Temperature
6002.5 K
5868 to 6085
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Stellar HostProfile
Kepler-1927
Unclassified star • 1091 pc
Records
13
literature rows
Planets
1
system count
References
9
distinct source labels
TIC: TIC 184427149
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 • System source: TICv8
Mass
1.11 Msun
0.99 to 1.42
Radius
2.25 Rsun
0.96 to 2.48
Luminosity
0.77 log(Lsun)
single adopted value
Distance
1091 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 2.25 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1927
2.25 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1927 b
Transit
◌
Discovery
2021
Period
73.75 days
Radius
3.41 R⊕
Mass
—
Eq. Temp
—
Kepler-1927 b: A Neptune-Like World in a Distant System
Kepler-1927 is a star located 3560 light-years away, with one planet in its orbit. The host star has a mass of 1.11 solar masses, a radius of 2.25 solar radii, and a temperature of 6000 K. Its radius is larger than the Sun's, and its temperature is hotter than the Sun's.
The single planet, Kepler-1927 b, is a Neptune-like world discovered in 2021 by the transit method, in which a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. Repeated dips help establish the planet's orbital period. Kepler-1927 b completes one orbit every 73.8 days. Its radius is 3.41 Earth radii, which is larger than Earth's.
Planet size classes compare radius with Earth's: a Neptune-like planet reaches four times Earth's radius, while a Jupiter-like planet exceeds that threshold. This classification describes the planet's size, not its composition.
Provenance
Underlying measurements and references
Evidence Summary
Rows
13
Stellar refs
8
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 |
|---|---|---|---|---|---|---|---|---|
| 6085 | 0.99 | 0.96 | — | — | — | 1091 | Q1-Q16 KOI Table | TICv8 |
| — | — | — | — | — | — | 1091 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6085 | 0.99 | 0.96 | — | — | — | 1091 | Q1-Q12 KOI Table | TICv8 |
| 6056 | 1.41 | 2.48 | — | — | — | 1091 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5868 | — | 1.00 | — | — | — | 1091 | Latham et al. 2005 | TICv8 |
| 6085 | 0.99 | 0.96 | — | — | — | 1091 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6080 | 1.42 | 2.06 | 2.88 | — | — | 1091 | Fulton & Petigura 2018 | TICv8 |
| 6085 | 0.99 | 0.96 | — | — | — | 1091 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6085 | 0.99 | 0.96 | — | — | — | 1091 | Q1-Q16 KOI Table | TICv8 |
| 6002.5 | 1.11 | 2.25 | — | 0.77 | — | 1091 | TICv8 | TICv8 |
| 6085 | 0.99 | 0.96 | — | — | — | 1091 | Q1-Q12 KOI Table | TICv8 |
| — | — | — | — | — | — | 1091 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6056 | 1.41 | 2.48 | — | — | — | 1091 | Q1-Q17 DR25 KOI Table | TICv8 |