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)