HD 108236 is a G-type main-sequence star. Its surface temperature is 5660±61 K. HD 108236 is severely depleted in heavy elements compared to the Sun, with a metallicity Fe/H index of −0.28±0.04 (52% of the Solar System), and is probably older than the Sun at an age of 6.7+3.3
−3.4 billion years.[3]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Centaurus |
Right ascension | 12h 26m 17.8916s[1] |
Declination | −51° 21′ 46.2141″[1] |
Apparent magnitude (V) | 9.24 |
Characteristics | |
Evolutionary stage | main-sequence star |
Spectral type | G5V |
Astrometry | |
Radial velocity (Rv) | 16.78±0.22[2] km/s |
Proper motion (μ) | RA: −70.627[2] mas/yr Dec.: −49.758[2] mas/yr |
Parallax (π) | 15.4861 ± 0.0127 mas[2] |
Distance | 210.6 ± 0.2 ly (64.57 ± 0.05 pc) |
Details[3] | |
Mass | 0.867+0.047 −0.046 M☉ |
Radius | 0.876±0.007 R☉ |
Luminosity | 0.707±0.032 L☉ |
Surface gravity (log g) | 4.49±0.11 cgs |
Temperature | 5660±61 K |
Metallicity [Fe/H] | −0.28±0.04 dex |
Age | 6.7+3.3 −3.4 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
According to WISE mission data, the star was suspected to be surrounded by a debris disk, but a reanalysis of the data rejected the debris disk hypothesis by 2014.[4] The reason for the false positive was contamination from a nearby infrared source.[5]
In 2020, four planets orbiting HD 108236 were discovered[6] by the transit method, followed by another one in 2021.[7]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 4.23+0.41 −0.39 M🜨 |
0.0451±0.0004 | 3.7958785+0.0000076 −0.0000070 |
0.067+0.025 −0.026 |
88.23±0.32° | 1.587±0.028 R🜨 |
c | 8.90+0.67 −0.64 M🜨 |
0.0626±0.0006 | 6.2036717+0.0000092 −0.0000100 |
0.091+0.021 −0.033 |
88.8±0.2° | 2.122±0.025 R🜨 |
d | 7.75+0.91 −0.62 M🜨 |
0.1087±0.0010 | 14.175818+0.000024 −0.000023 |
0.075+0.021 −0.022 |
88.8±0.1° | 2.629±0.031 R🜨 |
e | 8.2+3.8 −1.2 M🜨 |
0.1348±0.0012 | 19.5901277±0.000030 | 0.073+0.014 −0.017 |
89.3±0.1° | 3.008±0.032 R🜨 |
f | 3.95+0.46 −0.32 M🜨 |
0.1773±0.0016 | 29.53935+0.00012 −0.00014 |
0.024+0.024 −0.016 |
89.07±0.03° | 1.89±0.04 R🜨 |