Temperature
5806 K
5413 to 5806
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Stellar HostProfile
Kepler-926
Unclassified star • 921.4 pc
Records
18
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 394174412
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 • System source: TICv8
Mass
1.01 Msun
0.85 to 1.02
Radius
1.01 Rsun
0.53 to 1.33
Age
4.37 Gyr
0.40 to 4.37
Distance
921.4 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.01 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-926
1.01 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-926 b
Transit
◌
Discovery
2016
Period
52.07 days
Radius
2.31 R⊕
Mass
—
Eq. Temp
—
Kepler-926 and Its Super-Earth
Kepler-926 is a star located 3010 light-years away. It has 1.01 solar masses, a radius of 1.01 solar radii, and a temperature of 5810 K. Its age is 4.37 billion years. One planet orbits this host.
That planet is Kepler-926 b, a Super-Earth discovered in 2016 by the transit method. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. Kepler-926 b completes an orbit every 52.1 days, and its radius is 2.31 Earth radii. A size class compares radius with Earth's: a Super-Earth reaches 2.5 times Earth's radius, and Kepler-926 b's reported radius estimate is larger than Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
18
Stellar refs
13
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5513 | 0.85 | 0.75 | — | — | — | 921.4 | Batalha et al. 2013 | TICv8 |
| — | — | — | — | — | — | 921.4 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| — | — | — | — | — | — | 921.4 | Q1-Q12 KOI Table | TICv8 |
| 5693 | 0.88 | 0.80 | — | — | — | 921.4 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5724 | 0.96 | 0.85 | 0.40 | — | — | 921.4 | Q1-Q8 KOI Table | TICv8 |
| 5733 | 1.02 | 1.24 | — | 0.17 | — | 921.4 | TICv8 | TICv8 |
| 5513 | — | 0.75 | — | — | — | 921.4 | Q1-Q6 KOI Table | TICv8 |
| 5693 | 0.88 | 0.80 | — | — | — | 921.4 | Q1-Q16 KOI Table | TICv8 |
| 5806 | 1.01 | 1.01 | 4.37 | — | — | 921.4 | Morton et al. 2016 | TICv8 |
| 5693 | 0.88 | 0.80 | — | — | — | 921.4 | Q1-Q12 KOI Table | TICv8 |
| — | — | — | — | — | — | 921.4 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5724 | 0.96 | 0.85 | 0.40 | — | — | 921.4 | Q1-Q8 KOI Table | TICv8 |
| 5513 | — | 0.53 | — | — | — | 921.4 | Latham et al. 2005 | TICv8 |
| 5513 | — | 0.75 | — | — | — | 921.4 | Q1-Q6 KOI Table | TICv8 |
| 5565 | 1.01 | 1.25 | — | — | — | 921.4 | Q1-Q17 DR25 KOI Table | TICv8 |
| — | — | — | — | — | — | 921.4 | Q1-Q16 KOI Table | TICv8 |
| 5413 | — | 1.33 | — | 0.13 | — | 921.4 | Gaia DR2 | TICv8 |
| 5562 | — | 1.25 | — | — | — | 921.4 | Berger et al. 2018 | TICv8 |