HD 103949 b
Orbiting HD 103949
HD 103949 b is an exoplanet orbiting the star HD 103949, discovered in 2019 using the Radial Velocity method.
Minimum Mass (M sin i)
11.20
Earth masses
Orbital Period
120.9
days
Distance
26.5
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
11.20
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Feng et al. 2019
Orbital Period
120.878+0.446−0.446days
Semi-Major Axis
0.4390+0.0090−0.0090au
M sin(i) (Earth masses)
11.20+2.30−2.30
M sin(i) (Jupiter masses)
0.0352+0.0072−0.0072
Eccentricity
0.1900+0.1200−0.1200
Argument of Periastron
127.7+68.3−68.3deg
Radial Velocity Semi-Amplitude
1.77+0.35−0.35m/s
Distance from Earth
26.5 pc (~86 ly)
Spectral Type
K3 V
Temperature
4792 K
Mass (Solar)
0.77 M☉
Radius (Solar)
Unknown
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
179.5480°, -23.9241°
Discovery Method
Radial Velocity
Discovery Year
2019
Source ID: HD 103949 b
HD 103949 b orbits HD 103949 and was reported in 2019 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 11.2 Earth masses (M sin i) and an orbital period of 120.88 days.
Catalog data places the system at about 26.5 parsecs from Earth, a host star classified as K3 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 103949