[Home]History of Callisto the moon

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Revision 5 . . (edit) December 2, 2001 2:40 pm by Bryan Derksen
Revision 4 . . December 2, 2001 1:21 pm by Bryan Derksen [more evidence for the ocean]
Revision 3 . . (edit) November 23, 2001 5:19 pm by Magnus Manske [-"Also"]
Revision 2 . . November 23, 2001 11:16 am by Bryan Derksen
Revision 1 . . November 23, 2001 10:36 am by Bryan Derksen [split original Callisto article]
  

Difference (from prior major revision) (minor diff)

Changed: 5c5
Its battered surface lies on top of an icy layer that is about 200 kilometers thick. Beneath the crust lies a salty ocean in excess of 10 kilometers thick. The ocean was discovered from studies of the [magnetic field]?s around Jupiter and its moons. It was found that Callisto's magnetic field varies (flows in various directions at different times) in response to the background magnetic field generated by Jupiter; this suggested a layer of highly conductive fluid within Callisto.
Its battered surface lies on top of an icy layer that is about 200 kilometers thick. Beneath the crust lies a salty ocean in excess of 10 kilometers thick. The ocean was discovered from studies of the [magnetic field]?s around Jupiter and its moons. It was found that Callisto's magnetic field varies (flows in various directions at different times) in response to the background magnetic field generated by Jupiter; this suggested a layer of highly conductive fluid within Callisto. Another piece of evidence supporting the existance of an ocean under Callisto's crust is the fact that the surface of the moon directly opposite the massive impact crater Valhalla shows no fracturing or disrupted terrain, as the antipodes to similar massive impacts on the Moon and Mercury do; a liquid layer would serve to damp out the seismic waves before they could travel through Callisto to focus on the opposite side of its crust.

Changed: 18c18
*Mass: 1.08*1023 kg
*Mass: 1.08×1023 kg

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