HD 16417 b
Orbiting HD 16417
HD 16417 b is an exoplanet orbiting the star HD 16417, discovered in 2008 using the Radial Velocity method.
Minimum Mass (M sin i)
22.10
Earth masses
Orbital Period
17.2
days
Distance
25.4
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
22.10
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: O'Toole et al. 2009
Orbital Period
17.240+0.010−0.010days
Semi-Major Axis
0.1400+0.0100−0.0100au
M sin(i) (Earth masses)
22.10+2.00−2.00
M sin(i) (Jupiter masses)
0.0696+0.0063−0.0063
Eccentricity
0.2000+0.0900−0.0900
Epoch of Periastron
2450099.74+3.30−3.30days
Argument of Periastron
77.0+26.0−26.0deg
Radial Velocity Semi-Amplitude
5.00+0.40−0.40m/s
Distance from Earth
25.4 pc (~83 ly)
Spectral Type
G1 V
Temperature
Unknown
Mass (Solar)
1.20 M☉
Radius (Solar)
Unknown
Luminosity
Unknown
Planets in System
1
Stars in System
2
Coordinates (RA, Dec)
39.2441°, -34.5791°
Discovery Method
Radial Velocity
Discovery Year
2008
Source ID: HD 16417 b
HD 16417 b orbits HD 16417 and was reported in 2008 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 22.1 Earth masses (M sin i) and an orbital period of 17.24 days.
Catalog data places the system at about 25.4 parsecs from Earth, a host star classified as G1 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 16417