1992
DOI: 10.1130/spe272-p107
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Using granite to image the thermal state of the source terrane

Abstract: It should be possible to infer the thermal state of the source terrane for granitic bodies, provided we have independent means to establish the chemical nature of this terrane. The chemical nature of the granitic rocks, including their degree of hydration, implies the solidus temperature. The concentration of the heat-producing radioactive elements in the granite (K, U, and Th) probably provides an upper estimate of their concentration in the source rock, which is an important thermal parameter. The depth and … Show more

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Cited by 4 publications
(4 citation statements)
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“…This distribution is consistent with an average melt loss of approximately 10 vol% from a source of a similar horizontal area or footprint that was approximately 10 km thick (e.g. Zen 1992); such an estimate ignores any mass input owing to melting of asthenosphere in the mantle wedge, which not only will reduce the proportion of lower crustal melt required, but also is the likely driver of crustal differentiation in arc-related settings (e.g. Kemp et al 2007).…”
Section: (B) the Length Scales And Time Scales Of Melt Flow And The Volumes Of Melt Involved In Inflating Plutonssupporting
confidence: 77%
“…This distribution is consistent with an average melt loss of approximately 10 vol% from a source of a similar horizontal area or footprint that was approximately 10 km thick (e.g. Zen 1992); such an estimate ignores any mass input owing to melting of asthenosphere in the mantle wedge, which not only will reduce the proportion of lower crustal melt required, but also is the likely driver of crustal differentiation in arc-related settings (e.g. Kemp et al 2007).…”
Section: (B) the Length Scales And Time Scales Of Melt Flow And The Volumes Of Melt Involved In Inflating Plutonssupporting
confidence: 77%
“…Initial Sr isotopic ratios for the Late Cretaceous Boulder batholith, including the Butte quartz monzonite, Marysville stock, and Hell Creek pluton range from 0.7055 to 0.7092, and are significantly lower than values for the Pioneer batholith (Doe et al 1968;Mueller et al 1997). A Proterozoic Pb isotopic model age for the Boulder batholith (2.1 ± 0.3 Ga) is similar to that of the Pioneer plutons (Zen 1992). Inherited zircons from several granitic intrusions in the Boulder batholith give abundant ca.…”
Section: Evidence For the Selway Terranementioning
confidence: 60%
“…Initial Sr isotopic values for the Late Cretaceous Pioneer batholith range from 0.7110 to 0.7160 (Arth et al 1986;Mueller et al 1997), and Pb isotopes give a model age of 1.9 ± 0.2 Ga (Doe et al 1968;Zen 1992). These results suggest involvement of mainly Paleoproterozoic crust, as do inherited zircon ages of -1.4 and 1.7-1.8 Ga (SHRIMP-II) for the Grayling Lake granite and Uphill Creek granodiorite reported by Murphy et al (2002).…”
Section: Evidence For the Selway Terranementioning
confidence: 99%
“…Consider a source of area of 10 3 -10 4 km 2 beneath which an average of 1 km 3 per km 2 of melt is extracted from 10 km depth of suprasolidus continental crust (e.g. Zen 1992). For a pluton that is 1 km thick, the melting footprint, the region of melt throughput and the pluton area are identical.…”
Section: Fluxesmentioning
confidence: 99%