30 Ophiuchi

Star in the constellation Ophiuchus From Wikipedia, the free encyclopedia

30 Ophiuchi is a single[11] star in the equatorial constellation of Ophiuchus, and figures 0.99° east (specifically E½S) of the heart of cluster Messier 10.[12] It is visible to the naked eye as a faint, orange-hued point of light with an apparent visual magnitude of 4.82.[2] The distance to this star is approximately 350 light years based on parallax.[7] Its present motion is, net, one of approaching rather than parting, at 6.7 km/s, its "radial velocity".[6]

Right ascension17h 01m 03.60142s[1]
Declination−04° 13 21.5308[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
30 Ophiuchi
Location of 30 Ophiuchi (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Ophiuchus
Right ascension 17h 01m 03.60142s[1]
Declination −04° 13 21.5308[1]
Apparent magnitude (V) 4.82[2]
Characteristics
Spectral type K4III[3]
U−B color index +1.80[4]
B−V color index +1.48[4]
Variable type none[5]
Astrometry
Radial velocity (Rv)−6.70[6] km/s
Proper motion (μ) RA: −39.13[7] mas/yr
Dec.: −78.09[7] mas/yr
Parallax (π)9.3138±0.1676 mas[1]
Distance350 ± 6 ly
(107 ± 2 pc)
Absolute magnitude (MV)−0.65[2]
Details
Radius35.89+0.54
−2.12
[1] R
Luminosity299.8±6.2[1] L
Surface gravity (log g)1.73[8] cgs
Temperature4,009.00+126.67
−29.67
[1] K
Metallicity [Fe/H]−0.03[2] dex
Rotational velocity (v sin i)1.4[9] km/s
Other designations
30 Oph, NSV 8111, BD−04°4215, FK5 1445, GC 22937, HD 153687, HIP 83262, HR 6318, SAO 141483, CCDM J17011-0413A, WDS J17011-0413A[10]
Database references
SIMBADdata
Close

This is an aging giant star with a stellar classification of K4III,[3] having exhausted the supply of hydrogen at its core and expanded to 36[1] times the Sun's radius. The star is radiating 300[1] times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,009 K.[1] It is emitting a far infrared excess due to circumstellar dust,[13] which extends out to a diameter of 240 AU and has a mass of 62×1025 g.[14]

The primary presents with two visual companions: B, at magnitude 9.71 and separation 99.8″, and C, at magnitude 8.75 and separation 220.9″ (3′ 40.9″).[15]

References

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