FREE BOOKS

Author's List




PREV.   NEXT  
|<   349   350   351   352   353   354   355   356   357   358   359   360   361   362   363   364   365   366   367   368   369   370   371   372   373  
374   375   376   377   378   379   380   381   382   383   384   385   386   387   388   389   390   391   392   393   394   395   396   397   398   >>   >|  
llowed the energies which were potential in the vegetable, up to their local exhaustion in the animal. But in 1845 a new thought was forced upon him by his calculations. He then, for the first time, drew attention to the astounding amount of heat generated by gravity where the force has sufficient distance to act through. He proved, as I have before stated, the heat of collision of a body falling from an infinite distance to the earth, to be sufficient to raise the temperature of a quantity of water, equal to the falling body in weight, 17,356 deg.C. He also found, in 1845, that the gravitating force between the earth and sun was competent to generate an amount of heat equal to that obtainable from the combustion of 6,000 times the weight of the earth of solid coal. With the quickness of genius he saw that we had here a power sufficient to produce the enormous temperature of the sun, and also to account for the primal molten condition of our own planet. Mayer shows the utter inadequacy of chemical forces, as we know them, to produce or maintain the solar temperature. He shows that were the sun a lump of coal it would be utterly consumed in 5,000 years. He shows the difficulties attending the assumption that the sun is a cooling body; for, supposing it to possess even the high specific heat of water, its temperature would fall 15,000' in 5,000 years. He finally concludes that the light and heat of the sun are maintained by the constant impact of meteoric matter. I never ventured an opinion as to the truth of this theory; that is a question which may still have to be fought out. But I refer to it as an illustration of the force of genius with which Mayer followed the mechanical theory of heat through all its applications. Whether the meteoric theory be a matter of fact or not, with him abides the honour of proving to demonstration that the light and heat of suns and stars may be originated and maintained by the collisions of cold planetary matter. It is the man who with the scantiest data could accomplish all this in six short years, and in, the hours snatched from the duties of an arduous profession, that the Royal Society, in 1871, crowned with its highest honour. Comparing this brief history with that of the Copley Medalist of 1870, the differentiating influence of 'environment,' on two minds of similar natural cast and endowment, comes out in an instructive manner. Withdrawn from mechanical appliances
PREV.   NEXT  
|<   349   350   351   352   353   354   355   356   357   358   359   360   361   362   363   364   365   366   367   368   369   370   371   372   373  
374   375   376   377   378   379   380   381   382   383   384   385   386   387   388   389   390   391   392   393   394   395   396   397   398   >>   >|  



Top keywords:

temperature

 

matter

 
sufficient
 

theory

 

falling

 

weight

 

meteoric

 

maintained

 

genius

 

honour


produce

 
mechanical
 
distance
 

amount

 
question
 

influence

 

similar

 

environment

 

opinion

 

fought


illustration

 

appliances

 

Withdrawn

 

concludes

 
finally
 

constant

 
impact
 

natural

 

differentiating

 

endowment


manner

 
instructive
 

ventured

 

accomplish

 

scantiest

 
crowned
 

highest

 
Society
 

arduous

 

duties


profession

 

Comparing

 
Medalist
 

Copley

 

proving

 
abides
 

Whether

 
snatched
 

history

 

demonstration