WEBVTT

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Anna: Welcome to Astronomy Daily. I'm Anna and

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I'm so glad you could join us. For today's

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episode, we've got a jam packed show for you

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covering some really fascinating developments

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from across the universe and right here on

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Earth too. First up, we'll dive into

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the latest on space missions, including an

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update on the Axiom mission 4 and that

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unexpected anomaly that's caused a bit of a

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setback for SpaceX's Starship program.

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Then we'll turn our attention back in time to

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uncover how ancient life on Earth might have

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survived some truly brutal snowball Earth

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periods. After that, we're zooming out to the

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cosmos to talk about galaxy evolution and

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how scientists are getting closer to

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understanding the very birth of galaxies

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similar to our Milky Way. And speaking of

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searching, we'll explore how the hunt for

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alien life and advanced civilizations is now

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going real time, which is super exciting.

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Finally, we'll tackle one of those enduring

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planetary mysteries. Why giant planets

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often end up in the far reaches of their

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solar systems. It's a bit like a cosmic game

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of pinball, apparently. So stick around, it's

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going to be a really interesting ride.

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Alright, let's kick things off with some news

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from the International Space Station, or ISS.

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The launch of Axiom Mission 4, which was

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originally set for Sunday, June 22, has

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actually been put on hold again. NASA, Axiom

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Space and SpaceX are still reviewing new

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launch opportunities, so we'll have to wait

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and see when it's rescheduled. Now, why the

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delay? Well, NASA needs a little more time,

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it seems, to evaluate the ISS operations

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after some recent repair work on the Zvezda

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service modules aft segment. You see, the

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space station's systems are all really

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interconnected, so they want to make

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absolutely sure everything is totally ready

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for additional crew members. They're taking

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all the necessary time to review the data and

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make sure it's safe. The crew is currently in

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quarantine in Florida, but they're ready to

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go as soon as the station gives the green

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light. Meanwhile, SpaceX's Falcon

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9 rocket and Dragon spacecraft are reportedly

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in great shape, just waiting on the launch

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pad at Launch Complex 39A at NASA's

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Kennedy Space Center. Stay tuned for updates

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on that. It's on.

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Okay, shifting gears a bit to some not so

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great news after. As I reported yesterday,

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SpaceX experienced a pretty significant

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setback at their Massey's test site near

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Starbase Texas on the evening of June 18th.

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They were doing a routine six engine static

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fire test of ship 36 for their starship

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program and unfortunately There was a sudden

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energetic anomaly just after

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11pm Central Daylight Time. While propellant

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was being loaded onto the vehicle, a pair of

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explosions ripped ship 36 apart,

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producing a large fireball and causing

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significant damage to the test facility. This

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ship was actually slated for the 10th Test

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flight of Starship and super heavy, expected

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very soon, which obviously won't be happening

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now. So what happened? Well, according to

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SpaceX CEO Elon Musk, initial

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data points to a failure of a composite

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overwrapped pressure vessel, or COPV,

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in Ship 36's nose cone. These are

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lightweight tanks that hold high pressure

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gases. A rupture acted like a shaped charge,

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tearing the payload wall and header tank

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transfer tubes. This caused the liquid

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methane and oxygen to mix and instantly

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ignite, leading to the first explosion. The

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nose cone collapse. Seconds later, the rest

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of the propellant ignited, causing the

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second. Fires kept burning for several

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hours, indicating damage to the liquid

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methane farm. The good news is fire.

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Thankfully, SpaceX confirmed no personnel

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were injured and everyone was accounted for.

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All media and public members were safe too,

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thanks to preset exclusion zones. This is a

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crucial point, obviously for the Starship

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program, though this is a notable setback.

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It's the first time SpaceX has lost a ship in

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ground testing since May 2020. And

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what's more, they've lost the ability to

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perform testing at Massey's for now, due to

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all that significant damage to their static

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fire test stand and the surrounding

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infrastructure. It means that even ships like

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ship 37, which just started getting engines,

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can't be static fired without repairs. It's

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worth noting that the COPVs on Starship don't

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share commonality with those used on SpaceX's

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Falcon rockets. So this issue is isolated to

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the Starship program. The FAA won't be

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involved in the investigation since it

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happened during ground testing. SpaceX will

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conduct their own. This means we're likely

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looking at some significant changes and

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delays for the Starship program in the coming

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months as they assess repairs and

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potentially inspect other ships in their

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fleet. It's a tough break for sure, but as

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SpaceX has demonstrated in the past, they

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will bounce straight back from looking

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at challenges in space.

