Temperature
5521 K
5357 to 5810
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Stellar HostProfile
Kepler-783
Unclassified star • 516.1 pc
Records
20
literature rows
Planets
2
system count
References
15
distinct source labels
TIC: TIC 159642390
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
0.93 Msun
0.84 to 0.94
Radius
0.89 Rsun
0.85 to 1.26
Age
3.89 Gyr
3.89 to 9.70
Distance
516.1 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.89 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-783
0.89 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-783 b
Transit
◌
Discovery
2016
Period
4.29 days
Radius
0.78 R⊕
Mass
—
Eq. Temp
—
Kepler-783 c
Transit
◌
Discovery
2020
Period
7.05 days
Radius
2.33 R⊕
Mass
—
Eq. Temp
—
Kepler-783 and Its Two Planets
Kepler-783 is a star 1680 light-years away with a mass of 0.93 solar masses, a radius of 0.89 solar radii, a temperature of 5520 K, and an age of 3.89 billion years. Its reported mass and radius estimates are smaller than the Sun's, and its reported temperature is cooler than the Sun's. Two planets are known to orbit it.
Kepler-783 b is a Sub-Earth discovered by transit in 2016. Its radius is 0.78 Earth radii, smaller than Earth's, and its year lasts 4.29 days, the shortest among the listed planets.
Kepler-783 c is a Super-Earth discovered by transit in 2020, with a radius of 2.33 Earth radii, larger than Earth's. Its year is 7.05 days, the longest among the listed planets. A transit is a planet's passage in front of its star from our viewpoint, causing a small dip in observed brightness.
Provenance
Underlying measurements and references
Evidence Summary
Rows
20
Stellar refs
14
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 |
|---|---|---|---|---|---|---|---|---|
| 5381 | — | 0.86 | — | — | — | 516.1 | Berger et al. 2018 | TICv8 |
| — | — | — | — | — | — | 516.1 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| — | — | — | — | — | — | 516.1 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5388 | — | 0.86 | — | -0.25 | — | 516.1 | Gaia DR2 | TICv8 |
| 5775 | 0.84 | 1.11 | — | — | — | 516.1 | Q1-Q12 KOI Table | TICv8 |
| 5521 | 0.93 | 0.89 | 3.89 | — | — | 516.1 | Morton et al. 2016 | TICv8 |
| 5810 | 0.94 | 1.17 | 9.70 | — | — | 516.1 | Q1-Q8 KOI Table | TICv8 |
| 5549 | — | 1.02 | — | — | — | 516.1 | Q1-Q6 KOI Table | TICv8 |
| 5549 | — | 1.02 | — | — | — | 516.1 | Batalha et al. 2013 | TICv8 |
| 5775 | 0.84 | 1.11 | — | — | — | 516.1 | Q1-Q12 KOI Table | TICv8 |
| 5549 | — | 1.26 | — | — | — | 516.1 | Latham et al. 2005 | TICv8 |
| 5357 | 0.85 | 0.86 | — | — | — | 516.1 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5357 | 0.85 | 0.86 | — | — | — | 516.1 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5411.5 | 0.94 | 0.87 | — | -0.23 | — | 516.1 | TICv8 | TICv8 |
| 5775 | 0.84 | 1.11 | — | — | — | 516.1 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5381 | 0.88 | 0.85 | 4.68 | — | — | 516.1 | Fulton & Petigura 2018 | TICv8 |
| 5775 | 0.84 | 1.11 | — | — | — | 516.1 | Q1-Q16 KOI Table | TICv8 |
| 5810 | 0.94 | 1.17 | 9.70 | — | — | 516.1 | Q1-Q8 KOI Table | TICv8 |
| 5775 | 0.84 | 1.11 | — | — | — | 516.1 | Q1-Q16 KOI Table | TICv8 |
| 5775 | 0.84 | 1.11 | — | — | — | 516.1 | Q1-Q17 DR24 KOI Table | TICv8 |