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Origin of the Station 7 boulder - A noteThe origin of the matrix types from the Apollo 17 Station 7 boulder is considered along with the origin of boulder material from Station 2, Boulder 1, and 73215. It is pointed out that the formation of the matrix rocks in this boulder and in the other Apollo 17 boulders in a single impact event is consistent with the isotopic evidence, ages, major-element chemistry, large ion lithophile (LIL) trace-element abundances, and textures. It had been suggested by Winzer et al. (1974), based on calculations from crystal-liquid partition coefficients for LIL trace elements, that target rocks corresponding in trace-element composition to the matrix types could have been produced by partial fusion of rocks similar to 77215. Using the same type of calculation, liquids quite similar in trace-element composition to the Station 7 boulder matrix types can be produced.
Document ID
19780062729
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Winzer, S. R.
(Martin Marietta Laboratories Baltimore, Md., United States)
Nava, D. F.
(Martin Marietta Labs. Baltimore, MD, United States)
Schuhmann, S.
(Martin Marietta Labs. Baltimore, MD, United States)
Lum, R. K. L.
(Martin Marietta Labs. Baltimore, MD, United States)
Philpotts, J. A.
(NASA Goddard Space Flight Center Greenbelt, Md., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1975
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 17, 1975
End Date: March 21, 1975
Accession Number
78A46638
Distribution Limits
Public
Copyright
Other

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