CMD of M67 showing the positions of the components of S1082. Gray points are confirmed cluster members from Geller et al. (2015b). A 4.0 Gyr MIST isochrone (dashed black line; 850 pc, A_V = 0.093, solar metallicity) and single–star evolutionary tracks from 0.9–1.7 M_⊙ are overplotted. Circles mark the component positions from Sandquist et al. (2003), while triangles show the updated values derived in this study (blue: Aa, 1.30 ± 0.13 M_⊙, orange: Ab, 1.00 ± 0.07 M_⊙). Red arrows mark the shifts from the earlier estimates to the new ones.