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Speaker 1: Imagine just for a second that you are standing in

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a room and it's completely utterly pitch black.

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Speaker 2: Okay.

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Speaker 1: You can't see your hand in front of your face,

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you can't see the walls, you can't see the door.

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Speaker 2: But.

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Speaker 1: You know someone else is in there with you, you

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just know it. You can't see them, you can't hear

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them breathing, but you can feel I don't know, the

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floorboards shifting under a heavy weight.

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Speaker 2: That's a creepy thought, right.

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Speaker 1: You can feel the air sort of swirl as something

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massive moves past you. You can hear objects on a

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shelf across the room or rattling, even though you didn't

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touch them. It's that primal feeling of a presence you

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cannot verify with your eyes, but your gut, your instincts,

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they tell you it is undeniably real.

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Speaker 2: That is a terrifying image to start with. It's straight

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out of a horror movie.

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Speaker 1: It is, isn't it. It's so visceral. But that specific feeling,

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that sense of an invisible presence manipulating the environment, that

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is exactly what is happening in our solar system right now.

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Speaker 2: It's a perfect analogy.

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Speaker 1: The outer reach, the deep dark backyard of our sun

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are misbehaving, and we aren't talking about a few loose

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rocks tumbling around. We are talking about the fundamental architecture

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of our home.

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Speaker 2: Yeah, we're essentially looking at a cosmic crime scene. The

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suspect has fled or is hiding in the shadows, but

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they've left fingerprints everywhere. Fingerprints are like that massive gravitational

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fingerprints that simply shouldn't be there if the room was empty.

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Speaker 1: And that's what we are doing today. We are looking

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at those fingerprints. We're talking about objects way past Neptune,

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way out in the boonies that are clustering together in

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ways that defy.

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Speaker 2: All logic, all known logic.

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Speaker 1: Anyway, right, Mathematically, the chance of this happening by accident

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is less than one point.

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Speaker 2: One percent, less than a tenth of a percent.

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Speaker 1: So we aren't talking about a fluke. We are talking

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about a ghost in the gravity, a massive invisible object,

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what we're calling Planet nine, pulling strings from the darkness.

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Speaker 2: And that's the hook for me. It feels like a

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ghost story, you know, it feels like science fiction. But

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what we are going to talk talk about today is

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actually hard, rigorous physics. It's data It's a story about data,

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not magic.

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Speaker 1: Welcome to thrilling Threads. I am so excited for this one. Today.

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We are grabbing a massive stack of research, new studies

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from twenty twenty four, twenty twenty five, some archiabal data

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that's been dusted off, and some incredible physics to unravel

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perhaps the biggest mystery of our cosmic neighborhood.

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Speaker 2: Our mission today is really to complete the map. I

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think most people have this mental model of the Solar System,

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some eight planets, asteroid belt.

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Speaker 1: Maybe the Kuiper Belt, if they're paying attention in school.

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Speaker 2: Right, they're really paying attention, and then nothing, just empty

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space until the next star. But the data, it suggests

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we are missing a massive piece from the.

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Speaker 1: Puzzle and we are living through what you've called a

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Laverie moment, which sounds very fancy, but I want to

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break that down because it really frames this whole discussion.

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It does this isn't just about finding a rock. It's

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about a specific way of seeing the universe.

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Speaker 2: Right, that's absolutely right. To understand where we are now,

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we have to look back way back to eighteen forty six. Yeah,

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because this has happened before. It's the story of a

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French astronomer named Urban Leverier.

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Speaker 1: I love this story because it involves a guy with

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a pen defeating a bunch of people with telescopes.

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Speaker 2: It is the ultimate triumph of the nerd.

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Speaker 1: So what was happening?

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Speaker 2: Essentially, Yes, in the mid nineteenth century, astronomers had a problem.

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They were tracking the planet Uranus, which at the time

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was the furthest known planet, and Uranus was well, it

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was misbehaving. It wasn't following the rules.

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Speaker 1: And when you say rules, you mean Newton's laws of

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gravity exactly.

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Speaker 2: Newton's laws are very, very strict. They predict exactly where

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a planet should be based on the mass of the

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Sun and the other planets. It's a clockwork universe, supposedly.

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Speaker 1: But Urinus was off schedule.

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Speaker 2: It was accelerating and decelerating along its orbit in a

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way that made no sense. It was lagging behind where

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it should be that it would speed up. It was

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as if something invisible was tugging on it.

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Speaker 1: Okay, so the astronomers are scratching their heads. They're checking

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their telescopes, maybe assuming their charts are wrong or something right.

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Speaker 2: They're looking for an error in their own work. But

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Leverier sits down. And you have to remember, no supercomputers,

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no AI, just pen, paper and a candle, basically.

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Speaker 1: And a whole lot of mass.

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Speaker 2: An incredible amount of math. Yeah, and he crunches the numbers.

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He realized that the only explanation, the only thing that

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could make Urinus do that, was that there had to

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be another massive planet further.

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Speaker 1: Out, an unseen planet.

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Speaker 2: Totally unseen. Yeah. That was gravitationally interacting with Uranus. And

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he didn't just say there's a planet out there. He

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calculated its mass, its orbit, and the specific coordinates of

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this invisible object.

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Speaker 1: He drew a map to a place no one had

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ever seen.

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Speaker 2: She did. He sent a letter to a deservatory in

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Berlin saying, effectively, point your telescope at this specific patch

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of empty sky, you'll find it.

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Speaker 1: And this is the part that gives me chills every time,

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me too. They pointed the telescope aut his coordinates, and

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that very night, the very night.

