Temperature
5148 K
5078 to 5148
K2 โข 22.52 pc
Records
10
literature rows
Planets
2
system count
References
11
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: Turnbull 2015 โข System source: TICv8
Temperature
5148 K
5078 to 5148
Mass
0.90 Msun
0.85 to 0.90
Radius
0.87 Rsun
0.87 to 0.89
Age
9.40 Gyr
8.68 to 9.40
Luminosity
-0.26 log(Lsun)
-0.32 to -0.26
Distance
22.52 pc
single adopted value
Spectral Type
K2
Multiple classifications reported
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 0.87 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
HD 18143
0.87 Rโ
System Layout
2 planets linked to this host
Radial Velocity
Discovery
2022
Period
10.29 days
Radius
โ
Mass
10.81 Mโ
Eq. Temp
โ
Radial Velocity
Discovery
2022
Period
2.90e4 days
Radius
โ
Mass
3177.6 Mโ
Eq. Temp
โ
HD 18143 is a K2 star 73.5 light-years away with two planets orbiting it. The star is 9.4 billion years old, holds 0.9 solar masses, spans 0.87 solar radii, and has a temperature of 5150 K. Its mass and radius are smaller than the Sun's, and its temperature is cooler.
Both planets were found in 2022 using the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion. HD 18143 b has a minimum mass of 10.8 Earth masses, meaning its true mass is at least that much, and it completes an orbit every 10.3 days, the shortest period among the listed planets. HD 18143 b's minimum mass is larger than Earth's. HD 18143 c carries a mass of 3180 Earth masses, roughly 10 times Jupiter's mass and larger than Earth's, and its orbital period is 29000 days, the longest among the listed planets.
Provenance
Evidence Summary
Rows
10
Stellar refs
10
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| โ | 0.90 | 0.87 | 8.68 | โ | โ | 22.52 | Takeda et al. 2007 | TICv8 |
| 5148 | 0.90 | 0.87 | 9.40 | -0.26 | K2 | 22.52 | Turnbull 2015 | TICv8 |
| โ | 0.85 | โ | โ | โ | โ | 22.52 | Feng et al. 2022 | TICv8 |
| โ | โ | โ | โ | โ | K2 IV | 22.52 | Gray et al. 2003 | TICv8 |
| โ | โ | โ | โ | โ | โ | 22.52 | Valenti & Fischer 2005 | TICv8 |
| โ | โ | โ | โ | โ | G5 | 22.52 | Cannon & Pickering 1918 | TICv8 |
| โ | โ | โ | โ | โ | โ | 22.52 | Nidever et al. 2002 | TICv8 |
| โ | โ | โ | โ | โ | โ | 22.52 | Duncan et al. 1991 | TICv8 |
| 5078 | 0.85 | 0.89 | โ | -0.32 | โ | 22.52 | TICv8 | TICv8 |
| โ | โ | โ | โ | โ | โ | 22.52 | Wright et al. 2004 | TICv8 |