Temperature
5533 K
5413 to 5650
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Stellar HostProfile
Kepler-1036
Unclassified star • 489.4 pc
Records
14
literature rows
Planets
1
system count
References
15
distinct source labels
TIC: TIC 27396869
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
0.95 Msun
0.88 to 0.97
Radius
0.89 Rsun
0.82 to 0.89
Age
3.24 Gyr
0.80 to 3.24
Distance
489.4 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.89 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1036
0.89 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1036 b
Transit
◌
Discovery
2016
Period
122.9 days
Radius
3.01 R⊕
Mass
—
Eq. Temp
—
Kepler-1036 and Its Neptune-Like Planet
Kepler-1036 is a star 1600 light-years away with one known planet. The host star is 3.24 billion years old, has 0.95 solar masses and 0.89 solar radii, and a temperature of 5530 K. Its mass and radius are smaller than the Sun's, and it is cooler than the Sun.
The planet Kepler-1036 b is Neptune-like and was discovered by transit in 2016. It orbits every 123 days and has a radius of 3.01 Earth radii, larger than Earth's. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. Repeated dips help establish orbital periods.
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 |
|---|---|---|---|---|---|---|---|---|
| 5476 | — | 0.86 | — | — | — | 489.4 | Berger et al. 2018 | TICv8 |
| 5431 | — | 0.85 | — | — | — | 489.4 | Q1-Q6 KOI Table | TICv8 |
| 5476 | 0.96 | 0.86 | 1 | — | — | 489.4 | Fulton & Petigura 2018 | TICv8 |
| 5433 | 0.95 | 0.89 | — | -0.20 | — | 489.4 | TICv8 | TICv8 |
| 5650 | 0.97 | 0.87 | — | — | — | 489.4 | Q1-Q16 KOI Table | TICv8 |
| — | — | — | — | — | — | 489.4 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5431 | — | 0.84 | — | — | — | 489.4 | Latham et al. 2005 | TICv8 |
| 5650 | 0.97 | 0.87 | — | — | — | 489.4 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5413 | 0.88 | 0.86 | — | — | — | 489.4 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5431 | 0.95 | 0.85 | — | — | — | 489.4 | Batalha et al. 2013 | TICv8 |
| 5419 | — | 0.87 | — | -0.23 | — | 489.4 | Gaia DR2 | TICv8 |
| 5533 | 0.95 | 0.89 | 3.24 | — | — | 489.4 | Morton et al. 2016 | TICv8 |
| 5650 | 0.97 | 0.87 | — | — | — | 489.4 | Q1-Q12 KOI Table | TICv8 |
| 5590 | 0.92 | 0.82 | 0.80 | — | — | 489.4 | Q1-Q8 KOI Table | TICv8 |