Temperature
5352 K
5116.2 to 5475
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Stellar HostProfile
Kepler-1355
Unclassified star • 911.3 pc
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
TIC: TIC 48354835
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
0.88 Msun
0.88 to 0.91
Radius
0.83 Rsun
0.64 to 0.87
Age
4.27 Gyr
0.60 to 4.27
Distance
911.3 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.83 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1355
0.83 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1355 b
Transit
◌
Discovery
2016
Period
1.29 days
Radius
1.46 R⊕
Mass
—
Eq. Temp
—
Kepler-1355 and Its Earth-like Planet
Kepler-1355 is a star located 2970 light-years away, and it hosts one known planet. The star is estimated to be 4.27 billion years old, with a mass of 0.88 solar masses and a radius of 0.83 solar radii. Its temperature is 5350 K. The star's reported mass estimate is smaller than the Sun's, its reported radius estimate is smaller than the Sun's, and its reported temperature is cooler than the Sun's.
The planet Kepler-1355 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-1355 b has an orbital period of 1.29 days, so it completes one orbit in that time. Its radius is 1.46 Earth radii, and its reported radius estimate is larger than Earth's. As an Earth-like planet, it stays within 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 |
|---|---|---|---|---|---|---|---|---|
| 5471 | 0.90 | 0.81 | — | — | — | 911.3 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5293 | — | 0.64 | — | — | — | 911.3 | Latham et al. 2005 | TICv8 |
| 5471 | 0.90 | 0.81 | — | — | — | 911.3 | Q1-Q16 KOI Table | TICv8 |
| 5352 | 0.88 | 0.83 | 4.27 | — | — | 911.3 | Morton et al. 2016 | TICv8 |
| 5467 | 0.91 | 0.81 | — | — | — | 911.3 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5444 | 0.88 | 0.78 | 0.60 | — | — | 911.3 | Q1-Q8 KOI Table | TICv8 |
| 5475 | — | 0.77 | — | — | — | 911.3 | Berger et al. 2018 | TICv8 |
| 5255 | 0.90 | 0.83 | — | -0.33 | — | 911.3 | TICv8 | TICv8 |
| 5116.2 | — | 0.87 | — | -0.33 | — | 911.3 | Gaia DR2 | TICv8 |
| — | — | — | — | — | — | 911.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5471 | 0.90 | 0.81 | — | — | — | 911.3 | Q1-Q12 KOI Table | TICv8 |