HD 96167 b
Orbiting HD 96167
HD 96167 b is an exoplanet orbiting the star HD 96167, discovered in 2009 using the Radial Velocity method.
Minimum Mass (M sin i)
227.88
Earth masses
Orbital Period
498.0
days
Distance
85.3
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
227.88
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Luhn et al. 2019
Orbital Period
498.040+0.760−0.760days
Semi-Major Axis
1.3320+0.0980−0.0980au
M sin(i) (Earth masses)
227.88+12.71−12.71
M sin(i) (Jupiter masses)
0.7170+0.0400−0.0400
Eccentricity
0.6850+0.0290−0.0290
Epoch of Periastron
2453061.10+4.40−4.40days(JD)
Argument of Periastron
290.1+6.1−6.1deg
Radial Velocity Semi-Amplitude
21.50+1.40−1.40m/s
Distance from Earth
85.3 pc (~278 ly)
Spectral Type
Unknown
Temperature
5733 K
Mass (Solar)
1.27 M☉
Radius (Solar)
1.94 R☉
Luminosity
Unknown
Planets in System
1
Stars in System
2
Coordinates (RA, Dec)
166.3126°, -10.2913°
Discovery Method
Radial Velocity
Discovery Year
2009
Source ID: HD 96167 b
HD 96167 b orbits HD 96167 and was reported in 2009 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 227.88 Earth masses (M sin i) and an orbital period of 498.04 days.
Catalog data places the system at about 85.3 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 96167