HD 29399 b
Orbiting HD 29399
HD 29399 b is an exoplanet orbiting the star HD 29399, discovered in 2022 using the Radial Velocity method.
Minimum Mass (M sin i)
498.99
Earth masses
Orbital Period
892.7
days
Distance
44.2
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
498.99
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Pezzotti et al. 2022
Orbital Period
892.700+5.900−5.900days
Semi-Major Axis
1.9130+0.0080−0.0080au
M sin(i) (Earth masses)
498.99+34.96−34.96
M sin(i) (Jupiter masses)
1.5700+0.1100−0.1100
Eccentricity
0.0500+0.0500−0.0500
Epoch of Periastron
2455965.00+210.00−210.00days(BJD)
Argument of Periastron
-13.1+85.1−85.1deg
Radial Velocity Semi-Amplitude
29.90+2.20−2.20m/s
Distance from Earth
44.2 pc (~144 ly)
Spectral Type
K1 III
Temperature
4845 K
Mass (Solar)
1.17 M☉
Radius (Solar)
4.50 R☉
Luminosity
1.00 log L☉
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
68.3903°, -62.8238°
Discovery Method
Radial Velocity
Discovery Year
2022
Source ID: HD 29399 b
HD 29399 b orbits HD 29399 and was reported in 2022 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 498.99 Earth masses (M sin i) and an orbital period of 892.7 days.
Catalog data places the system at about 44.2 parsecs from Earth, a host star classified as K1 III, 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 29399