Temperature
6168 K
5743 to 6185
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Stellar HostProfile
Kepler-1354
Unclassified star • 1119.5 pc
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
TIC: TIC 137096633
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
1.16 Msun
0.99 to 1.16
Radius
1.24 Rsun
1.02 to 1.38
Age
2.95 Gyr
2 to 2.95
Distance
1119.5 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.24 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1354
1.24 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1354 b
Transit
◌
Discovery
2016
Period
76.61 days
Radius
2.97 R⊕
Mass
—
Eq. Temp
—
Kepler-1354 and Its Neptune-Like Planet
Kepler-1354 is a star 3650 light-years away with one known planet. The star is 2.95 billion years old, has a mass of 1.16 solar masses, a radius of 1.24 solar radii, and a temperature of 6170 K. Its reported mass and radius estimates are larger than the Sun's, and its reported temperature is hotter than the Sun's.
The planet Kepler-1354 b was discovered in 2016 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. Repeated dips help establish orbital periods. Kepler-1354 b completes an orbit every 76.6 days. Its radius is 2.97 Earth radii, larger than Earth's. As a Neptune-like planet, it falls within the size class that reaches 4 times Earth's radius.
Provenance
Underlying measurements and references
Evidence Summary
Rows
11
Stellar refs
11
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 |
|---|---|---|---|---|---|---|---|---|
| 6170 | — | 1.34 | — | — | — | 1119.5 | Berger et al. 2018 | TICv8 |
| 6185 | 1.08 | 1.07 | 2 | — | — | 1119.5 | Q1-Q8 KOI Table | TICv8 |
| 6170 | 0.99 | 1.02 | — | — | — | 1119.5 | Q1-Q12 KOI Table | TICv8 |
| — | — | — | — | — | — | 1119.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6170 | 0.99 | 1.02 | — | — | — | 1119.5 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5931 | — | 1.07 | — | — | — | 1119.5 | Latham et al. 2005 | TICv8 |
| 6170 | 0.99 | 1.02 | — | — | — | 1119.5 | Q1-Q16 KOI Table | TICv8 |
| 5743 | — | 1.35 | — | 0.25 | — | 1119.5 | Gaia DR2 | TICv8 |
| 5843.0 | 1.05 | 1.38 | — | 0.30 | — | 1119.5 | TICv8 | TICv8 |
| 6173 | 0.99 | 1.03 | — | — | — | 1119.5 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6168 | 1.16 | 1.24 | 2.95 | — | — | 1119.5 | Morton et al. 2016 | TICv8 |