Delta Sagittae
Binary star system in the constellation Sagitta
From Wikipedia, the free encyclopedia
Delta Sagittae, also named Zuoqi,[14] is a binary star in the constellation of Sagitta, with an apparent magnitude of +3.68. The primary component is a red M-type bright giant, and the secondary is a B-type main-sequence star.[2] It is approximately 430 light years from Earth, based on its Gaia Data Release 2 parallax.[1]

Delta Sagittae is a spectroscopic binary with a composite spectrum, meaning that light from both stars can be detected. It has an orbital period of about 10 years and an eccentricity of about 0.44.[4] It is also a variable star, with its brightness changing between a maximum of magnitude 3.75 and a minimum of 3.83 in an unpredictable way.[7]
Delta Sagittae is moving through the Galaxy at a speed of 9.8 km/s relative to the Sun. Its projected Galactic orbit carries it between 23,800 and 35,300 light years from the center of the Galaxy.[16][better source needed]
Naming
Delta Sagittae (Latinized from δ Sagittae, abbreviated Delta Sge, δ Sge) is the star's Bayer designation.
In Chinese astronomy, 左旗 (Zuǒ Qí), meaning Left Flag, refers to an asterism consisting of δ Sagittae, α Sagittae, β Sagittae, ζ Sagittae, γ Sagittae, 13 Sagittae, 11 Sagittae, 14 Sagittae and ρ Aquilae. Consequently, the Chinese name for δ Sagittae itself is 左旗三 (Zuǒ Qí sān, English: the Third Star of Left Flag.)[17] The IAU Working Group on Star Names adopted the name Zuoqi for δ Sagittae A on 18 June 2026, after the Chinese constellation.[14]
Notes
- calculated from a sin i divided by the sine of inclination.