Temperature
5572.7 K
5572.7 to 6043
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Stellar HostProfile
Kepler-1745
Unclassified star • 996.1 pc
Records
10
literature rows
Planets
1
system count
References
11
distinct source labels
TIC: TIC 270525576
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 • System source: TICv8
Mass
0.98 Msun
0.98 to 1.06
Radius
1.08 Rsun
0.98 to 1.40
Luminosity
6.51e-3 log(Lsun)
single adopted value
Distance
996.1 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.08 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1745
1.08 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1745 b
Transit
◌
Discovery
2021
Period
3.02 days
Radius
1.93 R⊕
Mass
—
Eq. Temp
—
Kepler-1745: A Distant Star and Its Super-Earth
Kepler-1745 is a star located 3250 light-years from Earth. It has one known planet. The star's reported mass estimate is 0.98 solar masses, its reported radius estimate is 1.08 solar radii, and its reported temperature is 5570 K. Its mass estimate is smaller than the Sun's, while its radius estimate is larger than the Sun's and its temperature is cooler than the Sun's.
The planet Kepler-1745 b is classified as a Super-Earth, a size class that reaches 2.5 times Earth's radius. It 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. Kepler-1745 b orbits its star every 3.02 days and has a radius of 1.93 Earth radii, larger than Earth's.
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 |
|---|---|---|---|---|---|---|---|---|
| 6043 | 1.06 | 1.00 | — | — | — | 996.1 | Q1-Q12 KOI Table | TICv8 |
| 5778 | — | 1 | — | — | — | 996.1 | Q1-Q6 KOI Table | TICv8 |
| 5778 | — | 0.99 | — | — | — | 996.1 | Latham et al. 2005 | TICv8 |
| 6043 | 1.06 | 1.00 | — | — | — | 996.1 | Q1-Q16 KOI Table | TICv8 |
| 6013 | 1.03 | 0.98 | 2.10 | — | — | 996.1 | Q1-Q8 KOI Table | TICv8 |
| — | — | — | — | — | — | 996.1 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5611 | 0.99 | 1.40 | — | — | — | 996.1 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5572.7 | 0.98 | 1.08 | — | 6.51e-3 | — | 996.1 | TICv8 | TICv8 |
| 5778 | — | 1 | — | — | — | 996.1 | Batalha et al. 2013 | TICv8 |
| 6043 | 1.06 | 1.00 | — | — | — | 996.1 | Q1-Q17 DR24 KOI Table | TICv8 |