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Speaker 1: What happens when an interstellar visitor, I mean, an object

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that started its life around a completely different star is

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about to get blasted by a massive, high energy eruption

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from our Sun.

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Speaker 2: It sounds like something out of science fiction, doesn't it

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an impossible cosmic alignment, But that is the precise high

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stake scenario unfolding in real time right now with interstellar

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Object three I.

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Speaker 1: At least absolutely, and that's exactly why we're here. Welcome

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to the deep dive today. We are undertaking well a

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really critical analysis of the latest data surrounding three I outlaws.

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This is a celestial tourist that it just continues to

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redefine our understanding of commentary and interstellar physics.

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Speaker 2: And we have two huge immediate updates that just demand

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our attention. First, NASA is finally breaking its silence with

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some definitive critical imagery, and at.

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Speaker 1: The same time, a new powerful coronal mass ejection a

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CME is already hurtling straight toward the object.

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Speaker 2: Our mission today is surgical. We need to unpack the

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complex science behind this object really mysterious and very active behavior.

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Speaker 1: Right We're going to delve deep into the baffling controversy

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over its true size, which is an uncertainty that throws

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off nearly every calculation we try to make.

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Speaker 2: And most importantly, we're going to explain why you absolutely

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have to understand some cutting edge plasma physics to make

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any sense of this visitor from outside our Solar system.

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Speaker 1: This object is forcing us to rewrite the rules. I mean,

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it's exhibiting features, a clear tail, distinct stable jets, a

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massive diffuse coma, all things you'd expect from a regular

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Solar system commet.

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Speaker 2: But it's not. It remains an interstellar anomaly. It could

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be an icy planetesimal, or maybe even a fragment that

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was ripped from an exoplanet.

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Speaker 1: So we're cutting through all the speculation and noise right

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now to bring you the essential thrilling details you need

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to be well informed and frankly ready for the incoming

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data tsunami.

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Speaker 2: Let's start with the release that the astronomical community has

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just been waiting for because the lack of certainty up

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to this point has created a real data vacuum.

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Speaker 1: Okay, let's unpack this. This is monumental news. For weeks,

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observation details on three iet lists were just incredibly sparse.

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It was hampered by its position relative to the Sun.

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Speaker 2: Right, it was in a really tough spot to observe

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from Earth.

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Speaker 1: But now NASA has officially broken its silence. So what's

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the definitive date and time for this critical data reveal.

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Speaker 2: The official release is scheduled via a livestream. It's set

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for Wednesday, November nineteenth at twelve pm Pacific time. And

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the expectation is, well, it's high. It's really high, because

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this isn't just a general image release. It's specifically targeted

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data that we've all been hoping for.

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Speaker 1: And the payload itself, the data, is the most crucial

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part of this announcement. The release promises to include high

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resolution imagery. Specifically, they're calling it high rise imagery. Why

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is that specific designation so vital to solving the mysteries

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of three iet lists?

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Speaker 2: Well, high rise is short for high resolution imaging science experiment.

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Like this is not your stand space camera. So the

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highest resolution camera ever sent to orbit another.

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Speaker 1: Planet, another planet, So it wasn't even designed for this.

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Speaker 2: No, not at all. It's on the Mars Reconnaissance Orbiter

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or MRO. The MRO is this phenomenal, incredibly stable platform

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and high rise imagery has a very specific function. It

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can resolve details down to about twenty five centimeters per

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pixel on the Martian's surface.

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Speaker 1: Wow, twenty five centimeters from Orgon exactly.

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Speaker 2: Now, obviously three at lace is much much farther away,

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but the quality of the optics means that if any

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instrument we have out there could resolve the tiny, obscured

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nucleus of this thing, it's mro's high rise camera.

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Speaker 1: So we're talking about an instrument designed to capture incredibly

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fine detail, even though, like you said, it wasn't originally

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intended for fast moving interstellar.

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Speaker 2: Objects precisely, and the timing of when they got this

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data is also key. It was captured on October third,

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during what astronomers were calling a period of reduced visibility

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or you know, an observation.

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Speaker 1: Shutdown, right, That's when we couldn't see it from Earth

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at all.

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Speaker 2: We couldn't. It was near what's called superior conjunction, meaning

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it was almost directly behind the Sun from our perspective.

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Terrestrial observation was just impossible because of the solar glare

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and all the background noise.

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Speaker 1: So we had to rely on assets in deep space entirely.

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Speaker 2: We were relying on things like MRO, which was strategically

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positioned relative to Mars to obtain this data when nobody

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else could.

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Speaker 1: It speaks volumes. Doesn't it that NASA devoted such a

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high value asset a Mars orbiter to capturing this image

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even when visibility was at its worst from Earth. They

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clearly knew this was the only chance to get a

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crucial glimpse of the object's core.

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Speaker 2: It was a calculated risk, absolutely, but it was a

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necessary one. Terrestrial observers were fighting the Sun, which makes

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the data just unusable. MRO, being millions of miles away,

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offered this unique vantage point away from the immediate glare

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and all the atmospheric distortions that played Earth based imaging.

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Speaker 1: Now, setting side the science for just a moment, there's

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a cultural element to this timing that I find fascinating.

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Our source noted that the date November nineteenth, it coincides

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with what's called a critical planetary geometry, and while this

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doesn't affect the data itself obviously, the source mentioned that

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this geometry is sometimes associated with communication breakdowns and paradigm

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shattering moments. As it relates to communications, it's.

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Speaker 2: An interesting narrative frame, isn't it. I mean, whether or

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not one adheres to those kinds of cultural observations, the

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fact remains that this piece of data is scientifically poised

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to shatter paradigms.

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Speaker 1: It really is.

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Speaker 2: For years we've struggled with these conflicting measurements about three iyeatlysts.

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If this high rise data finally resolves the nuclear size,

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it will irrevocably change the scientific conversation around this object.

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It is quite literally an information paradigm shift in astronomical communications.

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Speaker 1: And speaking of communication, there's a subtle but really important

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linguistic shift happening. While the original discoverers and many astronomers

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they formally refer to it as interstellar object three I out.

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Speaker 2: Lists, which is the correct neutral term.

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Speaker 1: Right, but NASA in their press releases about this image,

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they're explicitly calling it an interstellar comet.

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Speaker 2: And that terminology shift from object to commet is significant.