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Speaker 2: They found Neptune. Just like that, what in one degree

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of whereas math said it would be one degree. That's

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the width of your pinky finger held at arms light.

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Speaker 1: That is just incredible. He found a planet with the

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tip of his pen.

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Speaker 2: He discovered a world without ever looking through a telescope,

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and that established this fundamental precedent. Gravity acts as a

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tracer for the invisible. Right, if the math doesn't balance,

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it means there is mass hiding somewhere. And today you

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fast forward nearly one hundred and eighty years and we're

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doing the exact same thing.

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Speaker 1: Okay, but this time it's not Urinus that's being pulled on.

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We've already accounted for Neptune in our models, correct, So

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what's the evidence now, what's misbehaving?

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Speaker 2: It's things much much further out. We were looking at

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the Kuiper Belt, which is that big ring of icy

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debris beyond Neptune.

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Speaker 1: Like where Pluto lives exactly.

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Speaker 2: But we're looking even beyond that at a group of

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extremely distant objects called said nooids. Said nooids.

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Speaker 1: Good name is that from the dwarf planet said Nah Yes, named.

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Speaker 2: After no which is one of the most famous of

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these distant objects. It's a dwarf planet candidate that takes

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over eleven thousand years.

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Speaker 1: To orbit the Sun eleven thousand years.

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Speaker 2: These are objects that spend most of their time in

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the deep, deep frieze of space. Now here's the key.

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In a stable eight planet Solar system, these objects should

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be scattered randomly.

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Speaker 1: Okay, that makes sense.

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Speaker 2: Their orbits should point in all different directions because of

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billions of years of chaotic gravitational interactions.

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Speaker 1: Right, it's like entropy. If you spill a bag of

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marbles on the floor, they'd roll everywhere. They wouldn't all

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just roll into one corner and line up neatly.

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Speaker 2: That's a perfect way to put it. Yeah, but when

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we look at these said nois, and we only know

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of a handful because they are so incredibly hard to see,

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that is exactly what they are doing.

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Speaker 1: Are lining up.

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Speaker 2: They're physically clustered in space. They're all swinging out in

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the same direction, and their orbits are all tilted at

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similar ankles away from the main plane of the Solar system.

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Speaker 1: And the odds of that being a coincidence are dely zero.

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Speaker 2: As we said, it's less than point one percent. So

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in twenty sixteen, two astronomers at Caltech, Constantin Batagen and

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Mike Brown, who are I mean, absolute titans of planetary astronomy.

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Speaker 1: Mike Brown is the guy who killed Pluto, right, He's the.

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Speaker 2: Guy he feels a little guilty about it, I think,

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so he wants to find a new planet to make

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up for it.

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Speaker 1: Fair enough, so.

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Speaker 2: They publish a model. They ran simulations and asked what

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could possibly.

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Speaker 1: Cause this, and the answer wasn't bad luck.

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Speaker 2: No. The simulations show that if you introduce a ninth planet,

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something roughly five to ten times the mass of the Earth,

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into the deep Outer Solar System, huh, it's gravity would

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naturally herd these objects. It acts like a sheep dog.

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It forces them into these synchronized, clustered orbits over millions

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and millions of years.

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Speaker 1: So without the planet, the system makes no sense.

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Speaker 2: It makes no sense. But you add the planet and

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everything clicks perfectly into place.

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Speaker 1: Okay, so let's profile the suspect. We know it's there

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because of the math, But what is it? What are

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we actually looking for? Because Planet nine sounds a little.

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Speaker 2: Generic, it's a working title. What we are really looking

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for is a super.

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Speaker 1: Earth, which is a term I hear a lot, especially

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in science fiction, and I think people picture like crypton

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or something, But what does it mean physically in astronomy.

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Speaker 2: It's actually a pretty simple definition. It refers strictly to mass.

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A super Earth is a planet that is larger than

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Earth but smaller than Neptune. So Neptune is about seventeen

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Earth masses. Earth is well one Earth mass. We're looking

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for something in that sweet spot that five to ten

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Earth mass range.

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Speaker 1: And here's where it gets really really interesting for me

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looking at the context you provided, when we look outside

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our Solar System at other star systems yet exoplanets, Yeah,

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super earths are the most common type of planet out there.

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They are literally everywhere.

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Speaker 2: They are the standard galactic furniture. If you look at

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the data from the Kepler Space Telescope or the Test mission,

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super earths are the medium planet. They are the fault model,

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but we don't have one currently. No, we are the

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odd ones out. Our Solar system has small, rocky worlds

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like Earth and Mars, and then we have massive gas

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giants like Jupiter and Saturn. We are missing that whole

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middleweight category.

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Speaker 1: It's like walking into a house that has tiny footstools

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and massive sectional sofas but no regular sized chairs.

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Speaker 2: That's a great way to put it. It's a genuine

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architectural gap in our Solar system's design. Finding Planet nine

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would actually make our Solar system normal.

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Speaker 1: It would stop us from being an anomaly.

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Speaker 2: It would stop us from being the weirdos and align

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our architecture with what we see happening all across the galaxy.

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Speaker 1: So it's big, five to ten times the massive Earth.

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But where is it? Because if it's that big, shouldn't

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we have I don't know, tripped over it by now?

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Speaker 2: Well, it is incredibly far away. Its orbit is highly

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elongated or eccentric. It's not a nice circle like Earth's.

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It takes somewhere between ten thousand and twenty thousand years

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to circle the Sun just.

