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Deuteronilus Mensae is a region on Mars 937 km across and centered at 43°54′N 337°24′W / 43.9°N 337.4°W. It covers 344°–325° West and 40°–48° North. Deuteronilus region lies just to the north of Arabia Terra and is included in the Ismenius Lacus quadrangle. It is along the dichotomy boundary, that is between the old, heavily cratered southern highlands and the low plains of the northern hemisphere. The region contains flat-topped knobby terrain that may have been formed by glaciers at some time in the past. Deuteronilus Mensae is to the immediate west of Protonilus Mensae and Ismeniae Fossae. Glaciers persist in the region in modern times, with at least one glacier estimated to have formed as recently as 100,000 to 10,000 years ago. Recent evidence from the radar on the Mars Reconnaissan

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  • Deuteronilus Mensae (en)
  • Deuteronilus Mensae (de)
  • Deuteronilus Mensae (es)
  • Deuteronilus Mensae (it)
  • Deuteronilus Mensae (pt)
  • 都特罗尼勒斯桌山群 (zh)
rdfs:comment
  • Deuteronilus Mensae ist eine Region auf dem Mars im Ismenius-Lacus-Gradfeld. Sie liegt an der Grenze zur Mars-Dichotomie und ist durch zahlreiche freistehende Tafelberge charakterisiert, die bei der von Norden nach Süden vordringenden Erosion übriggeblieben sind und heute als „Zeugenberge“ frei in der Landschaft stehen. (de)
  • Le Deuteronilus Mensae sono una struttura geologica della superficie di Marte. (it)
  • 都特罗尼勒斯桌山群(Deuteronilus Mensae)是火星上一处方圆937公里的区域,其中心坐标为北纬43.9°、西经337.4°处,它东西横跨西经344°–西经325°,南北覆盖北纬40°–北纬48°。都特罗尼勒斯桌山群区坐落于阿拉伯台地北部,并被包含在伊斯墨诺斯湖区内。它紧邻火星南北分界线,处于古老崎岖的南部高地和北半球低地平原之间。该地区分布着众多可能形成于过去某个冰川期的平顶瘤状地形,东面则是普罗敦尼勒斯桌山群和伊斯墨诺斯槽沟群。目前该地区依然存有冰川,据估计至少有一道冰川形成于最近1万至10万年前,从最近火星勘测轨道飞行器的浅层雷达探测表明,都特罗尼勒斯桌山群部分地区确实蕴藏着水冰。 都特罗尼勒斯桌山群取名自古典返照率特征,“都特罗尼勒斯”(Deuteronilus)一词为拉丁语尼罗河(Nilus)的第二部分的意思。 (zh)
  • Deuteronilus Mensae is a region on Mars 937 km across and centered at 43°54′N 337°24′W / 43.9°N 337.4°W. It covers 344°–325° West and 40°–48° North. Deuteronilus region lies just to the north of Arabia Terra and is included in the Ismenius Lacus quadrangle. It is along the dichotomy boundary, that is between the old, heavily cratered southern highlands and the low plains of the northern hemisphere. The region contains flat-topped knobby terrain that may have been formed by glaciers at some time in the past. Deuteronilus Mensae is to the immediate west of Protonilus Mensae and Ismeniae Fossae. Glaciers persist in the region in modern times, with at least one glacier estimated to have formed as recently as 100,000 to 10,000 years ago. Recent evidence from the radar on the Mars Reconnaissan (en)
  • Deuteronilus Mensae es el nombre de una región en Marte de 937 km de ancho y centrada en las coordenadas 43,9 ° N 337,4 ° W. Cubre las corrdenadas 344 ° –325 ° Oeste y 40 ° –48 ° Norte.​ La región de Deuteronilus se encuentra justo al norte de Arabia Terra y está incluida en el cuadrángulo de Ismenius Lacus. Está a lo largo del límite de dicotomía, es decir, entre las antiguas tierras altas del sur, llenas de cráteres, y las llanuras bajas del hemisferio norte. La región contiene un terreno irregular de cima plana que puede haber sido formado por glaciares en algún momento del pasado. Deuteronilus Mensae está al oeste inmediato de Protonilus Mensae e .​​ Los glaciares persisten en la región en los tiempos modernos, y se estima que al menos un glaciar se formó hace entre 100.000 y 10.000 añ (es)
  • Deuteronilus Mensae é uma região em Marte com uma extensão de 937 quilômetros centrada a 43.9º N e 337.4º W. Ela cobre 344° -325° E e 40°-48° N. A região de Deuteronilus fica a norte de Arabia Terra e faz parte do quadrângulo de Ismenius Lacus. Ela se situa entre os planaltos do sul, de terreno antigo e repleto de crateras e as planícies baixas do hemisfério norte. A região contém terrenos elevados de topo achatado que podem ter sido formados por geleiras em algum ponto do passado. Geleiras persistem na região em tempos modernos, com ao menos uma galeira cuja formação estima-se se deu em um período recente de 100,000 a 10,000 anos atrás. Evidência recente do radar da Mars Reconnaissance Orbiter tem mostrado que partes de Deuteronilus Mensae contém gelo de fato. (pt)
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  • Deuteronilus Mensae (en)
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