Astronomers find exoplanets by detecting changes in electromagnetic radiation patterns from stars, which indicate the presence of planets. Current methods favor the discovery of large planets close to their stars, leading to the identification of many 'hot Jupiters' and 'wandering Neptunes.' Understanding the size and atmosphere of these exoplanets involves analyzing light spectra. While powerful telescopes can only view stars as pinpricks, advancements in imaging technology may eventually allow for detailed surface observations of exoplanets. Public resources, such as libraries, offer extensive information on exoplanet discoveries and their implications for our understanding of the universe.