ΕΠΙΣΤΗΜΟΝΙΚΑ ΑΡΘΡΑ-ΝΕΑ-ΑΝΑΚΟΙΝΩΣΕΙΣ ΑΠΟ ΟΜΑΔΑ ΥΠ. ΔΙΔΑΚΤΟΡΩΝ ΚΑΙ ΜΕΤΑΔΙΔΑΚΤΟΡΙΚΩΝ ΕΡΕΥΝΗΤΩΝ

A scientific blog from PhD and Post Doctoral Researchers NTUA, UOA, Athens, Greece.

Δευτέρα 26 Μαρτίου 2012

"Ice fountains of Enceladus"


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

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