Temperature
6099 K
5757.7 to 6267
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Stellar HostProfile
Kepler-1557
Unclassified star โข 1380.2 pc
Records
10
literature rows
Planets
1
system count
References
11
distinct source labels
TIC: TIC 270790313
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 โข System source: TICv8
Mass
1.11 Msun
1.07 to 1.12
Radius
1.17 Rsun
0.82 to 1.17
Age
3.31 Gyr
single adopted value
Distance
1380.2 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.17 Rโ โข circles scaled linearly by radius
Sun
1.0 Rโ baseline
Kepler-1557
1.17 Rโ
System Layout
Known planets
1 planets linked to this host
Kepler-1557 b
Transit
โ
Discovery
2016
Period
3.74 days
Radius
1.53 Rโ
Mass
โ
Eq. Temp
โ
Kepler-1557 b: A Super-Earth in a Distant System
Kepler-1557 is a star located 4,500 light-years away, with a single known planet in orbit around it. The star has a mass of 1.11 solar masses and a radius of 1.17 solar radii, both larger than the Sun's corresponding values, and its temperature of 6100 K is hotter than the Sun's. It is 3.31 billion years old.
The planet Kepler-1557 b was discovered in 2016 by the transit method, in which a planet passing in front of its star from our viewpoint causes a small dip in observed brightness, and repeated dips help establish its orbital period. Kepler-1557 b completes one orbit in 3.74 days. Its radius of 1.53 Earth radii is larger than Earth's, placing it in the Super-Earth size class, which spans radii up to 2.5 times Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
10
Stellar refs
10
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 6225 | 1.09 | 1.03 | โ | โ | โ | 1380.2 | Q1-Q12 KOI Table | TICv8 |
| โ | โ | โ | โ | โ | โ | 1380.2 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5904.5 | 1.07 | 1.10 | โ | 0.12 | โ | 1380.2 | TICv8 | TICv8 |
| 6099 | 1.11 | 1.17 | 3.31 | โ | โ | 1380.2 | Morton et al. 2016 | TICv8 |
| 5757.7 | โ | 1.09 | โ | 0.07 | โ | 1380.2 | Gaia DR2 | TICv8 |
| 6014 | โ | 0.82 | โ | โ | โ | 1380.2 | Latham et al. 2005 | TICv8 |
| 6225 | 1.09 | 1.03 | โ | โ | โ | 1380.2 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6260 | 1.12 | 1.06 | โ | โ | โ | 1380.2 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6267 | โ | 1.06 | โ | โ | โ | 1380.2 | Berger et al. 2018 | TICv8 |
| 6225 | 1.09 | 1.03 | โ | โ | โ | 1380.2 | Q1-Q16 KOI Table | TICv8 |