Planet WASP-71 b
| Name | WASP-71 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2012 | ||
| Mass | 2.258 ( -0.072 +0.072 ) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.04631 (± 0.0006) AU | |
|
| Orbital Period | 2.9036747 (± 6.8e-06) day | |
|
| Eccentricity | 0.0 | |
|
| ω | — | ||
| Tperi | — | ||
| Radius | 1.5 ( -0.11 +0.11 ) RJ | |
|
| Inclination | 84.2 (± 1.8) deg | |
|
| Update | 2012-11-14 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | — | ||
| Radius Detection Method | — | ||
| Primary transit | 2455738.84977 (± 0.0007) JD | |
|
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | — | ||
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | — | ||
| Calculated temperature | — | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | 3.36 | ||
| Alternate Names | — |
Star
WASP-71| Name | WASP-71 | ||
| Distance | 200.0 (± 20.0) pc | |
|
| Spectral type | F8 | ||
| Apparent magnitude V | — | ||
| Mass | 1.572 (± 0.062) MSun | |
|
| Age | — | ||
| Effective temperature | 6050.0 (± 100.0) K | |
|
| Radius | 2.32 (± 0.14) RSun | |
|
| Metallicity [Fe/H] | 0.15 (± 0.07) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 01:57:03.0 | ||
| Dec2000 | +00:45:32 | ||
| Alternate Names | |||
| Planetary system | 1 planet |
Related publications
Rossiter--McLaughlin models and their effect on estimates of stellar rotation, illustrated using six WASP systems
2017
BROWN D., TRIAUD A., DOYLE A., GILLON M., LENDL M. et al.
MNRAS, 464, 810
paper arxiv
The radial velocity fitting challenge. I. Simulating the data set including realistic stellar radial-velocity signals
2016
DUMUSQUE X.
Astron. & Astrophys., 593, A5
paper
paper
ADS
Tidal Dissipation and Obliquity Evolution in Hot Jupiter Systems
2014
VALSECCHI F. & RASIO F.
ApJ, 786, 102
paper arxiv
WASP-71b: a bloated hot Jupiter in an 2.9-day, prograde orbit around an evolved F8 star
2012
SMITH A., ANDERSON D., BOUCHY F., COLLIER CAMERON A., DOYLE A. & 17 additional authors
Astron. & Astrophys. , 552, A120
paper arxiv
