The Building of ‘Fossil Light’ · 3 Fossil Light Design Criteria •Undriven Dobsonian...
Transcript of The Building of ‘Fossil Light’ · 3 Fossil Light Design Criteria •Undriven Dobsonian...
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The Building of ‘Fossil Light’
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Naming based on a ‘Cosmic Gnome’Naming based on a ‘Cosmic Gnome’ on the side of the ‘Tower of the Ecliptic’ on Tower of the Ecliptic’ on Swansea waterfront
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Fossil Light Design Criteria
•Undriven Dobsonian Newtonian reflector optimised for visual use
on Deep Sky
•Collapse down and fit into the back of an Astra Hatchback
•Quick and easy one-person assembly- with no tools
•Maximum mirror size to meet these criteria thought to be 18”
•“Buy the Mirrors, make the Mechanics”
•Started by buying an f4.5, 18” Newtonian mirror set (Suprax) from
Jon Owen and went from there
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• Started project in 1993. Very few books available then to help with design.
• Some magazine articles from US magazine ‘Telescope Making’.
• Most useful was a small book called ‘Lightweight Giants’ by Steve Overholt
which promoted the use of lightweight materials and composites to make
large telescopes lighter and more manageable
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• The lack of suitable literature slowed me down
immensely, compared to how I would have been
able to progress these days
• However, the lack of information forced me to
come up with my own novel design ideas to solve
issues particularly associated with quick, one-
man assembly
• 3 years before first light. Cost £3,000 and 2,000
hours design and build time. Built almost entirely
in box bedroom in my flat in Colindale.
• ‘Finished’ in 1996
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Order of Play
• Make Upper Tube Assembly
-make as light as possible
-requires design solution for
attachment of truss tubes
• Make Mirror Box
-strong but not unduly heavy
• Make Altitude Bearing Box
-with truss tube attachment blocks
• Fit partly-made Truss Tubes
• Fit mirror and find UTA to mirror
separation for good focus position
• Fit lead weight mirror and find
balance in x and y
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• Make and fit Altitude Bearings to
Bearing Box according to location
of balance axis
• Make Azimuth Bearing Box
• Make Pedestal for Bearing Box
• Shroud and Fan
• Improve ad infinitum!!
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Upper Tube Assembly UTA
•Lightweight but strong, enclosed design
•Lightweight 60mm finder with erect image Amici prism
•Composite material for rings
•Ultra-low profile 2” focuser
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Lower UTA ring- Balsa wood
blocks as core with thin
fibreglass sheet epoxied on
outside to make shell
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Upper UTA ring of
fibreglass + resin
paper honeycomb
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Assembled UTA structure
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•Secondary holder is spring adjustable- non-locking, for quick adjust
•Hollow secondary mirror holder
•Black flocked on view side
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Secondary holder has stainless steel vanes with offset design for max. rigidity
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1460mm finder
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Pole attachment method
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16Finished UTA
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Extending hood on UTA
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Mirror Box
•Holds mirror in position without flexing- 18 pt support.
•Aluminium Framing to make lightweight but strong
•Self-contained transport box for mirror…Mirror ‘Cartridge’
•As small as possible to still hold mirror safely and allow to cool
•Mirror Box 27kg, of which
half is the 37mm thick mirror
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Mirror Box structure
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2018pt support
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Bearing Box
•Bearing Box holds big horseshoe
altitude bearings and connects to
the bottom of the truss tubes and is
the bulkiest structural part of a
truss tube Dobsonian reflector.
•Conventional design has Mirror in
Bearing Box but this makes the
bulkiest component by far the
heaviest too
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•I decided to have a separate Bearing Box and Mirror Box to keep
the heavy part as small as possible and the bulky part as light as
possible. Finished Bearing Box with shroud 17kg (Mirror Box 27kg)
•Aluminium Framing to make lightweight but strong
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23Bearing Box structure
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• Truss tube Clamp
Blocks of Bruynzeel
Multiply marine ply
• Resin coated
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Finding Focus then Balancing
•‘First focus’ with UTA and Mirror Box finished and Bearing Box and
Truss Tubes half-done
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• For balancing, cast a
12.7kg lead ‘dummy mirror’
• Balance both in X and Y
required
Balance point in Y
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Balance point in X
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Altitude Bearings
•Three layers of ½” Multiply marine ply formed into arcs and centred
on balance axis. Coated in black Formica
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Shaping of altitude bearings with disc sander and central pivot
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Mirror Box and Bearing
Box detailing
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Azimuth Box
•Is lower half of Altitude Bearings and whole of Azimuth Bearings
•Marine Ply with composite ground board
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32Mirror box bearing surfaces
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Composite Mirror Box baseboard for maximum stiffness- polyester
foam and 12mm ply sandwich. 75mm thickness total
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Gluing Composite Mirror box baseboard
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First Assembly
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Shroud and Fan•12v fan vital to help keep mirror close to ambient temperature
•Shroud keeps out stray light and convection from body
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Further Mods.
•Insulated aluminium radiator foil on truss poles etc and space
blanket over shroud to reduce ‘inverse tube currents’
•Green Laser Pointer
•Anti-dew measures
-heated Secondary mirror
-heated Finder eyepiece and
Finder objective
•Digital setting circles, Argo Navis
•Primary heaters to prevent
dewing when packed away
•Rollers instead of some of
bearings to improve movement
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Storage of scope
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39One Dobo stored Two Dobos stored
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Whatever you can do, or dream you can do, begin
it. Boldness has genius, power, and magic in it.
Goethe
Large Telescopes are tools that hopefully will receive hard use. They will quickly gather battle scars, as you travel around the country committing astronomy.
Tom Clark
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