HD 168009 b
Orbiting HD 168009
HD 168009 b is an exoplanet orbiting the star HD 168009, discovered in 2021 using the Radial Velocity method.
Minimum Mass (M sin i)
9.53
Earth masses
Orbital Period
15.1
days
Distance
23.3
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
9.53
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Rosenthal et al. 2021
Orbital Period
15.148+0.004−0.004days
Semi-Major Axis
0.1192+0.0017−0.0018au
M sin(i) (Earth masses)
9.53+1.21−1.18
M sin(i) (Jupiter masses)
0.0300+0.0038−0.0037
Eccentricity
0.1200+0.1100−0.0820
Argument of Periastron
13.2+45.8−63.0deg
Radial Velocity Semi-Amplitude
2.53+0.31−0.30m/s
Distance from Earth
23.3 pc (~76 ly)
Spectral Type
Unknown
Temperature
5778 K
Mass (Solar)
0.99 M☉
Radius (Solar)
1.21 R☉
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
273.8848°, 45.2088°
Discovery Method
Radial Velocity
Discovery Year
2021
Source ID: HD 168009 b
HD 168009 b orbits HD 168009 and was reported in 2021 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 9.53 Earth masses (M sin i) and an orbital period of 15.15 days.
Catalog data places the system at about 23.3 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 168009