HD 180902 is a star with two or more orbiting companions in the southern constellation of Sagittarius. This system is located at a distance of approximately 342 light years from the Sun based on parallax measurements, but is drifting closer with a radial velocity of −2.8 km/s. It has an absolute magnitude of 2.5, but at that distance the apparent visual magnitude of the system is 7.8, which is too faint to be seen with the naked eye.
The spectrum of the primary, component A, presents as an evolving subgiant star with a stellar classification of K0 III/IV. It is an estimated 2.8 billion years old with 1.7 times the mass of the Sun. The star has expanded to 4.2 times the radius of the Sun and is radiating 9.4 times the Sun's luminosity from an enlarged photosphere at an effective temperature of 5,030 K.
HD 180902 b was discovered using the Doppler spectroscopy method with observations taken at the W. M. Keck Observatory. The radial velocities showed a long term linear trend in the data indicating an additional companion of unknown nature with a longer orbital period. This was subsequently shown to be due to an orbiting brown dwarf or low mass stellar companion, designated component B.
There is a second unconfirmed planet, HD 180902 c, with a mass at least twice that of Neptune and an orbital period of 15 days.