Temperature
4799 K
4711 to 5213
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Stellar HostProfile
K2-65
Unclassified star
Records
5
literature rows
Planets
1
system count
References
6
distinct source labels
HIP: HIP 109656TIC: TIC 38200266
Approximate color
from effective temperature
Canonical Summary
Adopted host values from one source row
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
Mass
0.70 Msun
0.70 to 0.87
Radius
0.67 Rsun
0.67 to 0.84
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.67 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
K2-65
0.67 R☉
System Layout
Known planets
1 planets linked to this host
K2-65 b
Transit
◌
Discovery
2016
Period
12.65 days
Radius
1.58 R⊕
Mass
—
Eq. Temp
—
K2-65 and Its Super-Earth
K2-65 is a star with one known planet. Its mass is 0.702 solar masses, its radius is 0.669 solar radii, and its temperature is 4800 K, so each of these reported estimates is smaller or cooler than the corresponding value for the Sun. The system’s planet is K2-65 b, a Super-Earth discovered by transit in 2016. A transit occurs when a planet crosses in front of its star from our viewpoint, dimming the observed brightness.
K2-65 b orbits once every 12.6 days and has a radius of 1.58 Earth radii, larger than Earth’s. Its reported size class places it within the Super-Earth range, where radius reaches 2.5 times Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
5
Stellar refs
5
System refs
1
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Surface Gravitydisputed
Metallicitystable
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | — | Barros et al. 2016 | TICv8 |
| 5213 | 0.87 | 0.84 | — | — | — | — | Crossfield et al. 2016 | TICv8 |
| 4799 | 0.70 | 0.67 | — | — | — | — | Mayo et al. 2018 | TICv8 |
| 4711 | — | 0.72 | — | — | — | — | Vanderburg et al. 2016 | TICv8 |
| — | — | 0.72 | — | — | — | — | Kruse et al. 2019 | TICv8 |