Optical absorption and chemical composition of some lunar glassy spherules

Details Optical absorption and chemical composition of some lunar glassy spherules Optical absorption and chemical composition of some lunar glassy spherules

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jmsl....7..227s&link_type=abstract

Journal of Materials Science Letters (ISSN 0261-8028), vol. 7, March 1988, p. 227-229.

Physics

Condensed Matter

Materials Science

Chemical Composition, Electromagnetic Absorption, Heat Treatment, Lunar Soil, Spherules, Vitreous Materials, Absorptivity, Lunar Dust, Refractivity

Scientific paper

Optical absorption measurements are conducted on lunar glassy spherules as a function of wavelength, in order to better understand the history of lunar glassy spherules at the lunar surface. The extinction coefficients of lunar glass calculated on the basis of the observational results obtained are found to lie within an order of magnitude of the values determined by Anderson-Kraft (1931) for ferric iron. The lack of exact agreement between the extinction coefficient and previous results may be due to the coefficient's dependence on composition.

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