Temperature
5260 K
5260 to 5348
K0 • 117.6 pc
Records
5
literature rows
Planets
1
system count
References
6
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: Hellier et al. 2017 • System source: TICv8
Temperature
5260 K
5260 to 5348
Mass
0.90 Msun
0.90 to 0.92
Radius
0.87 Rsun
0.83 to 0.87
Age
0.50 Gyr
single adopted value
Distance
117.6 pc
single adopted value
Spectral Type
K0
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 0.87 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
WASP-140
0.87 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2016
Period
—
Radius
14.24 R⊕
Mass
—
Eq. Temp
1270 K
WASP-140 is a K0 star located 384 light-years away. Its reported mass is 0.9 solar masses and its reported radius is 0.87 solar radii, both smaller than the Sun's. The star's reported temperature is 5260 K, cooler than the Sun's, and its age carries a reported lower limit of 0.5 billion years. One planet is known to orbit this host.
That planet, WASP-140 b, was discovered in 2016 by the transit method, which detects the small dip in a star's brightness when a planet crosses in front of it from our viewpoint. WASP-140 b is Jupiter-like, a size class for planets exceeding 4 times Earth's radius. Its reported radius estimate is 14.2 Earth radii, larger than Earth's. No orbital period is reported for WASP-140 b.
Provenance
Evidence Summary
Rows
5
Stellar refs
5
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5260 | — | 0.84 | — | — | — | 117.6 | ExoFOP | TICv8 |
| 5348 | 0.92 | 0.84 | — | -0.28 | — | 117.6 | TICv8 | TICv8 |
| 5300 | — | — | — | — | K0 | 117.6 | Alexoudi 2022 | TICv8 |
| 5333.8 | — | 0.83 | — | -0.29 | — | 117.6 | Gaia DR2 | TICv8 |
| 5260 | 0.90 | 0.87 | 0.50 | — | K0 | 117.6 | Hellier et al. 2017 | TICv8 |