NASA’s Neil Gehrels Swift Observatory has made a groundbreaking discovery by detecting hydroxyl (OH) molecules, a chemical signature of water, in comet 3I/ATLAS, an interstellar comet passing through our solar system. This marks a significant milestone in our understanding of the composition and chemistry of comets originating beyond our solar system. 3I/ATLAS, discovered in July 2025, is only the third confirmed interstellar object observed within our solar system, following 1I/ʻOumuamua and 2I/Borisov. The presence of hydroxyl molecules signifies that 3I/ATLAS contains water ice, which sublimates to water vapor that then dissociates under solar radiation into hydroxyl gas. This finding is important for planetary science as it provides insight into the materials and conditions of cometary bodies formed in other star systems. Such knowledge has broad implications for theories of planetary formation and the distribution of water in the galaxy, which in turn relates to the potential for extraterrestrial life. Observations by Swift, complemented by data from other space telescopes like Hubble and Webb, revealed that 3I/ATLAS's nucleus is likely less than 1 km in diameter but rich in volatile compounds including water vapor, carbon dioxide, and carbon monoxide. This composition is somewhat similar to comets formed in our solar system, deepening our understanding of the commonality and diversity of cometary bodies across the cosmos. The detection of hydroxyl water molecules in 3I/ATLAS highlights the comet's active nature and opens new avenues for studying water delivery processes beyond Earth’s vicinity, fostering advancements in astrobiology and comparative planetology.