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1 Observations  





2 References  





3 External links  














Cryovolcano






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This is an old revision of this page, as edited by 69.161.116.59 (talk)at20:48, 6 September 2016 (Observations: Removed comment on 'few things are known about cryovolcanoes'. We've been learning a lot more lately. (Also, bright spots may be cryovolcanoes on Ceres)). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.
(diff)  Previous revision | Latest revision (diff) | Newer revision  (diff)

Doom Mons, one of the most reliably identified cryovolcanoes on Saturn's moon Titan.[1]

Acryovolcano (colloquially known as an ice volcano) is a volcano that erupts volatiles such as water, ammoniaormethane, instead of molten rock.[2] Collectively referred to as cryomagma or ice-volcanic melt,[2] 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 including dwarf planet Pluto[3]).

One potential energy source on some solar system bodies for melting ices and producing cryovolcanoes is tidal friction. It has also been suggested[by whom?] that translucent deposits of frozen materials could create a subsurface greenhouse effect that would accumulate the required heat.

Signs of past warming of the Kuiper belt object Quaoar[4] have led scientists to speculate that it exhibited cryovolcanism in the past. Radioactive decay could provide the energy necessary for such activity, as cryovolcanoes can emit water mixed with ammonia, which would melt at 180 K (−95 °C) and create an extremely cold liquid that would flow out of the volcano.

Observations

Plumes of Enceladus, feeding Saturn's E Ring, seem to arise from the "Tiger Stripes" near the south pole.

Ice volcanoes were first observed on Neptune's moon Triton during a Voyager 2 flyby in 1989.[2]

On November 27, 2005, Cassini photographed geysers on the south poleofEnceladus.[5] (See also: Enceladus (Cryovolcanism).)

Indirect evidence of cryovolcanic activity was later observed on several other icy moons of the Solar System, including Europa, Titan, Ganymede, and Miranda. Cassini has observed several features thought to be cryovolcanoes on Titan, notably Doom Mons with adjacent Sotra Patera, a feature regarded as "the very best evidence, by far, for volcanic topography anywhere documented on an icy satellite".[6] Cryovolcanism is one process hypothesized to be a significant source of the methane found in Titan's atmosphere.[7]

In 2007, observations by the Gemini Observatory showing patches of ammonia hydrates and water crystals on the surface of Pluto's moon Charon suggested the presence of active cryovolcanoes/cryogeysers.[8][9] Subsequent observations by New Horizons in 2015 found that Charon has a youthful surface, supporting this idea.[10] Pluto itself is also known to have two likely cryovolcanoes.[11]

In 2015, two distinct bright spots inside a crater of the dwarf planet Ceres were imaged by the Dawn spacecraft, leading to speculation about a possible cryovolcanic origin.[12]

In September 2016, NASA JPL and NASA Goddard scientists released findings that large Ahuna Dome on Ceres is a "volcanic dome unlike any seen elsewhere in the solar system[. The large] mountain is likely volcanic in nature. Specifically, it would be a cryovolcano -- a volcano that erupts a liquid made of volatiles such as water, instead of silicates. ... the only known example of a cryovolcano that potentially formed from a salty mud mix, and that formed in the geologically recent past."[13] In addition, at least some of Ceres' well known bright spots (notably including the ones in Occator crater) are likely also cryovolcanic in origin [14].

One possible scheme for Enceladus's cryovolcanism
  • Possible origins of methane found in plumes through its subsurface ocean
    Possible origins of methane found in plumes through its subsurface ocean
  • Chemical composition of the plumes of Enceladus
    Chemical composition of the plumes of Enceladus
  • References

    1. ^ Lopes, R. M. C.; Kirk, R. L.; Mitchell, K. L.; et al. (2013). "Cryovolcanism on Titan: New results from Cassini RADAR and VIMS". Journal of Geophysical Research: Planets. 118 (3): 416–435. Bibcode:2013JGRE..118..416L. doi:10.1002/jgre.20062.
  • ^ a b c Darling, David (ed.). "Cryovolcanism". Internet Encyclopedia of Science.
  • ^ Witze, Alexandra. "Ice volcanoes may dot Pluto's surface". Nature.
  • ^ Jewitt, D.C.; J. Luu (2004). "Crystalline water ice on the Kuiper belt object (50000) Quaoar". Nature. 432 (7018): 731–3. Bibcode:2004Natur.432..731J. doi:10.1038/nature03111. PMID 15592406.. Reprint on Jewitt's site (pdf)
  • ^ Chang, Kenneth (March 12, 2015). "Suddenly, It Seems, Water Is Everywhere in Solar System". New York Times. Retrieved March 12, 2015.
  • ^ "Cassini Spots Potential Ice Volcano on Saturn Moon". NASA, December 14, 2010
  • ^ Media Relations Office: Cassini Imaging Central Laboratory For Operations (2009). "Cassini Finds Hydrocarbon Rains May Fill The Lakes". Space Science Institute, Boulder, Colorado. Retrieved 4 March 2015.
  • ^ "Charon: An ice machine in the ultimate deep freeze". Gemini Observatory. 2007. Retrieved 18 July 2007.
  • ^ Cook; Desch, Steven J.; Roush, Ted L.; Trujillo, Chadwick A.; Geballe, T. R.; et al. (2007). "Near-Infrared Spectroscopy of Charon: Possible Evidence for Cryovolcanism on Kuiper Belt Objects". The Astrophysical Journal. 663 (2): 1406–1419. Bibcode:2007ApJ...663.1406C. doi:10.1086/518222.
  • ^ Beatty, Kelly (2 October 2015). "Charon: Cracked, Cratered, and Colorful". Sky and Telescope. Retrieved 2015-10-03.
  • ^ Witze, A. (2015-11-09). "Icy volcanoes may dot Pluto's surface". Nature News and Comment. Nature Publishing Group. doi:10.1038/nature.2015.18756. Retrieved 2015-11-09.
  • ^ O'Neill, I. (25 February 2015). "Ceres' Mystery Bright Dots May Have Volcanic Origin". Discovery Communications. Retrieved 1 March 2015.
  • ^ http://dawn.jpl.nasa.gov/news/news-detail.html?id=6611
  • ^ http://www.spacedaily.com/reports/Ceres_The_tiny_world_where_volcanoes_erupt_ice_999.html

  • Retrieved from "https://en.wikipedia.org/w/index.php?title=Cryovolcano&oldid=738086614"

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    This page was last edited on 6 September 2016, at 20:48 (UTC).

    This version of the page has been revised. Besides normal editing, the reason for revision may have been that this version contains factual inaccuracies, vandalism, or material not compatible with the Creative Commons Attribution-ShareAlike License.



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