Planet K2-32 e
| Name | K2-32 e | ||
| Planet Status | Confirmed | ||
| Discovered in | 2019 | ||
| Mass | — | ||
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.04951 (± 0.00055) AU |  |
|
| Orbital Period | 4.34882 ( -0.00075 +0.00069 ) day | |
|
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | 0.0901 (± 0.009) RJ | |
|
| Inclination | — | ||
| Update | 2019-04-02 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | — | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | — | ||
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | 0.22 ( -0.15 +0.17 ) | |
|
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | — | ||
| Calculated temperature | — | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
K2-32| Name | K2-32 | ||
| Distance | — | ||
| Spectral type | G9V | ||
| Apparent magnitude V | 12.31 | ||
| Mass | 0.87 (± 0.04) MSun | |
|
| Age | — | ||
| Effective temperature | 5315.0 (± 60.0) K | |
|
| Radius | 0.87 (± 0.05) RSun | |
|
| Metallicity [Fe/H] | 0.0 | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 16:49:42.3 | ||
| Dec2000 | -19:32:34 | ||
| Alternate Names | EPIC 205071984 | ||
| Planetary system | 4 planets |
Related publications
The Transit Least Squares Survey - I. Discovery and validation of an Earth-sized planet in the four-planet system K2-32 near the 1:2:5:7 resonance
2019
HELLER R., RODENBECK K. & HIPPKE M.
Astron. & Astrophys., 625, A31
paper arxiv
Close-in sub-Neptunes reveal the past rotation history of their host stars: atmospheric evolution of planets in the HD3167 and K2-32 planetary systems
2019
KUBYSHKINA D., CUBILLOS P., FOSSATI L., ERKAEV N., JOHNSTONE C. et al.
ApJ, 879, 26
paper arxiv
Eleven Multi-planet Systems from K2 Campaigns 1 & 2 and the Masses of Two Hot Super-Earths
2015
SINUKOFF E., HOWARD A., PETIGURA E., SCHLIEDER J., CROSSFIELD I. et al.
ApJ, 827, 78
arxiv
paper
ADS
