翻訳と辞書
Words near each other
・ Gori Teri Aankhen...
・ Gori TV Broadcasting Tower
・ Gori vatra
・ Gori, Burkina Faso
・ Gori, Chad
・ Gori, Georgia
・ Gori, Piéla
・ Gorgonius
・ Gorgonocephalidae
・ Gorgonocephalus
・ Gorgonocephalus arcticus
・ Gorgonocephalus eucnemis
・ Gorgonops
・ Gorgonopsia
・ Gorgons Head
Gorgonum Chaos
・ Gorgonzola
・ Gorgonzola (Milan Metro)
・ Gorgonzola, Milan
・ Gorgopas
・ Gorgopas (2nd century BC)
・ Gorgopas (4th century BC)
・ Gorgopas (butterfly)
・ Gorgophone
・ Gorgophone (skipper)
・ Gorgopis
・ Gorgopis alticola
・ Gorgopis anguistiptera
・ Gorgopis annulosa
・ Gorgopis armillata


Dictionary Lists
翻訳と辞書 辞書検索 [ 開発暫定版 ]
スポンサード リンク

Gorgonum Chaos : ウィキペディア英語版
Gorgonum Chaos

Gorgonum Chaos is a set of canyons in the Phaethontis quadrangle of Mars. It is located at
37.5° south latitude and 170.9° west longitude. Its name comes from an albedo feature at 24S, 154W.〔(Gazetteer of Planetary Nomenclature )〕 Some of the first gullies on Mars were found in Gorgonum Chaos.〔Malin, M., Edgett, K. 2000. Evidence for recent groundwater seepage and surface runoff on Mars. Science 288, 2330–2335.〕 It is generally believed that it once contained a lake.〔Howard, A. and J. Moore. 2004. Scarp-bounded benches in Gorgonum Chaos, Mars: Formed beneath an ice-covered lake? Geophys. Res. Lett. 31.〕Other nearby features are Sirenum Fossae, Maadim Vallis, Ariadnes Colles, and Atlantis Chaos. Some of the surfaces in the region are formed from the Electris deposits.〔Wendt, L., J. Bishop, G. Neakum. 2013. Knob fields in the Terra Cimmeria/Terra Sirenum region of Mars: Stratigraphy, mineralogy and morphology. Icarus 225, 200-215. 〕
==Gullies==
Gullies may be due to recent flowing water. Many are presnt in the Gorgonum Chaos.〔(Gorgonum Chaos Mesas (PSP_004071_1425) )〕 〔http://hirise.lpl.arizona.edu/PSP_001948_1425〕
Gullies occur on steep slopes, especially craters. Gullies are believed to be relatively young because they have few, if any craters, and they lie on top of sand dunes which are young. Usually, each gully has an alcove, channel, and apron. Although many ideas have been put forward to explain them, the most popular involve liquid water either coming from an aquifer or left over from old glaciers.〔Heldmann, J. and M. Mellon. Observations of martian gullies and constraints on potential formation mechanisms. 2004. Icarus. 168: 285-304.〕
There is evidence for both theories. Most of the gully alcove heads occur at the same level, just as one would expect of an aquifer. Various measurements and calculations show that liquid water could exist in an aquifer at the usual depths where the gullies begin.〔Heldmann, J. and M. Mellon. 2004. Observations of martian gullies and constraints on potential formation mechanisms. Icarus. 168:285-304〕 One variation of this model is that rising hot magma could have melted ice in the ground and caused water to flow in aquifers. Aquifers are layer that allow water to flow. They may consist of porus sandstone. This layer would be perched on top of another layer that prevents water from going down (in geological terms it would be called impermeable). The only direction the trapped water can flow is hoizontally. The water could then flow out onto the surface when it reaches a break, like a crater wall. Aquifers are quite common on Earth. A good example is "Weeping Rock" in Zion National Park Utah.〔Harris, A and E. Tuttle. 1990. Geology of National Parks. Kendall/Hunt Publishing Company. Dubuque, Iowa〕

On the other hand, much of the surface of Mars is covered by a thick smooth mantle that is thought to be a mixture of ice and dust. This ice-rich mantle, a few yards thick, smooths the land, but in places it has a bumpy texture, resembling the surface of a basketball. Under certain conditions the ice could melt and flow down the slopes to create gullies. Because there are few craters on this mantle, the mantle is relatively young. An excellent view of this mantle is shown below in the picture of the Ptolemaeus Crater Rim, as seen by HiRISE.
Changes in Mars's orbit and tilt cause significant changes in the distribution of water ice from polar regions down to latitudes equivalent to Texas. During certain climate periods water vapor leaves polar ice and enters the atmosphere. The water comes back to ground at lower latitudes as deposits of frost or snow mixed generously with dust. The atmosphere of Mars contains a great deal of fine dust particles. Water vapor will condense on the particles, then fall down to the ground due to the additional weight of the water coating. When ice at the top of the mantling layer goes back into the atmosphere, it leaves behind dust, which insulating the remaining ice.〔MLA NASA/Jet Propulsion Laboratory (2003, December 18). Mars May Be Emerging From An Ice Age. ScienceDaily. Retrieved February 19, 2009, from http://www.sciencedaily.com /releases/2003/12/031218075443.htmAds by GoogleAdvertise〕

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「Gorgonum Chaos」の詳細全文を読む



スポンサード リンク
翻訳と辞書 : 翻訳のためのインターネットリソース

Copyright(C) kotoba.ne.jp 1997-2016. All Rights Reserved.