Temperature
5612 K
5423.7 to 5761
Unclassified star • 233.5 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: Howard et al. 2025 • System source: TICv8
Temperature
5612 K
5423.7 to 5761
Mass
0.91 Msun
0.91 to 1.03
Radius
1.03 Rsun
0.93 to 1.06
Distance
233.5 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 1.03 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
K2-220
1.03 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2018
Period
13.68 days
Radius
2.37 R⊕
Mass
—
Eq. Temp
761 K
K2-220 is a star 762 light-years away with 0.91 solar masses, 1.03 solar radii, and a temperature of 5610 K. Its reported mass estimate is smaller than the Sun's, and its reported temperature is cooler than the Sun's. One planet orbits this host.
That planet is K2-220 b, a Super-Earth 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 orbital periods. K2-220 b completes an orbit every 13.7 days and has a radius of 2.37 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 |
|---|---|---|---|---|---|---|---|---|
| 5423.7 | — | 1.06 | — | -0.06 | — | 233.5 | Gaia DR2 | TICv8 |
| 5761 | 1.03 | 1.00 | — | -4.22e-3 | — | 233.5 | TICv8 | TICv8 |
| 5599 | 0.96 | 0.93 | — | — | — | 233.5 | Mayo et al. 2018 | TICv8 |
| — | — | 1.06 | — | — | — | 233.5 | Kruse et al. 2019 | TICv8 |
| 5660 | 0.96 | 1.02 | — | — | — | 233.5 | Livingston et al. 2018 | TICv8 |
| 5612 | 0.91 | 1.03 | — | — | — | 233.5 | Howard et al. 2025 | TICv8 |
| — | — | 0.99 | — | — | — | 233.5 | Petigura et al. 2018 | TICv8 |