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Apollo 14 mineral ages and the thermal history of the Fra Mauro formation.

Authors :
Compston, W
Vernon, M. J
Berry, H
Rudowski, R
Gray, C. M
Ware, N
Chappell, B. W
Kaye, M
Publication Year :
1972
Publisher :
United States: NASA Center for Aerospace Information (CASI), 1972.

Abstract

The thermal inertia of the Fra Mauro formation limits its rate of cooling. The calculations of Jaeger (1961) for the cooling of an extrusive sheet are used to estimate the time required for a central temperature drop of 10%. This time is found to be about 45 years. For a 90% temperature drop, the time is about 200 years. Analytical methods used in the investigations are discussed together with the diffusion of Rb and Sr within lunar basalt. Isochron diagrams for various minerals are presented.

Subjects

Subjects :
Space Sciences

Details

Language :
English
Database :
NASA Technical Reports
Notes :
NSR-09-051-001
Publication Type :
Report
Accession number :
edsnas.19730034974
Document Type :
Report