Temperature
4512 K
4322 to 4515
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Stellar HostProfile
Kepler-1136
Unclassified star • 491.4 pc
Records
16
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 164671623
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
0.72 Msun
0.60 to 0.72
Radius
0.68 Rsun
0.57 to 0.69
Age
3.24 Gyr
3.24 to 13.90
Distance
491.4 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.68 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1136
0.68 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1136 b
Transit
◌
Discovery
2016
Period
2.36 days
Radius
1.64 R⊕
Mass
—
Eq. Temp
—
Kepler-1136 b: A Super-Earth in a Close Orbit
Kepler-1136 is a star located 1600 light-years away, and one planet has been found orbiting it. The host star has a mass of 0.72 solar masses, a radius of 0.68 solar radii, and a temperature of 4510 K. Its reported age is 3.24 billion years. The star's reported mass estimate is smaller than the Sun's, its reported radius estimate is smaller than the Sun's, and its reported temperature is cooler than the Sun's.
The planet, Kepler-1136 b, is a Super-Earth, a size class that reaches 2.5 times Earth's radius. It was discovered by the transit method in 2016. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. Kepler-1136 b has a radius of 1.64 Earth radii, which is larger than Earth's. Its orbital period is 2.36 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
16
Stellar refs
13
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 |
|---|---|---|---|---|---|---|---|---|
| 4478 | 0.64 | 0.65 | — | — | — | 491.4 | Q1-Q12 KOI Table | TICv8 |
| — | — | — | — | — | — | 491.4 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4478 | 0.64 | 0.65 | — | — | — | 491.4 | Q1-Q17 DR24 KOI Table | TICv8 |
| 4478 | 0.64 | 0.65 | — | — | — | 491.4 | Q1-Q16 KOI Table | TICv8 |
| 4444 | 0.70 | 0.63 | — | -0.85 | — | 491.4 | TICv8 | TICv8 |
| 4485 | 0.63 | 0.60 | 13.90 | — | — | 491.4 | Q1-Q8 KOI Table | TICv8 |
| 4476 | — | 0.61 | — | — | — | 491.4 | Berger et al. 2018 | TICv8 |
| 4478 | 0.64 | 0.65 | — | — | — | 491.4 | Q1-Q16 KOI Table | TICv8 |
| 4322 | — | 0.69 | — | — | — | 491.4 | Latham et al. 2005 | TICv8 |
| 4322 | — | 0.57 | — | — | — | 491.4 | Q1-Q6 KOI Table | TICv8 |
| 4478 | 0.64 | 0.65 | — | — | — | 491.4 | Q1-Q17 DR25 KOI Table | TICv8 |
| 4515 | — | 0.59 | — | -0.88 | — | 491.4 | Gaia DR2 | TICv8 |
| 4322 | 0.60 | 0.57 | — | — | — | 491.4 | Batalha et al. 2013 | TICv8 |
| 4478 | 0.64 | 0.65 | — | — | — | 491.4 | Q1-Q12 KOI Table | TICv8 |
| 4512 | 0.72 | 0.68 | 3.24 | — | — | 491.4 | Morton et al. 2016 | TICv8 |
| — | — | — | — | — | — | 491.4 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |