44 Ophiuchi

44 Ophiuchi is a single star in the constellation Ophiuchus. It has the Bayer designation b Ophiuchi, while 44 Ophiuchi is the Flamsteed designation. It is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 4.16. The distance to this object is approximately 83.2 light years based on parallax. It is drifting closer to the Earth with a heliocentric radial velocity of -37.2 km/s, and is predicted to come within 30 light-years around 585,000 years from now.

44 Ophiuchi
Location of 44 Ophiuchi (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Ophiuchus
Right ascension 17h 26m 22.21749s
Declination −24° 10 31.1190
Apparent magnitude (V) 4.16
Characteristics
Spectral type kA5hA9mF1III
U−B color index +0.12
B−V color index +0.28
Astrometry
Radial velocity (Rv)−37.20 km/s
Proper motion (μ) RA: +0.10 mas/yr
Dec.: −118.18 mas/yr
Parallax (π)39.22 ± 0.24 mas
Distance83.2 ± 0.5 ly
(25.5 ± 0.2 pc)
Absolute magnitude (MV)2.13
Details
Mass1.77 M
Radius1.9 R
Luminosity13 L
Surface gravity (log g)4.15 cgs
Temperature7,559 K
Metallicity [Fe/H]+0.30 dex
Rotational velocity (v sin i)78 km/s
Age1.028 Gyr
Other designations
b Oph, 44 Oph, CD−24°13337, FK5 1457, GC 23597, GJ 9591, HD 157792, HIP 85340, HR 6486, SAO 185401
Database references
SIMBADdata

This is an Am star with a stellar classification of kA5hA9mF1III, indicating it has the luminosity class of a giant star with a spectrum that matches an A5 star based on the calcium K line, and an A9 star from the hydrogen and metal lines. It is around a billion years old with 1.77 times the mass of the Sun and 1.9 times the Sun's girth. The star is radiating 13 times the Sun's luminosity from its photosphere at an effective temperature of 7,559 K. It retains a moderately high rotation rate, showing a projected rotational velocity of 78 km/s.

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