Temperature
6036 K
5774 to 6103
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Stellar HostProfile
Kepler-1796
Unclassified star โข 825.9 pc
Records
10
literature rows
Planets
1
system count
References
11
distinct source labels
TIC: TIC 185336831
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
1.02 Msun
0.99 to 1.15
Radius
0.95 Rsun
0.89 to 1.02
Distance
825.9 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.95 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
Kepler-1796
0.95 Rโ
System Layout
Known planets
1 planets linked to this host
Kepler-1796 b
Transit
โ
Discovery
2021
Period
29.46 days
Radius
2.75 Rโ
Mass
โ
Eq. Temp
โ
Kepler-1796 b: A Neptune-Like World in a Distant System
Kepler-1796 is a star 2690 light-years away with a mass of 1.02 solar masses, a radius of 0.949 solar radii, and a temperature of 6040 K. Its reported temperature is hotter than the Sun's. One planet is known to orbit this host.
That planet, Kepler-1796 b, is Neptune-like, a size classification that compares radius with Earth's and reaches up to four times Earth's radius. It was discovered by transit in 2021, when it passed in front of its star from our viewpoint and caused a small dip in observed brightness. Its radius measures 2.75 Earth radii, a radius estimate larger than Earth's. The planet completes an orbit every 29.5 days, the period that repeated transits help establish.
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 |
|---|---|---|---|---|---|---|---|---|
| 5774 | โ | 0.89 | โ | โ | โ | 825.9 | Q1-Q6 KOI Table | TICv8 |
| 6034 | 1.04 | 0.95 | 0.40 | โ | โ | 825.9 | Q1-Q8 KOI Table | TICv8 |
| 6036 | 1.02 | 0.95 | โ | โ | โ | 825.9 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6036 | 1.02 | 0.95 | โ | โ | โ | 825.9 | Q1-Q16 KOI Table | TICv8 |
| 5774 | โ | 0.92 | โ | โ | โ | 825.9 | Latham et al. 2005 | TICv8 |
| โ | โ | โ | โ | โ | โ | 825.9 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6103 | 1.15 | 1.02 | โ | 0.12 | โ | 825.9 | TICv8 | TICv8 |
| 6036 | 1.02 | 0.95 | โ | โ | โ | 825.9 | Q1-Q12 KOI Table | TICv8 |
| 5774 | 0.99 | 0.89 | โ | โ | โ | 825.9 | Batalha et al. 2013 | TICv8 |
| 6036 | 1.02 | 0.95 | โ | โ | โ | 825.9 | Q1-Q17 DR25 KOI Table | TICv8 |