The James Webb Space Telescope (JWST) has observed a young, sun-like star actively forging and ejecting crystalline silicates, the same type of crystals found in comets within our own solar system. This discovery, made by analyzing the star known as ISO-Oph 102 located in the Ophiuchus constellation, offers crucial insights into the origins of these crystals and how they become incorporated into comets, which spend most of their lives far from the sun's warmth. Astronomers have long been puzzled by the presence of crystalline silicates in comets. These crystals require high temperatures to form, yet comets primarily reside in the frigid outer reaches of our solar system, in regions like the Kuiper Belt and Oort Cloud. The prevailing theory suggests that these crystals were initially formed closer to the sun and subsequently transported outwards, but direct observational evidence of this process has been elusive until now. JWST's infrared capabilities allowed researchers to analyze the dust disk surrounding ISO-Oph 102. The data revealed the distinct spectral signatures of crystalline silicates being ejected from the inner regions of the disk, where temperatures are sufficiently high for crystal formation. These crystals are then carried outwards by stellar winds and radiation pressure, eventually becoming part of the building blocks of comets. This observation supports the idea that comets are not simply primordial remnants of the early solar system, but rather dynamic objects that have undergone significant processing and transport of materials from different regions. The discovery also highlights the power of JWST to probe the inner workings of star-forming regions and unravel the mysteries of planet and comet formation. Further studies of ISO-Oph 102 and other similar systems will help refine our understanding of the processes that shape the composition of comets and the distribution of materials in protoplanetary disks. This knowledge is essential for understanding the origins of our own solar system and the conditions that led to the formation of planets and the delivery of water and organic molecules to early Earth.