This paper reports the results of attempts to model the spectral properties of the lunar regolith as consisting of crystalline rocks, glass and submicroscopic metallic iron (SMFe), produced by a process involving vapor phase differentiation. The models differ in the location of the SMFe.
Why is the Moon dark?
01.01.1993
Aufsatz (Konferenz)
Keine Angabe
Englisch
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