Temperature
5482 K
5172.9 to 5610
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Stellar HostProfile
Kepler-936
Unclassified star โข 823.4 pc
Records
12
literature rows
Planets
1
system count
References
13
distinct source labels
TIC: TIC 270619059
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
0.92 Msun
0.82 to 1.03
Radius
0.89 Rsun
0.89 to 1.19
Age
4.57 Gyr
4.57 to 14
Distance
823.4 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.89 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
Kepler-936
0.89 Rโ
System Layout
Known planets
1 planets linked to this host
Kepler-936 b
Transit
โ
Discovery
2016
Period
10.56 days
Radius
1.45 Rโ
Mass
โ
Eq. Temp
โ
Kepler-936 and Its Earth-Like Planet
Kepler-936 is a star located 2690 light-years away, and it hosts one known planet. The star's reported mass estimate is 0.92 solar masses, smaller than the Sun's, and its radius is 0.89 solar radii. Its reported temperature is 5480 K, cooler than the Sun's, and its age is 4.57 billion years.
The planet Kepler-936 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 Earth-like, a size class that stays within 1.5 times Earth's radius. Its radius is 1.45 Earth radii, larger than Earth's, and its orbital period is 10.6 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
12
Stellar refs
12
System refs
1
Distancestable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5382 | 0.97 | 1.15 | โ | โ | โ | 823.4 | Batalha et al. 2013 | TICv8 |
| 5172.9 | โ | โ | โ | โ | โ | 823.4 | TICv8 | TICv8 |
| 5437 | 0.82 | 0.93 | 14 | โ | โ | 823.4 | Q1-Q8 KOI Table | TICv8 |
| โ | โ | โ | โ | โ | โ | 823.4 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5610 | 1.03 | 1.17 | โ | โ | โ | 823.4 | Q1-Q12 KOI Table | TICv8 |
| 5610 | 1.03 | 1.17 | โ | โ | โ | 823.4 | Q1-Q16 KOI Table | TICv8 |
| 5382 | โ | 1.19 | โ | โ | โ | 823.4 | Latham et al. 2005 | TICv8 |
| 5610 | 1.03 | 1.17 | โ | โ | โ | 823.4 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5482 | 0.92 | 0.89 | 4.57 | โ | โ | 823.4 | Morton et al. 2016 | TICv8 |
| 5382 | โ | 1.15 | โ | โ | โ | 823.4 | Q1-Q6 KOI Table | TICv8 |
| 5610 | 1.03 | 1.17 | โ | โ | โ | 823.4 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5190.3 | โ | โ | โ | โ | โ | 823.4 | Gaia DR2 | TICv8 |