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General questions, comments, or suggestions?

Email the MESA-Web team at: m e s a - w e b - i n f o (at) asu . edu

Here we answer some of most frequently asked questions so that you can focus on the science!

How do I properly cite MESA-Web?

Proper citation of MESA-Web is given below:

Fields, C. E., & Timmes, F. X. (2015). MESA-Web. Retrieved from

What is MESA?

MESA provides a modern software infrastructure for sustained innovation in the stellar astrophysics community. MESA solves the 1D fully coupled structure and composition equations governing stellar evolution with an implicit finite volume scheme. State-of-the-art modules provide adaptive mesh refinement, sophisticated timestep controls, non-adiabatic oscillation capabilities, equation of state, opacity, nuclear reaction rates, element diffusion, boundary conditions, and changes to the mass of the star. The journal papers describing MESA can be found here (Paxton et al. 2011), here (Paxton et al. 2013), and here (Paxton et al. 2015). Since its inception, MESA has attracted over 800 registered users becoming one of the leading numerical tools for stellar astrophysics! If you'd like to join the MESA community, subscribe to the MESA Users List here, and visit the MESA homepage to learn how to download MESA!

What is the stopping criterion for my MESA-Web submission?

Each calculation runs for 60 minutes, or until the end of core Oxygen 16 fusion, whichever comes first.