Temperature
5549 K
5375 to 5609
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Stellar HostProfile
Kepler-1310
Unclassified star • 569.2 pc
Records
14
literature rows
Planets
1
system count
References
15
distinct source labels
TIC: TIC 120043638
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
0.91 Msun
0.82 to 0.99
Radius
0.88 Rsun
0.73 to 0.91
Age
4.17 Gyr
0.50 to 5.37
Distance
569.2 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.88 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1310
0.88 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1310 b
Transit
◌
Discovery
2016
Period
0.68 days
Radius
1.44 R⊕
Mass
—
Eq. Temp
—
Kepler-1310 and Its Earth-Like Planet
Kepler-1310 is a star 1860 light-years away with one known planet. The host star is 4.17 billion years old and has a mass of 0.91 solar masses, a radius of 0.88 solar radii, and a temperature of 5550 K. Its reported mass and radius estimates are smaller than the Sun's, and its reported temperature is cooler than the Sun's.
The planet Kepler-1310 b was discovered by transit in 2016. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. Repeated dips help establish orbital periods. Kepler-1310 b completes an orbit every 0.679 days, and its radius is 1.44 Earth radii. That radius is larger than Earth's. Planet size classes compare radius with Earth's, and an Earth-like planet stays within 1.5 times Earth's radius; Kepler-1310 b is classified as Earth-like.
Provenance
Underlying measurements and references
Evidence Summary
Rows
14
Stellar refs
14
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 |
|---|---|---|---|---|---|---|---|---|
| 5596 | 0.85 | 0.78 | — | — | — | 569.2 | Q1-Q16 KOI Table | TICv8 |
| 5375 | 0.82 | 0.73 | — | — | — | 569.2 | Batalha et al. 2013 | TICv8 |
| 5440 | 0.94 | 0.91 | — | — | — | 569.2 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5381.3 | — | 0.88 | — | -0.24 | — | 569.2 | Gaia DR2 | TICv8 |
| 5463 | — | 0.88 | — | — | — | 569.2 | Berger et al. 2018 | TICv8 |
| 5609 | 0.93 | 0.82 | 0.50 | — | — | 569.2 | Q1-Q8 KOI Table | TICv8 |
| 5599 | 0.99 | 0.85 | — | -0.19 | — | 569.2 | TICv8 | TICv8 |
| 5596 | 0.85 | 0.78 | — | — | — | 569.2 | Q1-Q12 KOI Table | TICv8 |
| 5549 | 0.91 | 0.88 | 4.17 | — | — | 569.2 | Morton et al. 2016 | TICv8 |
| 5375 | — | 0.73 | — | — | — | 569.2 | Q1-Q6 KOI Table | TICv8 |
| 5375 | — | 0.76 | — | — | — | 569.2 | Latham et al. 2005 | TICv8 |
| — | — | — | — | — | — | 569.2 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5463 | 0.88 | 0.87 | 5.37 | — | — | 569.2 | Fulton & Petigura 2018 | TICv8 |
| 5596 | 0.85 | 0.78 | — | — | — | 569.2 | Q1-Q17 DR24 KOI Table | TICv8 |