Temperature
3403 K
3318 to 4000.5
M3 V • 62.12 pc
Records
4
literature rows
Planets
1
system count
References
5
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: Waalkes et al. 2021 • System source: TICv8
Temperature
3403 K
3318 to 4000.5
Mass
0.31 Msun
0.31 to 0.32
Radius
0.33 Rsun
0.33 to 0.33
Age
2 Gyr
single adopted value
Luminosity
-1.85 log(Lsun)
-1.89 to -1.85
Distance
62.12 pc
single adopted value
Spectral Type
M3 V
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 0.33 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
TOI-122
0.33 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2020
Period
5.08 days
Radius
2.72 R⊕
Mass
—
Eq. Temp
471 K
TOI-122 is an M3 V star, a small, cool red dwarf, located 203 light-years away. Its reported mass is 0.312 solar masses, its reported radius is 0.334 solar radii, and its reported temperature is 3400 K. This star's reported mass and radius estimates are smaller than the Sun's, and its reported temperature is cooler than the Sun's. Its age is given as a reported lower limit of 2 billion years, a bound rather than an exact value. One planet is known to orbit this host.
That planet, TOI-122 b, is a Neptune-like world discovered in 2020 by the transit method. Its orbital period is 5.08 days, and its radius is 2.72 Earth radii, larger than Earth's. Because a Neptune-like classification compares radius with Earth's, it places the planet in the size range reaching up to four times Earth's radius.
Provenance
Evidence Summary
Rows
4
Stellar refs
4
System refs
1