Temperature
3342 K
3342 to 3683.4
Unclassified star โข 5.58 pc
Records
10
literature rows
Planets
2
system count
References
11
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: Beard et al. 2025 โข System source: TICv8
Temperature
3342 K
3342 to 3683.4
Mass
0.35 Msun
0.35 to 0.36
Radius
0.36 Rsun
0.36 to 0.38
Age
6.80 Gyr
single adopted value
Luminosity
-1.81 log(Lsun)
-1.81 to -1.70
Distance
5.58 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 0.36 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
GJ 251
0.36 Rโ
System Layout
2 planets linked to this host
GJ 251 is a small, cool star 18.2 light-years away with an M3.0V spectral type, meaning it is a red dwarf. Its mass is 0.35 solar masses, its radius is 0.36 solar radii, and its temperature is 3340 K. The star is estimated to be 6.8 billion years old. Two planets are known to orbit it.
Both planets were found using the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion. GJ 251 b, discovered in 2020, has a minimum mass of 3.85 Earth masses and an orbital period of 14.2 days. GJ 251 c, discovered in 2025, has a minimum mass of 3.88 Earth masses and an orbital period of 53.6 days. Minimum mass is a lower bound on a planet's true mass, not an ordinary mass estimate, so each planet's actual mass is at least the stated value. Both planets' minimum masses are larger than Earth's. Among the listed planets, GJ 251 b has the shortest year and the smallest minimum mass, while GJ 251 c has the longest year and the largest minimum mass.
Provenance
Evidence Summary
Rows
10
Stellar refs
10
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 3683.4 | โ | โ | โ | โ | โ | 5.58 | Gaia DR2 | TICv8 |
| 3423 | 0.35 | 0.38 | โ | -1.70 | M3.0V | 5.58 | Turnbull 2015 | TICv8 |
| โ | โ | โ | โ | โ | โ | 5.58 | Nidever et al. 2002 | TICv8 |
| 3342 | 0.35 | 0.36 | 6.80 | -1.81 | โ | 5.58 | Beard et al. 2025 | TICv8 |
| 3398 | 0.35 | 0.37 | โ | -1.79 | โ | 5.58 | TICv8 | TICv8 |
| 3451 | 0.36 | 0.36 | โ | -1.77 | M3.0 V | 5.58 | Stock et al. 2020 | TICv8 |
| โ | โ | โ | โ | โ | โ | 5.58 | Wright et al. 2004 | TICv8 |
| โ | โ | โ | โ | โ | M3 | 5.58 | Hawley et al. 1996 | TICv8 |
| โ | โ | โ | โ | โ | โ | 5.58 | Duncan et al. 1991 | TICv8 |
| โ | โ | โ | โ | โ | K0 | 5.58 | Cannon & Pickering 1918 | TICv8 |