FREE BOOKS

Author's List




PREV.   NEXT  
|<   285   286   287   288   289   290   291   292   293   294   295   296   297   298   299   300   301   302   303   304   305   306   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   >>   >|  
ticular class of inquirers has, as it were, secreted its own particular order of truths from the general mass of material which observation accumulates; and all other classes of inquirers have made use of these truths as fast as they were elaborated, with the effect of enabling them the better to elaborate each its own order of truths. It was thus in sundry of the cases we have quoted as at variance with M. Comte's doctrine. It was thus with the application of Huyghens's optical discovery to astronomical observation by Galileo. It was thus with the application of the isochronism of the pendulum to the making of instruments for measuring intervals, astronomical and other. It was thus when the discovery that the refraction and dispersion of light did not follow the same law of variation, affected both astronomy and physiology by giving us achromatic telescopes and microscopes. It was thus when Bradley's discovery of the aberration of light enabled him to make the first step towards ascertaining the motions of the stars. It was thus when Cavendish's torsion-balance experiment determined the specific gravity of the earth, and so gave a datum for calculating the specific gravities of the sun and planets. It was thus when tables of atmospheric refraction enabled observers to write down the real places of the heavenly bodies instead of their apparent places. It was thus when the discovery of the different expansibilities of metals by heat, gave us the means of correcting our chronometrical measurements of astronomical periods. It was thus when the lines of the prismatic spectrum were used to distinguish the heavenly bodies that are of like nature with the sun from those which are not. It was thus when, as recently, an electro-telegraphic instrument was invented for the more accurate registration of meridional transits. It was thus when the difference in the rates of a clock at the equator, and nearer the poles, gave data for calculating the oblateness of the earth, and accounting for the precession of the equinoxes. It was thus--but it is needless to continue. Here, within our own limited knowledge of its history, we have named ten additional cases in which the single science of astronomy has owed its advance to sciences coming _after_ it in M. Comte's series. Not only its secondary steps, but its greatest revolutions have been thus determined. Kepler could not have discovered his celebrated laws had it not been for Tycho
PREV.   NEXT  
|<   285   286   287   288   289   290   291   292   293   294   295   296   297   298   299   300   301   302   303   304   305   306   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   >>   >|  



Top keywords:

discovery

 

astronomical

 
truths
 

specific

 
determined
 

application

 

refraction

 
observation
 

bodies

 

places


heavenly

 

calculating

 

astronomy

 
enabled
 

inquirers

 

instrument

 
meridional
 

invented

 

telegraphic

 

accurate


transits
 

registration

 
difference
 
chronometrical
 

measurements

 
periods
 

correcting

 

expansibilities

 

metals

 

prismatic


recently

 

nature

 

spectrum

 
distinguish
 

electro

 

series

 

secondary

 

coming

 

advance

 

sciences


greatest

 

celebrated

 
discovered
 

revolutions

 

Kepler

 

science

 

single

 

accounting

 

precession

 
equinoxes