Venus' young surface age implies significant geologic activity. Several lines of evidence suggest current volcanism, but there is no data to directly constrain current tectonism. Wrinkle ridges are an abundant, globally distributed fault type, and may have formed relatively recently. We estimate seismicity using a scaling relationship between fault length and moment release. We obtain fault lengths from previously mapped wrinkle ridges and limit their lengths in two ways: (1) with realistic vertical slip extents (VSEs) of 50, 30, and 10 km, and (2) with four tiers of segmentation. A VSE limits fault dimensions and is constrained by faulting depth, and segmentation is important to produce a realistic magnitude-frequency distribution. We use 100 million years as a deformation time to calculate annual seismicity for the wrinkle ridges. Resulting moment release rates are 5.1×1017 N⋅m/yr, 3.7×1017 N⋅m/yr, and 9.1×1016 N⋅m/yr for fault VSEs of 50 km, 30 km, and 10 km, respectively. We predict seismicity roughly 1 order of magnitude more than the extrapolated Mars global seismicity from measurements at a single station, and ∼5 orders of magnitude less seismicity than is observed on Earth. This estimate is conservative since we assume each segment breaks once and the faults are mapped using low resolution global data. Moreover, Venus exhibits many other likely sources of seismicity, including volcanoes, ridge belts, graben, and other faults. Wrinkle ridges and other features likely produce quake magnitudes detectable through infrasound using a balloon-based barometer.