HD 111154 is a member of the Coma Cluster. It is here shown to be a somewha
t unequal pair of stars of approximately solar type. They are in an orbit t
hat has a period of just under 27 days and quite a high eccentricity (0.442
). Although the minimum masses (1.08 and 1.08 M-.) are large enough to enco
urage a search for eclipses, no such events have been detected.