Metalloseoseids

Metalloseoseids are a hypothetical class of celestial bodies proposed in theoretical astrophysics. The concept of metalloseoseids arises from the study of the early universe and the formation of the first stars and galaxies. In the extremely metal-poor conditions of the early cosmos, it is theorized that gravitational collapse could lead to the formation of massive stars composed almost entirely of hydrogen and helium, with trace amounts of lithium. As these stars evolve and eventually die, they are expected to produce heavier elements, a process known as nucleosynthesis.

If a star forms in an environment where even these initial heavy elements are scarce, and it undergoes a specific type of supernova explosion, the resulting remnant might be a dense object composed predominantly of these newly synthesized heavy elements, alongside the original hydrogen and helium. Metalloseoseids are envisioned as the remnants of such events, potentially existing in the outskirts of galaxies or in intergalactic space, far from regions of active star formation where heavy element enrichment is more pronounced. Their observational detection would be challenging due to their likely low luminosity and the extreme conditions under which they are presumed to form. The existence of metalloseoseids remains speculative, awaiting theoretical refinement and potential observational evidence.