- Great Paris Exhibition Telescope of 1900
The Great Paris Exhibition Telescope of 1900, with an objective lens of 1.25 m (49.2 inches) in diameter, was the largest
refracting telescopeever constructed. It was built as the centerpiece of the Paris Universal Exhibition of 1900. Its construction was instigated in 1892by 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.
The telescope had two interchangeable objective lenses (for visual and photographic use respectively) 1.25 m (49.2 inches) in diameter, with a
focal lengthof 57 m (187 ft). 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 movable plane mirror 2 m (6.56 ft) in diameter, mounted in a large cast-iron frame at the objective lens end of the telescope. The horizontal steel tube was 60 m (197 ft) 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. [Launay, pp. 463-466.] 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, near the Eiffel Tower. The tube, oriented north-south, was made up of 24 cylinders 1.5 meters in diameter and rested on 7 concrete and steel pillars; its axis was 7 meters above the floor. The room at the end which housed siderostat with the mirror had a movable dome to allow direct access to the sky. [Launay, pp. 467-468.]
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, made by Charles Le Morvan (1865–1933), were published in the " Strand Magazine", November 1900. [Launay, pp. 471-473.]
After the company, organized in 1886 to build the telescope, went bankrupt the telescope was put up for auction (1909). No buyer was found and eventually the components were scrapped. The 2-meter 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. [Launay, p. 468-471.]
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. But as the centrepiece of an exhibition showcasing the best of the recent advances in industry and technology it served its purpose. [Launay, pp. 461–462.]
* 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.
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