Temperature
6202 K
5937 to 6292
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Stellar HostProfile
Kepler-1370
Unclassified star • 1004.1 pc
Records
18
literature rows
Planets
2
system count
References
13
distinct source labels
TIC: TIC 120253552
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
1.19 Msun
1.08 to 1.27
Radius
1.29 Rsun
1.21 to 1.50
Age
2.88 Gyr
2.69 to 3.53
Distance
1004.1 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.29 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1370
1.29 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-1370 b
Transit
◌
Discovery
2016
Period
20.26 days
Radius
1.84 R⊕
Mass
—
Eq. Temp
—
Kepler-1370 c
Transit
◌
Discovery
2016
Period
7.44 days
Radius
1.27 R⊕
Mass
—
Eq. Temp
—
Kepler-1370 and Its Two Planets
Kepler-1370 is a star located 3,270 light-years away, and two planets have been found in orbit around it. The host star is 2.88 billion years old, holds 1.19 solar masses, spans 1.29 solar radii, and has a temperature of 6,200 K. Its reported mass and radius estimates are larger than the Sun's, and its temperature is hotter than the Sun's.
Both planets were discovered in 2016 by the transit method, in which a planet passing in front of its star from our viewpoint causes a small dip in observed brightness. Kepler-1370 b is a Super-Earth with a radius of 1.84 Earth radii and an orbital period of 20.3 days. Kepler-1370 c is Earth-like, with a radius of 1.27 Earth radii and an orbital period of 7.44 days. Both planets have reported radius estimates larger than Earth's, and size classes compare radius with Earth's rather than indicating composition. Among the listed planets, Kepler-1370 c has the shortest year and the smallest radius, while Kepler-1370 b has the longest year and the largest radius.
Provenance
Underlying measurements and references
Evidence Summary
Rows
18
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 | 1.10 | 1.21 | 3.53 | — | — | 1004.1 | Q1-Q8 KOI Table | TICv8 |
| 6234 | 1.10 | 1.21 | 3.53 | — | — | 1004.1 | Q1-Q8 KOI Table | TICv8 |
| 6190 | 1.27 | 1.47 | 2.69 | — | — | 1004.1 | Fulton & Petigura 2018 | TICv8 |
| 5937 | 1.08 | 1.29 | — | — | — | 1004.1 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6020 | — | 1.22 | — | — | — | 1004.1 | Latham et al. 2005 | TICv8 |
| 6030 | — | 1.50 | — | 0.43 | — | 1004.1 | Gaia DR2 | TICv8 |
| 6292 | 1.25 | 1.28 | — | — | — | 1004.1 | Q1-Q16 KOI Table | TICv8 |
| 6292 | 1.25 | 1.28 | — | — | — | 1004.1 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6292 | 1.25 | 1.28 | — | — | — | 1004.1 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6292 | 1.25 | 1.28 | — | — | — | 1004.1 | Q1-Q12 KOI Table | TICv8 |
| 6292 | 1.25 | 1.28 | — | — | — | 1004.1 | Q1-Q12 KOI Table | TICv8 |
| 6212.5 | 1.20 | 1.46 | — | 0.46 | — | 1004.1 | TICv8 | TICv8 |
| 6202 | 1.19 | 1.29 | 2.88 | — | — | 1004.1 | Morton et al. 2016 | TICv8 |
| 6190 | — | 1.50 | — | — | — | 1004.1 | Berger et al. 2018 | TICv8 |
| — | — | — | — | — | — | 1004.1 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| — | — | — | — | — | — | 1004.1 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6292 | 1.25 | 1.28 | — | — | — | 1004.1 | Q1-Q16 KOI Table | TICv8 |
| 5937 | 1.08 | 1.29 | — | — | — | 1004.1 | Q1-Q17 DR25 KOI Table | TICv8 |