Venus

Venus, imaged by NASA's Mariner 10 spacecraft

Venus is the second planet from the Sun and Earth’s closest planetary neighbor. Beneath its brilliant white clouds lies the hottest surface of any planet — hot enough to melt lead — the result of a runaway greenhouse effect driven by a crushing carbon dioxide atmosphere.

Distance from Sun 67 million miles (108 million km) — 0.72 AU
Diameter 7,521 miles (12,104 km)
Length of day 243 Earth days (longer than its year)
Length of year 225 Earth days
Moons 0
Temperature ~872°F (467°C) at the surface
Atmosphere Mostly carbon dioxide, with clouds of sulfuric acid

Interesting facts

  • Venus rotates backwards compared to most planets, and so slowly that its day is longer than its year.
  • The surface pressure on Venus is about 93 times that of Earth at sea level — similar to being nearly a mile underwater in Earth’s oceans.
  • Venus has no moons, but it does have a tiny quasi-satellite, nicknamed Zoozve, that shares its orbit around the Sun.
  • NASA’s Mariner 2 became the first spacecraft to visit another planet when it flew past Venus in 1962.
  • Two new NASA missions, VERITAS and DAVINCI, are being developed to study Venus’s surface and atmosphere in greater detail.

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