Temperature
5667 K
5440.2 to 5675
Unclassified star โข 247.6 pc
Records
7
literature rows
Planets
1
system count
References
8
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: Livingston et al. 2018 โข System source: TICv8
Temperature
5667 K
5440.2 to 5675
Mass
1 Msun
0.97 to 1
Radius
0.93 Rsun
0.91 to 0.98
Distance
247.6 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 0.93 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
K2-197
0.93 Rโ
System Layout
1 planets linked to this host
Transit
Discovery
2018
Period
8.36 days
Radius
2.56 Rโ
Mass
โ
Eq. Temp
848 K
K2-197 is a star 808 light-years away with a single known planet, K2-197 b. The host star has a mass of 1 solar masses, a radius of 0.93 solar radii, and a temperature of 5670 K. Its radius is smaller than the Sun's, and its temperature is cooler than the Sun's.
K2-197 b was discovered in 2018 by the transit method, in which a planet passes in front of its star from our viewpoint and causes a small dip in observed brightness. Repeated dips help establish the planet's orbital period. K2-197 b completes one orbit every 8.36 days.
K2-197 b is Neptune-like, a size class that reaches 4 times Earth's radius. Its radius is 2.56 Earth radii, larger than Earth's.
Provenance
Evidence Summary
Rows
7
Stellar refs
7
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| โ | โ | 0.96 | โ | โ | โ | 247.6 | Petigura et al. 2018 | TICv8 |
| 5440.2 | โ | 0.98 | โ | -0.12 | โ | 247.6 | Gaia DR2 | TICv8 |
| โ | โ | โ | โ | โ | โ | 247.6 | Barros et al. 2016 | TICv8 |
| 5627 | 1.00 | 0.92 | โ | -0.11 | โ | 247.6 | TICv8 | TICv8 |
| 5667 | 1 | 0.93 | โ | โ | โ | 247.6 | Livingston et al. 2018 | TICv8 |
| 5675 | 0.97 | 0.91 | โ | โ | โ | 247.6 | Mayo et al. 2018 | TICv8 |
| โ | โ | โ | โ | โ | โ | 247.6 | Pope et al. 2016 | TICv8 |