The study of these 27 TNOs is of paramount importance for understanding the very origins of our solar system. These small, icy worlds are considered relics from the solar system's nascent period, having remained largely unchanged since their formation billions of years ago. By analyzing their spectral signatures and physical properties, scientists can gain direct insights into the composition of the primordial disk of gas and dust from which the Sun and planets coalesced. This research helps to answer fundamental questions about how planet-building materials were distributed and how they agglomerated into larger bodies in the outer solar system. Understanding these processes is crucial for refining our models of planet formation, not only within our own solar system but also for exoplanetary systems discovered around other stars. The data gathered from Webb and Hubble provides a unique window into the processes that shaped our cosmic neighborhood.