Binary star systems consist of two stars orbiting a common center of mass, and they are crucial for understanding stellar masses and evolution. Observations of these systems can provide valuable insights into gravitational interactions and the life cycles of stars.

Binary Star Systems

Binary star systems

two stars

common center of mass

stellar masses

Stellar evolution is the process by which a star changes over the course of time, driven by nuclear fusion and gravitational forces. It encompasses a star's birth from a molecular cloud, its main sequence life, and its eventual death, which can lead to a supernova, white dwarf, neutron star, or black hole, depending on its initial mass.

Stellar Evolution

Gravitational interactions are fundamental forces of nature that govern the attraction between masses, influencing the structure and dynamics of the universe from galaxies to everyday objects on Earth. These interactions are described by Einstein's General Theory of Relativity, which explains gravity as the curvature of spacetime caused by mass and energy.

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