Temperature
5825 K
5348 to 5825
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Stellar HostProfile
Kepler-119
Unclassified star • 702.0 pc
Records
21
literature rows
Planets
2
system count
References
15
distinct source labels
TIC: TIC 271964647
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
1.01 Msun
0.91 to 1.01
Radius
1.03 Rsun
0.59 to 1.06
Age
3.63 Gyr
0.40 to 3.63
Distance
702.0 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.03 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
Kepler-119
1.03 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-119 b
Transit
◌
Discovery
2014
Period
2.42 days
Radius
3.60 R⊕
Mass
—
Eq. Temp
—
Kepler-119 c
Transit
◌
Discovery
2014
Period
4.13 days
Radius
0.92 R⊕
Mass
—
Eq. Temp
—
Kepler-119: A Distant Star With Two Known Planets
Kepler-119 is a star located 2290 light-years away, and it hosts two known planets. The star is 3.63 billion years old, with a mass of 1.01 solar masses, a radius of 1.03 solar radii, and a temperature of 5830 K.
Both planets were discovered in 2014 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. Kepler-119 b is a Neptune-like planet with a radius of 3.6 Earth radii and an orbital period of 2.42 days. Kepler-119 c is a Sub-Earth with a radius of 0.92 Earth radii and an orbital period of 4.13 days.
Among the listed planets, Kepler-119 b has the shortest year and the largest radius, while Kepler-119 c has the longest year and the smallest radius. Kepler-119 b's reported radius estimate is larger than Earth's.
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 |
|---|---|---|---|---|---|---|---|---|
| 5388 | — | 0.59 | — | — | — | 702.0 | Latham et al. 2005 | TICv8 |
| 5595 | — | 1.00 | — | — | — | 702.0 | Berger et al. 2018 | TICv8 |
| 5570 | 0.92 | 0.81 | 0.40 | — | — | 702.0 | Q1-Q8 KOI Table | TICv8 |
| 5586 | 0.99 | 1.02 | — | -0.04 | — | 702.0 | TICv8 | TICv8 |
| 5588 | 0.91 | 0.83 | — | — | — | 702.0 | Q1-Q16 KOI Table | TICv8 |
| 5598 | 0.93 | 0.83 | — | — | — | 702.0 | Q1-Q17 DR25 KOI Table | TICv8 |
| — | — | — | — | — | — | 702.0 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5588 | 0.91 | 0.83 | — | — | — | 702.0 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5388 | — | 0.79 | — | — | — | 702.0 | Q1-Q6 KOI Table | TICv8 |
| 5588 | 0.91 | 0.83 | — | — | — | 702.0 | Q1-Q12 KOI Table | TICv8 |
| 5348 | — | 1.06 | — | -0.08 | — | 702.0 | Gaia DR2 | TICv8 |
| — | — | — | — | — | — | 702.0 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5570 | 0.92 | 0.81 | 0.40 | — | — | 702.0 | Q1-Q8 KOI Table | TICv8 |
| 5588 | 0.91 | 0.83 | — | — | — | 702.0 | Q1-Q12 KOI Table | TICv8 |
| 5388 | — | 0.79 | — | — | — | 702.0 | Batalha et al. 2013 | TICv8 |
| 5388 | — | 0.79 | — | — | — | 702.0 | Q1-Q6 KOI Table | TICv8 |
| 5588 | 0.91 | 0.83 | — | — | — | 702.0 | Q1-Q16 KOI Table | TICv8 |
| 5588 | 0.91 | 0.83 | — | — | — | 702.0 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5598 | 0.93 | 0.83 | — | — | — | 702.0 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5825 | 1.01 | 1.03 | 3.63 | — | — | 702.0 | Morton et al. 2016 | TICv8 |
| 5595 | — | 0.84 | — | — | — | 702.0 | Rowe et al. 2014 | TICv8 |