The James Webb Space Telescope has provided a stunning view of young stars in the Orion Molecular Clouds, particularly focusing on OMC-2, which is located 1,280 light-years from Earth. This region showcases every stage of star formation, from protostars to pre-main sequence stars, all within a span of 150 light-years. Webb’s Near-Infrared Camera (NIRCam) was crucial in capturing these images, as the dense gas and dust in the area block visible light. The observations reveal protostars surrounded by swirling gas and dust, with their outflows creating visible shockwaves that illuminate the surrounding material. The research aims to explore how these outflows influence star formation and the chemical processes in the disks that may eventually form planets. This study is part of observing program #5804, which focuses on the star formation processes in OMC-2 and its neighboring OMC-3, providing valuable insights into the earliest stages of stellar evolution.