Planetary Atmospheres

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O Universo em Evolução

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Caltech

O Universo em Evolução

402 classificações

This is an introductory astronomy survey class that covers our understanding of the physical universe and its major constituents, including planetary systems, stars, galaxies, black holes, quasars, larger structures, and the universe as a whole.

Na lição

Week 3

Contents of the Solar System23:45

Formation of the Solar System14:41

Planetary Atmospheres4:34

Conheça os instrutores

S. George Djorgovski
Professor
Astronomy

Well, where do planets get their atmospheres?

Well, there are three sources of it.

First of all, you have planetesimals with light elements,

like comets, hit and that stuff can evaporate and

if the planet's massive enough it will retain that gaseous envelope.

And that's probably where water on the moon comes from.

Then there was certainly some stuff, the operation from protoplanetary

envelope wasn't 100% efficient and so there's still probably some water and

other things, gases mixed in with rocky planetesimals, and

then as planet settles down the stuff slowly outgasses out, goes to the surface.

And then that process can continue through volcanoes, which again, are pulling out

stuff from the inner parts of the planet, and gasses that evaporate do evaporate.

So now, how much atmosphere you keep depends on the surface

gravity of the planet.

Higher gravity, more atmosphere.

And Earth is unique among the rocky planets in having, well,

it's not unique, Venus does also, but

let's say less usual among the rocky planets to keep an atmosphere.

Moon doesn't have much of an atmosphere,

Mercury doesn't have any, Mars has very little.

But on the other hand, gaseous giants are very massive, plenty of gravity.

They retain all of this stuff and very thick envelopes,

which is hardly an atmosphere.

They really are fluffy envelopes of gas.

So that's where the atmospheres come from.

Then what happens to the atmospheres?

Well, the winds happen.

And there are two reasons how that gets to be.

The first one is sunlight.

Near the equator you get more sunlight because it falls directly, right?

Near a pole you get much less because it's an oblique angle.

So you have temperature differential.

That causes convection along the meridian.

The heat from the equator rises, goes up.

The cold air near poles sink, goes down.

And so you'd expect then that everywhere in the world there will be winds

blowing away from the, I'm sorry upper atmospheres away from the equator,

lower surface down from the poles will be very cold.

But that's not all.

Earth also rotates, any planet rotates.

Now if there was no disk differentiation, if there was no sun,

then atmosphere will tend to lag behind a planet in rotation, just

out of sheer inertia, and this friction is very low between gas and solid, and

so you tend to have east-west winds in the opposite direction of the rotation.

I combine these two things, there's Coriolis force and you learn in mechanics

where that comes from, it's essentially due to the conservation of the momentum.

If you push something on a radial orbit in a spinning disk or on a spinning sphere

it's going to get decelerated because of conservation of angular momentum.

So what that does, it breaks this convection cells, and

on planet Earth there are three of those on each hemisphere from equator to a pole.

They're called Hadley cells.

And so within each one of those, this convection mechanism,

more heat closer to the equator, less heat up there, causes the circulation.

But Coriolis force breaks them up.

Now on the other hand, in a really fast rotating planet, like Jupiter,

or Saturn, which also doesn't have a proper surface but

the whole thing kind of drags itself, you're going to

completely dominate atmospheric circulation by the planetary rotation.

And this is why Jupiter and Saturn, they have all these horizontal looking belts.

So the winds on fast rotating, thick atmosphere planets, go east-west.

On Venus, which doesn't rotate very much at all, they go north-south.

And on Earth, which is in between, they kind of go diagonal.

This is what the trade winds are.

Okay, we ran out of time and stuff.

And so next time we'll continue with some other interesting

things about planets such as like where does global warming coming from?

And then about extrasolar planets as well.

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