U-PB GEOCHRONOLOGY AND HF ISOTOPE GEOCHEMISTRY OF THE SOUTHERN COAST MOUNTAINS BATHOLITH, BRITISH COLUMBIA
Whereas U-Pb ages in northern and central areas of the CMB ages show a younging eastward trend, the southern CMB displays a more complicated pattern. Late Jurassic plutons commonly occur inboard (east) of Early Cretaceous plutons. We document a number of plutons with ages ranging from 140 – 120 Ma, an age population that is uncommon elsewhere along the Cordilleran margin.
Hafnium isotope signatures in plutons of all ages are juvenile, with ɛHf values ranging from +15 to +5. The highest ɛHf, which approach those in MORB, are found in plutons crystallizing at 150-120 and 80-60 Ma. The overall positive values suggest that plutons of the southern CMB were generated mainly from melting of Paleozoic arc-type terranes (e.g., Wrangellia, Alexander, and/or Stikine), with little or no melt contribution from older continental crust. ɛHf excursions may have resulted from basinal extension at ~150-120 Ma and a phase of extension between ~85 and ~60 Ma. However, at this time, we do not have structural evidence to verify an extensional regime in the southern CMB between 85 – 60 Ma.