Temperature
5694 K
5481.4 to 5876
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Stellar HostProfile
Kepler-767
Unclassified star • 2251.0 pc
Records
13
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 137220387
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
0.96 Msun
0.96 to 1.03
Radius
0.94 Rsun
0.55 to 1.92
Age
4.07 Gyr
0.40 to 4.07
Distance
2251.0 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.94 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-767
0.94 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-767 b
Transit
◌
Discovery
2016
Period
161.5 days
Radius
6.64 R⊕
Mass
—
Eq. Temp
—
Kepler-767 b: A Distant Jupiter-like World
Kepler-767 is a star 7340 light-years away with one known planet. The host star has a mass of 0.96 solar masses and a radius of 0.94 solar radii. Its temperature is 5690 K, and its age is 4.07 billion years.
The planet Kepler-767 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. Kepler-767 b completes an orbit every 162 days, and its radius is 6.64 Earth radii. This reported radius estimate is larger than Earth's. With a radius exceeding four times Earth's, the planet is classified as Jupiter-like.
Provenance
Underlying measurements and references
Evidence Summary
Rows
13
Stellar refs
13
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 |
|---|---|---|---|---|---|---|---|---|
| 5870 | 0.96 | 0.87 | — | — | — | 2251.0 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5870 | 0.96 | 0.87 | — | — | — | 2251.0 | Q1-Q12 KOI Table | TICv8 |
| 5665 | — | 0.83 | — | — | — | 2251.0 | Q1-Q6 KOI Table | TICv8 |
| 5779 | — | 1.80 | — | — | — | 2251.0 | Berger et al. 2018 | TICv8 |
| 5686 | 1.01 | 1.78 | — | 0.48 | — | 2251.0 | TICv8 | TICv8 |
| 5870 | 0.96 | 0.87 | — | — | — | 2251.0 | Q1-Q16 KOI Table | TICv8 |
| 5481.4 | — | 1.92 | — | 0.48 | — | 2251.0 | Gaia DR2 | TICv8 |
| 5694 | 0.96 | 0.94 | 4.07 | — | — | 2251.0 | Morton et al. 2016 | TICv8 |
| — | — | — | — | — | — | 2251.0 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5778 | 1.03 | 1.21 | — | — | — | 2251.0 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5665 | — | 0.55 | — | — | — | 2251.0 | Latham et al. 2005 | TICv8 |
| 5876 | 1.00 | 0.89 | 0.40 | — | — | 2251.0 | Q1-Q8 KOI Table | TICv8 |
| 5665 | — | 0.83 | — | — | — | 2251.0 | Batalha et al. 2013 | TICv8 |