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Speaker 1: One time, twenty thousand years for one year. That is

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just it's mind boggling. That means the last time it

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was in this part of its orbit, humans were just

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figuring them out agriculture.

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Speaker 2: Even earlier than that, maybe we were still paintying gabes. Wow.

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To give you a sense of scale, we use a

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measurement called an astronomical unit, or AU. One AU is

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the distance from the Earth to the Sun.

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Speaker 1: Right about ninety three million miles.

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Speaker 2: So at its closest approach to the Sun, what we

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call parahelium, planet nine is about two hundred AU away,

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so two hundred times further than us, but at its

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furthest point, it's a felion. It swings out to maybe

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a thousand au.

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Speaker 1: One thousand, and for comparison, Pluto is what thirty or

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forty au away exactly.

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Speaker 2: Pluto's orbit varies between about thirty and fifty AU. So

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Pluto is practically in our backyard compared to this thing.

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This object is in the deep deep freeze.

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Speaker 1: Okay. So we have this massive object five to ten

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times the size of Earth. We know roughly where it

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should be because of the math. This leads to the question.

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I think every single listener is screaming at their device

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right now.

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Speaker 2: I know the one.

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Speaker 1: Why haven't we seen it? Why can't we just point

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the Hupace telescope at that spot and snap a picture?

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Speaker 2: That is the most common question. If it's so big,

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why is it invisible? And the answer lies in the

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fundamental physics of light, specifically a little something called the

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inverse square law.

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Speaker 1: Okay, let's unpack the inverse square law, because this explains

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why space exploration is so hard in general. It's not

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just that things get a little dimmer further away.

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Speaker 2: No, it's not a linear dimming. Think about a simple

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light bulb or a candle. If you're standing one foot

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away from it, it's bright. Sure, if you step back

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to two feet away, it's not just half as bright,

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it's one quarter as bright. The intensity of the light

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drops off with the square of the.

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Speaker 1: Distance, so if you go three feet away, it's one

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ninth is bright.

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Speaker 2: Precisely. Now apply that to the sun. Sunlight has to

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travel let's pick a number, say seven hundred au out

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to hit planet nine.

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Speaker 1: That's a long way.

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Speaker 2: By the time the sunlight gets there, the light is

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incredibly weak. It's spread out over a huge area, so.

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Speaker 1: It's basically twilight or even darker.

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Speaker 2: On this planet, much much darker. Imagine a single candle

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in the middle of a football stadium at night. But then,

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and this is the absolute kicker, that tiny amount of

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light has to reflect off the surface of the planet

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and travel another seven hundred AU all the way back

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to our telescopes on Earth.

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Speaker 1: So the dimming happens twice.

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Speaker 2: It gets hit by the inverse square law on the

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way out and again on the way.

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Speaker 1: Back, so it's really the inverse fourth power.

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Speaker 2: Then, effectively, yes, the result is that planet nine is

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thousands upon thousands of times dimmer than even distant objects

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like Pluto to a standard optical telescope that's looking for

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a reflected sunlight. It is effectively a black object sitting

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against a black background.

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Speaker 1: So looking for it with a normal camera is like

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looking for a piece of coal and a dark cellar

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at midnight while wearing sunglasses.

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Speaker 2: Yes, it's just incredibly difficult.

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Speaker 1: Okay, that makes sense. So that strategy is out, which.

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Speaker 2: Is why researchers have shifted their strategy. They aren't just

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looking for reflected light anymore. They are looking for heat

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and for red exactly. Even a very cold planet way

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out in the vall still retains some heat from its

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formation billions of years ago. It's warmer than the absolute

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zero of empty space, so it should glow faintly in

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the infrared spectrum.

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Speaker 1: So we just need to put on our heat vision goggles. Basically,

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that sounds much easier.

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Speaker 2: You would think so, But of course there's a catch there.

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Chair This was always a catch, and the catch is

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the Milky Way.

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Speaker 1: Wait, our own galaxy is in the way.

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Speaker 2: How well, the galactic plane, that bright, hazy band you

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can see in the night sky from a dark location

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is crowded with billions of stars and clouds of dust

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and gas. All of that stuff emits infrared radiation. It's

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infrared noise.

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Speaker 1: So it's like static.

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Speaker 2: It's like trying to hear a specific faint whisper and

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a screaming stadium full of people. If Planet nine happens

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to be passing in front of the dense part of

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the Milky Way in its orbit, it's hidden. It's completely

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hidden behind this wall of infrared noise. And unfortunately, the

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predicted orbit takes it right across the galactic plane.

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Speaker 1: Of course it does. So it's faint, it's far, and

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it might be hiding in the galactic crowd. But despite

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all of that, we have some major breakthroughs happening right now.

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Speaker 2: You do.

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Speaker 1: Let's talk about the twenty twenty five study. I believe

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it was led by a researcher named Terry Longfan. This

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felt like a moment where the detective work really leveled up.

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Speaker 2: This is a brilliant piece of science. They used what

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we call the shift in stack method, but they did

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it using archival data.

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Speaker 1: I love this because it shows you don't always need

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a new, shiny, billion dollar telescope. Sometimes you just need

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to look at the old tapes differently precisely.

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Speaker 2: It's so clever. They took data from the IRAS satellite,

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which was an infrared satellite that scanned the sky way

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back in nineteen eighty three.

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Speaker 1: Okay, that's old data.

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Speaker 2: Very old, and they compared it with data from the

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Ocardi satellite, which is a Japanese infrared satellite that flew

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in two thousand and six.

