Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Cancer |
Right ascension | 08h 57m 14.95026s[1] |
Declination | +15° 19′ 21.9512″[1] |
Apparent magnitude (V) | +5.20[2] |
Characteristics | |
Spectral type | A5 III[3] |
B−V color index | +0.1540[2] |
Astrometry | |
Radial velocity (Rv) | −4.6±2.8[4] km/s |
Proper motion (μ) | RA: +61.47[1] mas/yr Dec.: +19.40[1] mas/yr |
Parallax (π) | 21.87 ± 0.26 mas[1] |
Distance | 149 ± 2 ly (45.7 ± 0.5 pc) |
Absolute magnitude (MV) | +1.92[5] |
Details | |
Mass | 2.02[6] M☉ |
Radius | 1.86[7] R☉ |
Luminosity | 13.4[8] L☉ |
Surface gravity (log g) | 4.16[6] cgs |
Temperature | 8,636±294[6] K |
Rotational velocity (v sin i) | 90[6] km/s |
Age | 598[6] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Omicron1 Cancri, Latinised from ο1 Cancri, is a solitary,[10] white-hued star in the zodiac constellation of Cancer. It is visible to the naked eye with an apparent visual magnitude of +5.20.[2] Based upon an annual parallax shift of 21.87 mas as seen from Earth,[1] this star is located around 149 light-years from the Sun. It most likely forms a co-moving pair with Omicron2 Cancri.[11]
With a stellar classification of A5 III,[3] this appears to be an evolved, A-type giant star. At the age of about 600 million years,[6] it has double[6] the mass of the Sun and 1.86 times the Sun's radius.[7] Omicron1 Cancri is radiating 13.4[8] times the solar luminosity from its photosphere at an effective temperature of about 8,636 K.[6]
Omicron1 Cancri has an infrared excess, indicating it surrounded by a circumstellar debris disk.[7] The signature matches a two-component disk with the spatially separated belts having temperatures of 146 K and 81 K.[8]
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