MESA-Web Mesa Logo

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Welcome

Stellar evolution codes can be complicated to use, so we are offering MESA-Web, a web-based interface to the stellar evolution code, Modules for Experiments in Stellar Astrophysics (MESA).

MESA-Web can be used for education purposes to calculate stellar models over a range of physical parameters, extending capabilities of similar online tools such as Rich Townsend's EZ-Web.


Test Suite Examples


Submit a Calculation - Single Star

(M)

Nuclear Reactions

New! More info here.
Upload Rate (must correspond to rate from list above):

Composition


Mixing
Convection



Convective Overshoot



Semi-Convection


Thermohaline



Winds





Rotation
ZAMScrit)i

Resolution
Spatial (Mass) Resolution - Global


Temporal (Time) Resolution - Global



Temporal (Time) Resolution - Hydrogen





Custom Stopping Condition



Output

Note that a maximum of 500 profiles will be stored for a given run.




For more info on the selection of these input parameters, visit the How To Use MESA-Web section.