HD 103197 b
Orbiting HD 103197
HD 103197 b is an exoplanet orbiting the star HD 103197, discovered in 2011 using the Radial Velocity method.
Minimum Mass (M sin i)
28.60
Earth masses
Orbital Period
47.8
days
Distance
57.1
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
28.60
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Stassun et al. 2017
Orbital Period
47.840+0.030−0.030days
Semi-Major Axis
0.2500+0.0000−0.0000au
M sin(i) (Earth masses)
28.60+6.36−6.36
M sin(i) (Jupiter masses)
0.0900+0.0200−0.0200
Eccentricity
0.0000
Radial Velocity Semi-Amplitude
5.90+0.30−0.30m/s
Distance from Earth
57.1 pc (~186 ly)
Spectral Type
Unknown
Temperature
5250 K
Mass (Solar)
0.80 M☉
Radius (Solar)
0.88 R☉
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
178.2202°, -50.2928°
Discovery Method
Radial Velocity
Discovery Year
2011
Source ID: HD 103197 b
HD 103197 b orbits HD 103197 and was reported in 2011 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 28.6 Earth masses (M sin i) and an orbital period of 47.84 days.
Catalog data places the system at about 57.1 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 103197