Temperature
4847.4 K
4847 to 4921.2
K0 • 162.6 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: Lee et al. 2015 • System source: TICv8
Temperature
4847.4 K
4847 to 4921.2
Mass
1.80 Msun
1.44 to 1.80
Radius
9.90 Rsun
9.90 to 10.73
Age
1.70 Gyr
single adopted value
Distance
162.6 pc
single adopted value
Spectral Type
K0
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 9.90 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
8 UMi
9.90 R☉
System Layout
1 planets linked to this host
Radial Velocity
Discovery
2015
Period
93.31 days
Radius
—
Mass
524.4 M⊕
Eq. Temp
—
8 UMi is a K0 star 530 light-years away with one known planet. The star is 1.7 billion years old, has a mass of 1.8 solar masses, and a radius of 9.9 solar radii. Its temperature of 4850 K is cooler than the Sun's, and both its mass and radius estimates are larger than the Sun's.
The planet, 8 UMi b, was discovered in 2015 using the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion. It has a minimum mass of 524 Earth masses and an orbital period of 93.3 days. That minimum mass is larger than Earth's and roughly 1.65 times Jupiter's mass.
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 |
|---|---|---|---|---|---|---|---|---|
| 4921.2 | — | 10.03 | — | 1.73 | — | 162.6 | Gaia DR2 | TICv8 |
| 4847 | 1.51 | 10.73 | — | 1.72 | — | 162.6 | Hon et al. 2023 | TICv8 |
| 4906 | — | 10.15 | — | — | — | 162.6 | TICv8 | TICv8 |
| — | — | — | — | — | K0 | 162.6 | Cannon & Pickering 1918 | TICv8 |
| 4847.4 | 1.80 | 9.90 | 1.70 | — | K0 | 162.6 | Lee et al. 2015 | TICv8 |
| 4847 | 1.44 | 10.30 | — | — | — | 162.6 | Stassun et al. 2017 | TICv8 |