Pluto's largest moon, Charon, has long intrigued scientists with its icy terrain and unusual characteristics. Recent research led by astronomer Silvia Protopapa revealed the presence of carbon dioxide and hydrogen peroxide on Charon's surface, offering key insights into the moon's composition and formation. Charon, smaller than Pluto but unique in its own right, orbits in a binary system with its parent body, showcasing a distinctive orbital dynamic. The discovery of carbon dioxide and hydrogen peroxide was made possible through data from NASA's James Webb Space Telescope, demonstrating the telescope's ability to detect crucial molecules on distant objects. Charon's composition, rich in water ice and other compounds, differs from that of Pluto and other trans-Neptunian objects, hinting at complex interactions in the outer Solar System. The newfound compounds provide researchers with valuable information about the moon's history and the processes shaping its surface. By studying Charon's composition, scientists aim to unravel the mysteries surrounding its formation, which could have implications for understanding other celestial bodies near Pluto. The ongoing exploration of Charon and its unique features promises to deepen our understanding of the distant realms of the Solar System and the fascinating worlds that inhabit them.