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The Great Paris Exhibition Telescope of 1900, with an
objective lens In optical engineering, the objective is the optical element that gathers light from the object being observed and focuses the light rays to produce a real image. Objectives can be a single lens or mirror, or combinations of several optical elem ...
of in diameter, was the largest
refracting telescope A refracting telescope (also called a refractor) is a type of optical telescope that uses a lens as its objective to form an image (also referred to a dioptric telescope). The refracting telescope design was originally used in spyglasses and a ...
ever constructed. It was built as the centerpiece of the Paris Universal Exhibition of 1900. Its construction was instigated in 1892 by François Deloncle (1856–1922), a member of the French Chambre des Députés. Since it was built for exhibit purposes within a large metropolis, and its design made it difficult to aim at astronomical objects, it was not suited for scientific use. When the year-long exposition was over, its builders were unable to sell it. It was ultimately broken up for scrap; the lenses are still stored away at the Paris Observatory.


Design

The telescope had two interchangeable objective lenses (for visual and photographic use respectively) in diameter, with a focal length of . Due to its extremely large size, the telescope was mounted in a fixed horizontal position. Light from astronomical objects was redirected into the optical tube assembly via a Foucault
siderostat A heliostat (from ''helios'', the Greek word for ''sun'', and ''stat'', as in stationary) is a device that includes a mirror, usually a plane mirror, which turns so as to keep reflecting sunlight toward a predetermined target, compensating f ...
, a movable plane mirror in diameter, mounted in a large cast-iron frame at the objective lens end of the telescope. The horizontal steel tube was long. The telescope's eyepiece/plate end could be shifted five feet on rails for focusing. With the lowest power of 500×, the field of view was 3 arc minutes.


Construction of the telescope

The mirror for the siderostat was ground mechanically by the Gautier Company (headed by Paul Gautier, 1842–1909) and took nine months to finish. The blank for the mirror was cast by Georges Despret, director of the Jeumont glassworks in northern France. The lens blanks were cast by Édouard Mantois (1848–1900) and ground by Gautier. By the time the Paris Exhibition opened only the object lens for photographic observation was ready. The visual object lens, unfinished, was put on display nearby.


Erection of the telescope

The telescope was erected in the Palais de l’Optique on the
Champ de Mars The Champ de Mars (; en, Field of Mars) is a large public greenspace in Paris, France, located in the seventh ''arrondissement'', between the Eiffel Tower to the northwest and the École Militaire to the southeast. The park is named after t ...
, near the
Eiffel Tower The Eiffel Tower ( ; french: links=yes, tour Eiffel ) is a wrought-iron lattice tower on the Champ de Mars in Paris, France. It is named after the engineer Gustave Eiffel, whose company designed and built the tower. Locally nicknamed "' ...
. The tube, oriented north-south, was made up of 24 cylinders in diameter and rested on 7 concrete and steel pillars; its axis was above the floor. The room at the end which housed
siderostat A heliostat (from ''helios'', the Greek word for ''sun'', and ''stat'', as in stationary) is a device that includes a mirror, usually a plane mirror, which turns so as to keep reflecting sunlight toward a predetermined target, compensating f ...
with the mirror had a movable dome to allow direct access to the sky.


Scientific observations

A few scientific observations were made using the giant telescope, even though it was not designed for scientific use. Théophile Moreux (1867–1954) observed sunspots through the telescope and made drawings of them. And Eugène Michel Antoniadi (1870–1944) made several drawings of nebulae. As well several large photographs of the surface of the
Moon The Moon is Earth's only natural satellite. It is the fifth largest satellite in the Solar System and the largest and most massive relative to its parent planet, with a diameter about one-quarter that of Earth (comparable to the width of ...
, made by Charles Le Morvan (1865–1933), were published in the '' Strand Magazine'', November 1900.


Aftermath

The company which had organized in 1886 to build the telescope declared bankruptcy after the Expo, and the telescope was put up for auction in 1909. No buyer was found and eventually the components were scrapped. The diameter mirror is on display at the Observatoire de Paris, and two of the lenses have recently been discovered in packing crates in the basement. Poor optics were not why the telescope did not work well. The telescope was located at a fair with much
light pollution Light pollution is the presence of unwanted, inappropriate, or excessive use of artificial Visible spectrum, lighting. In a descriptive sense, the term ''light pollution'' refers to the effects of any poorly implemented lighting, during the day ...
and near a very large city with much air pollution, and near sea level. The tube was not ventilated and the air inside was likely humid. Throughout its existence, the telescope was the butt of many derisive jokes and unflattering cartoons. In part this was due to the belief of the academic community that the telescope would be completely useless. As the centrepiece of an exhibition showcasing the best of the recent advances in industry and technology, it nonetheless served a purpose.Launay, pp. 461–462.


Bibliography

* Paul Gautier, “Note sur le sidérostat à lunette de 60 m de foyer et de 1,25 m d’ouverture,” in ''Annuaire du Bureau des Longitudes pour 1899'' (Paris, 1898), pp. C1–C26. * Françoise Launay, “The Great Paris Exhibition Telescope of 1900”, ''Journal for the History of Astronomy'', 38 (2007), 459–475.


See also

*
List of largest optical refracting telescopes Refracting telescopes use a lens to focus light. The largest refracting telescope in the world is the Yerkes Observatory 40 inch (102 cm) refractor, used for astronomical and scientific observation for over a century. The Swedish 1-m S ...
* List of largest optical telescopes historically


References

{{Authority control Optical telescopes
Telescope A telescope is a device used to observe distant objects by their emission, absorption, or reflection of electromagnetic radiation. Originally meaning only an optical instrument using lenses, curved mirrors, or a combination of both to observ ...
1900 in France 1900s in Paris 1900 in science Great refractors