b Persei (also known as HD 26961) is a spectroscopic triple star in the constellation Perseus. Its apparent magnitude is 4.60,[6] and it is about 320 light years away.[1]
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Perseus |
Right ascension | 04h 18m 14.61690s[1] |
Declination | +50° 17′ 43.8058″[1] |
Apparent magnitude (V) | 4.52 - 4.68[2] |
Characteristics | |
Spectral type | A1III[3] |
B−V color index | +0.04[4] |
Variable type | Ellipsoidal[2] |
Astrometry | |
Radial velocity (Rv) | 19.8±0.9[5] km/s |
Proper motion (μ) | RA: 45.42±0.40[1] mas/yr Dec.: −56.72±0.32[1] mas/yr |
Parallax (π) | 10.40 ± 0.35 mas[1] |
Distance | 310 ± 10 ly (96 ± 3 pc) |
Absolute magnitude (MV) | 0.3[6] |
Orbit[7] | |
Primary | A or Aa |
Companion | C or Ac |
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 | |
A or Aa | |
Mass | 2.25[6] M☉ |
Radius | 3.2[8] R☉ |
Luminosity | 10[9] L☉ |
Temperature | 9000[6] K |
Rotational velocity (v sin i) | 81[10] km/s |
B or Ab | |
Mass | 0.56[11] M☉ |
Radius | 0.25[8] R☉ |
C or Ac | |
Mass | 1.24[11] M☉ |
Luminosity | 2[9] L☉ |
Other designations | |
Database references | |
SIMBAD | data |
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 (star C or Ac) in an orbit calculated to be 702 days long.[6] The close binary pair forms a rotating ellipsoidal variable with a 1.53 day period. Star C forms an Algol-type variable system with the close binary, showing both primary eclipses (when star C passes in front of the inner pair) and secondary eclipses (when the inner pair passes in front of star C).[14] Timings of the eclipses show a 705.4-day period.[9]
References
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