Temperature
5363 K
5194.6 to 5552
Unclassified star • 758.5 pc
Records
19
literature rows
Planets
2
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
5363 K
5194.6 to 5552
Mass
0.88 Msun
0.84 to 0.95
Radius
0.84 Rsun
0.80 to 0.90
Age
4.37 Gyr
1.29 to 4.40
Distance
758.5 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 0.84 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-725
0.84 R☉
System Layout
2 planets linked to this host
Transit
Discovery
2016
Period
39.64 days
Radius
10.80 R⊕
Mass
—
Eq. Temp
514 K
Transit Timing Variations
Discovery
2025
Period
207.5 days
Radius
—
Mass
9.70 M⊕
Eq. Temp
268 K
Kepler-725 is a G-type star located 2470 light-years away, with two planets known to orbit it. The star is 4.37 billion years old and has a mass of 0.88 solar masses, a radius of 0.84 solar radii, and a temperature of 5360 K. Its reported mass and radius estimates are smaller than the Sun's, and its reported temperature is cooler than the Sun's.
Kepler-725 b is a Jupiter-like planet discovered by transit in 2016. It has an orbital period of 39.6 days and a radius of 10.8 Earth radii, which is larger than Earth's. Among the listed planets, it has the shortest year by reported estimates.
Kepler-725 c was discovered in 2025 by transit timing variations, in which a planet's passages across its star shift slightly in time. It has a mass of 9.7 Earth masses, larger than Earth's, and an orbital period of 208 days. Among the listed planets, it has the longest year by reported estimates.
Provenance
Evidence Summary
Rows
19
Stellar refs
15
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5552 | 0.91 | 0.83 | — | — | — | 758.5 | Q1-Q16 KOI Table | TICv8 |
| 5399 | — | 0.81 | — | — | — | 758.5 | Berger et al. 2018 | TICv8 |
| 5552 | 0.91 | 0.83 | — | — | — | 758.5 | Q1-Q12 KOI Table | TICv8 |
| 5231 | 0.84 | 0.90 | — | — | — | 758.5 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5552 | 0.91 | 0.83 | — | — | — | 758.5 | Q1-Q12 KOI Table | TICv8 |
| — | — | — | — | — | — | 758.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5552 | 0.91 | 0.83 | — | — | — | 758.5 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5526 | 0.88 | 0.83 | 4.40 | — | — | 758.5 | Q1-Q8 KOI Table | TICv8 |
| 5321 | — | 0.85 | — | — | — | 758.5 | Batalha et al. 2013 | TICv8 |
| 5363 | 0.88 | 0.84 | 4.37 | — | — | 758.5 | Morton et al. 2016 | TICv8 |
| 5194.6 | — | 0.85 | — | -0.32 | — | 758.5 | Gaia DR2 | TICv8 |
| 5552 | 0.91 | 0.83 | — | — | — | 758.5 | Q1-Q16 KOI Table | TICv8 |
| 5399 | 0.91 | 0.80 | 1.29 | — | — | 758.5 | Fulton & Petigura 2018 | TICv8 |
| 5321 | — | 0.85 | — | — | — | 758.5 | Q1-Q6 KOI Table | TICv8 |
| 5395 | 0.95 | 0.88 | 1.60 | — | — | 758.5 | Sun et al. 2025 | TICv8 |
| 5526 | 0.88 | 0.83 | 4.40 | — | — | 758.5 | Q1-Q8 KOI Table | TICv8 |
| — | — | — | — | — | — | 758.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5321 | — | 0.88 | — | — | — | 758.5 | Latham et al. 2005 | TICv8 |
| 5293 | 0.91 | 0.83 | — | -0.31 | — | 758.5 | TICv8 | TICv8 |