Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Pavo |
Right ascension | 19h 49m 06.43036s [1] |
Declination | −70° 11′ 16.7033″ [1] |
Apparent magnitude (V) | 8.76±0.01 [2] |
Characteristics | |
Spectral type | G3/5 V [3] |
B−V color index | 0.67 [4] |
Astrometry | |
Radial velocity (Rv) | −1.3±0.3 [5] km/s |
Proper motion (μ) |
RA: −24.004
[1]
mas/
yr Dec.: −38.804 [1] mas/ yr |
Parallax (π) | 17.6309 ± 0.0147 mas [1] |
Distance | 185.0 ± 0.2
ly (56.72 ± 0.05 pc) |
Absolute magnitude (MV) | +5.11 [6] |
Details [7] | |
Mass | 0.97±0.01 M☉ |
Radius | 0.95±0.01 R☉ |
Surface gravity (log g) | 4.47±0.01 cgs |
Temperature | 5,675±15 K |
Metallicity [Fe/H] | −0.03 [8] dex |
Rotational velocity (v sin i) | 2.30 [8] km/s |
Age | 4.5±0.81 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 186302 (also designated HIP 97507) [9] 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. [9] 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. [10] 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. [11]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Pavo |
Right ascension | 19h 49m 06.43036s [1] |
Declination | −70° 11′ 16.7033″ [1] |
Apparent magnitude (V) | 8.76±0.01 [2] |
Characteristics | |
Spectral type | G3/5 V [3] |
B−V color index | 0.67 [4] |
Astrometry | |
Radial velocity (Rv) | −1.3±0.3 [5] km/s |
Proper motion (μ) |
RA: −24.004
[1]
mas/
yr Dec.: −38.804 [1] mas/ yr |
Parallax (π) | 17.6309 ± 0.0147 mas [1] |
Distance | 185.0 ± 0.2
ly (56.72 ± 0.05 pc) |
Absolute magnitude (MV) | +5.11 [6] |
Details [7] | |
Mass | 0.97±0.01 M☉ |
Radius | 0.95±0.01 R☉ |
Surface gravity (log g) | 4.47±0.01 cgs |
Temperature | 5,675±15 K |
Metallicity [Fe/H] | −0.03 [8] dex |
Rotational velocity (v sin i) | 2.30 [8] km/s |
Age | 4.5±0.81 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 186302 (also designated HIP 97507) [9] 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. [9] 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. [10] 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. [11]