HD 34445

HD 34445 is a G0V-type star located approximately 150 light-years away in the constellation Orion. It is slightly more massive and luminous than our Sun.

HD 34445 is notable for hosting a system of multiple exoplanets. As of the most recent data, six planets have been confirmed orbiting the star. These planets are all gas giants, and their masses range from that of Neptune to several times the mass of Jupiter. The planets orbit at varying distances from the star, with orbital periods ranging from less than a year to several years.

The discovery of this multi-planetary system contributes significantly to our understanding of planet formation and the prevalence of such systems around Sun-like stars. The complex orbital dynamics of the planets also provide valuable insights into the processes that shape planetary systems. Studies of HD 34445 continue to refine our knowledge of the system's architecture and the characteristics of its constituent planets.