Temperature
6014 K
5596.7 to 6049
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Stellar HostProfile
Kepler-524
Unclassified star • 1058.2 pc
Records
20
literature rows
Planets
2
system count
References
15
distinct source labels
TIC: TIC 27914389
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
1.09 Msun
1.03 to 1.09
Radius
1.10 Rsun
1.08 to 1.68
Age
3.02 Gyr
3.02 to 7.76
Distance
1058.2 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.10 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-524
1.10 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-524 b
Transit
◌
Discovery
2016
Period
7.97 days
Radius
1.91 R⊕
Mass
—
Eq. Temp
—
Kepler-524 c
Transit
◌
Discovery
2016
Period
1.89 days
Radius
0.96 R⊕
Mass
—
Eq. Temp
—
Kepler-524 and Its Two Planets
Kepler-524 is a star located 3450 light-years away. It is 3.02 billion years old and has a mass of 1.09 solar masses, a radius of 1.1 solar radii, and a temperature of 6010 K. Its reported mass and radius estimates are larger than the Sun's, and its reported temperature is hotter than the Sun's. Two planets are known to orbit this host.
Both planets were discovered by transit in 2016. Kepler-524 b is a Super-Earth with a radius of 1.91 Earth radii, larger than Earth's, and an orbital period of 7.97 days. Kepler-524 c is a Sub-Earth with a radius of 0.96 Earth radii and an orbital period of 1.89 days. Among the listed planets, Kepler-524 c has the shortest year and the smallest radius by reported estimates, while Kepler-524 b has the longest year and the largest radius by reported estimates.
Provenance
Underlying measurements and references
Evidence Summary
Rows
20
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 |
|---|---|---|---|---|---|---|---|---|
| 6049 | 1.03 | 1.25 | — | — | — | 1058.2 | Q1-Q16 KOI Table | TICv8 |
| 5973 | 1.04 | 1.08 | — | — | — | 1058.2 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5749 | — | 1.31 | — | — | — | 1058.2 | Latham et al. 2005 | TICv8 |
| 6024 | 1.03 | 1.25 | 6.40 | — | — | 1058.2 | Q1-Q8 KOI Table | TICv8 |
| 5842.5 | 1.05 | 1.62 | — | 0.44 | — | 1058.2 | TICv8 | TICv8 |
| 6049 | 1.03 | 1.25 | — | — | — | 1058.2 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5973 | 1.04 | 1.08 | — | — | — | 1058.2 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6049 | 1.03 | 1.25 | — | — | — | 1058.2 | Q1-Q12 KOI Table | TICv8 |
| 5749 | — | 1.24 | — | — | — | 1058.2 | Q1-Q6 KOI Table | TICv8 |
| 5838 | 1.05 | 1.58 | 7.76 | — | — | 1058.2 | Fulton & Petigura 2018 | TICv8 |
| 5749 | — | 1.24 | — | — | — | 1058.2 | Batalha et al. 2013 | TICv8 |
| 6024 | 1.03 | 1.25 | 6.40 | — | — | 1058.2 | Q1-Q8 KOI Table | TICv8 |
| 6049 | 1.03 | 1.25 | — | — | — | 1058.2 | Q1-Q16 KOI Table | TICv8 |
| 6049 | 1.03 | 1.25 | — | — | — | 1058.2 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6014 | 1.09 | 1.10 | 3.02 | — | — | 1058.2 | Morton et al. 2016 | TICv8 |
| 5596.7 | — | 1.68 | — | 0.40 | — | 1058.2 | Gaia DR2 | TICv8 |
| 5838 | — | 1.61 | — | — | — | 1058.2 | Berger et al. 2018 | TICv8 |
| 6049 | 1.03 | 1.25 | — | — | — | 1058.2 | Q1-Q12 KOI Table | TICv8 |
| — | — | — | — | — | — | 1058.2 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| — | — | — | — | — | — | 1058.2 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |