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Asteroid Vesta: Spectral Reflectivity and Compositional Implications

McCord, Thomas B., Adams, John B., Johnson, Torrence V.·1970·Science

Abstract

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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Metadata

Authors
McCord, T. B., Adams, J. B., & Johnson, T. V.
Venue
Science
Published
1970-06-19
Volume
168
Issue
3938
Pages
1445-1447
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W1996858864
Cited by
758
References
0
FWCI
9.10
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Asteroid Vesta: Spectral Reflectivity and Compositional Implications. https://app.cochat.ai/papers/10.1126/science.168.3938.1445
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McCord, T. B., Adams, J. B., & Johnson, T. V. (1970). Asteroid Vesta: Spectral Reflectivity and Compositional Implications. Science. https://doi.org/10.1126/science.168.3938.1445

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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