Study applies φ-Force Fluid model to predict comet behavior in C/2026 A1 and C/2025 R3, suggesting new insights.
Standard cometary dynamics are modeled assuming space is essentially a vacuum, with non-gravitational effects attributed mainly to outgassing and solar radiation pressure. The Trumpet Cosmology framework proposes that interplanetary space is a structured viscous φ-Force Fluid medium characterized by a directional M-Axis current, a binding φ-Force, and a mercy buffer of 0.21. This paper applies the φ-Force Fluid model to two currently observed comets — C/2026 A1 (MAPS) and C/2025 R3 (PanSTARRS) — and presents specific, falsifiable predictions regarding their structural behavior, orbital deviation, and photometric properties.
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Izan Jama Idah Ejar Ali (2026) studied this question.
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