Temperature
5214 K
4913.7 to 5303
Unclassified star • 1030.8 pc
Records
19
literature rows
Planets
2
system count
References
12
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
5214 K
4913.7 to 5303
Mass
0.86 Msun
0.82 to 0.93
Radius
0.82 Rsun
0.77 to 0.92
Age
4.68 Gyr
4.68 to 6.92
Distance
1030.8 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 0.82 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1600
0.82 R☉
System Layout
2 planets linked to this host
Transit
Discovery
2016
Period
386.4 days
Radius
3.13 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2021
Period
7.30 days
Radius
1.94 R⊕
Mass
—
Eq. Temp
—
Kepler-1600 is a star 3360 light-years away with two known planets. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. Both planets were found this way: Kepler-1600 b in 2016 and Kepler-1600 c in 2021.
The host star is 4.68 billion years old, has 0.86 solar masses, 0.82 solar radii, and a temperature of 5210 K. Its reported mass and radius estimates are smaller than the Sun's, and its reported temperature is cooler than the Sun's.
Kepler-1600 b is Neptune-like, with a radius of 3.13 Earth radii and an orbital period of 386 days. Kepler-1600 c is a Super-Earth with a radius of 1.94 Earth radii and an orbital period of 7.3 days. Among the listed planets, Kepler-1600 c has the shortest year and the smallest radius by reported estimates, while Kepler-1600 b has the longest year and the largest radius by reported estimates. Both planets' reported radius estimates are larger than Earth's.
Provenance
Evidence Summary
Rows
19
Stellar refs
11
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | 1030.8 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| — | — | — | — | — | — | 1030.8 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5303 | 0.93 | 0.83 | — | — | — | 1030.8 | Q1-Q16 KOI Table | TICv8 |
| 5303 | 0.93 | 0.83 | — | — | — | 1030.8 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5090 | 0.84 | 0.83 | 6.92 | — | — | 1030.8 | Fulton & Petigura 2018 | TICv8 |
| 5303 | 0.93 | 0.83 | — | — | — | 1030.8 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5119 | 0.82 | 0.83 | — | — | — | 1030.8 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5098 | — | 0.77 | — | — | — | 1030.8 | Latham et al. 2005 | TICv8 |
| 5090 | — | 0.85 | — | — | — | 1030.8 | Berger et al. 2018 | TICv8 |
| 5303 | 0.93 | 0.83 | — | — | — | 1030.8 | Q1-Q16 KOI Table | TICv8 |
| 5303 | 0.93 | 0.83 | — | — | — | 1030.8 | Q1-Q16 KOI Table | TICv8 |
| 5102 | 0.86 | 0.87 | — | -0.34 | — | 1030.8 | TICv8 | TICv8 |
| 4913.7 | — | 0.92 | — | -0.35 | — | 1030.8 | Gaia DR2 | TICv8 |
| — | — | — | — | — | — | 1030.8 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5303 | 0.93 | 0.83 | — | — | — | 1030.8 | Q1-Q12 KOI Table | TICv8 |
| 5303 | 0.93 | 0.83 | — | — | — | 1030.8 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5119 | 0.82 | 0.83 | — | — | — | 1030.8 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5119 | 0.82 | 0.83 | — | — | — | 1030.8 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5214 | 0.86 | 0.82 | 4.68 | — | — | 1030.8 | Morton et al. 2016 | TICv8 |