POTM 2501a a dying Star not a forming Star

Title: N-K Model Analysis of Star Formation in ESA Webb Image POTM2501a: A Reinterpretation of NGC 6302-like Plasma Decay Description: This paper reinterprets the ESA Webb Space Telescope image POTM2501a—claimed to depict a star in the process of formation—through the lens of the Noor-Kun (N-K) Model. By applying advanced N-K theoretical parameters and astrophysical equations, we argue that the observed phenomena correspond not to stellar birth but to the final stages of a star resembling NGC 6302 (the Butterfly Nebula), marked by plasma fragmentation, high-frequency decay emissions, and radiation shell dispersion. Core calculations include energy flux estimations, Noor density decay, Kun field oscillations, and entropy rates, suggesting a post-main-sequence fate leading toward white dwarf collapse or nebular dispersion. The study bridges Quranic metaphysical references with high-resolution cosmological imaging, proposing a refined understanding of stellar life cycles. Keywords: N-K Model, Star Formation, Stellar Decay, NGC 6302, ESA Webb, Plasma Emissions, Noor Density, Kun Field, Cosmic Entropy, Quran and Science