Temperature
4255 K
3682 to 4304
Unclassified star • 561.1 pc
Records
25
literature rows
Planets
2
system count
References
17
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
4255 K
3682 to 4304
Mass
0.66 Msun
0.46 to 0.66
Radius
0.63 Rsun
0.44 to 0.77
Age
2.88 Gyr
2.88 to 13.80
Distance
561.1 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 0.63 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-225
0.63 R☉
System Layout
2 planets linked to this host
Transit
Discovery
2014
Period
6.74 days
Radius
1.20 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2014
Period
18.79 days
Radius
1.84 R⊕
Mass
—
Eq. Temp
—
Kepler-225 is an M1 V star, a small, cool red dwarf, located 1830 light-years away. It hosts two known planets. The star's reported mass estimate is 0.66 solar masses and its reported radius estimate is 0.63 solar radii, both smaller than the Sun's. Its reported temperature is 4260 K, cooler than the Sun's, and its age is 2.88 billion years.
Both planets were discovered by transit in 2014. Kepler-225 b is classified as Earth-like, with a reported radius estimate of 1.2 Earth radii, larger than Earth's. It has the shortest year among the listed planets at 6.74 days. Kepler-225 c is a Super-Earth with an orbital period of 18.8 days. Its reported radius estimate is 1.84 Earth radii, also larger than Earth's, and it has the longest year among the listed planets.
Among the listed planets, Kepler-225 b has the smallest radius by reported estimates, while Kepler-225 c has the longest year by reported estimates at 18.8 days.
Provenance
Evidence Summary
Rows
25
Stellar refs
16
System refs
1