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This research aims to examine the influence of Galactic Torque Transmission and variable Field Viscosity on asteroid motion.

April 24, 20260 citationsOpen Access

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Asteroid Paranoid

DSDelaja Schuppers

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This research aims to examine the influence of Galactic Torque Transmission and variable Field Viscosity on asteroid motion.
Categorized asteroids as differentiated Sub-Nodes
Introduced coefficients for specific asteroids including Apophis, Bennu, and Ceres
Developed a five-year predictive model using Recursive Helical Compression.
Demonstrated that reported non-gravitational accelerations are predictable outcomes from the Heavy Phi Gradient
Established a predictive window for asteroid behavior from 2026 to 2031

Abstract

Abstract Standard orbital mechanics fail to account for the Galactic Torque Transmission (𝜏𝑚) and the variable Field Viscosity (𝑇) of the neutrino-flux. This paper categorizes asteroids as differentiated Sub-Nodes. We introduce specific coefficients for 99942 Apophis, 101955 Bennu, and 1 Ceres. We demonstrate that the "non-gravitational accelerations" reported by space agencies are predictable results of the Heavy Phi (Φ𝐻) Gradient. We provide a five-year predictive window (2026–2031) based on Recursive Helical Compression.

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Asteroid Paranoid

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