HIP 948 b
Orbiting HIP 948
HIP 948 b is an exoplanet orbiting the star HIP 948, discovered in 2022 using the Radial Velocity method.
Mass
6547.27
Earth masses
Orbital Period
24955.5
days
Distance
34.9
parsecs
Radius (Earth radii)
Unknown
Mass (Earth masses)
6547.27
Measured
Equilibrium Temperature
Unknown
Parameter source: Feng et al. 2022
Orbital Period
24955.458+8914.752−10015.463days
Semi-Major Axis
15.0370+3.3150−4.4640au
Planet Mass (Earth masses)
6547.27+3132.52−2705.67
Planet Mass (Jupiter masses)
20.6000+9.8560−8.5130
Eccentricity
0.2300+0.1610−0.1100
Epoch of Periastron
2446439.43+3339.39−4719.02days(BJD)
Argument of Periastron
117.4+27.8−17.6deg
Radial Velocity Semi-Amplitude
169.73+55.36−43.06m/s
Distance from Earth
34.9 pc (~114 ly)
Spectral Type
Unknown
Temperature
Unknown
Mass (Solar)
0.71 M☉
Radius (Solar)
Unknown
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
2.9276°, -39.2305°
Discovery Method
Radial Velocity
Discovery Year
2022
Source ID: HIP 948 b
HIP 948 b orbits HIP 948 and was reported in 2022 and was detected with the Radial Velocity method.
Published measurements list a mass of 6,547.27 Earth masses and an orbital period of 24,955.46 days.
Catalog data places the system at about 34.9 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 HIP 948