(Terrestrial) Planetary Atmospheres II. Atmospheres consist of exospheres only Take either of...
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Transcript of (Terrestrial) Planetary Atmospheres II. Atmospheres consist of exospheres only Take either of...
Atmospheres consist of exospheres only
Take either of their atmospheres, could “almost store them in a dorm room”
No volcanic outgassing◦ Geologically dead
Moon and Mercury
Atmosphere persists because:◦ Micro-meteorite impacts◦ Solar wind trapped by weak mag field
Surface atoms set free
Moon and Mercury
Low atmospheric pressure◦ Mars is small, so less gravity◦ Liquid water is unstable
Mostly CO2
◦ Not enough to produce much greenhouse effect◦ Pressure is 13,000x greater on Venus
No oxygen, no ozone layer◦ UV light hits surface
Thin atmosphere
Mars’ Atmosphere
Southern hemisphere has hottest summers and coldest winters
Summer pole sublimates while winter pole condenses◦ This drives winds from summer to winter pole
Mars’ Atmosphere
These winds cause dust storms over the whole surface!
Previous astronomers thought they saw changes in vegetation!
Mars’ Atmosphere
Surface features and erosion suggest heavy rainfall
Used to have thick atmosphere◦ Otherwise water (which there was lots of) would
be unstable
Used to be geologically (…perhaps biologically?) thriving. What happened??
Mars’ Atmosphere
Mars’ Atmosphere
How?
Core temperature dropped
Became geologically dead
Volcanoes stopped
Due to low gravity on Mars, some atmosphere escaped◦ Not replenished by volcanoes
Mars’ Atmosphere
Mars’ Atmosphere
As Mars became geologicallydead, its core solidified. Mars lost its magnetic field and the solar wind stripped away most of its atmosphere.
Thick CO2 atmosphere
◦ 96.5% CO2
Volcanoes pump CO2 into the atmosphere
◦ Venus is large so remains geologically active
Atmosphere of Venus
Atmosphere of Venus
Venus’ atmosphere creates an extreme greenhouse effect due to the massive
amounts of CO2 in its atmosphere.
Atmospheric pressure at surface:
◦ 90x that of Earth (LOTS of CO2)
Density 10% that of water
“…would feel like a cross between swimming and flying.”
Atmosphere of Venus
Venus has thick clouds of sulfuric acid
Volcanoes blast sulfur dioxide◦ Reaches upper atmosphere◦ UV converts it to sulfuric acid
Sulfur compounds give Venus its yellowish color
Atmosphere of Venus
Slow rotation, surface at same temperature
◦ Not much wind
Sulfuric acid rain evaporates 10 miles above the surface
Poles just about as hot as the equator
◦ Greenhouse effect
No seasons (no axial tilt)
Atmosphere of Venus
Atmosphere of Venus
So why does Venus have somuch carbon dioxide in its
atmosphere?
(It does have volcanoes, but so doesEarth!)
Atmosphere of Venus
Because a planet needs oceansto dissolve CO2. Venus does not
have oceans.
Earth has about the same amountof CO2 as Venus– but most of it is locked away in rocks in the ocean!
It did! And so did Earth.
Venus closer to the Sun than Earth (50 oF hotter)
Oceans began to evaporate◦ What kind of gas is water vapor?
Atmosphere of Venus
Average temperature up by 30 oC More evaporation More greenhouse gases, higher temp. More evaporation Etc…
Runaway Greenhouse Effect: oceans fueled their own evaporation, did not dissolve and store CO2 in rocks
Atmosphere of Venus
Venus has no magnetic field
◦ Solar wind broke up water molecules in the atmosphere
Hydrogen flies off, oxygen reacts on surface
◦ No water left to dissolve the CO2 on the surface or in the atmosphere
Atmosphere of Venus
P. 323:
“We’ve seen that moving Earth to Venus’ orbit would cause our planet to become Venus-like. If we could somehow move Venus to Earth’s orbit, would it become Earth-like?”
Atmosphere of Venus
Temperature low enough for water to condense◦ So we have oceans
Carbon dioxide dissolved in the oceans◦ Right balance of
greenhouse gases
Atmosphere of Earth
Nitrogen (77%) and oxygen (21%)
Why so much nitrogen?
Volcanoes outgas CO2, water, and nitrogen◦ Water into oceans◦ CO2 into rocks◦ Nitrogen went up
Atmosphere of Earth
Why so much oxygen?
It came from (and still does) photosynthesis and CO2
◦ Air only breathable in last few hundred million years
Atmosphere of Earth
No runaway greenhouse effect (like Venus has)
No freezing (like Mars has)
Self-stabilizing greenhouse effect◦ Requires two parts: Volcanoes and oceans◦ Venus has one but not the other!
Stability of Earth’s Climate
It is stable.
◦ If it warms up: More evaporation, more rain, more CO2 taken out of
the atmosphere (ends up in rocks)
◦ If it cools off: Less evaporation, less rain, CO2 released from
volcanoes allowed to build up
Carbon Dioxide Cycle