S Normae
From Infogalactic: the planetary knowledge core
Observation data Epoch J2000 Equinox J2000 |
|
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Constellation | Norma |
Right ascension | 16h 18m 51.8325s |
Declination | -57° 53' 59.244"' |
Apparent magnitude (V) | 6.446 |
Characteristics | |
Spectral type | F8-G0Ib |
U−B color index | ? |
B−V color index | ? |
Variable type | Classical Cepheid |
Astrometry | |
Radial velocity (Rv) | 4.9 km/s |
Proper motion (μ) | RA: -1.10 mas/yr Dec.: -1.20 mas/yr |
Parallax (π) | 1.19 ± 0.75 mas |
Distance | approx. 3,000 ly (approx. 800 pc) |
Absolute magnitude (MV) | -4.02[1] |
Details | |
Mass | 6.3[1] M☉ |
Luminosity | 2800 L☉ |
Temperature | 6350 K |
Metallicity | ? |
Rotation | ? |
Age | ? years |
Other designations | |
S Normae (S Nor) is a variable star in the constellation Norma. It is the brightest member of the open cluster NGC 6087. It is a well-known Classical Cepheid variable with a range of 6.12 to 6.77 and a period of 9.75411 days.[2] It is a yellow-white supergiant that is 6.3 times as massive as the Sun of spectral type F8-G0Ib. A binary, it has a 2.4 solar mass (M☉) companion that is a blue-white main sequence star of spectral type B9.5V.[1]
References
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