Temperature
4377 K
4103 to 4415.5
Unclassified star โข 495.3 pc
Records
7
literature rows
Planets
1
system count
References
8
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: TICv8 โข System source: TICv8
Temperature
4377 K
4103 to 4415.5
Mass
0.68 Msun
0.50 to 0.68
Radius
0.77 Rsun
0.45 to 0.77
Luminosity
-0.71 log(Lsun)
-0.74 to -0.71
Distance
495.3 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 0.77 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
K2-45
0.77 Rโ
System Layout
1 planets linked to this host
Transit
Discovery
2016
Period
1.73 days
Radius
6.71 Rโ
Mass
โ
Eq. Temp
โ
K2-45 is a single-star system 1620 light-years away, and its one known planet orbits the star directly. The host star has 0.68 solar masses, a radius of 0.766 solar radii, and a temperature of 4380 K, meaning it is less massive, smaller, and cooler than the Sun.
The only cataloged planet is K2-45 b, a Jupiter-like world detected by transit in 2016. Its radius is 6.71 Earth radii, larger than Earth's, while its orbital period is 1.73 days. The combination of a Jupiter-like radius and a period of just 1.73 days places this planet very close to its host.
Provenance
Evidence Summary
Rows
7
Stellar refs
7
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| โ | โ | 0.73 | โ | โ | โ | 495.3 | Kruse et al. 2019 | TICv8 |
| 4103 | 0.50 | 0.45 | โ | โ | โ | 495.3 | Crossfield et al. 2016 | TICv8 |
| 4377 | 0.68 | 0.77 | โ | -0.71 | โ | 495.3 | TICv8 | TICv8 |
| 4415.5 | โ | 0.73 | โ | -0.74 | โ | 495.3 | Gaia DR2 | TICv8 |
| 4271 | โ | 0.66 | โ | โ | โ | 495.3 | Vanderburg et al. 2016 | TICv8 |
| 4377 | โ | 0.77 | โ | โ | โ | 495.3 | ExoFOP | TICv8 |
| 4262.1 | 0.68 | 0.69 | โ | โ | โ | 495.3 | Dressing et al. 2017 | TICv8 |