HD 111232

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HD 111232
Observation data
Epoch J2000      Equinox J2000
Constellation Musca
Right ascension 12h 48m 51.75258s[1]
Declination −68° 25′ 30.5471″[1]
Apparent magnitude (V) 7.59[2]
Characteristics
Spectral type G8 V Fe-1.0[3]
B−V color index 0.701±0.003[2]
Distance
94.24 ± 0.07 ly
(28.89 ± 0.02 pc)
Absolute magnitude (MV)5.25[2]
Details
Gyr
HIP 62534, 2MASS J12485177-6825304[8]
Database references
SIMBADdata

HD 111232 is a

light years based on parallax.[1] It is drifting away from the Sun with a radial velocity of +104 km/s,[2] having come to within 14.1 light-years some 264,700 years ago.[9] The absolute magnitude of this star is 5.25,[2]
indicating it would have been visible to the naked eye at that time.

This is an ancient,

Planetary system

A

Gaia DR3.[14] Later in 2022, these parameters were revised along with the detection of a second substellar companion, likely a brown dwarf.[15]

The HD 111232 planetary system[15]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(years)
Eccentricity Inclination Radius
b 7.965+1.128
−0.479
 MJ
2.148+0.088
−0.097
3.201+0.002
−0.001
0.214+0.005
−0.003
93.521+16.622
−18.063
°
c 18.063+4.209
−1.612
 MJ
17.250+2.158
−2.151
72.478+14.115
−12.341
0.558+0.027
−0.028
87.902+13.916
−22.591
°

References