Spectroscopic study of Apollo 16 and 17 lunar highland crust
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- Yamamoto Aya
- Remote Sensing Technology Center of Japan
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- Arai Tomoko
- National Institute of Polar Research
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- Takeda Hiroshi
- Chiba Institute of Technology
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- Miyamoto Masamichi
- Univ. of Tokyo
Bibliographic Information
- Other Title
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- 反射スペクトルで見る月表側地殻岩石の組織と組成の多様性
Abstract
To understand a correlation between reflectance spectra of Apollo samples that can be the ground truth data of the Moon and petrology and mineralogy of those samples is very important for analyzing remote sensing data such as SELENE. In this study, we measured UV/VIS/NIR reflectance spectra of five anorthosite samples from Apollo 16 landing sites, and examine the spectral result with their petrology and mineralogical compositions. Those samples show clear absorption feature of low-Ca pyroxene in their spectra except for 60025. These results indicate that anorthositic highland crust on the nearside of the moon shows various spectroscopic characteristics with brecciation and shock metamorphism.
Journal
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- Abstracts for fall meeting of the Japanese Society for Planetary Science
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Abstracts for fall meeting of the Japanese Society for Planetary Science 2006f (0), 17-17, 2006
THE JAPANESE SOCIETY FOR PLANETARY SCIENCES
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Details 詳細情報について
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- CRID
- 1390282680535508608
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- NII Article ID
- 130004636067
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- Data Source
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- JaLC
- CiNii Articles
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- Abstract License Flag
- Disallowed