Pavalan-Hakese System

From PavHaki Wiki
The printable version is no longer supported and may have rendering errors. Please update your browser bookmarks and please use the default browser print function instead.


Moon stability

Holman et al., 1999

This is the current method used to discern the stability of moons around binary planets. It's implemented in the Yakei-Odius System spreadsheet. It seems based off this, we can have stable moons past ~100,000km, avoiding n:1 resonances.

Lam et al., 2018

This paper provides a Python script written in Python 2 that requires a few adjustments to get working. Parker et al., 2021 mentions this but does not use it, instead relying on the methods described in Holman et al., 1999.

Parker et al., 2021


This program may be useful to try and simulate stability.