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Planetary Geology pdf - NASA

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Unit<br />

Three<br />

Earth is not unique in possessing an atmosphere.<br />

Venus, Mars, Pluto, and two of the<br />

satellites of the outer planetsÑTitan (a moon<br />

of Saturn) and Triton (a moon of Neptune) have<br />

atmospheres that envelop their surfaces. In addition,<br />

the giant planets of the outer solar systemÑ<br />

Jupiter, Saturn, Uranus, and NeptuneÑare composed<br />

predominantly of gases. Other bodies in the<br />

solar system possess extremely thin atmospheres.<br />

Such bodies are the Moon (sodium gas), Mercury<br />

(sodium gas), Europa (oxygen) and Io (sulfur).<br />

The compositions of planetary atmospheres are<br />

different, for a variety of reasons. First, surface gravity,<br />

the force that holds down an atmosphere, differs<br />

significantly among the planets. For example, the<br />

large gravitational force of the giant planet Jupiter is<br />

able to retain light gases such as hydrogen and helium<br />

that escape from lower gravity objects. Second,<br />

the distance from the sun determines the energy<br />

available to heat atmospheric gas to a planetÕs<br />

escape velocity, the speed at which gas molecules<br />

overcome a planetÕs gravitational grasp. Thus, the<br />

Introduction to<br />

<strong>Planetary</strong> Atmospheres<br />

EG-1998-03-109-HQ Activities in <strong>Planetary</strong> <strong>Geology</strong> for the Physical and Earth Sciences<br />

85<br />

distant and cold Titan, Triton, and Pluto are able to<br />

retain their atmospheres despite relatively low gravities.<br />

Finally, we know that the chemistry and geologic<br />

history are different for each planet. Because<br />

atmospheric makeup is generally related to chemistry<br />

and temperature during planetary formation<br />

and the subsequent escape of interior gases, the constituents<br />

and total pressures of planetary atmospheres<br />

are likely to be different. Moreover, on Earth,<br />

atmospheric composition is largely governed by the<br />

by-products of the very life that it sustains.<br />

From the perspective of the planetary geologist,<br />

atmospheres are important in the ways they shape<br />

planetary surfaces. Wind can transport particles,<br />

both eroding the surface and leaving deposits. Frost<br />

and precipitation can leave direct and indirect<br />

marks on a planetary surface. Climate changes can<br />

influence a planetÕs geological history. Conversely,<br />

studying surface geology leads to an understanding<br />

of the atmosphere and climate of a<br />

planetÑboth its present state and its past.

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