Temperature
5093 K
4994 to 5210
Unclassified star • 782.1 pc
Records
36
literature rows
Planets
4
system count
References
16
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: Morton et al. 2016 • System source: TICv8
Temperature
5093 K
4994 to 5210
Mass
0.78 Msun
0.74 to 0.84
Radius
0.71 Rsun
0.58 to 0.72
Age
2.29 Gyr
0.60 to 2.29
Distance
782.1 pc
single adopted value
Planets
4
Stable across source rows
Scale Comparison
Current adopted radius: 0.71 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-224
0.71 R☉
System Layout
4 planets linked to this host
Transit
Discovery
2014
Period
3.13 days
Radius
1.39 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2014
Period
5.93 days
Radius
3.12 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2014
Period
11.35 days
Radius
2.30 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2014
Period
18.64 days
Radius
1.97 R⊕
Mass
—
Eq. Temp
—
Kepler-224 is a star located 2550 light-years away. It is 2.29 billion years old and has a mass of 0.78 solar masses, a radius of 0.71 solar radii, and a temperature of 5090 K. Its reported mass estimate is smaller than the Sun's, its reported radius estimate is smaller than the Sun's, and its temperature is cooler than the Sun's. Four planets orbit this host: Kepler-224 b, Kepler-224 c, Kepler-224 d, and Kepler-224 e. All four were discovered by transit in 2014.
Kepler-224 b is an Earth-like planet with an orbital period of 3.13 days and a radius of 1.39 Earth radii. Its reported radius estimate is larger than Earth's. Among the listed planets, it has the shortest year and the smallest radius by reported estimates.
Kepler-224 c is a Neptune-like planet with an orbital period of 5.93 days and a radius of 3.12 Earth radii. Its reported radius estimate is larger than Earth's. Among the listed planets, it has the second-shortest year and the largest radius by reported estimates.
Kepler-224 d is a Super-Earth with an orbital period of 11.3 days and a radius of 2.3 Earth radii. Its reported radius estimate is larger than Earth's. Among the listed planets, it has the second-longest year and the second-largest radius by reported estimates.
Kepler-224 e is a Super-Earth with an orbital period of 18.6 days and a radius of 1.97 Earth radii. Its reported radius estimate is larger than Earth's. Among the listed planets, it has the longest year and the second-smallest radius by reported estimates.
Provenance
Evidence Summary
Rows
36
Stellar refs
15
System refs
1