2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/34074In this paper, we investigate the nature of the singularity in the spherically symmetrical, shear-free, gravitational collapse of a star with heat flux using a separable metric [cqg1]. For any non-singular, regular, radial density profile for a star described by this metric, eq. (2.1), the singularity of the gravitational collapse is not naked locally. Our results here unequivocally support the Strong Cosmic Censorship Hypothesis.Submitted to General Relativity and GravitationGeneral Relativity and Quantum Cosmologytext