HD 76920 b
Orbiting HD 76920
HD 76920 b is an exoplanet orbiting the star HD 76920, discovered in 2017 using the Radial Velocity method.
Minimum Mass (M sin i)
994.80
Earth masses
Orbital Period
415.9
days
Distance
184.0
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
994.80
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Bergmann et al. 2021
Orbital Period
415.891+0.043−0.039days
Semi-Major Axis
1.0910+0.0680−0.0770au
M sin(i) (Earth masses)
994.80+130.31−136.67
M sin(i) (Jupiter masses)
3.1300+0.4100−0.4300
Eccentricity
0.8782+0.0025−0.0025
Epoch of Periastron
2454812.47+0.30−0.33days(BJD)
Argument of Periastron
1.2+1.0−1.0deg
Radial Velocity Semi-Amplitude
178.10+2.70−2.60m/s
Distance from Earth
184.0 pc (~600 ly)
Spectral Type
Unknown
Temperature
4664 K
Mass (Solar)
1.00 M☉
Radius (Solar)
8.33 R☉
Luminosity
1.47 log L☉
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
133.8204°, -67.2654°
Discovery Method
Radial Velocity
Discovery Year
2017
Source ID: HD 76920 b
HD 76920 b orbits HD 76920 and was reported in 2017 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 994.8 Earth masses (M sin i) and an orbital period of 415.89 days.
Catalog data places the system at about 184 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 76920