In situ lunar phase curves measured by Chang'E-4 in the Von Karman Crater, South Pole-Aitken basin

Context. The Yutu-2 rover of the Chang'E-4 (CE-4) mission measured the lunar phase curves in the Von Karman crater, South Pole-Aitken basin. Aims. We aim to study the photometric properties of the regolith at CE-4's landing site and compare them with those of Chang'E-3 (CE-3) in order...

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Bibliographic Details
Published in:Astronomy & Astrophysics
Main Authors: Jiang, Te, Hu, Xiaoyi, Zhang, Hao, Ma, Pei, Li, Chunlai, Ren, Xin, Liu, Bin, Liu, Dawei, Yang, Jianfeng, Xue, Bin, Jin, Weidong, Zhu, Meng-Hua, Huang, Changning, Lin, Hongyu
Format: Report
Language:English
Published: EDP SCIENCES S A 2021
Subjects:
Moon
planets and satellites: surfaces
radiative transfer
techniques: photometric
Aitken
South Pole
South pole
Online Access:http://ir.opt.ac.cn/handle/181661/94520
https://doi.org/10.1051/0004-6361/202039252
Description
Summary:Context. The Yutu-2 rover of the Chang'E-4 (CE-4) mission measured the lunar phase curves in the Von Karman crater, South Pole-Aitken basin. Aims. We aim to study the photometric properties of the regolith at CE-4's landing site and compare them with those of Chang'E-3 (CE-3) in order to understand the regolith physical properties of the two landing sites. Methods. We extracted the insitu lunar phase curves measured by CE-4 with a very wide phase angle coverage (1 degrees-144 degrees) and performed photometric model inversions using both the Hapke model and the Lumme-Bowell model. Results. Compared with the CE-3 measurement taken in Mare Imbrium, the CE-4 phase curves show the colorimetric opposition effect and have a steeper and narrower opposition spike. The surface regolith at the CE-4 site is much darker, more porous, more forward scattering, and has a larger slope angle (Hapke model) than that of CE-3. Conclusions. The CE-4 site may have experienced more space weathering alterations than the CE-3 site, which is consistent with their different surface model ages (similar to 3.6 Ga for CE-4 and similar to 3 Ga for CE-3).

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