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Speaker 1: That's a twenty three year gap between the two pictures, and.

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Speaker 2: That gap is the key. Remember, Planet nine moves, but

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from our perspective, it moves very, very slowly across the sky.

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In a day or even a year, it barely budget

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against the background stars. But in twenty three years it

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moves just enough to be noticeable.

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Speaker 1: So if you layer the two images on top of

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each other, you shift and stack them. The stars should

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stay still, but the planet should jump from one spot

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to another exactly.

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Speaker 2: You layer the images to digitally cancel out all the

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static background noise, the stars, the distant galaxies, and you

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look for the one faint pixel that shifted position.

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Speaker 1: It's like looking at two frames of a movie. Real

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the background scenery doesn't change, but the actor moves from

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left to right.

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Speaker 2: That's the idea, and they found something.

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Speaker 1: They found a candidate.

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Speaker 2: They identified a very promising signal that appears in both

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data sets from both nineteen eighty three and two thousand

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and six, and its movement pattern matches the mathematical prediction

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for planet nine perfectly.

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Speaker 1: But I can hear a butt in your.

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Speaker 2: Voice, but it is extremely faint. It sits right at

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the very very edge of the detection limits for those

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old instruments. It's a ghost of a.

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Speaker 1: Signal, so it could be noise.

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Speaker 2: It could be a glitch in the data processing, or

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a random cosmic ray hitting the sensor in just the

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right way in both data sets, though that's unlikely. It's

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the most promising lead we have from archival data, but

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it requires conformation. We need a better look with a

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more powerful instrument to be sure it's a solid body.

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Speaker 1: So that's the visual hunt. We have a maybe, a

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very exciting maybe. But the mathematical case just got a

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huge upgrade too.

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Speaker 2: It did.

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Speaker 1: In twenty twenty four, Vatagen and Brown, the original duo,

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they dropped a new paper, and this one involves something

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called neptune crossing TNOs.

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Speaker 2: This for me, is arguably even more compelling than the

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clustering of the said noise we discussed earlier.

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Speaker 1: Okay, let's break it down. What is a Neptune crosser.

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It sounds like a traffic violation in space.

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Speaker 2: It's pretty much exactly what it sounds like. These are

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trans Neptunian objects or tno so icy bodies in the

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Kuiper Belt. But their orbits are so eccentric, so stretched out,

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that they periodically cross inside the orbit of Neptune.

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Speaker 1: And that's dangerous.

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Speaker 2: Right.

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Speaker 1: Neptune is a gas giant's huge. If you get too

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close to that, it's gravity should what kick you out?

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Speaker 2: Right. Neptune is a bully, It's a gravitational monster. Under

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normal physics, if a small icy rock crosses Neptune's path,

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one of two things is going to happen, and quickly. Okay,

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Either Neptune's gravity swallows it, pulling it in to crash

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into the planet, or Neptune acts like a gravitational sling

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shot and flings it out of the Solar System entirely.

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Speaker 1: So these objects should not be stable.

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Speaker 2: These should not exist. They should have been cleaned up

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and vanished within a few million years of the Solar

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System's formation.

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Speaker 1: But they're still there. We see them, we see them.

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Speaker 2: They exist. Yeah, and that was a huge puzzle for

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a long time. Why hasn't Neptune cleaned up its neighborhood.

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Speaker 1: So Beigeen and Brown ran these things called n body simulations,

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which or what they're massive computer models that calculate the

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gravitational pull of every object on every other object over

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billions and billions of years.

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Speaker 2: And what did the simulation say.

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Speaker 1: It showed that if you only have the eight known

401
00:17:58,759 --> 00:18:03,039
planets in your model, the Neptune crossing objects vanish every time.

402
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They simply cannot survive for the four point five billion

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year age of the Solar System.

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Speaker 2: But if you add planet nine into the simulation.

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Speaker 1: The bodyguard arrise, bodyguard arrives.

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00:18:12,880 --> 00:18:17,240
Speaker 2: Planet nine acts as a shepherd. Its gravity, even from

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way out there, exudes this subtle but persistent pull that

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keeps these objects in a state of what we call resonance.

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It gently nudges them, preventing them from getting too close

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to Neptune on their orbits.

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Speaker 1: So Planet nine is actively protecting these erratic objects from Neptune.

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Speaker 2: It's actively managing their orbits. And the statistical confidence here

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is what blew everyone away. They found the result was

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five sigma.

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Speaker 1: Five sigma. Now, for listeners who don't speak statistics, what

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does that actually mean? I know sigma from like six

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sigma in business, But this is physics.

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Speaker 2: Five sigma is the gold standard in science. It's the

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official threshold for declaring a discovery definitive. To give you

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00:18:56,200 --> 00:18:59,039
some context, the discovery of the Higgs boson the god

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00:18:59,079 --> 00:19:01,079
particle five sigma discovery.

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Speaker 1: So it's a big deal.

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Speaker 2: It means there is a one in three point five

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million chance that this is a statistical fluke.

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Speaker 1: One in three point five million.

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00:19:08,720 --> 00:19:12,039
Speaker 2: Yes, so this moves planet Metane from Hey, this is

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a possible explanation for some weird clustering we see to

428
00:19:16,519 --> 00:19:19,240
this is a mathematical requirement for the Solar System to

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exist as we currently observe it.

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Speaker 1: That is heavy. It's not just a guess anymore. The

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00:19:23,880 --> 00:19:27,079
math is saying the building falls down without this pillar exactly.

