REVOLUTION OF MOON. 



earth are equal, and on that line of demarkation be- 

 tween the forces of cold and heat the moon moves 

 about the earth. 



The moon also sinks to the medium in relativity 

 consistent with the gaseous center within it toward the 

 sun, and in consequence it is like a balloon bobbing up 

 and down on the line of demarkation of three forces. 



When located beyond the earth or being in oppo- 

 sition or superior conjunction it is then shielded from 

 the extreme rays of the sun by the earth and likewise 

 deprived of the heating rays of the earth which cannot 

 be deflected upon it owing to position. And in con- 

 sequence it moves toward the earth, thereby proving 

 why it nears to the earth during this portion of its trip 

 around the earth. It also solidifys in the particles that 

 constitute its make up by the congealing action of the 

 undetered cold during the secluded period. Having 

 gained in compression by the action of the cold during 

 this period, it will be naturally heavier in relativity. 

 And when the movements of the earth cause the earth 

 to change position owing to the movement in its orbit, 

 it leaves the moon falling toward the sun by the motion 

 already under way. And the body of the moon gain- 

 ing in weight all the time, owing to the action of the 

 cold, causes it to move further on toward the sun. And 

 at the same time the portion of the earth comes into 

 play with the deflected rays of heat propelling at right 

 angles upon the moon, thereby causing it to move in a 

 kind of elongated ellipse toward the sun. 



When this already accelerated motion gained 



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