2022
DOI: 10.3847/2041-8213/ac6e6c
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Radiative Transfer Modeling of Chang’e-4 Spectroscopic Observations and Interpretation of the South Pole-Aitken Compositional Anomaly

Abstract: Chang’e-4 landed in the Von Kármán basaltic zone affected by Finsen ejecta from the South Pole-Aitken (SPA) “compositional anomaly” (SPACA), providing an opportunity to untangle the origin of the SPACA. We developed a mineral abundance unmixing model and built a spectral library composed of mineral mixtures of plagioclase, low-Ca pyroxene, high-Ca pyroxene, and olivine. Based on the mineral abundances returned by our model, the average plagioclase abundance (60.4 vol.%) of SPACA is beyond the high-plagioclase … Show more

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Cited by 10 publications
(4 citation statements)
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“…In addition, VNIS is not sensitive to Fsp, and the visible and near‐infrared spectral peaks of silicate minerals partially overlap. Quantitative mineralogical using VNIS data sometimes lead to inconsistent results (Chen et al., 2022; Gou et al., 2019).…”
Section: Discussionmentioning
confidence: 99%
“…In addition, VNIS is not sensitive to Fsp, and the visible and near‐infrared spectral peaks of silicate minerals partially overlap. Quantitative mineralogical using VNIS data sometimes lead to inconsistent results (Chen et al., 2022; Gou et al., 2019).…”
Section: Discussionmentioning
confidence: 99%
“…Among its various characteristics, the Lunar South Polar Region's Microelement anomaly associated with the interior of the Lunar South Polar Region has attracted wide attention from the lunar scientific community . [7] Therefore, a series of related problems such as water and microelement in the moon and the existence of water (ice) in the permanent shadow region have always been the focus of international academic research and the focus of future engineering tasks. There are a large number of impact craters in the South Pole of the moon, many of which belong to permanent shadow region, which is an important place to reveal the above scientific problems and evaluate future resources.…”
Section: Conclusion and Perspectivementioning
confidence: 99%
“…Then, some significant dark/shadow pixels need to be removed before calculating the average VNIR reflectance in the field of view of SWIR detectors. Here, we regard the pixels with REFFs at 465 nm less than 0.02 as shadows 83 . The average VNIR reflectance is adjusted to SWIR with the overlapping points using linear regression fitting to acquire a continuous spectrum (Supplementary Fig.…”
Section: Rover Locomotion Simulationmentioning
confidence: 99%