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Re: Sky People's solar system

From:John Cowan <cowan@...>
Date:Tuesday, January 19, 1999, 16:07
Christopher Atavus scripsit:

> In fact, I want to know how you make the planet's revolution delays. I've > got a good idea for the planet of the Sky People (their sun is a little > hotter than ours, so their planet is slightly farther from their sun than > ours), but I don't know how to make it with the other 11 planets of this > solar system.
(^ marks superscripts) You can put the planets and satellites anywhere you want: no law dictates their periods of revolution or rotation. The only law you must observe is the harmonic law: p^2/r^3 must be constant, where p is the period of revolution and r is the radius of the orbit. The constant is (4*pi^2)/(M*G) where M is the mass of the primary body (the sun for a planet, the planet for a satellite) and G is the gravitational constant, approximately 6.67259*10^-11 m^3/kg sec^2. This version of the law does not hold if the mass of the planet/satellite is not negligible with respect to the mass of the sun/planet, which is most unlikely. So you can choose either period of revolution or distance, but not both. Rotations can be anything you want. -- John Cowan http://www.ccil.org/~cowan cowan@ccil.org You tollerday donsk? N. You tolkatiff scowegian? Nn. You spigotty anglease? Nnn. You phonio saxo? Nnnn. Clear all so! 'Tis a Jute.... (Finnegans Wake 16.5)