Temperature
6133 K
5679.7 to 6215
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Stellar HostProfile
Kepler-1346
Unclassified star โข 843.7 pc
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
TIC: TIC 63066410
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 โข System source: TICv8
Mass
1.14 Msun
0.98 to 1.14
Radius
1.21 Rsun
0.90 to 1.21
Age
3.09 Gyr
0.40 to 3.09
Distance
843.7 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.21 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
Kepler-1346
1.21 Rโ
System Layout
Known planets
1 planets linked to this host
Kepler-1346 b
Transit
โ
Discovery
2016
Period
3.40 days
Radius
1.58 Rโ
Mass
โ
Eq. Temp
โ
Kepler-1346 and Its Super-Earth
Kepler-1346 is a star 2750 light-years away with one known planet. The host star is 3.09 billion years old and has a mass of 1.14 solar masses and a radius of 1.21 solar radii. Its temperature is 6130 K. The star's mass, radius, and temperature are all larger or hotter than the Sun's.
The planet Kepler-1346 b is a Super-Earth discovered by transit in 2016. It orbits every 3.4 days. Its radius is 1.58 Earth radii, larger than Earth's. A Super-Earth's size class reaches 2.5 times Earth's radius. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness; repeated dips help establish orbital periods.
Provenance
Underlying measurements and references
Evidence Summary
Rows
11
Stellar refs
11
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 |
|---|---|---|---|---|---|---|---|---|
| 6177 | 0.98 | 0.91 | โ | โ | โ | 843.7 | Q1-Q12 KOI Table | TICv8 |
| 6186 | โ | 0.90 | โ | โ | โ | 843.7 | Berger et al. 2018 | TICv8 |
| 6177 | 0.98 | 0.91 | โ | โ | โ | 843.7 | Q1-Q16 KOI Table | TICv8 |
| 6133 | 1.14 | 1.21 | 3.09 | โ | โ | 843.7 | Morton et al. 2016 | TICv8 |
| โ | โ | โ | โ | โ | โ | 843.7 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6177 | 0.98 | 0.91 | โ | โ | โ | 843.7 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6177 | 0.98 | 0.91 | โ | โ | โ | 843.7 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5785.3 | โ | 0.95 | โ | -0.04 | โ | 843.7 | Gaia DR2 | TICv8 |
| 5956 | โ | 0.93 | โ | โ | โ | 843.7 | Latham et al. 2005 | TICv8 |
| 5679.7 | 1.01 | 1.02 | โ | -8.06e-3 | โ | 843.7 | TICv8 | TICv8 |
| 6215 | 1.11 | 1.03 | 0.40 | โ | โ | 843.7 | Q1-Q8 KOI Table | TICv8 |