Temperature
5932 K
5687.8 to 6003
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Stellar HostProfile
Kepler-335
Unclassified star • 1279.0 pc
Records
20
literature rows
Planets
2
system count
References
16
distinct source labels
TIC: TIC 272085033
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
1.23 Msun
0.99 to 1.37
Radius
1.68 Rsun
0.78 to 1.91
Age
4.37 Gyr
0.30 to 4.37
Distance
1279.0 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.68 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-335
1.68 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-335 b
Transit
◌
Discovery
2014
Period
6.56 days
Radius
3.39 R⊕
Mass
—
Eq. Temp
—
Kepler-335 c
Transit
◌
Discovery
2014
Period
67.84 days
Radius
3.07 R⊕
Mass
—
Eq. Temp
—
Kepler-335 and Its Two Neptune-Like Planets
Kepler-335 is a star located 4170 light-years away, and two planets have been reported orbiting it. The host star is 4.37 billion years old, with a mass of 1.23 solar masses, a radius of 1.68 solar radii, and a temperature of 5930 K. Its mass, radius, and temperature are all larger or hotter than the Sun's.
Both planets were discovered by transit in 2014, the method in which a planet passes in front of its star and causes a small dip in observed brightness. Kepler-335 b is Neptune-like, with a radius of 3.39 Earth radii and an orbital period of 6.56 days. Kepler-335 c is also Neptune-like, with a radius of 3.07 Earth radii and an orbital period of 67.8 days. Both planets are larger than Earth in radius.
Among the listed planets, Kepler-335 b has the shortest year by reported estimates, while Kepler-335 c has the longest. Kepler-335 b also has the largest radius, and Kepler-335 c has the smallest radius, at 3.07 Earth radii.
Provenance
Underlying measurements and references
Evidence Summary
Rows
20
Stellar refs
15
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 |
|---|---|---|---|---|---|---|---|---|
| 6003 | 1.02 | 0.93 | — | — | — | 1279.0 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6003 | 1.02 | 0.93 | — | — | — | 1279.0 | Q1-Q12 KOI Table | TICv8 |
| 5878 | 1.21 | 1.81 | — | — | — | 1279.0 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5687.8 | — | 1.91 | — | 0.54 | — | 1279.0 | Gaia DR2 | TICv8 |
| 5877 | — | 1.85 | — | — | — | 1279.0 | Rowe et al. 2014 | TICv8 |
| 6000 | 1.37 | 1.77 | 3.09 | — | — | 1279.0 | Fulton & Petigura 2018 | TICv8 |
| 5744 | — | 0.89 | — | — | — | 1279.0 | Q1-Q6 KOI Table | TICv8 |
| — | — | — | — | — | — | 1279.0 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5932 | 1.23 | 1.68 | 4.37 | — | — | 1279.0 | Morton et al. 2016 | TICv8 |
| 5878 | 1.21 | 1.81 | — | — | — | 1279.0 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6003 | 1.02 | 0.93 | — | — | — | 1279.0 | Q1-Q16 KOI Table | TICv8 |
| 5744 | 0.99 | 0.89 | — | — | — | 1279.0 | Batalha et al. 2013 | TICv8 |
| 5990 | 1.03 | 0.93 | 0.30 | — | — | 1279.0 | Q1-Q8 KOI Table | TICv8 |
| 6003 | 1.02 | 0.93 | — | — | — | 1279.0 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6003 | 1.02 | 0.93 | — | — | — | 1279.0 | Q1-Q16 KOI Table | TICv8 |
| 6000 | — | 1.82 | — | — | — | 1279.0 | Berger et al. 2018 | TICv8 |
| — | — | — | — | — | — | 1279.0 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5928.7 | 1.08 | 1.84 | — | 0.58 | — | 1279.0 | TICv8 | TICv8 |
| 5744 | — | 0.78 | — | — | — | 1279.0 | Latham et al. 2005 | TICv8 |
| 6003 | 1.02 | 0.93 | — | — | — | 1279.0 | Q1-Q12 KOI Table | TICv8 |