Temperature
6114 K
5350 to 6114
Unclassified star • 1143 pc
Records
22
literature rows
Planets
2
system count
References
16
distinct source labels
Approximate color
from effective temperature
Canonical Summary
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
Mass
1.11 Msun
0.85 to 1.12
Radius
1.20 Rsun
1.05 to 1.77
Age
3.72 Gyr
3.72 to 6.60
Distance
1143 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 1.20 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-187
1.20 R☉
System Layout
2 planets linked to this host
Transit
Discovery
2014
Period
4.94 days
Radius
1.41 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2014
Period
10.64 days
Radius
2.67 R⊕
Mass
—
Eq. Temp
—
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
Evidence Summary
Rows
22
Stellar refs
15
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | 1143 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6114 | 1.11 | 1.20 | 3.72 | — | — | 1143 | Morton et al. 2016 | TICv8 |
| 5945 | 0.90 | 1.10 | — | — | — | 1143 | Q1-Q16 KOI Table | TICv8 |
| 5350 | — | 1.77 | — | 0.36 | — | 1143 | Gaia DR2 | TICv8 |
| 5666 | — | 1.05 | — | — | — | 1143 | Q1-Q6 KOI Table | TICv8 |
| 6105 | — | 1.29 | — | — | — | 1143 | Rowe et al. 2014 | TICv8 |
| 5666 | 0.85 | 1.05 | — | — | — | 1143 | Batalha et al. 2013 | TICv8 |
| 5973 | 1 | 1.15 | 6.60 | — | — | 1143 | Q1-Q8 KOI Table | TICv8 |
| 5945 | 0.90 | 1.10 | — | — | — | 1143 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5945 | 0.90 | 1.10 | — | — | — | 1143 | Q1-Q12 KOI Table | TICv8 |
| 5997 | 1.08 | 1.57 | 6.46 | — | — | 1143 | Fulton & Petigura 2018 | TICv8 |
| 6030 | 1.12 | 1.62 | — | 0.49 | — | 1143 | TICv8 | TICv8 |
| 5945 | 0.90 | 1.10 | — | — | — | 1143 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5666 | — | 1.05 | — | — | — | 1143 | Q1-Q6 KOI Table | TICv8 |
| — | — | — | — | — | — | 1143 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5997 | — | 1.61 | — | — | — | 1143 | Berger et al. 2018 | TICv8 |
| 5945 | 0.90 | 1.10 | — | — | — | 1143 | Q1-Q12 KOI Table | TICv8 |
| 6112 | 1.06 | 1.23 | — | — | — | 1143 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5666 | — | 1.21 | — | — | — | 1143 | Latham et al. 2005 | TICv8 |
| 5945 | 0.90 | 1.10 | — | — | — | 1143 | Q1-Q16 KOI Table | TICv8 |
| 5973 | 1 | 1.15 | 6.60 | — | — | 1143 | Q1-Q8 KOI Table | TICv8 |
| 6112 | 1.06 | 1.23 | — | — | — | 1143 | Q1-Q17 DR25 KOI Table | TICv8 |