HD 96992 b
Orbiting HD 96992
HD 96992 b is an exoplanet orbiting the star HD 96992, discovered in 2021 using the Radial Velocity method.
Minimum Mass (M sin i)
362.33
Earth masses
Orbital Period
514.0
days
Distance
396.1
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
362.33
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Niedzielski et al. 2021
Orbital Period
514.000+4.000−4.000days
Semi-Major Axis
1.2400+0.0500−0.0500au
M sin(i) (Earth masses)
362.33+98.53−98.53
M sin(i) (Jupiter masses)
1.1400+0.3100−0.3100
Eccentricity
0.4100+0.2400−0.1200
Epoch of Periastron
2453620.50+30.00−40.00days(JD)
Argument of Periastron
149.0+24.0−31.0deg
Radial Velocity Semi-Amplitude
33.00+3.00−3.00m/s
Distance from Earth
396.1 pc (~1292 ly)
Spectral Type
Unknown
Temperature
4725 K
Mass (Solar)
0.96 M☉
Radius (Solar)
7.43 R☉
Luminosity
1.47 log L☉
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
167.5966°, 43.9190°
Discovery Method
Radial Velocity
Discovery Year
2021
Source ID: HD 96992 b
HD 96992 b orbits HD 96992 and was reported in 2021 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 362.33 Earth masses (M sin i) and an orbital period of 514 days.
Catalog data places the system at about 396.1 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 96992