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±0.01[3] |
Characteristics | |
Evolutionary stage | Main sequence[4] |
Spectral type | G0[4] |
Apparent magnitude (B) | 9.38±0.02[3] |
Apparent magnitude (J) | 7.896±0.018[5] |
Apparent magnitude (H) | 7.655±0.016[5] |
Apparent magnitude (K) | 7.629±0.020[5] |
Variable type | planetary transit |
Astrometry | |
Radial velocity (Rv) | 10.06±0.15[2] km/s |
Proper motion (μ) | RA: 14.838±0.010 mas/yr[2] Dec.: 44.635±0.012 mas/yr[2] |
Parallax (π) | 9.1607 ± 0.0152 mas[2] |
Distance | 356.0 ± 0.6 ly (109.2 ± 0.2 pc) |
Details[4] | |
Mass | 1.15±0.04 M☉ |
Radius | 1.43±0.02 R☉ |
Surface gravity (log g) | 4.19±0.03 cgs |
Temperature | 6310±100 K |
Metallicity [Fe/H] | −0.16±0.05 dex |
Rotation | 5.0±0.9 d |
Rotational velocity (v sin i) | 8.38±0.50 km/s |
Age | 3.97±0.75 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
HD 152843 (also designated as TOI-2319) is a single star with a pair of close-orbiting exoplanets,[4] 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.[4] 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.[4] It has 1.15 times the mass and 1.43 times the girth of the Sun. Around four billion years of age,[4] HD 152843 is a quiet star, showing very little magnetic activity in its chromosphere.[7] 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.[4]
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