Rb-Sr and Sm-Nd Isotopic Studies of Lunar Green and Orange GlassesLunar volcanic glassy beads have been considered as quenched basaltic magmas derived directly from deep lunar mantle during fire-fountaining eruptions [1]. Since these sub-mm size glassy melt droplets were cooled in a hot gaseous medium during free flight [2], they have not been subject to mineral fractionations. Thus, they represent primary magmas and are the best samples for the investigation of the lunar mantle. Previously, we presented preliminary Rb- Sr and Sm-Nd isotopic results for green and orange glassy samples from green glass clod 15426,63 and orange soil 74220,44, respectively [3]. Using these isotopic data, initial Sr-87/Sr-86 and Nd ratios for these pristine mare glass sources can be calculated from their respective crystallization ages previously determined by other age-dating techniques. These isotopic data were used to evaluate the mineralogy of the mantle sources. In this report, we analyzed additional glassy samples in order to further characterize isotopic signatures of their source regions. Also, we'll postulate a relationship between these two major mare basalt source mineralogies in the context of lunar magma ocean dynamics.
Document ID
20120001819
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Shih, C.-Y. (Jacobs Technologies Engineering Science Contract Group Houston, TX, United States)
Nyquist, L. E. (NASA Johnson Space Center Houston, TX, United States)
Reese, Y. (Muniz Engineering, Inc. Houston, TX, United States)
Date Acquired
August 25, 2013
Publication Date
January 1, 2012
Subject Category
Geophysics
Report/Patent Number
JSC-CN-25632Report Number: JSC-CN-25632
Meeting Information
Meeting: 43rd Lunar and Planetary Science Conference