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Speaker 2: And this study was so crucial because it addressed the

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00:19:29,920 --> 00:19:32,960
skeptics who would say, well, maybe you're just looking for

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00:19:32,960 --> 00:19:36,680
clustered objects in the wrong places. This isn't about observational bias.

435
00:19:36,680 --> 00:19:39,599
It's about the fundamental physics of survival. For these objects.

436
00:19:39,720 --> 00:19:42,119
They shouldn't be here, but they are. Okay.

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00:19:42,160 --> 00:19:45,480
Speaker 1: So the math is screaming it's there. The archival data

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00:19:45,519 --> 00:19:48,799
is whispering. I think I see it, but we want

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00:19:48,799 --> 00:19:51,160
to see it for real. We want the mugshot, We

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00:19:51,200 --> 00:19:53,880
want the picture. Enter the eye of the future. The

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00:19:54,000 --> 00:19:56,039
verraa C. Reuben Observatory.

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00:19:56,359 --> 00:19:59,319
Speaker 2: This is the game changer as of early twenty twenty six.

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00:19:59,440 --> 00:20:02,440
It is full operational and chili and it is an

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absolute beast.

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Speaker 1: It's not just a normal telescope, right, It's not like

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00:20:05,519 --> 00:20:06,680
looking through a small tube.

447
00:20:06,839 --> 00:20:08,599
Speaker 2: No, not at all. Think of it as a high

448
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speed mapping system. It has a huge eight point four

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00:20:11,720 --> 00:20:14,880
meter mirror. But the camera is the real star of

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the show. It's a three point two gigapick.

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Speaker 1: The camera three point two gigapixels. My phone has what

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twelve megapixels? Maybe forty eight.

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Speaker 2: It is the largest digital sensor ever built for astronomy.

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00:20:25,000 --> 00:20:27,400
To put another way, the field of view is so

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wide it can capture an area of the sky equivalent

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to forty full moons in a single snapshot.

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Speaker 1: Forty full moons. And what is it doing with all

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that power?

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Speaker 2: It's creating what they call a cosmic movie. It scans

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the entire southern sky every few nights, over and over

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00:20:42,359 --> 00:20:44,000
and over again. Yeah, for ten years.

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Speaker 1: So instead of staring at one tiny spot for a

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long time like.

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Speaker 2: Hubble does, right, Hubble has a tiny pinprick field of view.

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Speaker 1: Rubin is monitoring everything.

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Speaker 2: All the time, everything, And this is the perfect strategy

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for finding something like planet nine. Because Planet nine is

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faint and it moves right, the Ruben observe itt to

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or he can detect objects down to a brightness level

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or magnitude of twenty four point five in a single shot,

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which is already very faint. But because it visits the

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same patch of sky over eight hundred times during its survey,

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you can stack the images or back to the shift

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in status on.

475
00:21:14,279 --> 00:21:18,039
Speaker 1: A massive industrial scale. When you stack a year's worth

476
00:21:18,039 --> 00:21:21,559
of Reuben data, the sensitivity goes down to magnitude twenty

477
00:21:21,559 --> 00:21:24,799
seven point eight, which means in plain English, it means

478
00:21:25,000 --> 00:21:28,880
it can see things that are incredibly, unbelievably dim. Planet

479
00:21:28,960 --> 00:21:31,759
nine is expected to be about six hundred times fainter

480
00:21:31,839 --> 00:21:34,920
than Pluto. Reuben can see that, no problem, and.

481
00:21:34,839 --> 00:21:37,200
Speaker 2: We already have a proof of concept that the system works.

482
00:21:37,480 --> 00:21:39,160
From January of twenty twenty six.

483
00:21:39,279 --> 00:21:42,240
Speaker 1: Yes, the very first pure viewed paper to come out

484
00:21:42,279 --> 00:21:46,559
of the Reuben Observatory Science operations identified a new fast

485
00:21:46,599 --> 00:21:48,839
spinning asteroid called twenty twenty five.

486
00:21:49,319 --> 00:21:51,559
Speaker 2: M N forty five, So a different object.

487
00:21:51,720 --> 00:21:54,559
Speaker 1: Yes, that was much closer between Mars and Jupiter. But

488
00:21:54,640 --> 00:21:57,240
it proved the software works. It proved the automated system

489
00:21:57,279 --> 00:21:59,960
can isolate a single moving object from millions upon million

490
00:22:00,240 --> 00:22:01,200
of static stars.

491
00:22:01,400 --> 00:22:03,240
Speaker 2: So the trap is set, the camera.

492
00:22:03,039 --> 00:22:05,599
Speaker 1: Is rolling, the trap is set, the timeline is promising.

493
00:22:06,000 --> 00:22:07,799
If planet nine is where we think it is and

494
00:22:07,880 --> 00:22:10,119
as bright as we think it is, Ruben has a

495
00:22:10,240 --> 00:22:12,720
very strong chance of identifying it within the first one

496
00:22:12,720 --> 00:22:15,680
to two years of the survey. We're literally just waiting

497
00:22:15,680 --> 00:22:18,359
for the computer to ping. Now, in the spirit of

498
00:22:18,359 --> 00:22:20,279
good science, we have to look at the other side

499
00:22:20,279 --> 00:22:22,599
of the coin. Of course, is there any chance planet

500
00:22:22,680 --> 00:22:26,079
nine isn't a planet? What are the skeptics saying? Because

501
00:22:26,079 --> 00:22:28,400
I know there are some pretty wild alternative theories that

502
00:22:28,440 --> 00:22:29,960
don't involve a giant rock.

