MESA Isochrones and Stellar Tracks (MIST)
We are currently working on the MIST project using MESA to create an extensive grid of stellar evolutionary tracks and isochrones over a wide range of masses, metallicities, ages, and advanced stellar evolutionary phases. With these new models, we hope to tackle a variety of problems in both stellar evolution and extragalactic studies. The movie shows the evolution of a 2 solar mass star from the pre-main sequence to the white dwarf cooling phase. Read more about it in the first paper here.