Eta Andromedae
Eta Andromedae (Eta And, η Andromedae, η And) is a spectroscopic binary star in the constellation of Andromeda. It consists of two G-type subgiant or giant stars orbiting each other with a period of 115.7 days and has an overall apparent visual magnitude of approximately 4.403.
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Andromeda |
Right ascension | 00h 57m 12.4000s |
Declination | +23° 25′ 03.533″ |
Apparent magnitude (V) | 4.403 |
Characteristics | |
Spectral type | G8III-IV + G8III-IV |
U−B color index | +0.69 |
B−V color index | +0.94 |
R−I color index | +0.48 |
Astrometry | |
η And A | |
Radial velocity (Rv) | −10.3 ± 0.9 km/s |
Proper motion (μ) | RA: −43.72 mas/yr Dec.: −46.06 mas/yr |
Parallax (π) | 13.44 ± 0.75 mas |
Distance | 240 ± 10 ly (74 ± 4 pc) |
Absolute magnitude (MV) | 0.52 ± 0.06 |
η And B | |
Absolute magnitude (MV) | 1.07 ± 0.07 |
Orbit | |
Period (P) | 115.72 ± 0.01 d |
Semi-major axis (a) | 10.37 ± 0.03 mas |
Eccentricity (e) | 0.006 ± 0.002 |
Inclination (i) | 30.5 ± 0.4° |
Longitude of the node (Ω) | 69.4 ± 0.5° |
Periastron epoch (T) | 48013 ± 1 MJD |
Argument of periastron (ω) (secondary) | 215 ± 4° |
Details | |
η And A | |
Mass | 2.6 ± 0.35 M☉ |
Luminosity (bolometric) | 65 ± 3 L☉ |
Surface gravity (log g) | 2.8 cgs |
Temperature | 4900 K |
Age | 800 Million years |
η And B | |
Mass | 2.3 ± 0.31 M☉ |
Luminosity (bolometric) | 39 ± 3 L☉ |
Surface gravity (log g) | 3.0 cgs |
Temperature | 4900 K |
Other designations | |
Database references | |
SIMBAD | data |
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