HD 35759 b
Orbiting HD 35759
HD 35759 b is an exoplanet orbiting the star HD 35759, discovered in 2016 using the Radial Velocity method.
Minimum Mass (M sin i)
1195.04
Earth masses
Orbital Period
82.5
days
Distance
71.2
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
1195.04
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Hébrard et al. 2016
Orbital Period
82.467+0.019−0.019days
Semi-Major Axis
0.3890+0.0090−0.0090au
M sin(i) (Earth masses)
1195.04+54.03−54.03
M sin(i) (Jupiter masses)
3.7600+0.1700−0.1700
Eccentricity
0.3890+0.0060−0.0060
Epoch of Periastron
2456469.72+0.24−0.24days(BJD)
Argument of Periastron
-104.0+1.3−1.3deg
Radial Velocity Semi-Amplitude
173.90+1.30−1.30m/s
Distance from Earth
71.2 pc (~232 ly)
Spectral Type
G0
Temperature
6060 K
Mass (Solar)
1.15 M☉
Radius (Solar)
Unknown
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
82.8887°, 64.3184°
Discovery Method
Radial Velocity
Discovery Year
2016
Source ID: HD 35759 b
HD 35759 b orbits HD 35759 and was reported in 2016 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 1,195.04 Earth masses (M sin i) and an orbital period of 82.47 days.
Catalog data places the system at about 71.2 parsecs from Earth, a host star classified as G0, 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 35759