Geology of Aeolis Dorsa alluvial sedimentary basin, Mars

被引:14
|
作者
Di Pietro, Ilaria [1 ]
Ori, Gian Gabriele [1 ,2 ]
Pondrelli, Monica [1 ]
Salese, Francesco [1 ,3 ]
机构
[1] Univ Gabriele dAnnunzio, Int Res Sch Planetary Sci, Dipartimento Ingn & Geol, Viale Pindaro 42, I-65127 Pescara, Italy
[2] Univ Cadi Ayyad, Ibn Battuta Ctr, Blvd Abdelkrim Al Khattabi, Marrakech, Morocco
[3] Univ Nantes, Lab Planetol & Geodynam, 2 Rue Houssiniere, F-44300 Nantes, France
来源
JOURNAL OF MAPS | 2018年 / 14卷 / 02期
关键词
Aeolis Dorsa; Zephyria Planum; alluvial deposits; fluvial deposits; Gale Crater; Mars; FEATURES;
D O I
10.1080/17445647.2018.1454350
中图分类号
P9 [自然地理学]; K9 [地理];
学科分类号
0705 ; 070501 ;
摘要
Aeolis Dorsa is a topographic depression, approximate to 800km east of Gale Crater, located along the Mars' dichotomy boundary. This area hosts a set of fluvial sedimentary rocks displaying an exceptional record of depositional environments and fluvial channels patterns that suggest the presence of a large amount of surface and/or subsurface water. We interpreted the plain as an ancient waterlogged environment, a sedimentary basin passing into distal depositional environments. Regional mapping of the area revealed the presence of a large-scale fluvial system that points to a long-term and extensive hydrological cycle. A significant wet period with changing environmental conditions in Hesperian/Amazonian occurred in the study area diverging from the present-day climate. Our map (Main Map) contributes to the understanding of past climatic conditions on Mars. Moreover, it provides an interesting perspective for future missions looking for evidence of present-day and/or past extraterrestrial organisms as the life as we know it needs liquid water.
引用
收藏
页码:212 / 218
页数:7
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