Temperature
4857 K
4648 to 4859.5
โBack to Stellar Hosts
Stellar HostProfile
Kepler-1362
Unclassified star โข 731.3 pc
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
TIC: TIC 121660595
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 โข System source: TICv8
Mass
0.80 Msun
0.69 to 0.80
Radius
0.74 Rsun
0.66 to 0.81
Age
3.09 Gyr
3.09 to 13.90
Distance
731.3 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.74 Rโ โข circles scaled linearly by radius
Sun
1.0 Rโ baseline
Kepler-1362
0.74 Rโ
System Layout
Known planets
1 planets linked to this host
Kepler-1362 b
Transit
โ
Discovery
2016
Period
136.2 days
Radius
2.60 Rโ
Mass
โ
Eq. Temp
โ
Kepler-1362: A Distant Star and Its Neptune-Like Planet
Kepler-1362 is a star located 2390 light-years away, and it hosts one known planet. The star itself is estimated to be 3.09 billion years old, with a mass of 0.8 solar masses, a radius of 0.74 solar radii, and a temperature of 4860 K. Its mass and radius are both smaller than the Sun's, and it is cooler than the Sun as well.
The only planet known to orbit Kepler-1362 is Kepler-1362 b, a Neptune-like world discovered in 2016 by the transit method, in which a planet passes in front of its star from our viewpoint and causes a small dip in observed brightness. This planet has an orbital period of 136 days and a radius of 2.6 Earth radii, making it larger than Earth. That radius places it within the Neptune-like size class, which extends up to 4 times Earth's radius.
Provenance
Underlying measurements and references
Evidence Summary
Rows
11
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 |
|---|---|---|---|---|---|---|---|---|
| 4654 | 0.74 | 0.77 | โ | -0.60 | โ | 731.3 | TICv8 | TICv8 |
| 4650 | 0.70 | 0.69 | โ | โ | โ | 731.3 | Q1-Q17 DR24 KOI Table | TICv8 |
| 4683 | โ | 0.81 | โ | โ | โ | 731.3 | Latham et al. 2005 | TICv8 |
| 4786 | 0.69 | 0.67 | 13.90 | โ | โ | 731.3 | Q1-Q8 KOI Table | TICv8 |
| โ | โ | โ | โ | โ | โ | 731.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4648 | 0.71 | 0.68 | โ | โ | โ | 731.3 | Q1-Q17 DR25 KOI Table | TICv8 |
| 4650 | 0.70 | 0.69 | โ | โ | โ | 731.3 | Q1-Q16 KOI Table | TICv8 |
| 4857 | 0.80 | 0.74 | 3.09 | โ | โ | 731.3 | Morton et al. 2016 | TICv8 |
| 4859.5 | โ | 0.66 | โ | -0.65 | โ | 731.3 | Gaia DR2 | TICv8 |
| 4651 | โ | 0.72 | โ | โ | โ | 731.3 | Berger et al. 2018 | TICv8 |
| 4650 | 0.70 | 0.69 | โ | โ | โ | 731.3 | Q1-Q12 KOI Table | TICv8 |