HD 95872 b
Orbiting HD 95872
HD 95872 b is an exoplanet orbiting the star HD 95872, discovered in 2015 using the Radial Velocity method.
Minimum Mass (M sin i)
1188.68
Earth masses
Orbital Period
4375.0
days
Distance
72.2
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
1188.68
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Stassun et al. 2017
Orbital Period
4375.000+170.000−170.000days
Semi-Major Axis
5.1500+0.1600−0.1600au
M sin(i) (Earth masses)
1188.68+295.58−295.58
M sin(i) (Jupiter masses)
3.7400+0.9300−0.9300
Eccentricity
0.0600+0.0400−0.0400
Radial Velocity Semi-Amplitude
59.00+4.00−4.00m/s
Distance from Earth
72.2 pc (~236 ly)
Spectral Type
Unknown
Temperature
5312 K
Mass (Solar)
0.70 M☉
Radius (Solar)
0.84 R☉
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
165.8659°, -22.0943°
Discovery Method
Radial Velocity
Discovery Year
2015
Source ID: HD 95872 b
HD 95872 b orbits HD 95872 and was reported in 2015 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 1,188.68 Earth masses (M sin i) and an orbital period of 4,375 days.
Catalog data places the system at about 72.2 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 95872