HD 144899 b
Orbiting HD 144899
HD 144899 b is an exoplanet orbiting the star HD 144899, discovered in 2022 using the Radial Velocity method.
Minimum Mass (M sin i)
20.34
Earth masses
Orbital Period
40.4
days
Distance
115.7
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
20.34
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Feng et al. 2022
Orbital Period
40.439+0.031−0.050days
Semi-Major Axis
0.2420+0.0110−0.0120au
M sin(i) (Earth masses)
20.34+6.67−5.09
M sin(i) (Jupiter masses)
0.0640+0.0210−0.0160
Eccentricity
0.8210+0.0780−0.1710
Epoch of Periastron
2453156.30+3.22−2.64days(BJD)
Argument of Periastron
113.6+1.4−1.6deg
Radial Velocity Semi-Amplitude
6.01+0.07−0.07m/s
Distance from Earth
115.7 pc (~377 ly)
Spectral Type
Unknown
Temperature
Unknown
Mass (Solar)
1.16 M☉
Radius (Solar)
Unknown
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
242.5721°, -47.9147°
Discovery Method
Radial Velocity
Discovery Year
2022
Source ID: HD 144899 b
HD 144899 b orbits HD 144899 and was reported in 2022 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 20.34 Earth masses (M sin i) and an orbital period of 40.44 days.
Catalog data places the system at about 115.7 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 144899