FREE BOOKS

Author's List




PREV.   NEXT  
|<   80   81   82   83   84   85   86   87   88   89   90   91   92   93   94   95   96   97   98   99   100   101   102   103   104  
105   106   107   108   109   110   111   112   113   114   115   116   117   118   119   120   121   122   123   124   125   126   127   128   129   >>   >|  
. In future, therefore, we shall look upon those regions into which we may now penetrate by means of such large telescopes, as a naturalist regards a rich extent of ground or chain of mountains containing strata variously inclined and directed, as well as consisting of very different materials. The surface of a globe or map, therefore, will but ill delineate the interior parts of the heavens." HERSCHEL'S method of study was founded on a mode of observation which he called _star-gauging_. It consisted in pointing a powerful telescope toward various parts of the heavens, and ascertaining by actual count how thick the stars were in each region. His twenty-foot reflector was provided with such an eye-piece that, in looking into it, he saw a portion of the heavens about 15' in diameter. A circle of this size on the celestial sphere has about one quarter the apparent surface of the sun, or of the full moon. On pointing the telescope in any direction, a greater or less number of stars were visible. These were counted, and the direction in which the telescope pointed was noted. Gauges of this kind were made in all parts of the sky, and the results were tabulated in the order of right ascension. The following is an extract from the gauges, and gives the average number of stars in each field at the points noted in right ascension and north polar distance: ----------------------------------------------------------------- | N. P. D. || | N. P. D. R. A. |78 deg. to 80 deg. || R. A. |92 deg. to 94 deg. | No. of Stars. || | No. of Stars. ------------|-------------------||-----------|------------------- H. M. | || H. M. | 11 6 | 3.1 || 15 10 | 9.4 12 31 | 3.4 || 15 22 | 10.6 12 44 | 4.6 || 15 47 | 10.6 12 49 | 3.9 || 16 8 | 12.1 13 5 | 3.8 || 16 25 | 13.6 14 30 | 3.6 || 16 37 | 18.6 ----------------------------------------------------------------- In this small table, it is plain that a different law of clustering or of distribution obtains in the two regions. Such differences are still more marked, if we compare the extreme cases found by HERSCHEL, as R. A. = 19h 41m, N. P. D. = 74 deg. 33', number of stars per
PREV.   NEXT  
|<   80   81   82   83   84   85   86   87   88   89   90   91   92   93   94   95   96   97   98   99   100   101   102   103   104  
105   106   107   108   109   110   111   112   113   114   115   116   117   118   119   120   121   122   123   124   125   126   127   128   129   >>   >|  



Top keywords:

heavens

 

number

 

telescope

 
pointing
 

direction

 

ascension

 

regions

 
surface
 

HERSCHEL

 

distance


points

 

extreme

 
compare
 

results

 

tabulated

 
gauges
 

marked

 

extract

 

average

 

clustering


future
 

differences

 
distribution
 

obtains

 

greater

 

telescopes

 

founded

 

observation

 
method
 

naturalist


called
 

ascertaining

 

powerful

 

gauging

 
consisted
 

interior

 

inclined

 

extent

 
directed
 

variously


strata

 

mountains

 

consisting

 

delineate

 
materials
 

actual

 

quarter

 

apparent

 
celestial
 

sphere