Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
---|---|
Constellation | Aquarius |
Right ascension | 23h 24m 03.97947s [1] |
Declination | −21° 46′ 27.8819″ [1] |
Apparent magnitude (V) | 6.50 [2] |
Characteristics | |
Spectral type | F3IV/V [3] |
U−B color index | −0.03 [2] |
B−V color index | +0.42 [2] |
Astrometry | |
Radial velocity (Rv) | 24.5 [4] km/s |
Proper motion (μ) |
RA: −67.70
[1]
mas/
yr Dec.: −77.45 [1] mas/ yr |
Parallax (π) | 15.99 ± 0.72 mas [1] |
Distance | 204 ± 9
ly (63 ± 3 pc) |
Absolute magnitude (MV) | 2.50 [5] |
Details | |
Mass | 1.47 (1.41 to 1.52) [6] M☉ |
Temperature | 6,456 [5] K |
Metallicity [Fe/H] | −0.18 [5] dex |
Age | 2.0 [5] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 220466 is a F-type subgiant or main sequence star in the constellation Aquarius. It has apparent magnitude 6.47 and is about 200 light-years away. [1] In 1913, an apparent visual companion of apparent magnitude 10.3 was observed 1.9 arcseconds away from the star, [7] but it is doubtful whether it exists. [8]
Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
---|---|
Constellation | Aquarius |
Right ascension | 23h 24m 03.97947s [1] |
Declination | −21° 46′ 27.8819″ [1] |
Apparent magnitude (V) | 6.50 [2] |
Characteristics | |
Spectral type | F3IV/V [3] |
U−B color index | −0.03 [2] |
B−V color index | +0.42 [2] |
Astrometry | |
Radial velocity (Rv) | 24.5 [4] km/s |
Proper motion (μ) |
RA: −67.70
[1]
mas/
yr Dec.: −77.45 [1] mas/ yr |
Parallax (π) | 15.99 ± 0.72 mas [1] |
Distance | 204 ± 9
ly (63 ± 3 pc) |
Absolute magnitude (MV) | 2.50 [5] |
Details | |
Mass | 1.47 (1.41 to 1.52) [6] M☉ |
Temperature | 6,456 [5] K |
Metallicity [Fe/H] | −0.18 [5] dex |
Age | 2.0 [5] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 220466 is a F-type subgiant or main sequence star in the constellation Aquarius. It has apparent magnitude 6.47 and is about 200 light-years away. [1] In 1913, an apparent visual companion of apparent magnitude 10.3 was observed 1.9 arcseconds away from the star, [7] but it is doubtful whether it exists. [8]