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It's not an accident. It implies that NASA's internal analysis

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of the object's behavior, you know, the strength of its outgassing,

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the development of its tail and coma, is leaning heavily

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toward the conventional cometary classification.

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Speaker 1: Even though it's from another star system.

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Speaker 2: Even though it has a non Solar system origin, it's

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behaving at least outwardly in a very conventional cometary way

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in terms of its activity.

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Speaker 1: Hold on, if it's acting like a comet, why is

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it still fundamentally different from a comet that formed in, say,

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the ort cloud of our own solar system. Why does

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it retain that special interstellar status.

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Speaker 2: The difference really lies in its composition and its trajectory.

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Primarily the trajectory we know it came from outside our

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system because its hyperbolic orbit confirms it has enough velocity

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to escape the Sun's gravitational pull. It's not bound to

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our Sun.

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Speaker 1: It's just passing through.

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Speaker 2: It's just passing through. It didn't originate here. And while

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it exhibits activity, the jets the coma that looks very

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similar to a solar system commet, its internal composition, its

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volatile materials could be fundamentally different. How so well it

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may harbor ices, say nitrogen or carbon monoxide, ices that

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formed in a much colder or just different stellar environment,

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and that dictates how it out gases, when it out gases,

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and how it creates that plasma environment we're going to talk.

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Speaker 1: About, right and You have to contrast this with the

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other interstellar visitors we've had. Umua was rocky, it didn't outgas,

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it was shaped like a cigar. It was anything but

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a comma, completely different beast and two Iborisov. While it

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was clearly a comet, it was exceptionally dark and pristine.

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Three Idolys is in this fascinating middle ground. It's highly active,

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but it's still alien.

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Speaker 2: It is three eyedalysis is forcing us to expand the

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very definition of a comet to include these highly active bodies,

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regardless of their star of origin. The data they're releasing

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should help solidify whether its composition is chemically close to

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our comments or if it holds something unique that only

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physics from a different star system could produce.

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Speaker 1: And just as a final note for listeners who want

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to get directly involved, NASA plans to take questions from

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the public during the broadcast, So if you're quick, you

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can ask your own burning questions using the hashtag hashtag

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ask NASA on social media.

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Speaker 2: Okay, so now we shift from a data release, which

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remember deals with historical observations from back on October third,

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to something immediate and frankly spectacular, an imminent, real time

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cosmic interaction.

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Speaker 1: This is truly breaking news. A powerful new coronal mass ejection,

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a huge blast of solar plasma and magnetic energy. It

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blasted off today and it came from the very same

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active sunspot group that has been causing all the geomagnetic

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storming here on Earth. This is a huge wave of

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energy moving.

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Speaker 2: Across space, and this wave is not missing its target.

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That's the key. Stays with models are showing a direct

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shot toward three I at lists. The impact is predicted

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to occur around November twenty second at twelve Universal time.

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Speaker 1: The twenty second I mean, the timing is just astonishing.

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It's just three days after NASA's Big Data reveal.

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Speaker 2: It's almost too dramatic. It's like we get the scientific

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blueprint for the object and then the universe decides to

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immediately test it in a cosmic crucible.

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Speaker 1: So how certain are we about this trajectory.

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Speaker 2: The confirmation is key here and it's pretty solid. We

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were able to look at the chronograph imagery. Those are

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the instruments that block out the Sun's discs so we

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can see the corona, and it showed the ejection launching

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off the side of the Sun. It came from a

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sunspot group that was just around the limb, so slightly out.

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Speaker 1: Of our direct view, and that's how we know it's

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not coming for us.

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Speaker 2: Critically, Yes, those observations immediately confirmed it was not Earth's

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direct so Earth is safe from a major geomagnetic storm

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from this particular event.

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Speaker 1: But three ia plus is precisely in the.

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Speaker 2: Firing line exactly. The confidence level for a direct hit

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is high because of the angle of launch. CME observed

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launching slightly above the ecliptic plane, which is the plane

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the planet's orbit in, and that angle precisely matches the

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current inclination and position of three ilis. It's an extremely

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well aligned shot.

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Speaker 1: This raise is a really fascinating physics question. I mean,

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what does a hit like this even mean for an

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object that is already outgassing so rapidly and is surrounded

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by this vast cloud of plasma. This isn't a physical collision, right,

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It's an electromagnetic and energetic shock wave, right.

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Speaker 2: And this is where we learn the most. For the

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object itself, the solid nucleus, it's actually somewhat protected by

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its massive coma, But the coma and the tail, which

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are pure highly charged plasma, they will experience a violent interaction.

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And to understand the potential magnitude of this, we can

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look to the Rosetta precedent.

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Speaker 1: Okay, tell us more about that, the Rosetta emissions observations

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of Comet sixty seven P.

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Speaker 2: The Rosetta spacecraft which tracked Comet sixty seven P was

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in the perfect position to observe the effects of a

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powerful CME up close. For ordinary Solar system commets, a

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strong CME can do a couple of things. It can

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break off the plasma tail that's called a tail disconnection event,

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or can fundamentally reorganize the magnetic environment around the nucleus.

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Speaker 1: And what did Rosetta's instruments actually measure during that CME impact?

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What were the numbers?

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Speaker 2: The effect was dramatic. The impact caused the surrounding magnetic

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field strength is the field that's induced around the comet

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by the flowing plasma to surge. It went from a

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baseline of about thirty to fifty nanotesla.

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Speaker 1: Okay, which is a pretty low magnetic field.

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Speaker 2: Pretty low, yes, Yeah, it's surged up to an astounding

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three hundred nanotesla.

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Speaker 1: Three hundred That is a massive what is that? A

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tenfold increase in the local magnetic field strength?

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Speaker 2: Almost yeah, a huge jump. A tenfold increase is a

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great way to think about it. That tells you immediately

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that the environment changes from relatively calm space to a

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highly stressed, compressed, and violently charged bubble.

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Speaker 1: So what's happening there? Why does the field jump so much?

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Speaker 2: It happens because the CME is essentially a supersonic wave

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of high density magnetized plasma. When that wave hits the

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comets slower moving, denser cloud of ionized gas and dust,

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the COMA, it compresses the comet's own magnetic field structure.

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It's a boundary we call the comma pause, and that

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compression drastically increases its strength and changes the dynamics of

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the plasma flow almost instantly.

