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The strangest moon in the Solar System is bright yellow. This picture, showing Io's true colors, was taken in 1999 July by the Galileo spacecraft that orbited Jupiter from 1995 to 2003. Io's colors derive from sulfur and molten silicate rock. The unusual surface of Io is kept very young by its system of active volcanoes. The intense tidal gravity of Jupiter stretches Io and damps wobbles caused by Jupiter's other Galilean moons. The resulting friction greatly heats Io's interior, causing molten rock to explode through the surface. Io's volcanoes are so active that they are effectively turning the whole moon inside out. Some of Io's volcanic lava is so hot it glows in the dark.

Source: NASA/JPL

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Date/TimeThumbnailDimensionsUserComment
current03:34, May 5, 2014Thumbnail for version as of 03:34, May 5, 20142,796 × 2,796 (771 KB)Jcpag2010 (wall | contribs)
11:40, June 25, 2013Thumbnail for version as of 11:40, June 25, 2013900 × 900 (141 KB)Jcpag2010 (wall | contribs)

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