Temperature
3467 K
3241 to 3856.5
M3.5 • 8.80 pc
Records
13
literature rows
Planets
2
system count
References
14
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: Pinamonti et al. 2023 • System source: TICv8
Temperature
3467 K
3241 to 3856.5
Mass
0.45 Msun
0.42 to 0.65
Radius
0.45 Rsun
0.45 to 0.55
Luminosity
-1.59 log(Lsun)
-1.59 to -1.52
Distance
8.80 pc
single adopted value
Spectral Type
M3.5
Multiple classifications reported
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 0.45 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
GJ 849
0.45 R☉
System Layout
2 planets linked to this host
GJ 849 is an M3.5 star, a cool red dwarf, located 28.7 light-years away. Its spectral class places it among the smallest and coolest stellar types. The star's reported mass is 0.45 solar masses and its radius is 0.45 solar radii, both smaller than the Sun's. Its temperature of 3470 K is cooler than the Sun's.
Two planets are known to orbit this host. The first, GJ 849 b, was found by the radial velocity method in 2006. That technique detects the wobble a planet's gravity induces in its star's motion, with repeated wobbles revealing the planet and its orbital period. GJ 849 b has a minimum mass of 284 Earth masses, meaning its true mass is at least that value, and an orbital period of 1930 days - the shortest reported year among the listed planets.
GJ 849 c was discovered by the same method in 2014. Its minimum mass is 315 Earth masses - the largest among the listed planets - and its orbital period is 5990 days, the longest reported year among them. Both planets' minimum masses are larger than Earth's.
The star's reported mass estimate and radius estimate are each smaller than the Sun's, and its reported temperature is cooler than the Sun's.
Provenance
Evidence Summary
Rows
13
Stellar refs
13
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | 0.49 | — | 3 | — | M3.5 V | 8.80 | Butler et al. 2006 | TICv8 |
| 3407 | 0.46 | 0.46 | — | -1.58 | — | 8.80 | TICv8 | TICv8 |
| 3467 | 0.45 | 0.45 | — | -1.59 | M3.5 | 8.80 | Pinamonti et al. 2023 | TICv8 |
| 3241 | 0.65 | 0.53 | — | — | — | 8.80 | Stassun et al. 2017 | TICv8 |
| — | 0.49 | — | — | -1.55 | M3 V | 8.80 | Bonfils et al. 2013 | TICv8 |
| — | — | — | — | — | — | 8.80 | Wright et al. 2004 | TICv8 |
| 3856.5 | — | — | — | — | — | 8.80 | Gaia DR2 | TICv8 |
| 3562.7 | 0.50 | 0.47 | — | — | — | 8.80 | Rosenthal et al. 2021 | TICv8 |
| — | 0.49 | — | — | — | M3.5 | 8.80 | Montet et al. 2014 | TICv8 |
| — | — | — | — | — | M3 V | 8.80 | Walker 1983 | TICv8 |
| — | — | — | — | — | — | 8.80 | Nidever et al. 2002 | TICv8 |
| 3343 | 0.42 | 0.55 | — | -1.52 | M3 | 8.80 | Turnbull 2015 | TICv8 |
| — | — | — | — | — | M3.5 | 8.80 | Hawley et al. 1996 | TICv8 |