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Stellar HostProfile

K2-229

Unclassified star • 102.6 pc

Records

9

literature rows

Planets

2

system count

References

10

distinct source labels

TIC: TIC 98720809

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: Santerne et al. 2018 • System source: TICv8

Temperature

5185 K

5161.2 to 5315

8 values • 6 distinct

Mass

0.84 Msun

0.80 to 0.89

6 values • 6 distinct

Radius

0.79 Rsun

0.77 to 0.80

8 values • 7 distinct

Age

5.40 Gyr

single adopted value

1 values • 1 distinct

Distance

102.6 pc

single adopted value

9 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.79 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

K2-229

0.79 R☉

System Layout

Known planets

2 planets linked to this host

K2-229 b

Transit

◌

Discovery

2018

Period

0.58 days

Radius

1 R⊕

Mass

—

Eq. Temp

—

K2-229 c

Transit

◌

Discovery

2018

Period

8.33 days

Radius

2.03 R⊕

Mass

—

Eq. Temp

750 K

K2-229: A Sun-Like Star with Two Small Worlds

K2-229 is a G9 star located 335 light-years away. Its reported mass is 0.837 solar masses, its radius is 0.793 solar radii, and its temperature is 5190 K, all smaller or cooler than the Sun's corresponding values. The star is estimated to be 5.4 billion years old. Two planets are known to orbit it.

K2-229 b and K2-229 c were both discovered in 2018 by the transit method, in which a planet passes in front of its star from our viewpoint and causes a small dip in observed brightness. K2-229 b is an Earth-like planet with a radius of 1 Earth radii and an orbital period of 0.584 days. Among the listed planets, it has the shortest year and the smallest radius by reported estimates.

K2-229 c is a Super-Earth with a radius of 2.03 Earth radii, larger than Earth's, and an orbital period of 8.33 days. Among the listed planets, it has the longest year and the largest radius by reported estimates.

Provenance

Underlying measurements and references

Evidence Summary

Rows

9

Stellar refs

9

System refs

1

Distancestable

9 values • 1 distinct

Parallaxstable

9 values • 1 distinct

Temperaturedisputed

8 values • 6 distinct

Massdisputed

6 values • 6 distinct

Radiusdisputed

8 values • 7 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

7 values • 5 distinct

Metallicitydisputed

7 values • 5 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
5161.2—0.80—-0.39—102.6Gaia DR2TICv8
5315—0.79———102.6Adams et al. 2021TICv8
51850.800.78———102.6Dai et al. 2019TICv8
53150.870.79———102.6Livingston et al. 2018TICv8
—————G9102.6Luo et al. 2018TICv8
51850.840.795.40——102.6Santerne et al. 2018TICv8
51630.840.77———102.6Howard et al. 2025TICv8
52310.860.80———102.6Mayo et al. 2018TICv8
5214.50.890.79—-0.38—102.6TICv8TICv8