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Subophitic basalts from Mare Crisium - Cooling ratesSubophitic basalt is the most common rock type at Mare Crisium. The cooling rate of a sample of this rock was determined by: (1) an olivine cooling speedometer and (2) Zr partitioning between ilmenite and ulvospinel. The kinetic modeling of the olivine cooling speedometer starts with a calculation of the compositional profile of olivine (the 'as-solidified profile') and proceeds to re-equilibration by diffusion as a function of cooling rate. The estimated cooling rate for subophitic basalts from the Luna 24 site is in the range of 2 C/day (about 0.1 C/hr), which is reasonably well corroborated by dynamic crystallization studies of Grove (1978).
Document ID
19790048521
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Taylor, L. A.
(Tennessee Univ. Knoxville, TN, United States)
Coish, R. A.
(Tennessee, University Knoxville, Tenn., United States)
Onorato, P. I. K.
(Tennessee Univ. Knoxville, TN, United States)
Uhlmann, D. R.
(MIT Cambridge, Mass., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1978
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Mare Crisium: The view from Luna 24; Conference
Location: Houston, TX
Start Date: December 1, 1977
End Date: December 3, 1977
Sponsors: NSF
Accession Number
79A32534
Funding Number(s)
CONTRACT_GRANT: NGR-22-009-646
CONTRACT_GRANT: NGL-43-001-140
Distribution Limits
Public
Copyright
Other

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