Temperature
5592 K
5429 to 5614
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Stellar HostProfile
Kepler-1067
Unclassified star • 667.7 pc
Records
19
literature rows
Planets
2
system count
References
15
distinct source labels
TIC: TIC 351910733
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 1.01
Radius
0.93 Rsun
0.51 to 0.94
Age
4.79 Gyr
0.50 to 4.79
Distance
667.7 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-1067
0.93 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-1067 b
Transit
◌
Discovery
2016
Period
0.76 days
Radius
0.80 R⊕
Mass
—
Eq. Temp
—
Kepler-1067 c
Transit
◌
Discovery
2021
Period
5.43 days
Radius
1.75 R⊕
Mass
—
Eq. Temp
—
Kepler-1067: A Cooler, Less Massive Star with Two Small Planets
Kepler-1067 is a star located 2180 light-years away, with two planets known to orbit it. The host star is 4.79 billion years old, has a mass of 0.95 solar masses, a radius of 0.93 solar radii, and a temperature of 5590 K. Its mass is smaller than the Sun's, and its temperature is cooler than the Sun's.
The two planets were both found by the transit method, which detects the slight dimming caused when a planet crosses in front of its star. Kepler-1067 b was discovered in 2016 and is classified as a Sub-Earth, a size class for planets smaller than Earth. It has a radius of 0.8 Earth radii, smaller than Earth's, and an orbital period of 0.762 days. Kepler-1067 c was discovered in 2021 and is a Super-Earth, a class reaching up to 2.5 times Earth's radius. It has a radius of 1.75 Earth radii, larger than Earth's, and an orbital period of 5.43 days. Among the listed planets, Kepler-1067 b has the shortest year and the smallest radius, while Kepler-1067 c has the longest year and the largest 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 |
|---|---|---|---|---|---|---|---|---|
| 5429 | — | 0.77 | — | — | — | 667.7 | Q1-Q6 KOI Table | TICv8 |
| 5592 | 0.95 | 0.93 | 4.79 | — | — | 667.7 | Morton et al. 2016 | TICv8 |
| 5439.2 | — | 0.94 | — | -0.16 | — | 667.7 | Gaia DR2 | TICv8 |
| 5584 | — | 0.91 | — | — | — | 667.7 | Berger et al. 2018 | TICv8 |
| 5594 | 0.98 | 0.93 | — | — | — | 667.7 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5614 | 0.91 | 0.83 | — | — | — | 667.7 | Q1-Q16 KOI Table | TICv8 |
| 5429 | 0.88 | 0.77 | — | — | — | 667.7 | Batalha et al. 2013 | TICv8 |
| — | — | — | — | — | — | 667.7 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5429 | — | 0.51 | — | — | — | 667.7 | Latham et al. 2005 | TICv8 |
| 5614 | 0.91 | 0.83 | — | — | — | 667.7 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5614 | 0.91 | 0.83 | — | — | — | 667.7 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5614 | 0.91 | 0.83 | — | — | — | 667.7 | Q1-Q12 KOI Table | TICv8 |
| 5614 | 0.91 | 0.83 | — | — | — | 667.7 | Q1-Q16 KOI Table | TICv8 |
| 5594 | 0.98 | 0.93 | — | — | — | 667.7 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5584 | 1.01 | 0.90 | 0.81 | — | — | 667.7 | Fulton & Petigura 2018 | TICv8 |
| 5461 | 0.95 | 0.94 | — | -0.15 | — | 667.7 | TICv8 | TICv8 |
| 5597 | 0.92 | 0.82 | 0.50 | — | — | 667.7 | Q1-Q8 KOI Table | TICv8 |
| 5614 | 0.91 | 0.83 | — | — | — | 667.7 | Q1-Q12 KOI Table | TICv8 |
| — | — | — | — | — | — | 667.7 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |