Planet WASP-53 b
| Name | WASP-53 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2011 | ||
| Mass | 2.132 ( -0.094 +0.092 ) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.04101 ( -0.00091 +0.00083 ) AU | |
|
| Orbital Period | 3.3098443 (± 2e-06) day | |
+ |
| Eccentricity | 0.0 ( -0.0 +0.03 ) | ||
| ω | — | ||
| Tperi | — | ||
| Radius | 1.074 ( -0.037 +0.037 ) RJ | |
|
| Inclination | 87.08 ( -0.15 +0.16 ) deg | |
|
| Update | 2021-07-27 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | Radial Velocity | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | 2455943.56695 ( -0.00012 +0.00011 ) JD | ||
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | — | ||
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | 326.1 (± 1.8) m/s | |
|
| Calculated temperature | — | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
WASP-53| Name | WASP-53 | ||
| Distance | 235.0 (± 55.0) pc | |
|
| Spectral type | K3 | ||
| Apparent magnitude V | — | ||
| Mass | 0.839 (± 0.054) MSun | |
|
| Age | — | ||
| Effective temperature | 4953.0 ( -60.0 +59.0 ) K | |
|
| Radius | 0.798 (± 0.023) RSun | |
|
| Metallicity [Fe/H] | 0.22 (± 0.11) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 02:07:38.2 | ||
| Dec2000 | -20:39:43 | ||
| Alternate Names | 2MASS J02073820-2039426 | ||
| Planetary system | 2 planets |
Related publications
Exterior Companions to Hot Jupiters Orbiting Cool Stars are Coplanar
2017
BECKER J., VANDERBURG A., ADAMS F. & BRYAN M.
Astron. J., 154, 230
paper arxiv
Peculiar architectures for the WASP-53 and WASP-81 planet-hosting systems
2016
TRIAUD A., NEVEU-VANMALLE M., LENDL M., ANDERSON D., COLLIER CAMERON A. et al.
MNRAS, submitted
arxiv
A Uniformly Derived Catalogue of Exoplanets from Radial Velocities
2012
HOLLIS M., BALAN S., LEVER G. & LAHAV O.
MNRAS, 423, Issue 3, 2800-2814
paper arxiv
The Exoplanet Handbook
2011
PERRYMAN M.
Content
Content and Chapter 5
