HR 7955

HR 7955
Observation data
Epoch J2000      Equinox J2000
Constellation Cepheus
Right ascension 20h 45m 21.12879s
Declination +57° 34 47.0080
Apparent magnitude (V) 4.51
Characteristics
Spectral type F8IV-V + F9IV-V
Astrometry
Radial velocity (Rv)−32.82±0.04 km/s
Proper motion (μ) RA: −62.32 mas/yr
Dec.: −236.00 mas/yr
Parallax (π)36.64±0.48 mas
Distance89 ± 1 ly
(27.3 ± 0.4 pc)
Absolute magnitude (MV)2.35
Orbit
Period (P)494.16±0.58 d
Semi-major axis (a)0.065±0.001"
(≥50.2±0.5 Gm)
Eccentricity (e)0.551±0.004
Inclination (i)24.53±3.13°
Longitude of the node (Ω)325.21±1.05°
Periastron epoch (T)B 1996.335 ± 0.0017
Argument of periastron (ω)
(secondary)
68.86±0.76°
Details
HR 7955 A
Mass1.071±0.037 M
Age2.25 Gyr
HR 7955 B
Mass1.047±0.037 M
Other designations
BD+57°2240, FK5 782, GJ 9706, HD 198084, HIP 102431, HR 7955, SAO 32862
Database references
SIMBADdata

HR 7955 is a binary star system in the northern circumpolar constellation of Cepheus, near the constellation border with Cygnus. It has a yellow-white hue and is faintly visible to the naked eye with a combined apparent visual magnitude of 4.51. The system is located at a distance of 89 light-years (27.3 parsecs) from the Sun, based on parallax. It has a relatively high proper motion, traversing the celestial sphere at the rate of 0.243 arc seconds per annum, and is drifting closer to the Sun with a radial velocity of -33 km/s.

The double-lined nature of this spectroscopic binary system was not announced until 1972. It has an orbital period of 1.35 years and an eccentricity of 0.551. Both components appear to be slightly evolved stars that are leaving the main sequence and becoming subgiant stars, with stellar classifications of F8IV-V and F9IV-V. They each have slightly greater mass than the Sun: 107% and 105%, respectively. The system is about 2.25 billion years old.