Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) |
|
---|---|
Constellation | Triangulum Australe |
Right ascension | 16h 23m 00.1463s[1] |
Declination | −61° 41′ 19.542″[1] |
Apparent magnitude (V) | 8.4[1] |
Characteristics | |
Spectral type | G9V[1] |
Apparent magnitude (B) | 9.0[1] |
Apparent magnitude (J) | 6.963[1] |
Apparent magnitude (H) | 6.640[1] |
Apparent magnitude (K) | 6.571[1] |
B−V color index | 0.6[1] |
Astrometry | |
Radial velocity (Rv) | −27.9 ± 0.2[1] km/s |
Proper motion (μ) | RA: −178.50[1] mas/yr Dec.: −315.21[1] mas/yr |
Parallax (π) | 23.43 ± 0.95[1] mas |
Distance | 139 ± 6 ly (43 ± 2 pc) |
Absolute magnitude (MV) | 5.25[2] |
Details | |
Mass | 0.88 (0.86 to 0.95)[3] M☉ |
Temperature | 5400[4] K |
Metallicity | [Fe/H] = 0.06[4] |
Rotational velocity (v sin i) | 0[3] km/s |
Age | 12.6 (6.0 to 16.6) × 109[4] years |
Other designations | |
Database references | |
SIMBAD | data |
NStED | data |
Extrasolar Planets Encyclopaedia |
data |
HD 147018 is a G-type main sequence star in the constellation of Triangulum Australe.[1] It has an apparent visual magnitude of approximately 8.4.[1] In August 2009, two extrasolar planets, HD 147018 b and HD 147018 c, were reported to be orbiting this star. The planets were found using the radial velocity method, using the CORALIE spectrograph at La Silla Observatory, Chile.[5]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity |
---|---|---|---|---|
b | ≥2.12 ± 0.07 MJ | 0.2388 ± 0.0039 | 44.236 ± 0.008 | 0.4686 ± 0.0081 |
c | ≥6.56 ± 0.32 MJ | 1.922 ± 0.039 | 1008 ± 18 | 0.133 ± 0.011 |