Temperature
5301 K
5139.8 to 5482
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Stellar HostProfile
Kepler-1045
Unclassified star • 942.5 pc
Records
13
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 164670756
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
0.86 Msun
0.78 to 0.90
Radius
0.82 Rsun
0.68 to 0.85
Age
4.47 Gyr
0.70 to 4.47
Distance
942.5 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.82 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1045
0.82 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1045 b
Transit
◌
Discovery
2016
Period
26.41 days
Radius
2.69 R⊕
Mass
—
Eq. Temp
—
Kepler-1045 and Its Neptune-like Planet
Kepler-1045 is a star located 3070 light-years away, and it has one known planet. The host star is estimated to be 4.47 billion years old, with a mass of 0.86 solar masses, a radius of 0.82 solar radii, and a temperature of 5300 K. Its reported mass and radius estimates are smaller than the Sun's, and its reported temperature is cooler than the Sun's.
The planet Kepler-1045 b was discovered by transit 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-1045 b is Neptune-like, a size class that reaches 4 times Earth's radius. It orbits every 26.4 days and has a radius of 2.69 Earth radii, which is larger than Earth's.
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 |
|---|---|---|---|---|---|---|---|---|
| 5250 | 0.90 | 0.82 | — | -0.33 | — | 942.5 | TICv8 | TICv8 |
| 5448 | 0.81 | 0.73 | — | — | — | 942.5 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5247 | 0.78 | 0.68 | — | — | — | 942.5 | Batalha et al. 2013 | TICv8 |
| 5443 | 0.80 | 0.74 | — | — | — | 942.5 | Q1-Q16 KOI Table | TICv8 |
| 5482 | 0.89 | 0.79 | 0.70 | — | — | 942.5 | Q1-Q8 KOI Table | TICv8 |
| 5301 | 0.86 | 0.82 | 4.47 | — | — | 942.5 | Morton et al. 2016 | TICv8 |
| 5247 | — | 0.75 | — | — | — | 942.5 | Latham et al. 2005 | TICv8 |
| 5247 | — | 0.68 | — | — | — | 942.5 | Q1-Q6 KOI Table | TICv8 |
| 5443 | 0.80 | 0.74 | — | — | — | 942.5 | Q1-Q12 KOI Table | TICv8 |
| 5139.8 | — | 0.85 | — | -0.34 | — | 942.5 | Gaia DR2 | TICv8 |
| 5443 | 0.80 | 0.74 | — | — | — | 942.5 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5444 | — | 0.80 | — | — | — | 942.5 | Berger et al. 2018 | TICv8 |
| — | — | — | — | — | — | 942.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |