COSMOS 



YII. 



NEBULOUS SPOTS. AE.E THESE ONLY REMCITE AND VET.! 



DENSE CLUSTERS OF STARS ? THE TWO MAGELLANIC 



CLOUDS, IN WHICH CROWDED NEBULOUS SPOTS ARE IN- 

 TERSPERSED WITH NUMEROUS STELLAP^ SWARMS. THE SO- 

 CALLED COAL-SACKS OP THE SOUTHERN HEMISPHERE. 



Among the visible cosmical bodies occupying the regions 

 of space, besides those which shine with stellar light (wheth- 

 er self-himinous, or illumined like planets, stars isolated or 

 in multiple groups, and revolving round a common center of 

 gravity), there are also masses which present a faint and 

 milder nehidoiis light.^ These bodies, which appear at one 

 time as sharply defined, disk-formed, luminous clouds, at 

 another as irregularly and variously-shaped masses, widely 

 diffused over large spaces, seem to the naked eye, at first 

 sight, to be wholly difierent from those cosmical bodies of 

 which we treated fully in the last four sections of the Astrog- 

 nosy. In the same way that there is an inclination to infer 

 from the observed and as yet unexplained motion of the vis- 

 ible cosmical bodies, f the existence of others hitherto invisi- 

 ble, so the knowledge gained as to the resolvability of a con- 

 siderable number of nebulous spots has recently led to con- 

 clusions regarding the non-existence of all nebulae, and, in- 

 deed, of all cosmical vapor generally. But whether these 

 well-defined nebulous spots be a self-luminous vapory mat 

 ter, or remote, closely-throngyd globular clusters of stars, they 

 must ever remain objects of vast importance in the knowl- 

 edge of the structure of the universe and of the contents of 

 space. 



The number whose positions have been determined by 

 right ascension and declination exceeds 3600. Some of the 



* Cosmos, vol. i., p. 85-89, 91, and 142; vol. ii., p. 328; vol. iii., p 

 37-41. 140, 154, and 162. r Cosmos, vol. iii. p. ^85, 186 



