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Stellar HostProfile

Kepler-407

G • 338.4 pc

Records

16

literature rows

Planets

2

system count

References

17

distinct source labels

TIC: TIC 405688133

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: Brinkman et al. 2025 • System source: TICv8

Temperature

5487 K

5398.5 to 5627

14 values • 8 distinct

Mass

0.99 Msun

0.96 to 1.07

10 values • 7 distinct

Radius

1.04 Rsun

1.00 to 1.30

14 values • 11 distinct

Luminosity

-0.11 log(Lsun)

-0.11 to -0.04

3 values • 3 distinct

Distance

338.4 pc

single adopted value

16 values • 1 distinct

Spectral Type

G

Consistent across records

G (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.04 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

Kepler-407

1.04 R☉

System Layout

Known planets

2 planets linked to this host

◌

Discovery

2014

Period

0.67 days

Radius

1.19 R⊕

Mass

1.93 M⊕

Eq. Temp

—

Kepler-407 c

Radial Velocity

◌

Discovery

2014

Period

3000 days

Radius

—

Mass

4000 M⊕

Eq. Temp

—

Kepler-407 and Its Two Known Worlds

Kepler-407 is a G-type star located 1100 light-years away. Its mass is 0.99 solar masses, its radius is 1.04 solar radii, and its temperature is 5490 K. Its reported temperature is cooler than the Sun's. Two planets are known to orbit this host.

Kepler-407 b was discovered by the transit method in 2014. Its radius is 1.19 Earth radii and its mass is 1.93 Earth masses, both larger than Earth's. With a mean density of 6.31 g/cm³, 1.15 times Earth's, it is classified as Earth-like. Its orbital period is 0.669 days, the shortest year among the listed planets; its mass is also the smallest among them.

Kepler-407 c, discovered in 2014 by the radial velocity method, has a mass of 4000 Earth masses, roughly 12.6 times Jupiter's mass and larger than Earth's. Among the listed planets it has both the largest reported mass and the longest year, with an orbital period of 3000 days.

Provenance

Underlying measurements and references

Evidence Summary

Rows

16

Stellar refs

16

System refs

1

Distancestable

16 values • 1 distinct

Parallaxstable

16 values • 1 distinct

Temperaturedisputed

14 values • 8 distinct

Massdisputed

10 values • 7 distinct

Radiusdisputed

14 values • 11 distinct

Agedisputed

3 values • 3 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

11 values • 7 distinct

Metallicitydisputed

9 values • 6 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
55561.071.022.88——338.4Fulton & Petigura 2018TICv8
547611.017.47——338.4Marcy et al. 2014TICv8
——————338.4Q1-Q17 DR25 Supplemental KOI TableTICv8
56261.051.07———338.4Q1-Q16 KOI TableTICv8
54870.961.06—-0.04—338.4TICv8TICv8
54750.981.00———338.4Q1-Q17 DR25 KOI TableTICv8
5627—1.07———338.4Q1-Q6 KOI TableTICv8
5556—1.03———338.4Berger et al. 2018TICv8
5627—1.07———338.4Batalha et al. 2013TICv8
5469—1.30———338.4Latham et al. 2005TICv8
5398.5—1.08—-0.05—338.4Gaia DR2TICv8
56261.051.07———338.4Q1-Q12 KOI TableTICv8
54870.991.04—-0.11G338.4Brinkman et al. 2025TICv8
—1.07————338.4Weiss et al. 2024TICv8
54761.011.004.60——338.4Q1-Q8 KOI TableTICv8
56261.051.07———338.4Q1-Q17 DR24 KOI TableTICv8