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It has been suggested that the Jovian moon [[Ganymede (moon)|Ganymede]] and the Saturnian moon [[Enceladus (moon)|Enceladus]] may also possess sub-surface oceans. However the ice covering is expected to be thicker on Jupiter's Ganymede than on Europa.
It has been suggested that the Jovian moon [[Ganymede (moon)|Ganymede]] and the Saturnian moon [[Enceladus (moon)|Enceladus]] may also possess sub-surface oceans. However the ice covering is expected to be thicker on Jupiter's Ganymede than on Europa.
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==See also==
==See also==

Revision as of 13:48, 18 October 2008

The movement of water around, over, and through the Earth is called the water cycle, a key process of the hydrosphere.

A hydrosphere (from Greek ύδωρ - hydor, "water" + σφαίρα - sphaira, "sphere") in physical geography describes the collective mass of water found on, under, and over the surface of a planet.

Other hydrospheres

A thick hydrosphere is thought to exist around the Jovian moon Europa. The outer layer of this hydrosphere is almost entirely frozen, but current models predict that there is an ocean up to 100 km in depth underneath the ice. This ocean remains in a liquid form due to tidal flexing of the moon in its orbit around Jupiter.

It has been suggested that the Jovian moon Ganymede and the Saturnian moon Enceladus may also possess sub-surface oceans. However the ice covering is expected to be thicker on Jupiter's Ganymede than on Europa. you think i want this

See also

References

External links