BASIC TIPS DESIGNED TO IMPROVE YOUR TELESCOPE
All telescopes have design problems. The reason is that there are always tradeoffs, but 
the following tips are for the more simple and common problems.
 Diffraction: Diffraction is caused by light bouncing off an object in and out of the visual 
light cone that feed a telescope. The way to cut down on diffraction is to paint all 
objects in your telescope flat black so they will reflect less light, except for your mirrors 
obviously. But you might want to blacken the sides of your secondary mirror if it is not 
yet black (be careful). Then try to eliminate or shorten anything that protrudes to the 
inside of your telescope such as screws (many times turning the screw around will help 
alot, this way the extra thread is on the outside of the tube). If you use mirror clips to 
hold your mirror in place, try finding another method to attach the mirror such as clear 
silicone rubber. If you have all of that under control you might consider baffling your 
tube. Your tube is a large source of circular diffraction, which is not very visible in the 
eyepiece unless your are looking for it. It will show up as a not quite black background 
when viewing objects in the telescope. By placing baffles in the tube the diffraction is 
more limited to the edges of the baffle, not the whole length of the tube.
 Optimizing obstruction: If your are building a telescope from scratch or doing a major 
remodel, keep in mind that you can reduce your secondary obstruction by using a low 
profile focuser. Remember the light going to the eyepiece is cone shaped, so the 
closer in toward the tube your eyepiece is the smaller your secondary mirror can be. A 
good low profile focuser is a little pricey but look at the bright side, you will save a little 
money by using a smaller secondary mirror. If your are modifying an existing scope to a 
low profile focuser you will need to move your primary mirror down the tube (away from 
the secondary) the same distance that you have shortened your focuser length in order 
to have the benefit of using a smaller secondary mirror.
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