The Bholghati howardite: Chemical study

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Asteroid vesta: spectral reflectivity and compositional implications.

T McCord, J Adams, T. V. Johnson (1970)

The spectral reflectivity (0.30 to 1.10 microns) of several asteroids has been measured for the first time. The reflection spectrum for Vesta contains a strong absorption band centered near 0.9 micron and a weaker absorption feature between 0.5 and 0.6 micron. The reflectivity decreases strongly in the ultraviolet. The reflection spectrum for the asteroid Pallas and probably for Ceres does not contain the 0.9-micron band. Vesta shows the strongest and best-defined absorption bands yet seen in the reflection spectrum for the solid surface of an object in the solar system. The strong 0.9-micron band arises from electronic absorptions in ferrous iron on the M2 site of a magnesian pyroxene. Comparison with laboratory measurements on meteorites and Apollo 11 samples indicates that the surface of Vesta has a composition very similar to that of certain basaltic achondrites.

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Experimental petrology of eucritic meteorites

Edward Stolper (1977)

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The compositional classification of chondrites—I. The carbonaceous chondrite groups

Gregory W. Kallemeyn, John T. Wasson (1981)

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Author and article information

Journal

Title: Geochimica et Cosmochimica Acta

Abbreviated Title: Geochimica et Cosmochimica Acta

Publisher: Elsevier BV

ISSN (Print): 00167037

Publication date Created: August 1990

Publication date (Print): August 1990

Volume: 54

Issue: 8

Pages: 2167-2175

Article

DOI: 10.1016/0016-7037(90)90042-J

SO-VID: d2636ffb-4c2d-4630-8122-c5a857dc1339

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http://www.elsevier.com/tdm/userlicense/1.0/

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