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In mass and density, Venus is nearly the Earth's twin. Venus' atmosphere is very thick and opaque. The atmosphere is about 95% carbon dioxide. Other components are also present: Nitrogen, water vapor, sulfuric acid

Heat is trapped near the planet's surface by a runaway Greenhouse Effect, that produces a surface temperature of nearly 470C.

The planet has been imaged from orbit using the Magellan radar mapping system. The surface was photographed by the Russian Venera spacecraft.

Volcanoes and lava flows
Coronae, arachnoids, ``pancakes''
Impact craters: more than on the Earth, but less than on the Moon.

 

 

 

Venus Mars


 

 

Volcanos: Olympus Mons
Canyons: Valles Marineris
Traces of erosion: dry river beds
Winds and dust storms

Polar caps: frozen CO2

Venus Mars