FREE BOOKS

Author's List




PREV.   NEXT  
|<   307   308   309   310   311   312   313   314   315   316   317   318   319   320   321   322   323   324   325   326   327   328   329   330   331  
332   333   334   335   336   337   338   339   340   341   342   343   344   345   346   347   348   >>  
60,000,000,000,000 of miles, or 600,000 diameters of the earth's orbit, or about sixty million diameters of the sun himself. Taking this for the average distance between the stars, although it is doubtless much greater, and supposing them to be equal in magnitude to each other, and to the sun, we have these most striking results. The sun and the star in Cygnus (and so of the others) would present the same relation as that of two balls of ten inches diameter placed ten thousand miles apart, or one a thousand miles above the North Pole, and the other a like distance below the South Pole of our earth. Preserving the same ratio, we might represent them again, by two half-inch bullets placed, the one at Chicago, and the other on the top of the City Hall in the City of New York; and so on, until finally we would come down to two points, less than a thousandth part of an inch in diameter, requiring the microscope to render them visible, and situated at the distance of a mile asunder. Suppose then an inch of the finest thread of thistle-down cut into a thousand sections, and a globular space as large as the sphere of our earth, occupied with such invisible specks, at distances from each other never less than a mile at least, and we have a fair representation of the visible universe--on a reduced scale, it is true, yet still preserving all the relative magnitudes, and all the adjusted proportions of the parts to each other, and to the whole. On any scale we may assume, all that partakes, in the lowest degree, of sensible materiality, bears but an infinitessimal proportion to what _appears_ to be but vacant space. In this view of the matter it becomes more than a probability that there is no relatively denser solidity than this any where existing. Even in the hardest and apparently most impenetrable matter, the ultimate particles may be as sparse in their relative positions, as are, to each other, the higher compound and component bodies which we know are dispersed at such immense distances as mere points in space. But not to dwell on this idea, there is another of a kindred nature to which we would call attention, although it must often have come home to every serious mind. Who can soberly contemplate the mighty heavens without being struck with what may be called the ISOLATION of the universe, or rather, of the innumerable parts of which it is composed. To the most thoughtful spirit a sense of loneliness must be a main, if not a
PREV.   NEXT  
|<   307   308   309   310   311   312   313   314   315   316   317   318   319   320   321   322   323   324   325   326   327   328   329   330   331  
332   333   334   335   336   337   338   339   340   341   342   343   344   345   346   347   348   >>  



Top keywords:

thousand

 

distance

 
matter
 

visible

 

points

 
diameter
 
universe
 
relative
 

distances

 

diameters


existing
 

solidity

 

impenetrable

 
apparently
 
hardest
 
vacant
 
degree
 

materiality

 

lowest

 
partakes

assume

 

infinitessimal

 

proportion

 

probability

 

appears

 
denser
 

heavens

 

struck

 

mighty

 

contemplate


soberly

 

called

 
ISOLATION
 

loneliness

 

spirit

 

thoughtful

 

innumerable

 
composed
 

component

 

bodies


dispersed

 

compound

 

higher

 

particles

 

sparse

 
positions
 
immense
 

attention

 

nature

 

kindred