![]() | Europacompiled by Wm. Robert Johnstonlast updated 10 January 2003 |
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Europa's surface is covered by bright water ice and transversed by linear streaks and other features colored brownish orange. There are no large impact craters--very unusual for a planetary satellite, indicating that some geologic process has been at work to eliminate craters. (The largest unambiguous crater is 48 km across.) It is mostly rock underneath a 70-km to 200-km thick layer of water ice. The rocky interior is probably separated into a silicate mantle and a metal-rich core. Europa has no atmosphere except for trace amounts of gases such as oxygen.
Images of Europa's surface suggest that this water ice layer is mostly "warm" slushy ice or even liquid water. The linear streaks appear to be cracks in a solid ice layer 10 km thick or less. The absence of large craters is also explained by a relatively thin ice layer. It is possible that an ocean of water--90 km deep--could exist under the ice layer. The gravitational tides from the other Galilean satellites have melted Io's interior, giving it the most active known volcanoes in the solar system. The same effect could heat Europa's interior enough to maintain an ocean.
Since liquid water is essential for the existence of life, the recognition in 1980 that Europa could have an ocean made it the most likely abode for extraterrestrial life in the solar system. Recent discoveries of life on the Earth's ocean floor thriving around thermal vents lends to obvious comparisons to a possible dark ocean on Europa.
Europa was discovered by Galileo in 1610, but was little more than a point of light in telescopes until the Pioneer probes transmitted fuzzy images in 1973 and 1974 while swinging past Jupiter. Flybys in 1979 by Voyagers 1 and 2 produced the first images to provide details about the surface. Voyager 2 in particular provided enough information to lead to speculation about an ocean. In 1995 the Galileo orbiter entered orbit around Jupiter for long-term study of Jupiter and its satellites. Several close passes by Europa have provided evidence that below the surface most of Europa's ice is soft or liquid (i.e. an ocean). NASA hopes to send a spacecraft to orbit Europa exclusively from 2008 to 2012.
Data on Europa:
Primary: Jupiter
Discovery: 7 January 1610 by Galileo Galilei, named by Simon Marius
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