Temperature
5183 K
4898.5 to 5211
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Stellar HostProfile
Kepler-1164
Unclassified star • 431.6 pc
Records
19
literature rows
Planets
1
system count
References
15
distinct source labels
TIC: TIC 121275496
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
0.85 Msun
0.77 to 0.88
Radius
0.79 Rsun
0.76 to 0.90
Age
3.63 Gyr
1.41 to 13.90
Distance
431.6 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.79 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1164
0.79 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1164 b
Transit
◌
Discovery
2016
Period
3.98 days
Radius
1.12 R⊕
Mass
—
Eq. Temp
—
Kepler-1164 and Its Planet
Kepler-1164 is a star located 1410 light-years away, with one planet known to orbit it. The star's reported mass estimate is smaller than the Sun's, at 0.85 solar masses, and its reported radius estimate is also smaller than the Sun's, at 0.79 solar radii. Its temperature of 5180 K is cooler than the Sun's, and it is 3.63 billion years old.
The single planet, Kepler-1164 b, was discovered by the transit method in 2016. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness, and repeated dips help establish orbital periods. Kepler-1164 b completes an orbit every 3.98 days, and its radius of 1.12 Earth radii makes it larger than Earth. That radius places it within the Earth-like size class, which covers planets up to 1.5 times Earth's radius.
Provenance
Underlying measurements and references
Evidence Summary
Rows
19
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 |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | 431.6 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| — | — | — | — | — | — | 431.6 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5143 | 0.80 | 0.78 | — | — | — | 431.6 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5211 | 0.80 | 0.83 | — | — | — | 431.6 | Q1-Q12 KOI Table | TICv8 |
| 5179 | 0.77 | 0.79 | 13.90 | — | — | 431.6 | Q1-Q8 KOI Table | TICv8 |
| 5052 | — | 0.81 | — | — | — | 431.6 | Q1-Q6 KOI Table | TICv8 |
| 5052 | — | 0.90 | — | — | — | 431.6 | Latham et al. 2005 | TICv8 |
| 5197 | 0.88 | 0.78 | — | -0.40 | — | 431.6 | TICv8 | TICv8 |
| 5052 | — | 0.81 | — | — | — | 431.6 | Q1-Q6 KOI Table | TICv8 |
| 5183 | 0.85 | 0.79 | 3.63 | — | — | 431.6 | Morton et al. 2016 | TICv8 |
| 5211 | 0.80 | 0.83 | — | — | — | 431.6 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5211 | 0.80 | 0.83 | — | — | — | 431.6 | Q1-Q12 KOI Table | TICv8 |
| 5179 | 0.77 | 0.79 | 13.90 | — | — | 431.6 | Q1-Q8 KOI Table | TICv8 |
| 5176 | — | 0.77 | — | — | — | 431.6 | Berger et al. 2018 | TICv8 |
| 5052 | 0.79 | 0.81 | — | — | — | 431.6 | Batalha et al. 2013 | TICv8 |
| 5176 | 0.84 | 0.76 | 1.41 | — | — | 431.6 | Fulton & Petigura 2018 | TICv8 |
| 4898.5 | — | 0.85 | — | -0.43 | — | 431.6 | Gaia DR2 | TICv8 |
| 5211 | 0.80 | 0.83 | — | — | — | 431.6 | Q1-Q16 KOI Table | TICv8 |
| 5211 | 0.80 | 0.83 | — | — | — | 431.6 | Q1-Q16 KOI Table | TICv8 |