Red clump stars and red giant branch (RGB) stars have different ﹩\mathrm{log}\;g﹩ values but similar F₈: red clump stars (cyan and magenta points) cleanly separate from red giant stars (red points) in the F₈–asteroseismic ﹩\mathrm{log}\;g﹩ diagram, with clump stars having somewhat lower ﹩\mathrm{log}\;g﹩. Both populations, however, tend to have similar F₈ values, suggesting similar contributions to the F₈ signal from convective motions despite different evolutionary states. Clump and secondary clump stars also tend to separate, with the lower-mass clump stars tending to have lower ﹩\mathrm{log}\;g﹩ but larger F₈. Black points represent stars whose evolutionary state is unknown (see Stello et al. 2013); many of these lie on the red clump sequence of the F₈–﹩\mathrm{log}\;g﹩ diagram, suggesting that F₈ might be used as a constraint in addition to the asteroseismic analysis to help elucidate their nature.