Computer Science
Scientific paper
Aug 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jbis...46..311b&link_type=abstract
British Interplanetary Society, Journal (ISSN 0007-094X), vol. 46, no. 8, p. 311-313.
Computer Science
Angular Velocity, Energy Transfer, Kinetic Energy, Planetary Rotation, Mass Flow, Relativity, Venus (Planet)
Scientific paper
The rotation periods of planets like Venus may render them less suitable for terraforming. This paper describe how to spin a planet to obtain a 24-hour day. Dynamic compression members, formed from high-velocity mass-streams, thrust along the planet's equator, producing the required torque. Energy is obtained from a light-sail windmill in solar orbit. This procedure is more efficient and less costly than earlier concepts; a rotation rate of one revolution per day could be achieved within about 30 years.
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