Temperature
6086 K
5740 to 6086
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Stellar HostProfile
Kepler-1349
Unclassified star • 276.3 pc
Records
13
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 405719110
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
1.16 Msun
1.01 to 1.18
Radius
1.28 Rsun
1.01 to 1.47
Age
2.88 Gyr
2.88 to 4.60
Distance
276.3 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.28 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
Kepler-1349
1.28 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1349 b
Transit
◌
Discovery
2016
Period
2.13 days
Radius
0.70 R⊕
Mass
—
Eq. Temp
—
Kepler-1349 b: A Sub-Earth in a Close Orbit
Kepler-1349 is a single star located 901 light-years away. It has 1.16 solar masses and 1.28 solar radii, making both its mass and radius larger than the Sun's. Its temperature is 6090 K, hotter than the Sun's, and its age is 2.88 billion years. One planet orbits this star.
That planet is Kepler-1349 b, a Sub-Earth, a size class for planets with a radius smaller than Earth's. Its radius is 0.7 Earth radii. It was discovered in 2016 by the transit method, in which a planet crosses in front of its star from our viewpoint and causes a small dip in observed brightness; repeated dips help establish orbital periods. Kepler-1349 b completes one orbit every 2.13 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
13
Stellar refs
13
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 |
|---|---|---|---|---|---|---|---|---|
| 5740 | — | 1.04 | — | — | — | 276.3 | Latham et al. 2005 | TICv8 |
| 5763.2 | — | 1.47 | — | 0.33 | — | 276.3 | Gaia DR2 | TICv8 |
| 5970 | 1.18 | 1.37 | 4.27 | — | — | 276.3 | Fulton & Petigura 2018 | TICv8 |
| 5998 | 1.14 | 1.36 | — | — | — | 276.3 | Q1-Q12 KOI Table | TICv8 |
| 5998 | 1.14 | 1.36 | — | — | — | 276.3 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6086 | 1.16 | 1.28 | 2.88 | — | — | 276.3 | Morton et al. 2016 | TICv8 |
| 5952 | 1.17 | 1.38 | — | — | — | 276.3 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5835.5 | 1.05 | 1.45 | — | 0.34 | — | 276.3 | TICv8 | TICv8 |
| — | 1.16 | 1.37 | 4.60 | — | — | 276.3 | Chaplin et al. 2014 | TICv8 |
| 5998 | 1.01 | 1.01 | 3.40 | — | — | 276.3 | Q1-Q8 KOI Table | TICv8 |
| 5998 | 1.14 | 1.36 | — | — | — | 276.3 | Q1-Q16 KOI Table | TICv8 |
| — | — | — | — | — | — | 276.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5970 | — | 1.38 | — | — | — | 276.3 | Berger et al. 2018 | TICv8 |