HD 50499 c
Orbiting HD 50499
HD 50499 c is an exoplanet orbiting the star HD 50499, discovered in 2019 using the Radial Velocity method.
Minimum Mass (M sin i)
931.24
Earth masses
Orbital Period
8619.9
days
Distance
46.3
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
931.24
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Rickman et al. 2019
Orbital Period
8619.900+2622.495−405.428days
Semi-Major Axis
9.0200+1.7300−0.3300au
M sin(i) (Earth masses)
931.24+232.02−57.21
M sin(i) (Jupiter masses)
2.9300+0.7300−0.1800
Eccentricity
0.0000+0.1400−0.0200
Epoch of Periastron
2461832.00+3731.00−2885.00days(BJD)
Argument of Periastron
23.0+138.0−138.0deg
Radial Velocity Semi-Amplitude
24.23+3.79−0.95m/s
Distance from Earth
46.3 pc (~151 ly)
Spectral Type
G1 V
Temperature
6099 K
Mass (Solar)
1.31 M☉
Radius (Solar)
1.42 R☉
Luminosity
Unknown
Planets in System
2
Stars in System
1
Coordinates (RA, Dec)
103.0081°, -33.9153°
Discovery Method
Radial Velocity
Discovery Year
2019
Source ID: HD 50499 c
HD 50499 c orbits HD 50499 and was reported in 2019 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 931.24 Earth masses (M sin i) and an orbital period of 8,619.9 days.
Catalog data places the system at about 46.3 parsecs from Earth, a host star classified as G1 V, 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 50499More planets in this system