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Speaker 1: So if three to eight less experiences a similar compression,

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what are astronomers going to be watching for? What's the

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visual evidence that this event occurred and gave us new data?

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Speaker 2: The primary observation, the thing everyone will be looking for

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is that tail disconnection.

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Speaker 1: Event, the tail literally breaking off visually.

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Speaker 2: Yes, if the magnetic pressure from the CME is strong enough,

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it can literally sever the magnetic field lines that connect

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the ion tail to the head of the coma, And

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when you look at it, the tail appears to just

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float away and a new and immediately begins to form

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in its place.

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Speaker 1: That would be a breath taking visual confirmation. But what

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does that tell us scientifically? What's the takeaway?

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Speaker 2: It gives us real time evidence of two things. First,

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the density and speed of the CME, which we can track.

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But second, and much more importantly, it tells us about

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the resilience and structure of three I at leas's own

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plasma environment. How so, well, if it's tail snaps off easily,

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it tells us something about the magnetization of the material

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it's shedding. If it resists the pressure, or if the

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magnetic field surge is even greater than three hunderd nanotesla,

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it would suggest the material that's shedding is more conductive

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or maybe denser than a typical solar system.

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Speaker 1: Comments Ah, so it could hint at unique compositional differences

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that are rooted in its interstellar origin.

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Speaker 2: Exactly. So, the CME hit isn't just a spectacle. It's

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a controlled cosmic stress test happening right before our eyes,

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and it's allowing us to compare this interstellar object to

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our familiar Solar System commets like sixty seven p Okay.

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Speaker 1: So while we wait for that CME impact, we need

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to talk about the current state of three Aatles because

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after moving past perihelion, its closest approach to the Sun,

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and as its viewing position improves, the object is concerned

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to be, as our source put it, very much awake

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and alive.

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Speaker 2: It's putting on quite a show.

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Speaker 1: It really is one of the key features a strong

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are observing.

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Speaker 2: Right now. We see a very clear discernible tail. We

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see distinct, highly focused jets of material, and of course

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that vast diffuse coma enveloping the nucleus. This activity confirms

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that even weeks past its peak solar heating, the object

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is still shedding volatile materials at a very high rate.

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Speaker 1: Let's just emphasize the scale here, because this is where

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three ilis just transcends what you think of as a

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regular commet. We have a nucleus that is likely tiny,

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yet it produces this absurdly large cloud.

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Speaker 2: Of material that is the crucial point of disproportion. We

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have estimates that at one point the comma the enveloping

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00:14:37,279 --> 00:14:40,480
cloud of gas, dust and plasma was about seven hundred

297
00:14:40,519 --> 00:14:41,919
thousand kilometers across.

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Speaker 1: Seven hundred thousand kilometers. Let's just put that in perspective

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for everyone listening. The diameter of the Sun is about

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00:14:47,039 --> 00:14:50,720
one point four million kilometers. So this interstellar traveler, whose

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core is probably only a few kilometers wide, is generating

302
00:14:54,039 --> 00:14:56,519
an atmospheric bubble that is roughly half the diameter of

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00:14:56,519 --> 00:14:57,279
the Sun itself.

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00:14:57,559 --> 00:15:01,039
Speaker 2: It's immense, it is a vast region of influence, and

305
00:15:01,120 --> 00:15:04,159
its size just demonstrates the high rate of outgassing and

306
00:15:04,240 --> 00:15:07,440
the low density of the material being ejected. The coma

307
00:15:07,480 --> 00:15:10,320
typically grows as the object nears the Sun, and while

308
00:15:10,360 --> 00:15:12,639
it may have shrunk a little since its closest approach,

309
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it remains gargantuan relative to its tiny core.

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Speaker 1: And we also have some data on its rotation, which

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seems to complicate the picture even further.

312
00:15:21,120 --> 00:15:25,679
Speaker 2: Indeed, the rotation period has been calculated at approximately sixteen

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00:15:25,799 --> 00:15:29,720
point sixteen hours with very minimal variants. This suggests a

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relatively slow, maybe slightly irregular tumbling motion.

315
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Speaker 1: Okay, so here's where the physics puzzle deepens and it

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00:15:35,799 --> 00:15:38,039
really sets up the need for the plasma solution. We'll

317
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discuss next. How does that slow sixteen hour rotation square

318
00:15:42,440 --> 00:15:45,200
with the highly stable jets we are persistently observing.

319
00:15:45,320 --> 00:15:47,759
Speaker 2: This is the central anomaly, This is the big mystery.

320
00:15:48,120 --> 00:15:52,320
We observe specific persistent channels of material flow, including a

321
00:15:52,399 --> 00:15:55,600
sunward facing jet sometimes called an anti tail, and several

322
00:15:55,639 --> 00:15:59,000
other lateral jets that remain highly focused. They're like laser beams.

323
00:15:59,039 --> 00:16:01,200
Speaker 1: But if the nucleus is re rotating, right.

324
00:16:01,240 --> 00:16:04,240
Speaker 2: If the nucleus is rotating every sixteen hours and the

325
00:16:04,279 --> 00:16:08,000
only force governing the material is thermal outgassing and simple inertia,

326
00:16:08,720 --> 00:16:11,639
those jets should not hold their shape. They should smear out.

327
00:16:11,840 --> 00:16:13,519
Speaker 1: Why not? I mean, if I spray a can of

328
00:16:13,559 --> 00:16:16,399
paint from a rotating object, the spray spreads out, but

329
00:16:16,440 --> 00:16:19,000
the material is still leaving the object in a directed path.

330
00:16:19,039 --> 00:16:21,200
Speaker 2: Isn't it in a vacuum? Yes, But in the case

331
00:16:21,200 --> 00:16:24,279
of a comet, you have volatile ices turning directly into gas,

332
00:16:24,559 --> 00:16:27,759
and that gas immediately carries dust particles with it. As

333
00:16:27,799 --> 00:16:31,000
the nucleus rotates, that source point on the surface moves

334
00:16:31,440 --> 00:16:34,480
over sixteen hours, the rotation should smear the jet material

335
00:16:34,759 --> 00:16:38,480
across the entire spherical coma, it should turn those specific

336
00:16:38,600 --> 00:16:42,159
channels into a generalized homogeneous cloud a fog.

