Temperature
5557 K
5535 to 5803
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Stellar HostProfile
Kepler-1437
Unclassified star โข 2101.7 pc
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
TIC: TIC 26541175
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
0.93 Msun
0.93 to 0.97
Radius
0.90 Rsun
0.85 to 1.66
Age
4.57 Gyr
0.40 to 4.57
Distance
2101.7 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.90 Rโ โข circles scaled linearly by radius
Sun
1.0 Rโ baseline
Kepler-1437
0.90 Rโ
System Layout
Known planets
1 planets linked to this host
Kepler-1437 b
Transit
โ
Discovery
2016
Period
10.93 days
Radius
1.37 Rโ
Mass
โ
Eq. Temp
โ
Kepler-1437 b: A Close-In Earth-Like World
Kepler-1437 is a star located 6850 light-years away, and it hosts one known planet, Kepler-1437 b. The host star is 4.57 billion years old, with a mass of 0.93 solar masses and a radius of 0.9 solar radii. Its temperature is 5560 K, making it cooler than the Sun, and its mass is smaller than the Sun's.
Kepler-1437 b was discovered in 2016 by the transit method, which detects the small dip in a star's brightness when a planet passes in front of it. The planet is classified as Earth-like, meaning its radius stays within 1.5 times Earth's radius. Its radius is 1.37 Earth radii, which is larger than Earth's, and it completes one orbit every 10.9 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
11
Stellar refs
11
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositystable
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5803 | โ | 1.66 | โ | โ | โ | 2101.7 | Berger et al. 2018 | TICv8 |
| 5589 | โ | 0.85 | โ | โ | โ | 2101.7 | Latham et al. 2005 | TICv8 |
| 5789 | 0.97 | 0.87 | 0.40 | โ | โ | 2101.7 | Q1-Q8 KOI Table | TICv8 |
| 5796 | 0.97 | 0.87 | โ | โ | โ | 2101.7 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5796 | 0.97 | 0.87 | โ | โ | โ | 2101.7 | Q1-Q16 KOI Table | TICv8 |
| 5792 | 0.96 | 0.86 | โ | โ | โ | 2101.7 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5796 | 0.97 | 0.87 | โ | โ | โ | 2101.7 | Q1-Q12 KOI Table | TICv8 |
| 5535 | โ | โ | โ | โ | โ | 2101.7 | TICv8 | TICv8 |
| 5669.4 | โ | 1.49 | โ | 0.32 | โ | 2101.7 | Gaia DR2 | TICv8 |
| โ | โ | โ | โ | โ | โ | 2101.7 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5557 | 0.93 | 0.90 | 4.57 | โ | โ | 2101.7 | Morton et al. 2016 | TICv8 |