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Vesicles in Apollo 15 Green Glasses: The Nature of Ancient Lunar Gases

Authors :
Thomas-Keprta, K. L
Clemett, S. J
Berger, E. L
Rahman, Z
McKay, D. S
Gibson, E. K
Wentworth, S. J
Publication Year :
2014
Publisher :
United States: NASA Center for Aerospace Information (CASI), 2014.

Abstract

Detailed studies of Apollo 15 green glass and related beads have shown they were formed in gas-rich fire fountains.. As the magmatic fluid became super-saturated in volatile gas, bubbles or vesicles formed within the magma. These exsolved gases became trapped within vesicles as the glasses were ejected from the fire-fountain and subsequently quenched. One of the keys to understanding formation processes on the ancient moon includes determining the composition of volatile species and elements, including metals, dissolved in magmatic gases. Here we report the nature of mineral phases spatially associated with vesicles in a green glass bead from Apollo sample 15411,42. The phases reflect the composition of the cooling/degassing magmatic vapors and fluids present at the time of bead formation approx, 3 Ga ago

Details

Language :
English
Database :
NASA Technical Reports
Publication Type :
Report
Accession number :
edsnas.20140012598
Document Type :
Report