Galaxy Evolution News

Galaxy evolution is the study of how galaxies form and change over the course of the universe’s history. This complex process is influenced by various factors including gravitational interactions, mergers with other galaxies, and the internal processes of star formation and supernovae. Initially, galaxies begin as fluctuations in the density of matter in the early universe, which then collapse under gravity to form stars and eventually galaxies. Over billions of years, these galaxies undergo significant transformations — they may grow through the accumulation of gas from the intergalactic medium or through mergers with other galaxies, leading to new bursts of star formation.