 In addition, it may have disrupted the formation of terrestrial planets and reduced the delivery of water to any inner planets in the system.Therefore, planets located in the habitable zone of 47 Ursae Majoris are likely to be small and dry.It has been theorized that light reflections and infrared emissions from 47 UMa b, along with tidal influence, could warm any moons in orbit around it to be habitable, despite the planet being outside the normally accepted habitable zone.