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In our solar
system, Venus, Mars, and the earth are rocky planets that have
atmospheres. It has recently been discovered that the moon and
Mercury also have atmospheres, though their atmospheres are very
diffuse. The planets farther from the sun, Jupiter, Saturn, Neptune,
and Uranus, are called gas giants because they are made almost
entirely of hydrogen, helium and trace amounts of other gases.
These planets have colorful and turbulent atmospheres. What are some of the factors that determine what a planet's
atmosphere will be like?
- Planetary gravity,
- temperature, and
- the amount of gaseous material present all have effects.
Planetary Gravity and Density
Gravity causes objects to be
pulled towards each other. A gas molecule has no measurable effect
on a planet, but a planet pulls nearby gas molecules toward itself.
The more the mass of the planet, the more gravitational pull
it exerts on molecules of gas. This pull makes the larger atoms,
such as nitrogen and oxygen, heavier than the tiny hydrogen atoms,
and keeps most of them near the planet's surface.
As we saw in The
Layers of Earth's Atmosphere, 99% of the mass of the earth's
atmosphere is located in the thirty miles above the surface of
the planet. Even there, the closer that the atoms are to the
surface, the more thickly they are crowded together. How closely
they are crowded is referred to as atmospheric density.
The more atoms you have in a given space, the more dense the
atmosphere is.

Density refers to how tightly the atoms are packed together.
How Many Atoms?
Density is affected by gravity,
and also by how many atoms there are to pack together. Suppose
that you were given a cubic yard of the earth's sea level atmosphere
and asked to count the atoms in it. It would take practically
forever! That cube of air would have many billions of atoms in
it. Now, for comparison, let's think about a cubic yard of the
moon's atmosphere. The atmosphere of the moon is difficult to
detect and very diffuse when compared with the earth's atmosphere.
There just aren't many atoms to work with, comparatively speaking.
So would there be hundreds of atoms to count? Even thousands?
Maybe only one? Counting these atoms might actually be possible!
Why do some planets have more atoms in their atmospheres
than others?
Planets start out with
different amounts of atmospheric gases. There are many factors
that could influence this, some related to what the planet is
made of, some related to the level of volcanic activity, some
related to asteroid impacts, etc. You can probably give your
planet as dense an atmosphere as you wish. On earth, the elevation
above 20,000 feet is called the Death Zone, because there is
very little oxygen up there. Parts of the brain begin to die
above that height. We cannot live there permanently, though short
visits by mountain climbers are not necessarily lethal. Perhaps
animals and plants could evolve to live in this thin atmosphere,
but there must be an upper limit. A related problem is that dangerous
solar radiation is filtered out by the atmosphere. Where the
air is less dense, more radiation gets through.
Our "sister planet",
Venus, has an atmosphere 100 times as dense as earth. Earth life
forms would be squashed by the pressure there. However,
animals can live at even greater
pressures in the bottom of our
oceans, so perhaps they could evolve on such a world if the temperatures
were favorable. (Venus is much too hot.)
As planets cool, rocks and dust
and elements with high melting points solidify. Gases, which
have lower melting points, remain gaseous until the temperature
falls to the point at which they, too, become liquid and perhaps
even solid. As we saw in The States
of Matter atoms and molecules in a gaseous state are moving
rapidly and freely, and bumping into each other. The hotter they
get, the faster they move. If they are moving fast enough, they
can reach escape velocity, the point at which they
have enough momentum to escape from the planet's gravitational
field altogether. If they are moving away from the planet, they
can disappear into space. As the molecules leave, the planet's
atmosphere becomes just a tiny bit less. Over a long period of
time, the atmosphere can slowly drift away.
Atoms are especially liable
to leave a small planet or moon. Small, low mass moons and planets
have low gravity to begin with, so the atoms are not held to
the surface very strongly. Heat makes matters worse. Mercury
is a small planet, close to the sun. It has a day time high temperature
of 350 degrees Centigrade, which would make the atmospheric atoms
move rapidly. In addition, particles from the sun, the solar
wind collide with the atmospheric atoms, speeding them
up further and perhaps changing their direction of movement.
Mercury has only about a third of the gravity of the earth, so
it is easier for atoms to escape from Mercury. It is not surprising
that Mercury has no atmosphere to speak of.
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