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]

Quick Facts Constellation, Right ascension ...
b Persei
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Location of b Persei (circled)
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]
Distance310 ± 10 ly
(96 ± 3 pc)
Absolute magnitude (MV)0.3[6]
Orbit[7]
PrimaryA or Aa
CompanionC 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
Mass2.25[6] M
Radius3.2[8] R
Luminosity10[9] L
Temperature9000[6] K
Rotational velocity (v sin i)81[10] km/s
B or Ab
Mass0.56[11] M
Radius0.25[8] R
C or Ac
Mass1.24[11] M
Luminosity2[9] L
Other designations
BD+49°1150, GC 5174, HD 26961, HR 1324, HIP 20070, SAO 24531
Database references
SIMBADdata
Close
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Light curves for b Persei. The top panel, plotted from TESS data,[12] shows the variability of the inner binary pair. The lower panels, plotted from AAVSO data,[13] show two eclipses.

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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