HD 114837

Binary star system in the constellation Centaurus From Wikipedia, the free encyclopedia

HD 114837 is a suspected binary star[7][3] system in the southern constellation of Centaurus. The brighter star is faintly visible to the naked eye with an apparent visual magnitude of 4.90.[1] It has a magnitude 10.2 candidate common proper motion companion at an angular separation of 4.2″, as of 2014.[3] The distance to this system, based on an annual parallax shift of 54.825″ as seen from Earth's orbit,[2] is 59.5 light years. It is moving closer with a heliocentric radial velocity of −64 km/s,[5] and will approach to within 21.8 ly in around 240,600 years.[11]

Right ascension13h 14m 15.14474s[2]
Declination−59° 06′ 11.6540″[2]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
HD 114837
Location of HD 114837 (circled in red)
Observation data
Epoch J2000      Equinox J2000
Constellation Centaurus[1]
Right ascension 13h 14m 15.14474s[2]
Declination −59° 06′ 11.6540″[2]
Apparent magnitude (V) 4.90[1] + 10.2[3]
Characteristics
Evolutionary stage main sequence[2]
Spectral type F6 V Fe-0.4[4]
B−V color index 0.489±0.020[1]
Astrometry
Radial velocity (Rv)−64.0±0.3[5] km/s
Proper motion (μ) RA: âˆ’248.678[2] mas/yr
Dec.: âˆ’153.176[2] mas/yr
Parallax (π)54.8247±0.0809 mas[2]
Distance59.49 ± 0.09 ly
(18.24 ± 0.03 pc)
Absolute magnitude (MV)3.73[6]
Details
HD 114837 A
Mass1.14[7] M☉
Radius1.3[8] R☉
Luminosity3.12[1] L☉
Surface gravity (log g)4.21[9] cgs
Temperature6,346±80[9] K
Metallicity [Fe/H]−0.27[9] dex
Rotational velocity (v sin i)8.8±3.0[6] km/s
Age3.40[9] Gyr
Other designations
CD−58°4940, GJ 503, HD 114837, HIP 64583, HR 4989, SAO 240666, WDS J13143-5906A[10]
Database references
SIMBADdata
Close

The primary component is an F-type main-sequence star with a stellar classification of F6 V Fe-0.4,[4] showing a mild underabundance of iron in its spectrum. It is about 3.4[9] billion years old with 1.14[7] times the mass of the Sun and about 1.3[8] times the Sun's radius. This star is radiating 3.12[1] times the Sun's luminosity from its photosphere at an effective temperature of 6,346 K.[9]

References

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