The Pelona, Orocopia, and Rand Schists and the schists of Portal Ridge and Sierra de Salinas constitute a high-pressure/temperature terrane that was accreted beneath North American basement in Late Cretaceous-earliest Tertiary time. The schists crop out in a belt extending from the southern Coast Ranges through the Mojave Desert, central Transverse Ranges, southeastern California, and southwestern Arizona. Ion microprobe U-Pb results from 850 detrital zircons from 40 metagraywackes demonstrates a Late Cretaceous to earliest Tertiary depositional age for the sedimentary part of the schist's protolith. About 40% of the 206 Pb/ 238 U spot ages are Late Cretaceous. The youngest detrital zircon ages and post-metamorphic mica 40 Ar/ 39 Ar cooling ages bracket when the schist's graywacke protolith was eroded from its source region, deposited, underthrust, accreted, and metamorphosed. This interval averages 13 ± 10 m.y. but locally is too short (<~3 m.y.) to be resolved with our meth-
ods. The timing of accretion decreases systematically (in palinspastically restored coordinates) from about 91 ± 1 Ma in the southwesternmost Sierra Nevada (San Emigdio Mountains) to 48 ± 5 Ma in southwest Arizona (Neversweat Ridge). Our results indicate two distinct source regions: (1) The Rand Schist and schists of Portal Ridge and Sierra de Salinas were derived from material eroded from Early to early Late Cretaceous basement (like the Sierra Nevada batholith); and (2) The OrocopiaSchist was derived from a heterogeneous assemblage of Proterozoic, Triassic, Jurassic, and latest Cretaceous to earliest Tertiary crystalline rocks (such as basement in the Mojave/Transverse Ranges/southwest Arizona/northern Sonora). The Pelona Schist is transitional between the two.