The Stellar Death Clock: Engineering Analysis and Desing of an Asteroid-Assisted Orbital Migration Strategy
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The gradual increase in solar luminosity will render Earth uninhabitable in approximately 600 million years. This paper presents a preliminary feasibility analysis for migrating Earth’s orbit to 1.3 AU using repeated gravitational assists from 120 km asteroids. Optimal launch windows—defined by Venus–Earth angles of 170°–190° and Mars–Earth angles of 165°–195°—were identified to maximize momentum transfer while minimizing perturbations to neighboring planets. Using Newtonian N‑body approximations and angular‑momentum transfer equations, we estimate that each asteroid flyby contributes ~21.4 km to Earth’s semi‑major axis, with negligible cumulative effects on Venus (~546 m), Mars (~1,155 m), and the Moon’s eccentricity (~6.61 × 10⁻⁸ per flyby). Under a deployment rate of ~400 flybys per year, the full 0.3 AU migration could be achieved in ~5,257 years.
These results suggest that asteroid-assisted orbital migration may be analytically promising under the present simplifying assumptions within the inner Solar System. While this study does not address propulsion engineering or full N-body integration, it provides an analytical and conceptual foundation for future high-fidelity simulations. Given the long‑term constraints imposed by stellar evolution, early exploration of such astroengineering strategies may be essential for the preservation of Earth’s biosphere.
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The_Stellar_Death_Clock_Engineering_Analysis_and_Design_of_an_Asteroid‑Assisted_Orbital_Migration_Strategy_v2.pdf
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