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Amateur telescope making

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A 22" Newtonian reflector sits in front of the clubhouse at Stellafane, home of the Springfield Telescope Makers
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A 22" Newtonian reflector sits in front of the clubhouse at Stellafane, home of the Springfield Telescope Makers

The field of amateur telescope making is considered an offshoot of the amateur astronomy community. Amateur telescope makers (sometimes called ATM’s), as their name implies, are not paid professionals. They build their telescopes for the enjoyment of the hobby, or so they can make a personal contribution to the field of astronomy.

The beginnings of a “hobby”

Ever since Galileo took a Dutch invention and adapted it to astronomical use, telescope making has been an evolving discipline. Many astronomers after the time of Galileo built their own telescopes out of necessity, but the advent of amateurs in the field building telescopes for their own enjoyment and education seems to have come into prominence in the 20th century.

There were many published works that sparked interest in building telescopes, including Rev. William F. A. Ellison's 1920 book "The Amateur's Telescope" and several articles in Popular Astronomy by Russell W. Porter, including one appearing in March, 1923 about the [Telescope Makers of Springfield]. In 1925 Albert G. Ingalls featured Porter and the [Springfield Telescope Makers.] in an article he wrote for Scientific American magazine. There was so much public interest, a whole series of articles were written by Ingalls on the subject. Those articles (and later three books titled “Amateur Telescope Making” Vol. 1-3) helped people around the world take on the task of constructing their own instruments. In the US, the ready supply of surplus optical components after World War 2 and later Sputnik and the space race greatly expanded the hobby.

”The Poor Man's Telescope”

A 6” Newtonian reflector built by a school student on display at Stellafane
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A 6” Newtonian reflector built by a school student on display at Stellafane

The types of telescopes that amateurs build vary widely. They range from the very simple to complicated designs including Refractors, Schmidt Cassegrains and Maksutovs. The most popular telescope design is the Newtonian reflector, described by Russell W. Porter as “The Poor Man's Telescope”. The Newtonian has the advantage of being a simple design that allows for maximum size for the minimum expense. And since the design employs a single front surface mirror as its objective it means (for the person creating their own optical elements) that there is only one surface that has to be figured, as apposed to three for the Maksutov and four for the refractor and the Schmidt-Cassegrain. Typically a Newtonian Telescope of 6” aperture is considered a good starter project.

Mirror making

Since the Newtonian Reflector is the most common telescope built by amateur telescope makers, large sections of the literature on the subject are devoted to fabrication of the primary mirror. The mirror has to be carefully "figured" to an extremely accurate paraboloid shape. The tools used to achieve this shape are surprisingly simple, consisting of a of similarly sized glass "tool", a series of finer abrasives, and a polishing "pitch lap" made from a type of tree sap. Through a whole series of random strokes the “mirror” becomes a perfect spherical section. At that point it only takes a slight variation in polishing strokes to create the desired paraboliod shape.

Foucault test

The equipment most amateurs use to test the shape of the mirrors, a Foucault tester, is, like the tools used to create the surface, simple to fabricate. At its most basic it consists of a light bulb, a piece of tinfoil with a pinhole in it, and a razorblade.

Foucault test setup to measure a mirror
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Foucault test setup to measure a mirror

 Shadowing on the surface of the mirror as it appears during Foucault testing, depending on knife-edge position
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Shadowing on the surface of the mirror as it appears during Foucault testing, depending on knife-edge position

After the mirror is polished out it is placed vertically in a stand. The Foucault tester is set up at a distance close to the mirror's radius of curvature. The tester is adjusted so that the returning beam from the pinhole light source is interrupted by the knife edge. Viewing the mirror from behind the knife edge shows a pattern on the mirror surface. If the mirror surface is a perfect sphere, the mirror appears evenly lit across the entire surface. If the surface is parabolic, the mirror looks like a donut or lozenge. It is possible to calculate how closely the mirror surface resembles a perfect paraboloid by placing a special mask over the mirror and taking a series of measurement with the tester. This data is then reduced and graphed against an ideal parabolic curve.

Aluminizing or \"silvering\" the mirror

Once the mirror surface has the correct shape a very thin coating of a highly reflective material is added to the front surface.

Historically this coating was silver. Silvering was put on the mirror chemically. This was then polished. Silvering was typically done by the mirror maker.

Since the 1950s most mirror makers have the coating applied by a firm specializing in the work. Modern coatings usually contain Aluminum and other compounds.

The mirror is aluminized by placing it in a vacuum chamber with electrically-heated nichrome coils that can sublime aluminum. In a vacuum, the hot aluminum atoms travel in straight lines. When they hit the surface of the mirror, they cool and stick. Some mirror coating shops evaporate a layer of quartz on the mirror, others expose it to pure oxygen or air in an oven so that it will form a tough, clear layer of aluminum oxide.

Telescope design

A large fork mounted telescope and several other amateur built telescopes on display at Stellafane
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A large fork mounted telescope and several other amateur built telescopes on display at Stellafane

The telescopes amateur telescope makers build range from back yard variety all the way up to sophisticated instruments that make meaningful contributions to the field of astronomy. Instruments built by amateurs have been employed in planetary study, astrometry, photometry, comet and asteroid discovery to name just a few. Even the “hobbyist” end of the field can break down into several distinct categories such as: observing deep sky objects, observing the planets, solar observing, lunar observation, and astrophotography of all those class of objects. Therefore the design, size, and construction of the telescopes vary as well. Some amateur telescope makers build instruments that, while looking crude, are wholly suited to the purpose they are designed for. Others may strive for a more aesthetic look with high levels of mechanical “finish”.

The difficulty of construction can be a factor in an amateur’s choice of project. For a given design the difficulty of construction grows roughly as the square of the diameter of the objective. For example a Newtonian telescope of 4 inch (100 mm) aperture is a moderately easy science fair project. A 6 inch (150) to 8 inch (200 mm) Newtonian is considered a good compromise size since construction is not difficult and results in an instrument that would be expensive to purchase commercially. A 12 inch (300 mm) to 16 inch (400mm) reflecting telescope is difficult, but still within the ability of the average amateur who has had experience building smaller instruments. Amateurs have constructed telescopes as large as 1 meter across (39 inches), but small groups or astronomy clubs usually take on such projects.

The Dobsonian: A case in point

An amateur built Dobsonian telescope of moderate size
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An amateur built Dobsonian telescope of moderate size

Since the overall design of a telescope tends to be an exercise in creative problem solving the types of instruments amateurs come up with can be unique to their field. A case in point is the Dobsonian telescope. John Dobson, the originator of the design, wanted an instrument fully optimized for deep sky observing. Since Dobson was a monk living in a monastery at the time the telescopes he built had to meet the following criteria:

His solution was not only a unique design, it also consequently caused a quantum leap in the size of instruments that amateurs build.

Telescope making books and other published information

See also

External links

 


From Wikipedia, the Free Encyclopedia. Original article here. Support Wikipedia by contributing or donating.
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