Omega2 Cancri

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

ω2 Cancri is a star in the zodiac constellation Cancer. It has the Flamsteed designation 4 Cancri; ω2 Cancri is the Bayer designation, which is Latinised to omega2 Cancri and abbreviated to ω2 Cnc or omega2 Cnc. The star is near the lower limit of visibility to the naked eye, having an apparent visual magnitude of 6.32.[1] Based on parallax measurements, it is located around 432 light-years (133 pc) away from the Sun. It is moving closer to the Earth with a heliocentric radial velocity of −8 km/s.[5] The position of this star near the ecliptic means it is subject to lunar occultations.[7]

Quick facts Observation data Epoch J2000.0 Equinox J2000.0, Constellation ...
ω2 Cancri
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cancer[1]
Right ascension 08h 01m 43.757s[2]
Declination +25° 05 22.08[2]
Apparent magnitude (V) 6.32[1]
Characteristics
Evolutionary stage main sequence[3]
Spectral type A1 V[4]
B−V color index 0.023±0.006[1]
Astrometry
Radial velocity (Rv)−7.6±2.5[5] km/s
Proper motion (μ) RA: −25.138 mas/yr[2]
Dec.: +12.276 mas/yr[2]
Parallax (π)7.5434±0.0393 mas[2]
Distance432 ± 2 ly
(132.6 ± 0.7 pc)
Absolute magnitude (MV)0.51[1]
Details
Mass2.59±0.06[3] M
Radius2.55±0.02[2] R
Luminosity68.0+8.3
−7.3
[3] L
Surface gravity (log g)3.886±0.006[2] cgs
Temperature9,354+174
−171
[3] K
Rotational velocity (v sin i)159[3] km/s
Age506±75[2] Myr
Other designations
ω2 Cancri, 4 Cnc, BD+25°1816, HD 65856, HIP 39263, HR 3132, SAO 79869, CCDM J08017+2506A, WDS J08017+2505A, GSC 01930-00674[6]
Database references
SIMBADdata
Close

This is an ordinary A-type main-sequence star with a stellar classification of A1 V,[4] which indicates it is generating energy through hydrogen fusion at its core. At an estimated age of approximately 500[2] million years, it is spinning rapidly with a projected rotational velocity of 159 km/s.[3] It has 2.6[3] times the mass of the Sun and about 2.55 times the Sun's radius.[2] The star is radiating 68[3] times the Sun's luminosity from its photosphere at an effective temperature of 9,354 K.[3]

References

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