Temperature
3876 K
3876 to 4201.9
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Stellar HostProfile
TOI-1732
Unclassified star • 74.76 pc
Records
3
literature rows
Planets
1
system count
References
4
distinct source labels
TIC: TIC 470987100
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: TICv8 • System source: TICv8
Mass
0.61 Msun
single adopted value
Radius
0.63 Rsun
single adopted value
Luminosity
-1.09 log(Lsun)
single adopted value
Distance
74.76 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.63 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
TOI-1732
0.63 R☉
System Layout
Known planets
1 planets linked to this host
TOI-1732 b
Transit
◌
Discovery
2026
Period
4.12 days
Radius
2.50 R⊕
Mass
—
Eq. Temp
—
TOI-1732 and Its Super-Earth
TOI-1732 is a star 244 light-years away with a mass of 0.614 solar masses and a radius of 0.633 solar radii. Its temperature is 3880 K. The star's reported mass and radius estimates are each smaller than the Sun's, and its reported temperature is cooler than the Sun's. One planet orbits this star.
TOI-1732 b is a Super-Earth discovered by transit in 2026. It has an orbital period of 4.12 days and a radius of 2.5 Earth radii, larger than Earth's. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness, and repeated dips help establish orbital periods. A Super-Earth reaches 2.5 times Earth's radius, a size classification based on radius rather than composition.
Provenance
Underlying measurements and references
Evidence Summary
Rows
3
Stellar refs
3
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massstable
Radiusstable
Luminositystable
Surface Gravitydisputed