HD 13167 b
Orbiting HD 13167
HD 13167 b is an exoplanet orbiting the star HD 13167, discovered in 2018 using the Radial Velocity method.
Minimum Mass (M sin i)
1052.02
Earth masses
Orbital Period
2613.0
days
Distance
148.9
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
1052.02
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Luhn et al. 2019
Orbital Period
2613.000+17.000−17.000days
Semi-Major Axis
4.1000+0.3400−0.3400au
M sin(i) (Earth masses)
1052.02+50.85−50.85
M sin(i) (Jupiter masses)
3.3100+0.1600−0.1600
Eccentricity
0.5630+0.0330−0.0330
Epoch of Periastron
2462162.00+54.00−54.00days(JD)
Argument of Periastron
265.0+6.0−6.0deg
Radial Velocity Semi-Amplitude
48.20+2.70−2.70m/s
Distance from Earth
148.9 pc (~486 ly)
Spectral Type
Unknown
Temperature
5671 K
Mass (Solar)
1.35 M☉
Radius (Solar)
2.39 R☉
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
32.0576°, -24.6956°
Discovery Method
Radial Velocity
Discovery Year
2018
Source ID: HD 13167 b
HD 13167 b orbits HD 13167 and was reported in 2018 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 1,052.02 Earth masses (M sin i) and an orbital period of 2,613 days.
Catalog data places the system at about 148.9 parsecs from Earth and 1 known planet in the system.
Host star
Explore the stellar record for this system to compare temperature, spectral type, and known planets.
Open HD 13167