HD 109749 b

HD 109749 b is an exoplanet that orbits the yellow subgiant HD 109749 every 5.23947 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 2005 .

Circulation and mass

The planet orbits its star at a distance of approx. 0.0629 astronomical units and has a mass of approx. 88.06 Earth masses and 0.277 Jupiter masses.

Web links

• The exoplanet in the "Encyclopedia of Extrasolar Planets"