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Avery: Hello, and ah, welcome to Astronomy Daily,

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the podcast that brings the cosmos down to

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Earth. I'm Avery, and as always, I'm

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here with the brilliant Anna.

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Anna: Hello, Avery, and hello to all our

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listeners. We have a fascinating lineup today

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covering everything from cosmic giants

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to microscopic survivors.

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Avery: That's right. We'll be talking about a major

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confirmation of a Stephen Hawking theory.

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Moths that survived the vacuum of space.

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A telescope on a balloon. A planet that's

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orbiting completely off kilter. And we'll end

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by tackling one of the biggest questions out

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there. Is the universe infinite?

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Anna: It's a packed episode.

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Shall we start with the giants?

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Avery: Let's do it. Our first story is a big

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one. Two of the greatest minds in physics,

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Stephen Hawking and Albert Einstein,

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both had some of their most fundamental

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predictions confirmed by a single cosmic

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event.

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Anna: This involves the collision of two black

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holes. Using gravitational wave

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observatories, scientists got their clearest

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observation yet of such a merger.

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Avery: And the first big confirmation relates to

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Hawking's area theorem. Um, he predicted that

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the surface area of a black hole, its event

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horizon can never, ever shrink. It

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can only stay the same or grow.

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Anna: Right. It's a law of black hole mechanics.

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And in this merger, they measured the surface

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area of the two original black holes and

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compared it to the new, larger one that

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formed.

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Avery: And?

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Anna: And the new surface area was indeed

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greater than the sum of the two initial ones.

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Hawking was right.

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Avery: It's just incredible to see a theoretical

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prediction made decades ago proven so

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precisely. But that wasn't all they saw, was

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it?

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Anna: No, it wasn't. The signal was so

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clear that they could observe the ring down

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of the new black hole. Think of it like

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striking a bell.

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Avery: Mhm. The ringing.

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Anna: Exactly. The new black hole wobbled

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and settled into its final shape, sending out

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gravitational waves that faded over time,

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just like the sound of a bell. The specific

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frequencies and decay patterns of that ring

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down matched the predictions of Einstein's

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general theory of relativity perhaps

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perfectly.

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Avery: So in one event, we get a check mark for

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Hawking and a check mark for Einstein.

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And this new object they observed is called a

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Kerr black hole, right?

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Anna: That's correct. A Kerr black hole is one that

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is rotating. Since the two smaller black

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holes were spiraling around each other, the

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resulting merged black hole inherited that

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spin. It's the type of black hole we expect

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to be common in the universe.

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Avery: Wow. What a powerful confirmation of our

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understanding of gravity and the universe.

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From the colossal to the well to the very,

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very small.

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Our next story is almost the polar opposite.

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Anna: It really is. This story comes from

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the International Space Station, but it's not

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about the astronauts inside. It's about

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something that was living on the outside.

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Avery: On the outside? Fully exposed to space.

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Anna: Fully exposed. Scientists placed moss

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spores in a container on an external platform

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of the iss. For nine months, these

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spores endured the vacuum of space,

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extreme temperature swings, and the full

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force of cosmic radiation.

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Avery: That sounds like a recipe for total

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destruction. I can't imagine anything

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surviving that.

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Anna: That's what makes this so astonishing. When

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they brought the spores back to Earth, a high

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percentage of them were still able to

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germinate and grow.

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Avery: No way. They just started growing

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again after nine.

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Anna: Months in raw space as if nothing had

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happened. It speaks to the incredible

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resilience of life. Organisms like

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this, known as extremophiles, really

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push the boundaries of what we thought was

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possible.

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Avery: This has huge implications for theories like

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panspermia, doesn't it? The idea that life

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could travel between planets on asteroids or

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comets.

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Anna: It certainly makes it seem more plausible. If

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simple spores can survive the harshness of

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space for extended periods, it suggests

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that the building blocks of life might be

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tougher and more widespread than we ever

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imagined.

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Avery: From survivors in space to a new way of

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seeing in space.

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Our next story involves a very unusual

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observatory. We're not talking about a

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mountaintop or a satellite, but a telescope

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dangling from a giant balloon.

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Anna: This is the Excalibur mission. And while a

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balloon might sound low tech, it's actually

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an incredibly clever way to do astronomy.

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Avery: It carries a telescope up to about

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130,000ft, which is above

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99% of Earth's atmosphere. This

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gives it a much clearer view, especially for

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the kind of light it's designed to see. High

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energy X rays.

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Anna: Mm X rays that are blocked by our

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atmosphere. And Excalibur isn't just taking

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pictures. Its key function is to measure

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the polarization of these X rays.

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Avery: Can you break that down for us? What does

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measuring polarization actually tell?

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Anna: You think of light as a wave.

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Usually those waves are oriented randomly.

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Polarization is like filtering the light, so

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you only see waves oriented in a specific

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direction. For astronomers, the. The way X

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rays are polarized tells them about the

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powerful and complex magnetic fields

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near their source.

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Avery: So it's a way to map out invisible

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magnetic structures. And they pointed this

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thing at some pretty famous cosmic objects,

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right?

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Anna: They did. The mission focused on two

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main the Crab Nebula, which is the

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remnant of a supernova, and Cygnus

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X1, a famous system containing a

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black hole that's feeding off a companion

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star.

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Avery: And by measuring the X ray polarization.

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They are getting new insights into the

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physics of the neutron star powering the Crab

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Nebula and the geometry of the material

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swirling into the black hole in Cygnus X1.

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It's a whole new layer of information.

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Anna: It really is. Balloon based

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astronomy provides a fantastic, cost

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effective way to get above the atmosphere and

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test new technologies.

