LITHOSPHERIC STRUCTURE CONTROL ON CHANGES IN MAGMA SOURCE OVER TWO MAGMATIC PULSES IN THE WHITE–INYO RANGE, CA
Jurassic plutons of the WIR are characteristically amphibole-bearing gabbros to granites. Whole rock ƐNdi values of Jurassic plutons reflect a relatively juvenile source with values ranging from –0.15 to –8.32, 87Sr/86Sri ranging from 0.7045 to 0.7074, and 206Pb/204Pbi ranging from 18.55 to 19.26. Comparatively, Cretaceous plutons are dominantly aluminous, two-mica granitoids. Isotopic ratios for the Cretaceous plutons fall into two ranges, and the plutons are spatially distributed. In the southern WIR, the ƐNdi values range from –18.6 to –20.1, 87Sr/86Sri from 0.7110 to 0.7122, and 206Pb/204Pbi from 17.59 to 17.70. These ratios are atypical of the region in that they reflect an older, Paleozoic to Proterozoic crustal source. Contrastingly, Cretaceous plutons of the northern WIR have ƐNdi values that range from –5.76 to –9.19, 87Sr/86Sri from 0.7071 to 0.7080, and 206Pb/204Pbi from 18.52 to 19.11, reflecting a source like that for the Jurassic plutons.
We propose that the lower lithosphere below the WIR during the Jurassic was juvenile, but inhomogeneous in major and trace elements, perhaps due to underplating of compositionally heterogeneous material to the lithosphere. In contrast, the isotopic ratios of southern Cretaceous plutons suggest melting of upper-crustal sedimentary units with Proterozoic provenance. The sedimentary units in the WIR have ƐNdi values of –18.0 to –20.9 that match those of the plutons. The transition to a sedimentary source for some plutons in the WIR between the Jurassic and Cretaceous eras suggests heating of the crust, perhaps due to thickening during tectonic compression.