Temperature
5172.8 K
5172.8 to 5419
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Stellar HostProfile
Kepler-1767
Unclassified star โข 820.5 pc
Records
10
literature rows
Planets
1
system count
References
11
distinct source labels
TIC: TIC 270619473
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: TICv8 โข System source: TICv8
Mass
0.88 Msun
0.74 to 0.89
Radius
0.70 Rsun
0.58 to 0.83
Luminosity
-0.50 log(Lsun)
single adopted value
Distance
820.5 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.70 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
Kepler-1767
0.70 Rโ
System Layout
Known planets
1 planets linked to this host
Kepler-1767 b
Transit
โ
Discovery
2021
Period
59.66 days
Radius
3.01 Rโ
Mass
โ
Eq. Temp
โ
Kepler-1767 b: A Neptune-Like World Around a Cool Dwarf Star
Kepler-1767 is a star located 2680 light-years away. It has a reported mass of 0.88 solar masses and a reported radius of 0.698 solar radii. Its reported temperature is 5170 K. The star's reported mass estimate is smaller than the Sun's, its reported radius estimate is smaller than the Sun's, and its reported temperature is cooler than the Sun's. One planet is known to orbit this star.
That planet, Kepler-1767 b, was discovered in 2021 by the transit method, in which a planet passes in front of its star from our viewpoint and causes a small dip in observed brightness. It is classified as Neptune-like, a size class that reaches up to 4 times Earth's radius. Kepler-1767 b has a reported radius of 3.01 Earth radii, larger than Earth's, and an orbital period of 59.7 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
10
Stellar refs
10
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositystable
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5349 | 0.75 | 0.69 | โ | โ | โ | 820.5 | Q1-Q16 KOI Table | TICv8 |
| 5349 | 0.75 | 0.69 | โ | โ | โ | 820.5 | Q1-Q12 KOI Table | TICv8 |
| 5243 | 0.89 | 0.83 | โ | โ | โ | 820.5 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5419 | 0.88 | 0.77 | 0.60 | โ | โ | 820.5 | Q1-Q8 KOI Table | TICv8 |
| 5189 | โ | 0.65 | โ | โ | โ | 820.5 | Q1-Q6 KOI Table | TICv8 |
| 5172.8 | 0.88 | 0.70 | โ | -0.50 | โ | 820.5 | TICv8 | TICv8 |
| 5349 | 0.75 | 0.69 | โ | โ | โ | 820.5 | Q1-Q17 DR24 KOI Table | TICv8 |
| โ | โ | โ | โ | โ | โ | 820.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5189 | โ | 0.58 | โ | โ | โ | 820.5 | Latham et al. 2005 | TICv8 |
| 5189 | 0.74 | 0.65 | โ | โ | โ | 820.5 | Batalha et al. 2013 | TICv8 |