Temperature
6100 K
5818.8 to 6374
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Stellar HostProfile
Kepler-852
Unclassified star • 1619.0 pc
Records
14
literature rows
Planets
1
system count
References
15
distinct source labels
TIC: TIC 28089606
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
1.02 to 1.44
Radius
1.16 Rsun
1.16 to 2.38
Age
1.48 Gyr
1.48 to 3.37
Distance
1619.0 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.16 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-852
1.16 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-852 b
Transit
◌
Discovery
2016
Period
44.93 days
Radius
2.54 R⊕
Mass
—
Eq. Temp
—
Kepler-852 and Its Neptune-Like Planet
Kepler-852 is a star 5280 light-years away with one known planet. The host star is estimated to be 1.48 billion years old, with a mass of 1.19 solar masses, a radius of 1.16 solar radii, and a temperature of 6100 K. Its reported mass and radius estimates are larger than the Sun's, and its reported temperature is hotter than the Sun's.
The planet Kepler-852 b is Neptune-like, meaning its radius falls within the size class reaching four times Earth's radius. It was discovered by transit in 2016, when the planet passed in front of its star from our viewpoint and caused a small dip in observed brightness. Kepler-852 b has an orbital period of 44.9 days and a radius of 2.54 Earth radii, which is larger than Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
14
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 |
|---|---|---|---|---|---|---|---|---|
| 6101 | — | 1.33 | — | — | — | 1619.0 | Latham et al. 2005 | TICv8 |
| 6354 | 1.02 | 1.25 | — | — | — | 1619.0 | Q1-Q16 KOI Table | TICv8 |
| 6225.0 | 1.20 | 2.23 | — | 0.83 | — | 1619.0 | TICv8 | TICv8 |
| 6101 | — | 1.27 | — | — | — | 1619.0 | Q1-Q6 KOI Table | TICv8 |
| 6236 | — | 2.19 | — | — | — | 1619.0 | Berger et al. 2018 | TICv8 |
| 6100 | 1.19 | 1.16 | 1.48 | — | — | 1619.0 | Morton et al. 2016 | TICv8 |
| 6354 | 1.02 | 1.25 | — | — | — | 1619.0 | Q1-Q12 KOI Table | TICv8 |
| 6354 | 1.02 | 1.25 | — | — | — | 1619.0 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6236 | 1.44 | 2.11 | 2.51 | — | — | 1619.0 | Fulton & Petigura 2018 | TICv8 |
| — | — | — | — | — | — | 1619.0 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6374 | 1.18 | 1.38 | 3.37 | — | — | 1619.0 | Q1-Q8 KOI Table | TICv8 |
| 6121 | 1.23 | 1.16 | — | — | — | 1619.0 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6101 | — | 1.27 | — | — | — | 1619.0 | Batalha et al. 2013 | TICv8 |
| 5818.8 | — | 2.38 | — | 0.77 | — | 1619.0 | Gaia DR2 | TICv8 |