11h05m15.0681s, −10° 17′ 28.681″| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Crater |
| Right ascension | 11h05m 15.0688s[1] |
| Declination | –10° 17′ 28.6947″[1] |
| Apparent magnitude (V) | 8.09[2] |
| Characteristics | |
| Spectral type | G5V[3] + M4[4] |
| B−V color index | 0.731±0.017[2] |
| Variable type | none |
| Astrometry | |
| Radial velocity (Rv) | +12.05±0.19[1] km/s |
| Proper motion (μ) | RA: −50.494±0.081[1] mas/yr Dec.: −9.496±0.072[1] mas/yr |
| Parallax (π) | 11.6947 ± 0.0565 mas[1] |
| Distance | 279 ± 1 ly (85.5 ± 0.4 pc) |
| Absolute magnitude (MV) | 3.41[2] |
| Position (relative to HD 96167 A)[4] | |
| Component | HD 96167 B |
| Epoch of observation | 2013 |
| Angular distance | 5.873±0.018″ |
| Position angle | 297.06±0.10° |
| Projected separation | 506 AU |
| Details[5] | |
| HD 96167 A | |
| Mass | 1.16±0.05 M☉ |
| Radius | 1.73±0.18 R☉ |
| Luminosity | 3.39+1.18 −0.88 L☉ |
| Surface gravity (log g) | 4.15±0.06 cgs |
| Temperature | 5,749±25 K |
| Metallicity [Fe/H] | 0.35±0.05 dex |
| Rotational velocity (v sin i) | 1.03±0.36 km/s |
| Age | 5.62±0.83 Gyr |
| HD 96167 B | |
| Mass | 0.23[4] M☉ |
| Other designations | |
BD–09° 3201, Gaia DR2 3758718711877270784, HD 96167, HIP 54195, SAO 156444, PPM 223905, WDS 11053-1017, 2MASS J11051506-1017286[6] | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
HD 96167 is a double star system with an exoplanetary companion in the southern constellationofCrater. The apparent visual magnitude of this system is 8.09,[2] which is too faint to be readily visible to the naked eye. It is located at a distance of approximately 279 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +12 km/s.[1]
The primary component, designated HD 96167 A, is an ordinary G-type main-sequence star with a stellar classification of G5V.[3] It has also been classified as a subgiant star,[7] suggesting it is somewhat more evolved having exhausted the hydrogen at its core. The star has an absolute magnitude of 3.41,[2] placing it about a magnitude above the main sequence.[7] It is metal rich and is around six billion years old.[5] This star is larger, brighter and more massive than the Sun.
A faint co-moving stellar companion, component HD 96167 B, was detected in 2014 at a projected separation 506 AU from the primary. The existence of additional stellar companions was ruled out at projected distances from 51 to 740 astronomical units.[4]
In 2009 it was found that primary star HD 96167 A is orbited by a Jovian planet on an eccentric orbit.[7]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | ≥0.71±0.18 MJ | 1.332±0.092 | 498.1±0.81 | 0.681±0.033 | — | — |
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