Temperature
4822 K
4711 to 4879
K0 III • 47.40 pc
Records
6
literature rows
Planets
2
system count
References
7
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: Takarada et al. 2018 • System source: TICv8
Temperature
4822 K
4711 to 4879
Mass
1.47 Msun
1.47 to 1.78
Radius
11.10 Rsun
11.10 to 13.09
Age
2.82 Gyr
single adopted value
Luminosity
1.85 log(Lsun)
1.85 to 1.90
Distance
47.40 pc
single adopted value
Spectral Type
K0 III
Multiple classifications reported
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 11.10 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
gam Lib
11.10 R☉
System Layout
2 planets linked to this host
gam Lib is a star located 155 light-years away with two planets orbiting it. The host is a K0 III star, a classification indicating a cooler temperature class than the Sun, and its spectral type places it among the giant stars. It has an age of 2.82 billion years, a mass of 1.47 solar masses, a radius of 11.1 solar radii, and a temperature of 4820 K. Its reported mass estimate is larger than the Sun's, its reported radius estimate is larger than the Sun's, and its reported temperature is cooler than the Sun's.
The two planets are gam Lib b and gam Lib c, both discovered in 2018 by the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion. gam Lib b has a minimum mass of 358 Earth masses and an orbital period of 415 days. Its minimum mass is larger than Earth's and roughly 1.13 times Jupiter's mass. Among the listed planets, gam Lib b has the shortest year by reported estimates.
gam Lib c has a minimum mass of 1660 Earth masses and an orbital period of 966 days. Its minimum mass is larger than Earth's and roughly 5.23 times Jupiter's mass. Among the listed planets, gam Lib c has the longest year by reported estimates and the largest minimum mass.
A minimum mass is a lower bound on a planet's true mass, distinct from an ordinary mass estimate. The radial velocity method reveals a planet and its orbital period through repeated wobbles in the star's motion.
Provenance
Evidence Summary
Rows
6
Stellar refs
6
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 4778.5 | — | 12.01 | — | — | — | 47.40 | TICv8 | TICv8 |
| — | — | — | — | — | K0 | 47.40 | Cannon & Pickering 1918 | TICv8 |
| 4822 | 1.47 | 11.10 | 2.82 | 1.85 | K0 III | 47.40 | Takarada et al. 2018 | TICv8 |
| 4879 | 1.78 | 12.38 | — | 1.90 | K0 III | 47.40 | Teng et al. 2023 | TICv8 |
| — | — | — | — | — | K0 III | 47.40 | Michigan Catalog, Vol. 4 | TICv8 |
| 4711 | — | 13.09 | — | 1.88 | — | 47.40 | Gaia DR2 | TICv8 |