HD 37605 b

HD 37605 b is an extrasolar planet that orbits the 37605 main sequence star HD with an orbital period of 54.2 days.

The object was made using the radial velocity method of Cochran et al. discovered in 2004. The semi-major axis of the orbit is approximately 0.26 astronomical units, their eccentricity of 0.74. The minimum mass of the exoplanet is about 2.9 Jupiter masses (about 900 Earth masses ).