WEBVTT - How Does Planet Mercury Work?

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<v Speaker 1>Welcome to brain Stuff production of I Heart Radio. Hey

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<v Speaker 1>brain Stuff, Lauren Bogelbaum. Here. You'd like to think you

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<v Speaker 1>know your neighbors, but sometimes they'll catch you off guard.

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<v Speaker 1>That diminutive world called Mercury is the first planet from

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<v Speaker 1>our Sun, Venus's second, Earth is the third, and dear

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<v Speaker 1>old Mars is number four common knowledge, but that numbering

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<v Speaker 1>obscures certain truths. With its tight orbit around the Sun,

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<v Speaker 1>Mercury can't ventures far away from Earth as Venus and

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<v Speaker 1>Mars can during their larger orbits, so most of the time,

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<v Speaker 1>Mercury is closer to Earth than any other planet, despite

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<v Speaker 1>its place in the planetary lineup. And that's far from

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<v Speaker 1>the weirdest thing about Mercury's travel patterns. Of all the

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<v Speaker 1>planets in the Solar System, Mercury orbits our Sun at

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<v Speaker 1>the fastest rate. It zips around our star with an

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<v Speaker 1>average speed of around one hundred and five thousand, nine

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<v Speaker 1>hundred miles per hour or a hundred and seventy thousand,

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<v Speaker 1>five hundred kilometers per hour. The planet's namesake was a

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<v Speaker 1>real speedster too. In Roman mythology, Mercury was the fleet

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<v Speaker 1>footed god of commerce and communication, among other things. Recognizable

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<v Speaker 1>by his winged sandals. Earth takes a little more than

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<v Speaker 1>three hundred and sixty five days to loop around the sun.

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<v Speaker 1>Mercury does the same thing in a fraction of the time.

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<v Speaker 1>One Mercury in year is equal to a brisk eighty

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<v Speaker 1>eight earth days vacationing there would be a disorienting experience

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<v Speaker 1>on Mercury. The years may be quick, but the days

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<v Speaker 1>are very long. The planet finishes a new rotation around

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<v Speaker 1>its own axis once every fifty nine earth days, which

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<v Speaker 1>means that every day on Mercury takes up almost exactly

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<v Speaker 1>two thirds of every year. But due to some further strangeness,

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<v Speaker 1>each day on Mercury isn't guaranteed to have a sunrise

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<v Speaker 1>and a sunset. If we define a day not as

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<v Speaker 1>a complete rotation of a planet around its axis, but

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<v Speaker 1>rather as a solar day, a one complete day night cycle,

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<v Speaker 1>the amount of time it takes our son to return

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<v Speaker 1>to a specific point in the sky, then a single

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<v Speaker 1>day on Mercury is a hundred and seventy six earth

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<v Speaker 1>days long. That's the rough equivalent of two full Mercury

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<v Speaker 1>in years. That's because Mercury's orbit is what we refer

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<v Speaker 1>to as eccentric. No, not eccentric like Willy Wonka is eccentric.

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<v Speaker 1>Eccentricity is a term astronomers used to describe the shape

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<v Speaker 1>of a planet or moon's orbit. No planet orbits its

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<v Speaker 1>star in a perfect circle. The extent to which had

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<v Speaker 1>given orbit deviates from being circular is cold. It's eccentricity.

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<v Speaker 1>If an orbit was one circular, would say it had

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<v Speaker 1>an eccentricity of zero. Let The records show that Earth's

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<v Speaker 1>orbit boasts an eccentricity of just zero point zero one seven,

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<v Speaker 1>so it's almost a circle, but not quite. Mercury's orbit

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<v Speaker 1>looks more squashed or elliptical. By comparison of all the

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<v Speaker 1>planets in our beloved Solar system, Cury has the most

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<v Speaker 1>eccentric orbit. The amount of space between this world and

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<v Speaker 1>our Sun ranges from just twenty nine million miles to

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<v Speaker 1>thirty six million miles during the course of its elliptical

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<v Speaker 1>trip around the Sun. That's a forty six million to

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<v Speaker 1>fifty eight million kilometers. Consequently, Mercury's travel speed increases as

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<v Speaker 1>it gets closer to the star. Those changes in speed

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<v Speaker 1>and distance from the Sun account for the strange solar days.