337
00:16:42,440 --> 00:16:45,679
Speaker 1: So the fact that astronomers can identify stable, persistent jets

338
00:16:45,840 --> 00:16:48,519
is essentially proof that a simple mechanical model based on

339
00:16:48,639 --> 00:16:51,879
rotation and inertia is failing. It's not enough, it.

340
00:16:51,840 --> 00:16:55,519
Speaker 2: Is definitive evidence. It proves that something external to the

341
00:16:55,600 --> 00:17:00,799
nucleus's rotation, something much larger and more influential, is organizing

342
00:17:00,840 --> 00:17:04,240
and channeling the flow of the ejected material after it

343
00:17:04,319 --> 00:17:08,119
leaves the surface. And that something else cannot be gravity

344
00:17:08,240 --> 00:17:12,279
or simple thermal pressure. It has to be the electromagnetic environment.

345
00:17:12,000 --> 00:17:14,480
Speaker 1: Which is just a huge clue. But the anomaly of

346
00:17:14,519 --> 00:17:17,799
these stable jets is compounded by what is frankly the

347
00:17:17,920 --> 00:17:21,880
fundamental embarrassing truth of this entire observation. We still do

348
00:17:22,000 --> 00:17:25,240
not know the definitive size of three EE out losses nucleus. No,

349
00:17:25,319 --> 00:17:28,279
we don't, and this colossal uncertainty is why that NASA

350
00:17:28,359 --> 00:17:30,400
High rise data is so eagerly awaited.

351
00:17:30,680 --> 00:17:33,279
Speaker 2: This lack of certainty is the most critical scientific kurdle

352
00:17:33,319 --> 00:17:37,039
we face. Without an accurate size and mass estimate, all

353
00:17:37,079 --> 00:17:39,960
the subsequent calculations about its behavior are based on massive

354
00:17:39,960 --> 00:17:44,240
assumptions as the source material. Dryly noted, scientists are simply

355
00:17:44,559 --> 00:17:46,839
fiddling around with some of the values to make the

356
00:17:46,920 --> 00:17:47,480
numbers work.

357
00:17:47,519 --> 00:17:50,920
Speaker 1: Why does the size matter so fundamentally to everything else.

358
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Speaker 2: Because size, combined with density, determines mass. If we don't

359
00:17:54,880 --> 00:17:57,359
know the mass, we can't calculate the most important factor.

360
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It's mass loss.

361
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Speaker 1: Rate, how quickly it's dissolving exactly.

362
00:18:01,519 --> 00:18:04,559
Speaker 2: How quickly it's falling apart. Furthermore, we need the size

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00:18:04,599 --> 00:18:07,640
to accurately measure its non gravitational acceleration.

364
00:18:07,799 --> 00:18:10,759
Speaker 1: Okay, explain non gravitational acceleration.

365
00:18:10,839 --> 00:18:13,720
Speaker 2: For us, that's the slight deviation in its orbit that's

366
00:18:13,759 --> 00:18:16,599
caused by the momentum carried by the material in the jets.

367
00:18:17,359 --> 00:18:20,480
When gas and dust blast off the nucleus, it provides

368
00:18:20,519 --> 00:18:24,319
a tiny, continuous thrust, like a very very low power

369
00:18:24,400 --> 00:18:27,920
rocket engine, a little push. If the nucleus is large

370
00:18:27,960 --> 00:18:31,400
and massive, that thrust is negligible. But if the nucleus

371
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is tiny, that thrust can significantly alter its path, which

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00:18:34,799 --> 00:18:38,119
is critical for predicting its future trajectory and understanding its past.

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00:18:38,279 --> 00:18:44,240
Speaker 1: But the calculation of size requires another crucial, often overlooked variable, albedo.

374
00:18:44,599 --> 00:18:46,519
We need to be clear about what that term means.

375
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Speaker 2: Albedo is simply the measure of how reflective a surface is.

376
00:18:50,279 --> 00:18:52,799
It's a percentage. Think of wearing a black shirt versus

377
00:18:52,839 --> 00:18:55,400
a white shirt on a sunny day. A high albedo

378
00:18:55,480 --> 00:18:58,559
means the object is more reflective, it's whiter like fresh snow,

379
00:18:58,799 --> 00:19:02,079
and it absorbs less heat. A low albedo means it's dark,

380
00:19:02,160 --> 00:19:05,000
like soot or charcoal, and it absorbs a lot of heat.

381
00:19:05,160 --> 00:19:09,160
Speaker 1: And why is this so central to the size controversy.

382
00:19:08,799 --> 00:19:12,160
Speaker 2: Because when we observe a tiny faint dot surrounded by

383
00:19:12,160 --> 00:19:16,039
this massive bright coma, astronomers have to estimate the nucleus

384
00:19:16,079 --> 00:19:19,759
size by measuring how much light is reflecting off of it. Okay,

385
00:19:19,920 --> 00:19:22,559
so if we assume the nucleus is highly reflective a

386
00:19:22,640 --> 00:19:26,680
high albedo, we only need a small nucleus to account

387
00:19:26,720 --> 00:19:29,599
for the observed light. But if we assume the nucleus

388
00:19:29,640 --> 00:19:33,599
is incredibly dark a low albedo, we would need a

389
00:19:33,680 --> 00:19:37,079
much much larger nucleus to reflect that same amount of light. Ah.

390
00:19:37,200 --> 00:19:40,960
Speaker 1: So the uncertainty in albedo leads directly to this massive

391
00:19:41,000 --> 00:19:44,000
conflict in the size estimates. You're just guessing at how

392
00:19:44,039 --> 00:19:45,319
bright the surface.

393
00:19:44,960 --> 00:19:48,839
Speaker 2: Is precisely, and the conflicting measurements are drastically different, which

394
00:19:48,880 --> 00:19:52,440
really demonstrates the scale of this albedo uncertainty. The initial

395
00:19:52,480 --> 00:19:55,119
Hubble estimate from back in July suggested the nucleus was

396
00:19:55,200 --> 00:19:58,319
up to maybe two point eight kilometers in diameter. That

397
00:19:58,440 --> 00:20:00,880
estimate likely assumed a relative high albedo.

398
00:20:01,079 --> 00:20:03,000
Speaker 1: But what about the other end of the scale, The

399
00:20:03,119 --> 00:20:04,880
really big estimates well.

