Temperature
5735 K
5682 to 5905
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Stellar HostProfile
Kepler-565
Unclassified star
Records
10
literature rows
Planets
1
system count
References
11
distinct source labels
TIC: TIC 164556745
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
0.98 Msun
0.93 to 1.01
Radius
0.95 Rsun
0.81 to 0.95
Age
4.07 Gyr
0.30 to 4.07
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.95 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-565
0.95 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-565 b
Transit
◌
Discovery
2016
Period
4.24 days
Radius
3.64 R⊕
Mass
—
Eq. Temp
—
Kepler-565 and Its Neptune-Like Planet
Kepler-565 is a star with a single known planet. The host star is 4.07 billion years old and has a mass of 0.98 solar masses, a radius of 0.95 solar radii, and a temperature of 5740 K. Solar mass and radius compare stellar mass and radius with the Sun, so Kepler-565 is slightly less massive and slightly smaller than the Sun.
The planet Kepler-565 b 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. Repeated dips help establish orbital periods, and Kepler-565 b completes one orbit every 4.24 days. Its radius is 3.64 Earth radii, and its reported radius estimate is larger than Earth's. Earth radii compare radius, not volume. As a Neptune-like planet, it falls within the size class that reaches up to 4 times Earth's radius, based on radius rather than composition.
Provenance
Underlying measurements and references
Evidence Summary
Rows
10
Stellar refs
10
System refs
1
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5905 | 1.01 | 0.90 | 0.30 | — | — | — | Q1-Q8 KOI Table | TICv8 |
| 5682 | — | 0.87 | — | — | — | — | Latham et al. 2005 | TICv8 |
| — | — | — | — | — | — | — | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5735 | 0.98 | 0.95 | 4.07 | — | — | — | Morton et al. 2016 | TICv8 |
| 5682 | — | 0.81 | — | — | — | — | Q1-Q6 KOI Table | TICv8 |
| 5876 | 0.93 | 0.84 | — | — | — | — | Q1-Q16 KOI Table | TICv8 |
| 5876 | 0.93 | 0.84 | — | — | — | — | Q1-Q12 KOI Table | TICv8 |
| 5873 | 0.93 | 0.84 | — | — | — | — | Q1-Q17 DR25 KOI Table | TICv8 |
| 5682 | — | 0.81 | — | — | — | — | Batalha et al. 2013 | TICv8 |
| 5876 | 0.93 | 0.84 | — | — | — | — | Q1-Q17 DR24 KOI Table | TICv8 |