WEBVTT - Could Orbital Chaos Make the Planets Collide?

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<v Speaker 1>Welcome to Brainstuff, a production of iHeartRadio. Hey, brain Stuff,

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<v Speaker 1>Laurin Vogelbaum. Here, we all know that the planets of

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<v Speaker 1>the Solar System revolve around the Sun in a calm

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<v Speaker 1>and orderly fashion. In fact, the planets move with such

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<v Speaker 1>clockwork precision that astronomers can calculate orbital characteristics like eclipses

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<v Speaker 1>and planetary alignments with certainty. Want a list of solar

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<v Speaker 1>eclipses for the next ten thousand years, No problem. And

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<v Speaker 1>now let's say you want to look further into the future,

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<v Speaker 1>not thousands of years, but billions. How will those dusty

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<v Speaker 1>astronomical tables hold up? Then? Not so well if you

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<v Speaker 1>take into account the principles of chaos theory. A chaos

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<v Speaker 1>theory says that small inputs in an enormously complex system

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<v Speaker 1>can produce large scale outputs. This is what's sometimes called

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<v Speaker 1>the butterfly effect. The idea is that when a butterfly

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<v Speaker 1>flaps its wings in say Brazil, it could lead to

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<v Speaker 1>a chain reaction that causes a thunderstorm to develop over Australia.

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<v Speaker 1>Some scientists now propose that the evolution of the Solar

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<v Speaker 1>system may adhere to chaos theory, and that way way

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<v Speaker 1>way into the future. This could cause Earth to collide

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<v Speaker 1>with either Venus or Mars. A pair of scientists from

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<v Speaker 1>the Paris Observatory published a letter with this determination in

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<v Speaker 1>an issue of the journal Nature back in two thousand

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<v Speaker 1>and nine. For their research, they tapped into the power

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<v Speaker 1>of the Jade supercomputer, located at France's National Computing Center

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<v Speaker 1>for Higher Education and Research, which at the time was

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<v Speaker 1>around the twentieth most powerful computer in the world. So

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<v Speaker 1>what were they trying to calculate with that veritable muscle

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<v Speaker 1>car of computational capacity. It has to do with Isaac

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<v Speaker 1>Newton's universal law of gravitation, which states that gravity exists

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<v Speaker 1>between any to given objects. This gravitational force is directly

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<v Speaker 1>proportional to the object's masses and inversely proportional to the

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<v Speaker 1>square of the distance separating them, meaning that the more

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<v Speaker 1>massive an object is, the more gravity it will exert

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<v Speaker 1>on another object, but the further away an object is,

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<v Speaker 1>the less gravity it will exert on another object. A

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<v Speaker 1>Newton then proposed that the Sun's gravity is what holds

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<v Speaker 1>the planets in their orbits. But it's not that simple.

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<v Speaker 1>According to his own law, the planets and all of

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<v Speaker 1>the other objects in the Solar System, including moons and asteroids,

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<v Speaker 1>also exert at least a little gravity on each other.

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<v Speaker 1>So could the complex interplay of those forces cause the

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<v Speaker 1>stability of the Solar System to degrade over time in

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<v Speaker 1>the short term Nope. Even over longer periods, astronomers have

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<v Speaker 1>generally supported the idea that the Solar System would remain stable.

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<v Speaker 1>It just sort of makes sense. After all, the Sun

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<v Speaker 1>is overwhelmingly more massive than anything else in the Solar System.

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<v Speaker 1>Out of the Solar System's total mass, the Sun accounts

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<v Speaker 1>for ninety nine point eight percent of it. But a

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<v Speaker 1>few cosmologists began to wonder if chaos theory might apply

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<v Speaker 1>to planetary orbits. If so, small changes in planetary movements

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<v Speaker 1>could get magnified over time into something substantial. But how

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<v Speaker 1>long would it take? Thousands of years, millions billions? To

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<v Speaker 1>answer that question, you'd have to build a sort of

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<v Speaker 1>model to account for the movements of all of the planets,

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<v Speaker 1>as well as all of the forces being exerted as

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<v Speaker 1>that movement occurs. Then you'd need to let your Solar

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<v Speaker 1>system model run like a clock. So the planets cycled

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<v Speaker 1>through hundreds of thousands of orbits. As this occurred, you'd

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<v Speaker 1>need to track key data about each planet. One of

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<v Speaker 1>the most important pieces of data to collect would be

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<v Speaker 1>orbital eccentricity, which is a measure of how far a

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<v Speaker 1>planet deviates from a perfectly circular shape as it moves

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<v Speaker 1>around the Sun. Orbital eccentricity determines whether two planets might

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<v Speaker 1>come closer to having a close encounter. This is not

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<v Speaker 1>the kind of simulation you could run in your head

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<v Speaker 1>or with whatever fancy device you have at home, which

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<v Speaker 1>is why the researchers selected the Jade's supercomputer to do

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<v Speaker 1>their heavy lifting. Their inputs consisted of two five hundred

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<v Speaker 1>and one orbital scenarios, where each one altered Mercury's orbit

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<v Speaker 1>by just a few millimeters. They chose Mercury because, as

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<v Speaker 1>the runt of the Solar System, it's the biggest pushover,

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<v Speaker 1>and because its orbit synchronizes with jupiters to create changes

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<v Speaker 1>that ripple across the entire Solar System. For each hypothetical scenario,

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<v Speaker 1>they tracked the motion of all planets for more than

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<v Speaker 1>five billion years, which is the estimated life span of

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<v Speaker 1>the Sun. Even with the high powered CPU in the

