一种新发现的行星系统 在较小的岩石行星内有气态巨星 与标准的形成理论格格不入 A newly found planetary system has gas giants inside smaller rocky planets, defying standard formation theories.

新发现的行星系统与传统的形成理论格格不入,其特点是气体巨星的运行距离其恒星远比小的岩石行星更近。 A newly discovered planetary system defies conventional formation theories, featuring gas giants orbiting much closer to their star than smaller, rocky planets. 这种“外在”配置,即大型行星位于较小行星内,与行星形成的标准模型相矛盾,并挑战科学家对太阳系如何演变的理解。 This "inside-out" configuration, where massive planets lie inside smaller ones, contradicts standard models of planet formation and challenges scientists' understanding of how solar systems evolve. 目前正在研究使用先进望远镜观察的该系统,以发现其不寻常结构背后的机制。 The system, observed using advanced telescopes, is currently under study to uncover the mechanisms behind its unusual structure.