Temperature
5346 K
5125.2 to 5371
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Stellar HostProfile
Kepler-933
Unclassified star • 1017.2 pc
Records
13
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 159099716
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
0.87 Msun
0.71 to 0.91
Radius
0.84 Rsun
0.56 to 0.97
Age
4.68 Gyr
single adopted value
Distance
1017.2 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.84 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-933
0.84 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-933 b
Transit
◌
Discovery
2016
Period
14.20 days
Radius
2.46 R⊕
Mass
—
Eq. Temp
—
Kepler-933 b: A Super-Earth in a Distant System
Kepler-933 is a star located 3320 light-years away, and it hosts one planet. The star is estimated to be 4.68 billion years old, with a mass of 0.87 solar masses and a radius of 0.84 solar radii. Its temperature is 5350 K. The star's reported mass and radius estimates are smaller than the Sun's, and its reported temperature is cooler than the Sun's.
The planet Kepler-933 b was discovered in 2016 by the transit method, which detects the small dip in a star's brightness when a planet passes in front of it from our viewpoint. Repeated dips help establish the planet's orbital period, which is 14.2 days. Kepler-933 b is classified as a Super-Earth, a size class that reaches 2.5 times Earth's radius. Its radius is 2.46 Earth radii, which is larger than Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
13
Stellar refs
13
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 |
|---|---|---|---|---|---|---|---|---|
| 5125.2 | — | 0.97 | — | -0.23 | — | 1017.2 | Gaia DR2 | TICv8 |
| 5287 | 0.91 | 0.94 | — | -0.21 | — | 1017.2 | TICv8 | TICv8 |
| — | — | — | — | — | — | 1017.2 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5350 | 0.76 | 0.68 | — | — | — | 1017.2 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5362 | 0.74 | 0.69 | — | — | — | 1017.2 | Q1-Q16 KOI Table | TICv8 |
| 5169 | 0.87 | 0.56 | — | — | — | 1017.2 | Q1-Q8 KOI Table | TICv8 |
| 5169 | — | 0.62 | — | — | — | 1017.2 | Q1-Q6 KOI Table | TICv8 |
| 5371 | — | 0.94 | — | — | — | 1017.2 | Berger et al. 2018 | TICv8 |
| 5362 | 0.74 | 0.69 | — | — | — | 1017.2 | Q1-Q12 KOI Table | TICv8 |
| 5346 | 0.87 | 0.84 | 4.68 | — | — | 1017.2 | Morton et al. 2016 | TICv8 |
| 5169 | — | 0.56 | — | — | — | 1017.2 | Latham et al. 2005 | TICv8 |
| 5169 | 0.71 | 0.62 | — | — | — | 1017.2 | Batalha et al. 2013 | TICv8 |
| 5362 | 0.74 | 0.69 | — | — | — | 1017.2 | Q1-Q17 DR24 KOI Table | TICv8 |