Temperature
5929 K
5804 to 6060
Unclassified star • 377.8 pc
Records
6
literature rows
Planets
1
system count
References
7
distinct source labels
Approximate color
from effective temperature
Canonical Summary
Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.
Stellar source: Mayo et al. 2018 • System source: TICv8
Temperature
5929 K
5804 to 6060
Mass
0.99 Msun
0.96 to 1.11
Radius
1.09 Rsun
0.98 to 1.09
Distance
377.8 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 1.09 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
K2-74
1.09 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2016
Period
19.57 days
Radius
2.31 R⊕
Mass
—
Eq. Temp
—
K2-74 is a star 1230 light-years away with one known planet. The star has a mass of 0.987 solar masses, a radius of 1.09 solar radii, and a temperature of 5930 K, which is hotter than the Sun's reported temperature.
The planet K2-74 b was discovered in 2016 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. Repeated dips help establish orbital periods. K2-74 b completes one orbit every 19.6 days. Its radius is 2.31 Earth radii, larger than Earth's. That radius places it in the Super-Earth size class, which reaches 2.5 times Earth's radius; such classes compare radius, not composition.
Provenance
Evidence Summary
Rows
6
Stellar refs
6
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5929 | 0.99 | 1.09 | — | — | — | 377.8 | Mayo et al. 2018 | TICv8 |
| 6022 | 1.11 | 1.02 | — | 0.09 | — | 377.8 | TICv8 | TICv8 |
| 6060 | 0.96 | 0.98 | — | — | — | 377.8 | Crossfield et al. 2016 | TICv8 |
| — | — | 1.05 | — | — | — | 377.8 | Kruse et al. 2019 | TICv8 |
| 5838 | — | 1.05 | — | 0.06 | — | 377.8 | Gaia DR2 | TICv8 |
| 5804 | — | 1.01 | — | — | — | 377.8 | Vanderburg et al. 2016 | TICv8 |