HD 162826

HD 162826 (HR 6669, HIP 87382) is a star in the constellation Hercules. It is about 110 light-years (34 parsecs) away from Earth. With an apparent magnitude of 6.55, the star can be found with binoculars or a low-power telescope by reference to nearby Vega in the constellation Lyra.

HD 162826
HD 162826
Location of HD 162826 in the constellation Hercules

Observation data
Epoch J2000      Equinox J2000
Constellation Hercules
Right ascension 17h 51m 14.02244s
Declination +40° 04 20.8772
Apparent magnitude (V) 6.55±0.01
Characteristics
Spectral type F8 V
U−B color index +0.04
B−V color index +0.52
Astrometry
Radial velocity (Rv)1.9±0.1 km/s
Proper motion (μ) RA: −16.864 mas/yr
Dec.: +9.833 mas/yr
Parallax (π)30.068 ± 0.0646 mas
Distance108.5 ± 0.2 ly
(33.26 ± 0.07 pc)
Absolute magnitude (MV)+3.92
Details
Mass1.17 M
Radius1.32±0.04 R
Luminosity2.27 L
Surface gravity (log g)4.28+0.02
0.03
 cgs
Temperature6,158±9 K
Metallicity [Fe/H]+0.02±0.04 dex
Rotational velocity (v sin i)5 km/s
Age3.88 Gyr
Other designations
AG+40°1628, BD+40°3225, GC 24279, HD 162826, HIP 87382, HR 6669, SAO 47009, TYC 3093-1946-1, 2MASS J17511402+4004208
Database references
SIMBADdata

The star is considered to be a stellar sibling of the Sun and is the first such sibling to be discovered. Solar siblings are those stars that formed from the same gas cloud and in the same star cluster; the term was introduced in 2009. No planets have been detected orbiting HD 162826, but due to its metallicity, it is likely to harbor terrestrial planets; the star's spectra had been under observation previously.

In November 2018, a second potential solar twin was announced, HD 186302, an 8th magnitude star in the Pavo constellation.

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