400
00:20:04,759 --> 00:20:07,000
Speaker 2: Other measurements that have been floating around have suggested a

401
00:20:07,039 --> 00:20:11,759
diameter of up to fifty kilometers fifty five zero. To

402
00:20:11,799 --> 00:20:14,039
get that large a diameter from the amount of light

403
00:20:14,079 --> 00:20:16,640
we see, the object would have to be incredibly dark,

404
00:20:17,160 --> 00:20:19,880
a very low albedo like the darkest comets we've ever

405
00:20:19,880 --> 00:20:21,279
seen in our own solar system.

406
00:20:21,400 --> 00:20:24,720
Speaker 1: Fifty kilometers versus less than three kilometers, that is an

407
00:20:24,880 --> 00:20:27,160
enormous factor of uncertainty. It's not even in the same

408
00:20:27,160 --> 00:20:29,519
ballpark dot at all. It means that three E and

409
00:20:29,599 --> 00:20:33,119
oz is either a very small, highly efficient engine of activity,

410
00:20:33,519 --> 00:20:37,119
or it's a colossal dark body that frankly should be

411
00:20:37,200 --> 00:20:38,119
much brighter than it is.

412
00:20:38,440 --> 00:20:42,200
Speaker 2: The discrepancy just underscores the difficulty of observing the object

413
00:20:42,599 --> 00:20:44,880
during the period when the high rise data was captured.

414
00:20:45,359 --> 00:20:47,680
When the nucleus is obscured by a coma half the

415
00:20:47,720 --> 00:20:50,559
size of the Sun and the albedo is a complete unknown,

416
00:20:51,079 --> 00:20:54,759
any estimate is highly speculative. We are literally struggling to

417
00:20:54,839 --> 00:20:57,759
find the tiny dark needle within a massive bright haystack.

418
00:20:57,960 --> 00:21:00,240
Speaker 1: So all our hope is resting on the November nineteenth

419
00:21:00,359 --> 00:21:04,079
NASA release. Astronomers need the high rise imagery from MRO

420
00:21:04,319 --> 00:21:08,119
captured on October third to provide the necessary spatial resolution

421
00:21:08,279 --> 00:21:10,680
to constrain the size, and maybe it just maybe offer

422
00:21:10,759 --> 00:21:13,880
new photometric data that limits the range of possible albedos.

423
00:21:14,200 --> 00:21:16,640
Speaker 2: If high rise can resolve the core, or at least

424
00:21:16,640 --> 00:21:19,640
provide an unprecedented upper limit on the size that forces

425
00:21:19,680 --> 00:21:22,599
those fifty kilometer estimates out of the picture, it would

426
00:21:22,640 --> 00:21:27,039
fundamentally refine all subsequent calculations of mass density and crucially,

427
00:21:27,400 --> 00:21:31,480
its mass loss efficiency. Until then, the scientific community is

428
00:21:31,720 --> 00:21:34,079
just held hostage by this massive discrepancy.

429
00:21:34,240 --> 00:21:36,640
Speaker 1: This brings us right back to the central scientific puzzle

430
00:21:36,640 --> 00:21:40,240
that can't be solved by gravity or size alone. How

431
00:21:40,319 --> 00:21:43,079
does a tiny rotating core, whether it's three kilometers or

432
00:21:43,079 --> 00:21:47,279
fifty kilometers maintain those incredibly focused and stable jets within

433
00:21:47,319 --> 00:21:49,960
a half a million mile wide coma.

434
00:21:49,559 --> 00:21:52,559
Speaker 2: And the answer, as we hinted, lies in this specialized

435
00:21:52,559 --> 00:21:55,640
and often overlooked domain of dusty plasma physics.

436
00:21:55,759 --> 00:21:58,519
Speaker 1: This is truly the AHA moment for understanding three iOS,

437
00:21:58,599 --> 00:21:59,000
isn't it?

438
00:21:59,000 --> 00:22:01,640
Speaker 2: It is need to discard the idea of space as

439
00:22:01,640 --> 00:22:04,880
simply a vacuum where objects are governed only by Newtonian physics.

440
00:22:05,240 --> 00:22:07,759
The crucial principle here is that the moment gas and

441
00:22:07,839 --> 00:22:11,000
dusts are rejected, they are subjected to intense solar radiation

442
00:22:11,400 --> 00:22:14,279
and the solar wind, and this causes rapid ionization.

443
00:22:14,440 --> 00:22:16,960
Speaker 1: Okay, let's clearly define ionization for everyone.

444
00:22:17,160 --> 00:22:20,079
Speaker 2: Ionization is what happens when a gas molecule loses or

445
00:22:20,119 --> 00:22:23,680
gains an electron that gives it an electrical charge. And

446
00:22:23,720 --> 00:22:26,480
once it's charged, it is no longer an inert physical

447
00:22:26,519 --> 00:22:30,240
particle just floating around. It becomes highly susceptible to electric

448
00:22:30,279 --> 00:22:31,119
and magnetic fields.

449
00:22:31,160 --> 00:22:33,079
Speaker 1: And this happens through a few different ways.

450
00:22:33,200 --> 00:22:36,680
Speaker 2: Yes, there are several mechanisms at play. You have photoonization

451
00:22:36,799 --> 00:22:41,039
from the Sun's powerful UV light. You have charge transfer

452
00:22:41,079 --> 00:22:43,759
interactions with the particles in the solar wind, and you

453
00:22:43,799 --> 00:22:46,920
have electron impact, ionization. All of these things are working

454
00:22:46,920 --> 00:22:49,039
to strip electrons off the gas molecules.

455
00:22:49,319 --> 00:22:52,359
Speaker 1: So the poma isn't a passive physical cloud of neutral

456
00:22:52,400 --> 00:22:56,279
gas and inert dust. It's an immense turbulent, electrically charged

457
00:22:56,319 --> 00:22:58,000
bubble of plasma exactly.

458
00:22:58,440 --> 00:23:01,759
Speaker 2: And because it's charged, it becomes electrically conductive. It interacts

459
00:23:01,839 --> 00:23:05,200
dynamically with the Sun's magnetic field lines, which are carried

460
00:23:05,240 --> 00:23:08,799
outward by the solar wind. This whole interaction leads to

461
00:23:08,839 --> 00:23:13,039
the formation of distinct, structured magnetic regions around the comet.

462
00:23:13,240 --> 00:23:15,759
It's almost like a tiny planet with its own atmosphere

463
00:23:15,759 --> 00:23:16,680
and magnetosphere.

