Temperature
6195 K
5784 to 6241
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Stellar HostProfile
Kepler-1396
Unclassified star • 1066.5 pc
Records
17
literature rows
Planets
1
system count
References
12
distinct source labels
TIC: TIC 270954695
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
1.18 Msun
1.06 to 1.18
Radius
1.27 Rsun
0.99 to 1.27
Age
2.75 Gyr
0.26 to 2.75
Distance
1066.5 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.27 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1396
1.27 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1396 b
Transit
◌
Discovery
2016
Period
18.22 days
Radius
2.07 R⊕
Mass
—
Eq. Temp
—
Kepler-1396 and Its Super-Earth
Kepler-1396 is a star 3480 light-years away with one known planet. The host is 2.75 billion years old, has 1.18 solar masses, 1.27 solar radii, and a temperature of 6200 K. Each of these values is larger than the corresponding value for the Sun, and the temperature is hotter as well.
The planet is Kepler-1396 b, a Super-Earth discovered by transit in 2016. It orbits every 18.2 days and has a radius of 2.07 Earth radii, larger than Earth's. 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.
Provenance
Underlying measurements and references
Evidence Summary
Rows
17
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 |
|---|---|---|---|---|---|---|---|---|
| 6241 | 1.09 | 1.03 | — | — | — | 1066.5 | Q1-Q12 KOI Table | TICv8 |
| 5947 | — | 1.12 | — | — | — | 1066.5 | Berger et al. 2018 | TICv8 |
| 6241 | 1.09 | 1.03 | — | — | — | 1066.5 | Q1-Q12 KOI Table | TICv8 |
| 6238 | 1.11 | 1.03 | 0.26 | — | — | 1066.5 | Q1-Q8 KOI Table | TICv8 |
| 5951 | 1.12 | 1.26 | — | — | — | 1066.5 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5784 | — | 1.17 | — | 0.14 | — | 1066.5 | Gaia DR2 | TICv8 |
| — | — | — | — | — | — | 1066.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6241 | 1.09 | 1.03 | — | — | — | 1066.5 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6241 | 1.09 | 1.03 | — | — | — | 1066.5 | Q1-Q16 KOI Table | TICv8 |
| 6241 | 1.09 | 1.03 | — | — | — | 1066.5 | Q1-Q16 KOI Table | TICv8 |
| 6028 | — | 0.99 | — | — | — | 1066.5 | Latham et al. 2005 | TICv8 |
| 5951 | 1.12 | 1.26 | — | — | — | 1066.5 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5874.9 | 1.06 | 1.22 | — | 0.20 | — | 1066.5 | TICv8 | TICv8 |
| — | — | — | — | — | — | 1066.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6241 | 1.09 | 1.03 | — | — | — | 1066.5 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6195 | 1.18 | 1.27 | 2.75 | — | — | 1066.5 | Morton et al. 2016 | TICv8 |
| 6238 | 1.11 | 1.03 | 0.26 | — | — | 1066.5 | Q1-Q8 KOI Table | TICv8 |