503
00:22:30,200 --> 00:22:35,000
Speaker 2: Absolutely, science requires us to challenge every hypothesis. You have

504
00:22:35,079 --> 00:22:36,559
to try to break the theory to see if it

505
00:22:36,599 --> 00:22:39,440
stands up. And there are three main alternatives on the

506
00:22:39,480 --> 00:22:40,119
table right now.

507
00:22:40,200 --> 00:22:43,799
Speaker 1: Okay, let's run through them. Theory A, the laws of

508
00:22:43,839 --> 00:22:44,960
gravity are wrong.

509
00:22:45,480 --> 00:22:48,559
Speaker 2: This is a concept known as m own ND modified

510
00:22:48,640 --> 00:22:53,039
Newtonian dynamics. The core idea is that at very very

511
00:22:53,079 --> 00:22:55,720
low accelerations, like what you'd experienced way out in the

512
00:22:55,759 --> 00:22:59,079
deep boonies of the Solar System, gravity just doesn't behave

513
00:22:59,119 --> 00:23:00,799
the way Newton ORNs Steins said it does.

514
00:23:01,119 --> 00:23:03,000
Speaker 1: So we don't need a new planet, we just need

515
00:23:03,119 --> 00:23:04,279
new math exactly.

516
00:23:04,720 --> 00:23:07,319
Speaker 2: A twenty twenty three study by researchers named Brown and

517
00:23:07,400 --> 00:23:11,279
Mother suggested that the Milky Way's own galactic gravitational field

518
00:23:11,519 --> 00:23:13,880
could be tugging on the outer Solar System in a

519
00:23:13,920 --> 00:23:16,440
subtle way that mimics the pull of a planet. They

520
00:23:16,480 --> 00:23:18,200
call it the external field effect.

521
00:23:18,400 --> 00:23:20,279
Speaker 1: So the ghost in the room is the whole galaxy.

522
00:23:20,440 --> 00:23:24,079
Speaker 2: It's a valid theory, but it requires rewriting fundamental physics,

523
00:23:24,720 --> 00:23:28,839
and generally in science we follow Oukham's razor. The simplest

524
00:23:28,880 --> 00:23:30,880
explanation is usually the best.

525
00:23:30,680 --> 00:23:33,279
Speaker 1: And a planet is simpler than new physics.

526
00:23:33,519 --> 00:23:36,640
Speaker 2: Planet nine just requires adding one more rock to the inventory.

527
00:23:37,279 --> 00:23:41,359
Monda requires changing the fundamental laws of the universe. Okham's

528
00:23:41,440 --> 00:23:43,319
razor usually favors the rock.

529
00:23:43,519 --> 00:23:47,160
Speaker 1: Fair enough, okay. Theory B. This one is my favorite.

530
00:23:47,519 --> 00:23:49,480
The primordial black hole.

531
00:23:49,880 --> 00:23:53,000
Speaker 2: This one is fun. It was proposed by Unwinded Schultz.

532
00:23:53,440 --> 00:23:55,839
They suggest that the mass out there isn't a planet

533
00:23:55,920 --> 00:23:58,680
at all, but a black hole the size of a grapefruit.

534
00:23:58,799 --> 00:24:02,160
Speaker 1: A grapefruit size black hole that just sounds terrifying.

535
00:24:02,319 --> 00:24:04,440
Speaker 2: It would have the same mass as five to ten Earth,

536
00:24:04,799 --> 00:24:07,279
but compressed it to a tiny, tiny point. It would

537
00:24:07,319 --> 00:24:10,119
explain the gravity perfectly, and it would also perfectly explain

538
00:24:10,200 --> 00:24:10,640
why we.

539
00:24:10,559 --> 00:24:13,240
Speaker 1: Can't see it because black holes don't emit or reflect

540
00:24:13,319 --> 00:24:13,799
any light.

541
00:24:13,920 --> 00:24:15,319
Speaker 2: It's the ultimate stealth object.

542
00:24:15,440 --> 00:24:16,559
Speaker 1: So could Ruben see that?

543
00:24:16,799 --> 00:24:20,839
Speaker 2: No, not directly. If this is true, the Ruben Observatory

544
00:24:20,839 --> 00:24:23,119
won't see it. You'd have to look for very subtle

545
00:24:23,119 --> 00:24:26,359
gravitational lensing events starlight bending around it as it passes

546
00:24:26,359 --> 00:24:28,319
in front. Would be a nightmare to find.

547
00:24:28,680 --> 00:24:32,519
Speaker 1: A fun nightmare though, and theory see.

548
00:24:32,599 --> 00:24:35,799
Speaker 2: The debris disc. This is the idea that instead of

549
00:24:35,799 --> 00:24:39,599
one big planet, it's a huge diffuse ring of millions

550
00:24:39,640 --> 00:24:43,440
of small icy rocks that all together collectively have the

551
00:24:43,440 --> 00:24:45,359
mass of ten earths.

552
00:24:45,039 --> 00:24:47,079
Speaker 1: So like a really heavy hula hoop at the edge

553
00:24:47,119 --> 00:24:48,480
of the Solar system pretty much.

554
00:24:49,000 --> 00:24:51,319
Speaker 2: But the main rebuttal there is heat. If you had

555
00:24:51,400 --> 00:24:53,680
that much dust and debris spread out over that much

556
00:24:53,680 --> 00:24:57,400
surface area, we would likely see the combined infrared glow

557
00:24:57,440 --> 00:25:00,640
from it. We don't see that. Also, use ring like

558
00:25:00,680 --> 00:25:03,880
that tends to be gravitationally unstable over billions of years.

