Temperature
6010 K
5817 to 6086
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Stellar HostProfile
Kepler-1050
Unclassified star • 490.5 pc
Records
21
literature rows
Planets
2
system count
References
15
distinct source labels
TIC: TIC 48216453
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
1.09 Msun
1.01 to 1.28
Radius
1.13 Rsun
1.00 to 2.15
Age
3.55 Gyr
1.23 to 3.55
Distance
490.5 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.13 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1050
1.13 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-1050 b
Transit
◌
Discovery
2016
Period
15.38 days
Radius
1.60 R⊕
Mass
—
Eq. Temp
—
Kepler-1050 c
Transit
◌
Discovery
2016
Period
21.13 days
Radius
1.48 R⊕
Mass
—
Eq. Temp
—
Kepler-1050 and Its Two Planets
Kepler-1050 is a star located 1600 light-years away, and two planets have been found orbiting it. The host star is 3.55 billion years old and has a mass of 1.09 solar masses. Its radius is 1.13 solar radii, and its temperature is 6010 K.
Both planets were discovered by transit in 2016. Kepler-1050 b is a Super-Earth with an orbital period of 15.4 days and a radius of 1.6 Earth radii. Kepler-1050 c is Earth-like, with an orbital period of 21.1 days and a radius of 1.48 Earth radii. Among the listed planets, Kepler-1050 b has the shortest year and the largest radius, while Kepler-1050 c has the longest year and the smallest radius.
Provenance
Underlying measurements and references
Evidence Summary
Rows
21
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 |
|---|---|---|---|---|---|---|---|---|
| 5821 | — | 1.08 | — | — | — | 490.5 | Latham et al. 2005 | TICv8 |
| 6010 | 1.09 | 1.13 | 3.55 | — | — | 490.5 | Morton et al. 2016 | TICv8 |
| — | — | — | — | — | — | 490.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5846 | 1.06 | 1.00 | 1.23 | — | — | 490.5 | Fulton & Petigura 2018 | TICv8 |
| 6086 | 1.04 | 1.05 | — | — | — | 490.5 | Q1-Q16 KOI Table | TICv8 |
| 6086 | 1.04 | 1.05 | — | — | — | 490.5 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6086 | 1.04 | 1.05 | — | — | — | 490.5 | Q1-Q12 KOI Table | TICv8 |
| 6086 | 1.04 | 1.05 | — | — | — | 490.5 | Q1-Q16 KOI Table | TICv8 |
| 5830.7 | — | 1.02 | — | 0.04 | — | 490.5 | Gaia DR2 | TICv8 |
| 6064 | 1.03 | 1.05 | 3.50 | — | — | 490.5 | Q1-Q8 KOI Table | TICv8 |
| 6086 | 1.04 | 1.05 | — | — | — | 490.5 | Q1-Q12 KOI Table | TICv8 |
| 5821 | — | 1.01 | — | — | — | 490.5 | Q1-Q6 KOI Table | TICv8 |
| 5817 | 1.28 | 2.15 | — | — | — | 490.5 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6064 | 1.03 | 1.05 | 3.50 | — | — | 490.5 | Q1-Q8 KOI Table | TICv8 |
| 6086 | 1.04 | 1.05 | — | — | — | 490.5 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5846 | — | 1.01 | — | — | — | 490.5 | Berger et al. 2018 | TICv8 |
| 5821 | — | — | — | — | — | 490.5 | Q1-Q6 KOI Table | TICv8 |
| 5817 | 1.28 | 2.15 | — | — | — | 490.5 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5870.7 | 1.06 | 1.03 | — | 0.06 | — | 490.5 | TICv8 | TICv8 |
| 5821 | 1.01 | 1.01 | — | — | — | 490.5 | Batalha et al. 2013 | TICv8 |
| — | — | — | — | — | — | 490.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |