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We present the visual orbit of the double-lined eclipsing binary, HD 185912,from long baseline interferometry with the CHARA Array. We also obtain echellespectra from the Apache Point observatory to update the spectroscopic orbitalsolution and analyze new photometry from Burggraaff et al. to model theeclipses. By combining the spectroscopic and visual orbital solutions, we findcomponent masses of M1 = 1.361 +/- 0.004 Msun and M2 = 1.331 +/- 0.004 Msun,and a distance of d = 40.75 +/- 0.30 pc from orbital parallax. From the lightcurve solution, we find component radii of R1 = 1.348 +/- 0.016 Rsun and R2 =1.322 +/- 0.016 Rsun. By comparing these observed parameters to stellarevolution models, we find that HD 185912 is a young system near the zero agemain sequence with an estimated age of 500 Myr.

Visual Orbits of Spectroscopic Binaries with the CHARA Array. II. The eclipsing binary HD 185912