Temperature
6213 K
5596.7 to 6213
←Back to Stellar Hosts
Stellar HostProfile
Kepler-1592
Unclassified star • 1639.5 pc
Records
10
literature rows
Planets
1
system count
References
11
distinct source labels
TIC: TIC 138364751
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
1.18 Msun
0.91 to 1.18
Radius
1.28 Rsun
0.67 to 1.75
Age
2.69 Gyr
single adopted value
Distance
1639.5 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.28 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1592
1.28 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1592 b
Transit
◌
Discovery
2016
Period
3.06 days
Radius
1.54 R⊕
Mass
—
Eq. Temp
—
Kepler-1592 and Its Super-Earth
Kepler-1592 is a star 5350 light-years away with one known planet in orbit. The host star is 2.69 billion years old and has a mass of 1.18 solar masses, a radius of 1.28 solar radii, and a temperature of 6210 K. Its reported mass and radius estimates are larger than the Sun's, and its reported temperature is hotter than the Sun's.
The sole listed planet, Kepler-1592 b, was discovered in 2016 by the transit method, in which a planet passing in front of its star from our viewpoint causes a small dip in observed brightness. It is classified as a Super-Earth, a size class reaching 2.5 times Earth's radius. Its radius is 1.54 Earth radii, larger than Earth's, and it completes an orbit every 3.06 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
10
Stellar refs
10
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 |
|---|---|---|---|---|---|---|---|---|
| 5596.7 | — | 1.75 | — | 0.43 | — | 1639.5 | Gaia DR2 | TICv8 |
| 6020 | 0.91 | 0.83 | — | — | — | 1639.5 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6020 | 0.91 | 0.83 | — | — | — | 1639.5 | Q1-Q16 KOI Table | TICv8 |
| 6021 | 0.92 | 0.82 | — | — | — | 1639.5 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6097 | 1.15 | 1.61 | — | 0.51 | — | 1639.5 | TICv8 | TICv8 |
| 6031 | — | 1.61 | — | — | — | 1639.5 | Berger et al. 2018 | TICv8 |
| — | — | — | — | — | — | 1639.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6020 | 0.91 | 0.83 | — | — | — | 1639.5 | Q1-Q12 KOI Table | TICv8 |
| 6213 | 1.18 | 1.28 | 2.69 | — | — | 1639.5 | Morton et al. 2016 | TICv8 |
| 5809 | — | 0.67 | — | — | — | 1639.5 | Latham et al. 2005 | TICv8 |