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Black holes are famously said to have "no hair," meaning that they canbe described in General Relativity by only two parameters, effectivelymass and spin. Accurate masses can and have been measured for someblack holes, but the spin parameter has been a tougher nut to crack,because its effects are largely restricted to changes in thespace-time structure very near the event horizon. RXTE's largethroughput and fast timing ability have enabled new efforts to measureblack hole spins. Recently, two independent efforts have focused onthe micro-quasar GRS 1915+105, and have attempted to use spectralmodeling of emission from the inner accretion disk to measure itsspin. Jeff McClintock (MIT) and colleagues identify and fit dataintervals in which GRS 1915+105 shows spectral behavior characteristicof disk emission. Using fits with fully relativistic models, theyargue for a near maximal spin for GRS 1915+105. Matthew Middleton(University of Durham, UK) and collaborators use esentially the sametechnique, but have a different criteria for selecting the "diskdominated" states. Nevertheless, they also infer a rather high spinrate of 0.7. While each group argues that they've got it right,perhaps more interesting is that they both require a substantial spinrate for the black hole in GRS 1915+105. 2b1af7f3a8