09.760 --> 00:21:11.750
episode, please subscribe to Astronomy
00:21:11.760 --> 00:21:13.669
Daily wherever you get your podcasts.
00:21:13.679 --> 00:21:15.510
And don't forget to leave us a review.
00:21:15.520 --> 00:21:17.590
It really helps other space enthusiasts
00:21:17.600 --> 00:21:19.909
discover the show. You can find us on
00:21:19.919 --> 00:21:22.390
social media and at our website for more
00:21:22.400 --> 00:21:25.430
space news and updates. On the socials,
00:21:25.440 --> 00:21:28.549
search for astroaily pod and our website
00:21:28.559 --> 00:21:32.230
can be found at astronomyaily.io.
00:21:32.240 --> 00:21:34.149
Thanks so much for listening everyone.
00:21:34.159 --> 00:21:36.070
>> Until next time, keep looking up.
00:21:36.080 --> 00:21:40.390
>> Clear skies. Sunny day
00:21:40.400 --> 00:21:48.390
stories told
00:21:56.320 --> 00:21:59.039
stories