HD 222237
K-type main-sequence star
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HD 222237 is a K-type main-sequence star located 37.3 light-years (11.4 parsecs) away in the constellation Tucana. With an apparent magnitude of 7.1, it is too faint to be visible to the naked eye. It is somewhat smaller, fainter, and cooler than the Sun, with about 76% of the Sun's mass, 71% of its radius, and just 22% of its luminosity, with an effective temperature of 4,750 Kelvin. It is a low metallicity star, meaning the abundance of elements heavier than helium is lower than in the Sun.[5] No infrared excess has been detected that would otherwise indicate the presence of a circumstellar disk around this star.[8]
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Tucana[1] |
| Right ascension | 23h 39m 37.38737s[2] |
| Declination | −72° 43′ 19.7554″[2] |
| Apparent magnitude (V) | 7.09[3] |
| Characteristics | |
| Evolutionary stage | main sequence |
| Spectral type | K3+V[4] |
| U−B color index | 0.824[3] |
| B−V color index | 1.001[3] |
| V−R color index | 0.585[3] |
| Astrometry | |
| Radial velocity (Rv) | 69.62±0.13[2] km/s |
| Proper motion (μ) | RA: 143.736 mas/yr[2] Dec.: −736.907 mas/yr[2] |
| Parallax (π) | 87.3724±0.0187 mas[2] |
| Distance | 37.329 ± 0.008 ly (11.445 ± 0.002 pc) |
| Absolute magnitude (MV) | 6.80[3] |
| Details | |
| Mass | 0.76±0.09[5] M☉ |
| Radius | 0.71±0.06[5] R☉ |
| Luminosity | 0.22[6] L☉ |
| Surface gravity (log g) | 4.61±0.10[5] cgs |
| Temperature | 4751±139[5] K |
| Metallicity [Fe/H] | −0.32±0.02[5] dex |
| Rotational velocity (v sin i) | 2.4[6] km/s |
| Age | 8.8+5.3 −8.1[6] Gyr |
| Other designations | |
| CD−73 1672, GJ 902, HD 222237, HIP 116745, SAO 258167, LHS 3994, PLX 5721[7] | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
The star hosts one known exoplanet, the super-Jupiter HD 222237 b. This planet was discovered in 2024 using radial velocity as well as astrometry from the Hipparcos and Gaia space telescopes. It has about 5 times the mass of Jupiter, and has an eccentric orbit around its star with a period of about 40 years at a distance of about 11 AU, around the distance of Saturn from the Sun.[5] Direct imaging of the planet with the James Webb Space Telescope is planned.[9]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (years) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 5.19±0.58 MJ | 10.8+1.1 −1.0 |
40.8+5.8 −4.5 |
0.56±0.03 | 49.9+3.4 −2.8° |
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