Obliquity distribution for stars hosting planets on eccentric and circular orbits. Left: the cumulative sum of |λ| for eccentric planets shown in red, sorted by T_eff. The black line is the average of 5000 randomly sampled sets from the circular population with the gray shaded area denoting the 1σ and 2σ intervals. The vertical blue line denotes the Kraft break (T_eff = 6100 K). Right: histogram showing the distribution of the circular population and the value of the eccentric population at the Kraft break. The Gaussian is a fit to the histogram. The circular and eccentric samples only differ by 2.1 σ, meaning the eccentric population does not appear to be significantly more misaligned. Adapted from Rice et al. (2022).