Hello kikinho,
kikinho wrote:The orbits are not so good because I don't know too much about planet masses and kepler laws. And there are some calculations that I can't make, because it's too big or difficult for me. The big problem is that I don't have some notions about physics. Thats why my systems look like unrealistic. I only did a system in a W star because I think nobody wanted to do a system in this special kind of star.
I'd recommend you keep the spacing of your orbits, and correct the periods to match - your orbit sizes are reasonable. If you wish to make realistic orbital periods, here's what to do (I've tried to make it simple):
1. Decide a mass
M for your central star. For the W star I recommend the 20 solar masses your first planet is matched to. (By the way, the reason not many choose a W star to put planets around is that these high power stars are so short lived (millions of years, rather than billions of years) that professional astronomers think planets don't have much time to form around them, or they'd be so young, that they'd not evolve even microbial life).
2. For planets, the Celestia standard is to specify an orbit's semi-major axis in A.U., the period in Earth years, and the orbited mass in solar masses. If your planet's semi-major axis measured in A.U. is
A, then the period
P in Earth years is calculated as the square root of P ? A ? A ? A.
Here are the corrected periods for your Rabud planets:
Code: Select all
Planet Semi-Major Period, P
Axis, A
(A.U.) (Yr)
Hibrocadim 0.200 0.400
Heliomida 0.400 1.131
Sulberion 3.500 29.283
Tihocanuaran/Ourimia 6.000 65.727
Aqualakezome 8.000 101.193
Jerivania 12.000 185.903
Alexkidabrilandia 18.600 358.744
Jolistea 27.300 637.909
Saerimetnoshiba 72.000 2732.208
See if you can calculate the same numbers...
3. For moons of planets, you have to define a mass for the orbited planet in Earth masses (not solar masses). To get a moon's orbital period, it's like above, but you have to adjust for the different Celestia measurement standards for moons: Earth masses for orbited mass, Earth days for period and km for semi-major axis. Then, use this equation for P, M and A:
P = 27.321661 ? SquareRoot ( M ? A ? A ? A / 56,800,235,584,000,000 ) )
The equation's a bit more complicated, but the principle is the same.
4. If you want to make realistic masses for planets, try this. If you know the radius of a planet in km (R), then its density in Earth masses is:
M = 4/3 * 3.14159 * R * R * R * Density
Density is relative to Earth's average density ( 5,520 kilogrammes per cubic metre, or kg/m? ): Density = planet density divided by Earth's density. So, you just need to know typical densities for planets of certain sizes or compositions:
Terrestrial planets: 3,000 kg/m? to 6,000 kg/m? (Mercury 5,250, Venus 4,950, Earth 5,520, Moon 3,450, Mars 4,600).
Ice giants : 1,000 kg/m? to 2,500 kg/m? (Uranus 1,200, Neptune 1,800 ).
Gas giants: 500 kg/m? to 1,500 kg/m? ( Jupiter 1,350, Saturn 700 ).
Light brown dwarf: (10 Jupiters) 10,000 kg/m?.
Heavy brown dwarf: (80 Jupiters) 1,000,000 kg/m? (yes!).
Some materials.
Air you breathe: 13 kg/m?.
Water/Ice: 1,000 kg/m?.
Rock: 3,000 kg/m?.
Iron, Nickel: 8,000 kg/m?.
kikinho wrote:You will see my next addon... the biggest name I did is for a spaceship and is very, very simple...: Novalumercobasterinocomuterlaiscoverdometeilonismirantercrombarkrostermoloispirtingrus.
What do you think of this name for a alien spaceship?
Er, not very memorable...?
. Watch out that you don't hit a software limit with string lengths, and I think people won't like typing that name into anywhere!
kikinho wrote:Ah... and my next addon will have many systems. The major system have 40 planets and a G6V star with a size of 0.94 Rsun.
No particular reason why a G6V star can't have 40 planets, just so long as their orbits are not unstable through perturbations...
Spiff.