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B Persei

b Persei
Perseus constellation map.svg
Red circle.svg

Location of b Persei (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Perseus
Right ascension 04h 18m 14.61690s
Declination +50° 17′ 43.8058″
Apparent magnitude (V) 4.52 - 4.68
Characteristics
Spectral type A1III
B−V color index +0.04
Variable type Ellipsoidal
Astrometry
Radial velocity (Rv) 19.8 ± 0.9 km/s
Proper motion (μ) RA: 45.42 ± 0.40 mas/yr
Dec.: -56.72 ± 0.32 mas/yr
Parallax (π) 10.40 ± 0.35mas
Distance 310 ± 10 ly
(96 ± 3 pc)
Absolute magnitude (MV) 0.3
Orbit
Primary b Persei A
Companion b Persei C
Period (P) 701.76 days
Semi-major axis (a) 5.09 mas
Eccentricity (e) 0.235
Inclination (i) 83.46°
Longitude of the node (Ω) 115.29°
Periastron epoch (T) 2440143.3984
Argument of periastron (ω)
(secondary)
263°
Details
Mass 2.25 M
Radius 3.2 R
Temperature 9000 K
Rotational velocity (v sin i) 81 km/s
Other designations
BD+49°1150, GC 5174, HD 26961, HR 1324, HIP 20070, SAO 24531
Database references
SIMBAD data

b Persei (also known as HD 26961) is a spectroscopic triple star in the constellation Perseus. Its apparent magnitude is 4.60, and it is about 320 light years away.

In addition to the primary, an A-type giant, there is a smaller and cooler companion in a 1.53 day orbit, probably an F-class star around absolute magnitude 3.0, and a more distant companion in a 702-day orbit.



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