HD 167257

Star in the constellation Telescopium From Wikipedia, the free encyclopedia

HD 167257 (HR 6821) is a solitary star in the southern constellation Telescopium. It has an apparent magnitude of 6.05,[3] making it faintly visible to the naked eye. Parallax measurements place the star at a distance of 420 light years[2] and has a radial velocity of −5.1 km/s,[7] which is poorly constrained. This indicates that it is drifting towards the Solar System.

Right ascension18h 17m 00.9195s[2]
Declination–51° 04 05.7597[2]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
HD 167257
Observation data
Epoch J2000      Equinox J2000
Constellation Telescopium[1]
Right ascension 18h 17m 00.9195s[2]
Declination –51° 04 05.7597[2]
Apparent magnitude (V) 6.05±0.01[3]
Characteristics
Evolutionary stage main sequence[4]
Spectral type B9V[5]
B−V color index −0.06[6]
Astrometry
Radial velocity (Rv)−5.1±4.3[7] km/s
Proper motion (μ) RA: +1.260 mas/yr[2]
Dec.: −9.497 mas/yr[2]
Parallax (π)7.7579±0.0512 mas[2]
Distance420 ± 3 ly
(128.9 ± 0.9 pc)
Absolute magnitude (MV)+0.64[1]
Details
Mass2.63±0.06[4] M
Radius2.8±0.1[8] R
Luminosity64.6+7.7
−8.7
[4] L
Surface gravity (log g)3.97±0.06[8] cgs
Temperature10,139[9] K
Metallicity [Fe/H]0.00[10] dex
Rotational velocity (v sin i)61[11] km/s
Age239[10] Myr
Other designations
7 G. Telescopii, CD–51°11460, CPD−51°10795, GC 24909, HD 167257, HIP 89597, HR 6821, SAO 245372
Database references
SIMBADdata
Close

HD 167257 has a stellar classification of B9 V,[5] indicating that it is an ordinary B-type main-sequence star. It has 2.63 times the mass of the Sun,[4] and 2.8 times the radius of the Sun.[8] It shines with a luminosity of about 65 L[4] from its photosphere at an effective temperature of 10,139 K,[9] giving it a bluish white hue. HD 167257 is estimated to be about 240 million years old[10] – 58.6% through its main sequence lifetime[4] – and spins modestly with a projected rotational velocity of 61 km/s;[11] it has a solar metallicity.[10]

References

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