WASP-43b
| Temperature map of WASP-43b | |
| Discovery | |
|---|---|
| Discovered by | Coel Hellier et al. | 
| Discovery site | La Silla Observatory / South African Astronomical Observatory | 
| Discovery date | Published April 15, 2011 | 
| transit method (secondary occultation detected later) | |
| Designations | |
| Astrolábos | |
| Orbital characteristics | |
| 0.01526 (± 0.00018) AU | |
| Eccentricity | < 0.0298 | 
| 0.81347753 (± 0.00000071) d | |
| Inclination | 82.33 (± 0.20) | 
| Star | WASP-43 | 
| Physical characteristics | |
| 1.04 +0.07 −0.09 RJ | |
| Mass | 2.03 (± 0.1) MJ | 
| Albedo | <0.06 | 
| Temperature | 1479±13 K (1,206 °C; 2,203 °F, dayside) 755±46 K (482 °C; 899 °F, nightside) | 
WASP-43b, formally named Astrolábos, is a transiting planet in orbit around the young, active, and low-mass star WASP-43 in the constellation Sextans. The planet is a hot Jupiter with a mass twice that of Jupiter, but with a roughly equal radius. WASP-43b was flagged as a candidate by the SuperWASP program, before they conducted follow-ups using instruments at La Silla Observatory in Chile, which confirmed its existence and provided orbital and physical characteristics. The planet's discovery was published on April 14, 2011.
WASP-43b has an orbital period of approximately 0.8 days (19.2 hours), which at the time of discovery was the second-shortest known, surpassed only by WASP-19b. At the time of its discovery, the size of WASP-43b's orbit was the smallest known for a hot Jupiter, probably due to its host star's low mass.