Temperature
4754 K
4604 to 4915
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Stellar HostProfile
Kepler-1150
Unclassified star • 358.5 pc
Records
13
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 27913639
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
0.76 Msun
0.67 to 0.97
Radius
0.72 Rsun
0.60 to 1.91
Age
4.68 Gyr
4.68 to 13.90
Distance
358.5 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.72 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
Kepler-1150
0.72 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1150 b
Transit
◌
Discovery
2016
Period
2.79 days
Radius
1.02 R⊕
Mass
—
Eq. Temp
—
Kepler-1150 b: A Close-In Earth-Sized World
Kepler-1150 is a star system 1170 light-years away that is known to host one planet. The host star is estimated to be 4.68 billion years old, with a mass of 0.76 solar masses and a radius of 0.72 solar radii. Its temperature is 4750 K, and its mass, radius, and temperature are all smaller or cooler than the Sun's.
The planet, Kepler-1150 b, was discovered in 2016 by the transit method, in which a planet passes in front of its star from our viewpoint and causes a small dip in observed brightness. Repeated dips help establish orbital periods. Kepler-1150 b completes an orbit every 2.79 days and has a radius of 1.02 Earth radii. Its Earth-like classification places it within 1.5 times Earth's radius, a size class based on radius rather than composition.
Provenance
Underlying measurements and references
Evidence Summary
Rows
13
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 |
|---|---|---|---|---|---|---|---|---|
| 4655 | 0.97 | 1.91 | — | — | — | 358.5 | Batalha et al. 2013 | TICv8 |
| — | — | — | — | — | — | 358.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4706 | 0.67 | 0.65 | 13.90 | — | — | 358.5 | Q1-Q8 KOI Table | TICv8 |
| 4827 | 0.95 | 1.73 | — | — | — | 358.5 | Q1-Q16 KOI Table | TICv8 |
| 4827 | 0.95 | 1.73 | — | — | — | 358.5 | Q1-Q12 KOI Table | TICv8 |
| 4827 | 0.95 | 1.73 | — | — | — | 358.5 | Q1-Q17 DR24 KOI Table | TICv8 |
| 4655 | — | 1.91 | — | — | — | 358.5 | Q1-Q6 KOI Table | TICv8 |
| 4915 | — | 0.60 | — | -0.73 | — | 358.5 | Gaia DR2 | TICv8 |
| 4604 | 0.73 | 0.73 | — | -0.67 | — | 358.5 | TICv8 | TICv8 |
| 4820 | — | 0.68 | — | — | — | 358.5 | Berger et al. 2018 | TICv8 |
| 4655 | — | 1.43 | — | — | — | 358.5 | Latham et al. 2005 | TICv8 |
| 4754 | 0.76 | 0.72 | 4.68 | — | — | 358.5 | Morton et al. 2016 | TICv8 |
| 4827 | 0.95 | 1.73 | — | — | — | 358.5 | Q1-Q17 DR25 KOI Table | TICv8 |