Coupling the non-gravitational forces and Modified Newton Dynamics for cometary orbits
Lucie Maquet, Fr\'ed\'eric Pierret

TL;DR
This paper investigates how Modified Newton Dynamics (MOND) influences cometary orbits, especially for comets with large semi-major axes, and compares these effects to non-gravitational forces caused by sublimation.
Contribution
It provides the first detailed analysis of MOND effects on specific comets and compares them to non-gravitational forces, highlighting their significance for orbital modeling.
Findings
MOND effects are significant for comets with large semi-major axes.
MOND perturbations can be comparable to non-gravitational forces.
Different MOND functions produce varying orbital variations.
Abstract
In recent work (Milgrom 2009, Blanchet & Novak 2011), the authors showed that MOdified Newton Dynamics (MOND) have a non-negligible secular perturbation effect on planets with large semi-major axes (gaseous planets) in the Solar System. Some comets also have a very eccentric orbit with a large semi-major axis (Halley family comets) going far away from the Sun (more than 15 AU) in a low acceleration regime where they would be subject to MOND perturbation. They also approach the Sun very closely (less than 3 AU) and are affected by the sublimation of ices from their nucleus, triggering so-called non-gravitational forces. The main goal of this paper is to investigate the effect of MOND perturbation on three comets with various orbital elements (2P/Encke, 1P/Halley and 153P/Ikeya-Zhang) and then compare it to the non-gravitational perturbations. It is motivated by the fact that when fitting…
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