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Let's turn our attention back to Earth and a

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fascinating mystery from its deep past. New

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research out of MIT is shedding light on how

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early complex life forms, what we call

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eukaryotes, might have survived those extreme

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periods known as Snowball Earth between

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720 and 635 million years

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ago. Now, imagine our planet completely iced

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over. We're talking average global

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temperatures of minus 50 degrees Celsius.

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Geologists call this the cryogenian period.

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And whether Earth was a hardened snowball or

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more of a softer slushball. And is still

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debated. But one thing's for most of

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it was plunged into a deep freeze. So the big

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question has always been, how and where did

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life actually survive? Previously, ideas

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included patches of open ocean, deep sea,

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hydrothermal vents, or perhaps even under ice

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sheets. But this new study suggests another

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intriguing meltwater ponds on

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the surface of the ice. Fatima Hussain,

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a graduate student at mit, explained their

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interest, saying, we see evidence for

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eukaryotes before and after the cryogenian in

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the fossil record, but we largely lack direct

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evidence of where they may have lived during.

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She added, the great part of this mystery is

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we know life survived. We're just trying to

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understand how and where. To test this

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meltwater pond hypothesis, the researchers

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analyzed samples from modern meltwater ponds

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in Antarctica, specifically on the McMurdo

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Ice Shelf. These ponds, just a few feet deep

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and meters wide, form when trapped sediments

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rise to the surface, absorb sunlight, and

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melt the ice. The bottom of these ponds

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are lined with microbial mats, kind of like

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sticky, layered communities of cells.

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While we know simpler life like cyanobacteria

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can survive in these harsh environments, the

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researchers wanted to know if eukaryotes,

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those more complex organisms with a cell

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nucleus, could also weather such challenging

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circumstances. Using a combination of lipid

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analysis, specifically looking for sterols

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and genetic components called ribosomal rna,

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they found something pretty remarkable. They

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discovered a surprising diversity of

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eukaryotic life, including various types of

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algae, protists, and even microscopic animals

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thriving within these microbial mats.

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Houssain noted that no two ponds were alike,

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but they all hosted diverse eukaryotic

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assemblages from all the major groups. This

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really suggests that meltwater ponds during

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the snowball Earth episodes could have served

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as crucial above ice oases,

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nurturing the eukaryotic life that eventually

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led to the incredible diversification of

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complex life we see today, including us.

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The study was published in the journal Nature

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Communications.

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Okay, from understanding ancient life here on

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Earth, let's turn our gaze even further back

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in time, to the very early universe and the

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birth of galaxies. There's some really

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groundbreaking new research that's helping us

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understand how galaxies, including our own

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Milky Way, first came to be.

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We're talking about a period known as the

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cosmic noon, which spanned from 10 to 12

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billion years ago. During this incredibly

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active time, star formation was happening at

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a rate 10 to 100 times greater than it is

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today. And New research has been looking

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deeply into a particular type of ancient

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galaxy called Lyman Alpha emitters or

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laes. Now, without getting too technical,

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Lyman Alpha or Leia, is a hydrogen line

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emission in the UV spectrum. Basically, when

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young energetic stars form, they emit intense

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UV light that ionizes hydrogen gas around

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them. And when that hydrogen recombines, it

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emits this specific Lya line. So

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detecting it is like a really strong

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indicator of active star formation. LAEs are

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thought to be the direct progenitors of

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galaxies like our Milky Way. They're

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typically low mass and very young, only about

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200 to 600 million years old, and they have

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the highest star formation rates among all

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galaxies. But there's been a bit of, a

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puzzle surrounding them. Were they undergoing

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their very first intense burst of star

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formation or were they older galaxies just

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restarting their star forming engines after a

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quiet period? A new study titled

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Star Formation Histories Reveal Formative

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Starbursts Experienced by lea emitting

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Galaxies at Cosmic Noon. Led by Nicole

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Firestone from Rutgers University, set out to

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answer this. Firestone calls laes the most

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profound beacons of the high redshift

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universe, adding that they're fantastic

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probes of distant galaxy populations because

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they shine so brightly. M the team used

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machine learning to examine the light from 74

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LAEs detected by the 100 DCAM Imaging in

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Narrowband Survey, or ODIN.

