Temperature
6025 K
5661 to 6025
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Stellar HostProfile
Kepler-147
Unclassified star • 1042.0 pc
Records
22
literature rows
Planets
2
system count
References
16
distinct source labels
TIC: TIC 121458206
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
Mass
1.14 Msun
0.98 to 1.15
Radius
1.34 Rsun
1.19 to 1.59
Age
4.47 Gyr
4.47 to 8.30
Distance
1042.0 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.34 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-147
1.34 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-147 b
Transit
◌
Discovery
2014
Period
12.61 days
Radius
1.53 R⊕
Mass
—
Eq. Temp
—
Kepler-147 c
Transit
◌
Discovery
2014
Period
33.42 days
Radius
2.43 R⊕
Mass
—
Eq. Temp
—
Kepler-147 and Its Two Super-Earths
Kepler-147 is a star located 3400 light-years away, and it hosts two planets. The star is 4.47 billion years old, with a mass of 1.14 solar masses and a radius of 1.34 solar radii. Its temperature is 6030 K, and its reported mass and radius estimates are larger than the Sun's, while its reported temperature is hotter than the Sun's.
Both planets were discovered by transit in 2014. Kepler-147 b is a Super-Earth with an orbital period of 12.6 days and a radius of 1.53 Earth radii. Kepler-147 c is also a Super-Earth, with an orbital period of 33.4 days and a radius of 2.43 Earth radii. The radius of each planet is larger than Earth's.
Among the listed planets, Kepler-147 b has the shortest year by reported estimates, and Kepler-147 c has the longest year by reported estimates. Kepler-147 b also has the smallest radius by reported estimates, while Kepler-147 c has the largest radius by reported estimates.
Provenance
Underlying measurements and references
Evidence Summary
Rows
22
Stellar refs
15
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5661 | — | 1.59 | — | 0.37 | — | 1042.0 | Gaia DR2 | TICv8 |
| 5887.4 | 1.07 | 1.57 | — | 0.43 | — | 1042.0 | TICv8 | TICv8 |
| 6010 | 1.10 | 1.26 | — | — | — | 1042.0 | Q1-Q16 KOI Table | TICv8 |
| 6010 | 1.10 | 1.26 | — | — | — | 1042.0 | Q1-Q12 KOI Table | TICv8 |
| 5684 | — | 1.19 | — | — | — | 1042.0 | Q1-Q6 KOI Table | TICv8 |
| 6007 | 1.11 | 1.42 | — | — | — | 1042.0 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6010 | 1.10 | 1.26 | — | — | — | 1042.0 | Q1-Q12 KOI Table | TICv8 |
| — | — | — | — | — | — | 1042.0 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6010 | 1.10 | 1.26 | — | — | — | 1042.0 | Q1-Q16 KOI Table | TICv8 |
| 6025 | 1.14 | 1.34 | 4.47 | — | — | 1042.0 | Morton et al. 2016 | TICv8 |
| — | — | — | — | — | — | 1042.0 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5943 | 1.15 | 1.52 | 5.50 | — | — | 1042.0 | Fulton & Petigura 2018 | TICv8 |
| 5894 | 0.98 | 1.19 | 8.30 | — | — | 1042.0 | Q1-Q8 KOI Table | TICv8 |
| 5684 | — | 1.19 | — | — | — | 1042.0 | Q1-Q6 KOI Table | TICv8 |
| 6007 | 1.11 | 1.42 | — | — | — | 1042.0 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6012 | — | 1.47 | — | — | — | 1042.0 | Rowe et al. 2014 | TICv8 |
| 5684 | 1.01 | 1.19 | — | — | — | 1042.0 | Batalha et al. 2013 | TICv8 |
| 5684 | — | 1.25 | — | — | — | 1042.0 | Latham et al. 2005 | TICv8 |
| 6010 | 1.10 | 1.26 | — | — | — | 1042.0 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5894 | 0.98 | 1.19 | 8.30 | — | — | 1042.0 | Q1-Q8 KOI Table | TICv8 |
| 6010 | 1.10 | 1.26 | — | — | — | 1042.0 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5943 | — | 1.55 | — | — | — | 1042.0 | Berger et al. 2018 | TICv8 |