Zhurong reveals recent aqueous activities in Utopia Planitia, Mars

Author:

Liu Yang12ORCID,Wu Xing1ORCID,Zhao Yu-Yan Sara23ORCID,Pan Lu4ORCID,Wang Chi1ORCID,Liu Jia1ORCID,Zhao Zhenxing15,Zhou Xiang15,Zhang Chaolin15ORCID,Wu Yuchun15,Wan Wenhui6,Zou Yongliao1

Affiliation:

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

2. Center for Excellence in Comparative Planetology, Chinese Academy of Sciences, Hefei 200083, China.

3. Center for Lunar and Planetary Sciences, Institute of Geochemistry, Chinese Academy of Sciences, Guiyang 550081, China.

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

5. University of Chinese Academy of Sciences, Beijing 100049, China.

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

Abstract

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.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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