HD 48265 b
Orbiting HD 48265
HD 48265 b is an exoplanet orbiting the star HD 48265, discovered in 2008 using the Radial Velocity method.
Minimum Mass (M sin i)
484.69
Earth masses
Orbital Period
778.5
days
Distance
90.5
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
484.69
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Barbato et al. 2018
Orbital Period
778.510+5.380−5.180days
Semi-Major Axis
1.8140+0.0300−0.0310au
M sin(i) (Earth masses)
484.69+15.57−15.89
M sin(i) (Jupiter masses)
1.5250+0.0490−0.0500
Eccentricity
0.2110+0.0890−0.0960
Epoch of Periastron
2456036.70+67.70−36.50days(BJD)
Argument of Periastron
308.3+21.3−23.1deg
Radial Velocity Semi-Amplitude
28.65+1.59−1.57m/s
Distance from Earth
90.5 pc (~295 ly)
Spectral Type
Unknown
Temperature
5733 K
Mass (Solar)
1.31 M☉
Radius (Solar)
1.90 R☉
Luminosity
Unknown
Planets in System
2
Stars in System
1
Coordinates (RA, Dec)
100.0074°, -48.5418°
Discovery Method
Radial Velocity
Discovery Year
2008
Source ID: HD 48265 b
HD 48265 b orbits HD 48265 and was reported in 2008 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 484.69 Earth masses (M sin i) and an orbital period of 778.51 days.
Catalog data places the system at about 90.5 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 48265More planets in this system