15 Undergraduate Research Session (Posters)
Tuesday, 15 May 2018
8:30 AM - 6:30 PM
Outdoor Tents
OLIVINE CHEMISTRY OF INDIAN HEAVEN LAVAS, SOUTHERN WASHINGTON CASCADES
Paper number: 15-7
Program: Theme Sessions
Time: 8:30 AM – 6:30 PM
Authors
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Diane R. SmithTrinity University, San Antonio, TX
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Kurt KneselTrinity University, San Antonio, TX
Abstract
Temperatures and pressures were calculated by the methods described by Leeman et al. (2005) for samples with >7.5 wt % MgO; the two enigmatic samples noted above were excluded from these calculations. Pre-eruptive conditions range from 1210 to 1248°C and from 0.69 to 1.02 GPa, with no apparent relationship to basalt type (e.g., LKTs vs. IPBs). In contrast, segregation T-P estimates range from 1258 to 1473°C and from 0.96 to 2.41 GPa (corresponding to depths of ~32-80 km). There is a clear relationship between basalt type and segregation T-depth estimates. The deepest, hottest conditions (1369-1473°C and 55-80 km) are observed for the LKTs, with progressively lower T-depth estimates for IPBs (1303-1380°C and 37-60 km) and the SHOs (1258-1263°C and 32-34 km). These high segregation temperatures imply melting was triggered by decompression, consistent with the lack of slab-fluid input (Leeman et al. 2005).
Leeman, W.P., Lewis, J.F, Evarts, R.C., Conrey, R.M., and Streck, M.J., 2005, J. Volcanol. Geotherm. Res.: 140:67-105
Geological Society of America Abstracts with Programs. Vol. 50, No. 5
doi: 10.1130/abs/2018RM-313765
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