Nov. 24, 2025
Hawking's Triumph, Balloon Telescopes, and a Tilted Exoplanet
- Hawking and Einstein Confirmed: In a groundbreaking cosmic event, the collision of two black holes has validated predictions made by both Stephen Hawking and Albert Einstein. Observations from gravitational wave observatories confirmed Hawking's area theorem, showing that the surface area of the resulting black hole increased, and matched Einstein's predictions regarding the black hole's ring down, revealing a new Kerr black hole.
- Moss Survives in Space: Astonishingly, moss spores exposed to the harsh conditions of space on the International Space Station for nine months were able to germinate upon their return to Earth. This remarkable resilience of extremophiles supports theories like panspermia, suggesting that life's building blocks could survive interplanetary journeys.
- Balloon-Based Astronomy: The Excalibur mission is revolutionizing observational astronomy by utilizing a telescope suspended from a high-altitude balloon. Operating above 99% of Earth's atmosphere, it measures high-energy X-ray polarization from cosmic objects like the Crab Nebula and Cygnus X1, providing unprecedented insights into their magnetic fields and structures.
- Mystery of the Misaligned Exoplanet: Astronomers are puzzled by TOI 3884, a super Neptune with a bizarrely tilted orbit of 62 degrees. Lacking any nearby massive objects to explain its unusual trajectory, scientists are left with unconventional theories about its formation, highlighting the chaotic nature of planetary systems.
- Is the Universe Infinite? The question of whether the universe is infinite remains unresolved. While measurements of the cosmic microwave background suggest a flat geometry, which implies infinity, our observable horizon limits our ability to confirm this. The potential for a finite universe with complex topology adds further complexity to this profound inquiry.
- For more cosmic updates, visit our website at astronomydaily.io. Join our community on social media by searching for #AstroDailyPod on Facebook, X, YouTubeMusic, TikTok, and our new Instagram account! Don’t forget to subscribe to the podcast on Apple Podcasts, Spotify, iHeartRadio, or wherever you get your podcasts.
- Thank you for tuning in. This is Anna and Avery signing off. Until next time, keep looking up and exploring the wonders of our universe.
Black Hole Collision Insights
[NASA](https://www.nasa.gov/)
Moss in Space Study
[International Space Station](https://www.nasa.gov/mission_pages/station/main/index.html)
Excalibur Mission Overview
[NASA](https://www.nasa.gov/)
TOI 3884 Exoplanet Research
[NASA Exoplanet Archive](https://exoplanetarchive.ipac.caltech.edu/)
Cosmic Microwave Background Studies
[NASA](https://www.nasa.gov/)
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This episode includes AI-generated content.
WEBVTT
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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.
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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.