FREE BOOKS

Author's List




PREV.   NEXT  
|<   483   484   485   486   487   488   489   490   491   492   493   494   495   496   497   498   499   500   501   502   503   504   505   506   507  
508   509   510   511   512   513   514   515   516   517   518   519   520   521   522   523   524   525   526   527   528   529   530   531   532   >>   >|  
ended stratum of stars, but as an actual aggregation, highly irregular in structure, made up of stellar clouds and groups and nodosities. All the facts since ascertained fit in with this conception, to which Proctor added arguments favouring the view, since adopted by Barnard[1616] and Easton,[1617] that the stars forming the galactic stream are not only situated more closely together, but are also really, as well as apparently, of smaller dimensions than the lucid orbs studding our skies. By the laborious process of isographically charting the whole of Argelander's 324,000 stars, he brought out in 1871[1618] signs of relationship between the distribution of the brighter stars and the complex branchings of the Milky Way, which has been stamped as authentic by Newcomb's recent statistical inquiries.[1619] There is, besides, a marked condensation of stars, especially in the southern hemisphere, towards a great circle inclined some twenty degrees to the galactic plane; and these were supposed by Gould to form with the sun a subordinate cluster, of which the components are seen projected upon the sky as a zone of stellar brilliants.[1620] The zone has, however, galactic rather than solar affinities, and represents, perhaps, not a group, but a stream. The idea is gaining ground that the Milky Way is designed, in its main outlines, on a spiral pattern, and that its various branches and sections are consequently situated at very different distances from ourselves. Proctor gave a preliminarily interpretation of their complexities on this principle, and Easton of Rotterdam[1621] has renewed the attempt with better success. A most suggestive delineation of the Milky Way, completed in 1889, after five years of labour, by Dr. Otto Boedicker, Lord Rosse's astronomer at Parsonstown, was published by lithography in 1892. It showed a curiously intricate structure, composed of dimly luminous streams, and shreds, and patches, intermixed with dark gaps and channels. Ramifications from the main trunk ran out towards the Andromeda nebula and the "Bee-hive" cluster in Cancer, involved the Pleiades and Hyades, and, winding round the constellation of Orion, just attained the Sword-handle nebula. The last delicate touches had scarcely been put to the picture, when the laborious eye-and-hand method was, in this quarter, as already in so many others, superseded by a more expeditious process. Professor Barnard took the first photographs ever se
PREV.   NEXT  
|<   483   484   485   486   487   488   489   490   491   492   493   494   495   496   497   498   499   500   501   502   503   504   505   506   507  
508   509   510   511   512   513   514   515   516   517   518   519   520   521   522   523   524   525   526   527   528   529   530   531   532   >>   >|  



Top keywords:

galactic

 

stream

 

Barnard

 

cluster

 

situated

 

nebula

 
laborious
 
process
 

structure

 

Easton


stellar

 
Proctor
 

labour

 

spiral

 
Parsonstown
 

astronomer

 

published

 
lithography
 

Boedicker

 

interpretation


complexities

 

principle

 

branches

 
preliminarily
 

sections

 
Rotterdam
 

suggestive

 

delineation

 

completed

 

success


distances

 

pattern

 

renewed

 

attempt

 

channels

 

scarcely

 

picture

 

touches

 

attained

 

handle


delicate
 

method

 

quarter

 

photographs

 

Professor

 

expeditious

 

superseded

 

patches

 

shreds

 

intermixed