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Stellar HostProfile

Kepler-185

Unclassified star • 466.7 pc

Records

22

literature rows

Planets

2

system count

References

16

distinct source labels

TIC: TIC 123490444

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

5132 K

4979 to 5208

20 values • 9 distinct

Mass

0.82 Msun

0.76 to 0.85

14 values • 7 distinct

Radius

0.79 Rsun

0.72 to 0.85

20 values • 10 distinct

Age

4.90 Gyr

4.47 to 11.90

4 values • 3 distinct

Distance

466.7 pc

single adopted value

22 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

Kepler-185

0.79 R☉

System Layout

Known planets

2 planets linked to this host

◌

Discovery

2014

Period

1.63 days

Radius

1.17 R⊕

Mass

—

Eq. Temp

—

◌

Discovery

2014

Period

20.73 days

Radius

2.02 R⊕

Mass

—

Eq. Temp

—

Kepler-185 and Its Two Planets

Kepler-185 is a star located 1520 light-years away. It is 4.9 billion years old and has a mass of 0.82 solar masses and a radius of 0.79 solar radii. Its temperature is 5130 K, cooler than the Sun's, and both its reported mass and radius estimates are smaller than the Sun's. Two planets orbit this host.

Kepler-185 b and Kepler-185 c were both 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, and repeated dips help establish orbital periods.

Kepler-185 b is classified as Earth-like and has a radius of 1.17 Earth radii. It completes an orbit every 1.63 days, the shortest year among the listed planets. Kepler-185 c is classified as a Super-Earth and has a radius of 2.02 Earth radii, the largest among the listed planets. Its orbital period is 20.7 days, the longest year among the listed planets.

In size classification, an Earth-like planet stays within 1.5 times Earth's radius, while a Super-Earth reaches 2.5 times.

Provenance

Underlying measurements and references

Evidence Summary

Rows

22

Stellar refs

15

System refs

1

Distancestable

22 values • 1 distinct

Parallaxstable

22 values • 1 distinct

Temperaturedisputed

20 values • 9 distinct

Massdisputed

14 values • 7 distinct

Radiusdisputed

20 values • 10 distinct

Agedisputed

4 values • 3 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

17 values • 6 distinct

Metallicitydisputed

11 values • 5 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
5039—0.85———466.7Latham et al. 2005TICv8
52050.810.79———466.7Q1-Q17 DR24 KOI TableTICv8
50370.760.724.47——466.7Fulton & Petigura 2018TICv8
52050.810.79———466.7Q1-Q16 KOI TableTICv8
51740.770.7811.90——466.7Q1-Q8 KOI TableTICv8
52050.810.79———466.7Q1-Q12 KOI TableTICv8
50710.850.72—-0.50—466.7TICv8TICv8
50390.790.79———466.7Batalha et al. 2013TICv8
5037—0.73———466.7Berger et al. 2018TICv8
5208—0.81———466.7Rowe et al. 2014TICv8
5039—0.79———466.7Q1-Q6 KOI TableTICv8
51740.770.7811.90——466.7Q1-Q8 KOI TableTICv8
52050.810.79———466.7Q1-Q17 DR24 KOI TableTICv8
5039—0.79———466.7Q1-Q6 KOI TableTICv8
5045.9—0.72—-0.52—466.7Gaia DR2TICv8
49790.810.80———466.7Q1-Q17 DR25 KOI TableTICv8
51320.820.794.90——466.7Morton et al. 2016TICv8
52050.810.79———466.7Q1-Q16 KOI TableTICv8
——————466.7Q1-Q17 DR25 Supplemental KOI TableTICv8
49790.810.80———466.7Q1-Q17 DR25 KOI TableTICv8
52050.810.79———466.7Q1-Q12 KOI TableTICv8
——————466.7Q1-Q17 DR25 Supplemental KOI TableTICv8