Rho Coronae Borealis b

Rho Coronae Borealis b ( ρ Coronae Borealis b ) is an extrasolar planet orbiting the yellow dwarf Rho Coronae Borealis all 39.8449 days. Due to its mass is assumed that it is a gas planet. The planet was in 1997 using the radial velocity method by Robert W. Noyes et al. discovered.

Circulation and mass

The planet orbits its star at a distance of about 0.2 astronomical units at an eccentricity of 0.06 and a minimum mass of about 1.1 Jupiter masses.