} C) 



rolling motion to right and left and not from any fixed 

 slanting of their axes is clearly demonstrated in the 

 case of the planet Saturn. 



We have here two pictures of Saturn of which one 

 represents the imaginary inclination of that planet's axis 

 during the course of a solar year equal in the case 

 of Saturn to 30 years on earth, the other photographic 

 views of Saturn covering the same 30 years interval 



Saturn. 



From a comparison of these two illustrations it is not 

 difficult to assure oneself that between the presumptive 

 eclectic of received science and the actual position of the 

 planet Saturn in the sky there is absolutely nothing in 

 common. 



If we ascribe the eclectic to the inclination of the 

 earth's axis then, in view of the enormous distance of the 

 stars from our solar system, the Earth's axis at the North 



2* 



