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Aerothermodynamic simulation demonstrates hypersonic drag heating dynamics in a re-entry convenience burger, suggesting an extremely narrow transient window for achieving edible temperatures.
This deposit contains the full Carlo‑edition analysis of using atmospheric drag as a thermal optimisation method for a Rustlers™ microwave burger. The study evaluates hypersonic stagnation heating, structural ablation behaviour, and the brief but scientifically significant window in which the burger becomes “crispy but technically edible.” The work introduces the Rustlers Mach‑5 Heating Equation, describing the stagnation‑point thermal flux applied to a convenience sandwich undergoing ballistic re-entry: \[Q̇Rustlers = k √ρ/R_n \, v^3\] Where:- \( ρ \) is atmospheric density,- \( R_n \) is the burger nose radius (0.05 m),- \( v \) is the hypersonic velocity (Mach 5–25),- \( k \) is the Carlo‑calibrated snack‑heating constant. This equation governs the 3.8‑second heating interval during which the Rustlers™ burger transitions from “fridge cold” to “crispy but edible,” immediately before entering the plasma‑snack regime. Included:- Full ASCII diagrams- Thermal evolution charts- Structural integrity maps- Edibility analysis- Complete Carlo‑style hypersonic culinary framework Author:Matthew Arthur Carlo This upload includes an interactive 3D HTML visualiser designed to bring the hypersonic culinary physics of the accompanying paper to life. Powered by Three.js and real-time JavaScript telemetry, the simulation runs on the core equations outlined in the text—including the 30,000 J thermal energy requirement (Q = mcΔ T) and peak stagnation heat fluxes reaching 1 MW/m² from a 7.8 km/s re-entry trajectory. Visually, it renders a detailed structural integrity map of the Rustlers™ burger—featuring the front-face ablation bun, warmed patty core, non-Newtonian cheese smear, and pressurised sauce packet—all set against a dynamic hypersonic shockwave and glowing plasma particle stream that tracks the precise 4-second transition from sub-sonic warming to the fleeting $0.003$-second "perfectly warm" edibility window. Author’s Note: I’ve always wondered this, and for those who also wondered (all 0), the answer has finally been answered. The eternal question of whether a Rustlers burger can be heated using atmospheric drag at hypersonic velocity has now been resolved with the full force of Carlo-grade physics, ASCII diagrams, and unnecessary orbital mechanics. Keywords: atmospheric drag, hypersonic heating, Rustlers burger, ballistic re-entry, stagnation-point thermodynamics, Mach-5 culinary physics, snack aerothermodynamics, ablative bun mechanics, non-Newtonian cheese behaviour, orbital food science, Carlo-style absurd physics. Subjects: Hypersonic culinary analysis, applied thermodynamics of convenience foods, re-entry heating models, experimental snack engineering, orbital gastronomy, high-speed thermal optimisation, comedic physics, absurd academic studies, plasma-transition edibility research. Contact: For enquiries or research questions related to this work, email matthewcarlo.research@gmail.com
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Matthew Arthur Carlo (2026) studied this question.
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