This document provides an overview of detecting planets beyond our solar system. It begins with distinguishing key differences between stars and planets, noting that planets do not shine on their own. It then discusses what makes a planet habitable, focusing on factors like liquid water, breathable air, and an atmosphere that protects from radiation. The document outlines several tools used to detect exoplanets, including spectrographic imaging to analyze atmospheric compositions, the radial velocity method that detects wobbles in star movements caused by planetary gravitational pulls, and the photometry method that monitors star brightness changes when planets pass between stars and observers. It concludes by noting the ongoing efforts to discover potentially habitable Earth-like planets outside our solar system.