研究目的
Investigating the mineralogy of the Chang’e-4 landing site using visible and near-infrared imaging spectrometer (VNIS) data to understand the lunar interior.
研究成果
The ma?c components at the CE-4 landing site are clinopyroxene-bearing with intermediate composition, likely dominated by pigeonite. These findings suggest the materials are derived from rapid-cooling magmatic systems, possibly recrystallized from impact melt settings.
研究不足
The study is based on preliminary data from the Chang’e-4 mission, and the mineralogical interpretations are subject to further validation with more comprehensive datasets.
1:Experimental Design and Method Selection:
The study uses level 2B data from CE-4 VNIS for mineralogical analysis. A systematic processing pipeline is developed to derive credible reflectance spectra.
2:Sample Selection and Data Sources:
The data comes from the Yutu-2 rover's exploration area on the Moon's far side.
3:List of Experimental Equipment and Materials:
CE-4 VNIS instrument onboard the Yutu-2 rover.
4:Experimental Procedures and Operational Workflow:
Data processing includes in-flight radiometric calibration, solar distance correction, and continuum removal.
5:Data Analysis Methods:
Spectral and mineral indices are calculated to constrain the ma?c mineralogy.
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