464
00:23:16,839 --> 00:23:21,680
Speaker 1: And we mentioned three distinct regions earlier, the bowshock, the ionopause,

465
00:23:21,720 --> 00:23:25,319
and the comma pause. Can we differentiate those for the listeners?

466
00:23:25,359 --> 00:23:29,079
Speaker 2: Certainly? So. Imagine the comet is traveling through the solar wind,

467
00:23:29,359 --> 00:23:33,160
which is moving supersonically, that is faster than the speed

468
00:23:33,160 --> 00:23:34,640
of sound in that medium, like.

469
00:23:34,599 --> 00:23:37,079
Speaker 1: A supersonic jet flying through the air. You get a.

470
00:23:37,079 --> 00:23:40,519
Speaker 2: Shock wave perfect analogy. First, you hit the bowshock region.

471
00:23:40,839 --> 00:23:44,200
This is a standing shock wave where the supersonic solar

472
00:23:44,240 --> 00:23:47,720
wind abruptly slows down and becomes turbulent as it piles

473
00:23:47,759 --> 00:23:50,880
up against the dense, heavy material being ejected by the comet.

474
00:23:51,039 --> 00:23:52,160
It's the initial barrier.

475
00:23:52,480 --> 00:23:55,240
Speaker 1: Okay, So the solar wind hits that wall and slows down.

476
00:23:55,839 --> 00:23:59,920
Speaker 2: Then what the now slower but still charged particles can

477
00:24:00,000 --> 00:24:03,680
continue inward and they encounter the cometary material more directly.

478
00:24:04,279 --> 00:24:06,880
This leads to the commopause. Now, this is the key

479
00:24:06,960 --> 00:24:11,000
magnetic boundary. It's the region where the cometary magnetic magnetic field,

480
00:24:11,240 --> 00:24:13,839
the field that's induced by the comet's own plasma, is

481
00:24:13,920 --> 00:24:16,640
balanced against the magnetic field being carried by the solar wind.

482
00:24:16,880 --> 00:24:20,480
It acts like a massive, invisible, protective magnetic bubble around

483
00:24:20,519 --> 00:24:21,359
the entire coma.

484
00:24:21,440 --> 00:24:23,319
Speaker 1: And finally, the ionopause. What's that.

485
00:24:23,680 --> 00:24:27,119
Speaker 2: The ionopause is the innermost boundary, sitting closest to the nucleus.

486
00:24:27,319 --> 00:24:30,400
It's the sharp dividing line between the heavily magnetized solar

487
00:24:30,440 --> 00:24:33,920
wind plasma on the outside and the virtually magnetic field

488
00:24:33,960 --> 00:24:38,200
free region immediately surrounding the nucleus on the inside. So,

489
00:24:38,400 --> 00:24:42,119
in short, the bowshock is the slowdown, the chemopause is

490
00:24:42,119 --> 00:24:45,160
the main magnetic boundary, and the ionopause is the core.

491
00:24:44,960 --> 00:24:48,200
Speaker 1: Shield that makes the environment so much clearer. It's a

492
00:24:48,240 --> 00:24:51,880
series of nested magnetic bubbles. Now, how does this massive

493
00:24:51,960 --> 00:24:55,759
structured magnetic field, this comopause bubble, which is hundreds of

494
00:24:55,759 --> 00:24:59,119
thousands of kilometers across, how does that solve the problem

495
00:24:59,240 --> 00:25:01,279
of the tiny rotating core.

496
00:25:01,480 --> 00:25:03,680
Speaker 2: The key is that the nucleus is tiny and it's

497
00:25:03,799 --> 00:25:08,160
rotating slowly every sixteen hours inside this immense highly charged

498
00:25:08,200 --> 00:25:12,079
plasma bubble. The rotational inertia the nucleus is completely utterly

499
00:25:12,119 --> 00:25:16,359
overwhelmed by the organized channeling force of the massive electromagnetic

500
00:25:16,480 --> 00:25:17,960
environment it is created around itself.

501
00:25:18,000 --> 00:25:21,240
Speaker 1: So the magnetic fields are acting like invisible guide rails

502
00:25:21,240 --> 00:25:22,680
for all the material coming off the surface.

503
00:25:22,839 --> 00:25:26,319
Speaker 2: Precisely, the magnetic field lines that are generated or trapped

504
00:25:26,319 --> 00:25:29,279
within the coma can guide the flow of charged particles,

505
00:25:29,559 --> 00:25:32,400
and that even includes the dust grains through a process

506
00:25:32,400 --> 00:25:35,839
called dust charging. So instead of the material diffusing evenly

507
00:25:35,839 --> 00:25:39,039
outward because of the nucleus rotation, the field lines act

508
00:25:39,039 --> 00:25:43,200
as conduits. They're like magnetic hoses. They sort, accelerate and

509
00:25:43,319 --> 00:25:47,279
channel the ionized gas and dust into those specific stable

510
00:25:47,559 --> 00:25:48,480
observed jets.

511
00:25:48,880 --> 00:25:51,720
Speaker 1: That is a phenomenal explanation. So the stability of the

512
00:25:51,799 --> 00:25:54,839
jets isn't a function of some complex nozzle or weird

513
00:25:54,960 --> 00:25:58,000
structure on the nucleus itself. It's a function of the

514
00:25:58,119 --> 00:26:02,559
massive surrounding electromagnetic environment channeling the material along these magnetic

515
00:26:02,559 --> 00:26:03,200
field lines.

516
00:26:03,279 --> 00:26:06,640
Speaker 2: It is the most robust physics based explanation we have.

517
00:26:07,079 --> 00:26:10,519
It suggests that three Ietellis's active behavior is less about

518
00:26:10,559 --> 00:26:13,680
its internal mechanics and much more about its powerful rapid

519
00:26:13,680 --> 00:26:17,160
interaction with the solar environment, which creates this huge, self

520
00:26:17,279 --> 00:26:22,079
organizing plasma structure. This complex dusty plasma physics provides a

521
00:26:22,079 --> 00:26:25,240
compelling evidence, grounded reason for the anomaly, and it takes

522
00:26:25,240 --> 00:26:29,039
the explanation firmly out of the realm of unsupported speculation.

