Temperature
5983 K
5819.7 to 6068
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Stellar HostProfile
Kepler-134
Unclassified star • 334.8 pc
Records
22
literature rows
Planets
2
system count
References
17
distinct source labels
TIC: TIC 48448369
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
1.06 Msun
0.96 to 1.26
Radius
1.07 Rsun
0.97 to 1.53
Age
3.55 Gyr
3.55 to 4.17
Distance
334.8 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.07 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-134
1.07 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-134 b
Transit
◌
Discovery
2014
Period
5.32 days
Radius
2 R⊕
Mass
—
Eq. Temp
—
Kepler-134 c
Transit
◌
Discovery
2014
Period
10.11 days
Radius
1.26 R⊕
Mass
—
Eq. Temp
—
Kepler-134: A Star and Its Two Transit-Detected Planets
Kepler-134 is a star located 1090 light-years away, and it hosts two known planets. The star's reported mass estimate is larger than the Sun's, and its reported temperature is hotter than the Sun's. It is 3.55 billion years old, has a mass of 1.06 solar masses, a radius of 1.07 solar radii, and a temperature of 5980 K.
Both planets were discovered by the transit method in 2014. Kepler-134 b is classified as a Super-Earth and has a radius of 2 Earth radii, which is larger than Earth's. It completes one orbit in 5.32 days. Kepler-134 c is classified as Earth-like and has a radius of 1.26 Earth radii, also larger than Earth's. Its orbital period is 10.1 days.
Among the listed planets, Kepler-134 b has the shortest year and the largest radius by reported estimates, while Kepler-134 c has the longest year and the smallest radius by reported estimates.
Provenance
Underlying measurements and references
Evidence Summary
Rows
22
Stellar refs
16
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 |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | 334.8 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5936 | — | 1.06 | — | — | — | 334.8 | Q1-Q6 KOI Table | TICv8 |
| 5918 | — | 0.98 | — | — | — | 334.8 | Berger et al. 2018 | TICv8 |
| 6068 | 1.26 | 1.53 | — | — | — | 334.8 | Q1-Q16 KOI Table | TICv8 |
| 5923 | 0.97 | 1.05 | — | — | — | 334.8 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5819.7 | 1.05 | 1.05 | — | 0.06 | — | 334.8 | TICv8 | TICv8 |
| 5819.7 | — | 1.05 | — | — | — | 334.8 | ExoFOP | TICv8 |
| 6068 | 1.26 | 1.53 | — | — | — | 334.8 | Q1-Q12 KOI Table | TICv8 |
| 5993.3 | — | 0.97 | — | 0.04 | — | 334.8 | Gaia DR2 | TICv8 |
| — | — | — | — | — | — | 334.8 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6068 | 1.26 | 1.53 | — | — | — | 334.8 | Q1-Q12 KOI Table | TICv8 |
| 6068 | 1.26 | 1.53 | — | — | — | 334.8 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6068 | 1.26 | 1.53 | — | — | — | 334.8 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5918 | 0.96 | 0.97 | 4.17 | — | — | 334.8 | Fulton & Petigura 2018 | TICv8 |
| 6068 | 1.26 | 1.53 | — | — | — | 334.8 | Q1-Q16 KOI Table | TICv8 |
| 5936 | 1.01 | 1.03 | — | — | — | 334.8 | Q1-Q8 KOI Table | TICv8 |
| 5936 | 1.01 | 1.03 | — | — | — | 334.8 | Q1-Q8 KOI Table | TICv8 |
| 5936 | — | 1.06 | — | — | — | 334.8 | Batalha et al. 2013 | TICv8 |
| 5983 | 1.06 | 1.07 | 3.55 | — | — | 334.8 | Morton et al. 2016 | TICv8 |
| 5983 | — | 1.18 | — | — | — | 334.8 | Rowe et al. 2014 | TICv8 |
| 5923 | 0.97 | 1.05 | — | — | — | 334.8 | Q1-Q17 DR25 KOI Table | TICv8 |
| — | 0.96 | — | — | — | — | 334.8 | Weiss et al. 2024 | TICv8 |