On the Physical Properties of G-Type Main Sequence Stars

Bijan Nikouravan; Misha Nikouravan

doi:10.14331/ijfps.2023.330159

Authors

Bijan Nikouravan Department of Physics, Islamic Azad University (IAU), Varamin, Pishva Branch, Iran Author https://orcid.org/0000-0003-4308-1632 (unauthenticated)
Misha Nikouravan Department of Mechanical Engineering, Sharif University of Technology, Kish International Campus, Iran Author https://orcid.org/0000-0003-1976-8848 (unauthenticated)

DOI:

https://doi.org/10.14331/ijfps.2023.330159

Keywords:

Steller Classifications, G-Type main sequence stars, New discovered exoplanets

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.

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