Temperature
6005 K
5849.8 to 6302
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Stellar HostProfile
Kepler-1613
Unclassified star • 1508.3 pc
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
TIC: TIC 159180076
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
1.08 Msun
1.06 to 1.21
Radius
1.12 Rsun
1.12 to 2.03
Age
3.55 Gyr
3.55 to 4.68
Distance
1508.3 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.12 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
Kepler-1613
1.12 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1613 b
Transit
◌
Discovery
2016
Period
1.52 days
Radius
2.08 R⊕
Mass
—
Eq. Temp
—
Kepler-1613 and Its Super-Earth
Kepler-1613 is a star 4920 light-years away with one known planet in orbit. The host star is 3.55 billion years old and has a mass of 1.08 solar masses, a radius of 1.12 solar radii, and a temperature of 6010 K. Its reported mass estimate is larger than the Sun's, and its reported temperature is hotter than the Sun's.
The planet Kepler-1613 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; repeated dips help establish orbital periods. Kepler-1613 b is classified as a Super-Earth, a size class reaching 2.5 times Earth's radius, and its reported radius estimate is 2.08 Earth radii, larger than Earth's. It completes an orbit every 1.52 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
11
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 |
|---|---|---|---|---|---|---|---|---|
| 6063 | — | 1.30 | — | — | — | 1508.3 | Latham et al. 2005 | TICv8 |
| — | — | — | — | — | — | 1508.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5849.8 | — | 2.03 | — | 0.64 | — | 1508.3 | Gaia DR2 | TICv8 |
| 6302 | 1.06 | 1.27 | — | — | — | 1508.3 | Q1-Q16 KOI Table | TICv8 |
| 6302 | 1.06 | 1.27 | — | — | — | 1508.3 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6302 | 1.06 | 1.27 | — | — | — | 1508.3 | Q1-Q12 KOI Table | TICv8 |
| 6302 | 1.06 | 1.27 | — | — | — | 1508.3 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6037 | — | 1.99 | — | — | — | 1508.3 | Berger et al. 2018 | TICv8 |
| 6014 | 1.11 | 1.92 | — | 0.64 | — | 1508.3 | TICv8 | TICv8 |
| 6037 | 1.21 | 1.93 | 4.68 | — | — | 1508.3 | Fulton & Petigura 2018 | TICv8 |
| 6005 | 1.08 | 1.12 | 3.55 | — | — | 1508.3 | Morton et al. 2016 | TICv8 |