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Stellar HostProfile

Kepler-223

Unclassified star • 1859.7 pc

Records

38

literature rows

Planets

4

system count

References

18

distinct source labels

TIC: TIC 273876171

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

5746 K

5234.3 to 5832

32 values • 9 distinct

Mass

0.98 Msun

0.90 to 1.12

25 values • 8 distinct

Radius

0.98 Rsun

0.98 to 1.76

33 values • 11 distinct

Age

4.27 Gyr

4.27 to 8.91

6 values • 3 distinct

Distance

1859.7 pc

single adopted value

38 values • 1 distinct

Planets

4

Stable across source rows

4

Scale Comparison

Radius against the Sun

Current adopted radius: 0.98 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

Kepler-223

0.98 R☉

System Layout

Known planets

4 planets linked to this host

◌

Discovery

2014

Period

7.38 days

Radius

2.99 R⊕

Mass

7.40 M⊕

Eq. Temp

—

◌

Discovery

2014

Period

9.85 days

Radius

3.44 R⊕

Mass

5.10 M⊕

Eq. Temp

—

◌

Discovery

2014

Period

14.79 days

Radius

5.24 R⊕

Mass

8 M⊕

Eq. Temp

—

◌

Discovery

2014

Period

19.73 days

Radius

4.60 R⊕

Mass

4.80 M⊕

Eq. Temp

—

Kepler-223: A Four-Planet System

Kepler-223 is a star located 6070 light-years away. It hosts four planets, all discovered by the transit method in 2014. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. The host star is 4.27 billion years old and has a mass of 0.98 solar masses, a radius of 0.98 solar radii, and a temperature of 5750 K.

Kepler-223 b is a Neptune-like planet with a mass of 7.4 Earth masses, a radius of 2.99 Earth radii, and an orbital period of 7.38 days. Kepler-223 c is also Neptune-like, with a mass of 5.1 Earth masses, a radius of 3.44 Earth radii, and an orbital period of 9.85 days. Kepler-223 d is Jupiter-like, with a mass of 8 Earth masses, a radius of 5.24 Earth radii, and an orbital period of 14.8 days. Kepler-223 e is also Jupiter-like, with a mass of 4.8 Earth masses, a radius of 4.6 Earth radii, and an orbital period of 19.7 days. Each planet's radius estimate and mass estimate are larger than Earth's.

Among the listed planets, Kepler-223 b has the shortest year, at 7.38 days, and the smallest radius, at 2.99 Earth radii. Kepler-223 e has the longest year, at 19.7 days. Kepler-223 d has the largest radius, at 5.24 Earth radii, and the largest reported mass, at 8 Earth masses. Kepler-223 e has the smallest reported mass, at 4.8 Earth masses. Kepler-223 c has the second-shortest year, at 9.85 days, the second-smallest radius, at 3.44 Earth radii, and the second-smallest reported mass, at 5.1 Earth masses. Kepler-223 b has the second-largest reported mass, at 7.4 Earth masses, while Kepler-223 d has the second-longest year, at 14.8 days, and Kepler-223 e has the second-largest radius, at 4.6 Earth radii. The mean density of Kepler-223 b is 1.53 g/cm³, 0.277 times Earth's, the highest among these planets.

Provenance

Underlying measurements and references

Evidence Summary

Rows

38

Stellar refs

17

System refs

1

Distancestable

38 values • 1 distinct

Parallaxstable

38 values • 1 distinct

Temperaturedisputed

32 values • 9 distinct

Massdisputed

25 values • 8 distinct

Radiusdisputed

33 values • 11 distinct

Agedisputed

6 values • 3 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

29 values • 5 distinct

Metallicitydisputed

20 values • 6 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
5234.3—1.76—0.32—1859.7Gaia DR2TICv8
58031.041.52—0.37—1859.7TICv8TICv8
—1.10————1859.7Hadden & Lithwick 2017TICv8
5599—0.98———1859.7Q1-Q6 KOI TableTICv8
58250.901.00———1859.7Q1-Q16 KOI TableTICv8
58250.901.00———1859.7Q1-Q16 KOI TableTICv8
58250.901.00———1859.7Q1-Q16 KOI TableTICv8
58250.901.00———1859.7Q1-Q16 KOI TableTICv8
——————1859.7Q1-Q17 DR25 Supplemental KOI TableTICv8
—1.121.72———1859.7Mills et al. 2016TICv8
58250.901.00———1859.7Q1-Q17 DR24 KOI TableTICv8
58320.951.037.20——1859.7Q1-Q8 KOI TableTICv8
58250.901.00———1859.7Q1-Q12 KOI TableTICv8
58320.951.037.20——1859.7Q1-Q8 KOI TableTICv8
58320.951.037.20——1859.7Q1-Q8 KOI TableTICv8
58250.901.00———1859.7Q1-Q12 KOI TableTICv8
5829—1.02———1859.7Rowe et al. 2014TICv8
58250.901.00———1859.7Q1-Q12 KOI TableTICv8
5599—1.09———1859.7Latham et al. 2005TICv8
5697—1.64———1859.7Berger et al. 2018TICv8
58250.901.00———1859.7Q1-Q17 DR24 KOI TableTICv8
5599—0.98———1859.7Q1-Q6 KOI TableTICv8
5599—0.98———1859.7Batalha et al. 2013TICv8
58320.951.037.20——1859.7Q1-Q8 KOI TableTICv8
58141.051.25———1859.7Q1-Q17 DR25 KOI TableTICv8
58141.051.25———1859.7Q1-Q17 DR25 KOI TableTICv8
58250.901.00———1859.7Q1-Q17 DR24 KOI TableTICv8
58250.901.00———1859.7Q1-Q17 DR24 KOI TableTICv8
58250.901.00———1859.7Q1-Q12 KOI TableTICv8
5599—0.98———1859.7Q1-Q6 KOI TableTICv8
56971.041.578.91——1859.7Fulton & Petigura 2018TICv8
——————1859.7Q1-Q17 DR25 Supplemental KOI TableTICv8
57460.980.984.27——1859.7Morton et al. 2016TICv8
5599—0.98———1859.7Q1-Q6 KOI TableTICv8
——————1859.7Q1-Q17 DR25 Supplemental KOI TableTICv8
——————1859.7Q1-Q17 DR25 Supplemental KOI TableTICv8
58141.051.25———1859.7Q1-Q17 DR25 KOI TableTICv8
58141.051.25———1859.7Q1-Q17 DR25 KOI TableTICv8