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Early Earth
inhospitable
frequent asteroid and meteorite bombardment
frequent volcanic eruptions
very high temperature causing hydrogen and helium to escape
lots of water vapor with no oxygen
Later Earth
frequent volcanic eruptions produced water and gases such as carbon dioxide, carbon monoxide, nitrogen, hydrogen, ammonia, and methane
still no oxygen
As the Earth Cooled
water condensed to form oceans
carbon dioxide dissolved into oceans forming carbonates
nitrogen became a major component
Present-day Earth
mainly composed of nitrogen and oxygen with trace amounts of several gases
Nitrogen
the most abundant gas
Oxygen
the second most abundant gas
Troposphere
lowest layer
most water vapor
all weather associated cloud types
temperature decreases, altitude increases
clouds get thinner and absorbs less radiation
Stratosphere
above the troposphere
temperature increase, altitude increases
presence of ozone
where jet planes fly
lacks weather-producing air turbulence and is almost free of clouds and other forms of weather
Ozone
protects the Earth by absorbing ultraviolent radiation
Mesosphere
temperature decreases, altitude increases
protects Earth from meteoroids
meteorides that enter the Earth burn up due to intense friction
Burning Meteoroid
“shooting star” or “burning meteors”
Meteorites
meteoroids that manage to reach Earth
Thermosphere
second highest layer
temperature increases, altitude increases
nitrogen and oxygen absorb a great deal of ultraviolent radiation and turns it into heat
Ionosphere
consists of highly-ionized gas which was formed when ultraviolent rays knock off electron from nitrogen and oxygen
Kennelly-Heaviside Layer
layer of the ionosphere that reflects radio waves
Aurora
colorful display of lights formed when ions interact with air molecules, usually happens at the poles
Northern Lights - Aurora Borealis
Southern Lights - Aurora Australis
Exosphere
outermost layer
most of the orbiting satellites, as well as low density elements, like hydrogen and helium are found here