Planet WASP-148 b
| Name | WASP-148 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2020 | ||
| Mass | 0.287 ( -0.016 +0.022 ) MJ |  |
+ |
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.08215 ( -0.0015 +0.00086 ) AU | |
+ |
| Orbital Period | 8.80345 ( -0.00016 +0.00011 ) day | |
+ |
| Eccentricity | 0.208 (± 0.002) | |
+ |
| ω | 60.6 ( -6.0 +5.0 ) deg | |
+ |
| Tperi | — | ||
| Radius | 0.756 ( -0.017 +0.013 ) RJ | |
+ |
| Inclination | 89.3 (± 0.24) deg | |
|
| Update | 2022-04-15 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | Radial Velocity | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | 2457957.4877 (± 0.0059) JD | |
|
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | 0.2 ( -0.07 +0.05 ) | |
+ |
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | 30.1 ( -1.5 +1.6 ) m/s | |
+ |
| Calculated temperature | 940.0 (± 80.0) K | |
|
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
WASP-148| Name | WASP-148 | ||
| Distance | 248.1 (± 1.6) pc | |
|
| Spectral type | — | ||
| Apparent magnitude V | 12.0 | ||
| Mass | 1.0 (± 0.08) MSun | |
|
| Age | — | ||
| Effective temperature | 5460.0 (± 130.0) K | |
|
| Radius | 1.03 (± 0.2) RSun | |
|
| Metallicity [Fe/H] | 0.11 (± 0.08) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 16:56:31.0 | ||
| Dec2000 | +44:18:09 | ||
| Alternate Names | |||
| Planetary system | 2 planets |
Related publications
The Aligned Orbit of WASP-148b, the Only Known Hot Jupiter with a Nearby Warm Jupiter Companion, from NEID and HIRES
2022
WANG X.-Y., RICE M., WANG S., PU B., STEFANSSON G. et al.
ApJ. Letters, 026, L8
paper arxiv
Photodynamical analysis of the nearly resonant planetary system WASP-148. Accurate transit-timing variations and mutual orbital inclination
2022
ALMENARA J., HEBRARD G., DIAZ R., LASKAR J., CORREIA A. et al.
Astron. & Astrophys., in press
paper arxiv
Discovery and characterization of the exoplanets WASP-148b and c. A transiting system with two interacting giant planets
2020
HEBRARD G., DIAZ R., CORREIA A., COLLIER CAMERONA., LASKAR J. et al.
Astron. & Astrophys., 640, A32
paper arxiv
A Newtonian model for the WASP-148 exoplanetary system enhanced with TESS and ground-based photometric observations
2020
MACIEJEWSKI G., FERNANDEZ M., SOTA A. & SEGURA A.
Acta Astron., accepted
arxiv
