Temperature
3347 K
3347 to 3589.8
Unclassified star โข 15.20 pc
Records
9
literature rows
Planets
2
system count
References
10
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: TICv8 โข System source: TICv8
Temperature
3347 K
3347 to 3589.8
Mass
0.42 Msun
0.24 to 0.45
Radius
0.43 Rsun
0.40 to 0.43
Luminosity
-1.69 log(Lsun)
single adopted value
Distance
15.20 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 0.43 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
GJ 317
0.43 Rโ
System Layout
2 planets linked to this host
GJ 317 is a star 49.6 light-years away. Its spectral type, M2.5 V, marks it as a small, cool red dwarf. It has a mass of 0.421 solar masses and a radius of 0.427 solar radii, both smaller than the Sun's, and a temperature of 3350 K, which is cooler than the Sun's. Two planets are known to orbit this host.
Both planets were found by the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion; repeated wobbles reveal the planet and its orbital period. GJ 317 b was discovered in 2007 and has a minimum mass of 536 Earth masses, roughly 1.69 times Jupiter's mass, with an orbital period of 696 days. GJ 317 c was discovered in 2016 and has a minimum mass of 454 Earth masses, roughly 1.43 times Jupiter's mass, with an orbital period of 6500 days.
Among the listed planets, GJ 317 b has the shortest year, and GJ 317 c has the longest year, by reported estimates. GJ 317 b also has the largest minimum mass, while GJ 317 c has the smallest. As minimum masses, both values are lower bounds on the planets' true masses, and each is larger than Earth's.
Provenance
Evidence Summary
Rows
9
Stellar refs
9
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 3510 | 0.42 | โ | 5 | โ | M2.5 V | 15.20 | Anglada-Escudé et al. 2012 | TICv8 |
| โ | 0.24 | โ | โ | โ | โ | 15.20 | Bryan et al. 2016 | TICv8 |
| 3347 | 0.42 | 0.43 | โ | -1.69 | โ | 15.20 | TICv8 | TICv8 |
| โ | โ | โ | โ | โ | M3.5 V | 15.20 | Hawley et al. 1996 | TICv8 |
| โ | 0.42 | โ | โ | โ | โ | 15.20 | Feng et al. 2020 | TICv8 |
| 3589.8 | โ | โ | โ | โ | โ | 15.20 | Gaia DR2 | TICv8 |
| 3496 | 0.40 | 0.40 | โ | โ | M3.5 V | 15.20 | Morales et al. 2025 | TICv8 |
| 3492.7 | 0.45 | 0.43 | โ | โ | โ | 15.20 | Rosenthal et al. 2021 | TICv8 |
| โ | 0.26 | โ | โ | โ | M3.5 V | 15.20 | Johnson et al. 2007 | TICv8 |