SPHERICAL ABERRATION. 



image will be produced at a certain distance from the lens. Let 

 this distance be called d'. 



If the border of the lens be now covered with a ring of card, 

 and the central part with a card disc less in diameter than the 

 ring, so as to leave an uncovered space between the disc and the 

 ring, another faint but distinct image will be produced at a 

 certain distance ?", a little greater than d'. 



If the border be covered with a broader ring of card, and the 

 central part by a still less disc, so as to leave an uncovered ring 

 of surface smaller than the last, another image will be produced 

 still faint and distinct, and at a distance d' t " greater still than d". 



In fine, by continuing this process, it will be found that if the 

 lens be resolved into a series of annular surfaces, concentric with 

 each other and with the lens, a series of images will be produced 

 at distances d', d" } d"', d"", &c., gradually increasing, that pro- 

 duced by the external annulus being at the least distance, 

 and that produced by the spot surrounding the centre at the 

 greatest distance. 



On comparing the series of distances d', d", d'", d"" .... 

 at which these images are placed, a very important circum- 

 stance will be observed in their distribution. It will be found 

 that while those produced by the central annuli are crowded very 

 closely together, those produced by the annuli near the edge of 

 the lens are separated one from another by much more sensible 

 spaces. 



When the entire surface of the lens is uncovered and exposed 

 at once to the object, it is evident that this series of images will 

 be produced simultaneously. Some idea of their distribution 

 along the axis of the lens may be found by referring to fig. 26. 



Fig. 26. 



L 



JW 54321 



The object being oo, and the image produced by the small 

 central spot of lenticular surface being at 1 1, the images formed 

 by the rings of surface immediately contiguous to this spot will 

 be crowded together so closely in front of a screen held at 1 1, 

 that they will all be formed upon the screen with very little 



103 



