Temperature
5231 K
5055 to 5231
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Stellar HostProfile
Kepler-1829
Unclassified star โข 679.9 pc
Records
10
literature rows
Planets
1
system count
References
11
distinct source labels
TIC: TIC 299028577
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: Q1-Q12 KOI Table โข System source: TICv8
Mass
0.87 Msun
0.80 to 0.87
Radius
0.78 Rsun
0.73 to 0.83
Distance
679.9 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.78 Rโ โข circles scaled linearly by radius
Sun
1.0 Rโ baseline
Kepler-1829
0.78 Rโ
System Layout
Known planets
1 planets linked to this host
Kepler-1829 b
Transit
โ
Discovery
2021
Period
5.19 days
Radius
2.48 Rโ
Mass
โ
Eq. Temp
โ
Kepler-1829 b: A Super-Earth in a Close Orbit
Kepler-1829 is a single-star system 2220 light-years away. Its star has a reported mass of 0.869 solar masses, a radius of 0.781 solar radii, and a temperature of 5230 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. This system hosts one known planet.
Kepler-1829 b is a Super-Earth discovered by the transit method in 2021. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. Kepler-1829 b completes an orbit in 5.19 days and has a radius of 2.48 Earth radii, which is larger than Earth's. As a Super-Earth, its size class reaches up to 2.5 times Earth's radius.
Provenance
Underlying measurements and references
Evidence Summary
Rows
10
Stellar refs
10
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositystable
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5231 | 0.87 | 0.78 | โ | โ | โ | 679.9 | Q1-Q12 KOI Table | TICv8 |
| 5230 | 0.87 | 0.78 | โ | โ | โ | 679.9 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5068 | โ | 0.74 | โ | โ | โ | 679.9 | Q1-Q6 KOI Table | TICv8 |
| 5068 | 0.84 | 0.74 | โ | โ | โ | 679.9 | Batalha et al. 2013 | TICv8 |
| 5231 | 0.87 | 0.78 | โ | โ | โ | 679.9 | Q1-Q16 KOI Table | TICv8 |
| 5181 | 0.80 | 0.73 | 4.40 | โ | โ | 679.9 | Q1-Q8 KOI Table | TICv8 |
| โ | โ | โ | โ | โ | โ | 679.9 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5231 | 0.87 | 0.78 | โ | โ | โ | 679.9 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5068 | โ | 0.79 | โ | โ | โ | 679.9 | Latham et al. 2005 | TICv8 |
| 5055 | 0.84 | 0.83 | โ | -0.39 | โ | 679.9 | TICv8 | TICv8 |