K2-32

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K2-32
Observation data
Epoch J2000      Equinox J2000
Constellation Ophiuchus[1]
Right ascension 16h 49m 42.2602s[2]
Declination −19° 32′ 34.151″[2]
Apparent magnitude (V) 12.31±0.02[3]
Characteristics
Spectral type G9V[4]
Apparent magnitude (J) 10.404±0.024[5]
Apparent magnitude (H) 9.993±0.025[5]
Apparent magnitude (K) 9.821±0.019[5]
Variable type Planetary transit variable[6]
Distance
510 ± 1 ly
(156.4 ± 0.4 pc)
Details
Gyr
Other designations
Gaia DR2 4130539180358512768, EPIC 205071984, 2MASS J16494226-1932340[8]
Database references
SIMBADdata

K2-32 is a

transiting exoplanets are known to orbit this star.[9] A study of atmospheric escape from the planet K2-32b caused by high-energy stellar irradiation indicates that the star has always been a very slow rotator.[10]

Planetary system

Discovery

The star K2-32 was initially found to have three transiting planet candidates by Andrew Vanderburg and collaborators in 2016.

The Earth-sized planet K2-32e was discovered and validated by René Heller and team in 2019.[9][11]

Transit light curves of all four planets orbiting the star K2-32.[9]

Characteristics

With periods of 4.34, 8.99, 20.66 and 31.71 days the four planets

habitable zone located at 0.58 astronomical units.[12]

Planetary system of the star K2-32 showing planetary radii and orbital resonances.[9]
The K2-32 planetary system[9][3][13]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
K2-32e 2.1+1.3
−1.1
 M🜨
0.04899+0.00041
−0.00038
4.34934±0.00039 0.043+0.048
−0.030
89.0±0.7° 1.212+0.052
−0.046
 R🜨
K2-32b 15.0+1.8
−1.7
 M🜨
0.07950+0.00066
−0.00062
8.992±0.00008 0.03+0.032
−0.02
89.0+0.5
−0.3
°
5.299±0.191 R🜨
K2-32c 8.1±2.4 M🜨 0.13843+0.00115
−0.00108
20.66093+0.00080
−0.00079
0.049+0.046
−0.035
89.4+0.3
−0.2
°
2.134+0.123
−0.102
 R🜨
K2-32d 6.7±2.5 M🜨 0.18422+0.00152
−0.00144
31.71701+0.00101
−0.00096
0.05+0.053
−0.035
89.4±0.1° 3.484+0.112
−0.129
 R🜨

References

External links

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