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temperature dependence of individual absorptions bands in olivine: implications for inferring compositions of asteroid surfaces from spectraThe temperature variations of individual absorptions in olivine are modeled and found to narrow, move slightly in position, and change in relative strength as predicted by theory. These thermal changes may be confused with compositional differences.
Document ID
20000081595
Document Type
Conference Paper
Authors
Sunshine, J. M.
(Science Applications International Corp. Chantilly, VA United States)
Hinrichs, J. L.
(Hawaii Univ. Honolulu, HI United States)
Lucey, P. G.
(Hawaii Univ. Honolulu, HI United States)
Date Acquired
August 19, 2013
Publication Date
March 1, 2000
Publication Information
Publication: Lunar and Planetary Science XXXI
Subject Category
Lunar and Planetary Science and Exploration
Funding Number(s)
CONTRACT_GRANT: NASA Order W-91534
CONTRACT_GRANT: NAG5-4212
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle20000080557Analytic PrimaryLunar and Planetary Science XXXI