Kaleidoscope

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A kaleidoscope ( /kəˈldəskp/ ) is an optical instrument with two or more reflecting surfaces (or mirrors) tilted to each other at an angle, so that one or more (parts of) objects on one end of these mirrors are shown as a regular symmetrical pattern when viewed from the other end, due to repeated reflection. These reflectors are usually enclosed in a tube, often containing on one end a cell with loose, colored pieces of glass or other transparent (and/or opaque) materials to be reflected into the viewed pattern. Rotation of the cell causes motion of the materials, resulting in an ever-changing view being presented.

Contents

Etymology

Coined by its Scottish inventor David Brewster, [1] "kaleidoscope" is derived from the Ancient Greek word καλός (kalos), "beautiful, beauty", [2] εἶδος (eidos), "that which is seen: form, shape" [3] and σκοπέω (skopeō), "to look to, to examine", [4] hence "observation of beautiful forms." [5] It was first published in the patent that was granted on July 10, 1817. [6]

History

A comparison of the mirror constructions of Kircher (left) and Bradley (right) 1819 brewster - treatise on the kaleidoscope fig 39-40 (kircher - bradley comparison).jpg
A comparison of the mirror constructions of Kircher (left) and Bradley (right)
Patterns when seen through a kaleidoscope tube Kaleidoscopes.jpg
Patterns when seen through a kaleidoscope tube

Multiple reflection by two or more reflecting surfaces has been known since antiquity and was described as such by Giambattista della Porta in his Magia Naturalis (1558–1589). In 1646, Athanasius Kircher described an experiment with a construction of two mirrors, which could be opened and closed like a book and positioned in various angles, showing regular polygon figures consisting of reflected aliquot sectors of 360°. Mr. Bradley's New Improvements in Planting and Gardening (1717) described a similar construction to be placed on geometrical drawings to show an image with multiplied reflection. However, an optimal configuration that produces the full effects of the kaleidoscope was not recorded before 1815. [7]

Video of a rotating kaleidoscope view

In 1814, Sir David Brewster conducted experiments on light polarization by successive reflections between plates of glass and first noted "the circular arrangement of the images of a candle round a center, and the multiplication of the sectors formed by the extremities of the plates of glass". He forgot about it, but noticed a more impressive version of the effect during further experiments in February 1815. A while later he was impressed by the multiplied reflection of a bit of cement that was pressed through at the end of a triangular glass trough, which appeared more regular and almost perfectly symmetrical in comparison to the reflected objects that had been situated further away from the reflecting plates in earlier experiments. This triggered more experiments to find the conditions for the most beautiful and symmetrically perfect conditions. An early version had pieces of colored glass and other irregular objects fixed permanently and was admired by some Members of the Royal Society of Edinburgh, including Sir George Mackenzie who predicted its popularity. A version followed in which some of the objects and pieces of glass could move when the tube was rotated. The last step, regarded as most important by Brewster, was to place the reflecting panes in a draw tube with a concave lens to distinctly introduce surrounding objects into the reflected pattern. [7]

Brewster thought his instrument to be of great value in "all the ornamental arts" as a device that creates an "infinity of patterns". Artists could accurately delineate the produced figures of the kaleidoscope by means of the solar microscope (a type of camera obscura device), magic lantern or camera lucida. Brewster believed it would at the same time become a popular instrument "for the purposes of rational amusement". He decided to apply for a patent. [7] British patent no. 4136 "for a new Optical Instrument called "The Kaleidoscope" for exhibiting and creating beautiful Forms and Patterns of great use in all the ornamental Arts" was granted in July 1817. [6] [8] Unfortunately the manufacturer originally engaged to produce the product had shown one of the patent instruments to some of the London opticians to see if he could get orders from them. Soon the instrument was copied and marketed before the manufacturer had prepared any number of kaleidoscopes for sale. An estimated two hundred thousand kaleidoscopes sold in London and Paris in just three months. Brewster figured at most a thousand of these were authorized copies that were constructed correctly, while the majority of the others did not give a correct impression of his invention. Because so relatively few people had experienced a proper kaleidoscope or knew how to apply it to ornamental arts, he decided to publicize a treatise on the principles and the correct construction of the kaleidoscope. [7]

It was thought that the patent was reduced in a Court of Law since its principles were supposedly already known. Brewster stated that the kaleidoscope was different because the particular positions of the object and of the eye, played a very important role in producing the beautiful symmetrical forms. Brewster's opinion was shared by several scientists, including James Watt. [9]

Philip Carpenter originally tried to produce his own imitation of the kaleidoscope, but was not satisfied with the results. He decided to offer his services to Brewster as manufacturer. [10] Brewster agreed and Carpenter's models were stamped "sole maker". Realizing that the company could not meet the level of demand, Brewster gained permission from Carpenter in 1818 for the device to be made by other manufacturers. In his 1819 Treatise on the Kaleidoscope Brewster listed more than a dozen manufacturers/sellers of patent kaleidoscopes. [7] Carpenter's company would keep on selling kaleidoscopes for 60 years. [11]

In 1987, kaleidoscope artist Thea Marshall, working with the Willamette Science and Technology Center, a science museum located in the Eugene, Oregon, designed and constructed a 1,000 square foot traveling mathematics and science exhibition, "Kaleidoscopes: Reflections of Science and Art." With funding from the National Science Foundation, [12] and circulated under the auspices of the Smithsonian Institution Traveling Exhibition Service (SITES [13] ), the exhibition appeared in 15 science museums over a three-year period, reaching more than one million visitors in the United States and Canada. Interactive exhibit modules enabled visitors to better understand and appreciate how kaleidoscopes function.