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Okay, from new views to new mysteries,

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our next story presents a real puzzle.

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Avery: Yeah, this one is a head scratcher.

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Astronomers have found an exoplanet system

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named TOI 3884

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where things just don't add up.

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Anna: The planet itself is a super

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neptune, larger than Neptune, but smaller

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than Saturn. It orbits its star quite

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closely. But that's not the strange part. The

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strangeness lies in its orbit.

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Avery: It's wildly tilted. Most planets

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in a solar system form in a flat disk,

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so they tend to orbit in the same plane

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aligned with the star's equator. This

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one is misaligned by about

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62 degrees. It's orbiting on

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a crazy diagonal path.

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Anna: Right. A 62 degree tilt is

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extreme. Usually to get an orbit that

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tilted, you need a powerful gravitational

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nudge from m, another massive object in the

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system. Like a giant planet farther out

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or a, uh, companion star.

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Avery: And the mystery is there isn't one.

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Scientists have looked and they can't find

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anything massive enough nearby to explain

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how this planet got knocked so far off

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kilter.

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Anna: Precisely. The usual suspects are all

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missing. It leaves them with some

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unconventional theories. Perhaps the

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stars protoplanetary disk was tilted

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from the very beginning by a passing star

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early in its history. Or maybe there was

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another planet that knocked this one aside

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and then got ejected from the system

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entirely.

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Avery: A, uh, cosmic hit and run.

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Anna: Exactly.

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Avery: And that theory of an ejected planet, A, uh,

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cosmic hit and run. Why is that

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so difficult to prove?

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Anna: Because the getaway car is long gone

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and completely invisible. A planet

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ejected from its solar system would become a

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rogue planet, drifting cold and dark through

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interstellar space. There's no star to light

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it up. So finding it, let alone tracing

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it back to its home system, is practically

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impossible with our current technology.

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Avery: So scientists have a pretty big mystery.

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Anna: On their hands, essentially.

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For now, it's an open case file.

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It's a reminder that planet formation is a

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chaotic and complex process. And

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our own solar system systems neat alignment

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might be less common than we think.

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Avery: Speaking of things being less common than we

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think, our final story tackles maybe the

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biggest astronomical question of Is

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the universe infinite?

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Anna: It's a question that feels almost

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philosophical, but scientists are trying

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to answer it with actual measurements.

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The Key lies in determining the overall

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shape or geometry of the universe.

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Avery: And their best tool for that is the cosmic

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microwave background, or cmb.

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That's the leftover heat from the Big Bang,

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which fills all of space.

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Anna: Correct. By studying the tiny

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temperature fluctuations in the cmb,

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cosmologists can measure the universe's

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geometry. There are three basic

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possibilities. It could be closed,

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like the surface of a sphere, open

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like the surface of a saddle, or flat,

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like a sheet of paper.

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Avery: And so far, every measurement we've made

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points to one answer.

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Anna: Flat to within a very small

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margin of error. The universe appears to be

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geometrically flat. If the

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universe is truly flat, then in

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principle, it would extend infinitely in

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all directions.

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Avery: Case closed, then, the universe is infinite.

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Anna: Not quite. Here's the catch.

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We are limited by our observable

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horizon. We can only see the part of

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the universe from which light has had time to

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reach us since the Big Bang.

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Avery: The mind just reels at that. If it's truly

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infinite, that means that somewhere out

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there, an infinite distance away, there's

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another solar system exactly like ours, with

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another Earth and, and another you and I

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having this exact same conversation.

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Anna: That's the logical, if unsettling,

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conclusion. With an infinite number of

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chances, any event with a non zero

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probability must occur an infinite

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number of times. It pushes the boundaries

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of physics into the realm of philosophy.

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Avery: Oh, okay, so it's like standing in Kansas. It

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looks perfectly flat as far as you can see.

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But you know that on a large enough scale,

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the Earth is cur.

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Anna: That's a perfect analogy. The universe could

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be curved on a scale much, much

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larger than our observable horizon. It

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could be a steer or a saddle so vast

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that our little patch of it just looks flat.

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Avery: And there's another wrinkle, too, isn't

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there? The idea of topology.

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Anna: Yes. Even a flat universe

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might not be infinite. It could have a

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complex topology. For example, it could

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be shaped like a donut. If you travel in a

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straight line, you eventually end up back

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where you started. In that case, the universe

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would be flat but finite.

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Avery: Have scientists looked for evidence of that

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donut shape? For instance, by looking for

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repeating patterns in the cosmic microwave

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background, as if we were seeing the same

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region of space from different directions.

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Anna: They have, very carefully. So

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far, no such repeating patterns have been

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found. While this doesn't rule out a, uh,

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finite universe, it does mean that if

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the universe is finite, it must be

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vastly larger than the part we can see.

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So for all practical purposes, it might

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as well be infinite from our perspective.

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Avery: So in the end we're left without a definitive

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answer. Our measurements say flat, which

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points towards infinite, but we can't be sure

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exactly.

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Anna: It's possible that because of the horizon

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problem, this is a question we may never

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be able to answer for certain. It's one of

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the profound limits of cosmology.

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Avery: And what a profound place to end our journey

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today. From the laws of black holes to the

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hardiness of moss, from balloon telescopes to

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tilted worlds, and finally to the ultimate

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fate and size of the universe itself.

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Anna: It really shows you the incredible range of

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questions that astronomy seeks to answer.

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Thank you all for joining us on, um, this

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exploration.

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Avery: That's all for this episode of Astronomy

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Daily. You can find us wherever you get your

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podcasts. And we'll be back next time with

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more news from across the universe. Until

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then, I'm Avery.

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Anna: And I'm Anna. Keep looking up.
