Temperature
5274 K
4686 to 5428
G9 V • 157.7 pc
Records
16
literature rows
Planets
4
system count
References
15
distinct source labels
Approximate color
from effective temperature
Canonical Summary
Numeric fields use the median of non-null measurements. Disagreement stays visible through ranges, counts, and provenance.
Temperature
5274 K
4686 to 5428
Mass
0.87 Msun
0.83 to 0.92
Radius
0.84 Rsun
0.72 to 0.92
Age
7.90 Gyr
single adopted value
Luminosity
-0.39 log(Lsun)
-0.49 to -0.30
Distance
157.7 pc
single adopted value
Spectral Type
G9 V
Consistent across records
Planets
4
Stable across source rows
Scale Comparison
Current adopted radius: 0.84 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
K2-32
0.84 R☉
System Layout
4 planets linked to this host
Provenance
Evidence Summary
Rows
16
Stellar refs
14
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | 0.76 | — | — | — | 157.7 | Kruse et al. 2019 | TICv8 |
| 5428 | 0.88 | 0.92 | — | — | — | 157.7 | Crossfield et al. 2016 | TICv8 |
| 5315 | 0.87 | 0.87 | — | — | — | 157.7 | Dai et al. 2016 | TICv8 |
| 5271 | 0.83 | 0.86 | — | — | — | 157.7 | Lillo-Box et al. 2020 | TICv8 |
| 4686 | — | 0.72 | — | — | — | 157.7 | Vanderburg et al. 2016 | TICv8 |
| 5274 | 0.84 | 0.85 | — | — | — | 157.7 | Howard et al. 2025 | TICv8 |
| — | — | 0.76 | — | — | — | 157.7 | Kruse et al. 2019 | TICv8 |
| 5315 | 0.87 | 0.87 | — | — | G9 V | 157.7 | Sinukoff et al. 2016 | TICv8 |
| 5415 | 0.92 | 0.84 | — | — | — | 157.7 | Mayo et al. 2018 | TICv8 |
| — | — | — | — | — | — | 157.7 | Barros et al. 2016 | TICv8 |
| — | — | 0.76 | — | — | — | 157.7 | Kruse et al. 2019 | TICv8 |
| 5274 | — | 0.85 | — | — | — | 157.7 | ExoFOP | TICv8 |
| 5275 | 0.86 | 0.84 | 7.90 | — | — | 157.7 | Petigura et al. 2017 | TICv8 |
| 5274 | 0.90 | 0.85 | — | -0.30 | — | 157.7 | TICv8 | TICv8 |
| 5010 | — | 0.76 | — | -0.49 | — | 157.7 | Gaia DR2 | TICv8 |
| — | 0.86 | 0.84 | — | — | — | 157.7 | Heller et al. 2019 | TICv8 |