Sigma2 Cancri

White-hued subgiant star in the constellation Cancer From Wikipedia, the free encyclopedia

Sigma2 Cancri is a solitary,[8] white-hued star in the constellation Cancer. Its name is a Bayer designation that is Latinized from σ2 Cancri, and abbreviated Sigma2 Cnc σ2 Cnc. This star is faintly visible to the naked eye, having an apparent visual magnitude of +5.44.[3] Based upon an annual parallax shift of 17.04 mas as seen from Earth,[2] this star is located 191 light-years (59 pc) from the Sun. It is drifting closer to the Sun with a radial velocity of −26 km/s.[5]

Quick facts Constellation, Right ascension ...
Sigma2 Cancri
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Cancer[1]
Right ascension 08h 56m 56.598s[2]
Declination +32° 54 37.54[2]
Apparent magnitude (V) +5.436[3]
Characteristics
Evolutionary stage main sequence[4][2]
Spectral type A7 IV[4]
B−V color index +0.157[3]
Astrometry
Radial velocity (Rv)−26.2±0.7[5] km/s
Proper motion (μ) RA: −53.031 mas/yr[2]
Dec.: −66.186 mas/yr[2]
Parallax (π)17.0377±0.0716 mas[2]
Distance191.4 ± 0.8 ly
(58.7 ± 0.2 pc)
Absolute magnitude (MV)+1.57[1]
Details
Mass1.79[6] M
Radius2.28+0.02
0.04
[2] R
Luminosity21.5[4] L
Surface gravity (log g)4.17[6] cgs
Temperature8,309±283[6] K
Rotational velocity (v sin i)133[4] km/s
Age441[6] Myr
Other designations
σ2 Cnc, 59 Cancri, BD+33°1785, HD 76398, HIP 43932, HR 3555, SAO 61146[7]
Database references
SIMBADdata
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With an estimated age of 441[6] million years, this is an A-type subgiant star with a stellar classification of A7 IV.[4] It is spinning rapidly with a projected rotational velocity of 133 km/s.[4] The star has an estimated 1.8[6] times the mass of the Sun with 2.3 times the Sun's radius.[2] It is radiating 21.5[4] times the Sun's luminosity from its photosphere at an effective temperature of roughly 8,309 K.[6]

References

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