Temperature
4662 K
4337 to 4737.0
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Stellar HostProfile
Kepler-1341
Unclassified star • 477.0 pc
Records
12
literature rows
Planets
1
system count
References
13
distinct source labels
TIC: TIC 123126460
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
0.79 Msun
0.66 to 0.80
Radius
0.72 Rsun
0.56 to 0.79
Age
1.82 Gyr
1 to 2.40
Distance
477.0 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.72 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1341
0.72 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1341 b
Transit
◌
Discovery
2016
Period
133.0 days
Radius
2.99 R⊕
Mass
—
Eq. Temp
—
Kepler-1341 b: A Neptune-Like World
Kepler-1341 is a star located 1560 light-years away, and it hosts one known planet. The star has a mass of 0.79 solar masses, a radius of 0.72 solar radii, and a temperature of 4660 K. Its reported age is 1.82 billion years. These values describe the host star only, not both members of the system.
The single planet, Kepler-1341 b, was discovered in 2016 by the transit method, which detects the small dip in a star's brightness when a planet crosses in front of it. Kepler-1341 b has a radius of 2.99 Earth radii, classifying it as Neptune-like - a size class that extends up to four times Earth's radius but does not itself indicate composition. Its orbital period is 133 days, the time it takes to complete one orbit around its star.
Provenance
Underlying measurements and references
Evidence Summary
Rows
12
Stellar refs
12
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 |
|---|---|---|---|---|---|---|---|---|
| 4737.0 | — | 0.67 | — | -0.69 | — | 477.0 | Gaia DR2 | TICv8 |
| 4523 | 0.69 | 0.66 | — | — | — | 477.0 | Q1-Q17 DR25 KOI Table | TICv8 |
| 4535 | 0.66 | 0.59 | 1 | — | — | 477.0 | Q1-Q8 KOI Table | TICv8 |
| — | — | — | — | — | — | 477.0 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4530 | 0.69 | 0.66 | — | — | — | 477.0 | Q1-Q16 KOI Table | TICv8 |
| 4511 | 0.71 | 0.79 | — | -0.64 | — | 477.0 | TICv8 | TICv8 |
| 4530 | 0.69 | 0.66 | — | — | — | 477.0 | Q1-Q12 KOI Table | TICv8 |
| 4530 | 0.69 | 0.66 | — | — | — | 477.0 | Q1-Q17 DR24 KOI Table | TICv8 |
| 4662 | 0.79 | 0.72 | 1.82 | — | — | 477.0 | Morton et al. 2016 | TICv8 |
| 4683 | 0.80 | 0.72 | 2.40 | — | — | 477.0 | Fulton & Petigura 2018 | TICv8 |
| 4683 | — | 0.73 | — | — | — | 477.0 | Berger et al. 2018 | TICv8 |
| 4337 | — | 0.56 | — | — | — | 477.0 | Latham et al. 2005 | TICv8 |