559
00:25:04,200 --> 00:25:07,000
Speaker 1: So after weighing all the alternatives, planet nine is still

560
00:25:07,039 --> 00:25:07,720
the front runner.

561
00:25:07,920 --> 00:25:10,440
Speaker 2: It is still the simplest explanation that fits the most data,

562
00:25:10,839 --> 00:25:14,319
especially the orbital protection of those Neptune crossers. That five

563
00:25:14,359 --> 00:25:16,960
sigma result is very hard to explain with just modified

564
00:25:17,000 --> 00:25:20,400
gravity or a debris disc. Gravity from a single massive

565
00:25:20,480 --> 00:25:24,680
point source handles that shepherding resonance much more cleanly, So if.

566
00:25:24,599 --> 00:25:27,279
Speaker 1: It is there, this changes the map. We aren't just

567
00:25:27,319 --> 00:25:30,559
adding another dot to the chart. We are fundamentally redefining

568
00:25:30,599 --> 00:25:31,440
the Solar system.

569
00:25:31,599 --> 00:25:34,200
Speaker 2: We are proving the existence of what some astronomers are

570
00:25:34,200 --> 00:25:36,039
calling a third zone.

571
00:25:35,920 --> 00:25:38,200
Speaker 1: The third zone. I like the sound of that. What

572
00:25:38,240 --> 00:25:38,839
does that mean?

573
00:25:39,079 --> 00:25:41,519
Speaker 2: Well, we used to think the Solar system is pretty simple.

574
00:25:41,960 --> 00:25:44,920
You had Zone one, the inner rocky planets from Mercury

575
00:25:44,920 --> 00:25:47,680
to Mars. Then you had Zone two the gas and

576
00:25:47,759 --> 00:25:51,720
ized giants from Jupiter to Neptune and then the edge.

577
00:25:51,960 --> 00:25:54,079
Then we found the Kuiper Belt, which was sort of

578
00:25:54,119 --> 00:25:56,200
like the icy shoreline of the Solar.

579
00:25:55,920 --> 00:25:57,759
Speaker 1: System, and Planet nine changes that.

580
00:25:58,319 --> 00:26:02,640
Speaker 2: Planet nine implies a vast, deep third zone far beyond

581
00:26:02,680 --> 00:26:06,119
the giants, a region occupied by at least one massive

582
00:26:06,200 --> 00:26:09,519
world and maybe more. It tells us the Solar System

583
00:26:09,559 --> 00:26:11,920
doesn't just end it Neptune. It has a whole other chapter.

584
00:26:12,039 --> 00:26:14,799
Speaker 1: And this connects to the Nice model, right, the story

585
00:26:14,839 --> 00:26:17,000
of how our Solar system got here in the first place.

586
00:26:17,119 --> 00:26:19,680
Speaker 2: Exactly the Nice model, which is named after the city

587
00:26:19,680 --> 00:26:22,039
in France where it was developed, Not because it's just

588
00:26:22,079 --> 00:26:22,680
a nice.

589
00:26:22,480 --> 00:26:24,279
Speaker 1: Idea, although it is a nice idea.

590
00:26:24,359 --> 00:26:27,039
Speaker 2: It is a very nice idea. It describes the chaotic

591
00:26:27,240 --> 00:26:30,480
early days of the Solar System. The giant planets didn't

592
00:26:30,519 --> 00:26:33,519
form where they are now. They moved around, they migrated,

593
00:26:34,039 --> 00:26:37,640
and the simulation strongly suggest we didn't start with four giants.

594
00:26:37,920 --> 00:26:39,559
We likely started with five.

595
00:26:39,440 --> 00:26:40,319
Speaker 1: A lost sibling.

596
00:26:40,559 --> 00:26:46,039
Speaker 2: The lost sibling, the models showed Jupiter's immense gravity likely

597
00:26:46,079 --> 00:26:51,079
bullied this fifth giant planet, kicking it violently outward for

598
00:26:51,119 --> 00:26:53,319
a long time. The assumption was that it was ejected

599
00:26:53,319 --> 00:26:57,279
completely into interstellar space to become a rogue planet drifting

600
00:26:57,319 --> 00:26:58,519
alone between the stars.

601
00:26:58,799 --> 00:27:00,319
Speaker 1: But if Planet nine is the.

602
00:27:00,359 --> 00:27:02,359
Speaker 2: It's the one that got away but didn't actually leave.

603
00:27:02,440 --> 00:27:04,400
Speaker 1: It's just moved into the spare room exactly.

604
00:27:04,400 --> 00:27:06,119
Speaker 2: It didn't get kicked out of the house entirely. It

605
00:27:06,200 --> 00:27:08,720
just got pushed up into the attic. It's settled into

606
00:27:08,720 --> 00:27:14,240
this distant, lonely eccentric orbit. Finding it would be like

607
00:27:14,279 --> 00:27:16,880
finding a long lost brother of Jupiter and Neptune.

608
00:27:16,960 --> 00:27:19,079
Speaker 1: That is kind of poetic. It makes the Solar System

609
00:27:19,119 --> 00:27:21,519
feel like a family with the secret history we're just

610
00:27:21,559 --> 00:27:22,720
now uncovering, and it.

611
00:27:22,680 --> 00:27:25,640
Speaker 2: Confirms that our system is normal. If Plant nine is

612
00:27:25,640 --> 00:27:28,000
a super earth, we finally have the matching set. We

613
00:27:28,119 --> 00:27:29,680
finally fitted with the rest of the galaxy.

