Delta Andromedae is a triple star system in the northern constellation of Andromeda. Its identifier is a Bayer designation that is Latinized from ô Andromedae, and abbreviated Delta And or ô And, respectively. The system is visible to the naked eye as a point of light with a combined apparent visual magnitude of 3.28. Based upon parallax measurements, it is located at a distance of approximately from the Sun. The system is drifting closer with a radial velocity of âÂÂ10 km/s.
In Chinese, (), meaning Legs (asterism), refers to an asterism consisting of ô Andromedae, ÷ Andromedae, 65 Piscium, ö Andromedae, ù Piscium, õ Andromedae, àAndromedae, ý Andromedae, ü Andromedae, ò Andromedae, àPiscium, àPiscium, 91 Piscium, àPiscium, àPiscium, àPiscium and ÃÂ<sup>1</sup> Piscium. Consequently, the Chinese name for ô Andromedae itself is (, .) Apart from its Bayer designation, it was also given the title Delta by Elijah H. Burritt in his star atlas.
This is a long-period spectroscopic binary with an orbital period of approximately 15,000 days (41 years). The primary of the spectroscopic binary, component Aa, has a stellar classification of K3 III, indicating that it is an aging giant star. It most likely evolved from a F-type main sequence star after consuming the hydrogen at its core. The secondary, component Ab, is a relatively faint K-type dwarf, which has been imaged using a stellar coronagraph. The pair have a physical separation of .
The system has two companions, the closest of which is an orbiting red dwarf of class M3 with a separation of at least 940 astronomical units.
An excess of infrared emission from ô Andromedae suggested that it may be surrounded by a shell of dust. In 2003 it was determined that this is more likely a circumstellar debris disk.