Temperature
3505 K
3490 to 3805.5
M2.5 V • 9.44 pc
Records
11
literature rows
Planets
3
system count
References
12
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: Luque et al. 2019 • System source: TICv8
Temperature
3505 K
3490 to 3805.5
Mass
0.34 Msun
0.34 to 0.35
Radius
0.34 Rsun
0.34 to 0.36
Luminosity
-1.80 log(Lsun)
-1.80 to -1.70
Distance
9.44 pc
single adopted value
Spectral Type
M2.5 V
Multiple classifications reported
Planets
3
Stable across source rows
Scale Comparison
Current adopted radius: 0.34 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
GJ 357
0.34 R☉
System Layout
3 planets linked to this host
GJ 357 is an M2.5 V star, a small, cool red dwarf, located 30.8 light-years away. Its mass is 0.342 solar masses, its radius is 0.337 solar radii, and its temperature is 3510 K, all smaller or cooler than the Sun's corresponding values. Three planets are known to orbit this star: GJ 357 b, GJ 357 c, and GJ 357 d.
GJ 357 b was discovered in 2019 by the transit method, which detects the small dip in a star's brightness when a planet crosses in front of it. This planet's radius is 1.2 Earth radii, making it larger than Earth and placing it within the Earth-like size class, and its orbital period is 3.93 days, the shortest year among the listed planets.
GJ 357 c and GJ 357 d were both discovered in 2019 by the radial velocity method, which measures the wobble a planet's gravity induces in its star. GJ 357 c has a minimum mass of 3.4 Earth masses and an orbital period of 9.12 days, the second-shortest year among the listed planets. GJ 357 d has a minimum mass of 6.1 Earth masses and an orbital period of 55.7 days, the longest year among the listed planets. Both minimum masses are larger than Earth's.
Provenance
Evidence Summary
Rows
11
Stellar refs
11
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | 9.44 | Wright et al. 2004 | TICv8 |
| — | — | — | — | — | M2.5 | 9.44 | Hawley et al. 1996 | TICv8 |
| — | — | — | — | — | M2.5 V | 9.44 | Gray et al. 2006 | TICv8 |
| — | 0.35 | 0.36 | — | — | M2.5 V | 9.44 | Weisserman et al. 2026 | TICv8 |
| 3505 | 0.34 | 0.34 | — | — | M2.5 V | 9.44 | Oddo et al. 2023 | TICv8 |
| 3505 | 0.34 | 0.34 | — | -1.80 | M2.5 V | 9.44 | Luque et al. 2019 | TICv8 |
| 3490 | 0.35 | 0.36 | — | -1.76 | — | 9.44 | TICv8 | TICv8 |
| — | — | — | — | — | — | 9.44 | Nidever et al. 2002 | TICv8 |
| 3505 | — | 0.36 | — | — | — | 9.44 | ExoFOP | TICv8 |
| 3805.5 | — | — | — | — | — | 9.44 | Gaia DR2 | TICv8 |
| 3501 | 0.34 | 0.34 | — | -1.70 | K | 9.44 | Turnbull 2015 | TICv8 |