New observations from the James Webb Space Telescope (JWST) have revealed that a star called IRS 3, located just 0.55 light-years from Sagittarius A* (Sgr A*), the supermassive black hole at the center of the Milky Way, continues to release water and other molecules into its surroundings. Despite the extreme gravitational pull and high-energy radiation from the black hole, IRS 3 is still enriching its environment with dust and molecular material. This star is in the red giant phase, meaning it has evolved past its main sequence and is now expanding and shedding mass. It is about six times more massive than the Sun and around 72 million years old. IRS 3 is one of the brightest sources of mid-infrared light in the galactic center, and its massive dust envelope suggests significant mass loss over time. Using the JWST’s mid-infrared instrument, MIRI, scientists detected strong infrared signals from silicate dust—made of silicon and oxygen—and confirmed the presence of water in IRS 3’s surrounding envelope. This finding is significant because it shows that molecules can survive in environments with intense radiation, which was previously thought to be too harsh for such matter. The data, combined with models of how light travels through different structures around the star, suggest that the dust forms a layered shell-like structure extending up to about 10,000 astronomical units from the star. The temperature of this envelope decreases dramatically, from about 927 °C near the star to roughly −173 °C in the outer regions. These findings challenge previous assumptions that galactic centers are too hostile for stars to contribute dust and molecules. Florian Peißker of the University of Cologne in Germany, lead author of the study, emphasized that galactic centers are some of the most extreme environments in the universe. Understanding whether stars can still enrich their surroundings under these conditions is crucial. He noted that the JWST allows direct observation of such stars and confirms that dust production remains stable even near a supermassive black hole. Macarena Garcia Marin from the European Space Agency (ESA), co-author of the study and head of the MICONIC space program, highlighted the excitement around detecting water. She explained that the presence of molecular matter near Sgr A* suggests that stars can continue to contribute to their environment, even in the intense conditions near a black hole. The research findings have been published in the journal Astronomy and Astrophysics. The study adds to our understanding of how stars interact with their surroundings in extreme cosmic environments, showing that even near a supermassive black hole, stars can play a role in shaping the chemical composition of their galactic neighborhood.