Measuring the seismic properties of Tibetan bright spats: Evidence for free aqueous fluids in the Tibetan middle crust

Seismic bright spots are commonly interpreted to mark fluid concentrations, but their nature (melt or aqueous) is usually inferred only from circumsta ntial evidence of the geologic setting. A band of bright spot reflections h as been imaged by Project INDEPTH (International Deep Profiling of Tibet an d the Himalayas) at about 15 km depth along 150 km of the northern Yadong-G ulu rift, southern Tibet. We use INDEPTH three-component wide-angle seismic data to measure seismic velocities at the bright spot reflector, and theor etical rock physics bounds to constrain the nature of the fluids. Merging o f data from multiple bright spots allows us to use a one-dimensional approx imation. Travel time modeling yields average P and S velocities for the upp er crust above the bright spots of 5.3 +/- 0.2 and 3.2 +/- 0.2 km s(-1), re spectively. Reflection-amplitude variation with offset (AVO) modeling const rains the P and S velocities of the bright spots to 3.0 +/- 0.8 and 1.6 +/- 0.8 km s(-1), respectively. Multiple modeling procedures suggest these vel ocities are not model dependent. Our results imply that of the order of 10% volume of free aqueous fluids in the Tibetan middle crust produces the obs erved bright spot reflections. The presence of relatively large quantities of free aqueous fluids, presumably mostly saline supercritical H2O, does no t preclude the presence of melt but does constrain the maximum temperature at the bright spots to the wet granite solidus (about 650 degrees C) and th us the maximum surface heat flow to less than or equal to 110 mW m(-2). The observed bright spots can alternatively be explained as a result of transi ent flow of aqueous fluids through a lower temperature and lower heat flow southern Tibetan crust.