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<v Speaker 1>Jade unit, each solution required four months of computing to

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<v Speaker 1>generate results. Luckily, for any future life on Earth, the

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<v Speaker 1>Solar System remained stable in ninety nine percent of the

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<v Speaker 1>researcher's scenarios. That is, no planets got set on collision

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<v Speaker 1>courses or ejected from their orbits. But in one percent

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<v Speaker 1>of their models, the ones in which the orbital chaos

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<v Speaker 1>had the greatest cumulative effect, Mercury's orbit became eccentric enough

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<v Speaker 1>to cause catastrophic changes in the Solar System. Some of

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<v Speaker 1>those catastrophes only involved Mercury, which could either crash into

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<v Speaker 1>the Sun or get dislodged from its orbit and flung

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<v Speaker 1>out into space, but other scenarios played out with Earth

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<v Speaker 1>colliding into either Mars or Venus. According to their models,

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<v Speaker 1>collision with Venus would occur through five steps, all of

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<v Speaker 1>which illustrate the cumulative effects orbital chaos. First, interaction between

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<v Speaker 1>Jupiter and Mercury about three point one three seven billion

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<v Speaker 1>years in the future, could cause the orbital eccentricity of

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<v Speaker 1>Mercury to increase. This would transfer some angular momentum from

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<v Speaker 1>the outer planets to the inner planets. This transfer would

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<v Speaker 1>destabilize the rest of the inner planets, so the orbital

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<v Speaker 1>eccentricities of Venus, Earth, and Mars would increase. This would

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<v Speaker 1>cause Earth to have a near miss with Mars, which

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<v Speaker 1>would disturb the eccentricity of Mars even more. This would

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<v Speaker 1>cause some weird reinforcing interactions among the inner planets to

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<v Speaker 1>decrease the eccentricity of Mercury but further increase the eccentricities

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<v Speaker 1>of Venus and Earth. Venus and Earth would have several

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<v Speaker 1>near misses until at three point three five two eight

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<v Speaker 1>nine one billion years in the future, the two planets

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<v Speaker 1>collided in an epic explosion that would destroy both worlds. Again.

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<v Speaker 1>In ninety nine percent of their simulations, everything was fine

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<v Speaker 1>until the Sun died. Of course, none of these models

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<v Speaker 1>may be accurate at all. First of all, we're still

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<v Speaker 1>discovering new bodies around our Solar System like asteroids, moons,

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<v Speaker 1>and comets all the time, and relatedly, they could make

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<v Speaker 1>more of a difference than the researchers originally accounted for.

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<v Speaker 1>In a follow up study of the same scientists along

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<v Speaker 1>with a larger team, looked at interactions between some of

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<v Speaker 1>the large bodies in the belt between Mars and Jupiter,

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<v Speaker 1>including the dwarf planet Series and major asteroids like Palace

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<v Speaker 1>and Vesta. They then extrapolated out what those interactions would

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<v Speaker 1>mean for the planets. What they concluded was that the

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<v Speaker 1>chaotic interactions between Series and Vesta specifically, should quickly amplify

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<v Speaker 1>even the tiniest of measurement errors, making it impossible to

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<v Speaker 1>predict what planetary orbits should look like based on the

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<v Speaker 1>current information beyond just sixty million years into the future

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<v Speaker 1>or into the past. Basically, all of this means that

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<v Speaker 1>the Solar System is filled with lots of stuff, and

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<v Speaker 1>even though it's pretty spread out, all of these objects

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<v Speaker 1>exert gravitational force on one another, and these forces can

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<v Speaker 1>change planetary orbits a lot, even if we can't measure

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<v Speaker 1>those changes very accurately. In fact, astronomers have evidence of

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<v Speaker 1>other Solar systems self destructing. In two thousand and eight,

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<v Speaker 1>a team from the Harvard Smithsonian Center for Astrophysics spotted

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<v Speaker 1>a Saturn sized planet orbiting a star in the constellation

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<v Speaker 1>Centaurus that was giving off way too much heat for

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<v Speaker 1>its planetary size. The scientists believe that the planet is

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<v Speaker 1>radiating massive amounts of heat because of a collision with

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<v Speaker 1>a Urinous sized Protoplanet in the astronomically recent past, and

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<v Speaker 1>in two thousand and nine, NASA's Spitzer space telescope spotted

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<v Speaker 1>the aftermath of a mash up between an object the

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<v Speaker 1>size of our moon and another the size of mercury,

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<v Speaker 1>about one hundred light years away in the constellation Pavo.

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<v Speaker 1>The peacock instruments on Spitzer detected the teltale signatures of

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<v Speaker 1>amorphous silica, a substance that forms on Earth when meteorites

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<v Speaker 1>slam into the ground. Of course, even if our solar

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<v Speaker 1>system doesn't succumb to orbital chaos and a Billiard like

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<v Speaker 1>crashing of the inner planets, stars don't last forever. In

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<v Speaker 1>about five billion years, when the Sun exhausts fuel supply,

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<v Speaker 1>all of the inner planets will disappear into the belly

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<v Speaker 1>of our rapidly expanding star. Either way, chaos induced collision

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<v Speaker 1>or stellar death, our tiny blue world won't go out

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<v Speaker 1>with a whimper, but with a bang. Today's episode a

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<v Speaker 1>space the article will orbital chaos cause Earth, Venus, and

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<v Speaker 1>Mars to collide On HowStuffWorks dot com written by William Harris.

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<v Speaker 1>Rain Stuff is production of iHeartRadio in partnership with HowStuffWorks

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<v Speaker 1>dot com and it is produced by Tyler Klang. Four

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