HD 60532 b
Orbiting HD 60532
HD 60532 b is an exoplanet orbiting the star HD 60532, discovered in 2008 using the Radial Velocity method.
Minimum Mass (M sin i)
336.90
Earth masses
Orbital Period
201.9
days
Distance
26.0
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
336.90
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Borgniet et al. 2017
Orbital Period
201.900+0.300−0.300days
Semi-Major Axis
0.7700+0.0200−0.0200au
M sin(i) (Earth masses)
336.90+25.43−25.43
M sin(i) (Jupiter masses)
1.0600+0.0800−0.0800
Eccentricity
0.2600+0.0200−0.0200
Epoch of Periastron
2454594.70+2.80−2.80days(BJD)
Argument of Periastron
-3.7+5.7−5.7deg
Radial Velocity Semi-Amplitude
29.10+0.90−0.90m/s
Distance from Earth
26.0 pc (~85 ly)
Spectral Type
Unknown
Temperature
6245 K
Mass (Solar)
1.50 M☉
Radius (Solar)
2.57 R☉
Luminosity
Unknown
Planets in System
2
Stars in System
1
Coordinates (RA, Dec)
113.5131°, -22.2959°
Discovery Method
Radial Velocity
Discovery Year
2008
Source ID: HD 60532 b
HD 60532 b orbits HD 60532 and was reported in 2008 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 336.9 Earth masses (M sin i) and an orbital period of 201.9 days.
Catalog data places the system at about 26 parsecs from Earth and 2 known planets in the system.
Host star
Explore the stellar record for this system to compare temperature, spectral type, and known planets.
Open HD 60532More planets in this system