l>Planetary Science

Atmospheres

A planet\"s environment helps shield a planet\"s surface from harsh radiation from theSun and also it moderates the quantity of power lost to room from the planet\"s interior. An atmosphere likewise makes it feasible for liquid to exist top top a planet\"s surface ar by giving the pressure essential to keep the liquid from boiling away to space---life top top the surface of a planet or moon requires an atmosphere.All of the planets began out with settings of hydrogen and helium. The innerfour planets (Mercury, Venus, Earth, and also Mars) lost their initial atmospheres. The settings they have now room from gases released from their interiors, but Mercuryand Mars have even lost most of their secondary atmospheres. The outer four planets(Jupiter, Saturn, Uranus, and also Neptune) to be able to store their original atmospheres.They have really thick environments with proportionally tiny solid cores while thethe inner 4 planets have actually thin environments with proportionally large solid parts.The properties of each planet\"s atmosphere are summary in thePlanet Atmospheres table (will appear in a new window). Two vital determinants inhow thick a planet\"s atmosphere will be space the planet\"s escape velocity and thetemperature that the atmosphere.

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Escape of an Atmosphere

The thickness the a planet\"s setting depends top top the planet\"s gravity and also thetemperature that the atmosphere. A world with weaker gravity does not have actually as strong a organize on the molecules that comprise its atmosphereas a planet with stronger gravity. The gas molecules will be much more likely come escape theplanet\"s gravity. If the environment is cool enough, climate the gas molecules will not bemoving fast sufficient to to escape the planet\"s gravity. However how strong is ``strong enough\"\"and exactly how cool is ``cool enough\"\" to host onto one atmosphere? come answer the you require toconsider a planet\"s escape velocity and also how the molecule speeds rely on thetemperature.Escape VelocityIf you litter a rock up, it will increase up and then fall ago down because of gravity. If you litter it up v a faster speed, it will certainly rise greater before heaviness brings it ago down. If you litter it up fast sufficient it just escapes the heaviness of the planet---the absent initially had a velocity same to the escape velocity. The escape velocity is the initial velocity required to escape a substantial body\"s gravitational influence. In the Newton\"s law of heaviness chapter the escape velocity is discovered to = Sqrt<(2G × (planet or moon mass))/distance)>. The distance is measured native the planet or moon\"s center.

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Since the massis in the top of the fraction, the escape velocity boosts as the fixed increases. A moremassive earth will have stronger heaviness and, therefore, a higher escape velocity.Also, since the distance is in the bottom of the fraction, the escape velocitydecreases as the street increases. The escape velocity is reduced at greaterheights over the planet\"s surface. The planet\"s gravity has a weaker hold on themolecules at the optimal of the atmosphere than those close to the surface, therefore those highup molecules will be the an initial to ``evaporate away.\"\"Do not confuse the street from the planet\"s center with the planet\"sdistance from the Sun. The to escape velocity does NOT rely on how much the earth isfrom the Sun. Girlfriend would usage the Sun\"s distance just if you want to calculation theescape velocity from the Sun. In the exact same way, a moon\"s escape velocitydoes NOT depend on how much it is native the world it orbits.TemperatureThe temperature of a product is a measure up of the typical kinetic (motion) energyof the molecules in the material. As the temperature increases, a solid turns right into agas as soon as the corpuscle are moving fast sufficient to break free of the chemical bonds thatheld lock together.

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The particles in a name is gas are moving quicker thanthose in a cooler gas that the exact same type. Using Newton\"s regulations of motion, the relationbetween the speed of the molecules and also their temperature is discovered to be temperature = (gas molecule mass)×(average gas molecule speed)2 / (3k),where k is a universal continuous of nature dubbed the ``Boltzmann constant\"\".Gas molecule of the same kind and at the same temperature will have actually a spread of speeds---some relocating quickly, some moving slower---so usethe average speed.If you switch the temperature and also velocity, you can derive the typical gas moleculevelocity = Sqrt<(3k × temperature/(molecule mass))>. Rememberthat the mass below is the small mass that the gas particle, not the planet\"s mass. Sincethe massive is in the bottom that the fraction, the much more massive gas molecules will moveslower on typical than the lighter gas molecules. Because that example, carbon dioxidemolecules move slower on median than hydrogen molecules at the exact same temperature.Because substantial gas molecules move slower, planets through weaker gravity (e.g., theterrestrial planets) will have tendency to have settings made of just substantial molecules.The lighter molecules like hydrogen and helium will have actually escaped.
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Whereas the procedure described above leads to evaporation molecule by molecule, another type of atmospheric loss from heater happens as soon as the environment absorbs ultraviolet light, warms up and also expands upward leading to a planetary wind flowing outward to space. Planets with a most hydrogen in their environments are specifically subject come this kind of atmospheric loss from heating. The very light hydrogen deserve to bump more heavier molecules and atoms outward in the planetary wind.

Does Gravity win or Temperature?

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If a planet does not have a magnetic ar (for reasons described later), the solar wind have the right to strip an environment through a process called sputtering. without a magnetic field, the solar wind is able come hit the planet\"s atmosphere directly. The high-energy solar wind ions deserve to accelerate atmosphere particles at high altitudes to great enough speeds to escape. One additional method of environment escape referred to as photodissociation occurs when high-energy sunlight (e.g., ultraviolet or x-rays) hits high-altitude molecule in the planet\"s atmosphere and also breaks castle apart into individual atom or smaller molecules. These smaller particles have the same temperature together the bigger molecules and, therefore, as explained above, will relocate at much faster speeds, perhaps fast enough to escape.

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The processes defined so much in this section occupational particle to particle and work over lengthy time durations as the setting leaks away particle by particle. In comparison impacts through comets or asteroids can inject a huge amount of energy really quickly when the projectile vaporizes top top impact. The widening plume of warm gas drives off the air above the affect site, v the larger the affect energy, the wider is the cone of air that is removed above the influence site. The affect removal procedure was probably particularly effective for Mars (being so close to the asteroid belt) and also the huge moons the Jupiter (so close to Jupiter\"s strong gravity the attracts numerous comets and asteroids).

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Go back to previous ar -- \"next\"WIDTH=\"73\" go to next sectionGo come Astronomy note homelast updated: June 5, 2019Is this page a copy of Strobel\"s Astronomy Notes?Author of initial content: Nick Strobel