Unveiling the Dynamic Depths of Stellar Interiors
A new computer simulation is helping scientists understand the complex process of convection within stars. Convection, the cyclic flow of material that transfers heat energy to a star's surface, is difficult to model due to factors like viscosity and turbulent vortices. By studying the flickering of light emitted by stars, astronomers can gain insights into their interior. While current telescopes are unable to observe these flickers, future advancements may allow for a better understanding of stars through their light fluctuations.