HD 108236

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HD 108236
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
Distance
210.6 ± 0.2 ly
(64.57 ± 0.05 pc)
Details
Gyr
TYC 8243-1948-1, GSC 08243-01948, 2MASS J12261789-5121462[1]
Database references
SIMBADdata

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]

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]

Planetary system

HD 108236's planets

In 2020, four planets orbiting HD 108236 were discovered

transit method, followed by another one in 2021.[7]

The HD 108236 planetary system[3][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🜨

See also

References

  1. ^ a b c "HD 108236". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-01-17.
  2. ^ .
  3. ^
  4. .
  5. ^ .