HD 167257

HD 167257
Observation data
Epoch J2000      Equinox J2000
Constellation Telescopium
Right ascension 18h 17m 00.9195s
Declination –51° 04 05.7597
Apparent magnitude (V) 6.05±0.01
Characteristics
Evolutionary stage main sequence
Spectral type B9V
B−V color index −0.06
Astrometry
Radial velocity (Rv)−5.1±4.3 km/s
Proper motion (μ) RA: +1.260 mas/yr
Dec.: −9.497 mas/yr
Parallax (π)7.7579±0.0512 mas
Distance420 ± 3 ly
(128.9 ± 0.9 pc)
Absolute magnitude (MV)+0.64
Details
Mass2.63±0.06 M
Radius2.8±0.1 R
Luminosity64.6+7.7
−8.7
 L
Surface gravity (log g)3.97±0.06 cgs
Temperature10,139 K
Metallicity [Fe/H]0.00 dex
Rotational velocity (v sin i)61 km/s
Age239 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

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

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