Temperature
6250 K
6067.2 to 6400.4
Unclassified star • 275.6 pc
Records
6
literature rows
Planets
1
system count
References
7
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
6250 K
6067.2 to 6400.4
Mass
1.41 Msun
1.13 to 1.41
Radius
2.20 Rsun
2.10 to 2.39
Age
3.62 Gyr
single adopted value
Distance
275.6 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 2.20 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
WASP-136
2.20 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2016
Period
—
Radius
16.81 R⊕
Mass
—
Eq. Temp
1630 K
WASP-136 is a single star located 899 light-years away, with a spectral type of F. The star is 1.41 solar masses, making it more massive than the Sun, and its radius of 2.2 solar radii is larger than the Sun's. This star has an age of 3.62 billion years and a temperature of 6250 K, which is hotter than the Sun.
The planet orbiting this host, WASP-136 b, was discovered by the transit method in 2016. With a radius of 16.8 Earth radii, this planet fits within the Jupiter-like classification, since such planets exceed 4 times Earth's radius. The reported radius estimate is larger than Earth's. No orbital period is reported for WASP-136 b.
Provenance
Evidence Summary
Rows
6
Stellar refs
6
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | F | 275.6 | Alexoudi 2022 | TICv8 |
| 6067.2 | 1.13 | 2.39 | — | 0.84 | — | 275.6 | TICv8 | TICv8 |
| 6260 | 1.41 | 2.21 | 3.62 | — | — | 275.6 | Lam et al. 2017 | TICv8 |
| 6067.2 | — | 2.39 | — | — | — | 275.6 | ExoFOP | TICv8 |
| 6400.4 | — | 2.10 | — | 0.82 | — | 275.6 | Gaia DR2 | TICv8 |
| 6250 | 1.41 | 2.20 | 3.62 | — | — | 275.6 | Knudstrup et al. 2024 | TICv8 |