TY - JOUR
T1 - The distribution of radiogenic heat production as a function of depth in the Sierra Nevada Batholith, California
AU - Brady, Robert J.
AU - Ducea, Mihai N.
AU - Kidder, Steven B.
AU - Saleeby, Jason B.
N1 - Funding Information:
This research was partially supported by NSF grants EAR 00087347 (Ducea and Saleeby), EAR 0230383 (Saleeby), EAR 0087125 and EAR 0229470 (Ducea), and a California State University Bakersfield URC grant (Brady). The authors would like to thank D. Baron, R. Cox, F. Baumeister, and T. Kelly for assistance with analyses and data reduction and J. Ague for providing access to his database of Aluminum in hornblende barometry from the Sierra Nevada batholith. We would also like to thank two anonymous reviewers for their thorough and helpful comments.
PY - 2006/2
Y1 - 2006/2
N2 - Geochemical analyses and geobarometric determinations have been combined to create a depth vs. radiogenic heat production database for the Sierra Nevada batholith, California. This database shows that mean heat production values first increase, then decrease, with increasing depth. Heat production is ∼2 μW/m3 within the ∼3-km-thick volcanic pile at the top of the batholith, below which it increases to an average value of ∼3.5 μW/m3 at ∼5.5 km depth, then decreases to ∼0.5-1 μW/m3 at ∼15 km depth and remains at these values through the entire crust below 15 km. Below the crust, from depths of ∼40-125 km, the batholith's root and mantle wedge that coevolved beneath the batholith appears to have an average radiogenic heat production rate of ∼0.14 μW/m3. This is higher than the rates from most published xenolith studies, but reasonable given the presence of crustal components in the arc root assemblages. The pattern of radiogenic heat production interpreted from the depth vs. heat production database is not consistent with the downward-decreasing exponential distribution predicted from modeling of surface heat flow data. The interpreted distribution predicts a reasonable range of geothermal gradients and shows that essentially all of the present day surface heat flow from the Sierra Nevada could be generated within the ∼35 km thick crust. This requires a very low heat flux from the mantle, which is consistent with a model of cessation of Sierran magmatism during Laramide flat-slab subduction, followed by conductive cooling of the upper mantle for ∼70 m.y. The heat production variation with depth is principally due to large variations in uranium and thorium concentration; potassium is less variable in concentration within the Sierran crust, and produces relatively little of the heat in high heat production rocks. Because silica content is relatively constant through the upper ∼30 km of the Sierran batholith, while U, Th, and K concentrations are highly variable, radiogenic heat production does not vary directly with silica content.
AB - Geochemical analyses and geobarometric determinations have been combined to create a depth vs. radiogenic heat production database for the Sierra Nevada batholith, California. This database shows that mean heat production values first increase, then decrease, with increasing depth. Heat production is ∼2 μW/m3 within the ∼3-km-thick volcanic pile at the top of the batholith, below which it increases to an average value of ∼3.5 μW/m3 at ∼5.5 km depth, then decreases to ∼0.5-1 μW/m3 at ∼15 km depth and remains at these values through the entire crust below 15 km. Below the crust, from depths of ∼40-125 km, the batholith's root and mantle wedge that coevolved beneath the batholith appears to have an average radiogenic heat production rate of ∼0.14 μW/m3. This is higher than the rates from most published xenolith studies, but reasonable given the presence of crustal components in the arc root assemblages. The pattern of radiogenic heat production interpreted from the depth vs. heat production database is not consistent with the downward-decreasing exponential distribution predicted from modeling of surface heat flow data. The interpreted distribution predicts a reasonable range of geothermal gradients and shows that essentially all of the present day surface heat flow from the Sierra Nevada could be generated within the ∼35 km thick crust. This requires a very low heat flux from the mantle, which is consistent with a model of cessation of Sierran magmatism during Laramide flat-slab subduction, followed by conductive cooling of the upper mantle for ∼70 m.y. The heat production variation with depth is principally due to large variations in uranium and thorium concentration; potassium is less variable in concentration within the Sierran crust, and produces relatively little of the heat in high heat production rocks. Because silica content is relatively constant through the upper ∼30 km of the Sierran batholith, while U, Th, and K concentrations are highly variable, radiogenic heat production does not vary directly with silica content.
KW - Geothermal gradient
KW - Heat flow
KW - Heat producing elements
KW - Heat production
KW - Sierra Nevada
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U2 - 10.1016/j.lithos.2005.06.003
DO - 10.1016/j.lithos.2005.06.003
M3 - Article
AN - SCOPUS:30944455461
SN - 0024-4937
VL - 86
SP - 229
EP - 244
JO - Lithos
JF - Lithos
IS - 3-4
ER -