HD 186302

HD 186302 (also designated HIP 97507) is a star in the constellation of Pavo. It is 185 light-years (57 parsecs) away from Earth, with an apparent magnitude of 8.76. It was identified in November 2018 as a potential solar sibling to the Sun. Similar by spectrum and size, it was suspected to have formed in the same stellar nursery as the Sun 4.6 billion years ago. Common origin with Sun was found to be unlikely in a 2019 paper, as HD 186302's galactic orbit is very different from Sun's.

HD 186302
Location of HD 186302 (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Pavo
Right ascension 19h 49m 06.43036s
Declination −70° 11 16.7033
Apparent magnitude (V) 8.76±0.01
Characteristics
Spectral type G3/5 V
B−V color index 0.67
Astrometry
Radial velocity (Rv)−1.3±0.3 km/s
Proper motion (μ) RA: −24.004 mas/yr
Dec.: −38.804 mas/yr
Parallax (π)17.6309 ± 0.0147 mas
Distance185.0 ± 0.2 ly
(56.72 ± 0.05 pc)
Absolute magnitude (MV)+5.11
Details
Mass0.97±0.01 M
Radius0.95±0.01 R
Surface gravity (log g)4.47±0.01 cgs
Temperature5,675±15 K
Metallicity [Fe/H]−0.03 dex
Rotational velocity (v sin i)2.30 km/s
Age4.5±0.81 Gyr
Other designations
HD 186302, HIP 97507, 2MASS J19490644-7011167, CD−70°1724
Database references
SIMBADdata
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