T189 Planetary Geology Division's G.K. Gilbert Award Session in Honor of Dr. Allan Treiman: A Long Strange Trip
Tuesday, 11 October 2022
1:30 PM - 5:30 PM
501
FORMATION, EQUILIBRATION, AND EVOLUTION OF LUNAR METEORITES AND METAMORPHIC ROCKS
Paper number: T189-14
Program: Technical Sessions
Time: 4:30 PM – 4:45 PM
Authors
Abstract
Lunar meteorite Northwest Africa (NWA5000) is a polymict leucogabbronorite breccia that is unique in its high concentrations (2%) of metal. Mineralogically, NWA5000 contains >200µm anorthite (An96) fragments that are interpreted to be unmelted, refractory lunar highlands material surrounded by a ‘melt-rock’ texture of subophitic anorthite (An92), subhedral olivine, and interstitial augite and pigeonite. It is likely that NWA5000 formed via a series of impacts, first a large metal rich asteroid melted the lunar highlands, concentrating the metal, followed by a second impact, which brecciated the melt deposit, prior to the meteorite being ejected from the surface of the Moon to the Earth.
Under increasing pressure and temperature conditions, metamorphic rocks recrystallize such that their mineralogy and mineral compositions reflect the lowest energy state of the system. However, the atomic scale processes by which minerals recrystallize and equilibrate is not well understood. Garnet specifically, is an important mineral, as its composition reflects changing equilibration conditions in the crust, leading to its utility in interpreting the tectono-metamorphic evolution of terranes. Microstructural data on garnet-bearing metapelites reveals that garnet crystallizes with one of three crystal directions parallel to the foliation of the rock. Atomic-scale crystal structure models show that the crystal structure of garnet and muscovite (specifically the spacing and orientation of Al and Si atoms) is similar enough that garnet could crystallize by templating on the crystal structure of muscovite. This is then interpreted as an epitaxial relationship which reduces garnet’s energy barrier to nucleation.
Geological Society of America Abstracts with Programs. Vol. 54, No. 6
doi: 10.1130/abs/2022AM-380592
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