HR 3407

Last updated
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 supergiant
Spectral type K1.5Ib [3]
U−B color index +1.38 [2]
B−V color index +1.33 [2]
Variable type microvariable [4]
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]
Distance 1,040 ± 50  ly
(320 ± 20  pc)
Absolute magnitude  (MV)–2.06 [5]
Details
Mass 3.3±1.1 [6]   M
Radius 73 [7]   R
Luminosity 34.36 - 38.02 [7]   L
Surface gravity (log g)2.0 [8]   cgs
Temperature 3,745±170 [7]   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
SIMBAD data

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]

This object is an aging K-type supergiant star with a stellar classification of K1.5Ib. [3] It has about three [6] times the mass of the Sun and has expanded to around 71 [1] times the Sun's radius. The latter is equivalent to 0.33  AU, or about one third the distance from the Sun to the Earth. 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. [4] It is radiating around 1,600 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,324 K. [1]

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References

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