Temperature
6112 K
5919.6 to 6141
Unclassified star • 623.9 pc
Records
20
literature rows
Planets
2
system count
References
14
distinct source labels
Approximate color
from effective temperature
Canonical Summary
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
Temperature
6112 K
5919.6 to 6141
Mass
1.10 Msun
1.03 to 1.14
Radius
1.09 Rsun
1.03 to 1.67
Age
2.04 Gyr
0.93 to 6.46
Distance
623.9 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 1.09 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-520
1.09 R☉
System Layout
2 planets linked to this host
Transit
Discovery
2016
Period
19.67 days
Radius
1.66 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2016
Period
5.21 days
Radius
1.07 R⊕
Mass
—
Eq. Temp
—
Kepler-520 is a star located 2030 light-years away, and two planets have been found orbiting it. The host is 2.04 billion years old, with a mass of 1.1 solar masses, a radius of 1.09 solar radii, and a temperature of 6110 K. Its reported mass and radius estimates are larger than the Sun's, and its reported temperature is hotter than the Sun's.
Both planets were discovered by transit, the small dip in a star's brightness when a planet crosses in front of it, and both were reported in 2016. Kepler-520 b is classified as a Super-Earth, a size class reaching 2.5 times Earth's radius, and has a radius of 1.66 Earth radii, larger than Earth's. Its orbital period is 19.7 days, the longest year among the listed planets. Kepler-520 c is classified as Earth-like, a size class staying within 1.5 times Earth's radius, and has a radius of 1.07 Earth radii, larger than Earth's yet the smallest among the listed planets. Its orbital period is 5.21 days, the shortest year among the listed planets.
Provenance
Evidence Summary
Rows
20
Stellar refs
13
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | 623.9 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6141 | — | 1.09 | — | — | — | 623.9 | Q1-Q6 KOI Table | TICv8 |
| 6023 | 1.03 | 1.03 | — | — | — | 623.9 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6009 | 1.08 | 1.67 | 6.46 | — | — | 623.9 | Fulton & Petigura 2018 | TICv8 |
| 6108 | 1.13 | 1.03 | — | — | — | 623.9 | Q1-Q12 KOI Table | TICv8 |
| 6108 | 1.13 | 1.03 | — | — | — | 623.9 | Q1-Q16 KOI Table | TICv8 |
| 6108 | 1.13 | 1.03 | — | — | — | 623.9 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6108 | 1.13 | 1.03 | — | — | — | 623.9 | Q1-Q16 KOI Table | TICv8 |
| 6141 | 1.14 | 1.09 | 0.93 | — | — | 623.9 | Q1-Q8 KOI Table | TICv8 |
| 6108 | 1.13 | 1.03 | — | — | — | 623.9 | Q1-Q12 KOI Table | TICv8 |
| — | — | — | — | — | — | 623.9 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6141 | 1.14 | 1.09 | 0.93 | — | — | 623.9 | Q1-Q8 KOI Table | TICv8 |
| 6141 | — | 1.09 | — | — | — | 623.9 | Q1-Q6 KOI Table | TICv8 |
| 6081 | — | 1.11 | — | — | — | 623.9 | Latham et al. 2005 | TICv8 |
| 6141 | 1.14 | 1.09 | — | — | — | 623.9 | Batalha et al. 2013 | TICv8 |
| 6112 | 1.10 | 1.09 | 2.04 | — | — | 623.9 | Morton et al. 2016 | TICv8 |
| 6023 | 1.03 | 1.03 | — | — | — | 623.9 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6028 | — | 1.65 | — | 0.51 | — | 623.9 | Gaia DR2 | TICv8 |
| 5919.6 | — | — | — | — | — | 623.9 | TICv8 | TICv8 |
| 6108 | 1.13 | 1.03 | — | — | — | 623.9 | Q1-Q17 DR24 KOI Table | TICv8 |