←Back to Stellar Hosts
Stellar HostProfile

Kepler-203

Unclassified star • 703.3 pc

Records

30

literature rows

Planets

3

system count

References

17

distinct source labels

TIC: TIC 169084431

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

5794 K

5676 to 5949

26 values • 8 distinct

Mass

1 Msun

0.97 to 1.06

20 values • 6 distinct

Radius

1.03 Rsun

0.88 to 1.11

27 values • 11 distinct

Age

5.50 Gyr

0.50 to 5.50

5 values • 3 distinct

Distance

703.3 pc

single adopted value

30 values • 1 distinct

Planets

3

Stable across source rows

3

Scale Comparison

Radius against the Sun

Current adopted radius: 1.03 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

Kepler-203

1.03 R☉

System Layout

Known planets

3 planets linked to this host

◌

Discovery

2014

Period

3.16 days

Radius

2.57 R⊕

Mass

—

Eq. Temp

—

◌

Discovery

2014

Period

5.37 days

Radius

2.47 R⊕

Mass

—

Eq. Temp

—

◌

Discovery

2014

Period

11.33 days

Radius

1.44 R⊕

Mass

—

Eq. Temp

—

Kepler-203 and Its Three Planets

Kepler-203 is a star located 2290 light-years away. It is 5.5 billion years old, has 1 solar masses, 1.03 solar radii, and a temperature of 5790 K. Three planets are known to orbit this host.

All three planets were discovered by transit in 2014. Kepler-203 b is Neptune-like, with a radius of 2.57 Earth radii and an orbital period of 3.16 days. Among the listed planets, it has the shortest year and the largest radius. Kepler-203 c is a Super-Earth with a radius of 2.47 Earth radii and an orbital period of 5.37 days, the second-shortest year and second-smallest radius among the listed planets. Kepler-203 d is Earth-like, with a radius of 1.44 Earth radii and an orbital period of 11.3 days, the longest year and smallest radius among the listed planets. Each planet's reported radius estimate is larger than Earth's. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness; repeated dips help establish orbital periods.

Provenance

Underlying measurements and references

Evidence Summary

Rows

30

Stellar refs

16

System refs

1

Distancestable

30 values • 1 distinct

Parallaxstable

30 values • 1 distinct

Temperaturedisputed

26 values • 8 distinct

Massdisputed

20 values • 6 distinct

Radiusdisputed

27 values • 11 distinct

Agedisputed

5 values • 3 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

23 values • 8 distinct

Metallicitydisputed

16 values • 6 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—1.010.94———703.3Hadden et al. 2014TICv8
58210.971.08———703.3Q1-Q17 DR25 KOI TableTICv8
58210.971.08———703.3Q1-Q17 DR25 KOI TableTICv8
5676—0.88———703.3Q1-Q6 KOI TableTICv8
59491.010.94———703.3Q1-Q17 DR24 KOI TableTICv8
5821—1.11———703.3Rowe et al. 2014TICv8
58871.061.031.78——703.3Fulton & Petigura 2018TICv8
5676—0.88———703.3Q1-Q6 KOI TableTICv8
——————703.3Q1-Q17 DR25 Supplemental KOI TableTICv8
5676—0.88———703.3Q1-Q6 KOI TableTICv8
59491.010.94———703.3Q1-Q17 DR24 KOI TableTICv8
59491.010.94———703.3Q1-Q12 KOI TableTICv8
59491.010.94———703.3Q1-Q16 KOI TableTICv8
——————703.3Q1-Q17 DR25 Supplemental KOI TableTICv8
59491.010.94———703.3Q1-Q12 KOI TableTICv8
5676—0.93———703.3Latham et al. 2005TICv8
58210.971.08———703.3Q1-Q17 DR25 KOI TableTICv8
59491.010.94———703.3Q1-Q12 KOI TableTICv8
5871.21.061.08—0.09—703.3TICv8TICv8
59241.010.910.50——703.3Q1-Q8 KOI TableTICv8
579411.035.50——703.3Morton et al. 2016TICv8
59241.010.910.50——703.3Q1-Q8 KOI TableTICv8
59241.010.910.50——703.3Q1-Q8 KOI TableTICv8
56760.980.88———703.3Batalha et al. 2013TICv8
59491.010.94———703.3Q1-Q16 KOI TableTICv8
5676.2—1.05—9.92e-3—703.3Gaia DR2TICv8
——————703.3Q1-Q17 DR25 Supplemental KOI TableTICv8
59491.010.94———703.3Q1-Q17 DR24 KOI TableTICv8
5887—1.04———703.3Berger et al. 2018TICv8
59491.010.94———703.3Q1-Q16 KOI TableTICv8