Tsang, Constantine Southwest Research Institute, Boulder, Colorado.
Last reviewed:November 2018
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- Transits of Venus
- Atmospheric composition
- Impact craters
- Wind features
- History of volcanism
- Links to Primary Literature
- Additional Readings
The second planet in distance from the Sun. Venus has been called “Earth's twin” because it is similar to Earth in gross characteristics, such as mass, radius, and density (Fig. 1 and see table). In other ways, Venus is significantly different: Its atmospheric mass is almost a hundred times that of the Earth, with an atmospheric surface more than 90 times that of Earth; its atmosphere is mostly carbon dioxide, rather than nitrogen and oxygen; an extensive cloud layer of concentrated sulfuric acid is present; its surface temperature is an searing 464°C (867°F); it slowly rotates "backwards," or retrograde, on its axis, such that one Venusian day is equal to 243 Earth days, with the Sun rising in the west. Some of these differences are due more to alternate evolutionary paths of the two planets than to totally different initial conditions. See also: Atmosphere; Carbon dioxide; Cloud; Density; Earth; Mass; Nitrogen; Oxygen; Planet; Sulfuric acid; Sun; Temperature
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