FREE BOOKS

Author's List




PREV.   NEXT  
|<   220   221   222   223   224   225   226   227   228   229   230   231   232   233   234   235   236   237   238   239   240   241   242   243   244  
245   246   247   248   249   250   251   252   253   254   255   256   257   258   259   260   261   262   263   264   265   266   267   268   269   >>   >|  
here when he first began to observe, they really did decline, and they really disappeared; but this disappearance was only for a time--they again came into view. They were then subjected to ceaseless examination, until gradually their nature became unfolded. With increased telescopic power it was found that the two bodies which Galileo had described as globes on either side of Saturn were not really spherical--they were rather two luminous crescents with the concavity of each turned towards the central globe. It was also perceived that these objects underwent a remarkable series of periodic changes. At the beginning of such a series the planet was found with a truly circular disc. The appendages first appeared as two arms extending directly outwards on each side of the planet; then these arms gradually opened into two crescents, resembling handles to the globe, and attained their maximum width after about seven or eight years; then they began to contract, until after the lapse of about the same time they vanished again. The true nature of these objects was at length discovered by Huyghens in 1655, nearly half a century after Galileo had first detected their appearance. He perceived the shadow thrown by the ring upon the globe, and his explanation of the phenomena was obtained in a very philosophical manner. He noticed that the earth, the sun, and the moon rotated upon their axes, and he therefore regarded it as a general law that each one of the bodies in the system rotates about an axis. It is true, observations had not yet been made which actually showed that Saturn was also rotating; but it would be highly, nay, indeed, infinitely, improbable that any planet should be devoid of such movement. All the analogies of the system pointed to the conclusion that the velocity of rotation would be considerable. One satellite of Saturn was already known to revolve in a period of sixteen days, being little more than half our month. Huyghens assumed--and it was a most reasonable assumption--that Saturn in all probability rotated rapidly on its axis. It was also to be observed that if these remarkable appendages were attached by an actual bodily connection to the planet they must rotate with Saturn. If, however, the appendages were not actually attached it would still be necessary that they should rotate if the analogy of Saturn to other objects in the system were to be in any degree preserved. We see satellites near Jupiter whic
PREV.   NEXT  
|<   220   221   222   223   224   225   226   227   228   229   230   231   232   233   234   235   236   237   238   239   240   241   242   243   244  
245   246   247   248   249   250   251   252   253   254   255   256   257   258   259   260   261   262   263   264   265   266   267   268   269   >>   >|  



Top keywords:

Saturn

 

planet

 

appendages

 

objects

 

system

 
perceived
 

rotated

 

crescents

 
remarkable
 

Huyghens


series
 
bodies
 

Galileo

 

gradually

 
rotate
 

attached

 

nature

 

devoid

 

movement

 
general

conclusion

 

pointed

 
analogies
 

regarded

 

showed

 

velocity

 
rotating
 

highly

 
infinitely
 
rotates

observations

 

improbable

 
connection
 

bodily

 

observed

 

actual

 

analogy

 

satellites

 

Jupiter

 
degree

preserved

 

rapidly

 

probability

 

revolve

 

period

 
sixteen
 

considerable

 

satellite

 

reasonable

 
assumption