Temperature
6251 K
5990.7 to 6388
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Stellar HostProfile
Kepler-135
Unclassified star • 621.9 pc
Records
21
literature rows
Planets
2
system count
References
16
distinct source labels
TIC: TIC 122450088
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
1.25 Msun
1.05 to 1.26
Radius
1.35 Rsun
1.19 to 1.56
Age
2.45 Gyr
2.45 to 6.76
Distance
621.9 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.35 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-135
1.35 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-135 b
Transit
◌
Discovery
2014
Period
6.00 days
Radius
1.81 R⊕
Mass
—
Eq. Temp
—
Kepler-135 c
Transit
◌
Discovery
2014
Period
11.45 days
Radius
1.16 R⊕
Mass
—
Eq. Temp
—
Kepler-135 and Its Two Known Planets
Kepler-135 is a star located 2030 light-years away, and two planets have been found orbiting it. The host star is 2.45 billion years old and has a mass of 1.25 solar masses, a radius of 1.35 solar radii, and a temperature of 6250 K, making it more massive, larger, and hotter than the Sun.
Both planets were discovered by transit in 2014. Kepler-135 b is a Super-Earth with a radius of 1.81 Earth radii and an orbital period of 6 days. This radius is larger than Earth's, and among the listed planets it is the largest, with the shortest year. Kepler-135 c is an Earth-like planet with a radius of 1.16 Earth radii and an orbital period of 11.4 days. It has the smallest radius among the listed planets and the longest year, at 11.4 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
21
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 |
|---|---|---|---|---|---|---|---|---|
| 6014 | 1.05 | 1.41 | 6.76 | — | — | 621.9 | Fulton & Petigura 2018 | TICv8 |
| 6388 | 1.19 | 1.21 | — | — | — | 621.9 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6388 | 1.19 | 1.21 | — | — | — | 621.9 | Q1-Q16 KOI Table | TICv8 |
| 6388 | 1.19 | 1.21 | — | — | — | 621.9 | Q1-Q12 KOI Table | TICv8 |
| 5990.7 | 1.10 | 1.56 | — | 0.45 | — | 621.9 | TICv8 | TICv8 |
| 6251 | 1.25 | 1.35 | 2.45 | — | — | 621.9 | Morton et al. 2016 | TICv8 |
| 6204 | 1.26 | 1.36 | — | — | — | 621.9 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6014 | — | 1.43 | — | — | — | 621.9 | Berger et al. 2018 | TICv8 |
| 6131 | — | 1.22 | — | — | — | 621.9 | Batalha et al. 2013 | TICv8 |
| 6131 | — | 1.19 | — | — | — | 621.9 | Latham et al. 2005 | TICv8 |
| 6337 | 1.14 | 1.21 | 2.62 | — | — | 621.9 | Q1-Q8 KOI Table | TICv8 |
| 6388 | 1.19 | 1.21 | — | — | — | 621.9 | Q1-Q17 DR24 KOI Table | TICv8 |
| — | — | — | — | — | — | 621.9 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6131 | — | 1.22 | — | — | — | 621.9 | Q1-Q6 KOI Table | TICv8 |
| 6388 | 1.19 | 1.21 | — | — | — | 621.9 | Q1-Q16 KOI Table | TICv8 |
| 6204 | 1.26 | 1.36 | — | — | — | 621.9 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6337 | 1.14 | 1.21 | 2.62 | — | — | 621.9 | Q1-Q8 KOI Table | TICv8 |
| — | — | — | — | — | — | 621.9 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6090 | — | 1.27 | — | — | — | 621.9 | Rowe et al. 2014 | TICv8 |
| 6388 | 1.19 | 1.21 | — | — | — | 621.9 | Q1-Q12 KOI Table | TICv8 |
| 6051.3 | — | 1.44 | — | 0.40 | — | 621.9 | Gaia DR2 | TICv8 |