Volcanism of Outer Satellites



Europa
Image taken from http://www.mufor.org/
Image taken from http://www.mufor.org/

Europa is a moon of Jupiter, but unlike Io, it is covered with a smooth layer of ice.  It does experience tidal heating, which allows for a layer of water beneath the ice.  Europa displays cryovolcanism, where water replaces magma as the substance being erupted.  They cryovolcanism explains the smoothness of the surface.
Ganymede
Image taken from http://www.planetary.org/html/news/articlearchive/headlines/2001/ganymede.html
Image taken from http://www.planetary.org/html/news/articlearchive/headlines/2001/ganymede.html

Ganymede shows both old, dark surface and young, light surface.  It has a variety of grooves, fractures, and grabens indicating tectonism.  Ganymede as well as Europa may experience cryovolcanism.
Enceladus
Image taken from http://saturn.jpl.nasa.gov/news/saturn-story/moons.cfm
Image taken from http://saturn.jpl.nasa.gov/news/saturn-story/moons.cfm

Saturn's moon Enceladus has a very smooth, fresh surface.  It is an icy satellite, and displays cryovolcanism.  It has very new ridges and plains, probably caused by ice flows or an explosion of ice particles.  It is still active currently.
Triton
Image taken from http://www.astrosurf.com/lombry/sysol-kbo.htm
Image taken from http://www.astrosurf.com/lombry/sysol-kbo.htm

Triton is an ice covered moon of Neptune.  It's surface is relatively smooth, indicating cryovolcanism.  The surface of Triton is riddled with cryovolcanic geysers that throw plumes of ice into the atmosphere.  The geysers may be solar driven despite the fact that Triton is so far from the sun and is so cold.  


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