T337 Impact Cratering on Earth and throughout the Solar System (Posters)
Wednesday, 28 September 2016
9:00 AM - 6:30 PM
Exhibit Hall E/F
IMPACT PLUME CHEMISTRY DETERMINED FROM FERROPSEUDOBROOKITE INCLUSIONS IN ACCRETIONARY SPHERULES AT THE CRETACEOUS-PALEOGENE BOUNDARY, SOUTH CAROLINA
Paper number: T337-10
Program: Technical Sessions
Time: 9:00 AM – 6:30 PM
Authors
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Steven J. JaretStony Brook University, Stony Brook, NY
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Christopher J. FleisherUniversity of Georgia, Athens, GA
Abstract
An unusual population of Ti-Fe oxides most clearly shows the high-T history of the spherules. Quantitative composition (WDS) data were collected using a JEOL 8600 electron microprobe. The data show that the dominant phase is ferropseudobrookite, Fe0.75Ti2.1O5. The grains contain elevated Cr (1360-4260 ppm) and occasionally Ni (~1200 ppm). Stoichiometry suggests that all iron is divalent and some of the titanium is reduced. Assuming plume conditions approximating equilibrium at high T and applying a number of FeO-TiO thermometers, a range of temperatures was calculated between 1259 ̊C and 1505 ̊C. These conditions, and correspondingly low fO2, are consistent with the observation of native Fe, Ni, and Al-Mg alloy in the spherules. Abundant graphite veins in the ferropseudobrookite can then be explained by reduction of a carbonate-rich fluid, the likely matrix material ultimately replaced by phosphate. As many Cretaceous-Paleogene “melt” ejecta seem to have altered to goyazite, we are investigating the timing of diagenesis to determine if something was unique about the post-impact environment endemic to the Chicxulub event.
Although the ferropseudobrookite may be explained by high T and low fO2 in the impact plume, it also is possible that they were inherited from the bolide. The coexisting Ti-Fe phase is a Cr, Nb-rich rutile, most commonly derived from deep mantle or meteoritic sources.
Geological Society of America Abstracts with Programs. Vol. 48, No. 7
doi: 10.1130/abs/2016AM-286266
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