Temperature
3435 K
3435 to 3457
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Stellar HostProfile
TOI-2094
M3 V • 50.02 pc
Records
3
literature rows
Planets
1
system count
References
4
distinct source labels
TIC: TIC 356016119
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: Jiang et al. 2026 • System source: TICv8
Mass
0.42 Msun
0.37 to 0.42
Radius
0.38 Rsun
0.38 to 0.38
Luminosity
-1.74 log(Lsun)
-1.74 to -1.74
Distance
50.02 pc
single adopted value
Spectral Type
M3 V
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.38 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
TOI-2094
0.38 R☉
System Layout
Known planets
1 planets linked to this host
TOI-2094 b
Transit
◌
Discovery
2026
Period
18.79 days
Radius
1.90 R⊕
Mass
—
Eq. Temp
276 K
TOI-2094 and Its Planet
TOI-2094 is a star 163 light-years from Earth with a spectral type of M3 V, an M-type main-sequence dwarf that is small and cool and red. Its reported mass estimate is 0.425 solar masses and its reported radius estimate is 0.384 solar radii, both smaller than the Sun's, and its temperature of 3440 K is cooler than the Sun's. One planet is known to orbit this host.
TOI-2094 b is a Super-Earth discovered by transit in 2026. It completes an orbit every 18.8 days and has a radius of 1.9 Earth radii, larger than Earth's. A transit occurs when a planet passes in front of its star from our viewpoint, dimming the star slightly; repeated dips reveal the planet's orbital period.
Provenance
Underlying measurements and references
Evidence Summary
Rows
3
Stellar refs
3
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitystable
Spectral Typestable