523
00:26:29,400 --> 00:26:32,720
Speaker 1: It fundamentally changes how we view comments. They aren't just

524
00:26:32,880 --> 00:26:37,400
orbiting dirty snowballs anymore. They are highly dynamic, electrically active

525
00:26:37,480 --> 00:26:40,960
generators of magnetospheres, even if they are just passing through.

526
00:26:41,319 --> 00:26:44,039
Speaker 2: Given all the excitement over the NASA data and the

527
00:26:44,079 --> 00:26:48,240
anticipation for the CME impact, a lot of amateur astronomers

528
00:26:48,240 --> 00:26:51,039
and curious observers are trying to spot three iout lists now,

529
00:26:51,359 --> 00:26:53,480
But we need to be realistic about the challenges.

530
00:26:53,559 --> 00:26:56,680
Speaker 1: Absolutely, this is important three I out list is not Jupiter.

531
00:26:57,000 --> 00:27:00,319
It is quite dim even with decent equipment. If you

532
00:27:00,400 --> 00:27:02,799
just look at a single live feed image, you will

533
00:27:02,880 --> 00:27:05,759
likely see only a blurry, pale, little dot, and.

534
00:27:05,640 --> 00:27:08,880
Speaker 2: That leads to tremendous confusion Online. You see people who

535
00:27:08,880 --> 00:27:11,799
watch a live stream and they confidently state the astronomers

536
00:27:11,799 --> 00:27:14,359
are lying. There's no tail, It's just a fuzzy blob.

537
00:27:15,160 --> 00:27:18,160
And this denial is rooted entirely in a misunderstanding of

538
00:27:18,240 --> 00:27:19,559
observational technique.

539
00:27:19,720 --> 00:27:23,359
Speaker 1: Let's clarify the essential technique then stacking images. Why is

540
00:27:23,400 --> 00:27:26,359
stacking mandatory to resolve the faint tail and the jets?

541
00:27:26,480 --> 00:27:28,799
Speaker 2: Okay, so to resolve faint objects like the three ie

542
00:27:28,799 --> 00:27:30,680
at us tail. It's the signal you want. You need

543
00:27:30,720 --> 00:27:33,680
a long exposure to gather enough light. But a single,

544
00:27:33,839 --> 00:27:36,200
very long exposure captures way too much noise.

545
00:27:36,480 --> 00:27:38,920
Speaker 1: And what do you mean by noise? In this context?

546
00:27:39,160 --> 00:27:43,960
Speaker 2: The noise includes the constantly shimmering atmospheric distortions, any tiny

547
00:27:44,000 --> 00:27:47,240
movement in the telescope mount, and the inherent electrical noise

548
00:27:47,279 --> 00:27:50,960
from the camera sensor itself. The longer the exposure, the

549
00:27:51,000 --> 00:27:54,400
more blurred and noisy the image becomes. The signal gets

550
00:27:54,480 --> 00:27:54,880
washed out.

551
00:27:55,279 --> 00:27:57,680
Speaker 1: So the signal is the light from the comet, but

552
00:27:57,720 --> 00:28:00,759
the noise is all the distortion and unwanted back ground data.

553
00:28:00,759 --> 00:28:06,440
Speaker 2: Correct stacking solves this problem. You take dozens, sometimes hundreds,

554
00:28:06,480 --> 00:28:10,480
of shorter, medium length exposures, say thirty to sixty seconds each.

555
00:28:11,039 --> 00:28:15,519
Then sophisticated software digitally aligns all those images perfectly on

556
00:28:15,559 --> 00:28:16,480
the target object.

557
00:28:16,599 --> 00:28:19,400
Speaker 1: So it layers them all on top of each other exactly, and.

558
00:28:19,400 --> 00:28:23,480
Speaker 2: By mathematically averaging all those aligned frames, the consistent signal

559
00:28:23,519 --> 00:28:25,400
the photons that are actually forming the tail and the

560
00:28:25,440 --> 00:28:28,839
jets is reinforced and integrated. It gets stronger. Meanwhile, the

561
00:28:28,880 --> 00:28:32,680
random noise like that atmospheric wobble and random sensor artifacts,

562
00:28:32,880 --> 00:28:35,400
it's effectively canceled out or drastically diminished.

563
00:28:35,519 --> 00:28:38,839
Speaker 1: It's the only way to dramatically improve the crucial signal

564
00:28:38,839 --> 00:28:41,480
to noise ratio and to pull out those fine details

565
00:28:41,480 --> 00:28:45,000
that are otherwise completely hidden. So if someone is looking

566
00:28:45,000 --> 00:28:49,079
at an unprocessed live single frame image, they are failing

567
00:28:49,119 --> 00:28:52,839
to perform the necessary due diligence for dim object astronomy.

568
00:28:53,119 --> 00:28:56,960
Speaker 2: Exactly those beautiful images you see online showing the faint,

569
00:28:57,079 --> 00:29:01,640
extensive tail and the distinct sounward face jet. Those are

570
00:29:01,680 --> 00:29:05,519
the result of many hours of acquisition and post processing

571
00:29:05,559 --> 00:29:10,039
work by dedicated AFTRA photographers who understand this technique. They

572
00:29:10,039 --> 00:29:13,440
are not fabricated, They are simply the result of necessary processing.

573
00:29:13,559 --> 00:29:15,759
Speaker 1: The good news, though, is that the viewing conditions are

574
00:29:15,759 --> 00:29:17,559
actually starting to improve dramatically.

575
00:29:17,680 --> 00:29:22,599
Speaker 2: Yes, during the most difficult observation period around that superior conjunction,

576
00:29:23,000 --> 00:29:25,160
if the tail was there, it would have been stretching

577
00:29:25,160 --> 00:29:27,799
effectively directly away from us. It would be pointing right

578
00:29:27,839 --> 00:29:30,279
back along our line of sight, making it very difficult

579
00:29:30,279 --> 00:29:31,799
to distinguish from background glare.

580
00:29:31,920 --> 00:29:34,880
Speaker 1: But as the object moves further along its orbit toward

581
00:29:34,920 --> 00:29:37,920
its closest approach to Earth on December nineteenth, it's viewing

582
00:29:37,960 --> 00:29:39,400
geometry gets better.

583
00:29:39,400 --> 00:29:42,319
Speaker 2: Much better. We're now seeing it at a more oblique

584
00:29:42,480 --> 00:29:43,640
or lateral angle.

585
00:29:43,799 --> 00:29:44,920
Speaker 1: And what does that mean visually?

