Temperature
5812 K
5744.4 to 6014
Unclassified star • 1039.0 pc
Records
21
literature rows
Planets
2
system count
References
13
distinct source labels
Approximate color
from effective temperature
Canonical Summary
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
Temperature
5812 K
5744.4 to 6014
Mass
1.02 Msun
0.99 to 1.04
Radius
1.03 Rsun
1 to 1.05
Age
4.27 Gyr
4 to 4.27
Distance
1039.0 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 1.03 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-365
1.03 R☉
System Layout
2 planets linked to this host
Transit
Discovery
2014
Period
10.66 days
Radius
2.04 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2014
Period
17.78 days
Radius
1.64 R⊕
Mass
—
Eq. Temp
—
Kepler-365 is a star 3390 light-years away with two known planets, both discovered by transit in 2014. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. The host star is 4.27 billion years old, with a mass of 1.02 solar masses, a radius of 1.03 solar radii, and a temperature of 5810 K.
Both planets are classified as Super-Earths, a size class that reaches 2.5 times Earth's radius. Kepler-365 b has an orbital period of 10.7 days and a radius of 2.04 Earth radii. Kepler-365 c has an orbital period of 17.8 days and a radius of 1.64 Earth radii. Among the listed planets, Kepler-365 b has the shortest year and the largest radius by reported estimates, while Kepler-365 c has the longest year and the smallest radius by reported estimates. Kepler-365 b's reported radius estimate is larger than Earth's.
Provenance
Evidence Summary
Rows
21
Stellar refs
12
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5759 | — | 1 | — | — | — | 1039.0 | Q1-Q6 KOI Table | TICv8 |
| — | — | — | — | — | — | 1039.0 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6014 | 1.04 | 1.02 | — | — | — | 1039.0 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5980 | 1.00 | 1.01 | 4 | — | — | 1039.0 | Q1-Q8 KOI Table | TICv8 |
| 6011 | 1.03 | 1.03 | — | — | — | 1039.0 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6011 | 1.03 | 1.03 | — | — | — | 1039.0 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6011 | 1.03 | 1.03 | — | — | — | 1039.0 | Q1-Q16 KOI Table | TICv8 |
| 6011 | 1.03 | 1.03 | — | — | — | 1039.0 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6011 | 1.03 | 1.03 | — | — | — | 1039.0 | Q1-Q12 KOI Table | TICv8 |
| 6011 | 1.03 | 1.03 | — | — | — | 1039.0 | Q1-Q16 KOI Table | TICv8 |
| 6014 | 1.04 | 1.02 | — | — | — | 1039.0 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5759 | — | 1.04 | — | — | — | 1039.0 | Latham et al. 2005 | TICv8 |
| — | — | — | — | — | — | 1039.0 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5744.4 | — | — | — | — | — | 1039.0 | TICv8 | TICv8 |
| 6011 | 1.03 | 1.03 | — | — | — | 1039.0 | Q1-Q12 KOI Table | TICv8 |
| 5812 | 1.02 | 1.03 | 4.27 | — | — | 1039.0 | Morton et al. 2016 | TICv8 |
| 6011 | 1.03 | 1.03 | — | — | — | 1039.0 | Q1-Q16 KOI Table | TICv8 |
| — | — | — | — | — | — | 1039.0 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5759 | 0.99 | 1 | — | — | — | 1039.0 | Batalha et al. 2013 | TICv8 |
| 6012 | — | 1.05 | — | — | — | 1039.0 | Rowe et al. 2014 | TICv8 |
| 6014 | 1.04 | 1.02 | — | — | — | 1039.0 | Q1-Q17 DR25 KOI Table | TICv8 |