WEBVTT - What If Earth Had Rings?

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<v Speaker 1>Welcome to BrainStuff, a production of iHeartRadio. Hey BrainStuff, Lauren

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<v Speaker 1>Vogelbaum here. Earth's moon feels like an ever-present feature in

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<v Speaker 1>our skies, even if it's really only visible from any

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<v Speaker 1>given point on Earth about half the time. But what

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<v Speaker 1>if you looked skyward and saw not a moon, but

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<v Speaker 1>a ring, much like the ones that encircle our solar

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<v Speaker 1>system's gas giants? Saturn in particular is known for its

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<v Speaker 1>brilliant ring system, the most extensive we know of. But Jupiter, Uranus,

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<v Speaker 1>and Neptune have rings too. Today, let's talk about planetary rings,

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<v Speaker 1>and what it would be like if Earth boasted its own.

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<v Speaker 1>Scientists believe Earth did have a ring once, albeit a

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<v Speaker 1>few billion years ago. This ring would have appeared early

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<v Speaker 1>in the formation of Earth's moon. Our best hypothesis for

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<v Speaker 1>how the moon formed is what's called the giant impact hypothesis.

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<v Speaker 1>The idea is that about four and a half billion

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<v Speaker 1>years ago, while the Earth itself was still forming, a

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<v Speaker 1>large object or fellow proto-planet about the size of Mars

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<v Speaker 1>hit Earth at an angle. The impact threw debris into

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<v Speaker 1>space from Earth's crust and mantle. The impactor itself, which

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<v Speaker 1>we've named Theia, melted and merged with Earth's interior. Meanwhile,

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<v Speaker 1>some of the hot debris got caught in Earth's orbit

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<v Speaker 1>and eventually cooled and coalesced to form the moon. The

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<v Speaker 1>giant impact hypothesis would explain why moon rocks have a

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<v Speaker 1>composition similar to Earth's mantle and why they seem to

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<v Speaker 1>have been baked, and why the moon has no iron core,

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<v Speaker 1>because the iron in Earth's core and Theia's core remained

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<v Speaker 1>on Earth. But while the moon was coming together... all

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<v Speaker 1>of that debris would have been hovering in a ring

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<v Speaker 1>in Earth's orbit. Now, planetary rings are temporary structures. We

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<v Speaker 1>talked about this a while ago on the show, when,

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<v Speaker 1>back in 2018, researchers found that Saturn's glorious rings have

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<v Speaker 1>only been around for about 100 million years, and that

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<v Speaker 1>they'll be gone, having fallen into the gassy planet, and

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<v Speaker 1>100 million more. So, no matter what, this early ring

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<v Speaker 1>of Earth's wouldn't have lasted until today. But the reason

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<v Speaker 1>that this debris became a moon and not a ring

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<v Speaker 1>is that it existed outside of what's called the Roche limit.

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<v Speaker 1>The Roche limit is named for the French mathematician Edouard Roche, who,

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<v Speaker 1>in 1848, figured out that any given planet's gravitational pull

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<v Speaker 1>on a moon will be unequal across the surface of

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<v Speaker 1>that moon. That a planet exerts a greater gravitational force

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<v Speaker 1>on the side of the moon closest to the planet.

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<v Speaker 1>and a lesser gravitational force on the side facing away.

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<v Speaker 1>This means that if a moon or other object that

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<v Speaker 1>wanders into a planet's orbit is too close to the planet,

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<v Speaker 1>the unequal pull of the planet's gravity could tear it apart. Essentially,

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<v Speaker 1>the Roche limit is the minimum distance an object can

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<v Speaker 1>be from a planet and still hold itself together by

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<v Speaker 1>its own gravity. Inside the Roche Limit, any debris from

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<v Speaker 1>a giant impact, or any object that the planet attracts

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<v Speaker 1>with its gravitational pull, say smaller moons or asteroids, will

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<v Speaker 1>get torn apart again and again, eventually ground down to water, ice,

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<v Speaker 1>and dust particles, traveling along the planet's gravitational orbit like

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<v Speaker 1>water running down a drain, very slowly. Researchers estimate that

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<v Speaker 1>around Saturn, Ring material, to the amount of some 10

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<v Speaker 1>tons or 9,000 kilos, is falling into the planet every second.

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<v Speaker 1>Part of why our gas giants all have rings, but

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<v Speaker 1>our rocky inner planets don't, is that the outer planets

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<v Speaker 1>have masses large enough to attract ring material, and they

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<v Speaker 1>orbit far away enough from the sun for water ice

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<v Speaker 1>to stay frozen. Part of how we figured out that

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<v Speaker 1>Saturn's rings are so young is that they're predominantly made

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<v Speaker 1>of ice. If they were older, that ice would have

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<v Speaker 1>gotten contaminated over time with interplanetary debris, making them dull.

