'Mali rdeči točki' so morda pulzirajoče pošasti, ki so ustvarile črne luknje v zgodnjem vesolju

Astronomers have proposed a groundbreaking explanation for the mysterious “little red dots” detected by the James Webb Space Telescope in the early universe. These enigmatic objects, appearing as compact, red, and extremely bright sources of light, may actually be supermassive stars, gigantic stellar bodies capable of creating the conditions necessary for the formation of early supermassive black holes. According to a new study led by Devesh Nandal of the Harvard College Observatory, these stars could account for the peculiar characteristics of the LRDs, including their unusual spectra, compact appearance, and high levels of nitrogen. The LRDs were first identified in images captured by the James Webb Space Telescope, revealing features that defy conventional astrophysical models. While previous speculation suggested they might be galaxies, black holes, or other exotic phenomena, Nandal’s research offers a compelling alternative. His team has demonstrated that supermassive stars, ranging up to 100,000 times the mass of the Sun, can replicate the spectral signatures and morphological traits observed in the LRDs. These findings suggest that such stars may serve as the progenitors of the earliest supermassive black holes in the cosmos. Supermassive stars exhibit unique behaviors that set them apart from typical stellar objects. Unlike most stars, which gradually shed mass throughout their lifetimes, these giants undergo periodic, intense pulsations known as “strange-mode” events. During these episodes, they expel shell-like structures of gas, contributing to the compact, glowing appearance of the LRDs. The ejected material consists primarily of hydrogen and helium, but also includes nitrogen, a chemical signature increasingly observed in LRD data. This nitrogen enrichment provides further support for the hypothesis that the LRDs originate from supermassive stars rather than other cosmic entities. According to the study, these stars eventually reach a stage of extreme instability, leading to a process known as direct collapse. In this phase, the remaining core of the star collapses under its own gravity, forming a seed for a supermassive black hole. This mechanism aligns with theories suggesting that the earliest black holes in the universe formed rapidly and played a crucial role in shaping the structure of the cosmos. Nandal emphasized the significance of this discovery, noting that the model unifies multiple observational clues into a coherent framework. “The spectrum and the morphology are two sides of the same physical problem,” he explained. “The spectrum tells us what kind of source is producing the light and how that light is processed, while the shape tells us where the surrounding material is and how compact it must be.” The researchers aim to refine their model by generating detailed predictions about the spectra of LRDs. These predictions will allow scientists to compare theoretical expectations with actual observations made by the James Webb Space Telescope. By doing so, they hope to confirm or challenge the hypothesis that supermassive stars are responsible for the phenomenon. As the field continues to explore the origins of the universe’s most elusive objects, the study represents a major step forward in understanding the complex interplay between stellar evolution and black hole formation. With more data emerging from the James Webb mission, the mystery of the little red dots may soon yield to the insights of modern astronomy.