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Lunar Surface Features: Mid-Infrared Spectral Observations
Author(s) -
Graham R. Hunt,
John W. Salisbury
Publication year - 1964
Publication title -
science
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 12.556
H-Index - 1186
eISSN - 1095-9203
pISSN - 0036-8075
DOI - 10.1126/science.146.3644.641
Subject(s) - infrared , wavelength , remote sensing , astrobiology , infrared window , surface (topology) , window (computing) , geology , environmental science , materials science , optics , physics , computer science , geometry , mathematics , operating system
The moon has been observed and spectrally scanned at midinfrared wavelengths, in particular through the 16- to 24-micron atmospheric window. The data indicate that there are differences in mineral composition among several features of the lunar surface.

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