Infrared spectra of carbonaceous chondrites and the composition of interstellar grains

Details Infrared spectra of carbonaceous chondrites and the composition of interstellar grains Infrared spectra of carbonaceous chondrites and the composition of interstellar grains

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ap%26ss..37....3z&link_type=abstract

Astrophysics and Space Science, vol. 37, Oct. 1975, p. 3-9.

Astronomy and Astrophysics

Astrophysics

32

Carbonaceous Chondrites, Infrared Spectra, Interstellar Matter, Meteoritic Composition, Silicates, Absorption Spectra, Cosmic Dust, Interstellar Extinction, Olivine

Scientific paper

Infrared spectra (7 to 40 microns) of the Cold Bokkeveld, Murray, and
Orgueil carbonaceous chondrites are compared with phyllosilicate-mineral
and interstellar-grain spectra. Similarities in the position and shape
of the silicate feature near 9.8 microns suggest that similar silicate
minerals are present in primitive meteorites and the interstellar dust.

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