HD 173417

Star in the constellation Lyra From Wikipedia, the free encyclopedia

HD 173417 is a single[9] star in the northern constellation of Lyra. It is dimly visible to the naked eye with an apparent visual magnitude of 5.68,[3] positioned about two degrees to the southwest of the bright star Sheliak.[10] The distance to this star is approximately 169 light years based on parallax measurements, and it is slowly drifting closer with a radial velocity of −3 km/s.[2]

Right ascension18h 43m 51.59217s[2]
Declination+31° 55 35.8058[2]
Quick facts Constellation, Right ascension ...
HD 173417
Observation data
Epoch J2000.0      Equinox ICRS
Constellation Lyra[1]
Right ascension 18h 43m 51.59217s[2]
Declination +31° 55 35.8058[2]
Apparent magnitude (V) 5.68[3]
Characteristics
Spectral type F1III-IV[4]
B−V color index +0.360±0.004[3]
Variable type Constant[5]
Astrometry
Radial velocity (Rv)−3.26±0.57[2] km/s
Proper motion (μ) RA: −32.768[2] mas/yr
Dec.: −125.812[2] mas/yr
Parallax (π)19.27±0.60 mas[2]
Distance169 ± 5 ly
(52 ± 2 pc)
Absolute magnitude (MV)2.17[1]
Details
Mass1.60[6] M
Radius2.243[3] R
Luminosity10.407[3] L
Surface gravity (log g)3.91[6] cgs
Temperature6,928[3] K
Metallicity [Fe/H]−0.21[6] dex
Rotational velocity (v sin i)53.9±2.7[7] km/s
Age1.70[6] Gyr
Other designations
BD+31°3348, GC 25643, HD 173417, HIP 91883, HR 7044, SAO 67293, GSC 02641-02397[8]
Database references
SIMBADdata
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The stellar classification of this star is F1III-IV,[4] matching an evolving star with the mixed luminosity traits of a subgiant and giant star. It is 1.7 billion years old with a low metallicity and a relatively high projected rotational velocity of 54 km/s.[7] The star has 1.6[6] times the mass of the Sun and 2.2 times the Sun's radius. It is radiating over 10 times the luminosity of the Sun from its photosphere at an effective temperature of 6,928 K.[3]

References

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