HD 60292 b
Orbiting HD 60292
HD 60292 b is an exoplanet orbiting the star HD 60292, discovered in 2020 using the Radial Velocity method.
Minimum Mass (M sin i)
2065.89
Earth masses
Orbital Period
495.4
days
Distance
315.2
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
2065.89
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Lee et al. 2020
Orbital Period
495.400+3.000−3.000days
Semi-Major Axis
1.5000+0.1000−0.1000au
M sin(i) (Earth masses)
2065.89+317.83−317.83
M sin(i) (Jupiter masses)
6.5000+1.0000−1.0000
Eccentricity
0.2700+0.1000−0.1000
Epoch of Periastron
2455773.70+19.40−19.40days(JD)
Argument of Periastron
83.5+14.2−14.2deg
Radial Velocity Semi-Amplitude
120.00+15.30−15.30m/s
Distance from Earth
315.2 pc (~1028 ly)
Spectral Type
K0 III
Temperature
4348 K
Mass (Solar)
1.70 M☉
Radius (Solar)
27.00 R☉
Luminosity
2.39 log L☉
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
114.6202°, 66.2351°
Discovery Method
Radial Velocity
Discovery Year
2020
Source ID: HD 60292 b
HD 60292 b orbits HD 60292 and was reported in 2020 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 2,065.9 Earth masses (M sin i) and an orbital period of 495.4 days.
Catalog data places the system at about 315.2 parsecs from Earth, a host star classified as K0 III, 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 60292