  Galactic archaeology represents a multidisciplinary approach aimed at
unraveling the intricate history of the Milky Way galaxy through the study of
its stellar populations. This abstract delves into the significance of galactic
archaeology as a vital tool for understanding the formation and evolution of
the Milky Way. By examining the distribution, kinematics, chemical
compositions, and ages of stars within the galaxy, researchers gain insights
into the dynamic processes that have shaped its structure over billions of
years.
  Stellar populations serve as invaluable relics of past epochs, preserving
clues about the conditions prevalent during their formation. The utilization of
spectroscopic and photometric data has enabled the classification and analysis
of stars, allowing astronomers to discern distinct populations and unveil their
origin stories. Through these studies, the emergence of the Milky Way's various
components, such as the thin and thick disk, halo, and bulge, becomes
discernible.
