Chi Wang

Chi Wang


Research Focus & Metrics

Academic Career Length

25Years (2002-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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19 July 2019 in Science
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Journal Article
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CLChunlai Li
Chunlai Li
CWChi Wang
Chi Wang
YWYong Wei
Yong Wei
YLYangting Lin
Yangting Lin
Since the beginning of the 21st century, the pace of lunar exploration has accelerated, with more than a dozen probes having undertaken scientific exploration of the Moon. Prominent among these have been the robotic “Chang’E” (CE) missions of the China Lunar Exploration Program (CLEP). We discuss technological and scientific goals and achievements for the four completed, and four planned, CE missions, and longer-term goals and plans of the CLEP beyond the CE missions. The exploration plan is flexible and iterative, with an emphasis on international cooperation.

25 September 2020 in Science Advances
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Journal Article
Open access
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SZShenyi Zhang
Shenyi Zhang
RWRobert F. Wimmer-Schweingruber
Robert F. Wimmer-Schweingruber
JYJia Yu
Jia Yu
CWChi Wang
Chi Wang
QFQiang Fu
Qiang Fu
QZQuan Zida
Quan Zida
The first measurements of the radiation dose on the lunar surface are reported in preparation for human exploration of the Moon.

13 July 2020 in Nature Astronomy
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Journal Article
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WWW. X. Wan
W. X. Wan
CWChi Wang
Chi Wang
CLC. L. Li
C. L. Li
YWYong Wei
Yong Wei

13 May 2022 in Science Advances
Verified
Journal Article
Open access
YLYang Liu
Yang Liu
XWXing Wu
Xing Wu
YZYu-Yan Sara Zhao
Yu-Yan Sara Zhao
LPLu Pan
Lu Pan
CWChi Wang
Chi Wang
YZYongliao Zou
Yongliao Zou
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.

14 October 2005 in Journal of Geophysical Research
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Journal Article
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CWChi Wang
Chi Wang
DDD. Du
D. Du
JRJ. D. Richardson
J. D. Richardson

7 January 2022 in Science Advances
Verified
Journal Article
Open access
HLHonglei Lin
Honglei Lin
SLShuai Li
Shuai Li
RXRui Xu
Rui Xu
YLYang Liu
Yang Liu
XWXing Wu
Xing Wu
CWChi Wang
Chi Wang
Variations of total water contents were detected in situ from the lunar regolith and rock at the Chang’E-5 landing site.