Planetary Geology: Formation and Features of Planets
Classified in Geology
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Origin of Terrestrial Atmospheres
Venus, Earth, and Mars received their atmospheres through outgassing. Chemical reactions caused CO2 on Earth to dissolve in oceans and go into carbonate rocks, like limestone. Mars lost much of its atmosphere through impacts.
Formation of the Maria
- The Moon once had a molten interior.
- Several large impacts made huge crater basins.
- This “runny” lava filled in the basins.
Mercury: A Dead Planet
- No atmosphere.
- Has no maria, but small lava plains.
- Has fewer craters than the Moon.
- Craters are shallower than the Moon's due to higher gravity on Mercury.
- Evidence for tectonic processes.
- Evidence for ice at the North Pole.
Mars: Mountains and Canyons
- Mountains and canyons.
- Volcanoes.
- Thin atmosphere.
- No plate tectonics; volcanoes