Omicron1 Cancri

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Omicron1 Cancri
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Cancer[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) +5.20[3]
Characteristics
Spectral type A5 III[4]
B−V Template:Engvar +0.1540[3]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[5] km/s
Proper motion (μ) RA: +60.732 mas/yr[2]
Dec.: +20.396 mas/yr[2]
Parallax (π)20.3294±0.0891 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)+1.92[1]
Details
Mass2.02[6] Template:Solar mass
Radius1.86[7] Template:Solar radius
Luminosity13.4[8] Template:Solar luminosity
Surface gravity (log g)3.982Script error: No such module "Su".[9] cgs
Temperature8,145±3[9] K
Metallicity [Fe/H]−0.85Script error: No such module "Su".[9] dex
Rotational velocity (v sin i)90[6] km/s
Age598[6] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[10]
Database references
SIMBADdata

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Omicron1 Cancri is a solitary,[11] white-hued star in the zodiac constellation of Cancer. Its name is a Bayer designation that is Latinized from ο1 Cancri, and abbreviated Omicron1 Cancri or ο1 Cnc. This star is faintly visible to the naked eye with an apparent visual magnitude of +5.20.[3] Based upon an annual parallax shift of Script error: No such module "val". as seen from Earth,[2] it is located Script error: No such module "convert". away from the Sun. It most likely forms a co-moving pair with Omicron2 Cancri.[12]

With a stellar classification of A5 III,[4] this presents as 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 Script error: No such module "val"..[9] It has a high rate of spin, showing a projected rotational velocity of 90 km/s.[13]

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]

References

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Template:Stars of Cancer