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<v Speaker 1>But they're still beautifully bright. Saturn has seven main rings,

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<v Speaker 1>each composed of thousands of tiny ringlets. They're massively wide,

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<v Speaker 1>extending up to 175,000 miles, or 280,000 kilometers, out into space.

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<v Speaker 1>But they're proportionally very thin, only about 30 feet or

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<v Speaker 1>10 meters thick. ranging up to a little over half

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<v Speaker 1>a mile or a kilometer at the thickest. They're made

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<v Speaker 1>up of chunks of water ice, rock, and other materials,

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<v Speaker 1>varying in size from specks to enormous house-sized pieces that

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<v Speaker 1>collide constantly, shattering the larger chunks. Scientists think the rings

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<v Speaker 1>formed when comets or asteroids collided with one or more

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<v Speaker 1>of the planet's moons. The fragments from the collisions spread

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<v Speaker 1>out around Saturn within the Roche limit. Saturn's two innermost

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<v Speaker 1>rings are very transparent. The next two out are the

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<v Speaker 1>brightest and largest. The fifth ring is very narrow and

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<v Speaker 1>held together by two moons, Pandora and Prometheus, that sit

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<v Speaker 1>on either side of the ring. The final two are

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<v Speaker 1>farther out, with the farthest made up of near-microscopic ice particles,

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<v Speaker 1>thought to have been ejected from the moon Enceladus, sprayed

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<v Speaker 1>out of volcanic geysers near its south pole. Saturn's rings

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<v Speaker 1>are named after the first seven letters of the alphabet,

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<v Speaker 1>in the order that they were discovered. So, from innermost

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<v Speaker 1>to outermost, that's D, C, B, A, F, G, and E.

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<v Speaker 1>The rings aren't perfect circles, but instead have bends in

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<v Speaker 1>them caused by the pull of gravity from nearby moons.

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<v Speaker 1>There's also a mysterious phenomenon among the rings, referred to

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<v Speaker 1>as spokes. These are features that rotate along with the rings,

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<v Speaker 1>but appear and disappear in ways that we haven't entirely

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<v Speaker 1>been able to explain yet. They look like spokes on

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<v Speaker 1>the wheels of the rings, and researchers think that they

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<v Speaker 1>may be formed by seasonal interactions between solar wind and

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<v Speaker 1>Saturn's magnetic field, creating some kind of static electricity that

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<v Speaker 1>pulls fine dust particles into different shapes. Saturn's rings are

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<v Speaker 1>bright enough that Galileo observed them way back in 1610,

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<v Speaker 1>though he didn't know what he was looking at. Their

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<v Speaker 1>extension from the sides of Saturn reminded him of ears,

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<v Speaker 1>and he wrote about them being two smaller stars, or

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<v Speaker 1>perhaps two large moons. It wasn't until 1655 that Dutch

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<v Speaker 1>scientist Christian Huygens identified them as rings. The other gas giants'

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<v Speaker 1>rings went undetected for over 300 years. Uranuses were the

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<v Speaker 1>first to be discovered in 1977. They run parallel to

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<v Speaker 1>its tilted equator, which is nearly at a right angle

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<v Speaker 1>to its orbit, so the rings appear to go up

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<v Speaker 1>and over the planet. It has two sets, nine inner

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<v Speaker 1>rings that are narrow and gray, and then two outer rings,

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<v Speaker 1>one reddish and one blue. Jupiter's rings weren't discovered until

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<v Speaker 1>Voyager 1's initial flyby in 1979. They're very faint. and

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<v Speaker 1>they're thought to have been created by meteoroid impacts on

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<v Speaker 1>small nearby moons. They have four components, an inner halo

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<v Speaker 1>of dust, a bright, thin main ring, and then two wide,

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<v Speaker 1>dim outer rings called the gossamer rings. Neptune's rings weren't

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<v Speaker 1>definitively detected until 1989, when Voyager 2 captured images of

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<v Speaker 1>them on its flyby. It has five main rings and

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<v Speaker 1>four prominent ring arcs, which are smaller rings that are

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<v Speaker 1>formed by faint, thin collections of micrometer-sized dust that's shepherded

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<v Speaker 1>around the ring system by Neptune's four small moons. But

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<v Speaker 1>back to Earth. It's unlikely that our planet will form

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<v Speaker 1>its own ring system anytime soon. In order to break

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<v Speaker 1>apart properly, an asteroid or a bunch of space rubble

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<v Speaker 1>would need to enter our orbit at around 9,000 kilometers,

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<v Speaker 1>which is in low-to-mid-medium Earth orbit. But what would it

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<v Speaker 1>be like if Earth did have rings? Okay, any rings

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<v Speaker 1>would most likely form parallel to the equator, and thus

