Discovery Method
Transit
Consistent across records
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ExoplanetDetail
WASP-113 b
Host star WASP-113 • 15.79 R⊕ • 4.54 d orbit
Records
7
archive rows
Discovery
2016
Transit
Radius
15.79 R⊕
default parameter set
Mass
151.0 M⊕
default parameter set
WASP-113
1496 K equilibrium
Canonical Summary
Adopted planet values from the default parameter set
Values come from the archive's default parameter set. Missing values stay missing. Ranges and counts describe all source rows.
Selected source: Barros et al. 2016
Host Star
WASP-113
Stable across source rows
Discovery Year
2016
Stable across source rows
Orbital Period
4.54 day
4.54 to 4.54
Semi-Major Axis
0.06 au
single adopted value
Radius
15.79 Rearth
15.79 to 17.38
Mass
151.0 Mearth
single adopted value
Density
0.23 g/cm**3
0.20 to 0.23
Equilibrium Temperature
1496 K
1460 to 1496
Scale Comparison
Radius against familiar reference worlds
Current adopted radius: 15.79 R⊕ • circles scaled linearly by radius
Earth
1.0 R⊕ baseline
WASP-113 b
15.79 R⊕
Jupiter
11.2 R⊕ reference
Provenance
Underlying measurements and references
Evidence Summary
Rows
7
Refs
7
Methods
1
Discoverystable
Facilitystable
Periodstable
Radiusdisputed
Massstable
Eq. Tempdisputed
| Year | Method | Facility | Telescope | Period | Radius | Mass | Eq. Temp | Reference |
|---|---|---|---|---|---|---|---|---|
| 2016 | Transit | SuperWASP-North | Canon 200mm f/1.8L | — | 16.48 Rearth | — | 1460 K | Alexoudi 2022 |
| 2016 | Transit | SuperWASP-North | Canon 200mm f/1.8L | 4.54 day | 15.79 Rearth | 151.0 Mearth | 1496 K | Barros et al. 2016 |
| 2016 | Transit | SuperWASP-North | Canon 200mm f/1.8L | 4.54 day | — | — | — | Ivshina & Winn 2022 |
| 2016 | Transit | SuperWASP-North | Canon 200mm f/1.8L | 4.54 day | — | — | — | Patel & Espinoza 2022 |
| 2016 | Transit | SuperWASP-North | Canon 200mm f/1.8L | 4.54 day | 17.38 Rearth | — | 1491 K | ExoFOP |
| 2016 | Transit | SuperWASP-North | Canon 200mm f/1.8L | 4.54 day | — | — | — | Kokori et al. 2023 |
| 2016 | Transit | SuperWASP-North | Canon 200mm f/1.8L | 4.54 day | — | — | — | Kokori et al. 2022 |