Fluids associated with the San Andreas and companion faults in central
and southcentral California have high He-3/He-4 ratios. The lack of c
orrelation between helium isotopes and fluid chemistry or local geolog
y requires that fluids enter the fault system from the mantle. Mantle
fluids passing through the ductile lower crust must enter the brittle
fault zone at or near lithostatic pressures; estimates of fluid flux b
ased on helium isotopes suggest that they may thus contribute directly
to fault-weakening high-fluid pressures at seismogenic depths.