1988
DOI: 10.1130/0016-7606(1988)100<0938:fotmac>2.3.co;2
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Fragments of the mantle and crust from beneath the Sierra Nevada batholith: Xenoliths in a volcanic pipe near Big Creek, California

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Cited by 61 publications
(31 citation statements)
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“…The Cretaceous Sierra Nevada batholith was once underlain by a thick layer of mafic cumulates in the form of garnet-pyroxenites making up the lower crust and parts of the lithospheric mantle (Figures 2(a) and 3; Dodge et al, 1988;Ducea, 2001Ducea, , 2002Saleeby, 1996, 1998b;Lee et al, 2006Lee et al, , 2007Mukhopadhyay and Manton, 1994). These cumulates have been shown to be petrogenetically linked to the granodioritic plutons dominating the batholith (Ducea, 2002;Ducea and Saleeby, 1998b;Lee et al, 2006Lee et al, , 2007.…”
Section: Sierra Nevada Californiamentioning
confidence: 98%
“…The Cretaceous Sierra Nevada batholith was once underlain by a thick layer of mafic cumulates in the form of garnet-pyroxenites making up the lower crust and parts of the lithospheric mantle (Figures 2(a) and 3; Dodge et al, 1988;Ducea, 2001Ducea, , 2002Saleeby, 1996, 1998b;Lee et al, 2006Lee et al, , 2007Mukhopadhyay and Manton, 1994). These cumulates have been shown to be petrogenetically linked to the granodioritic plutons dominating the batholith (Ducea, 2002;Ducea and Saleeby, 1998b;Lee et al, 2006Lee et al, , 2007.…”
Section: Sierra Nevada Californiamentioning
confidence: 98%
“…Pressure-temperature SCIENCE VOL. 271 data for CS garnet peridotites and garnet websterites (19) yield an adiabatic slope (Trend B, Fig. 5), suggesting that the convective upper mantle was as shallow as -60 km.…”
mentioning
confidence: 98%
“…Xenoliths from Late Cenozoic volcanic flows from the central Sierra (CS suite), the High Sierra, Owens Valley, and Inyo Mountains (HS suite) show variations in texture, composition, and thermal history consistent with the MT and seismic anomalies. The CS suite includes feldspathic granulites, garnet-pyroxenites, eclogites, cumulate gabbros and amphibolites, garnet and spinel peridotites, and garnet websterites (18)(19)(20). The HS suite includes spinel lhetzolites, hatzburgites, spinel dunites, spinel webterites, clinopyroxenites, gabbros, and mafic granulites, but lacks garnet.…”
mentioning
confidence: 99%
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“…There are three groups of xenoliths: garnet pyroxenites and garnet peridotites (both erupted before 8 Ma) constituting the old mantle lithosphere (2,20) and fertile, olivine-rich, garnet-free spinel peridotites (erupted since 4 Ma) with an asthenospheric affinity (2). Chemically, the garnet and pyroxene in the pyroxenites tend to have low Mg, whereas the olivine in the peridotites has a higher Mg number (2).…”
mentioning
confidence: 98%