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This allowed them to trace the star formation

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history of each galaxy. They identified three

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main those undergoing their first burst,

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those with a dominant burst happening now,

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but some past activity, and those where the

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dominant burst occurred in the past.

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The exciting finding a strong majority,

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67% of the LAEs they studied were indeed

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experiencing their very first major star

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formation burst, with at most only modest

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activity in their past. In fact,

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95% were experiencing what the researchers

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called dominant bursts of star

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formation at the time of observation.

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Firestone emphasized, for the very first

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time, we have been able to definitively show

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that most LAEs are experiencing their first

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major starburst at the time of observation

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and only have very young stars. This

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is a big deal, because if LAEs are truly the

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precursors to galaxies like ours, then this

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research has essentially unlocked a part of

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our own galaxy's origin story. As Eric

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Gowiser, also from Rutgers, put it, now we

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know the answer to that question is yes. When

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asked if we'd looked far enough back to find

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the starting points for galaxies like the

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Milky Way. It really builds on those

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fascinating JWST findings that showed

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surprisingly massive, well, structured

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spiral galaxies in the early universe. I

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mean, it's all part of this incredible story

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of galaxy evolution.

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Alright, let's shift gears a little bit from

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the cosmic past to the future of searching

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for alien civilizations. Imagine

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scanning the night sky for signs of alien

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technology using the very same systems that

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hunt for exploding stars. That's exactly

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what researchers are starting to do now.

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Transforming astronomical alert systems

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originally designed to catch things like

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supernovae into powerful tools for

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detecting potential technosignatures.

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That's the evidence of advanced civilizations

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beyond Earth. Every single night, the

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Zwicky Transient Facility, or ztf,

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generates up to a million alerts as it

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monitors the sky for changing objects.

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These alerts flow through what are called

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alert brokers, which are basically

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sophisticated software systems that process

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and distribute information about anything

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that brightens, dims or suddenly appears

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in the sky. And the upcoming Legacy Survey

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of Space and Time, or lsst,

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is going to increase this volume by an order

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of magnitude, creating just an unprecedented

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flood of astronomical data. While these

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systems were initially built to catch

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explosive events like supernovae and to track

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asteroids, new research by Eleanor Gallet,

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James Davenport and Steve Croft is

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demonstrating their untapped potential for

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seti, the search for Extraterrestrial

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intelligence. Their work shows how we can

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totally repurpose these existing astronomical

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systems to search for those subtle signatures

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that might indicate artificial structures or

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technology around distant stars. The

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inspiration for this approach actually comes

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partly from Boyajian's Star, also known as

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Tabby's Star. This star, officially KIC

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846-2852, really puzzled

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astronomers with its mysterious dimming

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patterns a few years back. And while natural

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explanations like dust clouds ultimately

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proved most likely in that case, the study of

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Boyajian's star highlighted how unusual

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stellar behavior could potentially indicate

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artificial megastructures like a Dyson

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sphere, which is a hypothetical construct an

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advanced civilization might build around its

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star. So this new research takes that

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concept even further, creating automated

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systems to identify what they call stellar

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dippers. These are stars that suddenly and

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dramatically dim without any obvious natural

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causes like a classical stellar variability

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or other astrophysical phenomena. The

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challenge of course, is immense. How do you

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filter millions of nightly alerts? To find

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the handful that might represent something

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truly anomalous, the researchers

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developed a two stage approach. First,

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they use the alert broker's built in

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filtering capabilities to narrow down

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candidates. Then they apply additional

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analysis using historical data to identify

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stars showing unprecedented dimming behavior.

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They're even deploying clever optical SETI

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techniques like looking for planetary transit

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zone geometries. And using something called

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the Ceti ellipsoid The SETI ellipsoid

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is this particularly neat concept that

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identifies the zone in space where

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hypothetical alien observers would have seen

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Earth transit across our sun, potentially

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prompting them to send signals in our

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direction. Now the researchers are

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honest about the current limitations. The

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SETI methods that these alert brokers can

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execute are still somewhat limited, but

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they're providing suggestions to enhance

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future technosignature and anomaly searches.

