Theoretical modeling demonstrates exact geometric solutions for deep-space astrodynamic anomalies, eliminating the need for hypothetical planetary bodies and cometary outgassing.
This preprint resolves three long-standing anomalies in astrodynamics and deep-space celestial mechanics using geometric scale invariance and spatial information bounds. We provide an exact, parameter-free derivation of the planetary flyby velocity anomaly observed in spacecraft trajectories like NEAR and Galileo. Furthermore, we explain the orbital clustering of extreme trans-Neptunian objects as an intrinsic secular precession effect at low accelerations, eliminating the need for an undiscovered Planet Nine. Finally, the non-gravitational radial acceleration of the interstellar interloper 'Oumuamua is derived from metric refraction and its observed geometric aspect ratio without requiring cometary outgassing.
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Pi3 Andres G. (2026) studied this question.
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