In a recent breakthrough, scientists have identified the presence of carbon dioxide and hydrogen peroxide on Charon, the largest moon of Pluto. These findings are significant in unraveling the mysteries of icy body origins and evolution in the outer regions of our Solar System. Charon, initially discovered in 1978, has been under scrutiny due to its extreme cold temperatures and icy composition, making it inhospitable for life. The research, conducted by a team led by researchers at the Southwest Research Institute in the US, highlights the unique detection of these gases on Charon for the first time. As ice on Charon interacts with charged particles, hydrogen and oxygen atoms combine to form hydrogen peroxide, a reactive compound with various industrial applications. The utilization of NASA's James Webb Telescope enabled scientists to study Charon's surface in previously unattainable wavelengths, enhancing their understanding of the moon's composition. Lead author Silvia Protopapa suggested that the carbon dioxide layer on Charon likely originated from its interior and was exposed through cratering events. Moreover, the presence of hydrogen peroxide indicates surface alterations influenced by solar radiation and cosmic rays. This study, published in Nature Communications, underscores the continuous advancements in space exploration and the critical role of technological innovation in unraveling celestial mysteries.