30 Ophiuchi

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

30 Ophiuchi
Location of 30 Ophiuchi (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Ophiuchus
Right ascension 17h 01m 03.60142s
Declination −4° 13 21.5308
Apparent magnitude (V) 4.82
Characteristics
Spectral type K4III
U−B color index +1.80
B−V color index +1.48
Astrometry
Radial velocity (Rv)−6.70 km/s
Proper motion (μ) RA: −39.13 mas/yr
Dec.: −78.09 mas/yr
Parallax (π)9.3138 ± 0.1676 mas
Distance350 ± 6 ly
(107 ± 2 pc)
Absolute magnitude (MV)−0.65
Details
Radius35.89+0.54
−2.12
 R
Luminosity299.8±6.2 L
Surface gravity (log g)1.73 cgs
Temperature4,009.00+126.67
−29.67
 K
Metallicity [Fe/H]−0.03 dex
Rotational velocity (v sin i)1.4 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
Database references
SIMBADdata

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

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″).

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.