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Ar-39 - Ar-40 ages of acapulcoites and lodranites: Evidence for early parent body heating

Authors :
Bogard, D. D
Garrison, D. H
Mccoy, T. J
Keil, K
Source :
Lunar and Planetary Inst., Twenty-fourth Lunar and Planetary Science Conference. Part 1: A-F.
Publication Year :
1993
Publisher :
United States: NASA Center for Aerospace Information (CASI), 1993.

Abstract

New age dating of acapulcoites (Acapulco, Monument Draw) and lodranites (Gibson) allow us to reconstruct the history of their parent body in a chronological framework. These meteorites originated on a common parent body -4.55 Ga ago. Non-collisional heating caused partial melting, with lodranites having been heated slightly higher than acapulcoites. This parent body cooled to the Ar closure temperature at -4.51 Ga for acapulcoites and -4.48 Ga for lodranites. The difference in ages is consistent with the higher temperature and longer cooling time for lodranites. Cooling probably occurred at a few to tens of deg C/Ma, with slower cooling rates at lower temperatures.

Subjects

Subjects :
Geophysics

Details

Language :
English
Database :
NASA Technical Reports
Journal :
Lunar and Planetary Inst., Twenty-fourth Lunar and Planetary Science Conference. Part 1: A-F
Publication Type :
Report
Accession number :
edsnas.19940007611
Document Type :
Report