| The moon Io is a very remarkable moon - probably the 
							most fascinating body in our Solar System. It has 
							the most active volcanism of any body that we know.
 
							Io is 3,630 km in diameter and is 421,600 km away 
							from Jupiter. Its silicate mantle and crust are under constant 
							tidal flex from Jupiter and the three other Galilean 
							satellites. The result of this are the 
							constant violent eruptions of its volcanoes. It may 
							seem strange that Europa, Ganymede and Callisto can 
							provide a counterforce for Jupiter, but Ganymede and 
							Callisto are larger than Io. Additional "energy" 
							generated by Europa and Ganymede are the result of
							orbital resonance which is 1:2:4 - for every 
							1 orbit of Europa, Io orbits twice and for every 1 
							orbit of Ganymede, Io orbits four times. This timing 
							sequence creates a resonance. 
							 The face of Io has been describes as looking like 
							a pizza. All of the dots on the face are volcanoes, 
							and this image shows the active ones: 
							 
							Close examinations by both Voyager and Galileo have 
							images volcanoes "caught in the act." 
							 
							 
							In addition to the volcanic activity, sulfur dust is 
							also introduced to the surface: 
							 
							seen in the image above as the ring. In addition to 
							sulfur dust, lava flows are also very common: 
							 
							With all of the violet eruptions constantly spewing 
							material upward, an atmosphere might be present - 
							but there isn't one. The gravity of Jupiter grabs 
							hold of the material and is put into orbit within 
							the Io Torus: 
							 
							The Torus is an area of intense 
							electromagnetic 
							energy and is an area of constant study. More data 
							on the Io Torus can be found at the
							
							Io Plasma Torus links. 
							Back to Top |