Corrigendum to “Faster paleospin and deep-seated uncompensated mass as possible explanations for Ceres’ present-day shape and gravity” [Icarus 299 (2018) 430-442] (S0019103517301689) (10.1016/j.icarus.2017.08.033))

The authors regret that Fig. 4 was mistakenly switched with a similar figure from the response to the reviewers, showing solutions to 1% faster spin rate. It is stated in the text that the effect of any faster spin is to lower the degree-2 gravity (J₂) implied by Ceres’ shape and thus any required contribution from deep-seated non-hydrostatic density structure to the gravity and topography. The corrected Fig. 4 thus shifts these curves upward and is the basis for Figs. 5 and 6.