Hi,
I was wondering if anyone could help me. I’m trying to design a planet with two moons for a story I’m writing.
The planet will be 98% as dense as earth but it’s radius will be 2% bigger than earth’s, giving it about 99.996% earth gravity (if my calculations are correct, which is by no means guaranteed).
I want the orbits of the two moons to be stable because they are in mean resonance to each other. So far I’ve been using, amongst other things, the research of Canup and Stewart, which you can see here.
http://www.xtec.es/recursos/astronom/moon/canupe.htm
Following their information I’d like to work out orbits and the mean resonance ratio of a large inner moon (4.6368 × 10 to the power of 22 kilograms) and a small outer moon (2.87776 × 10 to the power of 22 kilograms).
So now for the question; can anyone help me work out what the semimajor axes of these moons need to be for them to enter a stable relationship with each other and their primary (I know terrestrial multiple moon systems are unlikely, but I’m trying to figure out the likeliest configuration)?
Later on I’d like to figure out when the moons will be in conjunction and what the tides on the planet would be like, for now I’d be very happy to figure out semimajor axes and orbital eccentricity.
Any help would really be much appreciated. If I ever get published I will, of course, acknowledge anyone who helps (but for the moment it’s just a hobby).
Thanks again
Karl
