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Stellar HostProfile

Kepler-233

Unclassified star • 856.4 pc

Records

20

literature rows

Planets

2

system count

References

15

distinct source labels

TIC: TIC 27843776

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

5261 K

5054 to 5360

18 values • 7 distinct

Mass

0.84 Msun

0.84 to 0.88

12 values • 4 distinct

Radius

0.80 Rsun

0.44 to 0.89

18 values • 9 distinct

Age

4.68 Gyr

0.60 to 4.68

3 values • 2 distinct

Distance

856.4 pc

single adopted value

20 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.80 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

Kepler-233

0.80 R☉

System Layout

Known planets

2 planets linked to this host

◌

Discovery

2014

Period

8.47 days

Radius

2.43 R⊕

Mass

—

Eq. Temp

—

◌

Discovery

2014

Period

60.42 days

Radius

2.71 R⊕

Mass

—

Eq. Temp

—

Kepler-233: A Cool Star With Two Known Planets

Kepler-233 is a star located 2790 light-years away, with two planets reported to orbit it. The star is estimated to be 4.68 billion years old, with a mass of 0.84 solar masses, a radius of 0.8 solar radii, and a temperature of 5260 K. Its reported mass and radius estimates are smaller than the Sun's, and its reported temperature is cooler than the Sun's.

Both planets were discovered by transit in 2014. 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. Kepler-233 b is a Super-Earth with an orbital period of 8.47 days and a radius of 2.43 Earth radii, larger than Earth's. Kepler-233 c is Neptune-like, with an orbital period of 60.4 days and a radius of 2.71 Earth radii, also larger than Earth's. Among the listed planets, Kepler-233 b has the shortest orbital period and the smallest radius by reported estimates, while Kepler-233 c has the longest orbital period and the largest radius by reported estimates.

Provenance

Underlying measurements and references

Evidence Summary

Rows

20

Stellar refs

14

System refs

1

Distancestable

20 values • 1 distinct

Parallaxstable

20 values • 1 distinct

Temperaturedisputed

18 values • 7 distinct

Massdisputed

12 values • 4 distinct

Radiusdisputed

18 values • 9 distinct

Agedisputed

3 values • 2 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

16 values • 7 distinct

Metallicitydisputed

10 values • 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
5360—0.76———856.4Rowe et al. 2014TICv8
5176—0.72———856.4Batalha et al. 2013TICv8
——————856.4Q1-Q17 DR25 Supplemental KOI TableTICv8
53540.880.79———856.4Q1-Q16 KOI TableTICv8
5176—0.44———856.4Latham et al. 2005TICv8
53540.880.79———856.4Q1-Q12 KOI TableTICv8
5360—0.83———856.4Berger et al. 2018TICv8
5176—0.72———856.4Q1-Q6 KOI TableTICv8
53540.880.79———856.4Q1-Q16 KOI TableTICv8
53540.880.79———856.4Q1-Q17 DR25 KOI TableTICv8
53310.850.750.60——856.4Q1-Q8 KOI TableTICv8
53540.880.79———856.4Q1-Q12 KOI TableTICv8
53540.880.79———856.4Q1-Q17 DR24 KOI TableTICv8
——————856.4Q1-Q17 DR25 Supplemental KOI TableTICv8
53540.880.79———856.4Q1-Q17 DR24 KOI TableTICv8
5054—0.89—-0.33—856.4Gaia DR2TICv8
53310.850.750.60——856.4Q1-Q8 KOI TableTICv8
52610.840.804.68——856.4Morton et al. 2016TICv8
51750.880.85—-0.33—856.4TICv8TICv8
53540.880.79———856.4Q1-Q17 DR25 KOI TableTICv8