The following outline is provided as an overview of and topical guide to Venus:

Venus – second planet from the Sun, orbiting it every 224.7 Earth days. It has the longest rotation period (243 days) of any planet in the Solar System and rotates in the opposite direction to most other planets. It has no natural satellite. It is named after the Roman goddess of love and beauty. It is the second-brightest natural object in the night sky after the Moon, reaching an apparent magnitude of −4.6, bright enough to cast shadows. Because Venus orbits within Earth's orbit it is an inferior planet. Venus is a terrestrial planet and is sometimes called Earth's "sister planet" because of their similar size, mass, proximity to the Sun, and bulk composition. It is radically different from Earth in other respects. It has the densest atmosphere of the four terrestrial planets, consisting of more than 96% carbon dioxide. The atmospheric pressure at the planet's surface is 92 times that of Earth, or roughly the pressure found 900 m (3,000 ft) underwater on Earth.

Classification of Venus edit

Location of Venus edit

Features of Venus edit

History of Venus edit

History of Venus

Exploration of Venus edit

Flybys and direct missions to explore Venus edit

Cancelled missions to explore Venus edit

Future of Venus exploration edit

Proposed missions to explore Venus edit

Venus in popular culture edit

See also edit

References edit

External links edit

Cartographic resources