Temperature
6681 K
5776.2 to 6681
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Stellar HostProfile
Kepler-1586
Unclassified star • 552.5 pc
Records
14
literature rows
Planets
1
system count
References
12
distinct source labels
TIC: TIC 273866337
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
1.45 Msun
0.99 to 1.45
Radius
1.75 Rsun
1.07 to 2.15
Age
1.70 Gyr
1.70 to 5.50
Distance
552.5 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.75 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
Kepler-1586
1.75 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1586 b
Transit
◌
Discovery
2016
Period
15.60 days
Radius
1.52 R⊕
Mass
—
Eq. Temp
—
Kepler-1586 b: A Super-Earth Around a Hot, Massive Star
Kepler-1586 is a star located 1800 light-years away, and it hosts one known planet. The star is 1.7 billion years old, has a mass of 1.45 solar masses, a radius of 1.75 solar radii, and a temperature of 6680 K. Its reported mass and radius estimates are both larger than the Sun's, and its reported temperature is hotter than the Sun's.
The planet, Kepler-1586 b, is classified as a Super-Earth. A Super-Earth is a size class that reaches 2.5 times Earth's radius, and Kepler-1586 b's reported radius estimate of 1.52 Earth radii is larger than Earth's. It 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. Repeated dips help establish orbital periods, and Kepler-1586 b completes one orbit every 15.6 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
14
Stellar refs
11
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 |
|---|---|---|---|---|---|---|---|---|
| 6254 | 1.11 | 1.71 | — | — | — | 552.5 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6130 | 0.99 | 1.14 | 5.50 | — | — | 552.5 | Fulton & Petigura 2018 | TICv8 |
| 5984 | — | 2.15 | — | — | — | 552.5 | Latham et al. 2005 | TICv8 |
| 6245 | 1.20 | 2.11 | — | — | — | 552.5 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6190.3 | 1.19 | 1.07 | — | 0.18 | — | 552.5 | TICv8 | TICv8 |
| — | — | — | — | — | — | 552.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6130 | — | 1.16 | — | — | — | 552.5 | Berger et al. 2018 | TICv8 |
| 6681 | 1.45 | 1.75 | 1.70 | — | — | 552.5 | Morton et al. 2016 | TICv8 |
| 5776.2 | — | 1.18 | — | 0.15 | — | 552.5 | Gaia DR2 | TICv8 |
| 6245 | 1.20 | 2.11 | — | — | — | 552.5 | Q1-Q12 KOI Table | TICv8 |
| 6245 | 1.20 | 2.11 | — | — | — | 552.5 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6254 | 1.11 | 1.71 | — | — | — | 552.5 | Q1-Q17 DR25 KOI Table | TICv8 |
| — | — | — | — | — | — | 552.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6245 | 1.20 | 2.11 | — | — | — | 552.5 | Q1-Q16 KOI Table | TICv8 |