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Spectra of Fe-Ti silicate glasses - Implications to remote-sensing of planetary surfacesOptical spectra of synthetic Fe-Ti silicate glasses and the temperature variations of the spectral features were investigated. The spectra are assigned to absorptions due to crystal field (CF) transitions in Ti(3+), Fe(2+) in octahedral coordination, and Fe(2+) in tetrahedral coordination, and to metal-metal and oxygen-metal charge transfer (CT) transitions which contribute to the near ultraviolet absorption edge. Temperature variations of the optical bands have been studied to explore implications for remote sensing. Caution is urged in the use of the absorption edge as a measure of TiO2 concentrations on planetary surfaces and in regolith samples.
Document ID
19800039487
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Nolet, D. A.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Burns, R. G.
(MIT Cambridge, Mass., United States)
Flamm, S. L.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Besancon, J. R.
(Wellesley College Wellesley, Mass., United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1979
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Houston, TX
Start Date: March 19, 1979
End Date: March 23, 1979
Accession Number
80A23657
Funding Number(s)
CONTRACT_GRANT: NGR-22-009-551
Distribution Limits
Public
Copyright
Other

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