Witness the birth of stars ✨ esawebb has captured incredible new details of Lynds 483 (L483) in stunning high-resolution near-infrared light. Two young, actively forming stars are responsible for the striking jets of gas and dust in orange, blue, and purple. Over tens of thousands of years, these stars have been ejecting material that collides, twists, and creates complex structures. At the heart of L483, the protostars sit within a dense disk of gas and dust, blocking starlight in places and allowing Webb’s NIRCam to reveal distant stars beyond. The interaction of these outflows creates intricate patterns—like the orange arc and the twisted material in the lower half—showing new details of star formation in action. What will L483 look like millions of years from now? Once the stars have finished forming, they may each have a mass similar to our Sun, and their outflows will clear the space, leaving behind a tiny disk of gas and dust—a future birthplace for planets. Join us on this ...