GASES IN OUTER SPACE
 

Outer space was once believed to be a perfect vacuum. However, this is not the case. There is plenty of stuff out there, and much of it is hydrogen and helium gas. (There are also trace amounts of heavier gases and some solid rocks and ice chunks as well.) All the atoms in outer space interact gravitationally with all the others. This might be hard to imagine at first, but if you think about it, there’s no escaping it. Even a single atom of hydrogen exerts a gravitational pull on another atom 1 million km away.
The motion of atoms in outer space is almost random but not quite. The slightest perturbation in the randomness of the motion gives gravitation a chance to cause the gas to clump into huge clouds. Once this process begins, it can continue until a globe of gas forms in which the central particle density is significant. As gravitation continues to pull the atoms in toward the center, the mutual attraction among the atoms there becomes greater and greater. If the gas cloud has some spin, it flattens into an oblate spherical shape and eventually into a disk with a bulge at the center. A vicious circle ensues, and the density in the central region skyrockets. The gas pressure in the center rises, and this causes it to heat up. Ultimately, it gets so hot that nuclear fusion begins, and a star is born. Similar events among the atoms of the gas on a smaller scale can result in the formation of asteroids, planets, and planetary moons.

مواضيع ذات صلة

Evaporation

Evaporation of a liquid

The ideal gas law

Temperature and kinetic energy

Compressibility of radiation

The pressure of a gas

Properties of matter

Matter is made of atoms

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GAS PRESSURE

GASES NEAR A PLANET

DIFFUSION IN SMALL CONTAINERS