Temperature
6356 K
6234 to 6664
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Stellar HostProfile
Kepler-1435
Unclassified star • 704.2 pc
Records
12
literature rows
Planets
1
system count
References
13
distinct source labels
TIC: TIC 159647919
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
1.21 Msun
1.09 to 1.26
Radius
1.32 Rsun
1.20 to 1.41
Age
2.63 Gyr
1.03 to 4.90
Distance
704.2 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.32 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1435
1.32 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1435 b
Transit
◌
Discovery
2016
Period
4.45 days
Radius
0.86 R⊕
Mass
—
Eq. Temp
—
Kepler-1435: A Distant Star With a Sub-Earth Planet
Kepler-1435 is a star 2300 light-years away. It is 2.63 billion years old and has 1.21 solar masses, 1.32 solar radii, and a temperature of 6360 K. Its mass, radius, and temperature are all reported as larger or hotter than the Sun's. One known planet orbits it.
That planet, Kepler-1435 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-1435 b has an orbital period of 4.45 days and a radius of 0.86 Earth radii, smaller than Earth's. Its size class, Sub-Earth, refers to a radius below Earth's rather than to composition, and its radius comparison describes radius, not volume.
Provenance
Underlying measurements and references
Evidence Summary
Rows
12
Stellar refs
12
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 |
|---|---|---|---|---|---|---|---|---|
| 6234 | — | 1.40 | — | — | — | 704.2 | Berger et al. 2018 | TICv8 |
| 6664 | 1.24 | 1.34 | — | — | — | 704.2 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6356 | 1.21 | 1.32 | 2.63 | — | — | 704.2 | Morton et al. 2016 | TICv8 |
| 6664 | 1.24 | 1.34 | — | — | — | 704.2 | Q1-Q12 KOI Table | TICv8 |
| 6256 | 1.09 | 1.27 | — | — | — | 704.2 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6431 | — | 1.20 | — | — | — | 704.2 | Latham et al. 2005 | TICv8 |
| 6360.2 | 1.26 | 1.41 | — | 0.47 | — | 704.2 | TICv8 | TICv8 |
| 6640 | 1.25 | 1.26 | 1.03 | — | — | 704.2 | Q1-Q8 KOI Table | TICv8 |
| 6664 | 1.24 | 1.34 | — | — | — | 704.2 | Q1-Q16 KOI Table | TICv8 |
| 6234 | 1.09 | 1.38 | 4.90 | — | — | 704.2 | Fulton & Petigura 2018 | TICv8 |
| 6390.5 | — | 1.34 | — | 0.43 | — | 704.2 | Gaia DR2 | TICv8 |
| — | — | — | — | — | — | 704.2 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |