For years, Uranus and Neptune have been labeled as 'ice giants', suggesting they are primarily composed of icy materials. However, new research led by Yamila Miguel from the Netherlands Institute for Space Research indicates that these planets may actually have a greater proportion of rock-rich material in their interiors. The research utilized computer models to simulate the internal structures of both planets under extreme conditions, revealing that silicate materials could condense under high pressure, potentially altering their classification. The study draws parallels with rocky objects found in the Kuiper Belt, such as comets and Pluto, leading researchers to reconsider the building blocks of Uranus and Neptune. While the planets have not been officially reclassified, the findings underscore the complexity of their internal structures and the need for a more accurate terminology, possibly suggesting terms like 'minor giants' instead of 'icy' or 'rocky'. This research not only challenges existing perceptions but also enhances our understanding of giant planet formation and evolution.