Multiple Star Systems
Multiple Star Systems
Single Stars (56%): The majority of stars in our galaxy are single stars, like our own Sun, which do not share their system with other stellar companions.
Binary Systems (33%): Comprising nearly a third of the galaxy's known star systems, binary stars are pairs of stars that orbit a common center of mass, demonstrating the dynamic nature of stellar relationships.
Triple Systems (8%): Less common are triple star systems, where three stars are gravitationally bound in a variety of orbital configurations, often presenting complex celestial mechanics.
Quadruple or More (3%): The rarest are systems with four or more stars, which highlight the incredible diversity and complexity possible within stellar formations.