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<v Speaker 1>would arc across the sky from east to west. And

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<v Speaker 1>your view of them would depend on your latitude away

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<v Speaker 1>from the equator. Near the equator, the rings would be

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<v Speaker 1>like thin slices of light erupting from the distant horizons

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<v Speaker 1>and stretching up into the sky as far as the

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<v Speaker 1>eye could see. The farther north or south you were,

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<v Speaker 1>the more the appearance of the rings would change. They'd

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<v Speaker 1>become markedly wider and more visible, and would, from some

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<v Speaker 1>vantage points, appear close enough to the horizon to reach

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<v Speaker 1>out and touch. Just as the moon currently does, the

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<v Speaker 1>rings would reflect sunlight back to Earth and appear to glow,

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<v Speaker 1>especially at night. Depending on exactly what they were made of,

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<v Speaker 1>the rings could reflect so much sunlight that the planet

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<v Speaker 1>would never fully plunge into darkness, but remain in a

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<v Speaker 1>gentle twilight, even in the depth of night. Even daylight

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<v Speaker 1>might be brighter because of them. Rings around Earth would

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<v Speaker 1>have significant climatic implications. These vast sheets of debris could

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<v Speaker 1>act as a shield in some regions, potentially preventing some

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<v Speaker 1>of the sun's rays from reaching Earth's surface. This could

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<v Speaker 1>lead to cooler temperatures in some areas, especially those beneath

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<v Speaker 1>the densest parts of the ring. Conversely, the reflected sunlight

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<v Speaker 1>from the rings could cause a warming effect in other regions.

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<v Speaker 1>Climate models would need to account for these new variables,

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<v Speaker 1>making our understanding of global weather patterns even more complex.

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<v Speaker 1>Planetary rings would also pose challenges to our current satellite infrastructure.

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<v Speaker 1>After all, we have stuff in our medium Earth orbit.

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<v Speaker 1>Just a bit farther out than a ring would sit,

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<v Speaker 1>we've placed a lot of telecommunications and GPS equipment, and

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<v Speaker 1>above that, a lot of weather platforms. rings could interfere

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<v Speaker 1>with the trajectories of nearby platforms or with communication from

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<v Speaker 1>the ground to anything orbiting above them. The presence of

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<v Speaker 1>a dense ring could also present navigational hazards for space

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<v Speaker 1>missions leaving or entering Earth's atmosphere. If material from the

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<v Speaker 1>rings should rain down onto the planet the way that

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<v Speaker 1>Saturn's ring material does, it could also pose a hazard

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<v Speaker 1>to the equipment in low Earth orbit, like the International

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<v Speaker 1>Space Station. Space agencies and other satellite constructors would need

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<v Speaker 1>to recalibrate and perhaps even redesign spacecraft to safely navigate

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<v Speaker 1>in or through such an environment. On the flip side,

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<v Speaker 1>falling ring material might create some spectacular meteor showers. And

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<v Speaker 1>just think of all the new sayings we'd have to

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<v Speaker 1>come up with. Perhaps we'd no longer shoot for the moon,

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<v Speaker 1>but aim for the rings instead. It's not completely out

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<v Speaker 1>of the realm of possibility. We're still learning about planetary rings.

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<v Speaker 1>Just in 2023, an international team of astronomers published a

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<v Speaker 1>study in the journal Nature about a new ring system

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<v Speaker 1>they discovered in the far reaches of our solar system.

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<v Speaker 1>The rings are around Quawar, a dwarf planet that's about

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<v Speaker 1>as wide as Texas and orbits beyond Neptune. The rings

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<v Speaker 1>are too faint to see directly from Earth, the team

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<v Speaker 1>discovered them by observing an oculation, meaning that they watched

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<v Speaker 1>the light from a background star, as Quawar blocked it

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<v Speaker 1>by passing between us and the star during its orbit.

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<v Speaker 1>What makes this ring system especially interesting is that it's

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<v Speaker 1>twice as far out from the surface of the dwarf

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<v Speaker 1>planet as scientists previously thought was possible according to the

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<v Speaker 1>Roche limit. So who knows? Maybe rings are in Earth's

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<v Speaker 1>future after all. Today's episode is based on the articles

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<v Speaker 1>Does Earth Have Rings? by Laurie L. Dove and The

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<v Speaker 1>Four Planets with Rings Might Surprise You by Mitch Ryan,

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<v Speaker 1>both on HowStuffWorks.com. BrainStuff is a production of iHeartRadio in

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<v Speaker 1>partnership with HowStuffWorks.com and is produced by Tyler Klang. For

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<v Speaker 1>more shows from iHeart Podcasts, visit the iHeartRadio app, Apple Podcasts,

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<v Speaker 1>or wherever you listen to your favorite shows.