How to move a planet

Computer Science

Scientific paper

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Mass Flow, Orbital Mechanics, Planetary Orbits, Relativistic Velocity, Angular Momentum, Momentum Transfer

Scientific paper

The orbits of planets like Venus and Mars may render them unsuitable for terraforming without the use of soletta mirrors. This paper describes how to move a planet to the right distance from the sun. Dynamic compression members, formed from high-velocity mass-streams, thrust against the planet, effecting the desired orbital shift and transferring angular momentum. Energy is supplied by a light-sail windmill in solar orbit, allowing the procedure to be completed within a period of about 30 years.

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