Temperature
3734 K
3734 to 4006.0
Unclassified star • 16.03 pc
Records
9
literature rows
Planets
4
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: Stassun et al. 2017 • System source: TICv8
Temperature
3734 K
3734 to 4006.0
Mass
0.73 Msun
0.56 to 0.73
Radius
0.69 Rsun
0.63 to 0.73
Distance
16.03 pc
single adopted value
Planets
4
Stable across source rows
Scale Comparison
Current adopted radius: 0.69 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
GJ 676 A
0.69 R☉
System Layout
4 planets linked to this host
Radial Velocity
Discovery
2010
Period
1051.4 days
Radius
—
Mass
1840.9 M⊕
Eq. Temp
—
Radial Velocity
Discovery
2016
Period
1.39e4 days
Radius
—
Mass
4288.1 M⊕
Eq. Temp
—
Radial Velocity
Discovery
2012
Period
3.60 days
Radius
—
Mass
3.81 M⊕
Eq. Temp
—
Radial Velocity
Discovery
2012
Period
35.47 days
Radius
—
Mass
6.67 M⊕
Eq. Temp
—
GJ 676 A is an M0 V star, a small, cool red dwarf, located 52.3 light-years away. Its reported mass estimate is 0.73 solar masses, its radius is 0.69 solar radii, and its temperature is 3730 K. Each of these values is smaller or cooler than the corresponding value for the Sun. Four planets have been reported orbiting this star.
GJ 676 A b was discovered in 2010 by the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion. Its mass is 1840 Earth masses, roughly 5.79 times Jupiter's mass, and its orbital period is 1050 days. GJ 676 A c, also found by radial velocity, was discovered in 2016. Its mass is 4290 Earth masses, roughly 13.5 times Jupiter's mass, and its orbital period is 13900 days, the longest among these four planets.
The two remaining planets were both discovered in 2012 by radial velocity. GJ 676 A d has a minimum mass of 3.81 Earth masses and an orbital period of 3.6 days, the shortest among the listed planets. GJ 676 A e has a minimum mass of 6.67 Earth masses and an orbital period of 35.5 days. For both of these planets, the reported minimum mass is larger than Earth's, and the value represents a lower bound on the planet's true mass rather than an ordinary mass estimate.
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 |
|---|---|---|---|---|---|---|---|---|
| 3734 | 0.73 | 0.69 | — | — | — | 16.03 | Stassun et al. 2017 | TICv8 |
| 4006.0 | — | 0.63 | — | -1.04 | — | 16.03 | Gaia DR2 | TICv8 |
| — | — | — | — | — | M0 V | 16.03 | Forveille et al. 2011 | TICv8 |
| 3851 | 0.63 | 0.65 | — | -1.08 | — | 16.03 | TICv8 | TICv8 |
| — | 0.71 | — | — | — | M0 V | 16.03 | Anglada-Escude & Tuomi 2012 | TICv8 |
| — | — | — | — | — | M0.0 | 16.03 | Hawley et al. 1996 | TICv8 |
| — | 0.63 | — | — | — | — | 16.03 | Feng et al. 2022 | TICv8 |
| 3851 | 0.56 | 0.73 | — | -0.96 | M0 | 16.03 | Turnbull 2015 | TICv8 |
| — | — | — | — | — | — | 16.03 | Sahlmann et al. 2016 | TICv8 |