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Especially in the era of the Vera C Rubin

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Observatory. The existing systems weren't

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designed with SETI in mind, so some

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modifications and new approaches will

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definitely be needed to fully realize their

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potential. However, the foundation is

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really solid. Alert brokers already have

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sophisticated tools for identifying unusual

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astronomical events. The LaserRE alert

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broker, for instance, offers a watchmap

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feature that can monitor specific regions of

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the sky for anomalous signals. And as the

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Vera C Rubin Observatory comes online with

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lsst, the volume of astronomical

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alerts is just going to increase

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dramatically, which creates both huge

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00:14:52.409 --> 00:14:54.050
opportunities and challenges for

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00:14:54.050 --> 00:14:56.850
technosignature research. More data means

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better chances of catching rare anomalous

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events. But it also means developing even

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00:15:01.570 --> 00:15:03.690
more sophisticated filtering techniques so we

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00:15:03.690 --> 00:15:06.550
don't get completely overwhelmed. This work

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00:15:06.550 --> 00:15:08.670
represents a really sensible approach to SETI

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because it uses existing infrastructure

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rather than requiring dedicated alien hunting

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telescopes. By utilizing systems

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that are already scanning the entire visible

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sky every few nights, we're essentially

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getting a free ride on one of the most

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comprehensive surveillance networks ever

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pointed at the sky. And

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while we shouldn't expect to find alien

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megastructures next week, this research is

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definitely establishing the groundwork for a

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00:15:34.440 --> 00:15:37.200
new generation of SETI that could operate

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00:15:37.200 --> 00:15:40.160
continuously, scanning millions of stars

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for those signs that we are not alone in the

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universe.

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Okay, so we've talked about searching for

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life, but, what about the formation of

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planets themselves? Let's turn our attention

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to one of the really big mysteries in

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00:15:52.670 --> 00:15:55.590
planetary why are enormous and

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mysterious worlds sometimes found silently

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looping around their stars far beyond the

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00:16:01.310 --> 00:16:04.310
orbit of known planets? Like some drift

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00:16:04.310 --> 00:16:07.030
as far as 10,000 times the distance

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00:16:07.030 --> 00:16:09.670
between Earth and the Sun? For decades,

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astronomers really struggled to explain how

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00:16:11.750 --> 00:16:14.110
these lonely giants ended up so far from the

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00:16:14.110 --> 00:16:16.910
warm center of their systems. But thanks to

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00:16:16.910 --> 00:16:19.310
new research out of Rice University, the

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00:16:19.310 --> 00:16:21.190
mystery might finally have a solution.

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00:16:22.150 --> 00:16:24.630
A new study published in Nature Astronomy

395
00:16:25.260 --> 00:16:27.420
reveals that these distant worlds aren't just

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00:16:27.420 --> 00:16:30.020
cosmic flukes. They're actually the natural

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00:16:30.020 --> 00:16:32.340
results of wild early life behavior in

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00:16:32.340 --> 00:16:35.100
planetary systems. During this chaotic

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00:16:35.100 --> 00:16:38.020
stage, young planets collide. They bounce,

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00:16:38.020 --> 00:16:40.779
and they scatter, almost like balls on a

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00:16:40.779 --> 00:16:43.380
pinball machine. And sometimes, if the

402
00:16:43.380 --> 00:16:45.580
conditions are just right, one of these

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00:16:45.580 --> 00:16:47.700
planets Gets pushed to the outer limits of

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00:16:47.700 --> 00:16:50.220
the system. And believe it or not, it just

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00:16:50.220 --> 00:16:53.110
stays there. As Andre Isidoro,

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00:16:53.110 --> 00:16:54.990
A lead author and assistant professor at

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00:16:54.990 --> 00:16:57.430
Rice, put it, essentially, we're watching

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00:16:57.430 --> 00:17:00.270
pinballs In a cosmic arcade. He explained

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00:17:00.270 --> 00:17:02.350
that when giant planets Scatter each other

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00:17:02.350 --> 00:17:04.910
through gravitational interactions, Some are

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00:17:04.910 --> 00:17:07.390
flung really far away. But if the timing and

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00:17:07.390 --> 00:17:09.030
the surrounding environment Are just right,

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00:17:09.350 --> 00:17:11.510
those planets don't get ejected completely.

