Temperature
4528 K
4356.5 to 4528
Unclassified star • 118.0 pc
Records
5
literature rows
Planets
1
system count
References
6
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: Mayo et al. 2018 • System source: TICv8
Temperature
4528 K
4356.5 to 4528
Mass
0.68 Msun
0.68 to 0.70
Radius
0.64 Rsun
0.64 to 0.74
Distance
118.0 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 0.64 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
K2-130
0.64 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2017
Period
2.49 days
Radius
1.25 R⊕
Mass
—
Eq. Temp
—
K2-130 is a star 385 light-years away with one known planet, K2-130 b. The star's reported mass estimate is 0.675 solar masses and its reported radius estimate is 0.644 solar radii, both smaller than the Sun's. Its reported temperature is 4530 K, cooler than the Sun's.
K2-130 b was discovered in 2017 by the transit method, which detects the small dip in a star's observed brightness when a planet passes in front of it from our viewpoint. Repeated dips help establish the planet's orbital period. K2-130 b completes one orbit in 2.49 days, and its radius is 1.25 Earth radii. Its reported radius estimate is larger than Earth's, placing it within the Earth-like size class, which covers planets up to 1.5 times Earth's radius.
Provenance
Evidence Summary
Rows
5
Stellar refs
5
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 4387 | 0.69 | 0.71 | — | -0.78 | — | 118.0 | TICv8 | TICv8 |
| 4356.5 | 0.70 | 0.74 | — | — | — | 118.0 | Dressing et al. 2017 | TICv8 |
| — | — | 0.66 | — | — | — | 118.0 | Kruse et al. 2019 | TICv8 |
| 4476.8 | — | 0.66 | — | -0.80 | — | 118.0 | Gaia DR2 | TICv8 |
| 4528 | 0.68 | 0.64 | — | — | — | 118.0 | Mayo et al. 2018 | TICv8 |