T290 Impact Cratering on Earth and throughout the Solar System
Wednesday, 28 September 2016
8:00 AM - 12:00 PM
Room 201
INSIGHTS INTO IMPACT MELT CONDITIONS FROM DISSOCIATED ZIRCON IN MEDIEVAL TIN SLAG
Paper number: T290-15
Program: Technical Sessions
Time: 11:30 AM – 11:45 AM
Authors
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Nick TimmsCurtin University, Perth
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Dori FarthingSUNY Geneseo, Geneseo, NY
Abstract
Dissociated zircon grains contain 5 to 20 µm-wide coronas of 1-5 µm-size grains of rounded and twinned baddeleyite surrounded by glass. Two types of cores were documented in zircon grains that partially dissociated. Most cores preserve inherited oscillatory zoning, with evidence of localized infiltration of melt along discrete fractures. In one dissociated zircon, primary igneous zoning in the core is absent, and high-strain domains are irregularly interspersed with newly formed low-strain domains that contain cryptic oscillatory zoning. Regions of the modified core recrystallized to a granular texture of interlocking neoblasts. Many features observed in the slag zircon population are observed in zircon from impact melt, such as coronas of twinned baddeleyite surrounding inherited cores [2]. As shown here, both dissociation and granular texture can occur when zircon is immersed in high temperature melt, and are not unique to shock deformation. We are now characterizing the glass to evaluate chemical disequilibrium.
Supported by NSF (EAR-1145118), NASA Astrobiology, a Curtin Research Fellowship, and SUNY Geneseo.
[1] Gibson et al. 1997 [2] Timms et al. 2016 in review [3] Kaiser et al. 2008 [4] Tylecote et al. 1989 [5] Farthing and Pivarunas 2015
Geological Society of America Abstracts with Programs. Vol. 48, No. 7
doi: 10.1130/abs/2016AM-282161
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