HD 92788 b
HD 92788 b is an exoplanet that orbits the yellow dwarf HD 92788 every 325.81 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 2000 .
Circulation and mass
The planet orbits its star at a distance of approx. 0.965 astronomical units and has a mass of approx. 1167 earth masses or 3.67 Jupiter masses.
Web links
- The exoplanet in the "Encyclopedia of Extrasolar Planets"