Possible Non‐Mare Lithologies in the Regolith at the Chang’E‐5 Landing Site: Evidence From Remote Sensing Data

Author:

Fu Xiaohui12ORCID,Hou Xuting1,Zhang Jiang1,Li Bo1ORCID,Ling Zongcheng12ORCID,Jolliff Bradley L.3,Xu Lin4,Zou Yongliao4

Affiliation:

1. Shandong Key Laboratory of Optical Astronomy and Solar‐Terrestrial Environment School of Space Science and Physics Institute of Space Sciences Shandong University Weihai Shandong China

2. CAS Center for Excellence in Comparative Planetology Hefei China

3. Department of Earth and Planetary Sciences and The McDonnell Center for the Space Sciences Washington University in St. Louis St. Louis MO USA

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

Funder

Chinese Academy of Sciences

State Key Laboratory of Lunar and Planetary Sciences

National Outstanding Youth Science Fund Project of National Natural Science Foundation of China

Shandong University

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Reference90 articles.

1. The geochemical and petrochemical features of regolith and rocks from Mare Crisium (preliminary data);Barsukov V. L.;Proceedings of the Lunar and Planetary Science Conference,1977

2. Ages of flow units in the lunar nearside maria based on lunar orbiter IV photographs;Boyce J. M.;Proceedings of the Lunar and Planetary Science Conference,1976

3. Geology of Mairan middle dome: Its implication to silicic volcanism on the Moon

4. Analysis of lunar samples: Implications for planet formation and evolution

5. The Aristarchus Plateau on the Moon: Mineralogical and structural study from integrated Clementine UV–Vis–NIR spectral data

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