3 Ceti

Star in the constellation Cetus From Wikipedia, the free encyclopedia

3 Ceti is a single,[11] orange-hued star located around 2,100 light years away[12] in the equatorial constellation of Cetus. It is visible to the naked eye with an apparent visual magnitude of 4.95.[2] The star is moving closer to the Earth with a heliocentric radial velocity of −42 km/s.[5] It has a peculiar velocity of 60.7+3.8
−6.2
 km/s
and is a candidate runaway star.[6]

Right ascension00h 04m 30.11827s[1]
Declination−10° 30 34.2849[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
3 Ceti
Observation data
Epoch J2000      Equinox J2000
Constellation Cetus
Right ascension 00h 04m 30.11827s[1]
Declination −10° 30 34.2849[1]
Apparent magnitude (V) 4.953[2]
Characteristics
Spectral type K3 III[3] or K3 Ib[4]
B−V color index +1.66[2]
Astrometry
Radial velocity (Rv)−42.10±0.33[5] km/s
Proper motion (μ) RA: −6.85[1] mas/yr
Dec.: −12.02[1] mas/yr
Parallax (π)1.56±0.31 mas[1]
Distanceapprox. 2,100 ly
(approx. 600 pc)
Details
Mass9.0±0.6[6] M
Radius182[7] R
Luminosity (bolometric)7,877[7] L
Surface gravity (log g)0.90[8] cgs
Temperature4,152[8] K
Metallicity [Fe/H]0.08[8] dex
Rotational velocity (v sin i)5.8±1.0[9] km/s
Age29.7±3.6[6] Myr
Other designations
3 Cet, NSV 13, BD−11°6194, FK5 2001, HD 225212, HIP 355, HR 9103, SAO 147066, 2MASS J00043012-1030344[10]
Database references
SIMBADdata
Close

This is a red supergiant star with a stellar classification of K3 Ib,[4] although Houk and Swift (1999) classed it as a normal giant at K3 III.[3] It displays microvariability, undergoing changes in brightness with a frequency of 11.2 times per day and an amplitude of 0.0053 in magnitude.[4] The star is about 30 million years old with nine times the mass of the Sun[6] and 182 times the radius of the Sun. It is radiating 7,877[7] times the Sun's luminosity from its photosphere at an effective temperature of 4,152 K.[8]

It is a possible supernova candidate.[12]

References

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