Temperature
5886.3 K
5830 to 6112
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Stellar HostProfile
Kepler-1876
Unclassified star โข 259.9 pc
Records
10
literature rows
Planets
1
system count
References
11
distinct source labels
TIC: TIC 171883078
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: TICv8 โข System source: TICv8
Mass
1.07 Msun
1.07 to 1.27
Radius
1.58 Rsun
1.47 to 2.17
Luminosity
0.43 log(Lsun)
single adopted value
Distance
259.9 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.58 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
Kepler-1876
1.58 Rโ
System Layout
Known planets
1 planets linked to this host
Kepler-1876 b
Transit
โ
Discovery
2021
Period
6.99 days
Radius
0.85 Rโ
Mass
2.40 Mโ
Eq. Temp
1299 K
Kepler-1876 b: A Sub-Earth in a Close Orbit
Kepler-1876 is a star 848 light-years away with one known planet. The host star has a mass of 1.07 solar masses, a radius of 1.58 solar radii, and a temperature of 5890 K. Its radius estimate is larger than the Sun's.
The planet, Kepler-1876 b, was discovered in 2021 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. It is classified as a Sub-Earth, meaning its radius is smaller than Earth's. Its radius is 0.853 Earth radii, and its reported radius estimate is smaller than Earth's. Its mass is a reported upper limit of 2.4 Earth masses. It completes an orbit every 6.99 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
10
Stellar refs
10
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositystable
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 6112 | 1.27 | 2.17 | โ | โ | โ | 259.9 | Q1-Q16 KOI Table | TICv8 |
| 6057 | 1.08 | 1.47 | โ | โ | โ | 259.9 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6095 | 1.23 | 2.07 | 4.50 | โ | โ | 259.9 | Q1-Q8 KOI Table | TICv8 |
| 5886.3 | 1.07 | 1.58 | โ | 0.43 | โ | 259.9 | TICv8 | TICv8 |
| 6104 | 1.19 | 1.48 | 4.40 | โ | โ | 259.9 | Bonomo et al. 2023 | TICv8 |
| 6112 | 1.27 | 2.17 | โ | โ | โ | 259.9 | Q1-Q17 DR24 KOI Table | TICv8 |
| โ | โ | โ | โ | โ | โ | 259.9 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6057 | 1.13 | 1.48 | 5.13 | โ | โ | 259.9 | Fulton & Petigura 2018 | TICv8 |
| 5830 | โ | 2.09 | โ | โ | โ | 259.9 | Latham et al. 2005 | TICv8 |
| 6112 | 1.27 | 2.17 | โ | โ | โ | 259.9 | Q1-Q12 KOI Table | TICv8 |