Temperature
4920 K
4899 to 5044
Unclassified star • 475.8 pc
Records
12
literature rows
Planets
1
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: Ikwut-Ukwa et al. 2020 • System source: TICv8
Temperature
4920 K
4899 to 5044
Mass
0.86 Msun
0.81 to 0.89
Radius
0.82 Rsun
0.82 to 0.90
Age
7.20 Gyr
7.20 to 9.90
Luminosity
-0.44 log(Lsun)
-0.44 to -0.39
Distance
475.8 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 0.82 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
K2-114
0.82 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2017
Period
11.39 days
Radius
10.59 R⊕
Mass
638.8 M⊕
Eq. Temp
701.4 K
K2-114 is a star located 1550 light-years from Earth. It has one known planet. The host star is 7.2 billion years old and contains 0.86 solar masses. Its radius is 0.824 solar radii, and its temperature is 4920 K. The star's reported mass estimate is smaller than the Sun's, its reported radius estimate is smaller than the Sun's, and its reported temperature is cooler than the Sun's.
The planet K2-114 b is a Jupiter-like world discovered by the transit method in 2017, when it passed in front of its star from our viewpoint, causing a small dip in observed brightness. It completes an orbit every 11.4 days. Its radius is 10.6 Earth radii, which exceeds 4 times Earth's radius and places it in the Jupiter-like class, and its reported radius estimate is larger than Earth's. Its mass is 639 Earth masses, a figure larger than Earth's and roughly 2.01 times Jupiter's mass. Its mean density is 2.96 g/cm³, 0.538 times Earth's.
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 |
|---|---|---|---|---|---|---|---|---|
| 4913 | 0.81 | 0.88 | — | -0.39 | — | 475.8 | TICv8 | TICv8 |
| — | — | 0.90 | — | — | — | 475.8 | Petigura et al. 2018 | TICv8 |
| 5027 | 0.83 | 0.83 | 9.90 | — | — | 475.8 | Shporer et al. 2017 | TICv8 |
| 4899 | 0.86 | 0.83 | 7.60 | -0.44 | — | 475.8 | Thygesen et al. 2023 | TICv8 |
| — | — | — | — | — | — | 475.8 | Pope et al. 2016 | TICv8 |
| 5044 | 0.89 | 0.84 | — | — | — | 475.8 | Livingston et al. 2018 | TICv8 |
| 5027 | — | 0.88 | — | — | — | 475.8 | ExoFOP | TICv8 |
| — | — | — | — | — | — | 475.8 | Barros et al. 2016 | TICv8 |
| 5039 | 0.89 | 0.87 | — | — | — | 475.8 | Castro-González et al. 2022 | TICv8 |
| 4920 | 0.86 | 0.82 | 7.20 | -0.44 | — | 475.8 | Ikwut-Ukwa et al. 2020 | TICv8 |
| — | — | 0.85 | — | — | — | 475.8 | Kruse et al. 2019 | TICv8 |
| 4907 | — | 0.85 | — | -0.42 | — | 475.8 | Gaia DR2 | TICv8 |