NASA has released a new image obtained by the James Webb Space Telescope, capturing the turbulent star-forming region N159. This region is located in the Large Magellanic Cloud — one of the satellite galaxies of the Milky Way, at a distance of approximately 161,000 light-years from Earth. The image demonstrates dense clouds of gas where the active formation of new stars is taking place. A distinctive feature of the N159 region is its reduced metallicity — that is, a lower content of elements heavier than hydrogen and helium — compared to most star-forming regions in our own galaxy. Studying such regions helps astronomers better understand the processes of star birth under conditions different from those typical of the Milky Way. The low metallicity makes N159 similar in composition to early galaxies of the young Universe, making this region particularly valuable for research. The James Webb Telescope, launched into space in late 2021, thanks to its infrared optics, is capable of peering through dense clouds of dust and gas that hide star-forming processes from ordinary optical telescopes. This allows scientists to observe the finest details of the structure of such nebulae and track the formation of new stellar systems. The new image continues a series of pictures that the telescope regularly transmits to Earth, providing astronomers with ever-new data about the dynamics and evolution of cosmic objects.