614
00:27:29,920 --> 00:27:32,039
Speaker 1: So where do we stand right now? We're in early

615
00:27:32,079 --> 00:27:34,599
twenty twenty six. What's the status.

616
00:27:34,640 --> 00:27:37,200
Speaker 2: We are in the final countdown. We're in the endgame.

617
00:27:37,759 --> 00:27:40,119
The search area in the sky has been narrowed down

618
00:27:40,160 --> 00:27:42,119
to less than ten percent of the predicted path.

619
00:27:42,240 --> 00:27:42,960
Speaker 1: That's huge.

620
00:27:43,240 --> 00:27:47,319
Speaker 2: The Ruben Observatory is scanning that very region night after night.

621
00:27:47,759 --> 00:27:50,920
The twenty twenty five archival candidate from the fan study

622
00:27:51,279 --> 00:27:53,359
is being rigorously re examined by.

623
00:27:53,279 --> 00:27:55,240
Speaker 1: Other teams, it really feels like we are right on

624
00:27:55,279 --> 00:27:57,039
the precipice of a major discovery.

625
00:27:57,599 --> 00:28:01,000
Speaker 2: I think detection is getting closer to being a logistical certainty.

626
00:28:01,599 --> 00:28:04,880
The conversation has shifted in the astronomical community. It's no

627
00:28:04,920 --> 00:28:08,279
longer is it there? It's where is it? And who

628
00:28:08,319 --> 00:28:09,440
is going to find it first?

629
00:28:09,759 --> 00:28:12,880
Speaker 1: And once we find it, what then? After the champagne

630
00:28:12,880 --> 00:28:14,519
and the headlines, what happens next?

631
00:28:14,720 --> 00:28:18,359
Speaker 2: We celebrate and then the real science begins. The moment

632
00:28:18,400 --> 00:28:21,240
we have a location, every major telescope on Earth will

633
00:28:21,279 --> 00:28:24,200
point at it. We can use spectroscopy to analyze the

634
00:28:24,240 --> 00:28:26,200
light coming from it, which will tell us what it's made.

635
00:28:26,079 --> 00:28:27,480
Speaker 1: Of, so we can know its composition.

636
00:28:27,759 --> 00:28:30,799
Speaker 2: Does it have a thick hydrogen atmosphere like Neptune? Is

637
00:28:30,839 --> 00:28:33,440
it a rocky world with a thin atmosphere? Does it

638
00:28:33,519 --> 00:28:36,759
have moons? We can start to answer those questions almost immediately.

639
00:28:36,839 --> 00:28:40,160
Speaker 1: Could we send a probe like Voyager or New Horizons?

640
00:28:40,359 --> 00:28:43,279
Speaker 2: We could, but you'd have to pack a lunch. It

641
00:28:43,319 --> 00:28:45,279
would take fifty years or more to get there with

642
00:28:45,319 --> 00:28:50,200
our current propulsion technology. But just knowing it's there it

643
00:28:50,240 --> 00:28:53,720
completes the picture. It changes how we view our place

644
00:28:53,720 --> 00:28:54,480
and the cosmos.

645
00:28:54,559 --> 00:28:57,079
Speaker 1: It's just incredible to think that right now, in twenty

646
00:28:57,119 --> 00:29:00,799
twenty six, we are still discovering may your pieces of

647
00:29:00,839 --> 00:29:02,319
geography in our own home.

648
00:29:02,680 --> 00:29:05,519
Speaker 2: Our home is bigger, weirder, and more crowded than we

649
00:29:05,599 --> 00:29:06,200
ever thought.

650
00:29:06,319 --> 00:29:08,559
Speaker 1: So here's the provocative thought I want to leave you

651
00:29:08,680 --> 00:29:12,960
the listener with. If Planet nine is a captured rogue planet,

652
00:29:13,519 --> 00:29:16,680
or if it's our solar system's lost sibling, what else

653
00:29:16,720 --> 00:29:18,519
is hiding out there in the third zone.

654
00:29:18,720 --> 00:29:21,640
Speaker 2: That's the question that keeps planetary scientists up at night.

655
00:29:21,960 --> 00:29:24,079
The universe rarely makes just one of anything.

656
00:29:24,160 --> 00:29:25,440
Speaker 1: Are we sure it's the only one?

657
00:29:25,839 --> 00:29:27,640
Speaker 2: Or is the darkness full of other ghosts we haven't

658
00:29:27,640 --> 00:29:28,240
even felt yet.

659
00:29:28,279 --> 00:29:30,119
Speaker 1: I love that, and I want to ask you directly

660
00:29:30,240 --> 00:29:32,359
if we find it, When we find it, what should

661
00:29:32,359 --> 00:29:34,759
we name it? The tradition is Roman and Greek gods.

662
00:29:34,799 --> 00:29:39,079
Who's left? Or do you prefer the grapefruit sized black

663
00:29:39,119 --> 00:29:42,200
hole theory? Because that is a movie waiting to happen.

664
00:29:42,519 --> 00:29:44,440
Speaker 2: I'm personally rooting for the planet. I want to see

665
00:29:44,480 --> 00:29:46,400
the picture on add it to the family portrait.

666
00:29:46,640 --> 00:29:48,880
Speaker 1: Me too. Let us know what you think in the

667
00:29:48,880 --> 00:29:52,920
comments below. This has been thrilling threads. Thanks for listening

668
00:29:52,920 --> 00:29:56,079
to us unravel the universe, Keep looking up, see next time.

