Results 121 to 130 of about 274 (137)
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Lunar and Martian Surfaces: Petrologic Significance of Absorption Bands in the Near-Infrared

Science, 1968
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
openaire   +2 more sources

Tracing the source of Apollo lunar soil (E21): Petrological evidence

Acta Petrologica Sinica, 2022
CHEN Yi   +8 more
openaire   +1 more source

Petrology of Lunar Soils

Collected Reprint Series, 1977
Collected Reprint Series
exaly  

Geochemistry, petrology and ages of the lunar meteorites Kalahari 008 and 009: New constraints on early lunar evolution

Geochimica Et Cosmochimica Acta, 2008
Vera A Fernandes   +2 more
exaly  

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