The James Webb Space Telescope (JWST) has revealed a stunning image of a dying star's 'exposed cranium', a nebula known as PMR 1. This star, several times more massive than our Sun, is in its final stages of life, just a few thousand years from its ultimate fate. The nebula's structure, as seen by JWST, provides a unique insight into the star's complex ejecta and the star's potential future as a white dwarf or a supernova. The article explores the star's mass, nature, and fate, and how JWST's multi-wavelength imaging has unveiled unprecedented cosmic details. It also discusses the star's potential as a Wolf-Rayet star, which could die in a supernova, or as a pre-planetary nebula, eventually becoming a white dwarf. The author emphasizes the importance of JWST's ability to reveal diverse details by observing the universe in various wavelengths, providing a more comprehensive understanding of cosmic phenomena.
