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Mercury - Surface composition from the reflection spectrum.The reflection spectrum for the integral disk of the planet Mercury was measured and was found to have a constant positive slope from 0.32 to 1.05 micrometers, except for absorption features in the infrared. The reflectivity curve matches closely the curve for the lunar upland and mare regions. Thus, the surface of Mercury is probably covered with a lunar-like soil rich in dark glasses of high iron and titanium content. Pyroxene is probably the dominant mafic mineral.
Document ID
19730027618
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Mccord, T. B.
Adams, J. B.
(Fairleigh Dickinson University St. Croix, Virgin Islands, United States)
Date Acquired
August 7, 2013
Publication Date
November 17, 1972
Publication Information
Publication: Science
Volume: 178
Subject Category
Space Sciences
Accession Number
73A12420
Funding Number(s)
CONTRACT_GRANT: NGR-22-009-350
Distribution Limits
Public
Copyright
Other

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