HD 63765 b
Orbiting HD 63765
HD 63765 b is an exoplanet orbiting the star HD 63765, discovered in 2011 using the Radial Velocity method.
Minimum Mass (M sin i)
168.45
Earth masses
Orbital Period
358.0
days
Distance
32.5
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
168.45
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Stassun et al. 2017
Orbital Period
358.000+1.000−1.000days
Semi-Major Axis
0.9400+0.0200−0.0200au
M sin(i) (Earth masses)
168.45+9.53−9.53
M sin(i) (Jupiter masses)
0.5300+0.0300−0.0300
Eccentricity
0.2400+0.0400−0.0400
Radial Velocity Semi-Amplitude
20.90+1.30−1.30m/s
Distance from Earth
32.5 pc (~106 ly)
Spectral Type
Unknown
Temperature
5449 K
Mass (Solar)
0.65 M☉
Radius (Solar)
0.83 R☉
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
116.9583°, -54.2653°
Discovery Method
Radial Velocity
Discovery Year
2011
Source ID: HD 63765 b
HD 63765 b orbits HD 63765 and was reported in 2011 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 168.45 Earth masses (M sin i) and an orbital period of 358 days.
Catalog data places the system at about 32.5 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 63765