Evaluation of small-sized mounds formation mechanisms in China's Zhurong landing region

被引:4
|
作者
Lin, Yu [1 ]
Zhao, Jiannan [2 ]
Wang, Le [1 ]
Huang, Jun [1 ]
Zhang, Liang [1 ]
Xiao, Long [1 ]
机构
[1] China Univ Geosci, Planetary Sci Inst, Sch Earth Sci, State Key Lab Geol Proc & Mineral Resources, Wuhan 430074, Peoples R China
[2] China Univ Geosci, Key Lab Geol Survey & Evaluat, Minist Educ, Wuhan 430074, Peoples R China
基金
中国国家自然科学基金;
关键词
Small -sized mounds; Volatile; Utopia Planitia; Tianwen-1; Mars; UTOPIA PLANITIA; MUD VOLCANISM; GROUND ICE; DACITE CRYPTODOME; GLACIER DEPOSITS; IMPACT CRATERS; MARS; PINGOS; SUBLIMATION; HEMISPHERE;
D O I
10.1016/j.icarus.2022.115256
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Tianwen-1 is China's first independent Mars exploration mission. The rover "Zhurong" landed in the southern Utopia Planitia where various landforms such as impact craters, pitted cones, troughs, and aeolian features are present. In this study, we identified a special type of small-sized mounds in the Zhurong landing region using high-resolution images acquired by the Tianwen-1 orbiter. We made a detailed investigation on the morphology of the small-sized mounds as well as pits occurring on them. The small-sized mounds are usually <10 m in height and 50-150 m in diameter, while the pits are-45 m in width and-3.4 m in depth. By comparing with landforms of similar appearance, e.g., mud volcanos, ring-molded craters (RMCs), pingos, pedestal craters, and lava domes, we suggest that the small-sized mounds are most likely to be lava domes in origin due to similarities in the shape and rocky materials of the mounds. The pits spatially associated with the mounds are likely to be generated by the sublimation of subsurface volatiles after the formation of the mounds. This study provides additional interesting targets for the future exploration of the Zhurong rover to reveal the magmatic activities and volatile distribution and circulation in the Utopia Planitia.
引用
收藏
页数:10
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