Wikiwand AI

44 Ophiuchi

Star in the constellation Ophiuchus From Wikipedia, the free encyclopedia

44 Ophiuchi is a single[10] 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.[2] The distance to this object is approximately 83.2 light years based on parallax.[1] It is drifting closer to the Earth with a heliocentric radial velocity of -37.2 km/s,[6] and is predicted to come within 30 light-years around 585,000 years from now.[11]

Right ascension17h 26m 22.21749s[1]
Declination−24° 10 31.1190[1]
Quick facts Constellation, Right ascension ...
44 Ophiuchi
Location of 44 Ophiuchi (circled)
Observation data
Epoch J2000      Equinox ICRS
Constellation Ophiuchus
Right ascension 17h 26m 22.21749s[1]
Declination −24° 10 31.1190[1]
Apparent magnitude (V) 4.16[2]
Characteristics
Evolutionary stage main sequence[3]
Spectral type kA5hA9mF1III[4]
U−B color index +0.12[5]
B−V color index +0.28[5]
Astrometry
Radial velocity (Rv)−37.20[6] km/s
Proper motion (μ) RA: +0.10[1] mas/yr
Dec.: −118.18[1] mas/yr
Parallax (π)39.22±0.24 mas[1]
Distance83.2 ± 0.5 ly
(25.5 ± 0.2 pc)
Absolute magnitude (MV)2.13[2]
Details
Mass1.77[3] M
Radius1.9[7] R
Luminosity13[3] L
Surface gravity (log g)4.15[8] cgs
Temperature7,559[8] K
Metallicity [Fe/H]+0.30[2] dex
Rotational velocity (v sin i)78[3] km/s
Age1.028[8] Gyr
Other designations
b Oph, 44 Oph, CD−24°13337, FK5 1457, GC 23597, GJ 9591, HD 157792, HIP 85340, HR 6486, SAO 185401[9]
Database references
SIMBADdata
Close
44 Ophiuchi (44 Oph) is the big bright blue star near the bottom center. Near the middle is the Snake Nebula

This is an Am star with a stellar classification of kA5hA9mF1III,[4] 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[8] with 1.77[3] times the mass of the Sun and 1.9[7] times the Sun's girth. The star is radiating 13[3] times the Sun's luminosity from its photosphere at an effective temperature of 7,559 K.[8] It retains a moderately high rotation rate, showing a projected rotational velocity of 78 km/s.[3]

References

Related Articles

Timelines

Top Qs

Fact Checks