A recent study titled 'The Life and Death of Stars That Capture Primordial Black Holes' by Ore Gottlieb and colleagues from MIT investigates the fate of stars that engulf primordial black holes (PBH). These hypothetical objects may have formed in the early Universe and could play a role in dark matter. The research reveals that when a star captures a PBH, two distinct outcomes are possible based on the accretion rate of stellar material. If the PBH rapidly accretes material, it can lead to the star's explosive destruction, creating phenomena such as x-ray flashes and potential gamma-ray bursts. Alternatively, if the accretion is slow, the star may survive in a quasi-steady state, leading to a quiet terminal phase. The study emphasizes the importance of understanding the conditions that dictate these outcomes, as they have significant implications for future observations of dark matter and stellar evolution. The authors propose that their findings serve as a roadmap for future research into the dynamics of PBH capture and its effects on stars.