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==Theories== ==Theories==
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The energy required to melt ices and produce cryovolcanoes usually comes from ]. It has also been suggested that translucent deposits of frozen materials could create a sub-surface ] that would accumulate the required heat.

It is hypothesised that the ] object ] has exhibited cryovolcanism in the past. In this case, the source of energy would be ].


==Observations== ==Observations==

Revision as of 17:22, 15 May 2007

Ganesa Macula, a dark feature on Saturn's moon Titan, might be a cryovolcanic dome.

A cryovolcano is, literally, an icy volcano. Cryovolcanoes form on icy moons, and possibly on other low-temperature astronomical objects (e.g. Kuiper belt objects). Rather than molten rock, these volcanoes erupt volatiles such as water, ammonia or methane. Collectively referred to as cryomagma or ice-volcanic melt, these substances are usually liquids and form plumes, but can also be in vapour form. After eruption cryomagma condenses to a solid form when exposed to the very low surrounding temperature. Some scientists speculate that the cryovolcanoes on Titan, Saturn's largest moon, may harbor extraterrestrial life.

Theories

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Observations

Cryovolcanoes are found on icy moons. Ice volcanoes were first observed on Neptune's moon Triton during the Voyager 2 flyby in 1989.

Plumes above the limb of Enceladus feeding Saturn's E Ring. These appear to emanate from the "tiger stripes" near the south pole.

The Cassini-Huygens mission has found a methane-spewing cryovolcano on Titan, and such volcanism is now believed to be a significant source of the methane found in Titan's atmosphere. On November 27, 2005 Cassini photographed geysers on the south pole of Enceladus (See also: Cryovolcanism on Enceladus).

Indirect evidence of cryovolcanic activity was later observed on several other icy moons of our solar system, including Europa, Ganymede, and Miranda.

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