Model the conductive cooling of small planetary bodies with temperature-dependent material properties
You might want to read our documentation, look at some examples, or try it out in an interactive notebook.
If you want to see more, you can look at our GitHub repositoryor read some scientific background to the project.
If you want to be able to model meteorite parent bodies, calculate meteorite formation depths, and estimate the timing of core-dynamo activity, install the package on your machine.
If you’re having any issues, just leave us a message, and please remember to cite us.