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Stellar HostProfile

Kepler-430

Unclassified star • 917.5 pc

Records

20

literature rows

Planets

2

system count

References

16

distinct source labels

TIC: TIC 26748113

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

5917 K

5809 to 6242

18 values • 9 distinct

Mass

1.08 Msun

0.96 to 1.21

14 values • 8 distinct

Radius

1.21 Rsun

1.04 to 1.53

18 values • 11 distinct

Age

5.13 Gyr

2.84 to 5.13

3 values • 3 distinct

Distance

917.5 pc

single adopted value

20 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.21 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

Kepler-430

1.21 R☉

System Layout

Known planets

2 planets linked to this host

◌

Discovery

2015

Period

35.97 days

Radius

3.25 R⊕

Mass

—

Eq. Temp

667 K

◌

Discovery

2015

Period

111.0 days

Radius

1.75 R⊕

Mass

—

Eq. Temp

458 K

Kepler-430 and Its Two Known Planets

Kepler-430 is a star located 2990 light-years away. The star is estimated to be 5.13 billion years old, with a mass of 1.08 solar masses, a radius of 1.21 solar radii, and a temperature of 5920 K. Its mass and radius are larger than the Sun's, and its temperature is hotter than the Sun's.

Two planets are known to orbit Kepler-430. Both were discovered in 2015 by the transit method, in which a planet passing in front of its star from our viewpoint causes a small dip in observed brightness. Kepler-430 b is Neptune-like, with a radius of 3.25 Earth radii and an orbital period of 36 days. Kepler-430 c is a Super-Earth with a radius of 1.75 Earth radii and an orbital period of 111 days. Both planets are larger in radius than Earth.

Among the listed planets, Kepler-430 b has the shortest year and the largest radius, while Kepler-430 c has the longest year and the smallest radius.

Provenance

Underlying measurements and references

Evidence Summary

Rows

20

Stellar refs

15

System refs

1

Distancestable

20 values • 1 distinct

Parallaxstable

20 values • 1 distinct

Temperaturedisputed

18 values • 9 distinct

Massdisputed

14 values • 8 distinct

Radiusdisputed

18 values • 11 distinct

Agedisputed

3 values • 3 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

15 values • 7 distinct

Metallicitydisputed

13 values • 5 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
5967—1.04———917.5Q1-Q6 KOI TableTICv8
——————917.5Q1-Q17 DR25 Supplemental KOI TableTICv8
58311.031.24———917.5Q1-Q16 KOI TableTICv8
5936—1.37———917.5Berger et al. 2018TICv8
62421.101.162.84——917.5Q1-Q8 KOI TableTICv8
59670.961.04———917.5Batalha et al. 2013TICv8
58311.031.24———917.5Q1-Q17 DR24 KOI TableTICv8
58311.031.24———917.5Q1-Q16 KOI TableTICv8
5809—1.38—0.29—917.5Gaia DR2TICv8
58311.031.24———917.5Q1-Q12 KOI TableTICv8
58311.031.24———917.5Q1-Q17 DR24 KOI TableTICv8
5959.81.091.34—0.31—917.5TICv8TICv8
58831.211.53———917.5Q1-Q17 DR25 KOI TableTICv8
58841.171.49———917.5Everett et al. 2015TICv8
58311.031.24———917.5Q1-Q12 KOI TableTICv8
58831.211.53———917.5Q1-Q17 DR25 KOI TableTICv8
5967—1.17———917.5Latham et al. 2005TICv8
59171.081.215.13——917.5Morton et al. 2016TICv8
——————917.5Q1-Q17 DR25 Supplemental KOI TableTICv8
59361.151.344.68——917.5Fulton & Petigura 2018TICv8