FREE BOOKS

Author's List




PREV.   NEXT  
|<   31   32   33   34   35   36   37   38   39   40   41   42   43   44   45   46   47   48   49   50   51   52   53   54   55  
56   57   58   59   60   61   62   63   64   65   66   67   68   69   70   71   72   73   74   75   76   77   78   79   80   >>   >|  
being taken as a centre, then the existing Universe of stars is the result of _irradiation_ from that centre. Now, the laws of irradiation are _known_. They are part and parcel of the _sphere_. They belong to the class of _indisputable geometrical properties_. We say of them, "they are true--they are evident." To demand _why_ they are true, would be to demand why the axioms are true upon which their demonstration is based. _Nothing_ is demonstrable, strictly speaking; but _if_ anything _be_, then the properties--the laws in question are demonstrated. But these laws--what do they declare? Irradiation--how--by what steps does it proceed outwardly from a centre? From a _luminous_ centre, _Light_ issues by irradiation; and the quantities of light received upon any given plane, supposed to be shifting its position so as to be now nearer the centre and now farther from it, will be diminished in the same proportion as the squares of the distances of the plane from the luminous body, are increased; and will be increased in the same proportion as these squares are diminished. The expression of the law may be thus generalized:--the number of light-particles (or, if the phrase be preferred, the number of light-impressions) received upon the shifting plane, will be _inversely_ proportional with the squares of the distances of the plane. Generalizing yet again, we may say that the diffusion--the scattering--the irradiation, in a word--is _directly_ proportional with the squares of the distances. [Illustration] For example: at the distance B, from the luminous centre A, a certain number of particles are so diffused as to occupy the surface B. Then at double the distance--that is to say at C--they will be so much farther diffused as to occupy four such surfaces:--at treble the distance, or at D, they will be so much farther separated as to occupy nine such surfaces:--while, at quadruple the distance, or at E, they will have become so scattered as to spread themselves over sixteen such surfaces--and so on forever. In saying, generally, that the irradiation proceeds in direct proportion with the squares of the distances, we use the term irradiation to express _the degree of the diffusion_ as we proceed outwardly from the centre. Conversing the idea, and employing the word "concentralization" to express _the degree of the drawing together_ as we come back toward the centre from an outward position, we may say that concen
PREV.   NEXT  
|<   31   32   33   34   35   36   37   38   39   40   41   42   43   44   45   46   47   48   49   50   51   52   53   54   55  
56   57   58   59   60   61   62   63   64   65   66   67   68   69   70   71   72   73   74   75   76   77   78   79   80   >>   >|  



Top keywords:

centre

 

irradiation

 
squares
 

distance

 

distances

 

number

 

proportion

 

surfaces

 

occupy

 
luminous

farther
 

shifting

 

position

 
outwardly
 
proceed
 

received

 

proportional

 
diffused
 

express

 
degree

diffusion

 
increased
 
particles
 

diminished

 

properties

 

demand

 
treble
 

existing

 

quadruple

 
Universe

separated
 

double

 

Illustration

 

surface

 

result

 

scattered

 

concentralization

 

drawing

 

employing

 
Conversing

outward
 
concen
 

sixteen

 

directly

 

spread

 
forever
 

direct

 

proceeds

 

generally

 

parcel