EVIDENCE FOR LATE ADAKITE MAGMATISM IN THE TRIASSIC-JURASSIC ARC, SIERRA NEVADA CENTRAL BELT, CALIFORNIA
Mafic-to-intermediate dikes cross-cut the ultramafic and overlying sedimentary sections of the ophiolite. The dikes generally contain hornblende and plagioclase phenocrysts. Based on high MgO, Ni, Cr, Sr, and La/Yb from a small number of these dikes at a single locality, previous studies interpreted these rocks as boninites formed at the initiation of subduction. However, a reassessment of the data shows that the geochemistry does not match modern criteria for boninites, especially the high La/Yb, which is more consistent with adakitic magmatism.
Preliminary whole-rock geochemistry on a larger number of these dikes from multiple localities at Jarbo Gap, including several that cross-cut the sedimentary cover of the ophiolite, show these dikes to have mean values of SiO2=55%, Al2O3=15%, MgO=6%, Sr/Y=38, La/Yb=12, Sr=530 ppm, Ni=130 ppm, and Cr=240 ppm. Based on the high values of Sr/Y, La/Yb, MgO, Ni, and Cr; depleted HREE; and low SiO2 we interpret these rocks as low-silica adakites (LSA). We note however that they have lower Sr than is usually reported in LSAs.
LSAs are thought to be generated by the interaction of melt from a garnet-bearing slab with a thin mantle wedge. This has been proposed to occur during subduction of a ridge or melting of the edge of a slab window. Whereas the LSAs at Jarbo Gap could have been caused by these processes, we instead propose that they may have been generated by melting of the high-pressure subduction complex that underlies the ophiolite.