Temperature
5236 K
5000.4 to 5335
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Stellar HostProfile
Kepler-1302
Unclassified star • 634.6 pc
Records
13
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 417678115
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
0.86 Msun
0.79 to 0.86
Radius
0.82 Rsun
0.71 to 0.93
Age
4.68 Gyr
4.68 to 13.70
Distance
634.6 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.82 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
Kepler-1302
0.82 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1302 b
Transit
◌
Discovery
2016
Period
8.84 days
Radius
1.43 R⊕
Mass
—
Eq. Temp
—
Kepler-1302 b: A Close-In Earth-Like World
Kepler-1302 is a star located 2070 light-years away, and it hosts one known planet. The star is estimated to be 4.68 billion years old, with a mass of 0.86 solar masses and a radius of 0.82 solar radii. Its temperature is 5240 K, cooler than the Sun's, and both its mass and radius estimates are smaller than the Sun's.
The planet, Kepler-1302 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. Kepler-1302 b has an orbital period of 8.84 days and a radius of 1.43 Earth radii, larger than Earth's. That radius places it within the Earth-like size class.
Provenance
Underlying measurements and references
Evidence Summary
Rows
13
Stellar refs
13
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitystable
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5330 | 0.85 | 0.87 | — | — | — | 634.6 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5330 | 0.85 | 0.87 | — | — | — | 634.6 | Q1-Q16 KOI Table | TICv8 |
| 5236 | 0.86 | 0.82 | 4.68 | — | — | 634.6 | Morton et al. 2016 | TICv8 |
| 5141 | 0.82 | 0.84 | — | — | — | 634.6 | Batalha et al. 2013 | TICv8 |
| 5330 | 0.85 | 0.87 | — | — | — | 634.6 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5141 | — | 0.93 | — | — | — | 634.6 | Latham et al. 2005 | TICv8 |
| 5071 | 0.85 | 0.76 | — | -0.47 | — | 634.6 | TICv8 | TICv8 |
| 5141 | — | 0.84 | — | — | — | 634.6 | Q1-Q6 KOI Table | TICv8 |
| 5330 | 0.85 | 0.87 | — | — | — | 634.6 | Q1-Q12 KOI Table | TICv8 |
| 5000.4 | — | 0.77 | — | -0.48 | — | 634.6 | Gaia DR2 | TICv8 |
| — | — | — | — | — | — | 634.6 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5335 | — | 0.71 | — | — | — | 634.6 | Berger et al. 2018 | TICv8 |
| 5278 | 0.79 | 0.83 | 13.70 | — | — | 634.6 | Q1-Q8 KOI Table | TICv8 |