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Science 29 March 1968:
Vol. 159. no. 3822, pp. 1453 - 1455
DOI: 10.1126/science.159.3822.1453

Articles

Lunar and Martian Surfaces: Petrologic Significance of Absorption Bands in the Near-Infrared

John B. Adams 1

1 Jet Propulsion Laboratory, California Institute of Technology, Pasadena 91103

A reflection minimum at 1 micron, reported for Moon and for Mars, indicates olivine or iron- and calcium-bearing clinopyroxene, or both—major constituents of many basaltic rocks. If the 1-micron absorption features are real, both chondritic and acidic rocks are ruled out as primary constituents of the surfaces of the bodies. The reflectance spectrum of Mars matches closely that of an oxidized basalt.


THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
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Asteroids: Surface Composition from Reflection Spectroscopy.
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Spectral Reflectivity of Lunar Samples.
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Chemical Composition of the Lunar Surface in Sinus Medii.
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Preliminary Examination of Lunar Samples from Apollo 11.
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Spectral Reflectivity of Mars.
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Martian Surface Materials: Effect of Particle Size on Spectral Behavior.
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