HR: 11:50h
AN: V52B-07    [Abstracts]
TI: Short Timescales of High-silica Rhyolite Generation in the Mono-Inyo Craters Indicated by U-Th Isotopic Disequilibrium
AU: * Hart, G L
EM: ghart@wsu.edu
AF: Washington State University, 1228 Webster, Pullman, WA 99164 United States
AU: DePaolo, D J
EM: depaolo@eps.berkeley.edu
AF: University of California, 473 McCone Hall, Berkeley, CA 94720 United States
AU: DePaolo, D J
EM: depaolo@eps.berkeley.edu
AF: Lawrence Berkeley National Laboratory, 1 Cyclotron Rd, MS 70A-4418, Berkeley, CA 94720 United States
AU: Christensen, J N
EM: jnchristensen@lbl.gov
AF: Lawrence Berkeley National Laboratory, 1 Cyclotron Rd, MS 70A-4418, Berkeley, CA 94720 United States
AB: Uranium and Th isotope measurements for some of the youngest basaltic- to rhyolitic lava flows associated with the Long Valley caldera and Mono-Inyo Craters indicate that the lavas have pronounced U and Th isotopic disequilibrium. The (238U/232Th) activity ratios range from 0.69 to 1.23, and the (230Th/232Th) activity ratios range from 0.80 to 1.03. The majority of the lavas plot to the right of the equiline, which corresponds with a subduction zone influence on the U and Th isotope compositions. A basaltic inclusion from the Mono Inyo dacite (age = 18 Ka, epsilon-Nd = +2) is one of the samples farthest to the right of the equiline, which indicates that the basaltic magmatism associated with the formation of the silicic magma system is subduction-like. In contrast, an older (ca. 100 Ka) trachybasalt lava from the Long Valley north moat (epsilon-Nd= -3) plots to the left of the equiline. We interpret these differences as reflecting lithospheric sources for the small-volume alkalic lavas and asthenospheric (subduction-affected) sources for the larger volume silicic system. The preservation of strong U-Th isotopic disequilibrium in high-silica lavas clearly indicates that the rhyolites do not have long magma chamber residence times as has been inferred for other silicic systems in western North America. This observation is in accord with the young age of the Mono Craters (less than about 18 Ka) and suggests that this system has not yet stored up a large amount of silicic magma that could feed an eruption of Bishop Tuff size.
DE: 1749 Volcanology, geochemistry, and petrology
DE: 1040 Isotopic composition/chemistry
SC: Volcanology, Geochemistry, Petrology [V]
MN: 2004 AGU Fall Meeting