Temperature
6334.8 K
6258 to 6477
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Stellar HostProfile
Kepler-1713
Unclassified star • 295.3 pc
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
TIC: TIC 158432813
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: TICv8 • System source: TICv8
Mass
1.25 Msun
1.17 to 1.32
Radius
1.45 Rsun
1.26 to 1.58
Luminosity
0.49 log(Lsun)
single adopted value
Distance
295.3 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.45 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1713
1.45 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1713 b
Transit
◌
Discovery
2021
Period
18.01 days
Radius
1.72 R⊕
Mass
—
Eq. Temp
—
Kepler-1713 b: A Super-Earth in Transit
Kepler-1713 is a star located 963 light-years away. Its reported mass is 1.25 solar masses, its reported radius is 1.45 solar radii, and its temperature is 6330 K. Each of these estimates is larger or hotter than the corresponding value for the Sun. The star hosts one known planet.
That planet is Kepler-1713 b, a Super-Earth discovered by transit in 2021. A transit occurs when a planet passes in front of its star from our viewpoint, dimming the observed starlight and helping establish the planet's orbital period. Kepler-1713 b completes one orbit in 18 days. Its radius is 1.72 Earth radii, larger than Earth's. As a Super-Earth, its size class places it by radius at up to 2.5 times Earth's radius, without implying anything about its composition.
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 |
|---|---|---|---|---|---|---|---|---|
| 6364 | 1.24 | 1.26 | 1.45 | — | — | 295.3 | Q1-Q8 KOI Table | TICv8 |
| 6302 | 1.17 | 1.43 | 3.72 | — | — | 295.3 | Fulton & Petigura 2018 | TICv8 |
| 6463 | 1.32 | 1.45 | — | — | — | 295.3 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6364 | — | 1.26 | — | — | — | 295.3 | Batalha et al. 2013 | TICv8 |
| 6364 | — | 1.26 | — | — | — | 295.3 | Q1-Q6 KOI Table | TICv8 |
| 6334.8 | 1.25 | 1.45 | — | 0.49 | — | 295.3 | TICv8 | TICv8 |
| 6477 | 1.30 | 1.46 | — | — | — | 295.3 | Q1-Q17 DR25 KOI Table | TICv8 |
| — | — | — | — | — | — | 295.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6463 | 1.32 | 1.45 | — | — | — | 295.3 | Q1-Q16 KOI Table | TICv8 |
| 6463 | 1.32 | 1.45 | — | — | — | 295.3 | Q1-Q12 KOI Table | TICv8 |
| 6258 | — | 1.58 | — | — | — | 295.3 | Latham et al. 2005 | TICv8 |