Temperature
4916 K
4772.4 to 4953
Unclassified star • 109.7 pc
Records
12
literature rows
Planets
2
system count
References
13
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: Damasso et al. 2019 • System source: TICv8
Temperature
4916 K
4772.4 to 4953
Mass
0.79 Msun
0.76 to 0.81
Radius
0.72 Rsun
0.72 to 0.75
Age
1.40 Gyr
single adopted value
Luminosity
-0.57 log(Lsun)
-0.59 to -0.57
Distance
109.7 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 0.72 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
K2-36
0.72 R☉
System Layout
2 planets linked to this host
K2-36 is a K-type main-sequence dwarf 358 light-years away. A spectral type of K2 V places it in the cooler, redder part of the K class, and its measured properties are 0.79 solar masses, 0.718 solar radii, a temperature of 4920 K, and an age of 1.4 billion years. Its mass and radius are each smaller than the Sun's, and its temperature is cooler. Two planets are known to orbit this host.
Both planets were found by the transit method, in which a planet passes in front of its star from our viewpoint and produces a small dip in observed brightness; repeated dips help establish orbital periods. K2-36 b, discovered in 2016, is an Earth-like planet with a radius of 1.43 Earth radii, a mass of 4.3 Earth masses, and an orbital period of 1.42 days. Its radius and mass are both larger than Earth's, and its mean density is 8.1 g/cm³, 1.47 times Earth's. Among the listed planets, K2-36 b has the shortest year and the smallest radius and mass.
K2-36 c, also discovered in 2016 by transit, is Neptune-like. It has a radius of 3.2 Earth radii, a mass of 7.9 Earth masses, and an orbital period of 5.34 days. Its radius and mass are larger than Earth's, and its mean density is 1.33 g/cm³, 0.241 times Earth's. Among the listed planets, K2-36 c has the longest year and the largest radius and mass.
Provenance
Evidence Summary
Rows
12
Stellar refs
12
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | 0.73 | — | — | — | 109.7 | Kruse et al. 2019 | TICv8 |
| 4808.2 | — | 0.73 | — | -0.59 | — | 109.7 | Gaia DR2 | TICv8 |
| 4836 | 0.76 | 0.72 | — | — | — | 109.7 | Howard et al. 2025 | TICv8 |
| 4953 | 0.81 | 0.73 | — | — | — | 109.7 | Duck et al. 2021 | TICv8 |
| 4772.4 | 0.77 | 0.75 | — | -0.58 | — | 109.7 | TICv8 | TICv8 |
| 4916 | 0.79 | 0.72 | 1.40 | -0.57 | — | 109.7 | Damasso et al. 2019 | TICv8 |
| 4886 | — | 0.74 | — | — | — | 109.7 | Vanderburg et al. 2016 | TICv8 |
| 4924 | 0.80 | 0.74 | — | — | K2 V | 109.7 | Sinukoff et al. 2016 | TICv8 |
| 4916 | 0.79 | 0.72 | — | — | — | 109.7 | Bonomo et al. 2023 | TICv8 |
| 4953 | 0.81 | 0.75 | — | — | — | 109.7 | Crossfield et al. 2016 | TICv8 |
| 4944 | 0.80 | 0.75 | — | — | — | 109.7 | Mayo et al. 2018 | TICv8 |
| — | — | — | — | — | — | 109.7 | Barros et al. 2016 | TICv8 |