HD 32963 b
Orbiting HD 32963
HD 32963 b is an exoplanet orbiting the star HD 32963, discovered in 2015 using the Radial Velocity method.
Minimum Mass (M sin i)
222.48
Earth masses
Orbital Period
2372.0
days
Distance
38.1
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
222.48
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Rowan et al. 2016
Orbital Period
2372.000+26.000−26.000days
Semi-Major Axis
3.4100+0.0200−0.0200au
M sin(i) (Earth masses)
222.48+9.53−9.53
M sin(i) (Jupiter masses)
0.7000+0.0300−0.0300
Eccentricity
0.0700+0.0400−0.0400
Epoch of Periastron
2450532.00+324.00−324.00days
Argument of Periastron
107.0+35.0−35.0deg
Radial Velocity Semi-Amplitude
11.10+0.40−0.40m/s
Distance from Earth
38.1 pc (~124 ly)
Spectral Type
Unknown
Temperature
5727 K
Mass (Solar)
0.94 M☉
Radius (Solar)
Unknown
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
76.9820°, 26.3277°
Discovery Method
Radial Velocity
Discovery Year
2015
Source ID: HD 32963 b
HD 32963 b orbits HD 32963 and was reported in 2015 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 222.48 Earth masses (M sin i) and an orbital period of 2,372 days.
Catalog data places the system at about 38.1 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 32963