Temperature
3363 K
3247 to 3363
M4 V • 126.1 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: Kanodia et al. 2025 • System source: TICv8
Temperature
3363 K
3247 to 3363
Mass
0.34 Msun
0.33 to 0.34
Radius
0.35 Rsun
0.34 to 0.35
Age
7.80 Gyr
single adopted value
Luminosity
-1.92 log(Lsun)
-1.93 to -1.92
Distance
126.1 pc
single adopted value
Spectral Type
M4 V
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 0.35 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
TOI-7149
0.35 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2025
Period
2.65 days
Radius
13.20 R⊕
Mass
224 M⊕
Eq. Temp
593 K
TOI-7149 is an M4 V star, a small, cool red dwarf, located 411 light-years away. It hosts one known planet. The star is estimated to be 7.8 billion years old, with a mass of 0.344 solar masses, a radius of 0.351 solar radii, and a temperature of 3360 K. Its mass and radius are each smaller than the Sun's, and its temperature is cooler than the Sun's.
The planet, TOI-7149 b, was discovered in 2025 by the transit method, in which a planet passes in front of its star from our viewpoint and causes a small dip in observed brightness, with repeated dips helping to establish its orbital period. It is classified as Jupiter-like, meaning its radius exceeds four times Earth's. Its radius is 13.2 Earth radii, larger than Earth's, and its mass is 224 Earth masses, also larger than Earth's. Its mean density is 0.537 g/cm³, 0.0974 times Earth's. TOI-7149 b completes an orbit every 2.65 days.
Provenance
Evidence Summary
Rows
3
Stellar refs
3
System refs
1