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Accumulation and Erosion of Mars' South Polar Layered Deposits

机译:火星南极层状沉积物的堆积和侵蚀

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Mars' polar regions are covered with ice-rich layered deposits that potentially contain a record of climate variations. The sounding radar 5HARAD on the Mars Reconnaissance Orbiter mapped detailed subsurface stratigraphy in the Promethei Lingula region of the south polar plateau, Planum Australe. Radar reflections interpreted as layers are correlated across adjacent orbits and are continuous for up to 150 kilometers along spacecraft orbital tracks. The reflectors are often separated into discrete reflector sequences, and strong echoes are seen as deep as 1 kilometer. In some cases, the sequences are dipping with respect to each other, suggesting an interdepositional period of erosion. In Australe Sulci, layers are exhumed, indicating recent erosion.
机译:火星的极地地区覆盖着富含冰的分层沉积物,这些沉积物可能包含气候变化的记录。火星侦察轨道飞行器上的探空雷达5HARAD绘制了南极高原普兰纽姆普罗米塞林格拉地区的详细地下地层图。解释为层的雷达反射在相邻轨道上相互关联,并且沿着航天器的轨道连续长达150公里。反射器通常分为离散的反射器序列,并且强烈的回声被视为深达1公里。在某些情况下,这些序列彼此相对下降,表明侵蚀的沉积期。在Australe Sulci,挖掘出层,表明最近有侵蚀。

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