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Stellar HostProfile

Kepler-725

Unclassified star • 758.5 pc

Records

19

literature rows

Planets

2

system count

References

16

distinct source labels

TIC: TIC 164652841

Approximate color

from effective temperature

Canonical Summary

Adopted host values from one source row

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

17 values • 9 distinct

Mass

0.88 Msun

0.84 to 0.95

12 values • 7 distinct

Radius

0.84 Rsun

0.80 to 0.90

17 values • 11 distinct

Age

4.37 Gyr

1.29 to 4.40

5 values • 4 distinct

Distance

758.5 pc

single adopted value

19 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.84 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

Kepler-725

0.84 R☉

System Layout

Known planets

2 planets linked to this host

◌

Discovery

2016

Period

39.64 days

Radius

10.80 R⊕

Mass

—

Eq. Temp

514 K

Kepler-725 c

Transit Timing Variations

◌

Discovery

2025

Period

207.5 days

Radius

—

Mass

9.70 M⊕

Eq. Temp

268 K

Kepler-725 and Its Two Planets

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

Underlying measurements and references

Evidence Summary

Rows

19

Stellar refs

15

System refs

1

Distancestable

19 values • 1 distinct

Parallaxstable

19 values • 1 distinct

Temperaturedisputed

17 values • 9 distinct

Massdisputed

12 values • 7 distinct

Radiusdisputed

17 values • 11 distinct

Agedisputed

5 values • 4 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

13 values • 5 distinct

Metallicitydisputed

9 values • 4 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
55520.910.83———758.5Q1-Q16 KOI TableTICv8
5399—0.81———758.5Berger et al. 2018TICv8
55520.910.83———758.5Q1-Q12 KOI TableTICv8
52310.840.90———758.5Q1-Q17 DR25 KOI TableTICv8
55520.910.83———758.5Q1-Q12 KOI TableTICv8
——————758.5Q1-Q17 DR25 Supplemental KOI TableTICv8
55520.910.83———758.5Q1-Q17 DR24 KOI TableTICv8
55260.880.834.40——758.5Q1-Q8 KOI TableTICv8
5321—0.85———758.5Batalha et al. 2013TICv8
53630.880.844.37——758.5Morton et al. 2016TICv8
5194.6—0.85—-0.32—758.5Gaia DR2TICv8
55520.910.83———758.5Q1-Q16 KOI TableTICv8
53990.910.801.29——758.5Fulton & Petigura 2018TICv8
5321—0.85———758.5Q1-Q6 KOI TableTICv8
53950.950.881.60——758.5Sun et al. 2025TICv8
55260.880.834.40——758.5Q1-Q8 KOI TableTICv8
——————758.5Q1-Q17 DR25 Supplemental KOI TableTICv8
5321—0.88———758.5Latham et al. 2005TICv8
52930.910.83—-0.31—758.5TICv8TICv8