Temperature
4951 K
4901 to 5094
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Stellar HostProfile
Kepler-1414
Unclassified star โข 570.8 pc
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
TIC: TIC 164828419
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
0.80 Msun
0.80 to 0.92
Radius
0.75 Rsun
0.75 to 1.94
Age
4.68 Gyr
4.68 to 14
Distance
570.8 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.75 Rโ โข circles scaled linearly by radius
Sun
1.0 Rโ baseline
Kepler-1414
0.75 Rโ
System Layout
Known planets
1 planets linked to this host
Kepler-1414 b
Transit
โ
Discovery
2016
Period
3.52 days
Radius
1.23 Rโ
Mass
โ
Eq. Temp
โ
Kepler-1414 and Its Lone Planet
Kepler-1414 is a star located 1860 light-years away, and it hosts one known planet. The star is estimated to be 4.68 billion years old, with a mass of 0.8 solar masses and a radius of 0.75 solar radii, making it smaller and less massive than the Sun. Its temperature of 4950 K is also cooler than the Sun's.
The single planet orbiting this star is Kepler-1414 b, discovered in 2016 by the transit method. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. Kepler-1414 b completes one orbit every 3.52 days, and its radius of 1.23 Earth radii is larger than Earth's. This measurement places it within the Earth-like size class, which covers planets up to 1.5 times Earth's radius.
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 |
|---|---|---|---|---|---|---|---|---|
| 5094 | 0.83 | 0.90 | โ | โ | โ | 570.8 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5094 | 0.83 | 0.90 | โ | โ | โ | 570.8 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5094 | 0.83 | 0.90 | โ | โ | โ | 570.8 | Q1-Q12 KOI Table | TICv8 |
| 5094 | 0.83 | 0.90 | โ | โ | โ | 570.8 | Q1-Q16 KOI Table | TICv8 |
| 4901 | โ | 1.26 | โ | โ | โ | 570.8 | Latham et al. 2005 | TICv8 |
| 4914 | 0.81 | 0.81 | โ | -0.46 | โ | 570.8 | TICv8 | TICv8 |
| 5003.5 | โ | 0.75 | โ | -0.50 | โ | 570.8 | Gaia DR2 | TICv8 |
| 5080 | โ | 0.80 | โ | โ | โ | 570.8 | Berger et al. 2018 | TICv8 |
| โ | โ | โ | โ | โ | โ | 570.8 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4951 | 0.80 | 0.75 | 4.68 | โ | โ | 570.8 | Morton et al. 2016 | TICv8 |
| 4977 | 0.92 | 1.94 | 14 | โ | โ | 570.8 | Q1-Q8 KOI Table | TICv8 |