T141 Rocks from Space! Using Meteorites to Understand the Physical, Chemical, and Mineralogical Evolution of Planetary Bodies
Wednesday, 28 October 2020
1:30 PM - 5:30 PM
Meeting Rooms
EVIDENCE FOR A CERES-SIZED, WATER-RICH, CARBONACEOUS CHONDRITE PARENT ASTEROID: A MISSING LINK FOUND IN THE ALMAHATA SITTA METEORITE
Paper number: T141-4
Program: Technical Sessions
Time: 2:15 PM – 2:30 PM
Authors
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Cyrena GoodrichLunar and Planetary Institute, USRA, Houston, TX
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Allan TreimanLunar and Planetary Institute, Houston, TX
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Harold C. ConnollyUniversity of Arizona, Glassboro, NJ
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Michael ZolenskyNASA Johnson Space Center, Houston, TX
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Muawia H. ShaddadUniversity of Khartoum, Khartoum
Abstract
The previous detection of amphibole in a CC, even at very low abundances, is noteworthy as it indicates that conditions for that mineral’s formation existed in the early solar system, no matter how briefly or how localized. However, our detection of abundant amphibole in a second CC that implicates a second, large parent body suggests that moderately elevated, hydrous P/T conditions may have been more widespread than previously thought based on meteorites. The apparent absence of amphibole in most carbonaceous chondrites may reflect bias in our meteorite collections and/or failure to identify it in other samples. Finally, samples like AhS 202 provide important missing links if spaceflight missions such as Hayabusa2 and OSIRIS-REx return samples that differ from what exists in meteorite collections.
Geological Society of America Abstracts with Programs. Vol. 52, No. 6
doi: 10.1130/abs/2020AM-356227
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