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Time and duration of lunar highlands crust formationDue to remaining uncertainties in model parameters and assumptions in the calculation of model ages, it is not yet possible to resolve the precise dating and duration of lunar crust-mantle differentiation phenomena. Norites 78236 and 73255,27,45 were examined utilizing the Sm-Nd radiometric system. The systematics of 78236 show post-crystallization disturbance but indicate a crystallization date 4.34 AE ago. An isochron is defined by the 73255,27,45 data, with a crystallization date of 4.23 AE. The initial Nd isotopic composition of both norites is within uncertainty limits for a 'chondritic' reference reservoir at the time of their respective crystallizations. The implications for lunar crustal formation persisting over a time span of nearly 350 million years are discussed.
Document ID
19810041387
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Carlson, R. W.
(California Univ. La Jolla, CA, United States)
Lugmair, G. W.
(California, University La Jolla, Calif., United States)
Date Acquired
August 11, 2013
Publication Date
February 1, 1981
Publication Information
Publication: Earth and Planetary Science Letters
Volume: 52
Issue: 2, Fe
Subject Category
Lunar And Planetary Exploration
Accession Number
81A25791
Funding Number(s)
CONTRACT_GRANT: NGL-05-009-150
Distribution Limits
Public
Copyright
Other

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