Could the discovery of a new type of exoplanet transform our understanding of planetary formation?

Traditional models of planetary formation are based on our solar system, where we classify planets mainly as terrestrial or gas giants. However, recent astronomical data suggests the existence of a new type of exoplanet that doesn't fit neatly into these categories. These so-called "hybrid planets" exhibit characteristics of both rocky and gas planets, challenging our existing paradigms. What implications could the discovery of such planets have on our theories about how solar systems develop, and what questions would these findings raise about the potential for diverse and exotic life-bearing environments beyond Earth?