Temperature
4684 K
4581 to 4897
K3 • 336.2 pc
Records
5
literature rows
Planets
2
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: Herath et al. 2019 • System source: TICv8
Temperature
4684 K
4581 to 4897
Mass
0.69 Msun
0.69 to 0.72
Radius
0.67 Rsun
0.55 to 0.67
Distance
336.2 pc
single adopted value
Spectral Type
K3
Consistent across records
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 0.67 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
EPIC 212737443
0.67 R☉
System Layout
2 planets linked to this host
Transit
Discovery
2019
Period
13.60 days
Radius
2.59 R⊕
Mass
—
Eq. Temp
536 K
Transit
Discovery
2019
Period
65.55 days
Radius
2.69 R⊕
Mass
—
Eq. Temp
316 K
EPIC 212737443 is a K3 star located 1,100 light-years away. Its mass is 0.69 solar masses and its radius is 0.673 solar radii, both smaller than the Sun's, and its temperature of 4,680 K is cooler than the Sun's. Two planets orbit this host.
Both planets are Neptune-like and were discovered by transit in 2019. EPIC 212737443 b orbits every 13.6 days and has a radius of 2.59 Earth radii. EPIC 212737443 c orbits every 65.6 days and has a radius of 2.69 Earth radii. Both are larger than Earth. Among the listed planets, EPIC 212737443 b has the shortest year and the smallest radius, while EPIC 212737443 c has the longest year and the largest 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 |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | 336.2 | Pope et al. 2016 | TICv8 |
| 4684 | 0.69 | 0.67 | — | — | K3 | 336.2 | Herath et al. 2019 | TICv8 |
| 4897 | — | 0.55 | — | -0.80 | — | 336.2 | Gaia DR2 | TICv8 |
| 4581 | 0.72 | 0.67 | — | -0.75 | — | 336.2 | TICv8 | TICv8 |
| — | — | — | — | — | — | 336.2 | Barros et al. 2016 | TICv8 |