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] |
Astrometry | |
Radial velocity (Rv) | −1.82±0.14[7] km/s |
Proper motion (μ) | RA: −16.662(18)[2] mas/yr Dec.: −53.564(13)[2] mas/yr |
Parallax (π) | 6.3939 ± 0.0153 mas[2] |
Distance | 510 ± 1 ly (156.4 ± 0.4 pc) |
Details[3] | |
Mass | 0.856±0.028 M☉ |
Radius | 0.845+0.044 −0.035 R☉ |
Surface gravity (log g) | 4.49±0.05 cgs |
Temperature | 5275±60 K |
Metallicity [Fe/H] | −0.02±0.04 dex |
Rotational velocity (v sin i) | 0.7 km/s |
Age | 7.9±4.5 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
K2-32 is a G9-type main sequence star slightly smaller and less massive than the sun.[4] Four confirmed 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]
Roman1987
was invoked but never defined (see the help page).Gaia EDR3
was invoked but never defined (see the help page).Petigura2017
was invoked but never defined (see the help page).Dai2016
was invoked but never defined (see the help page).Skrutskie2006
was invoked but never defined (see the help page).Sinukoff2016
was invoked but never defined (see the help page).Vanderburg2016
was invoked but never defined (see the help page).Simbad
was invoked but never defined (see the help page).Heller2019
was invoked but never defined (see the help page).Kubyshkina2019
was invoked but never defined (see the help page).