HD 213519 b
Orbiting HD 213519
HD 213519 b is an exoplanet orbiting the star HD 213519, discovered in 2022 using the Radial Velocity method.
Minimum Mass (M sin i)
9.22
Earth masses
Orbital Period
11.1
days
Distance
41.0
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
9.22
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Feng et al. 2022
Orbital Period
11.122+0.001−0.001days
Semi-Major Axis
0.0990+0.0040−0.0040au
M sin(i) (Earth masses)
9.22+2.86−1.27
M sin(i) (Jupiter masses)
0.0290+0.0090−0.0040
Eccentricity
0.4130+0.1720−0.1440
Epoch of Periastron
2430050.45+842.87−1328.19days(BJD)
Argument of Periastron
35.6+21.7−16.7deg
Radial Velocity Semi-Amplitude
2.81+1.42−0.39m/s
Distance from Earth
41.0 pc (~134 ly)
Spectral Type
Unknown
Temperature
Unknown
Mass (Solar)
1.05 M☉
Radius (Solar)
Unknown
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
337.7728°, 45.1452°
Discovery Method
Radial Velocity
Discovery Year
2022
Source ID: HD 213519 b
HD 213519 b orbits HD 213519 and was reported in 2022 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 9.22 Earth masses (M sin i) and an orbital period of 11.12 days.
Catalog data places the system at about 41 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 213519