14 Sagittae is a binary star[7] system in the equatorial constellation of Aquila.
[2] The system is located 660 light years away, as determined from its annual parallax shift of 4.91 mas.
[4] This is a single-lined spectroscopic binary with an orbital period of 61.5 days and an eccentricity of 0.49.
[7] The visible component is a chemically peculiar mercury-manganese star[11] with a stellar classification of B9p HgMn.
[8] The star is radiating 292[6] times the Sun's luminosity from its photosphere at an effective temperature of 13,200 K.[3]