HR 3407

Star in the constellation Vela From Wikipedia, the free encyclopedia

HR 3407 is a single[10] star in the southern constellation of Vela. It has the Bayer designation C Velorum; HR 3407 is the designation in the Bright Star Catalogue.[9] It is an orange-hued star that is dimly visible to the naked eye with an apparent visual magnitude of 5.01.[2] The distance to this object is approximately 1,040 light years based on parallax measurements, and it is drifting further away with a radial velocity of 4 km/s.[1]

Right ascension08h 34m 43.59703s[1]
Declination−49° 56 39.1359[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
HR 3407
Observation data
Epoch J2000      Equinox J2000
Constellation Vela
Right ascension 08h 34m 43.59703s[1]
Declination −49° 56 39.1359[1]
Apparent magnitude (V) 5.01[2]
Characteristics
Evolutionary stage Giant star[3]
Spectral type K1.5Ib[4]
U−B color index +1.38[2]
B−V color index +1.33[2]
Variable type microvariable[5]
Astrometry
Radial velocity (Rv)4.25±0.17[1] km/s
Proper motion (μ) RA: −14.236±0.322[1] mas/yr
Dec.: +18.540±0.353[1] mas/yr
Parallax (π)3.1501±0.1571 mas[1]
Distance1,040 ± 50 ly
(320 ± 20 pc)
Absolute magnitude (MV)–2.06[6]
Details
Mass3.3±1.1[3] M
Radius56[7] R
Luminosity1,010±131[3] L
Surface gravity (log g)2.0[8] cgs
Temperature4,245[3] K
Metallicity [Fe/H]−0.4[8] dex
Rotational velocity (v sin i)4.1[8] km/s
Other designations
C Vel, CD−49°3646, FK5 2674, HD 73155, HIP 42088, HR 3407, SAO 220138[9]
Database references
SIMBADdata
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This star has stellar classification of K1.5Ib,[4] which would suggest it is a supergiant, but is actually a giant star according to modern studies.[3] It has about three times the mass of the Sun[3] and has expanded to around 56 times the Sun's radius.[7] The latter is equivalent to 0.26 AU. It is spinning with a projected rotational velocity of 4.1.[8] The star displays microvariability with a period of 10.99 cycles per day and an amplitude of 0.0036 in magnitude.[5] It is radiating around 1,010 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,245 K.[3]

References

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