6 Cassiopeiae
|
Star 6 Cassiopeiae |
|||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| AladinLite | |||||||||||||||||
|
Observation dates equinox : J2000.0 , epoch : J2000.0 |
|||||||||||||||||
| Constellation | Cassiopeia | ||||||||||||||||
| Right ascension | 23 h 48 m 50.17 s | ||||||||||||||||
| declination | + 62 ° 12 ′ 52.3 ″ | ||||||||||||||||
| Apparent brightness | 5.55 mag | ||||||||||||||||
| Typing | |||||||||||||||||
| B − V color index | +0.67 | ||||||||||||||||
| U − B color index | −0.02 | ||||||||||||||||
| Spectral class | A3 Ia + e | ||||||||||||||||
| Astrometry | |||||||||||||||||
| Radial velocity | −55.7 km / s | ||||||||||||||||
| distance | approx. 8200 ly approx. 2500 pc |
||||||||||||||||
| Visual absolute brightness M vis | −8.3 mag | ||||||||||||||||
| Proper movement | |||||||||||||||||
| Rec. Share: | (−3.57 ± 0.35) mas / a | ||||||||||||||||
| Dec. portion: | (−1.57 ± 0.33) mas / a | ||||||||||||||||
| Physical Properties | |||||||||||||||||
| Dimensions | ~ 25 M ☉ | ||||||||||||||||
| radius | ~ 190 R ☉ | ||||||||||||||||
| Luminosity |
~ 195,000 L ☉ |
||||||||||||||||
| Effective temperature | approx. 8800 K | ||||||||||||||||
| Rotation time | 82 d | ||||||||||||||||
|
Other names and catalog entries |
|||||||||||||||||
|
|||||||||||||||||
6 Cassiopeiae is a quadruple star system approximately 8,200 light years away and located in the constellation Cassiopeia .
6 Cas A is a white supergiant of the spectral class A. After Rho Cassiopeiae , 6 Cas A is the most luminous star of the stellar association Cas OB5 , which can be found in the constellation Cassiopeia in the northern hemisphere.
6 Cas A is probably at least 25 times as heavy as the sun. Its apparent brightness is +5.43 mag, so it is faintly perceptible to the naked eye under good conditions. With an absolute visual magnitude of –8.3 mag, it is one of the brightest stars at all. Compared to the sun , it is 195,000 times brighter.
At the moment 6 Cassiopeiae is developing into a red supergiant like Deneb .
Little is known about the three small components.
Web links
Individual evidence
- ↑ a b Hipparcos catalog
- ↑ a b c SIMBAD database
- ↑ a b Bright Star Catalog