An aerial telescope is a type of very long focal length refracting telescope, built in the second half of the 17th century, that did not use a tube. Instead, the objective was mounted on a pole, tree, tower, building or other structure on a swivel ball-joint. The observer stood on the ground and held the eyepiece, which was connected to the objective by a string or connecting rod. By holding the string tight and maneuvering the eyepiece, the observer could aim the telescope at objects in the sky. The idea for this type of telescope may have originated in the late 17th century with the Dutch mathematician, astronomer and physicist Christiaan Huygens and his brother Constantijn Huygens, Jr., though it is not clear that they invented it.
Invention and application
Very long "tubed" telescopes
Telescopes built in the 17th and early 18th century used single element non-achromatic objective lenses that suffered from interfering rainbow halos (chromatic aberration) introduced by the non-uniform refractive properties of single glass lenses. This degraded the quality of the images they produced. Telescope makers from that era found that a very long focal length objectives had no appreciable chromatic aberration (the uncorrected chromatic aberration fell within the large diffraction pattern at focus). They also realized that when they doubled the diameter of their objectives they had to make the objective's focal length 4 times as long (focal length had to be squared) to achieve the same amount of minimal chromatic aberration. As the objective diameter of these refracting telescopes was increased to gather more light and resolve finer detail they began to have focal lengths as long as 150 feet. Besides having really long tubes these telescopes needed scaffolding or long masts and cranes to hold them up. Their value as research tools was minimal since the telescope's support frame and tube flexed and vibrated in the slightest breeze and sometimes collapsed altogether.
Tubeless "aerial" telescopes
Around 1675 the brothers Christiaan and Constantine Huygens decided to accommodate the very long focal length objectives they were creating by eliminating the tube altogether. In the Huygens' "aerial" telescope the objective was mounted inside a short iron tube mounted on a swiveling ball-joint on top of an adjustable mast. The eyepiece was mounted in another short tube (sometimes on a stand), and the two tubes were kept aligned by a taut connecting string. Christiaan Huygens published designs for these tubeless "aerial telescopes" in his 1684 book Astroscopia Compendiaria, and their invention has been attributed to him and his brother Constantijn, although similar designs were also used by Adrien Auzout; the idea is even sometimes attributed to Christopher Wren.
The Huygens contrived some ingenious arrangements for aiming these "aerial telescopes" at an object visible in the night sky. The telescope could be aimed at bright objects such as planets by looking for their image cast on a white pasteboard ring or oiled translucent paper screen and then centering them in the eyepiece. Fainter objects could be found by looking for the reflection of a lamp held in the observer's hand being bounced back by the objective and then centering that reflection on the object. Other contrivances for the same purpose are described by Philippe de la Hire and by Nicolaas Hartsoeker. The objectives for aerial telescopes sometimes had very long focal lengths. Christiaan Huygens states that in 1686 he and his brother made objectives of 8 inch (200 mm) and 8.5 inch (220 mm) diameter and 170 and 210 ft (52 and 64 m) focal length, respectively. Constantijn Huygens, Jr. presented a 7.5 inch (190 mm) diameter 123 ft (37.5 m) focal length objective to the Royal Society of London in 1690. Adrien Auzout and others made telescopes of from 300 to 600 ft (90 to 180 m) focal length, and Auzout proposed a huge aerial telescope 1,000 ft in length that he would use "to observe animals on the Moon".
Astronomer Giovanni Domenico Cassini had the wooden Marly Tower, originally built as part of the Machine de Marly to lift water for the reservoirs and fountains at the Gardens of Versailles, moved to the grounds of the Paris Observatory. On this tower he mounted long tubed telescopes and the objectives of aerial telescopes made for him by the Italian optician Giuseppe Campani. In 1684 he used one of his aerial telescopes to find Dione and Tethys, two satellites of Saturn. James Bradley, on December 27, 1722, measured the diameter of Venus with an aerial telescope whose objective had a focal length of 212 ft (65 m). Francesco Bianchini tried to map the surface of that same planet and deduce its rotational period in Rome in 1726 using a 2.6" (66 mm) 100 foot focal length aerial telescope.
The extreme difficulty of using these very long focal length telescopes led astronomers to develop alternative designs. One was the reflecting telescope. In 1721 John Hadley showed a Newtonian reflecting telescope to the British Royal Society with 6 inch in diameter mirror. The instrument was examined by Society members James Pound and James Bradley who compared its performance to the 7.5 inch (190 mm) diameter aerial telescope built by Constantijn Huygens, Jr. that the Society had in their collection. In the comparison they noted that the Hadley reflector "will bear such a charge as to make it magnify the object as many times as the latter with its due charge", and that it represented objects as distinct, though not altogether so clear and bright as the Huygens aerial telescope.
The need for very long focal length refracting telescope objectives was finally eliminated with the invention of the achromatic lens in the middle of the 18th century.
- "The Telescope". The Galileo Project. Retrieved 5 March 2012. "After about 1675, therefore, astronomers did away with the telescope tube. The objective was mounted on a building or pole by means of a ball-joint and aimed by means of a string..."
- King, Henry C. (2003), The history of the telescope, ISBN 978-0-486-43265-6
- "The First Telescopes", Cosmic Journey: A History of Scientific Cosmology (Center for History of Physics, a Division of the American Institute of Physics)
- Bell. Ph.D., M.Sc., A. E., Christian Huygens and the Development of Science in the Seventeenth Century
- "Galileo's telescope - Chromatic aberration". Museo Galileo - Istituto e Museo di Storia della Scienza. Retrieved 5 March 2012.
- "How Telescopes Improved", History of Telescopes (Cartage)
- Mém. de l'Acad., 1715
- Miscel. Berol., 1710, vol. i. p. 261
- Paul Schlyter, Largest optical telescopes of the world
- Mark Pendergrast, The 600-foot telescope and monstrous insects in Mirror, Mirror: A History of the Human Love Affair with Reflection, page 97.ISBN 0-465-05470-C
- Price, Fred William (2000-12-11), The planet observer's handbook, p. 279, ISBN 978-0-521-78981-3
- This paragraph is adapted from the 1888 edition of the Encyclopædia Britannica.
- Moore, P, The Mapping of Venus, BRITISH ASTRON. ASSOC. JOURNAL V. 95, NO.2/FEB, P. 50, 1985
- amazing-space.stsci.edu - Hadley’s Reflector
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- Pound reported upon it in Phil. Trans., 1723, No. 378, p. 382.
- Sheehan, William. The Planet Mars: A History of Observation and Discovery.
- Huygens and His Great Refractor
- Institute and Museum of the History of Science - Galileo's telescope - Chromatic aberration Animation explaining the need for very long focal length lenses due to Chromatic aberration.
- ESA - Proceedings of the International Conference Titan, from discovery to Encounter. Extensive detail on Cassini, Huygens and Optics, and Campani's lenses.