3 Camelopardalis
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Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Camelopardalis |
Right ascension | 04h 39m 54.68s |
Declination | +53° 04′ 46.327″ |
Apparent magnitude (V) | 5.085 |
Characteristics | |
Spectral type | K0III |
U−B color index | 0.89 |
B−V color index | 1.07 |
Variable type | Cepheid variable NSV 1681 |
Astrometry | |
Radial velocity (Rv) | -40.5 km/s |
Proper motion (μ) | RA: -7.38 mas/yr Dec.: -15.95 mas/yr |
Parallax (π) | 6.58 ± 0.78 mas |
Distance | approx. 500 ly (approx. 150 pc) |
Absolute magnitude (MV) | 6.166[citation needed] |
Details | |
Mass | 0,8[citation needed] M☉ |
Radius | 0,9[citation needed] R☉ |
Luminosity | 0,4[citation needed] L☉ |
Temperature | 3,500–5,000 K |
Rotation | < 17 Km/s 0,0146962 Year |
Orbit | |
Companion | CCDM 04399+5305 B BU 1043 |
Period (P) | 0,33128 yr |
Semi-major axis (a) | 3.8" |
Inclination (i) | 297° |
Other designations | |
Database references | |
SIMBAD | data |
Data sources: | |
Hipparcos Catalogue, CCDM (2002), Bright Star Catalogue (5th rev. ed.) |
3 Camelopardalis is a spectroscopic binary in the constellation Camelopardalis. It is approximately 496 light years from Earth.
The primary component, 3 Camelopardalis A, is an orange K-type giant with a mean apparent magnitude of +5.07. It is a Cepheid variable star and its brightness varies from magnitude +5.05 to +5.10. The binary star revolves around its common centre of mass once every 121 days.
References
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