Celestron Scope 90 Manuale Utente

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A telescope is an instrument that collects and focuses light.  The nature of the optical design determines how the 
light is focused.  Some telescopes, known as refractors, use lenses, .and other telescopes, known as reflectors 
(Newtonians), use mirrors. 
 
Developed in the early 1600s, the refractor is the oldest telescope design.  It derives its name from the method it 
uses to focus incoming light rays.  The refractor uses a lens to bend or refract incoming light rays, hence the name 
(see Figure 3-1).  Early designs used single element lenses.  However, the single lens acts like a prism and breaks 
light down into the colors of the rainbow, a phenomenon known as chromatic aberration.  To get around this 
problem, a two-element lens, known as an achromat, was introduced.  Each element has a different index of 
refraction allowing two different wavelengths of light to be focused at the same point.  Most two-element lenses, 
usually made of crown and flint glasses, are corrected for red and green light.  Blue light may still be focused at a 
slightly different point. 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
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To focus your telescope, simply turn the focus knob located directly below the eyepiece holder (see Figures 1-1).   
Turning the knob clockwise allows you to focus on an object that is farther than the one you are currently observing.  
Turning the knob counterclockwise from you allows you to focus on an object closer than the one you are currently 
observing. 
 
Note:  If you wear corrective lenses (specifically glasses), you may want to remove them when observing with an 
eyepiece attached to the telescope.  However, when using a camera you should always wear corrective lenses to 
ensure the sharpest possible focus.  If you have astigmatism, corrective lenses must be worn at all times. 
 
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You can change the power of your  telescope just by changing the eyepiece (ocular).  To determine the 
magnification of your telescope, simply divide the focal length of the telescope by the focal length of the eyepiece 
used.  In equation format, the formula looks like this: 
 
 
 
 
 
 
Focal Length of Telescope (mm) 
Figure 3-1 
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