A cryovolcano (colloquially
known as an ice volcano) is a volcano that erupts volatiles such as water,
ammonia or methane, instead of molten rock. 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. Cryovolcanoes
form on icy moons, and possibly on other low-temperature astronomical objects (e.g.,
Kuiper belt objects).
The
energy required to melt ices and produce cryovolcanoes usually comes from tidal
friction. It has also been suggested that translucent deposits of frozen
materials could create a sub-surface greenhouse effect that would accumulate
the required heat.
Some
hypothesize that the Kuiper belt object Quaoar exhibited cryovolcanism in the
past. Radioactive decay could also provide the energy necessary for such
activity, as cryovolcanoes can emit water mixed with ammonia, which would
melt at -95°C and create an extremely cold liquid that would flow out of the
volcano.
Searching
for an optical view of this topic, we found this video which shows some of the
best photos of the moon of Saturn, Enceladus...
Πηγές: www.bbc.co.uk
Δεν υπάρχουν σχόλια:
Δημοσίευση σχολίου