Planet TAP 26 b
| Name | TAP 26 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2017 | ||
| Mass | — | ||
| Mass*sin(i) | 1.73 ( -0.27 +0.27 ) MJ |  |
|
| Semi-Major Axis | 0.0975 (± 0.0032) AU | |
|
| Orbital Period | 10.91 (± 0.11) day | |
|
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | — | ||
| Inclination | — | ||
| Update | 2017-01-09 | ||
| Detection Method | Radial Velocity | ||
| Mass Detection Method | Radial Velocity | ||
| Radius Detection Method | — | ||
| Primary transit | — | ||
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | — | ||
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | 154.0 (± 22.0) m/s | |
|
| Calculated temperature | — | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
TAP 26| Name | TAP 26 | ||
| Distance | — | |
|
| Spectral type | K7 | ||
| Apparent magnitude V | 12.4 | ||
| Mass | 1.04 (± 0.1) MSun | |
|
| Age | 0.017 Gyr | |
|
| Effective temperature | — | ||
| Radius | 1.36 (± 0.17) RSun | |
|
| Metallicity [Fe/H] | — | ||
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 04:18:52.0 | ||
| Dec2000 | +17:23:17 | ||
| Alternate Names | |||
| Planetary system | 1 planet |
Related publications
Close-by planets and flares in their host stars
2018
LANZA A.
Astron. & Astrophys., 610, A81
paper arxiv
A hot Jupiter around the very active weak-line T Tauri star TAP 26
2017
YU L., DONATI J.-F., HEBRARD G., MOUTOU C., MALO L. et al.
MNRAS, submitted
arxiv
The fate of close-in planets: tidal or magnetic migration?
2017
STRUGAREK A., BOLMONT E., MATHIS S., BRUN S., REVILLE V. et al.
ApJ. Letters, 847, L16
paper arxiv
