Temperature
4950 K
4814 to 5006
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Stellar HostProfile
Kepler-1782
Unclassified star • 305.8 pc
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
TIC: TIC 123202646
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: Fulton & Petigura 2018 • System source: TICv8
Mass
0.79 Msun
0.72 to 0.79
Radius
0.74 Rsun
0.71 to 1.24
Age
2.88 Gyr
2.88 to 14
Distance
305.8 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.74 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
Kepler-1782
0.74 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1782 b
Transit
◌
Discovery
2021
Period
5.76 days
Radius
2.23 R⊕
Mass
—
Eq. Temp
—
Kepler-1782 and Its Super-Earth
Kepler-1782 is a star located 997 light-years away, and it hosts one known planet. The star is estimated to be 2.88 billion years old, with a mass of 0.794 solar masses and a radius of 0.736 solar radii. Its temperature is 4950 K, which is cooler than the Sun's, and both its reported mass and radius estimates are smaller than the Sun's.
The planet Kepler-1782 b is classified as a Super-Earth. It was discovered in 2021 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. Repeated dips help establish orbital periods. Kepler-1782 b orbits its star every 5.76 days and has a radius of 2.23 Earth radii, larger than Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
11
Stellar refs
11
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositystable
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 4814 | 0.79 | 0.79 | — | — | — | 305.8 | Batalha et al. 2013 | TICv8 |
| 4814 | — | 0.79 | — | — | — | 305.8 | Q1-Q6 KOI Table | TICv8 |
| 4867 | 0.79 | 0.74 | — | -0.56 | — | 305.8 | TICv8 | TICv8 |
| 4931 | 0.79 | 0.73 | — | — | — | 305.8 | Q1-Q17 DR25 KOI Table | TICv8 |
| 4926 | 0.72 | 0.71 | 14 | — | — | 305.8 | Q1-Q8 KOI Table | TICv8 |
| 5006 | 0.79 | 0.83 | — | — | — | 305.8 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5006 | 0.79 | 0.83 | — | — | — | 305.8 | Q1-Q12 KOI Table | TICv8 |
| 5006 | 0.79 | 0.83 | — | — | — | 305.8 | Q1-Q16 KOI Table | TICv8 |
| 4814 | — | 1.24 | — | — | — | 305.8 | Latham et al. 2005 | TICv8 |
| — | — | — | — | — | — | 305.8 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4950 | 0.79 | 0.74 | 2.88 | — | — | 305.8 | Fulton & Petigura 2018 | TICv8 |