The inclination of the planetary system relative to the solar equator may be explained by the presence of Planet 9
Rodney Gomes, Rogerio Deienno, Alessandro Morbidelli

TL;DR
This paper investigates how a hypothetical Planet 9 could cause the observed 6-degree tilt of the solar system's giant planets relative to the solar equator, providing an analytical model and numerical validation.
Contribution
It introduces a new analytical framework linking Planet 9's properties to the solar system's tilt, constraining its possible orbital elements.
Findings
Planet 9's presence can explain the solar tilt.
The model constrains Planet 9's orbital parameters.
Configurations compatible with Kuiper belt observations are identified.
Abstract
We evaluate the effects of a distant planet, commonly known as planet 9, on the dynamics of the giant planets of the Solar System. We find that, given the large distance of planet 9, the dynamics of the inner giant planets can be decomposed into a classic Lagrange-Laplace dynamics relative to their own invariant plane (the plane orthogonal to their total angular momentum vector) and a slow precession of said plane relative to the total angular momentum vector of the Solar System, including planet 9. Under some specific configurations for planet 9, this precession can explain the current tilt of approximately 6 degrees between the invariant plane of the giant planets and the solar equator. An analytical model is developed to map the evolution of the inclination of the inner giant planets' invariant plane as a function of the planet 9's mass, inclination, eccentricity and semimajor axis,…
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