Temperature
5251 K
5190 to 5251
K0 V • 222.9 pc
Records
3
literature rows
Planets
1
system count
References
4
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: Osborn et al. 2023 • System source: TICv8
Temperature
5251 K
5190 to 5251
Mass
0.88 Msun
single adopted value
Radius
0.87 Rsun
0.87 to 0.96
Age
5 Gyr
single adopted value
Distance
222.9 pc
single adopted value
Spectral Type
K0 V
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
TOI-332
0.87 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2023
Period
0.78 days
Radius
3.20 R⊕
Mass
57.20 M⊕
Eq. Temp
1871 K
TOI-332 is a K0 V star 727 light-years away. Its spectral type identifies a main-sequence dwarf, and it is cooler than the Sun, with a temperature of 5250 K. It is also smaller than the Sun in both mass and radius: 0.88 solar masses and 0.87 solar radii. The star is 5 billion years old, and it hosts one known planet, TOI-332 b.
TOI-332 b is a Neptune-like planet, meaning its radius falls within the range of Neptune-class worlds, up to four times Earth's radius. It was discovered by the transit method, in which a planet crossing the face of its star causes a slight dip in brightness; repeated dips reveal the planet's orbital period. TOI-332 b has an orbital period of 0.777 days.
Its radius measures 3.2 Earth radii, larger than Earth's, and its mass is 57.2 Earth masses, also greater than Earth's. Its mean density is 9.62 g/cm³, 1.75 times Earth's.
Provenance
Evidence Summary
Rows
3
Stellar refs
3
System refs
1