The First Ground-based White Light Lunar Polarization Imaging:A New Kind of FeO Observation on the Near Side of the Moon

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外文摘要：Lunar optical polarization is a fascinating phenomenon that occurs when sunlight reflects off the surface of the Moon and becomes polarized.This study employs a novel split-focus plane polarimetric camera to conduct the initial white light polarimetric observations on the near side of the Moon.We obtained the linear degree of polarization(DOP)parameters of white light by observation from the eastern and western hemispheres of the Moon.The findings indicate that the white light polarization is lower in the lunar highland than in the lunar maria overall.Combining the analysis of lunar soil samples,we noticed and determined that the DOP parameters of white light demonstrate high consistency with iron oxide on the Moon.This study may serve as a new diagnostic tool for the Moon.

外文关键词：

techniques:photometricpolarizationmethods:observationalMoon

作者：

Wei-Nan Wang、Jin-Song Ping、Ming-Yuan Wang、Wen-Zhao Zhang、Han-Lin Ye、Xing-Wei Han、Song-Feng Kou

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作者单位：

Changchun Observatory,National Astronomical Observatories Chinese Academy of Sciences Changchun 130117,China

University of Chinese Academy of Sciences,Beijing 101408,China

National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100101,China

Astronomy Department,Beijing Normal University,Beijing 100875,China

International Center for Climate and Environment Sciences,Institute of Atmospheric Physics,Chinese Academy of Sciences,Beijing 100029,China

Nanjing Institute of Astronomical Optics and Technology,Chinese Academy of Sciences,Nanjing 210042,China

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基金：

National Key Research and Development Program of ChinaNational LLR station project,the National Natural Science Foundation of China(NSFC)National LLR station project,the National Natural Science Foundation of China(NSFC)Jilin Province Midyouth science and technology innovation and entrepreneurship outstanding talent projectChangchun City and Chinese Academy of Sciences Science and Technology Cooperation Hightech Industrialization Special Fund Pr

项目编号：

2021YFA0715101119730644210141320220508147RC21SH05

出版年：

2024

DOI：

10.1088/1674-4527/ad44f1

天文和天体物理学研究

中国科学院国家天文台

天文和天体物理学研究

CSTPCD

影响因子：0.406

ISSN：1674-4527

年,卷(期)：2024.24(6)