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Second planet from the Sun From Wikipedia, the free encyclopedia
Venus is the second planet from the Sun. It is a terrestrial planet and is the closest in mass and size to its orbital neighbour Earth. Venus has by far the densest atmosphere of the terrestrial planets, composed mostly of carbon dioxide with a thick, global sulfuric acid cloud cover. At the surface it has a mean temperature of 737 K (464 °C; 867 °F) and a pressure of 92 times that of Earth's at sea level. These extreme conditions compress carbon dioxide into a supercritical state at Venus's surface.
Designations | |||||
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Pronunciation | /ˈviːnəs/ | ||||
Named after | Roman goddess of love (see goddess Venus) | ||||
Adjectives | Venusian /vɪˈnjuːziən, -ʒən/,[1] rarely Cytherean /sɪθəˈriːən/[2] or Venerean / Venerian /vɪˈnɪəriən/[3] | ||||
Symbol | |||||
Orbital characteristics[4][5] | |||||
Epoch J2000 | |||||
Aphelion | 0.728213 AU (108.94 million km) | ||||
Perihelion | 0.718440 AU (107.48 million km) | ||||
0.723332 AU (108.21 million km) | |||||
Eccentricity | 0.006772[6] | ||||
583.92 days[4] | |||||
Average orbital speed | 35.02 km/s | ||||
50.115° | |||||
Inclination |
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76.680°[6] | |||||
54.884° | |||||
Satellites | None | ||||
Physical characteristics | |||||
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Flattening | 0[8] | ||||
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Volume |
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Mass |
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Mean density | 5.243 g/cm3 | ||||
8.87 m/s2 (0.904 g0) | |||||
10.36 km/s (6.44 mi/s)[10] | |||||
−116.75 d (retrograde)[11]
1 Venus solar day | |||||
−243.0226 d (retrograde)[12] | |||||
Equatorial rotation velocity | 1.81 m/s | ||||
2.64° (for retrograde rotation) 177.36° (to orbit)[4][note 1] | |||||
North pole right ascension | |||||
North pole declination | 67.16° [14] | ||||
Albedo | |||||
Temperature | 232 K (−41 °C) (blackbody temperature)[17] | ||||
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