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Stellar HostProfile

WASP-132

K4 V • 122.9 pc

Records

7

literature rows

Planets

3

system count

References

7

distinct source labels

TIC: TIC 127530399

Approximate color

from effective temperature

Canonical Summary

Adopted host values from one source row

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

7 values • 5 distinct

Mass

0.79 Msun

0.76 to 0.80

4 values • 4 distinct

Radius

0.76 Rsun

0.73 to 0.79

7 values • 5 distinct

Age

7.20 Gyr

0.50 to 7.20

3 values • 3 distinct

Luminosity

-0.58 log(Lsun)

-0.60 to -0.55

4 values • 4 distinct

Distance

122.9 pc

single adopted value

7 values • 1 distinct

Spectral Type

K4 V

Multiple classifications reported

K4 (2), K4 V (1)

Planets

3

Stable across source rows

3

Scale Comparison

Radius against the Sun

Current adopted radius: 0.76 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

WASP-132

0.76 R☉

System Layout

Known planets

3 planets linked to this host

WASP-132 b

Transit

◌

Discovery

2016

Period

7.13 days

Radius

10.10 R⊕

Mass

136.0 M⊕

Eq. Temp

682 K

WASP-132 c

Transit

◌

Discovery

2022

Period

1.01 days

Radius

1.84 R⊕

Mass

6.26 M⊕

Eq. Temp

1329 K

WASP-132 d

Radial Velocity

◌

Discovery

2024

Period

1816.6 days

Radius

—

Mass

1640.0 M⊕

Eq. Temp

107 K

WASP-132: A K-Type Dwarf and Its Three Known Planets

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

Underlying measurements and references

Evidence Summary

Rows

7

Stellar refs

6

System refs

1

Distancestable

7 values • 1 distinct

Parallaxstable

7 values • 1 distinct

Temperaturedisputed

7 values • 5 distinct

Massdisputed

4 values • 4 distinct

Radiusdisputed

7 values • 5 distinct

Agedisputed

3 values • 3 distinct

Luminositydisputed

4 values • 4 distinct

Surface Gravitydisputed

6 values • 5 distinct

Metallicitydisputed

3 values • 3 distinct

Spectral Typedisputed

3 values • 2 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
47420.760.79—-0.55—122.9TICv8TICv8
4812.3—0.73—-0.58—122.9Gaia DR2TICv8
46860.790.767.20-0.58K4 V122.9Grieves et al. 2025TICv8
47140.780.753.20-0.60K4122.9Hord et al. 2022TICv8
47750.800.740.50—K4122.9Hellier et al. 2017TICv8
4775—0.79———122.9ExoFOPTICv8
4775—0.79———122.9ExoFOPTICv8