Temperature
5400 K
5400 to 5518
Unclassified star • 184.8 pc
Records
10
literature rows
Planets
1
system count
References
11
distinct source labels
Approximate color
from effective temperature
Canonical Summary
Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.
Stellar source: Knudstrup et al. 2024 • System source: TICv8
Temperature
5400 K
5400 to 5518
Mass
0.89 Msun
0.89 to 1.06
Radius
0.84 Rsun
0.84 to 1.01
Age
7 Gyr
single adopted value
Distance
184.8 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 0.84 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
WASP-50
0.84 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2011
Period
1.96 days
Radius
13.07 R⊕
Mass
466.8 M⊕
Eq. Temp
1394.8 K
WASP-50 is a star 603 light-years away, and the single planet reported to orbit it is WASP-50 b. The star is 7 billion years old, with a reported mass of 0.89 solar masses and a reported radius of 0.84 solar radii, both smaller than the Sun's. Its temperature is 5400 K, cooler than the Sun's.
WASP-50 b is a Jupiter-like planet, a class defined by a radius exceeding 4 times Earth's. It was discovered by transit, the method in which a planet passing in front of its star from our viewpoint causes a small dip in observed brightness; repeated dips help establish orbital periods. Its orbital period is 1.96 days.
The planet's radius is 13.1 Earth radii, larger than Earth's, and its mass is 467 Earth masses, also larger than Earth's and roughly 1.47 times Jupiter's mass. Its mean density is 1.15 g/cm³, 0.209 times Earth's.
Provenance
Evidence Summary
Rows
10
Stellar refs
10
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5400 | — | 0.87 | — | — | — | 184.8 | ExoFOP | TICv8 |
| 5400 | 0.89 | 0.84 | 7 | — | — | 184.8 | Knudstrup et al. 2024 | TICv8 |
| 5518 | 0.93 | 1.01 | — | — | — | 184.8 | Mortier et al. 2013 | TICv8 |
| 5518 | 0.97 | 0.87 | — | -0.20 | — | 184.8 | TICv8 | TICv8 |
| 5400 | 0.89 | 0.84 | 7 | — | — | 184.8 | Bonomo et al. 2017 | TICv8 |
| 5400 | 1.06 | 0.89 | — | — | — | 184.8 | Stassun et al. 2017 | TICv8 |
| 5400 | — | — | — | — | — | 184.8 | Yalçınkaya et al. 2024 | TICv8 |
| 5400 | 0.89 | 0.84 | — | — | — | 184.8 | Chakrabarty & Sengupta 2019 | TICv8 |
| 5434 | — | 0.90 | — | -0.20 | — | 184.8 | Gaia DR2 | TICv8 |
| 5400 | 0.89 | 0.84 | — | — | — | 184.8 | Gillon et al. 2011 | TICv8 |