Gratinoiduts

Gratinoiduts are a hypothetical class of celestial bodies that have been theorized to exist within certain extreme astrophysical environments. The term itself is derived from the concept of a gratin, a culinary dish often characterized by a baked, crispy top layer, and the suffix "-oid," implying a resemblance or relation. In the context of astrophysics, a gratinoidut is envisioned as a planet or other substantial celestial object that has undergone an intense, prolonged period of surface bombardment by high-energy particles or radiation. This bombardment is theorized to cause significant changes to the surface composition and structure, potentially leading to the formation of a hardened, vitrified, or otherwise altered crust.

The formation of gratinoiduts is thought to be linked to phenomena such as close proximity to active galactic nuclei, frequent supernova events in their vicinity, or prolonged exposure to powerful stellar winds from unusually energetic stars. The intense energy flux is hypothesized to effectively "bake" or "sear" the surface layers of the celestial body, leading to a geological transformation distinct from typical planetary differentiation or erosional processes. While no definitive observational evidence for gratinoiduts has yet been confirmed, the theoretical framework allows for their potential existence in specific cosmic niches. Further research and advancements in observational capabilities may eventually provide insights into whether such celestial bodies are a reality.