FREE BOOKS

Author's List




PREV.   NEXT  
|<   174   175   176   177   178   179   180   181   182   183   184   185   186   187   188   189   190   191   192   193   194   195   196   197   198  
199   200   201   202   203   204   205   206   207   208   209   210   211   212   213   214   215   216   217   218   219   220   221   222   223   >>   >|  
he remaining one, which is the middle star of the group, is of the third. The Greek letters, as borne by the individual stars of the Plough, are a plain transgression of Bayer's method as above described, for they have certainly not been allotted here in accordance with the proper order of brightness. For instance, the third magnitude star, just alluded to as being in the middle of the group, has been marked with the Greek letter [d] (Delta); and so is made to take rank _before_ the stars composing what is called the "handle" of the Plough, which are all of the second magnitude. Sir William Herschel long ago drew attention to the irregular manner in which Bayer's system had been applied. It is, indeed, a great pity that this notation was not originally worked out with greater care and correctness; for, were it only reliable, it would afford great assistance to astronomers in judging of what changes in relative brightness have taken place among the stars. Though we may speak of using the constellations as a method of finding our way about the sky, it is, however, to certain marked groupings in them of the brighter stars that we look for our sign-posts. Most of the constellations contain a group or so of noticeable stars, whose accidental arrangement dimly recalls the outline of some familiar geometrical figure and thus arrests the attention.[30] For instance, in an almost exact line with the two front stars of the Plough, or "pointers" as they are called,[31] and at a distance about five times as far away as the interval between them, there will be found a third star of the second magnitude. This is known as Polaris, or the Pole Star, for it very nearly occupies that point of the heaven towards which the north pole of the earth's axis is _at present_ directed (see Plate XIX., p. 292). Thus during the apparently daily rotation of the heavens, this star looks always practically stationary. It will, no doubt, be remembered how Shakespeare has put into the mouth of Julius Caesar these memorable words:-- "But I am constant as the northern star, Of whose true-fix'd and resting quality There is no fellow in the firmament." [Illustration: PLATE XIX. THE SKY AROUND THE NORTH POLE We see here the Plough, the Pole Star, Ursa Minor, Auriga, Cassiopeia's Chair, and Lyra. Also the Circle of Precession, along which the Pole makes a complete revolution in a period of 25,868 years, and the Temporary Star discovered by Tycho
PREV.   NEXT  
|<   174   175   176   177   178   179   180   181   182   183   184   185   186   187   188   189   190   191   192   193   194   195   196   197   198  
199   200   201   202   203   204   205   206   207   208   209   210   211   212   213   214   215   216   217   218   219   220   221   222   223   >>   >|  



Top keywords:

Plough

 

magnitude

 

called

 

marked

 
constellations
 
attention
 

middle

 

method

 

brightness

 

instance


directed

 
present
 

revolution

 

apparently

 
rotation
 

complete

 
period
 
interval
 
discovered
 

distance


Temporary

 

occupies

 
heavens
 

heaven

 

Polaris

 
fellow
 

firmament

 

Circle

 
Illustration
 
quality

resting
 

Cassiopeia

 
AROUND
 
northern
 

Shakespeare

 

remembered

 

practically

 

stationary

 
Auriga
 

Precession


constant

 
Julius
 

Caesar

 

memorable

 

irregular

 

manner

 

Herschel

 

William

 

composing

 

handle