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Venus

Venus - Rotating Model
Credit: Almond/NASA

Venus is the second planet out from the Sun, and is the brightest object in the night sky other than the Moon. Whilst it has no satellites, it is very unusual in that it spins in a different direction to all the other planets.

The planet is covered in a thick layer of cloud and has a surface pressure around 90 times that seen on Earth. However, we can now see beneath the atmosphere of Venus thanks to recent surface radar images.

The temperature at the surface is very high (up to 460 °C), and is actually hotter than the closest planet to the Sun, Mercury. This is because it has a very strong Greenhouse Effect.

Since the first visit of Mariner 2 in 1962, more than 20 spacecraft have been to Venus.

Planet Data Sheet show »« hide
Facts and FiguresMercuryVenus EarthMarsJupiter SaturnUranusNeptune
Orbital Distance (AU)10.380.72 1.01.525.2 9.4519.230.06
Radius (KM)2,4406,052 6,3783,39771,492 60,26825,55924,746
Mass (Earth Masses)20.0550.82 1.00.11318 95.214.517.1
Year Length
(Earth Days)
88225 365.2568711.9
Years
29.45
Years
84.0
Years
164.8
Years
Day Length
(Earth Days)
176117 1.01.030.41 0.430.750.67
Surface Gravity (g)30.380.91 1.00.382.34 0.930.921.12
Surface Temperature-200 to
400 °C
460 °C -80 to
50 °C
-150 to
20 °C
-110 °C -140 °C-190 °C-200 °C
Number of moons00 1263 602713
Notes: 1 1 AU (or Astronomical Unit) = 149,600,000 KM and is the mean distance from the Earth to the Sun
2 1 Earth Mass = 5,980,000,000,000,000,000,000,000 KG : 3 1 g = 9.8 m/s2