Kinematic measurements hold some promise of dramatically enhancing the
prospects of traditional weak lensing. In this talk I outline the
method and describe how it eliminates or suppresses the effects of
traditional weak lensing systematic errors arising from shear
calibration, photometric redshifts, and intrinsic alignments. I also
discuss what it would take to scale kinematic lensing up to a level
competitive with other advanced dark energy probes.