Simulating the Phases of the Moon Shortly After Its Formation
Emil Noordeh, Patrick Hall, Matija Cuk

TL;DR
This paper presents simulations of the Moon's early phases following its formation, highlighting its highly elliptical initial orbit and discussing the educational value of these models.
Contribution
It introduces a simulation model of the Moon's early orbital phases based on the giant impact hypothesis, emphasizing its pedagogical utility.
Findings
Moon's early orbit was highly elliptical
Simulations show the Moon's phases shortly after formation
Educational value of the simulation models
Abstract
The leading theory for the origin of the Moon is the giant impact hypothesis, in which the Moon was formed out of the debris left over from the collision of a Mars-sized body with the Earth. Soon after its formation, the orbit of the Moon may have been very different than it is today. We have simulated the phases of the Moon in a model for its formation wherein the Moon develops a highly elliptical orbit with its major axis tangential to the Earth's orbit. This note describes these simulations and their pedagogical value.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
