Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Cassiopeia |
Right ascension | 00h 04m 13.6625s [1] |
Declination | +62° 17′ 15.591″ [1] |
Apparent magnitude (V) | +5.884 [2] |
Characteristics | |
Spectral type | A1II-III [3] |
U−B color index | +0.29 [4] |
B−V color index | +0.30 [4] |
Astrometry | |
Radial velocity (Rv) | −23.43±0.16 [1] km/s |
Proper motion (μ) |
RA: −0.936
[1]
mas/
yr Dec.: −0.263 [1] mas/ yr |
Parallax (π) | 1.3781 ± 0.0237 mas [1] |
Distance | 2,370 ± 40
ly (730 ± 10 pc) |
Details | |
Mass | 5.1 [5] M☉ |
Radius | 26 [6] R☉ |
Luminosity | 2,208 [6] L☉ |
Surface gravity (log g) | 2.08 [5] cgs |
Temperature | 7,719 [6] K |
Metallicity [Fe/H] | −0.32 [5] dex |
Rotational velocity (v sin i) | 33 [7] km/s |
Age | 25.1 [8] Myr |
Other designations | |
Database references | |
SIMBAD | data |
9 Cassiopeiae (9 Cas) is a white giant star in the constellation Cassiopeia, about 2,370 light years away.
9 Cassiopeiae is classified as an A1 type giant or bright giant. One study noted peculiarities in the spectrum that could indicate a λ Boötis star, [9] but other researchers have refuted this. [10] [7]
At an age of 25 million years, 9 Cassiopeiae has expanded away from the main sequence after exhausting its core hydrogen and now has a radius about 26 times that of the Sun. With an effective temperature of about 7,700 K, it emits more than two thousand times the luminosity of the Sun.
9 Cassiopeiae has a number of faint companions listed in multiple star catalogues, [11] but they all appear to be at different distances [12] and none are thought to be gravitationally associated. [13]
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Cassiopeia |
Right ascension | 00h 04m 13.6625s [1] |
Declination | +62° 17′ 15.591″ [1] |
Apparent magnitude (V) | +5.884 [2] |
Characteristics | |
Spectral type | A1II-III [3] |
U−B color index | +0.29 [4] |
B−V color index | +0.30 [4] |
Astrometry | |
Radial velocity (Rv) | −23.43±0.16 [1] km/s |
Proper motion (μ) |
RA: −0.936
[1]
mas/
yr Dec.: −0.263 [1] mas/ yr |
Parallax (π) | 1.3781 ± 0.0237 mas [1] |
Distance | 2,370 ± 40
ly (730 ± 10 pc) |
Details | |
Mass | 5.1 [5] M☉ |
Radius | 26 [6] R☉ |
Luminosity | 2,208 [6] L☉ |
Surface gravity (log g) | 2.08 [5] cgs |
Temperature | 7,719 [6] K |
Metallicity [Fe/H] | −0.32 [5] dex |
Rotational velocity (v sin i) | 33 [7] km/s |
Age | 25.1 [8] Myr |
Other designations | |
Database references | |
SIMBAD | data |
9 Cassiopeiae (9 Cas) is a white giant star in the constellation Cassiopeia, about 2,370 light years away.
9 Cassiopeiae is classified as an A1 type giant or bright giant. One study noted peculiarities in the spectrum that could indicate a λ Boötis star, [9] but other researchers have refuted this. [10] [7]
At an age of 25 million years, 9 Cassiopeiae has expanded away from the main sequence after exhausting its core hydrogen and now has a radius about 26 times that of the Sun. With an effective temperature of about 7,700 K, it emits more than two thousand times the luminosity of the Sun.
9 Cassiopeiae has a number of faint companions listed in multiple star catalogues, [11] but they all appear to be at different distances [12] and none are thought to be gravitationally associated. [13]