HD 95089 c
Orbiting HD 95089
HD 95089 c is an exoplanet orbiting the star HD 95089, discovered in 2016 using the Radial Velocity method.
Minimum Mass (M sin i)
1096.51
Earth masses
Orbital Period
1785.0
days
Distance
137.0
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
1096.51
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Luhn et al. 2019
Orbital Period
1785.000+32.000−32.000days
Semi-Major Axis
3.3300+0.3100−0.3100au
M sin(i) (Earth masses)
1096.51+44.50−44.50
M sin(i) (Jupiter masses)
3.4500+0.1400−0.1400
Eccentricity
0.2840+0.0420−0.0420
Epoch of Periastron
2441170.00+260.00−260.00days(JD)
Argument of Periastron
66.0+10.0−10.0deg
Radial Velocity Semi-Amplitude
45.10+1.90−1.90m/s
Distance from Earth
137.0 pc (~447 ly)
Spectral Type
Unknown
Temperature
4918 K
Mass (Solar)
1.54 M☉
Radius (Solar)
5.08 R☉
Luminosity
Unknown
Planets in System
2
Stars in System
1
Coordinates (RA, Dec)
164.6987°, 1.7290°
Discovery Method
Radial Velocity
Discovery Year
2016
Source ID: HD 95089 c
HD 95089 c orbits HD 95089 and was reported in 2016 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 1,096.51 Earth masses (M sin i) and an orbital period of 1,785 days.
Catalog data places the system at about 137 parsecs from Earth and 2 known planets in the system.
Host star
Explore the stellar record for this system to compare temperature, spectral type, and known planets.
Open HD 95089More planets in this system