| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Hercules[1] |
| Right ascension | 16h 55m 08.35611s[2] |
| Declination | +20° 29′ 28.7945″[2] |
| Apparent magnitude (V) | 8.85[3] |
| Characteristics | |
| Evolutionary stage | Main sequence[3] |
| Spectral type | G0[3] |
| B−V color index | 0.53[3] |
| Astrometry | |
| Radial velocity (Rv) | 10.06±0.15[2] km/s |
| Proper motion (μ) | RA: 14.838 mas/yr[2] Dec.: 44.635 mas/yr[2] |
| Parallax (π) | 9.1607 ± 0.0152 mas[2] |
| Distance | 356.0 ± 0.6 ly (109.2 ± 0.2 pc) |
| Details[3] | |
| Mass | 1.15±0.04 M☉ |
| Radius | 1.43±0.02 R☉ |
| Surface gravity (log g) | 4.19±0.03 cgs |
| Temperature | 6,310±100 K |
| Metallicity [Fe/H] | −0.16±0.05 dex |
| Rotation | 5.0±0.9 days |
| Rotational velocity (v sin i) | 8.38±0.50 km/s |
| Age | 3.97±0.75 Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 152843 (also designated as TOI-2319) is a single star with a pair of close-orbiting exoplanets,[3] located in the northern constellation of Hercules. It is positioned at a distance of 356 light years from the Sun based on parallax measurements,[2] and at that range is too faint to be viewed with the naked eye, having an apparent visual magnitude of 8.85.[3] The system is receding further away with a radial velocity of 10 km/s.[2]
This is a G-type main-sequence star with a stellar classification of G0.[3] It has 1.15 times the mass and 1.43 times the girth of the Sun. Around four billion years of age,[3] HD 152843 is a quiet star, showing very little magnetic activity in its chromosphere.[5] The abundance of iron, a measure of the star's metallicity, is somewhat lower than in the Sun. It is spinning with a projected rotational velocity of 8.4 km/s.[3]
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