We exhibit a stable finite time blowup regime for the 1-corotational energy critical harmonic heat flow from R 2 into a smooth compact revolution surface of R 3 that reduces to the semilinear parabolic problem @ t u @ 2 r u @ r u r C f .u/ r 2 D 0 for a suitable class of functions f . The corresponding initial data can be chosen smooth, well localized, and arbitrarily close to the ground state harmonic map in the energy-critical topology. We give sharp asymptotics on the corresponding singularity formation that occurs through the concentration of a universal bubble of energy at the speed predicted by van den Berg, Hulshof, and King. Our approach lies in the continuation of the study of the 1-equivariant energy critical wave map and Schrödinger map with S 2 target by Merle, Raphaël, and Rodnianski.