Temperature
3129 K
3129 to 3837.2
M4 • 4.68 pc
Records
13
literature rows
Planets
4
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: von Braun et al. 2014 • System source: TICv8
Temperature
3129 K
3129 to 3837.2
Mass
0.37 Msun
0.32 to 0.37
Radius
0.38 Rsun
0.30 to 0.40
Luminosity
-1.91 log(Lsun)
-1.91 to -1.70
Distance
4.68 pc
single adopted value
Spectral Type
M4
Multiple classifications reported
Planets
4
Stable across source rows
Scale Comparison
Current adopted radius: 0.38 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
GJ 876
0.38 R☉
System Layout
4 planets linked to this host
Radial Velocity
Discovery
1998
Period
61.12 days
Radius
—
Mass
723.2 M⊕
Eq. Temp
—
Radial Velocity
Discovery
2000
Period
30.09 days
Radius
—
Mass
227.0 M⊕
Eq. Temp
—
Radial Velocity
Discovery
2005
Period
1.94 days
Radius
—
Mass
6.83 M⊕
Eq. Temp
—
Radial Velocity
Discovery
2010
Period
124.3 days
Radius
—
Mass
14.60 M⊕
Eq. Temp
—
GJ 876 is a small, cool red dwarf of spectral type M4, located 15.2 light-years away. Its mass is 0.37 solar masses and its radius is 0.376 solar radii, both smaller than the Sun's corresponding values, and its temperature of 3130 K is cooler than the Sun's. Four planets are known to orbit this star, all discovered by the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion.
GJ 876 b, found in 1998, has a reported mass of 723 Earth masses, larger than Earth's and roughly 2.28 times Jupiter's mass, and the largest reported mass among the listed planets. Its orbital period is 61.1 days, the second-longest among these worlds. GJ 876 c, discovered in 2000, has a reported mass of 227 Earth masses and an orbital period of 30.1 days, the second-shortest among the listed planets.
The two remaining planets are less massive. GJ 876 d, discovered in 2005, has a reported mass of 6.83 Earth masses, the smallest among the listed planets, and completes an orbit in 1.94 days, the shortest period of the four. GJ 876 e, found in 2010, has a reported mass of 14.6 Earth masses, the second-smallest among the listed planets, and an orbital period of 124 days, the longest of the group.
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 |
|---|---|---|---|---|---|---|---|---|
| 3837.2 | — | — | — | — | — | 4.68 | Gaia DR2 | TICv8 |
| — | 0.32 | 0.30 | 1 | -1.91 | — | 4.68 | Rivera et al. 2010 | TICv8 |
| 3271 | 0.34 | 0.35 | — | -1.89 | — | 4.68 | TICv8 | TICv8 |
| — | — | — | — | — | — | 4.68 | Wright et al. 2004 | TICv8 |
| — | — | — | — | — | M4 | 4.68 | Hawley et al. 1996 | TICv8 |
| — | — | — | — | — | — | 4.68 | Nidever et al. 2002 | TICv8 |
| — | 0.33 | — | 2.55 | -1.89 | M4 V | 4.68 | Correia et al. 2010 | TICv8 |
| — | 0.37 | — | — | — | — | 4.68 | Nelson et al. 2016 | TICv8 |
| — | — | — | — | — | M3.5 V | 4.68 | Henry et al. 1994 | TICv8 |
| 3293.7 | 0.37 | 0.37 | — | — | — | 4.68 | Rosenthal et al. 2021 | TICv8 |
| 3129 | 0.37 | 0.38 | — | -1.91 | M4 | 4.68 | von Braun et al. 2014 | TICv8 |
| — | — | — | 15 | — | — | 4.68 | Sanz-Forcada et al. 2010 | TICv8 |
| 3227 | 0.34 | 0.40 | — | -1.70 | M2.5V | 4.68 | Turnbull 2015 | TICv8 |