HD 33564 b

HD 33564 b is an exoplanet that orbits the main sequence star HD 33564 every 388 days . Due to its high mass , it is assumed that it is a gas planet .

discovery

The planet was determined using the radial velocity method by Franck Galland et al. discovered in 2005 .

Circulation and mass

The planet orbits its star at a distance of approx. 1.12 astronomical units and has a mass of approx. 2902 earth masses or 9.13 Jupiter masses.

Web links

• The exoplanet in the "Encyclopedia of Extrasolar Planets"