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Stellar HostProfile

Kepler-187

Unclassified star • 1143 pc

Records

22

literature rows

Planets

2

system count

References

16

distinct source labels

TIC: TIC 269264648

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

6114 K

5350 to 6114

20 values • 9 distinct

Mass

1.11 Msun

0.85 to 1.12

14 values • 7 distinct

Radius

1.20 Rsun

1.05 to 1.77

20 values • 11 distinct

Age

3.72 Gyr

3.72 to 6.60

4 values • 3 distinct

Distance

1143 pc

single adopted value

22 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.20 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

Kepler-187

1.20 R☉

System Layout

Known planets

2 planets linked to this host

◌

Discovery

2014

Period

4.94 days

Radius

1.41 R⊕

Mass

—

Eq. Temp

—

◌

Discovery

2014

Period

10.64 days

Radius

2.67 R⊕

Mass

—

Eq. Temp

—

Kepler-187 and Its Two Known Planets

Kepler-187 is a star located 3730 light-years from Earth. It hosts two known planets. The star is 3.72 billion years old, with a mass of 1.11 solar masses and a radius of 1.2 solar radii. Its temperature is 6110 K, and both its mass and radius estimates are larger than the Sun's, while its reported temperature is hotter than the Sun's.

The two planets, Kepler-187 b and Kepler-187 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; repeated dips help establish orbital periods. Kepler-187 b is an Earth-like planet with an orbital period of 4.94 days and a radius of 1.41 Earth radii, larger than Earth's. Kepler-187 c is a Neptune-like planet with an orbital period of 10.6 days and a radius of 2.67 Earth radii, also larger than Earth's. Among the listed planets, Kepler-187 b has the shortest year by reported estimates, while Kepler-187 c has the longest. Kepler-187 b also has the smallest radius by reported estimates, and Kepler-187 c has the largest.

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 • 11 distinct

Agedisputed

4 values • 3 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

17 values • 7 distinct

Metallicitydisputed

11 values • 5 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
——————1143Q1-Q17 DR25 Supplemental KOI TableTICv8
61141.111.203.72——1143Morton et al. 2016TICv8
59450.901.10———1143Q1-Q16 KOI TableTICv8
5350—1.77—0.36—1143Gaia DR2TICv8
5666—1.05———1143Q1-Q6 KOI TableTICv8
6105—1.29———1143Rowe et al. 2014TICv8
56660.851.05———1143Batalha et al. 2013TICv8
597311.156.60——1143Q1-Q8 KOI TableTICv8
59450.901.10———1143Q1-Q17 DR24 KOI TableTICv8
59450.901.10———1143Q1-Q12 KOI TableTICv8
59971.081.576.46——1143Fulton & Petigura 2018TICv8
60301.121.62—0.49—1143TICv8TICv8
59450.901.10———1143Q1-Q17 DR24 KOI TableTICv8
5666—1.05———1143Q1-Q6 KOI TableTICv8
——————1143Q1-Q17 DR25 Supplemental KOI TableTICv8
5997—1.61———1143Berger et al. 2018TICv8
59450.901.10———1143Q1-Q12 KOI TableTICv8
61121.061.23———1143Q1-Q17 DR25 KOI TableTICv8
5666—1.21———1143Latham et al. 2005TICv8
59450.901.10———1143Q1-Q16 KOI TableTICv8
597311.156.60——1143Q1-Q8 KOI TableTICv8
61121.061.23———1143Q1-Q17 DR25 KOI TableTICv8