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Specific surface area as a maturity index of lunar finesMature surface fines have an equilibrium specific surface area of about 0.6 sq m/g the equivalent mean particle size being about 3 microns. The adsorption behavior of inert gases (reversible isotherms) indicates that the particles are also nonporous in the size range of pores from 10 to 3000 A. Apparently, in mature soils there is a balance in the forces which cause fining, attrition, pore filling, and growth of lunar dust grains. Immature, lightly irradiated soils usually have coarser grains which reduce in size as aging proceeds. The specific surface area, determined by nitrogen or krypton sorption at 77 K, is a valuable index of soil maturity.
Document ID
19760027515
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Gammage, R. B.
(Holifield National Lab. Oak Ridge, TN, United States)
Holmes, H. F.
(Holifield National Laboratory Oak Ridge, Tenn., United States)
Date Acquired
August 8, 2013
Publication Date
October 1, 1975
Publication Information
Publication: Earth and Planetary Science Letters
Volume: 27
Issue: 3, Oc
Subject Category
Lunar And Planetary Exploration
Accession Number
76A10481
Distribution Limits
Public
Copyright
Other

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