Backyard Voyager

Amateur Telescope Making -- Building an ultra light 12" dob
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My amateur telescope making page

The "Deep Space Scope" Design

DS-3 | Mirror cell construction | Secondary cage construction | Mirror box construction | Plop Design | NEWT design | Finish the mirror box | Truss construction | Bearing construction and mounting | Rocker box construction | Details, current issues and future enhancements | Baffling and Contrast |

Overview

The mirror cell for DS-3 was created using experience, guesswork and trial and error.  These worked quite well, but there should be a better way.  Fortunately, there is.  It is a program called Plop.  See the section "Sources and Supplies" for where to find and download Plop.  I want to thank Toshimi Taki for the original formulas (Sky & Telescope, April 1996), and especially David Lewis for creating the graphical program Plop.  David, you did the ATM community a great service!

A few important issues about plop:

  • All measurements are in millimeters.  Multiply inches by 25.4 to get millimeters.  Also, divide millimeters by 25.4 to get inches.
  • Human vision is most sensitive to light in the 500 nanometer range (0.0005 millimeters)
  • Plop returns PV (Peak to Valley) analysis as millimeters.  To get fractional wavelengths of error, use this formula: WaveFracDen  = 0.0005 / PV.
  • Colour Plot shows highs and lows as red and blue, with middle ground shown as green.  Green is good, red and/or blue are BAD.
  • BUT - Plop scales highs and lows, thus ALWAYS shows red and blue.  As recommended by Mark Holm on the ATM list, use the following setup options: in Colour Plot, Options, Picture Options, Z-axis range in plots, insert 0.00003125.  This represents a 1/16 wave mirror, or a 1/8 wave P-V mirror at the eyepiece.
  • Note that we are talking about errors due to the mirror cell.  Errors in the mirror will ADD to these mirror cell induced errors.

A few items about DS-3 and simulating it's mirror cell:

  • I used three series of six support points to simulate DS-3's mirror cell.
  • The 12" mirror for DS-3 is made from BK7 glass.

Input parameters that model a 3 support cell (NOT DS-3's cell) are as follows:

  • Primary mirror diameter: 304.8mm
  • Primary mirror thickness: 38.1mm
  • Focal length: 1524mm
  • Secondary mirror diameter: 52.1mm
  • Modulus:  8100
  • Poisson: 0.208
  • Density: 2.51e-6
  • 1 ring, 3 support points.
  • Support radius: 0.409 percent from center.

Results of a 3 support system:

  • Visible P-V Error: 2.21747e-05mm
  • Visible RMS Error: 4.991e-06mm
C plotC plot

Here is the mesh that PLOP created, and the location of the three supports.


C plot

Color plot of the deformities of the mirror.  Blue is high, red is low.

Input parameters that kind of simulate DS-3 that I used for plop are as follows:

  • Primary mirror diameter: 304.8mm
  • Primary mirror thickness: 38.1mm
  • Focal length: 1524mm
  • Secondary mirror diameter: 52.1mm
  • Modulus:  8100
  • Poisson: 0.208
  • Density: 2.51e-6
  • 6 rings, 18 support points.  (E-mail me if you want details)
  • Support radius: Variable

Results:

  • Visible P-V Error: 2.37061e-05mm
  • Visible RMS Error: 5.46034e-06mm

C plotC plot

Here is the mesh that PLOP created, and the location of all of the supports.  I am trying to model the pads that hold the mirror.

DS3 color plot

Color plot of the deformities of the mirror.  Blue is high, red is low.


Conclusions:

  • Assuming a perfect mirror, the P-V numbers translate into a 1/21 wave mirror cell.  This is 10.5 wave at the eyepiece.  Ummm.
  • The mirror cell that I used on DS-3 was theoretically acceptable, but no better than acceptable.
  • In real life, this mirror cell works well.  Since I am pretty sure that Plop is mathematically correct, I can only assume that the standard that I set for this analysis is strict enough.  BUT, I wouldn't want it to be any worse!
  • It turns out that if the most outside supports are widened, which would be true for supports that were triangles rather than circles, the mirror cell is MUCH better.  Sounds like a great rainy weekend project.
 

Details of the steps to design and build this scope are in the following pages:

 
     
     

 

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