Temperature
3291 K
3267 to 3588.5
M3.5 V • 8.07 pc
Records
10
literature rows
Planets
1
system count
References
11
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: Caballero et al. 2022 • System source: TICv8
Temperature
3291 K
3267 to 3588.5
Mass
0.33 Msun
0.31 to 0.34
Radius
0.34 Rsun
0.32 to 0.37
Age
4 Gyr
single adopted value
Luminosity
-1.92 log(Lsun)
-2 to -1.92
Distance
8.07 pc
single adopted value
Spectral Type
M3.5 V
Multiple classifications reported
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 0.34 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
GJ 486
0.34 R☉
System Layout
1 planets linked to this host
Radial Velocity
Discovery
2021
Period
1.47 days
Radius
1.29 R⊕
Mass
2.77 M⊕
Eq. Temp
696.3 K
GJ 486 is an M3.5 V star, a small, cool red dwarf, located 26.3 light-years from Earth. It has one known planet. Its spectral type places it in the M class, the coolest and reddest of the main-sequence temperature classes. The star's mass is 0.333 solar masses, its radius is 0.339 solar radii, and its temperature is 3290 K. Its age is 4 billion years. Each of these stellar measurements applies to the host star itself, and the reported mass, radius, and temperature estimates all fall below the corresponding values for the Sun.
The single planet, GJ 486 b, was discovered in 2021 by the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion; repeated wobbles reveal the planet and its orbital period. GJ 486 b orbits its host in 1.47 days, and its mean density is 7.13 g/cm³, 1.29 times Earth's. The planet's radius is 1.29 Earth radii, larger than Earth's, which keeps it within the Earth-like size class of 1.5 times Earth's radius. Its mass is 2.77 Earth masses, also larger than Earth's.
Provenance
Evidence Summary
Rows
10
Stellar refs
10
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 3297 | 0.31 | 0.33 | — | -1.93 | — | 8.07 | TICv8 | TICv8 |
| — | — | — | — | — | M3.5 | 8.07 | Hawley et al. 1996 | TICv8 |
| — | — | — | — | — | — | 8.07 | Nidever et al. 2002 | TICv8 |
| — | — | — | — | — | — | 8.07 | Wright et al. 2004 | TICv8 |
| 3297 | — | 0.33 | — | — | — | 8.07 | ExoFOP | TICv8 |
| 3291 | 0.33 | 0.34 | 4 | -1.92 | M3.5 V | 8.07 | Caballero et al. 2022 | TICv8 |
| 3267 | 0.34 | 0.37 | — | -2 | M4 | 8.07 | Turnbull 2015 | TICv8 |
| 3588.5 | — | — | — | — | — | 8.07 | Gaia DR2 | TICv8 |
| 3340 | 0.32 | 0.33 | — | -1.92 | M3.5 V | 8.07 | Trifonov et al. 2021 | TICv8 |
| 3317 | 0.31 | 0.32 | — | -1.94 | — | 8.07 | Weiner Mansfield et al. 2024 | TICv8 |