Algol

Algol
Location of β Persei (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Perseus
Right ascension 03h 08m 10.13245s
Declination +40° 57 20.3280
Apparent magnitude (V) 2.12 (- 3.39)
Characteristics
Spectral type Aa1: B8V
Aa2: K0IV
Ab: F1V (kA4hA9.5mF0:)
U−B colour index −0.37
B−V colour index −0.05
Variable type EA/SD
Astrometry
Radial velocity (Rv)3.7 km/s
Proper motion (μ) RA: 2.99 mas/yr
Dec.: −1.66 mas/yr
Parallax (π)34.7±0.6 mas
Distance94 ± 2 ly
(28.8 ± 0.5 pc)
A or Aa1
Absolute magnitude (MV)−0.07
B or Aa2
Absolute magnitude (MV)2.9
C or Ab
Absolute magnitude (MV)2.3
Orbit
PrimaryA or Aa1
CompanionB or Aa2
Period (P)2.867328 days
Semi-major axis (a)0.00215″
Eccentricity (e)0
Inclination (i)98.70°
Longitude of the node (Ω)43.43°
Orbit
PrimaryAa
CompanionAb
Period (P)680.168 days
Semi-major axis (a)0.09343″
Eccentricity (e)0.227
Inclination (i)83.66°
Longitude of the node (Ω)132.66°
Periastron epoch (T)2446927.22
Argument of periastron (ω)
(primary)
310.02°
Details
A or Aa1
Mass3.17 ± 0.21 M
Radius2.73 ± 0.20 R
Luminosity182 L
Surface gravity (log g)4.0 cgs
Temperature13,000 K
Rotational velocity (v sin i)49 km/s
Age570 Myr
B or Aa2
Mass0.70±0.08 M
Radius3.48±0.28 R
Luminosity6.92 L
Surface gravity (log g)3.5 cgs
Temperature4,500 K
C or Ab
Mass1.76±0.15 M
Radius1.73±0.33 R
Luminosity10.0 L
Surface gravity (log g)4.5 cgs
Temperature7,500 K
Other designations
Algol, Gorgona, Gorgonea Prima, Demon Star, El Ghoul, β Persei, β Per, 26 Persei, BD+40°673, FK5 111, GC 3733, HD 19356, HIP 14576, HR 936, PPM 45864, SAO 38592.
Database references
SIMBADdata

Algol /ˈælɡɒl/, designated Beta Persei (β Persei, abbreviated Beta Per, β Per), known colloquially as the Demon Star, is a bright multiple star in the constellation of Perseus and one of the first non-nova variable stars to be discovered.

Algol is a three-star system, consisting of Beta Persei Aa1, Aa2, and Ab – in which the hot luminous primary β Persei Aa1 and the larger, but cooler and fainter, β Persei Aa2 regularly pass in front of each other, causing eclipses. Thus Algol's magnitude is usually near-constant at 2.1, but regularly dips to 3.4 every 2.86 days during the roughly 10-hour-long partial eclipses. The secondary eclipse when the brighter primary star occults the fainter secondary is very shallow and can only be detected photoelectrically.

Algol gives its name to its class of eclipsing variable, known as Algol variables.