Temperature
4686 K
4686 to 4812.3
K4 V • 122.9 pc
Records
7
literature rows
Planets
3
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: Grieves et al. 2025 • System source: TICv8
Temperature
4686 K
4686 to 4812.3
Mass
0.79 Msun
0.76 to 0.80
Radius
0.76 Rsun
0.73 to 0.79
Age
7.20 Gyr
0.50 to 7.20
Luminosity
-0.58 log(Lsun)
-0.60 to -0.55
Distance
122.9 pc
single adopted value
Spectral Type
K4 V
Multiple classifications reported
Planets
3
Stable across source rows
Scale Comparison
Current adopted radius: 0.76 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
WASP-132
0.76 R☉
System Layout
3 planets linked to this host
Transit
Discovery
2016
Period
7.13 days
Radius
10.10 R⊕
Mass
136.0 M⊕
Eq. Temp
682 K
Transit
Discovery
2022
Period
1.01 days
Radius
1.84 R⊕
Mass
6.26 M⊕
Eq. Temp
1329 K
Radial Velocity
Discovery
2024
Period
1816.6 days
Radius
—
Mass
1640.0 M⊕
Eq. Temp
107 K
WASP-132 is a K4 V star, a spectral type that marks it as somewhat cooler than the Sun, located 401 light-years away. It has three known planets. The star's reported mass estimate is 0.789 solar masses and its radius estimate is 0.758 solar radii, both smaller than the Sun's, and its temperature of 4690 K is cooler than the Sun's. Its age is 7.2 billion years.
WASP-132 b is a Jupiter-like planet discovered by transit in 2016. It has a mass of 136 Earth masses and a radius of 10.1 Earth radii, both larger than Earth's, with a mean density of 0.728 g/cm³, 0.132 times Earth's. Its orbital period is 7.13 days, the second-shortest among the listed planets.
WASP-132 c is a Super-Earth discovered by transit in 2022. Its mass is 6.26 Earth masses and its radius is 1.84 Earth radii, both larger than Earth's, and its mean density is 5.53 g/cm³, 1 times Earth's. It orbits in 1.01 days, the shortest period among the listed planets.
WASP-132 d was discovered in 2024 using the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion. Its minimum mass is 1640 Earth masses, a lower bound on its true mass and roughly 5.16 times Jupiter's mass, also larger than Earth's. Its orbital period is 1820 days, the longest among the listed planets.
Provenance
Evidence Summary
Rows
7
Stellar refs
6
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 4742 | 0.76 | 0.79 | — | -0.55 | — | 122.9 | TICv8 | TICv8 |
| 4812.3 | — | 0.73 | — | -0.58 | — | 122.9 | Gaia DR2 | TICv8 |
| 4686 | 0.79 | 0.76 | 7.20 | -0.58 | K4 V | 122.9 | Grieves et al. 2025 | TICv8 |
| 4714 | 0.78 | 0.75 | 3.20 | -0.60 | K4 | 122.9 | Hord et al. 2022 | TICv8 |
| 4775 | 0.80 | 0.74 | 0.50 | — | K4 | 122.9 | Hellier et al. 2017 | TICv8 |
| 4775 | — | 0.79 | — | — | — | 122.9 | ExoFOP | TICv8 |
| 4775 | — | 0.79 | — | — | — | 122.9 | ExoFOP | TICv8 |