This orange-hued double has a combined stellar classification of K3III, matching an aging giant star that has exhausted the supply of hydrogen at its core. In 1984, C. J. Corbally found a class of K4IIIab for the primary and K2IIIb for the fainter secondary.
This orange-hued double has a combined stellar classification of K3III, corresponding to an aging giant star that has exhausted its core hydrogen. In 1984, C. J. Corbally found a class of K4IIIab for the primary and K2IIIb for the secondary.