Temperature
5121 K
4956.9 to 5381
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Stellar HostProfile
Kepler-1614
Unclassified star โข 1191.2 pc
Records
10
literature rows
Planets
1
system count
References
11
distinct source labels
TIC: TIC 48451562
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
0.79 Msun
0.79 to 0.90
Radius
0.76 Rsun
0.68 to 0.99
Age
5.50 Gyr
single adopted value
Distance
1191.2 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.76 Rโ โข circles scaled linearly by radius
Sun
1.0 Rโ baseline
Kepler-1614
0.76 Rโ
System Layout
Known planets
1 planets linked to this host
Kepler-1614 b
Transit
โ
Discovery
2016
Period
3.95 days
Radius
1.49 Rโ
Mass
โ
Eq. Temp
โ
Kepler-1614 and Its Lone Planet
Kepler-1614 is a single-star system 3890 light-years away. The host star is 5.5 billion years old and has a mass of 0.79 solar masses, a radius of 0.76 solar radii, and a temperature of 5120 K. Its mass and radius estimates are smaller than the Sun's, and its temperature is cooler than the Sun's. One planet orbits this star.
That planet is Kepler-1614 b, an Earth-like world discovered by transit in 2016. A transit occurs when a planet crosses in front of its star from our viewpoint, dimming the observed brightness; repeated dips help establish orbital periods. Kepler-1614 b completes one orbit every 3.95 days, and its radius of 1.49 Earth radii is larger than Earth's, placing it within the Earth-like size class, which stays within 1.5 times Earth's radius.
Provenance
Underlying measurements and references
Evidence Summary
Rows
10
Stellar refs
10
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5107 | 0.86 | 0.94 | โ | -0.27 | โ | 1191.2 | TICv8 | TICv8 |
| 5376 | 0.90 | 0.81 | โ | โ | โ | 1191.2 | Q1-Q16 KOI Table | TICv8 |
| 5381 | โ | 0.90 | โ | โ | โ | 1191.2 | Berger et al. 2018 | TICv8 |
| 5376 | 0.90 | 0.81 | โ | โ | โ | 1191.2 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5376 | 0.90 | 0.81 | โ | โ | โ | 1191.2 | Q1-Q12 KOI Table | TICv8 |
| 5212 | โ | 0.68 | โ | โ | โ | 1191.2 | Latham et al. 2005 | TICv8 |
| 4956.9 | โ | 0.99 | โ | -0.28 | โ | 1191.2 | Gaia DR2 | TICv8 |
| 5376 | 0.90 | 0.81 | โ | โ | โ | 1191.2 | Q1-Q17 DR24 KOI Table | TICv8 |
| โ | โ | โ | โ | โ | โ | 1191.2 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5121 | 0.79 | 0.76 | 5.50 | โ | โ | 1191.2 | Morton et al. 2016 | TICv8 |