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Petrology of a stratified boulder from South Massif, Taurus-LittrowBoulder 1 from Station 2 at the foot of South Massif is unique in being the only stratified boulder sampled by the Apollo 17 astronauts. Our studies of two of the four specimens that were collected from separate layers show that the boulder is composed of glass-poor, fragment-rich breccias which are aggregates of differentially annealed terra material, mainly ANT, but including basaltic troctolite, pigeonite basalt, granitic particles, dark breccia-rimmed anorthositic clasts, and a KREEPless norite that has not been recognized elsewhere at the Apollo 17 site. The boulder appears to derive from the uppermost blue-gray layer on South Massif, which we believe consists of ejecta deposited from a single large impact event (possibly the one which excavated the Serenitatis Basin).
Document ID
19750055493
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Stoeser, D. B.
Marvin, U. B.
Wood, J. A.
Wolfe, R. W.
Bower, J. F.
(Smithsonian Astrophysical Observatory and Harvard College Observatory Cambridge, Mass., United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1974
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 18, 1974
End Date: March 22, 1974
Accession Number
75A39565
Funding Number(s)
CONTRACT_GRANT: NGL-09-015-150
Distribution Limits
Public
Copyright
Other

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