•Amount of CO2 in
atmosphere on Venus
roughly equal to
amount of CO2 in
limestone on Earth
–
•With no oceans, don’t have a way to get CO2 out of
atmosphere and back into
rocks
–
•Runaway effect, because high T causes faster loss of water to space.
–If H2O gets into upper atmosphere it is broken down into O, H by UV sunlight
–H is so light it escapes to space
–On Earth cooler T traps H2O in lower atmosphere (it condenses if it gets to high)
–
•Location
closer to the sun pushed Venus “over the edge” compared to Earth