HD 200964 is a star with a pair of orbiting exoplanets[5] located in the northern constellation of Equuleus.
[1] It has an apparent visual magnitude of +6.48,[1] which puts it at the lower limit of visibility to the naked eye, but binoculars would make it easy to see.
Based on parallax measurements, the distance to this system is 238 light years, but it is drifting closer with a heliocentric radial velocity of −72.6 km/s.
[5] The star has 44% more mass than the Sun and is spinning with a projected rotational velocity of 2.3 km/s.
The outer planet is 9/10 the mass of Jupiter and takes 825 days to orbit eccentrically around the star at the average distance of 1.95 AU (292 Gm).