Temperature
6214 K
5734 to 6269
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Stellar HostProfile
Kepler-1475
Unclassified star • 1568.4 pc
Records
10
literature rows
Planets
1
system count
References
11
distinct source labels
TIC: TIC 271970692
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
1.18 Msun
1.02 to 1.18
Radius
1.28 Rsun
0.80 to 1.28
Age
2.82 Gyr
single adopted value
Distance
1568.4 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.28 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1475
1.28 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1475 b
Transit
◌
Discovery
2016
Period
82.18 days
Radius
2.92 R⊕
Mass
—
Eq. Temp
—
Kepler-1475 and Its Neptune-Like Planet
Kepler-1475 is a star located 5120 light-years away, and it hosts one known planet. The star is estimated to be 2.82 billion years old, with a mass of 1.18 solar masses and a radius of 1.28 solar radii, making it larger than the Sun in both mass and radius. Its temperature of 6210 K is hotter than the Sun's.
The single planet in this system is Kepler-1475 b, a Neptune-like world discovered by the transit method 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-1475 b orbits its star every 82.2 days and has a radius of 2.92 Earth radii, larger than Earth's. As a Neptune-like planet, its size class reflects a radius reaching up to four times Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
10
Stellar refs
10
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 6247 | 1.02 | 0.95 | — | — | — | 1568.4 | Q1-Q12 KOI Table | TICv8 |
| 6247 | 1.02 | 0.95 | — | — | — | 1568.4 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6034 | — | 0.80 | — | — | — | 1568.4 | Latham et al. 2005 | TICv8 |
| 5734 | — | 1.26 | — | 0.19 | — | 1568.4 | Gaia DR2 | TICv8 |
| 6247 | 1.02 | 0.95 | — | — | — | 1568.4 | Q1-Q17 DR24 KOI Table | TICv8 |
| — | — | — | — | — | — | 1568.4 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6214 | 1.18 | 1.28 | 2.82 | — | — | 1568.4 | Morton et al. 2016 | TICv8 |
| 6247 | 1.02 | 0.95 | — | — | — | 1568.4 | Q1-Q16 KOI Table | TICv8 |
| 6269 | — | 1.18 | — | — | — | 1568.4 | Berger et al. 2018 | TICv8 |
| 6084 | 1.14 | 1.21 | — | 0.25 | — | 1568.4 | TICv8 | TICv8 |