Unuvun Rain: Created page with "= References = ==Moon stability== ===Holman et al., 1999=== https://iopscience.iop.org/article/10.1086/300695/fulltext/980335.text.html This is the current method used to di..."

2022-01-30T20:23:58Z

Created page with "= References = ==Moon stability== ===Holman et al., 1999=== https://iopscience.iop.org/article/10.1086/300695/fulltext/980335.text.html This is the current method used to di..."

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= References =
==Moon stability==

===Holman et al., 1999===
https://iopscience.iop.org/article/10.1086/300695/fulltext/980335.text.html

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===
https://arxiv.org/abs/1801.03955

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===
https://arxiv.org/abs/2108.07815

===REBOUND===
https://rebound.readthedocs.io/en/latest/

This program may be useful to try and simulate stability.

Pavalan-Hakese System - Revision history

Unuvun Rain: Created page with "= References = ==Moon stability== ===Holman et al., 1999=== https://iopscience.iop.org/article/10.1086/300695/fulltext/980335.text.html This is the current method used to di..."