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Evidence for a Light-Rare-Earth-Element-Depleted Source for Some Ferroan AnorthositesIn the lunar magma ocean model, ferroan anorthosites (FANs) are expected to be derived from a relatively undifferentiated source with chondritic REE abundances and yield the oldest radiometric ages of any lunar rocks. Samarium-neodymium-isotopic analyses of 60025 and 67016 yielded ages of 4.44 +/- 0.02 Ga and 4.53 +/- 0.12 Ga and initial Epsilon(sub Nd)(sup 143) values in excess of -0.5. These ages are within error of ages determined on some Mg-suite rocks by researchers. Thus, the existing data are not completely consistent with the standard magma ocean model. We have completed isotopic analysis on the pristine FAN 62236 in order to place further constraints on lunar crust-forming processes.
Document ID
20000000492
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Borg, L. E.
(NASA Johnson Space Center Houston, TX United States)
Norman, M.
(MacQuarie Univ. Sydney, Australia)
Nyquist, L. E.
(NASA Johnson Space Center Houston, TX United States)
Bogard, D.
(NASA Johnson Space Center Houston, TX United States)
Snyder, G.
(Tennessee Univ. Knoxville, TN United States)
Taylor, L.
(Tennessee Univ. Knoxville, TN United States)
Date Acquired
August 19, 2013
Publication Date
January 1, 1998
Publication Information
Publication: Origin of the Earth and Moon
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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