Variations

Polyangular Kaleidoscope of R.B. Bate (with adjustable reflector angles), as illustrated in Treatise on the Kaleidoscope (1819) 1819 brewster - treatise on the kaleidoscope fig 18-20.jpg
Polyangular Kaleidoscope of R.B. Bate (with adjustable reflector angles), as illustrated in Treatise on the Kaleidoscope (1819)

General variations

David Brewster defined several variables in his patent and publications:

Different versions suggested by Brewster

In his patent Brewster perceived two forms for the kaleidoscope:

In his Treatise on the Kaleidoscope (1819) he described the basic form with an object cell:

diagrams of the patterns of polycentral kaleidoscoped in Treatise on the Kaleidoscope (1819) 1819 brewster - treatise on the kaleidoscope fig 33-36.jpg
diagrams of the patterns of polycentral kaleidoscoped in Treatise on the Kaleidoscope (1819)

Brewster also developed several variations:

Alternative positions of the reflectors in the kaleidoscope, as illustrated in the 1817 patent. 1817 brewster - kaleidoscope patent fig 4-5.jpg
Alternative positions of the reflectors in the kaleidoscope, as illustrated in the 1817 patent.

Brewster also imagined another application for the kaleidoscope:

Later variations

Manufacturers and artists have created kaleidoscopes with a wide variety of materials and in many shapes. A few of these added elements that were not previously described by inventor David Brewster:

Publications

Cozy Baker (d. October 19, 2010)—founder of the Brewster Kaleidoscope Society—collected kaleidoscopes and wrote books about many of the artists making them in the 1970s through 2001. Her book Kaleidoscope Artistry [15] is a limited compendium of kaleidoscope makers, containing pictures of the interior and exterior views of contemporary artworks. Baker is credited with energizing a renaissance in kaleidoscope-making in the US; she spent her life putting kaleidoscope artists and galleries together so they would know each other and encourage each other. [16]

In 1999 a short-lived magazine dedicated to kaleidoscopes—Kaleidoscope Review—was published, covering artists, collectors, dealers, events, and including how-to articles. This magazine was created and edited by Brett Bensley, at that time a well-known kaleidoscope artist and resource on kaleidoscope information. Changed name to The New Kaleidoscope Review, and then switched to a video presentation on YouTube, "The Kaleidoscope Maker."

Applications

A woman looks into a large kaleidoscope Kaleidoscope San Diego.jpg
A woman looks into a large kaleidoscope

Most kaleidoscopes are mass-produced from inexpensive materials, and intended as children's toys. At the other extreme are handmade pieces that display fine craftsmanship. Craft galleries often carry a few kaleidoscopes, while other enterprises specialize in them, carrying dozens of different types from different artists and craftspeople. Most handmade kaleidoscopes are now made in India, Bangladesh, Japan, the US, Russia and Italy, following a long tradition of glass craftsmanship in those countries.[ citation needed ]

See also

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References

  1. Brewster, David (1858). The Kaleidoscope: Its History, Theory, and Construction with its Application to the Fine and Useful Arts (2 ed.). J. Murray.
  2. καλός Archived 2014-03-17 at the Wayback Machine , Henry George Liddell, Robert Scott, A Greek-English Lexicon, on Perseus
  3. εἶδος Archived 2013-05-25 at the Wayback Machine , Henry George Liddell, Robert Scott, A Greek-English Lexicon, on Perseus
  4. σκοπέω Archived 2012-03-14 at the Wayback Machine , Henry George Liddell, Robert Scott, A Greek-English Lexicon, on Perseus
  5. "Online Etymology Dictionary". Etymonline.com. Archived from the original on 26 June 2010. Retrieved 28 May 2010.
  6. 1 2 3 4 5 6 7 8 9 10 11 12 The Repertory of Patent Inventions. 1817. Archived from the original on 27 November 2017.
  7. 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 Brewster, David (1819). A Treatise on the Kaleidoscope. Edinburgh: Archibald Constable & Co.
  8. "Kaleidoscope patents". Archived from the original on 16 December 2016.
  9. Annals of Philosophy, Or, Magazine of Chemistry, Mineralogy, Mechanics, Natural History, Agriculture, and the Arts. Robert Baldwin. 31 August 1818. p.  451 via Internet Archive. brewster kaleidoscope patent.
  10. The Repertory Of Arts And Manufactures - Second series, volume 33. 1818. Archived from the original on 20 December 2016.
  11. The Perfectionist Projectionist Archived 2011-10-07 at the Wayback Machine , Victorian Microscope Slides. Accessed 1 August 2011
  12. "NSF Award Search". nsf.gov.
  13. "SITES". sites.si.edu.
  14. 1 2 3 4 "Brewster Society - Kaleidoscope U - Kaleidoscopes Periods & Styles". Archived from the original on 1 June 2016.
  15. Cozy, Baker (2001). Kaleidoscope Artistry. USA: C&T Publishing, Inc. p. 144. ISBN   1-57120-135-1.
  16. Bindrim, Kira (19 June 2017). "Long before iPhones, this 19th-century gadget made everyone a mobile addict". Quartz (publication) . Archived from the original on 19 June 2017. Retrieved 19 June 2017.