HD 21411 b
Orbiting HD 21411
HD 21411 b is an exoplanet orbiting the star HD 21411, discovered in 2019 using the Radial Velocity method.
Minimum Mass (M sin i)
65.90
Earth masses
Orbital Period
84.3
days
Distance
29.1
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
65.90
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Feng et al. 2019
Orbital Period
84.288+0.127−0.127days
Semi-Major Axis
0.3620+0.0070−0.0070au
M sin(i) (Earth masses)
65.90+25.60−25.60
M sin(i) (Jupiter masses)
0.2073+0.0805−0.0805
Eccentricity
0.4000+0.1500−0.1500
Argument of Periastron
332.4+17.7−17.7deg
Radial Velocity Semi-Amplitude
11.48+4.33−4.33m/s
Distance from Earth
29.1 pc (~95 ly)
Spectral Type
G8 V
Temperature
5605 K
Mass (Solar)
0.89 M☉
Radius (Solar)
Unknown
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
51.5474°, -30.6168°
Discovery Method
Radial Velocity
Discovery Year
2019
Source ID: HD 21411 b
HD 21411 b orbits HD 21411 and was reported in 2019 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 65.9 Earth masses (M sin i) and an orbital period of 84.29 days.
Catalog data places the system at about 29.1 parsecs from Earth, a host star classified as G8 V, 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 21411