Temperature
6106 K
5999.0 to 6292
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Stellar HostProfile
Kepler-514
Unclassified star • 455.3 pc
Records
14
literature rows
Planets
1
system count
References
15
distinct source labels
TIC: TIC 405717552
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
1.28 Msun
1.10 to 1.29
Radius
1.44 Rsun
1.27 to 1.46
Age
2.69 Gyr
2.69 to 3.53
Distance
455.3 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.44 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-514
1.44 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-514 b
Transit
◌
Discovery
2016
Period
5.65 days
Radius
1.72 R⊕
Mass
—
Eq. Temp
—
Kepler-514 b: A Super-Earth Orbiting a Distant Star
Kepler-514 is a star located 1490 light-years away, and it hosts one known planet. The star is estimated to be 2.69 billion years old, with a reported mass estimate larger than the Sun's at 1.28 solar masses. Its reported radius estimate is also larger than the Sun's, at 1.44 solar radii, and its reported temperature of 6110 K is hotter than the Sun's.
The planet Kepler-514 b is a Super-Earth, a size class that reaches 2.5 times Earth's radius. Its reported radius estimate is 1.72 Earth radii, larger than Earth's. The planet was discovered in 2016 by the transit method, in which a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. Its orbital period is 5.65 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
14
Stellar refs
14
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 |
|---|---|---|---|---|---|---|---|---|
| 6292 | 1.10 | 1.27 | — | — | — | 455.3 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6085 | 1.29 | 1.46 | — | — | — | 455.3 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6106 | 1.28 | 1.44 | 2.69 | — | — | 455.3 | Morton et al. 2016 | TICv8 |
| 6050 | — | 1.28 | — | — | — | 455.3 | Batalha et al. 2013 | TICv8 |
| 6292 | 1.10 | 1.27 | — | — | — | 455.3 | Q1-Q12 KOI Table | TICv8 |
| 6292 | 1.10 | 1.27 | — | — | — | 455.3 | Q1-Q16 KOI Table | TICv8 |
| 6155 | — | 1.34 | — | — | — | 455.3 | Berger et al. 2018 | TICv8 |
| — | — | — | — | — | — | 455.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5999.0 | 1.11 | 1.39 | — | 0.35 | — | 455.3 | TICv8 | TICv8 |
| 6050 | — | 1.28 | — | — | — | 455.3 | Q1-Q6 KOI Table | TICv8 |
| 6282 | 1.13 | 1.28 | 3.53 | — | — | 455.3 | Q1-Q8 KOI Table | TICv8 |
| 6050 | — | 1.30 | — | — | — | 455.3 | Latham et al. 2005 | TICv8 |
| 6155 | 1.18 | 1.32 | 3.39 | — | — | 455.3 | Fulton & Petigura 2018 | TICv8 |
| 6218.0 | — | 1.27 | — | 0.34 | — | 455.3 | Gaia DR2 | TICv8 |