AN INTEGRATED APPROACH TO PLANETARY HABITABILITY ASSESSMENT FOCUSING ON ATMOSPHERIC COMPOSITION, SURFACE TEMPERATURE, AND POTENTIAL BIOSIGNATURE DETECTION ON EXOPLANETS

Abstract

The discovery of thousands of exoplanets has spurred interest in understanding planetary habitability. This paper explores an integrated approach for assessing habitability, focusing on atmospheric composition, surface temperature, and potential biosignature detection. By analyzing recent advancements in observational techniques and modeling, it identifies key parameters that contribute to habitability, including the presence of liquid water, stable atmospheres, and potential biosignatures like oxygen, methane, and other organics.