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Star in Cassiopeia From Wikipedia, the free encyclopedia
V669 Cassiopeiae or V669 Cas is an OH/IR star, a type of particularly cool red giant, with a spectral type of M9III.
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Cassiopeia |
Right ascension | 01h 33m 51.21s[1] |
Declination | 62° 26′ 53.2″[1] |
Apparent magnitude (V) | 17.48[2] |
Characteristics | |
Evolutionary stage | AGB[3] |
Spectral type | M9III[3] |
Apparent magnitude (J) | 16.747[1] |
Apparent magnitude (H) | 11.232[1] |
Apparent magnitude (K) | 7.097[1] |
Variable type | Mira?[4] |
Astrometry | |
Proper motion (μ) | RA: −2.813[5] mas/yr Dec.: −2.147[5] mas/yr |
Parallax (π) | 1.9523 ± 0.7049 mas[5] |
Distance | 2,100[6] pc |
Details | |
Radius | 370 – 702[6] R☉ |
Luminosity | 10,000 - 36,000[6] L☉ |
Temperature | 3,000[6] K |
Database references | |
SIMBAD | data |
With a mean visual apparent magnitude 17.5, V669 Cassiopeiae varies with an amplitude of about half a magnitude.[2] In the mid-infrared L band, its magnitude range is 1.57 to 3.02. It is listed as a possible Mira variable, but with the extremely long period of 1,994 days.[4]
Jan Herman and Harm Jan Habing reported in 1985 that the star's OH maser emission varied in intensity with a 1994 day period.[7] In 1990, Paolo Persi et al. showed that V669 Cassiopeiae varied in infrared brightness,[8] and for that reason it was given its variable star designation in 1993.[9]
The distance and physical properties of V669 Cassiopeiae are highly uncertain. Based on parallax, it is about 1,600 light years away, but a distance of about 20,000 light years has been derived based on observations of masers around the star.[3] Based on a luminosity derived from its pulsations and spectral energy distribution, it would be at a distance of 6,850 light years.[6]
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