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<v Speaker 1>When you view the Sun from some places on Mercury,

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<v Speaker 1>it appears to freeze in place part way through its

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<v Speaker 1>journey across the sky, then move backwards before going forward

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<v Speaker 1>again in its route to the opposite horizon. Depending on

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<v Speaker 1>where you are on the planet, this might mean that

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<v Speaker 1>you get to sunrises in a row as the Sun

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<v Speaker 1>dips back below the skyline before fully rising, or two

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<v Speaker 1>sunsets in a row as it pops back up before

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<v Speaker 1>fully setting, And of course all of this reeks havoc

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<v Speaker 1>on the planet's temperatures on Mercury, they can range as

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<v Speaker 1>high as eight hundred degrees fahrenheit that's four thirty celsius,

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<v Speaker 1>or as low as negative two nine degrees fahrenheit or

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<v Speaker 1>negative one eight celsius. As you could expect, the side

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<v Speaker 1>of the planet that's facing the Sun at any time

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<v Speaker 1>will be a good deal hotter, and on hot days

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<v Speaker 1>we could all use some ice in NASA's Messenger spacecraft

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<v Speaker 1>observed deposits of frozen water on Mercury. The ice was

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<v Speaker 1>found at the bottoms of deep craters around the northern pole,

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<v Speaker 1>which are protected from the sun all year long due

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<v Speaker 1>to Mercury's lack of tilt around its axis of rotation.

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<v Speaker 1>Earth tilts twenty three point five degrees on its axis,

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<v Speaker 1>giving us seasons and exposing the poles to the Sun.

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<v Speaker 1>But Mercury only tilts two degrees, meaning it spins almost

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<v Speaker 1>completely upright, protecting its poles and preventing seasons from occurring.

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<v Speaker 1>But back to that ice. Paradoxically, Mercury's hottest temperatures could

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<v Speaker 1>be responsible for some of the ice that it possesses.

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<v Speaker 1>Our Sun is constantly releasing charged protons and electrons in

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<v Speaker 1>streams known as solar winds. Earth is shielded by a

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<v Speaker 1>powerful magnetic field, which deflects many of these. Mercury has

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<v Speaker 1>had a magnetic field of its own four around three

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<v Speaker 1>point nine billion years. However, it's significantly weaker than the

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<v Speaker 1>one we enjoy here on Earth. If a recent scientific

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<v Speaker 1>model is correct, The intense heat of the planet's sun

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<v Speaker 1>facing side triggers chemical reactions between solar wind particles and

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<v Speaker 1>minerals buried in the soil. These are thought to create

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<v Speaker 1>traveling water molecules that later become ice. Of all the

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<v Speaker 1>frozen water on Mercury may have been generated this way,

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<v Speaker 1>Mercury doesn't have any moons to call its own. As

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<v Speaker 1>a matter of fact, With a diameter of just three thousand,

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<v Speaker 1>thirty miles or four thousand kilometers, Mercury isn't much bigger

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<v Speaker 1>than Earth's Moon easily. Mercury is the smallest planet in

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<v Speaker 1>our Sun's orbit, yet evidence tells us that it used

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<v Speaker 1>to be larger. Mercury is interesting to look at from

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<v Speaker 1>a topographic standpoint. The thin atmosphere for his very little

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<v Speaker 1>protection from asteroids, so impact craters are abundant. A single

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<v Speaker 1>photo taken by the Messenger Probe in two thousand eight

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<v Speaker 1>shows seven hundred and sixty three identifiable craters within a

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<v Speaker 1>region of the planet's surface just a hundred and seventy

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<v Speaker 1>two miles wide. That's two hundred and seventy six kilometers.

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<v Speaker 1>It's traditional to name these craters after writers, given that

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<v Speaker 1>eloquence is one of the realms of the mythological god Mercury.

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<v Speaker 1>Truman Capote, Batteline la Engel, Betty Alver, and John Lennon

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<v Speaker 1>are just some of the visionaries with their own namesake craters.

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<v Speaker 1>The planet's face is also marked by fault scarps. These

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<v Speaker 1>are cliff ridges that were first sighted on Mercury in

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<v Speaker 1>the nineteen seventies. Some of the smaller ones appeared to

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<v Speaker 1>be around just fifty million years old, making them geologically

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<v Speaker 1>pretty young. Mercury itself formed around four point five billion

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<v Speaker 1>years ago. Since then, its metallic core has been cooling

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<v Speaker 1>down at a rapid pace, and as a result, the

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<v Speaker 1>whole planet is currently shrinking. The diameter of mercury may

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<v Speaker 1>have contracted by as much as eight and a half

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<v Speaker 1>miles or fourteen kilometers over the eons. This has had

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<v Speaker 1>a tremendous effect on the planet's rocky outer surface. Those

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<v Speaker 1>previously mentioned fault scarps are born when crust materials break

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<v Speaker 1>apart and press into each other, forcing some terrain upward.

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<v Speaker 1>And because it's tectonically active in its own peculiar way, Mercury,

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<v Speaker 1>like Earth, may experience surface level earthquakes. Mercury quakes will

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<v Speaker 1>definitely be a topic worth investigating as we plot out

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<v Speaker 1>future pro missions to our curious little neighbor. Today's episode

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<v Speaker 1>was written by Mark Mancini and produced by Tyler clang Or.

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<v Speaker 1>More on this and lots of other curious topics, visit

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<v Speaker 1>how stuff works dot com. Brain Stuff is production of

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<v Speaker 1>Iyheart Radio. Or more podcasts my heart Radio, visit the

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