On the Physical Properties of G-Type Main ‎Sequence Stars

Abstract

This research focuses on the classification and properties of G-Type main sequence stars. It discusses the historical ‎‎development of star classification systems and their importance in understanding stellar evolution, composition, ‎and galactic ‎structures. The paper also examines the mass-radius and mass-luminosity relationships of stars, ‎highlighting the strong positive ‎correlations between mass and radius, as well as mass and luminosity. The findings ‎suggest that more massive stars tend to be ‎larger and more luminous. However, further analysis is needed to explore ‎the underlying relationships between these variables.‎‎