Temperature
6826 K
6175.7 to 6826
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Stellar HostProfile
Kepler-1626
Unclassified star โข 1368.8 pc
Records
9
literature rows
Planets
1
system count
References
10
distinct source labels
TIC: TIC 184559893
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
1.51 Msun
1.18 to 1.51
Radius
1.85 Rsun
0.95 to 1.85
Age
1.55 Gyr
single adopted value
Distance
1368.8 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.85 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
Kepler-1626
1.85 Rโ
System Layout
Known planets
1 planets linked to this host
Kepler-1626 b
Transit
โ
Discovery
2016
Period
4.14 days
Radius
2.02 Rโ
Mass
โ
Eq. Temp
โ
Kepler-1626 and Its Super-Earth
Kepler-1626 is a star located 4460 light-years away, and it hosts one known planet. The star is 1.55 billion years old, with a mass of 1.51 solar masses, a radius of 1.85 solar radii, and a temperature of 6830 K. Its reported mass, radius, and temperature are each larger or hotter than the Sun's corresponding values.
The planet, Kepler-1626 b, was discovered in 2016 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. It is classified as a Super-Earth, a size class that reaches 2.5 times Earth's radius. Kepler-1626 b has an orbital period of 4.14 days and a radius of 2.02 Earth radii. Its reported radius estimate is larger than Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
9
Stellar refs
9
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 |
|---|---|---|---|---|---|---|---|---|
| 6517 | 1.18 | 1.16 | โ | โ | โ | 1368.8 | Q1-Q16 KOI Table | TICv8 |
| 6697 | 1.42 | 1.50 | โ | 0.61 | โ | 1368.8 | TICv8 | TICv8 |
| 6826 | 1.51 | 1.85 | 1.55 | โ | โ | 1368.8 | Morton et al. 2016 | TICv8 |
| 6553 | โ | 1.52 | โ | โ | โ | 1368.8 | Berger et al. 2018 | TICv8 |
| 6316 | โ | 0.95 | โ | โ | โ | 1368.8 | Latham et al. 2005 | TICv8 |
| 6535 | 1.20 | 1.18 | โ | โ | โ | 1368.8 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6517 | 1.18 | 1.16 | โ | โ | โ | 1368.8 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6175.7 | โ | 1.52 | โ | 0.48 | โ | 1368.8 | Gaia DR2 | TICv8 |
| โ | โ | โ | โ | โ | โ | 1368.8 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |