Ferman's Cosmos Model
Gravitational Systems Measures
In this page we can see the formulas to obtain the different parameters in the gravitational systems, mainly in the solar or stellar systems.
Although, these formulas are applicable in atoms in the same way. In atoms the parameter M/uM is the atomic weight.
Firstly, we have formula of relation between mass and radius of any solar system by means of using systems' units of mass and radius ( uM, uR ) as we make with atoms.
Advice: The unit of mass and radius are taken from the sun mass 9,1 x 10^30 kg.Although theoretically, a middling star model of our sun could have a little less mass and so that, a little small units of mass and radius.
(4,11 x 10^29 kg--and--3,15 x 10^12 m.)  Nevertheless, this is not significant for our study and formulas.
In stars we can also use the general formula Mass =  4/3. Pi..R^3 x Pi.cube root of M/uM (kg-dcm) aplying the Hidden Parameter (x 10^12)
In the following formula we see the relation between radius of any solar system
(radius in cohesion) and its initial radius.
Also we can see formula to obtain the cohesion coefficient, so later, we can obtain density of gravity in any solar system.
Following we have formula to obtain the maximum gravity density in solar systems, taking as unit of gravity for system to the value  uG .
This value will take at the moment, as indicative or approximate value only.
This maximum density has relative character (among systems) because when nuclei augment their masses, the increasing magnetic forces and temperature expand these nuclei, decreasing this way the gravity central potential.
>>>  Spin Consequences. Polar Direction N-S
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