HD_44780
HD 44780
Binary star system in the constellation Gemini
HD 44780 is a binary star system in the northern constellation of Gemini, located about 3° north of Mu Geminorum.[1][7] The pair have a combined apparent visual magnitude of 6.35,[3] which is near the lower limit of visibility to the naked eye. Although it is above magnitude 6.5, it was not included in the Bright Star Catalogue;[1] the designation HD 44780 comes from the Henry Draper catalogue. Based upon parallax measurements, the system is located at a distance of approximately 960 light years from the Sun. It is drifting further away with a radial velocity of +17 km/s.[3]
The variable velocity of this system was first noted during a study at Mount Wilson observatory in 1952.[1] It is a double-lined spectroscopic binary[5] system with an orbital period of 1.581 years and an eccentricity of 0.24. Both components are similar, aging giant stars, a relatively rare combination.[1] Their combined spectrum matches a stellar classification of K2 III;[4] with the secondary being a slightly earlier type than the primary. They have an age of about 400 million years, with masses 3.10 and 3.02 times that of the Sun.[5]