Temperature
5322 K
5033 to 5423
←Back to Stellar Hosts
Stellar HostProfile
Kepler-760
Unclassified star • 792.3 pc
Records
20
literature rows
Planets
2
system count
References
15
distinct source labels
TIC: TIC 158494681
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
0.89 Msun
0.81 to 1.02
Radius
0.85 Rsun
0.85 to 1.17
Age
4.57 Gyr
2.63 to 4.57
Distance
792.3 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.85 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-760
0.85 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-760 b
Transit
◌
Discovery
2016
Period
8.70 days
Radius
3.06 R⊕
Mass
—
Eq. Temp
—
Kepler-760 c
Transit
◌
Discovery
2016
Period
2.47 days
Radius
1.48 R⊕
Mass
—
Eq. Temp
—
Kepler-760 and Its Two Planets
Kepler-760 is a star 2580 light-years away with two planets orbiting it. The host star is 4.57 billion years old, has a mass of 0.89 solar masses, a radius of 0.85 solar radii, and a temperature of 5320 K. Its mass, radius, and temperature are all smaller or cooler than the Sun's.
The two planets were both discovered by transit in 2016. Kepler-760 b is a Neptune-like planet with an orbital period of 8.7 days and a radius of 3.06 Earth radii. Kepler-760 c is Earth-like, with an orbital period of 2.47 days and a radius of 1.48 Earth radii. Both planets are larger than Earth, and among the listed planets Kepler-760 c has the shortest year and smallest radius, while Kepler-760 b has the longest year and largest radius.
Provenance
Underlying measurements and references
Evidence Summary
Rows
20
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 |
|---|---|---|---|---|---|---|---|---|
| 5074 | 0.81 | 0.86 | — | — | — | 792.3 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5033 | — | 0.93 | — | -0.30 | — | 792.3 | Gaia DR2 | TICv8 |
| 5221 | 0.92 | 1.11 | — | — | — | 792.3 | Batalha et al. 2013 | TICv8 |
| 5221 | — | 1.11 | — | — | — | 792.3 | Q1-Q6 KOI Table | TICv8 |
| 5221 | — | 1.17 | — | — | — | 792.3 | Latham et al. 2005 | TICv8 |
| — | — | — | — | — | — | 792.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5221 | 1.02 | 1.17 | — | — | — | 792.3 | Q1-Q8 KOI Table | TICv8 |
| 5423 | 0.92 | 1.12 | — | — | — | 792.3 | Q1-Q16 KOI Table | TICv8 |
| 5423 | 0.92 | 1.12 | — | — | — | 792.3 | Q1-Q12 KOI Table | TICv8 |
| 5423 | 0.92 | 1.12 | — | — | — | 792.3 | Q1-Q17 DR24 KOI Table | TICv8 |
| — | — | — | — | — | — | 792.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5162 | 0.87 | 0.91 | — | -0.28 | — | 792.3 | TICv8 | TICv8 |
| 5239 | — | 0.86 | — | — | — | 792.3 | Berger et al. 2018 | TICv8 |
| 5423 | 0.92 | 1.12 | — | — | — | 792.3 | Q1-Q16 KOI Table | TICv8 |
| 5423 | 0.92 | 1.12 | — | — | — | 792.3 | Q1-Q12 KOI Table | TICv8 |
| 5074 | 0.81 | 0.86 | — | — | — | 792.3 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5221 | 1.02 | 1.17 | — | — | — | 792.3 | Q1-Q8 KOI Table | TICv8 |
| 5423 | 0.92 | 1.12 | — | — | — | 792.3 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5322 | 0.89 | 0.85 | 4.57 | — | — | 792.3 | Morton et al. 2016 | TICv8 |
| 5239 | 0.93 | 0.85 | 2.63 | — | — | 792.3 | Fulton & Petigura 2018 | TICv8 |