Chandler and precession periods of Venus computed for the density profiles of Shah et al. (2022), featuring either a fully liquid core (green), a solid inner core with a liquid outer core (blue), or a fully solid core (orange). For each core state, the 99% contour of a kernel density estimate is shown. Black bars correspond to the density profiles from Dumoulin et al. (2017), all featuring fully liquid cores. Black level lines indicate the core size of the models in kilometers, to within 50 km.