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00:17:11.750 --> 00:17:14.110
Instead, they get trapped in these extremely

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00:17:14.110 --> 00:17:16.910
wide orbits. This happens while

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00:17:16.910 --> 00:17:18.510
stars are still part of crowded birth

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00:17:18.510 --> 00:17:20.630
clusters, which contain hundreds or even

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00:17:20.630 --> 00:17:23.370
thousands of stars. The Rice team,

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00:17:23.370 --> 00:17:26.090
along with collaborators, Ran thousands of

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00:17:26.090 --> 00:17:28.330
computer simulations of early planetary

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systems Living in these dense clusters.

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00:17:31.170 --> 00:17:33.050
Many of these virtual universes Showed

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00:17:33.050 --> 00:17:35.130
planets being kicked into orbits between one

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00:17:35.130 --> 00:17:37.450
hundred and ten thousand astronomical units

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00:17:37.450 --> 00:17:40.330
from their stars. That's up to 250

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00:17:40.330 --> 00:17:43.090
times farther than Neptune. Now. Usually

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00:17:43.170 --> 00:17:45.130
when planets are pushed that far, they don't

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00:17:45.130 --> 00:17:47.690
survive. They just get ejected into deep

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00:17:47.690 --> 00:17:50.320
space and become rogue planets Wandering the

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00:17:50.320 --> 00:17:52.920
galaxy alone. But in these simulations,

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00:17:53.160 --> 00:17:54.520
Some actually survived.

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00:17:55.640 --> 00:17:57.800
Gravitational nudges from neighboring stars

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00:17:57.800 --> 00:18:00.200
in the cluster Helped stabilize these extreme

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00:18:00.200 --> 00:18:03.040
orbits. As Nathan Kaib, A co author

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00:18:03.040 --> 00:18:05.000
of the study, explained, when these

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00:18:05.000 --> 00:18:07.240
gravitational kicks happen at just the right

437
00:18:07.240 --> 00:18:10.040
moment, A planet's orbit becomes decoupled

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00:18:10.040 --> 00:18:12.760
from the inner planetary system. This creates

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00:18:12.760 --> 00:18:15.040
a wide orbit planet that's essentially frozen

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00:18:15.040 --> 00:18:17.000
in place after the cluster disperses.

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00:18:18.160 --> 00:18:20.880
And get this. These findings Might shed new

442
00:18:20.880 --> 00:18:23.000
light on one of our own solar system's Most

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00:18:23.000 --> 00:18:25.520
intriguing mysteries, Planet Nine.

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00:18:26.080 --> 00:18:28.920
This theorized world, if it exists, could

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00:18:28.920 --> 00:18:31.520
be between five and ten times Earth's mass

446
00:18:31.680 --> 00:18:34.560
and orbits somewhere between 250 and

447
00:18:34.560 --> 00:18:37.040
a thousand astronomical units from the sun.

448
00:18:37.440 --> 00:18:40.040
It hasn't been observed directly, but several

449
00:18:40.040 --> 00:18:42.560
icy bodies Beyond Neptune have these strange

450
00:18:42.640 --> 00:18:45.040
clustered orbits. That suggests they're being

451
00:18:45.040 --> 00:18:47.960
pulled by something big and unseen. Planet

452
00:18:47.960 --> 00:18:50.280
nine could be that something. According to

453
00:18:50.280 --> 00:18:52.440
the study, if the early solar system

454
00:18:52.440 --> 00:18:54.920
Experienced two specific instability phases,

455
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One during the growth of Uranus and Neptune,

456
00:18:57.800 --> 00:18:59.919
and another during the later scattering among

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00:18:59.919 --> 00:19:02.880
gas giants, there's up to a 40% chance

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00:19:02.880 --> 00:19:05.080
that Planet Nine was actually trapped in its

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00:19:05.080 --> 00:19:08.000
current location. Isidoro said. Our

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00:19:08.000 --> 00:19:10.120
simulations show that these kinds of orbits

