General Relativity May Account for Scarcity of Planets in Binary Systems

Scientists have long observed a surprising lack of planets orbiting close binary star systems. New research proposes that Albert Einstein's theory of general relativity could provide an explanation for this phenomenon. Detailed calculations suggest that relativistic effects can destabilize planetary orbits around tight binary stars, potentially causing planets to be ejected or destroyed over time. This offers a novel perspective on the distribution of exoplanets in such environments.