Psi Ophiuchi

Star in the constellation Ophiuchus From Wikipedia, the free encyclopedia

Psi Ophiuchi, which is Latinized from ψ Ophiuchi, is a single[9] star in the equatorial constellation of Ophiuchus, next to the western constellation border with Scorpius. It has an orange hue and is visible to the naked eye as a faint point of light with an apparent visual magnitude of 4.50.[2] It is approximately 199 light-years from Earth, based on parallax.[1]

Right ascension16h 24m 06.18464s[1]
Declination−20° 02 14.3784[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
Psi Ophiuchi
Location of ψ Ophiuchi (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Ophiuchus
Right ascension 16h 24m 06.18464s[1]
Declination −20° 02 14.3784[1]
Apparent magnitude (V) 4.50[2]
Characteristics
Evolutionary stage horizontal branch[3]
Spectral type K0- II-III[4]
U−B color index +0.84[2]
B−V color index +1.03[2]
Astrometry
Radial velocity (Rv)+0.60[5] km/s
Proper motion (μ) RA: −20.29[1] mas/yr
Dec.: −47.65[1] mas/yr
Parallax (π)16.35±0.25 mas[1]
Distance199 ± 3 ly
(61.2 ± 0.9 pc)
Absolute magnitude (MV)0.806[3]
Details[6]
Mass1.61 M
Radius11.45 R
Luminosity65.9 L
Surface gravity (log g)2.56 cgs
Temperature4,864 K
Metallicity [Fe/H]−0.20 dex
Rotational velocity (v sin i)< 1.0[7] km/s
Other designations
ψ Oph, 4 Ophiuchi, BD−19°4365, FK5 1373, GC 22042, HD 147700, HIP 80343, HR 6104, SAO 159892[8]
Database references
SIMBADdata
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It is an aging giant or bright giant star with a stellar classification of K0- II-III,[4] indicating it has exhausted the supply of hydrogen at its core, then cooled and expanded. It presently has 11 times the girth of the Sun and 1.6 times the Sun's mass.[6] It is a red clump giant, meaning it is on the horizontal branch and is generating energy through core helium fusion.[3] It is radiating 66 times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,864 K.[6]

References

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