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58 Ophiuchi

Star in the constellation Ophiuchus From Wikipedia, the free encyclopedia

58 Ophiuchi is a single[9] star in the equatorial constellation of Ophiuchus. It is visible to the naked eye as a faint, yellow-white hued star with an apparent visual magnitude of 4.86.[1] This object is 56 light years away based on parallax,[2] and is drifting further from the Earth with a heliocentric radial velocity of +10 km/s.[5]

Quick facts Constellation, Right ascension ...
58 Ophiuchi
Location of 58 Ophiuchi (circled)
Observation data
Epoch J2000      Equinox ICRS
Constellation Ophiuchus[1]
Right ascension 17h 43m 25.79354s[2]
Declination −21° 40 59.4989[2]
Apparent magnitude (V) 4.86[1]
Characteristics
Evolutionary stage main sequence[2]
Spectral type F5V[3]
U−B color index -0.03[4]
B−V color index +0.47[4]
Astrometry
Radial velocity (Rv)+10.20[5] km/s
Proper motion (μ) RA: −97.253[2] mas/yr
Dec.: −44.614[2] mas/yr
Parallax (π)58.2437±0.1484 mas[2]
Distance56.0 ± 0.1 ly
(17.17 ± 0.04 pc)
Absolute magnitude (MV)+3.63[1]
Details[6]
Mass1.20 M
Radius1.43±0.05 R
Luminosity3.02[1] L
Surface gravity (log g)4.21±0.10 cgs
Temperature6,305±80 K
Metallicity [Fe/H]−0.16±0.06 dex
Rotational velocity (v sin i)12.2±0.7 km/s
Age2.652[7] Gyr
Other designations
58 Oph, BD−21°4712, FK5 1463, GC 24030, GJ 692, HD 160915, HIP 86736, HR 6595, SAO 185660[8]
Database references
SIMBADdata
Close

This is an ordinary F-type main-sequence star with a stellar classification of F5V.[3] It is 2.7[7] billion years old with a projected rotational velocity of 12 km/s. The star has an estimated 1.2 times the mass of the Sun and 1.43 times the Sun's radius.[6] It is radiating three[1] times the luminosity of the Sun from its photosphere at an effective temperature of 6,305 K.[6]

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