SPIDER

Simulating Planetary Interior Dynamics with Extreme Rheology

SPIDER is a 1-D parameterised interior dynamics code for rocky planets with molten and/or solid interiors and support for volatile cycling, redox reactions, and radiative transfer in the atmosphere.

Note: This documentation describes the version of SPIDER as part of the PROTEUS Framework. For the original SPIDER code, see djbower/SPIDER.

Getting started

• Installation guide
• Publications
• Model overview
• Source code

If you plan to contribute to SPIDER, please read our Code of Conduct. If you are running into problems, please do not hesitate to raise an Issue.

Copyright

See the included license. Copyright 2021 Daniel J. Bower and Patrick Sanan.