Temperature
6449 K
6047.8 to 6774
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Stellar HostProfile
Kepler-1345
Unclassified star • 1355.0 pc
Records
12
literature rows
Planets
1
system count
References
13
distinct source labels
TIC: TIC 63288941
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
1.32 Msun
1.13 to 1.32
Radius
1.55 Rsun
1.39 to 2.02
Age
2.24 Gyr
1.78 to 3.55
Distance
1355.0 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.55 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1345
1.55 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1345 b
Transit
◌
Discovery
2016
Period
44.62 days
Radius
2.36 R⊕
Mass
—
Eq. Temp
—
Kepler-1345 b: A Super-Earth in a Distant System
Kepler-1345 is a single star located 4420 light-years away. The star is 2.24 billion years old and has a mass of 1.32 solar masses, a radius of 1.55 solar radii, and a temperature of 6450 K. Its reported mass and radius estimates are larger than the Sun's, and its reported temperature is hotter than the Sun's. One planet orbits this host.
That planet is Kepler-1345 b, a Super-Earth discovered by transit in 2016. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness; repeated dips help establish orbital periods. Kepler-1345 b completes an orbit every 44.6 days and has a radius of 2.36 Earth radii, larger than Earth's. Its size classification reflects this radius rather than its composition.
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 |
|---|---|---|---|---|---|---|---|---|
| 6394 | — | 1.78 | — | 0.68 | — | 1355.0 | Gaia DR2 | TICv8 |
| 6333 | — | 1.82 | — | — | — | 1355.0 | Berger et al. 2018 | TICv8 |
| 6763 | 1.24 | 1.42 | — | — | — | 1355.0 | Q1-Q12 KOI Table | TICv8 |
| 6333 | 1.23 | 1.76 | 3.55 | — | — | 1355.0 | Fulton & Petigura 2018 | TICv8 |
| 6763 | 1.24 | 1.42 | — | — | — | 1355.0 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6763 | 1.24 | 1.42 | — | — | — | 1355.0 | Q1-Q16 KOI Table | TICv8 |
| 6774 | 1.31 | 1.46 | 1.78 | — | — | 1355.0 | Q1-Q8 KOI Table | TICv8 |
| — | — | — | — | — | — | 1355.0 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6763 | 1.24 | 1.42 | — | — | — | 1355.0 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6047.8 | 1.13 | 2.02 | — | 0.69 | — | 1355.0 | TICv8 | TICv8 |
| 6449 | 1.32 | 1.55 | 2.24 | — | — | 1355.0 | Morton et al. 2016 | TICv8 |
| 6535 | — | 1.39 | — | — | — | 1355.0 | Latham et al. 2005 | TICv8 |