Planet Kepler-411 e
| Name | Kepler-411 e | ||
| Planet Status | Confirmed | ||
| Discovered in | 2018 | ||
| Mass | 0.03398 ( -0.00346 +0.00346 ) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.186 (± 0.003) AU | |
|
| Orbital Period | 31.509728 (± 8.5e-05) day | |
|
| Eccentricity | 0.016 ( -0.001 +0.002 ) | |
|
| ω | -103.3 ( -1.5 +1.5 ) deg | |
|
| Tperi | — | ||
| Radius | — | ||
| Inclination | 88.04 (± 0.02) deg | |
|
| Update | 2021-02-05 | ||
| Detection Method | TTV | ||
| Mass Detection Method | TTV | ||
| Radius Detection Method | — | ||
| Primary transit | — | ||
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | 1.688 ( -0.006 +0.006 ) | |
|
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | — | ||
| Calculated temperature | 503.0 (± 9.0) K | |
|
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | 2MASS J19102533+4931237 e, KIC 11551692 e, KOI-1781 e, Kepler-411 A e, WISE J191025.33+493124.4 e |
Star
Kepler-411| Name | Kepler-411 | ||
| Distance | 153.59 ( -0.48 +0.48 ) pc | ||
| Spectral type | K2 V | ||
| Apparent magnitude V | 12.5 | ||
| Mass | 0.87 ( -0.04 +0.04 ) MSun | ||
| Age | 0.212 ( --0.031 +0.031 ) Gyr | ||
| Effective temperature | 4974.0 ( -51.0 +46.0 ) K | |
|
| Radius | 0.82 ( -0.02 +0.02 ) RSun | ||
| Metallicity [Fe/H] | 0.23 ( -0.48 +0.37 ) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 19:10:25.3 | ||
| Dec2000 | +49:31:24 | ||
| Alternate Names | KOI-1781, 2MASS J19102533+4931237, KIC 11551692, Kepler-411 A, WISE J191025.33+493124.4 | ||
| Planetary system | 4 planets |
Related publications
Kepler-411 Differential Rotation from Three Transiting Planets
2021
ARAUJO A. & VALIO A.
ApJ. Lett., 907, L5
paper arxiv
Kepler-411 star activity: connection between starspots and superflares
2021
ARAUJO A. & VALLO A.
ApJ. Letters, 922, L23
paper arxiv
Kepler-411: a four-planet system with an active host star
2019
SUN L., IOANNIDIS P., GU Sh., SCHMITT J., WANG X. & KOUWENHOVEN M.
Astron. & Astrophys., 624, A15
paper arxiv
Influence of Stellar Multiplicity on Planet Formation. I. Evidence of Suppressed Planet Formation due to Stellar Companions within 20 AU and Validation of Four Planets from the Kepler Multiple Planet Candidates
2014
WANG J., XIE J.-W., BARCLAY Th. & FISCHER D.
ApJ, 783, 4
paper arxiv ADS
