HD 114783 b

HD 114783 b is an exoplanet, of the main sequence star HD 114783 orbits every 496.9 days. Due to its high mass is assumed that it is a gas planet.

Discovery

As the majority of exoplanets discovered also that using the radial velocity method, and indeed in 2001 by Paul Butler, Geoffrey Marcy, Steven S. Vogt et al.

Circulation and mass

The planet orbits its star at a distance of approximately 1.17 astronomical units and has a mass of about 327.4 Earth masses and 1.03 Jupiter masses.