Deriving asteroid mineralogies from reflectance spectra: Implications for the MUSES-C target asteroid

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概要

• 論文の詳細を見る

• In an effort to both bolster the spectral database on ordinary chondrites and constrain our ability to deconvolve modal, mineral chemistry and bulk chemical composition information from ordinary chondrites, we have initiated a spectral study of samples with known bulk compositions from the Smithsonian Institution's Analyzed Meteorite Powder collection. In this paper, we focus on deriving a better formula for determining asteroid mineralogies from reflectance spectra. The MUSES-C mission to asteroid 25143 1998 SF36 will allow any derived mineralogies to be tested with a returned sample.

• 国立極地研究所の論文

著者

• Sunshine Jessica

  Advanced Technology Applications Division Science Applications International Corporation

• Mccoy Timothy

  Department Of Mineral Sciences Mrc 119 National Museum Of Natural History Smithsonian Institution

• Mccoy Timothy

  Department Of Mineral Sciences National Museum Of Natural History Smithsonian Institution

• Jarosewich Eugene

  Department Of Mineral Sciences National Museum Of Natural History Smithsonian Institution

• Burbine Thomas

  Department of Mineral Sciences, National Museum of Natural History, Smithsonian Institution

• Burbine Thomas

  Department Of Mineral Sciences National Museum Of Natural History Smithsonian Institution

関連論文

• Deriving asteroid mineralogies from reflectance spectra: Implications for the MUSES-C target asteroid
• A pyroxene-oldhamite clast in Bustee: Igneous aubritic oldhamite and a mechanism for the Ti enrichment in aubritic troilite

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