Temperature
4903 K
4830 to 5032
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Stellar HostProfile
Kepler-1335
Unclassified star • 621.9 pc
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
TIC: TIC 164827658
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
0.77 Msun
0.72 to 0.79
Radius
0.74 Rsun
0.68 to 0.86
Age
4.90 Gyr
4.90 to 13.80
Distance
621.9 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.74 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1335
0.74 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1335 b
Transit
◌
Discovery
2016
Period
6.26 days
Radius
1.45 R⊕
Mass
—
Eq. Temp
—
Kepler-1335 and Its Earth-Like Planet
Kepler-1335 is a star located 2030 light-years away with one planet in orbit around it. The host star is 4.9 billion years old, with a mass of 0.77 solar masses and a radius of 0.74 solar radii. Its temperature is 4900 K, which is cooler than the Sun's. The star's reported mass and radius estimates are both smaller than the Sun's.
The planet Kepler-1335 b was discovered in 2016 by the transit method, which detects the small dip in a star's brightness when a planet passes in front of it. This planet has an orbital period of 6.26 days, the time it takes to complete one orbit. Its radius is 1.45 Earth radii, making it larger than Earth. That radius places it within the Earth-like size class, which covers planets up to 1.5 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 |
|---|---|---|---|---|---|---|---|---|
| 5032 | 0.79 | 0.82 | — | — | — | 621.9 | Q1-Q17 DR25 KOI Table | TICv8 |
| 4903 | 0.77 | 0.74 | 4.90 | — | — | 621.9 | Morton et al. 2016 | TICv8 |
| — | — | — | — | — | — | 621.9 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5032 | — | 0.73 | — | — | — | 621.9 | Berger et al. 2018 | TICv8 |
| 4969.2 | — | 0.68 | — | -0.60 | — | 621.9 | Gaia DR2 | TICv8 |
| 4830 | 0.78 | 0.75 | — | -0.56 | — | 621.9 | TICv8 | TICv8 |
| 5032 | 0.79 | 0.82 | — | — | — | 621.9 | Q1-Q16 KOI Table | TICv8 |
| 5032 | 0.79 | 0.82 | — | — | — | 621.9 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5032 | 0.79 | 0.82 | — | — | — | 621.9 | Q1-Q12 KOI Table | TICv8 |
| 4855 | — | 0.86 | — | — | — | 621.9 | Latham et al. 2005 | TICv8 |
| 4969 | 0.72 | 0.72 | 13.80 | — | — | 621.9 | Q1-Q8 KOI Table | TICv8 |