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HD 176871
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HD 176871
HD 176871
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Lyra[1]
Right ascension 19h 01m 17.35683s[2]
Declination +26° 17′ 29.0764″[2]
Apparent magnitude (V) 5.69[1]
Characteristics
Spectral type B5V[3][1][4]
U−B color index −0.55[3]
B−V color index −0.086±0.002[1]
Astrometry
Radial velocity (Rv)−20.4±1.2[1] km/s
Proper motion (μ) RA: −0.489[2] mas/yr
Dec.: −9.207[2] mas/yr
Parallax (π)4.1038±0.0835 mas[2]
Distance790 ± 20 ly
(244 ± 5 pc)
Absolute magnitude (MV)−0.80[1]
Details
Mass4.1[5] M
Radius5.2[6] R
Luminosity394[5] L
Surface gravity (log g)4.5[4] cgs
Temperature11,688[6] K
Rotational velocity (v sin i)268±34[7] km/s
Age11[4] Myr
Other designations
BD+26°3429, FK5 3518, GC 26151, HD 176871, HIP 93393, HR 7202, SAO 86707[8]
Database references
SIMBADdata

HD 176871 is a single[9] star in the northern constellation of Lyra, positioned near the southern constellation border with Vulpecula. This object has a blue-white hue and is dimly visible to the naked eye with an apparent visual magnitude of 5.69.[1] It is located at a distance of approximately 790 light years from the Sun based on parallax, and has an absolute magnitude of −0.80.[1] The star is drifting closer with a radial velocity of −20 km/s.[1]

This is a normal B-type main-sequence star with a stellar classification of B5V,[3] which means it is generating energy via core hydrogen fusion. The star is around 11[4] million years old with 5.4[4] times the mass of the Sun and is spinning rapidly with a projected rotational velocity of 268 km/s.[7] It is radiating 233[10] times the luminosity of the Sun from its photosphere at an effective temperature of 10,540 K.[10]

References

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