Turbulence in fluid dynamics does not have a definitive limit, as it can become increasingly chaotic without a discernible pattern. The complexity of modeling turbulence is highlighted by the challenges in accurately resolving the Kolmogorov scale, which requires extremely fine mesh that is often impractical even for supercomputers. While the Reynolds number is commonly used to characterize flow regimes, the onset of turbulence is influenced by various factors beyond just this number, such as surface roughness and external disturbances. Research has shown that turbulence can occur at very high Reynolds numbers, with some regimes reaching values as high as 10^12 in stellar interiors. Overall, turbulence remains a complex phenomenon that continues to challenge researchers in fluid dynamics.