Temperature
4439 K
4225 to 4439
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Stellar HostProfile
Kepler-1351
Unclassified star • 202.8 pc
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
TIC: TIC 270609625
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
0.70 Msun
0.60 to 0.70
Radius
0.67 Rsun
0.53 to 1.03
Age
4.17 Gyr
4.17 to 13.90
Distance
202.8 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.67 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1351
0.67 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1351 b
Transit
◌
Discovery
2016
Period
0.92 days
Radius
0.65 R⊕
Mass
—
Eq. Temp
—
Kepler-1351 b: A Sub-Earth World
Kepler-1351 is a star located 661 light-years away, and it hosts one planet. The star is estimated to be 4.17 billion years old, with a mass of 0.7 solar masses and a radius of 0.67 solar radii. Its temperature is 4440 K, making it cooler than the Sun, and both its mass and radius estimates are smaller than the Sun's.
The planet, Kepler-1351 b, was discovered in 2016 by the transit method, in which a planet passes in front of its star from our viewpoint and causes a small dip in observed brightness. Repeated dips help establish orbital periods. Kepler-1351 b completes an orbit every 0.916 days. Its radius is 0.65 Earth radii, smaller than Earth's, and it is classified as a Sub-Earth, a size class for planets smaller than Earth.
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 |
|---|---|---|---|---|---|---|---|---|
| 4321.5 | 0.68 | 0.58 | — | -0.98 | — | 202.8 | TICv8 | TICv8 |
| 4374 | 0.60 | 0.61 | — | — | — | 202.8 | Q1-Q17 DR25 KOI Table | TICv8 |
| 4365 | — | 0.56 | — | — | — | 202.8 | Berger et al. 2018 | TICv8 |
| 4374 | 0.60 | 0.61 | — | — | — | 202.8 | Q1-Q16 KOI Table | TICv8 |
| 4410 | 0.61 | 0.58 | 13.90 | — | — | 202.8 | Q1-Q8 KOI Table | TICv8 |
| — | — | — | — | — | — | 202.8 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4374 | 0.60 | 0.61 | — | — | — | 202.8 | Q1-Q17 DR24 KOI Table | TICv8 |
| 4225 | — | 1.03 | — | — | — | 202.8 | Latham et al. 2005 | TICv8 |
| 4397.5 | — | 0.53 | — | -1.02 | — | 202.8 | Gaia DR2 | TICv8 |
| 4439 | 0.70 | 0.67 | 4.17 | — | — | 202.8 | Morton et al. 2016 | TICv8 |
| 4374 | 0.60 | 0.61 | — | — | — | 202.8 | Q1-Q12 KOI Table | TICv8 |