A Survey of Refractive Systems
for Astronomical Telescopes


by
Roger Ceragioli



This Website is Dedicated to Wolfgang Busch,
Who made the First Practical Oil-Immersion
Triplet Apochromat for Amateur Astronomy in 1974.

 

Introduction.

This web site is meant to describe and illustrate for amateur astronomers and telescope makers some types of refractive systems in use for visual observing with astronomical telescopes--primarily doublet achromats and triplet apochromats--in long and short focal ratios.  It assumes that the reader already has a fundamental knowledge of how telescopes work, and will not discuss the basics.  That information is easily available both from books and many currently existing websites.  Moreover, books and the web also contain extensive information about reflective telescopes, especially the Newtonian reflector.  But what has been lacking is equivalent in-depth information about the design and function of refractive telescopes.  This website aims to remedy that lack.

The site does not try to be comprehensive, although it does strive for depth.  Thus, the term "refractive" does not include catadioptric systems such as Maksutovs, Schmidts, or Houghtons which use mirrors to collect light and refractive elements to correct image errors.  Rather, it concentrates on systems which employ either lenses alone to collect light and correct images, or lenses to collect and mirrors to help correct images.  Therefore, it includes not just achromats and apochromats, but also Schupmann's Medial and Brachymedial telescopes.  The reader should also note that the site is not an equipment review.  Names of living people and current products are avoided, except where minimal reference is necessary.   Reviews of current products can be found on other websites and in books and magazines.

An excellent place from which to begin examining telescopic systems--for both newcomers and those already somewhat familiar with them--is the book, Telescope Optics--a Comprehensive Manual for Amateur Astronomers, by H. Rutten and M. van Venrooij  (Willmann-Bell, 1988).  This text covers all the basics of telescope function and design, as well as the principles of optical ray-tracing, which will be used extensively on this web site to illustrate the error residuals ("aberrations") of the various designs.  In fact, since the subject of refractor design is already an advanced topic, I will assume that the reader has a good working knowledge of this book or something similar.  A more advanced treatment can be found in Uwe Laux's Astrooptik, 2nd ed. (Sterne und Weltraum, 1999), which gives an extensive description and analysis of optical systems currently in use for amateur and professional telescopes, as well as a copious bibliography.  Another excellent text is G.H. Smith's, Practical Computer-Aided Lens Design (Willmann-Bell, 1998), which clearly discusses the basics of geometrical and physical optics and shows in-depth how to go about designing optical systems using current ray tracing software for PCs.  

One of the best and most widely used of these software packages is ZEMAX, marketed by ZEMAX Development Corporation.  All the graphics on this website which show image spots, ray fans, lens layouts and other data regarding refractive systems were derived using ZEMAX.  In Smith's book, mentioned above, he discusses how ZEMAX functions and how it represents optical performance through its many different graphical outputs [cf. Smith, pp. 39-97].  Anyone wishing more information than I give regarding my ZEMAX graphics will do well to consult Smith.  My goal is essentially to extend the discussion of refractive systems found in Rutten and van Venrooij to more types than they cover.
 

N.B.  Special thanks go to Wolfgang Busch, and to his friends Walter Stephani and Hans-Christian Schröder for their valuable help in understanding classic German lenses.  Special thanks also go to James R. Lynch III, an optical engineer of 30 years experieince, who has given useful criticism of my work and made it possible to extract the maximum amount of information from the early Schott glass catalogs.  Without the labor of these gentlemen, my work would be much poorer.  Of course, it goes without saying that the remaining errors on the site are my own.

Table of Contents:
Chapter 1.    Optical Conventions.
Chapter 2.    Primer of Image Aberrations and their Graphical Representation.
Chapter 3a.  Achromats (General Considerations & Cemented Doublets).
Chapter 3b.  Achromats (Contact & Non-Contact Types).
Chapter 4a.  Apochromats (General Considerations & Doublets).
Chapter 4b.  Apochromats (Triplet Systems).
Chapter 5.    The Petzval Telescope & Sub-Aperture Color Correctors.
Chapter 6.    Schupmann's Medial Telescopes.


Last Updated:  June 14, 2005.

Contact:  rogerc@as.arizona.edu