586
00:29:45,359 --> 00:29:48,400
Speaker 2: That oblique angle means the tail is no longer stretching

587
00:29:48,440 --> 00:29:51,240
directly away from our line of sight, but is presented

588
00:29:51,279 --> 00:29:54,119
more to the sign. It gives us much better contrast

589
00:29:54,160 --> 00:29:57,359
against the background sky. Assuming a course that we employ

590
00:29:57,440 --> 00:29:58,720
the stacking technique, and.

591
00:29:58,680 --> 00:30:02,240
Speaker 1: We have some really clear examples contrasting the effort. If

592
00:30:02,240 --> 00:30:04,799
you try to use a basic smart telescope like a

593
00:30:04,799 --> 00:30:08,160
five hundred dollars c star. You might capture the bright

594
00:30:08,279 --> 00:30:11,279
central coma with a few stacked images, but the.

595
00:30:11,200 --> 00:30:14,640
Speaker 2: Tail will remain invisible. You need the commitment to process.

596
00:30:15,160 --> 00:30:17,720
For instance, you can compare that simple image to the

597
00:30:17,799 --> 00:30:21,920
professional results taken using say six hundred and eighty two exposures.

598
00:30:22,440 --> 00:30:24,839
That is, one hundred and eighty two exposures in six

599
00:30:24,880 --> 00:30:27,960
different filtered bands, resulting in thousands of captured frames that

600
00:30:28,000 --> 00:30:28,759
are then stacked.

601
00:30:28,920 --> 00:30:30,440
Speaker 1: The difference must be staggering.

602
00:30:30,559 --> 00:30:33,359
Speaker 2: It is one shows a fuzzy doc the other shows

603
00:30:33,359 --> 00:30:36,400
a fully formed active inter cellar body with clear jets

604
00:30:36,440 --> 00:30:37,480
and a long, faint tail.

605
00:30:37,680 --> 00:30:40,200
Speaker 1: It is a clear reminder that in deep space observation,

606
00:30:40,400 --> 00:30:43,680
your technique often matters just as much as your equipment. Okay,

607
00:30:43,759 --> 00:30:47,440
let's synthesize the critical elements of this incredible situation. We

608
00:30:47,480 --> 00:30:51,359
have tracked the immediate imminent news NASA's critical high rise

609
00:30:51,400 --> 00:30:54,759
image reveal on November nineteenth, and that holds the key

610
00:30:54,839 --> 00:30:58,400
to solving the object's true size, the most fundamental unknown,

611
00:30:58,720 --> 00:30:59,000
and we.

612
00:30:59,000 --> 00:31:02,640
Speaker 2: Have identified the real time high stakes threat, the CME

613
00:31:02,759 --> 00:31:06,519
strike around November twenty second. This provides an involuntary high

614
00:31:06,680 --> 00:31:09,960
energy physics experiment that's set to test the resilient and

615
00:31:10,000 --> 00:31:12,440
density of the object's plasma environment.

616
00:31:12,640 --> 00:31:15,079
Speaker 1: And crucially, we've learned that making sense of three ilo

617
00:31:15,160 --> 00:31:19,200
less requires moving past simple Newtonian physics and really embracing

618
00:31:19,319 --> 00:31:23,119
dusty plasma dynamics. The stable persistent jets are likely not

619
00:31:23,240 --> 00:31:26,200
features of the tiny nucleus, but rather a function of

620
00:31:26,240 --> 00:31:30,200
the massive electromagnetic fields within its enormous coma channeling the

621
00:31:30,240 --> 00:31:32,759
ionized material along these magnetic conduits.

622
00:31:32,920 --> 00:31:36,400
Speaker 2: This interstellar object is forcing the absolute application of our

623
00:31:36,440 --> 00:31:39,400
most cutting edge physics to a body that originated outside

624
00:31:39,440 --> 00:31:42,000
of our stellar neighborhood, and that brings us to the

625
00:31:42,039 --> 00:31:45,079
final necessary question that's raised by this whole saga.

626
00:31:45,160 --> 00:31:47,640
Speaker 1: What stands out to you is the ultimate takeaway from

627
00:31:47,640 --> 00:31:50,920
this ongoing observation, What should we be thinking about?

628
00:31:51,079 --> 00:31:54,079
Speaker 2: The CME hit on November twenty second is more than

629
00:31:54,119 --> 00:31:57,559
just a passing headline. It represents a unique opportunity to

630
00:31:57,599 --> 00:32:01,200
gain new fundamental knowledge. If we see a dramatic tail

631
00:32:01,240 --> 00:32:04,799
disconnection event, or if instruments confirm a massive surge in

632
00:32:04,839 --> 00:32:08,680
the surrounding magnetic field, say comperal to that tenfold increase

633
00:32:08,680 --> 00:32:11,160
scene during the Rosetta mission at Comet sixty seven P.

634
00:32:11,880 --> 00:32:16,279
What new profound information about the composition, density, and magnetic

635
00:32:16,319 --> 00:32:19,720
interaction capabilities of objects born around other stars will that

636
00:32:19,759 --> 00:32:20,680
force us to integrate?

637
00:32:20,960 --> 00:32:23,319
Speaker 1: It's a measure of how different the environment of another

638
00:32:23,359 --> 00:32:25,079
star system might make these objects.

639
00:32:25,319 --> 00:32:28,640
Speaker 2: Exactly? Will the severity of the plasma interaction tell us

640
00:32:28,680 --> 00:32:32,880
that three Iatlys is shedding denser, more highly volatile material

641
00:32:32,920 --> 00:32:36,319
than we ever expected from a typical comment? What boundaries

642
00:32:36,359 --> 00:32:40,440
of cometary science was interstellar challenger help us shatter? Next?

643
00:32:40,759 --> 00:32:43,640
So think about this. How profoundly does the knowledge of

644
00:32:43,640 --> 00:32:46,400
plasma dynamics, the fact that the space around this object

645
00:32:46,480 --> 00:32:49,680
is an electrically charged active environment, How does that change

646
00:32:49,680 --> 00:32:52,960
how you view space itself? We are observing something born

647
00:32:53,000 --> 00:32:56,200
somewhere else being violently tested by our own son, and

648
00:32:56,240 --> 00:32:58,480
the results coming in the next few days could genuinely

649
00:32:58,480 --> 00:33:00,799
rewrite the rule book on interstellar visitors

