Galaxy Evolution | Vibepedia

Galaxy evolution is the study of how galaxies formed, changed, and diversified over billions of years, from the homogeneous universe after the Big Bang to the complex, heterogeneous cosmos we observe today. The Lambda-CDM model, supported by hydrodynamics simulations, suggests that galaxy formation and evolution are driven by the clustering and merging of matter, influenced by both baryons and dark matter. Researchers like Neil deGrasse Tyson, Brian Greene, and Lisa Randall have contributed significantly to our understanding of galaxy evolution, often leveraging tools like the Hubble Space Telescope and computational platforms like NASA's Astrophysics Data System.