Eta Andromeda A/B. |
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Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) |
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Constellation | Andromeda | |
Right ascension | 00h 57m 12.4000s[1] | |
Declination | +23° 25′ 03.533″[1] | |
Apparent magnitude (V) | 4.403[1] | |
Characteristics | ||
Spectral type | G8III-IV[2] | G8III-IV[2] |
U-B color index | +0.69[3] | |
B-V color index | +0.94[3] | |
R-I color index | +0.48[3] | |
Astrometry | ||
Radial velocity (Rv) | −10.3 ± 0.9[1] km/s | |
Proper motion: | ||
RA (μα cos δ) | −43.72[1] mas/yr | |
Dec. (μδ) | −46.06[1] mas/yr | |
Parallax (π) | 13.44 ± 0.75[1] mas | |
Distance | 240 ± 10 ly (74 ± 4 pc) |
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Absolute magnitude (MV) | 0.52 ± 0.06[2] | 1.07 ± 0.07[2] |
Details | ||
Mass | 2.6 ± 0.35[4] M☉ | 2.3 ± 0.31[4] M☉ |
Surface gravity (log g) | 2.8[2] | 3.0[2] |
Luminosity (bolometric) | 65 ± 3[2] L☉ | 39 ± 3[2] L☉ |
Temperature | 4900[2] K | 4900[2] K |
Age | 8×108 [2] years | |
Orbit[5] | ||
Period (P) | 115.72 ± 0.01 d | |
Semimajor axis (a) | 10.37 ± 0.03 mas | |
Eccentricity (e) | 0.006 ± 0.002 | |
Inclination (i) | 30.5 ± 0.4° | |
Longitude of node (Ω) | 69.4 ± 0.5° | |
Periastron epoch (T) | 48013 ± 1 MJD | |
Argument of periastron (ω) (secondary) |
215 ± 4° | |
Database references | ||
SIMBAD | data | |
Other designations | ||
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.[1][2]
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Eta Andromedae was discovered to be a double-lined spectroscopic binary in a series of spectra taken in 1899 and 1900.[8] Its orbit was computed in 1946 from spectroscopic observations.[9] Because spectroscopy only reveals the radial velocity of a star towards or away from the viewer, such a computation does not determine all orbital elements. In observations made from 1990 to 1992, Eta Andromedae was resolved interferometrically by the Mark III Stellar Interferometer at Mount Wilson Observatory, California, United States. This allowed a more complete orbit to be computed and, in 1993, published.[2]
This star's location in the constellation Andromeda can be seen in the following diagram:
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) |
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Constellation | Andromeda |
Right ascension | 00h 57m 04.9s[10] |
Declination | +23° 23′ 43″[10] |
Apparent magnitude (V) | 11.5[10] |
Position (relative to η And) | |
Epoch of observation | 1997 |
Angular distance | 129.2″ [7] |
Position angle | 232° [7] |
Database references | |
SIMBAD | data |
Other designations | |
The star has a visual companion star of apparent visual magnitude 11.5, BD+22°153B, visible 129.2 arcseconds away.[7]
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