HD 125612 b

HD 125612 b is an exoplanet that orbits the yellow dwarf HD 125612 every 502 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 Debra Fischer et al. discovered in 2007 .

Circulation and mass

The planet orbits its star at a distance of approx. 1.2 astronomical units and has a mass of approx. 1017 earth masses or 3.2 Jupiter masses.

Web links

• The exoplanet in the "Encyclopedia of Extrasolar Planets"