Temperature
5853 K
5585 to 5853
โBack to Stellar Hosts
Stellar HostProfile
Kepler-1980
Unclassified star โข 1709.4 pc
Records
11
literature rows
Planets
1
system count
References
8
distinct source labels
TIC: TIC 139036617
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: Q1-Q12 KOI Table โข System source: TICv8
Mass
0.90 Msun
0.90 to 1.05
Radius
0.83 Rsun
0.83 to 1.34
Distance
1709.4 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.83 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
Kepler-1980
0.83 Rโ
System Layout
Known planets
1 planets linked to this host
Kepler-1980 b
Transit
โ
Discovery
2023
Period
33.03 days
Radius
2.21 Rโ
Mass
โ
Eq. Temp
564 K
Kepler-1980 and Its Super-Earth
Kepler-1980 is a star located 5580 light-years away. It has a mass of 0.902 solar masses, a radius of 0.83 solar radii, and a temperature of 5850 K. One planet orbits this host.
That planet is Kepler-1980 b, a Super-Earth discovered by transit in 2023. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. Kepler-1980 b has an orbital period of 33 days, meaning it completes one orbit in that time. Its radius is 2.21 Earth radii, and its reported radius estimate is larger than Earth's. Earth radii compare radius, not volume, and a Super-Earth reaches 2.5 times Earth's radius.
Provenance
Underlying measurements and references
Evidence Summary
Rows
11
Stellar refs
7
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Luminositystable
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| โ | โ | โ | โ | โ | โ | 1709.4 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| โ | โ | โ | โ | โ | โ | 1709.4 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5853 | 0.90 | 0.83 | โ | โ | โ | 1709.4 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5853 | 0.90 | 0.83 | โ | โ | โ | 1709.4 | Q1-Q16 KOI Table | TICv8 |
| 5585 | โ | 0.83 | โ | โ | โ | 1709.4 | Latham et al. 2005 | TICv8 |
| 5819 | 1.05 | 0.99 | โ | โ | โ | 1709.4 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5853 | 0.90 | 0.83 | โ | โ | โ | 1709.4 | Q1-Q12 KOI Table | TICv8 |
| 5819 | 1.05 | 0.99 | โ | โ | โ | 1709.4 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5853 | 0.90 | 0.83 | โ | โ | โ | 1709.4 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5671 | 1.01 | 1.34 | โ | 0.22 | โ | 1709.4 | TICv8 | TICv8 |
| 5853 | 0.90 | 0.83 | โ | โ | โ | 1709.4 | Q1-Q16 KOI Table | TICv8 |