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Statements

Subject Item
dbr:Ganges_Mensa
rdf:type
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rdfs:label
恒河桌山 Ganges Mensa Ganges Mensa Ganges Mensa
rdfs:comment
恒河桌山(Ganges Mensa)是一座位于火星水手谷外侧支谷—恒河峡谷内的台地和内部层状沉积物。该桌山高出恒河峡谷谷底4公里,几乎与周围的卢娜高原一样高。同赫柏桌山一样,该桌山也已与周围峡谷崖壁完全分离,并受到持续的严重侵蚀,导致其覆盖范围出现缩退。 该桌山由分解为凹槽状的易碎薄单元层组成,多数研究人员将其解释为侵蚀性风成特征,并称之为雅丹地貌,其顶部覆盖着一层起源于火山的更耐蚀冠岩。据了解,虽然桌山是通过火山活动和沉积作用的某种组合而形成,但与桌山有关的火山作用是发生在冰下(巨型冰岩盖内),还是发生在水下(古湖泊内)仍存在争议。支持冰下假说的人认为恒河桌山是一座平顶火山,与在俄罗斯图瓦共和国阿扎斯高原所观察到的类似物极其相似。 La Ganges Mensa è una struttura geologica della superficie di Marte. Ganges Mensa é uma mesa no quadrângulo de Coprates em Marte, localizada a 7.2° S e 48.8° W. Seu diâmetro é de 140.0 km e seu nome vem do nome de uma formação de albedo. Ganges Mensa (also occasionally termed Gangis Mensa in literature) is a mesa and an interior layered deposit in Ganges Chasma, one of the peripheral valleys of Valles Marineris on Mars. The mesa rises up to 4 kilometres (13,000 ft) from the floor of Ganges Chasma, nearly to the same elevation as the surrounding plateaux of Lunae Planum. Like Hebes Mensa, the mesa is completely separated from the surrounding canyon walls and has sustained significant erosion that has caused it to retreat in areal extent.
dbp:name
Ganges Mensa
geo:lat
-7.199999809265137
geo:long
-48.79999923706055
foaf:depiction
n10:Groundwaterseries8final.jpg n10:Ganges_Mensa.jpg n10:The_Table1.jpg n10:Ganges_Chasma_(Themis_Day).png
dcterms:subject
dbc:Coprates_quadrangle dbc:Mensae_on_Mars
dbo:wikiPageID
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dbo:wikiPageRevisionID
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dbo:wikiPageWikiLink
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owl:sameAs
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dbo:thumbnail
n10:Ganges_Chasma_(Themis_Day).png?width=300
dbp:caption
A THEMIS infrared image of Ganges Chasma. North is up. Ganges Mensa is the prominent mountain-like feature near the center of the image.
dbp:location
dbr:Ganges_Chasma dbr:Coprates_quadrangle
georss:point
-7.2 -48.8
dbo:abstract
Ganges Mensa (also occasionally termed Gangis Mensa in literature) is a mesa and an interior layered deposit in Ganges Chasma, one of the peripheral valleys of Valles Marineris on Mars. The mesa rises up to 4 kilometres (13,000 ft) from the floor of Ganges Chasma, nearly to the same elevation as the surrounding plateaux of Lunae Planum. Like Hebes Mensa, the mesa is completely separated from the surrounding canyon walls and has sustained significant erosion that has caused it to retreat in areal extent. The mesa is composed of friable, thinly-layered units which decompose into fluted patternations, interpreted by most researchers as erosional aeolian features known as yardangs. It is capped by a more resistant layer that is interpreted by many researchers to be volcanic in origin. Although the mesa is understood to have formed through some combination of volcanism and sedimentary deposition, there is ongoing contention over whether the volcanism associated with the mesa occurred subglacially (into an ice megalaccolith) or subaqueously (into a paleolake). Those who favor the subglacial hypothesis believe that Ganges Mensa is a tuya that is extremely similar to analogues observed in the Azas Plateau of Tuva, Russia. Ganges Mensa é uma mesa no quadrângulo de Coprates em Marte, localizada a 7.2° S e 48.8° W. Seu diâmetro é de 140.0 km e seu nome vem do nome de uma formação de albedo. La Ganges Mensa è una struttura geologica della superficie di Marte. 恒河桌山(Ganges Mensa)是一座位于火星水手谷外侧支谷—恒河峡谷内的台地和内部层状沉积物。该桌山高出恒河峡谷谷底4公里,几乎与周围的卢娜高原一样高。同赫柏桌山一样,该桌山也已与周围峡谷崖壁完全分离,并受到持续的严重侵蚀,导致其覆盖范围出现缩退。 该桌山由分解为凹槽状的易碎薄单元层组成,多数研究人员将其解释为侵蚀性风成特征,并称之为雅丹地貌,其顶部覆盖着一层起源于火山的更耐蚀冠岩。据了解,虽然桌山是通过火山活动和沉积作用的某种组合而形成,但与桌山有关的火山作用是发生在冰下(巨型冰岩盖内),还是发生在水下(古湖泊内)仍存在争议。支持冰下假说的人认为恒河桌山是一座平顶火山,与在俄罗斯图瓦共和国阿扎斯高原所观察到的类似物极其相似。
dbp:naming
dbr:Classical_albedo_features_on_Mars
gold:hypernym
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geo:geometry
POINT(-48.799999237061 -7.1999998092651)