Recent Aqueous Activity on Mars Evidenced by Transverse Aeolian Ridges in the Zhurong Exploration Region of Utopia Planitia

被引:20
|
作者
Wang, Jiang [1 ,2 ,3 ,4 ]
Zhao, Jiannan [2 ]
Xiao, Long [1 ,5 ]
Peng, Shuai [1 ]
Zhang, Liang [1 ]
Zhang, Zhixin [6 ]
Gao, Antong [1 ]
Qiao, He [1 ]
Wang, Le [1 ]
Zhang, Shiqi [2 ]
Xiao, Xiao [1 ]
Shi, Yutong [1 ]
Zhao, Siyuan [1 ]
Zhao, Jiawei [1 ]
Qian, Yuqi [1 ]
Zhang, Jun [1 ]
Zhang, Xubing [6 ]
Huang, Jun [1 ,5 ]
机构
[1] China Univ Geosci, Planetary Sci Inst, Sch Earth Sci, State Key Lab Geol Proc & Mineral Resources, Wuhan, Peoples R China
[2] China Univ Geosci, Key Lab Geol Survey & Evaluat, Minist Educ, Wuhan, Peoples R China
[3] Macau Univ Sci & Technol, State Key Lab Lunar & Planetary Sci, Macau, Peoples R China
[4] China Univ Geosci, Hubei Key Lab Crit Zone Evolut, Wuhan, Peoples R China
[5] Chinese Acad Sci, Ctr Excellence Comparat Planetol, Beijing, Peoples R China
[6] China Univ Geosci, Sch Geog & Informat Engn, Wuhan, Peoples R China
基金
中国博士后科学基金; 中国国家自然科学基金;
关键词
Mars; Utopia Planitia; transverse aeolian ridge; aqueous activity; polygonal feature; hydrated mineral; RECURRING SLOPE LINEAE; MERIDIANI-PLANUM; POLYGONAL CRACKS; WATER; ICE; SUBSURFACE; TERRAINS; RIPPLES; FLOWS; BASIN;
D O I
10.1029/2022GL101650
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Aqueous activities on Mars have gradually declined since the Noachian (>3.7 Ga). Although water can be stored in the subsurface during the latest epochs, geomorphological evidence is still limited. In this study, we used in situ imaging and spectral data acquired by China's Zhurong rover, as well as high-resolution remote-sensing data, to investigate the transverse aeolian ridges (TARs) in the Zhurong landing region of Utopia Planitia. A two-stage evolutionary scenario of the TARs is proposed and polygonal features with hydrated minerals are identified for the first time on the surface of Martian TARs. We discussed the possible formation mechanisms of the polygonal features, and proposed that they could be related to recent aqueous activity and atmosphere-surface water exchange on Mars, which sheds light on the hydrological cycle of Mars in current cold and dry climate.
引用
收藏
页数:11
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