23 Petrology and Planetary Geology (Posters)
Friday, 31 March 2017
8:00 AM - 12:00 PM
James River Ballroom
AN OVERVIEW OF THE TYPE II CHONDRULES IN THE CM CHONDRILTE JBILET WINSELWAN
Paper number: 23-4
Program: Technical Sessions
Time: 8:00 AM – 12:00 PM
Authors
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Amy L. FaganWestern Carolina University, Cullowhee, NC
Abstract
A total of 39 type II chondrules were identified between the two thin sections, ranging from ~40µm-1100µm in diameter. Not a single type II chondrule contained crystalline pyroxene with each being some subset of porphyritic olivine, contrary to the mean composition within the entire sample. Both individual grain size and degree of alteration apparently had no bearing on chondrule type. The primary difference observed between type I and II chondrules was the ubiquitous zoning in the latter. In a significant portion of type II chondrules, these relict core compositions roughly matched that of type I chondrule material while rim compositions ranged from roughly 15-45% less Mg. “Dusty” type zoned relict grains were also observed in a few chondrules, but they were not visually distinct enough from type I chondrules rich in metal blebs to be confidently labeled as more than just zoned examples of these chondrules.
The observations in this overview of type II chondrules in Jbilet Winselwan works to support the hypothesis that type II chondrules were derived from type I chondrite material. The ubiquitous zoning suggests either growth in a depleting system or external alteration of the crystals. This combined with the measurements showing the correlation between the cores of zoned relict grains and type I chondrule material, the relict fine grained aggregates, and the visual link between dusty relicts and Fe/Ni bleb-rich type I grains shows that the latter case is much more likely.
Geological Society of America Abstracts with Programs. Vol. 49, No. 3
doi: 10.1130/abs/2017SE-291370
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