Petrography and Geochemistry of Lunar Meteorite Miller Range 13317

Miller Range (MIL) 13317 is a 32-g lunar meteorite collected during the 2013-2014 ANSMET (Antarctic Search for Meteorites) field season. It was initially described as having 25% black fusion crust covering a light- to dark-grey matrix, with numerous clasts ranging in size up to 1 cm; it was tenta-ti...

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Bibliographic Details
Main Authors: Zeigler, R. A., Korotev, R. L.
Format: Other/Unknown Material
Language:unknown
Published: 2016
Subjects:
Instrumentation and Photography
Lunar and Planetary Science and Exploration
Antarctic
Miller Range
Antarc*
Online Access:http://hdl.handle.net/2060/20160002393
Description
Summary:Miller Range (MIL) 13317 is a 32-g lunar meteorite collected during the 2013-2014 ANSMET (Antarctic Search for Meteorites) field season. It was initially described as having 25% black fusion crust covering a light- to dark-grey matrix, with numerous clasts ranging in size up to 1 cm; it was tenta-tively classified as a lunar anorthositic breccia. Here we present the petrography and geochemistry of MIL 13317, and examine possible pairing relationships with previously described lunar meteorites.

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