HD 86267

Star in the constellation of Antlia From Wikipedia, the free encyclopedia

HD 86267, also known as HR 3932, is a solitary[14] orange-hued star located in the southern constellation Antlia. It has an apparent magnitude of 5.82,[3] allowing it to be faintly seen with the naked eye. Parallax measurements place it a distance of 514 light years[2] and it is currently receding with a heliocentric radial velocity of 3.7 km/s.[6]

Right ascension09h 56m 35.4937s[2]
Declination−33° 25 06.587[2]
Quick facts Constellation, Right ascension ...
HD 86267
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Antlia[1]
Right ascension 09h 56m 35.4937s[2]
Declination −33° 25 06.587[2]
Apparent magnitude (V) 5.82±0.01[3]
Characteristics
Evolutionary stage RGB[2]
Spectral type K1 III[4]
B−V color index +1.2[5]
Astrometry
Radial velocity (Rv)3.7±0.4[6] km/s
Proper motion (μ) RA: +34.064 mas/yr[2]
Dec.: +22.102 mas/yr[2]
Parallax (π)6.3494±0.0453 mas[2]
Distance514 ± 4 ly
(157 ± 1 pc)
Absolute magnitude (MV)−0.15[1]
Details
Mass1.73+1.24
0.71
[7] M
Radius19.7[8] R
Luminosity158±11[7] L
Surface gravity (log g)1.86[9] cgs
Temperature4430±110[7] K
Metallicity [Fe/H]−0.15[10] dex
Rotational velocity (v sin i)<1[11] km/s
Other designations
36 G. Antliae[12], CD−32°6895, CPD−32°2771, FK5 2796, GC 13695, HD 86267, HIP 48748, HR 3932, SAO 200889[13]
Database references
SIMBADdata
Close

HD 86267 has a stellar classification of K1 III,[4] indicating that it is a red giant. At present it has 1.73 times the mass of the Sun[7] but has expanded to 19.7 times its girth.[8] It shines with a luminosity of 158 L from its enlarged photosphere at an effective temperature of 4,430 K.[7] It is a member of the old disk population, having a metallicity 71% that of the Sun.[10] The value means that it is metal deficient. Its current rotation rate is too low to be measured accurately.[11]

References

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