Empirical density profiles from Neuenschwander & Helled (2022) we considered in this study. Also shown are published density profiles of Uranus. The blue curves show Uranus models that use the rotation period estimated by the Voyager 2 mission, while the green curves show models that use the rotation period proposed by Helled et al. (2010). The red curves show models with 1100 km deep winds, and the yellow curves correspond to solutions with high central densities.