Laboratory study of silicates and application to cometary dust |
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Authors: | A Blanco V Orofino M Martino S Fonti and J R Stephens |
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Institution: | (1) Dipartimento di Fisica dell'Università, C.P. 193, 73100 Lecce, Italia;(2) Istituto di Fisica Sperimentale, IUN, Via Acton 38, 80133 Napoli, Italia;(3) Los Alamos National Laboratory, 87545 Los Alamos, NM, USA |
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Abstract: | Summary The mass absorption coefficients of some glassy and crystalline silicates of astrophysical relevance have been measured. We
produced and characterized also synthetic silicates of olivine type since this material is considered one of the most likely
components of cometary dust grains. The experimental data are used to fit the emission feature observed in the Comet Halley
spectrum between 8 and 13 μm. Satisfactory results are obtained by using synthetic olivine mixed with a small amount (5%)
of crystalline grains.
Paper presented at the V Cosmic Physics National Conference, S. Miniato, November 27–30, 1990. |
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Keywords: | Interplanetary space |
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