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Published 1976 | public
Book Section - Chapter

Alkali mobility in shocked basalt

Abstract

Plagioclase (An_(45)-An_(55)) in unshocked and experimentally shocked samples of Vacaville basalt was analyzed by electron microprobe. Sodium X-ray intensity measurements were found to be unstable for the diaplectic and shock-fused plagioclases, and for synthetic plagioclase glasses with An ≾ 80. Unstable microprobe analyses have also been reported for shocked chondritic meteorites. That is, sodium is mobilized and volatilized under the electron beam, probably by a thermal mechanism. Crystalline plagioclase, even when shocked to just below the transition pressure to diaplectic glass, gives stable analyses as does synthetic plagioclase glass with An > 80, and shocked calcic plagioclase in Apollo 16 sample 68415. In this study, we conclude that: (i) there is no evidence for selective sodium loss due to the shock process; (ii) sodium mobilization under the electron beam reflects increasingly severe lattice damage for increasing shock pressures; (iii) sodium mobilization is, in any case, not significant for calcic plagioclase. Thus we find no evidence supporting shock-related alkali loss as an important lunar process for impacts generating maximum pressures below about 1 Mbar, corresponding to projectile velocities ~4 km/sec for metallic objects and ⪝6 km/sec for silicate objects.

Additional Information

© 1976 Lunar and Planetary Institute. We would like to thank Arden Albee, A. A. Chodos, and George Rossman for advice and assistance in this study, as well as W. R. Van Schmus for his critical comments and suggestions. We appreciate technical assistance provided by David Johnson. This research was supported by NASA grants NGL-05-002-105 and NSG-9019. This paper constitutes the Division of Geological and Planetary Sciences Contribution no. 2709.

Additional details

Created:
August 19, 2023
Modified:
January 13, 2024