Temperature
5635 K
5213.7 to 5668
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Stellar HostProfile
Kepler-1065
Unclassified star • 1122.5 pc
Records
18
literature rows
Planets
2
system count
References
14
distinct source labels
TIC: TIC 378012771
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
0.94 Msun
0.94 to 1.01
Radius
0.93 Rsun
0.85 to 1.00
Age
4.47 Gyr
single adopted value
Distance
1122.5 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.93 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1065
0.93 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-1065 b
Transit
◌
Discovery
2016
Period
3.61 days
Radius
3.73 R⊕
Mass
—
Eq. Temp
—
Kepler-1065 c
Transit
◌
Discovery
2016
Period
2.37 days
Radius
1.60 R⊕
Mass
—
Eq. Temp
—
Kepler-1065 and Its Two Planets
Kepler-1065 is a star located 3660 light-years away. It has a mass of 0.94 solar masses, a radius of 0.93 solar radii, a temperature of 5640 K, and an age of 4.47 billion years. Two planets are known to orbit this host.
Kepler-1065 c is a Super-Earth discovered by transit in 2016. It has a radius of 1.6 Earth radii and an orbital period of 2.37 days, the shortest orbital period among the listed planets. Kepler-1065 b is a Neptune-like world also discovered by transit in 2016. It has a radius of 3.73 Earth radii and an orbital period of 3.61 days, the longest orbital period among the listed planets. Both planets have reported radii larger than Earth's, with Kepler-1065 b having the largest radius among the listed planets and Kepler-1065 c the smallest.
Provenance
Underlying measurements and references
Evidence Summary
Rows
18
Stellar refs
13
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5668 | 0.96 | 0.87 | — | — | — | 1122.5 | Q1-Q12 KOI Table | TICv8 |
| 5213.7 | — | 1.00 | — | -0.18 | — | 1122.5 | Gaia DR2 | TICv8 |
| 5668 | 0.96 | 0.87 | — | — | — | 1122.5 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5443 | 0.94 | 0.85 | — | — | — | 1122.5 | Batalha et al. 2013 | TICv8 |
| 5668 | 0.96 | 0.87 | — | — | — | 1122.5 | Q1-Q16 KOI Table | TICv8 |
| 5443 | — | 0.85 | — | — | — | 1122.5 | Q1-Q6 KOI Table | TICv8 |
| 5663 | — | 0.97 | — | — | — | 1122.5 | Berger et al. 2018 | TICv8 |
| 5668 | 0.96 | 0.87 | — | — | — | 1122.5 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5443 | — | 0.89 | — | — | — | 1122.5 | Latham et al. 2005 | TICv8 |
| 5443 | 1.01 | 0.89 | — | — | — | 1122.5 | Q1-Q8 KOI Table | TICv8 |
| 5635 | 0.94 | 0.93 | 4.47 | — | — | 1122.5 | Morton et al. 2016 | TICv8 |
| 5668 | 0.96 | 0.87 | — | — | — | 1122.5 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5469 | 0.96 | 0.97 | — | -0.12 | — | 1122.5 | TICv8 | TICv8 |
| 5668 | 0.96 | 0.87 | — | — | — | 1122.5 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5668 | 0.96 | 0.87 | — | — | — | 1122.5 | Q1-Q16 KOI Table | TICv8 |
| — | — | — | — | — | — | 1122.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5668 | 0.96 | 0.87 | — | — | — | 1122.5 | Q1-Q12 KOI Table | TICv8 |
| — | — | — | — | — | — | 1122.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |