T141 From Stardust to Planets: A Geological Tour of the Career of Harry Y. McSween Jr.
Monday, 26 September 2016
1:30 PM - 5:30 PM
Room 201
ARE THE HEDS AND THE IIIABS KEEPING IT ALL IN THE FAMILY?
Paper number: T141-5
Program: Technical Sessions
Time: 2:30 PM – 2:45 PM
Authors
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Timothy J. McCoySmithsonian Institution, Washington, DC
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Catherine CorriganSmithsonian Institution, Washington, DC
Abstract
Puente del Zacate, a IIIAB iron meteorite, contains a primitive silicate clast. If the HEDs and the IIIABs are genetically linked, the chondritic compositions of Puente del Zacate silicates, when partially melted, should produce HED-like basaltic materials. MELTS modeling using the bulk composition of Puente del Zacate determined by Olsen et al. (1996) was conducted to test the proposed IIIAB-HED relationship. The Fe/Mg of the melts produced from Puente del Zacate is around 0.1. While some diogenites contain orthopyroxenes with Fe/Mg as low as 0.19, no HED silicates have values as low as the Puente del Zacate melts. In fact, the eucrites have even higher Fe/Mg values that vary from 0.4 to 2, with the lower end of the range representing the cumulate eucrites. This indicates that FeO-poor chondritic starting materials, like Puente del Zacate, cannot produce melts as FeO-rich as the HEDs, eliminating them as possible source materials. This further strengthens the argument that the IIIABs and HEDs do not originate from the same parent body.
Geological Society of America Abstracts with Programs. Vol. 48, No. 7
doi: 10.1130/abs/2016AM-283284
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