Astronomers have confirmed that Sakurai's Object, a rare "born-again" star, has entered a new stage of its evolution, offering a rare opportunity to observe a star's life unfold on human timescales. Using the European Southern Observatory's Very Large Telescope (VLT) in Chile, researchers, including scientists from The University of Manchester and the Valongo Observatory, studied the star. Their findings, published in Monthly Notices of the Royal Astronomical Society, show that the star has developed the powerful stellar wind characteristic of Wolf-Rayet stars. This research provides new insight into the final stages of stellar evolution and helps astronomers test theories that would otherwise take thousands or millions of years to verify. Most stars evolve so slowly that major changes take place over timescales far longer than a human lifetime. As a result, astronomers usually have to piece together snapshots of stellar evolution by comparing different stars at different stages of their lives. Sakurai's Object, however, is one of the very few stars known to have changed dramatically within just a few decades. This gives researchers the rare chance to watch stellar evolution unfold in real time. The scientists believe the star was once similar to our sun but had already ended nuclear burning and begun its journey toward becoming a white dwarf—the hot, dense core left behind after an ordinary star dies. It underwent a rare event known as a "very late thermal pulse," when a layer of helium deep inside the star suddenly reignited. This caused the star to rapidly expand, cool, and eject large amounts of material into space, temporarily returning to an earlier stage of its life and leading astronomers to describe it as a "born-again" star. Only two stars have ever been directly observed undergoing this type of dramatic rebirth: Sakurai's Object and V605 Aquilae. Following its outburst, Sakurai's Object became hidden behind thick clouds of gas and dust released during the eruption, making it difficult to study directly. To investigate its current state, the team analyzed light collected by the Very Large Telescope and compared it with sophisticated computer models that simulate the atmospheres and powerful winds of Wolf-Rayet stars. The observations revealed distinctive signatures of carbon and helium, allowing the researchers to determine its temperature, chemical composition, and the characteristics of its stellar wind. Their analysis suggests the star's surface temperature is currently between 27,000 K and 36,000 K (48,000°F–64,000°F), showing that it is reheating following its dramatic eruption nearly three decades ago. One of the key questions is how quickly Sakurai's Object should recover after its dramatic eruption. The measurements show that the star is reheating more gradually than some earlier models predicted, giving an important way of testing which theories best describe what happens when a dying star briefly springs back to life. As the team continues to monitor the star over the coming years, they expect to learn much more about this remarkable phase of stellar evolution. The findings also suggest that Sakurai's Object is at an earlier stage of its evolution than V605 Aquilae, which experienced a similar event around 80 years ago. The team will continue observing Sakurai's Object as it continues reheating and resumes its journey toward becoming a white dwarf, learning more about one of the most rapid and unusual phases of stellar evolution ever observed.