A comparison of normalized velocity distributions for Venus, as estimated by various studies, is presented: the DMZC model (black line), the SWARMS model (blue line) (A. A. Christou & M. Gritsevich 2024), the Galileo Dust Detector probe (red line) (J. P. Pabari et al. 2023), and a model for the asteroidal and cometary dust flux in the inner solar system (green line) (P. Borin et al. 2017).