Temperature
3024 K
2902 to 3024
M5.5 V • 4.85 pc
Records
3
literature rows
Planets
2
system count
References
4
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: Suárez Mascareño et al. 2023 • System source: TICv8
Temperature
3024 K
2902 to 3024
Mass
0.12 Msun
0.12 to 0.12
Radius
0.14 Rsun
0.14 to 0.14
Luminosity
-2.85 log(Lsun)
-2.88 to -2.85
Distance
4.85 pc
single adopted value
Spectral Type
M5.5 V
Multiple classifications reported
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 0.14 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
GJ 1002
0.14 R☉
System Layout
2 planets linked to this host
GJ 1002 is a nearby star just 15.8 light-years away, with a spectral type of M5.5 V that marks it as a small, cool red dwarf. Its reported mass estimate is 0.12 solar masses and its reported radius estimate is 0.137 solar radii, both smaller than the Sun's, while its temperature of 3020 K is cooler than the Sun's. Two planets are known to orbit this star, both detected in 2022 by the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion; repeated wobbles reveal the planet and its orbital period.
GJ 1002 b has a minimum mass of 1.08 Earth masses and an orbital period of 10.3 days. GJ 1002 c has a minimum mass of 1.36 Earth masses and an orbital period of 21.2 days. Both are minimum masses, meaning lower bounds on the planets' true masses rather than ordinary estimates. Among the listed planets, GJ 1002 b has the shortest year by reported estimates and the smallest minimum mass, while GJ 1002 c has the longest year by reported estimates and the largest minimum mass.
Provenance
Evidence Summary
Rows
3
Stellar refs
3
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | M5.5 | 4.85 | Hawley et al. 1996 | TICv8 |
| 2902 | 0.12 | 0.14 | — | -2.88 | — | 4.85 | TICv8 | TICv8 |
| 3024 | 0.12 | 0.14 | — | -2.85 | M5.5 V | 4.85 | Suárez Mascareño et al. 2023 | TICv8 |