Zhurong reveals recent aqueous activities in Utopia Planitia, Mars.


Journal

Science advances
ISSN: 2375-2548
Titre abrégé: Sci Adv
Pays: United States
ID NLM: 101653440

Informations de publication

Date de publication:
13 05 2022
Historique:
entrez: 11 5 2022
pubmed: 12 5 2022
medline: 12 5 2022
Statut: ppublish

Résumé

The Mars' climate is cold and dry in the most recent epoch, and liquid water activities are considered extremely limited. Previous orbital data only show sporadic hydrous minerals in the northern lowlands of Mars excavated by large impacts. Using the short-wave infrared spectral data obtained by the Zhurong rover of China's Tianwen-1 mission, which landed in southern Utopia Planitia on Mars, we identify hydrated sulfate/silica materials on the Amazonian terrain at the landing site. These hydrated minerals are associated with bright-toned rocks, interpreted to be duricrust developed locally. The lithified duricrusts suggest that formation with substantial liquid water originates by either groundwater rising or subsurface ice melting. In situ evidence for aqueous activities identified at Zhurong's landing site indicates a more active Amazonian hydrosphere for Mars than previously thought.

Identifiants

pubmed: 35544566
doi: 10.1126/sciadv.abn8555
pmc: PMC9094648
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

eabn8555

Subventions

Organisme : Key Research Program of the Chinese Academy of Sciences
ID : ZDBS-SSW-TLC001

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Auteurs

Yang Liu (Y)

State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China.
Center for Excellence in Comparative Planetology, Chinese Academy of Sciences, Hefei 200083, China.

Xing Wu (X)

State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China.

Yu-Yan Sara Zhao (YS)

Center for Excellence in Comparative Planetology, Chinese Academy of Sciences, Hefei 200083, China.
Center for Lunar and Planetary Sciences, Institute of Geochemistry, Chinese Academy of Sciences, Guiyang 550081, China.

Lu Pan (L)

Center for Star and Planet Formation, GLOBE Institute, University of Copenhagen, Copenhagen, Denmark.

Chi Wang (C)

State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China.

Jia Liu (J)

State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China.

Zhenxing Zhao (Z)

State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China.
University of Chinese Academy of Sciences, Beijing 100049, China.

Xiang Zhou (X)

State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China.
University of Chinese Academy of Sciences, Beijing 100049, China.

Chaolin Zhang (C)

State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China.
University of Chinese Academy of Sciences, Beijing 100049, China.

Yuchun Wu (Y)

State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China.
University of Chinese Academy of Sciences, Beijing 100049, China.

Wenhui Wan (W)

State Key Laboratory of Remote Sensing Science, Aerospace Information Research Institute, Chinese Academy of Sciences, Beijing 100101, China.

Yongliao Zou (Y)

State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China.

Classifications MeSH