Temperature
5530 K
5361 to 5555
โBack to Stellar Hosts
Stellar HostProfile
Kepler-1808
Unclassified star โข 1022.0 pc
Records
10
literature rows
Planets
1
system count
References
11
distinct source labels
TIC: TIC 121215333
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
0.77 Msun
0.77 to 0.96
Radius
0.89 Rsun
0.86 to 1.07
Distance
1022.0 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.89 Rโ โข circles scaled linearly by radius
Sun
1.0 Rโ baseline
Kepler-1808
0.89 Rโ
System Layout
Known planets
1 planets linked to this host
Kepler-1808 b
Transit
โ
Discovery
2021
Period
23.34 days
Radius
3.03 Rโ
Mass
โ
Eq. Temp
โ
Kepler-1808 b: A Neptune-Like Planet in a Distant System
Kepler-1808 is a star located 3330 light-years away, and it hosts one known planet. The star has a mass of 0.773 solar masses and a radius of 0.892 solar radii. Its temperature is 5530 K, which is cooler than the Sun's, and its mass is smaller than the Sun's.
The planet Kepler-1808 b was discovered in 2021 by the transit method, which detects the small dip in a star's brightness when a planet passes in front of it. The planet's orbital period is 23.3 days, the time it takes to complete one orbit. Its radius is 3.03 Earth radii, larger than Earth's. This radius places it in the Neptune-like size class, which includes planets reaching up to 4 times Earth's radius.
Provenance
Underlying measurements and references
Evidence Summary
Rows
10
Stellar refs
10
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositystable
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5530 | 0.77 | 0.89 | โ | โ | โ | 1022.0 | Q1-Q12 KOI Table | TICv8 |
| 5361 | โ | 0.86 | โ | โ | โ | 1022.0 | Q1-Q6 KOI Table | TICv8 |
| 5491 | 0.96 | 1.03 | โ | -0.06 | โ | 1022.0 | TICv8 | TICv8 |
| 5530 | 0.77 | 0.89 | โ | โ | โ | 1022.0 | Q1-Q16 KOI Table | TICv8 |
| 5530 | 0.77 | 0.89 | โ | โ | โ | 1022.0 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5555 | 0.86 | 0.97 | 12.10 | โ | โ | 1022.0 | Q1-Q8 KOI Table | TICv8 |
| โ | โ | โ | โ | โ | โ | 1022.0 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5530 | 0.77 | 0.89 | โ | โ | โ | 1022.0 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5361 | โ | 1.07 | โ | โ | โ | 1022.0 | Latham et al. 2005 | TICv8 |
| 5361 | 0.80 | 0.86 | โ | โ | โ | 1022.0 | Batalha et al. 2013 | TICv8 |