Temperature
6161 K
5814.5 to 6161
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Stellar HostProfile
Kepler-1382
Unclassified star • 738.3 pc
Records
12
literature rows
Planets
1
system count
References
13
distinct source labels
TIC: TIC 184014439
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
1.36 Msun
1.03 to 1.38
Radius
1.72 Rsun
0.93 to 1.79
Age
2.75 Gyr
0.60 to 2.75
Distance
738.3 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.72 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
Kepler-1382
1.72 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1382 b
Transit
◌
Discovery
2016
Period
16.36 days
Radius
1.88 R⊕
Mass
—
Eq. Temp
—
Kepler-1382 and Its Super-Earth
Kepler-1382 is a star 2410 light-years away with one known planet in orbit. The host star is estimated to be 2.75 billion years old, with a mass of 1.36 solar masses and a radius of 1.72 solar radii. Its temperature is 6160 K, and its reported mass, radius, and temperature are all larger or hotter than the Sun's.
The planet, Kepler-1382 b, was discovered in 2016 by the transit method, in which a planet passing in front of its star from our viewpoint causes a small dip in observed brightness. Repeated dips help establish orbital periods. Kepler-1382 b completes an orbit every 16.4 days and has a radius of 1.88 Earth radii, larger than Earth's. It is classified as a Super-Earth, a size class that reaches up to 2.5 times Earth's radius.
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 |
|---|---|---|---|---|---|---|---|---|
| 6139 | — | 1.75 | — | — | — | 738.3 | Berger et al. 2018 | TICv8 |
| 6133 | 1.38 | 1.76 | — | — | — | 738.3 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5842 | — | 0.94 | — | — | — | 738.3 | Latham et al. 2005 | TICv8 |
| 5814.5 | — | 1.79 | — | 0.52 | — | 738.3 | Gaia DR2 | TICv8 |
| 6054 | 1.13 | 1.76 | — | 0.57 | — | 738.3 | TICv8 | TICv8 |
| 6161 | 1.36 | 1.72 | 2.75 | — | — | 738.3 | Morton et al. 2016 | TICv8 |
| 6139 | 1.37 | 1.73 | 2.69 | — | — | 738.3 | Fulton & Petigura 2018 | TICv8 |
| 5983 | 1.03 | 0.93 | 0.60 | — | — | 738.3 | Q1-Q8 KOI Table | TICv8 |
| — | — | — | — | — | — | 738.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6046 | 1.11 | 1.01 | — | — | — | 738.3 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6046 | 1.11 | 1.01 | — | — | — | 738.3 | Q1-Q16 KOI Table | TICv8 |
| 6046 | 1.11 | 1.01 | — | — | — | 738.3 | Q1-Q12 KOI Table | TICv8 |