Temperature
3960 K
3789 to 3970.4
Unclassified star โข 364.0 pc
Records
8
literature rows
Planets
1
system count
References
9
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: TICv8 โข System source: TICv8
Temperature
3960 K
3789 to 3970.4
Mass
0.63 Msun
0.43 to 0.63
Radius
0.65 Rsun
0.39 to 0.71
Luminosity
-1.03 log(Lsun)
-1.03 to -0.97
Distance
364.0 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 0.65 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
K2-14
0.65 Rโ
System Layout
1 planets linked to this host
Transit
Discovery
2015
Period
8.37 days
Radius
4.81 Rโ
Mass
โ
Eq. Temp
488 K
K2-14 is an M0-type star located 1190 light-years away, with a mass of 0.626 solar masses and a radius of 0.648 solar radii. Its temperature is 3960 K, cooler than the Sun's. The star's reported mass and radius estimates are both smaller than the Sun's.
One planet orbits this host: K2-14 b, a Jupiter-like world discovered by transit in 2015. It completes an orbit in 8.37 days. Its radius is 4.81 Earth radii, larger than Earth's. Jupiter-like planets exceed 4 times Earth's radius.
Provenance
Evidence Summary
Rows
8
Stellar refs
8
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| โ | โ | โ | โ | โ | M0 | 364.0 | Luo et al. 2018 | TICv8 |
| 3866 | 0.43 | 0.39 | โ | โ | โ | 364.0 | Crossfield et al. 2016 | TICv8 |
| 3789 | 0.47 | 0.45 | โ | โ | โ | 364.0 | Montet et al. 2015 | TICv8 |
| 3879 | โ | 0.56 | โ | โ | โ | 364.0 | Vanderburg et al. 2016 | TICv8 |
| 3929 | โ | 0.71 | โ | -0.97 | โ | 364.0 | Gaia DR2 | TICv8 |
| 3960 | 0.63 | 0.65 | โ | -1.03 | โ | 364.0 | TICv8 | TICv8 |
| โ | โ | 0.71 | โ | โ | โ | 364.0 | Kruse et al. 2019 | TICv8 |
| 3970.4 | 0.62 | 0.62 | โ | โ | โ | 364.0 | Dressing et al. 2017 | TICv8 |