HD 17092 b
Orbiting HD 17092
HD 17092 b is an exoplanet orbiting the star HD 17092, discovered in 2007 using the Radial Velocity method.
Minimum Mass (M sin i)
3219.62
Earth masses
Orbital Period
359.9
days
Distance
228.4
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
3219.62
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Stassun et al. 2017
Orbital Period
359.900+2.400−2.400days
Semi-Major Axis
1.3100+0.0600−0.0600au
M sin(i) (Earth masses)
3219.62+727.83−727.83
M sin(i) (Jupiter masses)
10.1300+2.2900−2.2900
Eccentricity
0.1700+0.0500−0.0500
Radial Velocity Semi-Amplitude
82.40+3.20−3.20m/s
Distance from Earth
228.4 pc (~745 ly)
Spectral Type
Unknown
Temperature
4326 K
Mass (Solar)
6.73 M☉
Radius (Solar)
13.58 R☉
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
41.5924°, 49.6530°
Discovery Method
Radial Velocity
Discovery Year
2007
Source ID: HD 17092 b
HD 17092 b orbits HD 17092 and was reported in 2007 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 3,219.62 Earth masses (M sin i) and an orbital period of 359.9 days.
Catalog data places the system at about 228.4 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 17092