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Gravity and Thermal Models of the Twin Peaks Magma System, West-Central Utah

Carrier, D. L.; Chapman, D. S.

Key words
Exploration; USA; Utah; Twin Peaks; Geophysical Surveys; Gravity; Heat Flow; Geochemical Surveys; Geological Surveys
Location
Twin Peaks, Utah
Conference
Geothermal Resources Council Transactions
Year
1980
Session
Exploration; Geophysical surveys; Volcanism; Gravity surveys
Language
English

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Abstract

Gravity, heat flow, surface geology, and geochemistry have been integrated to evaluation geothermal potential of a site of late Tertiary silicic volcanism at Twin Peaks, Utah. Volcanism began in the area with the extrusion of the Coyote Hills rhyolite 2.74 +/- .1 m.y. ago, and was resumed, after .2 m.y. of quiescence, with extrusion of a complex sequence of domes and flows that lasted until 2.35 +/- .07 m.y. ago. Residual gravity in the Twin Peaks area is characterized by a roughly circular and broad 7 mgal gravity low possibly related to a body approximated by a three dimensional vertical cylinder with a roof at a depth of 3 km, ad radius about 6 km, and a thickness of 2.25-3.5 km. Simple conductive thermal models predict a maximum anomalous heat flow of 175 mW/m2 at the surface, 90,000 years after emplacement of the intrusions. Model prediction of negligible residual heat flow at the present is consistent with measured heat flow of 96mW/m2 at Twin Peaks, which is indistinguishable from background Basin and Range heat flow.

Copyright 1980, Geothermal Resources Council. Readers who download papers from this site should honour the copyright of the original authors, and may not copy or distribute the work further without the permission of the original publisher.

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