461
00:19:10.120 --> 00:19:12.930
Are entirely possible. The solar system

462
00:19:12.930 --> 00:19:15.370
might not be unique, but it could be One of

463
00:19:15.370 --> 00:19:17.250
the more efficient ones when it comes to

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00:19:17.250 --> 00:19:20.130
trapping these wide orbit planets. The

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00:19:20.130 --> 00:19:22.050
study also provides A bit of a roadmap for

466
00:19:22.050 --> 00:19:24.930
future exoplanet hunters. Wide orbit planets

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00:19:24.930 --> 00:19:27.010
Are super hard to detect because they're so

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00:19:27.010 --> 00:19:29.730
far away and dim, but the research suggests

469
00:19:29.730 --> 00:19:31.970
they're more likely to appear around metal

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00:19:31.970 --> 00:19:34.250
rich stars that already have gas giants.

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These stars could become prime targets for

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00:19:36.690 --> 00:19:39.150
deep imaging surveys, and instruments like

473
00:19:39.150 --> 00:19:41.510
the upcoming Vera C Rubin Observatory will be

474
00:19:41.510 --> 00:19:44.270
absolutely essential. This telescope is

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00:19:44.270 --> 00:19:46.670
expected to help either find Planet nine or

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00:19:46.670 --> 00:19:49.190
disprove its existence by scanning the sky in

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00:19:49.190 --> 00:19:51.750
unprecedented detail. It's really

478
00:19:51.750 --> 00:19:53.990
fascinating to think that the chaos of early

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00:19:54.149 --> 00:19:56.470
planetary systems, combined with the

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00:19:56.470 --> 00:19:58.950
gravitational influence of a crowded stellar

481
00:19:58.950 --> 00:20:01.230
neighborhood, could be responsible for these

482
00:20:01.230 --> 00:20:03.950
distant, stable worlds. It really

483
00:20:03.950 --> 00:20:06.510
adds another piece to the complex puzzle of

484
00:20:06.510 --> 00:20:08.710
how planetary systems, including our own,

485
00:20:08.710 --> 00:20:09.110
came.

486
00:20:11.490 --> 00:20:13.570
And that wraps up another exciting episode of

487
00:20:13.570 --> 00:20:16.330
Astronomy Daily. It's always amazing to

488
00:20:16.330 --> 00:20:18.050
delve into the latest breakthroughs and

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00:20:18.050 --> 00:20:20.370
mysteries of the cosmos, isn't it? From

490
00:20:20.370 --> 00:20:22.250
delayed space missions and unexpected

491
00:20:22.250 --> 00:20:24.610
incidents to the ancient secrets of life on

492
00:20:24.610 --> 00:20:26.690
Earth and even the search for alien

493
00:20:26.690 --> 00:20:28.890
civilizations, there's just so much to

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00:20:28.890 --> 00:20:31.770
explore. Thank you so much for joining me

495
00:20:31.770 --> 00:20:33.730
on this journey through the universe's latest

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00:20:33.730 --> 00:20:36.010
happenings. If you want to catch up on all

497
00:20:36.010 --> 00:20:38.200
the latest space and astronomy news with our

498
00:20:38.200 --> 00:20:40.640
constantly updating news feed, or if you want

499
00:20:40.640 --> 00:20:42.400
to listen to all our back episodes, be sure

500
00:20:42.400 --> 00:20:45.080
to visit our website@astronomydaily.IO

501
00:20:45.320 --> 00:20:48.040
that's a S T R O N o M M y

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00:20:48.040 --> 00:20:50.880
D A I L y IO and

503
00:20:50.880 --> 00:20:52.600
hey, don't forget to subscribe to Astronomy

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00:20:52.600 --> 00:20:55.360
Daily on Apple podcasts, Spotify and

505
00:20:55.360 --> 00:20:57.160
YouTubeMusic, or wherever you get your

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00:20:57.160 --> 00:20:59.480
podcasts. We'll be back tomorrow with more

507
00:20:59.480 --> 00:21:01.920
news from beyond our world. Until then, this

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00:21:01.920 --> 00:21:04.140
is Anna signing off and reminding you to keep

509
00:21:04.140 --> 00:21:04.700
looking up.
