Abstract
The first modern refractor was built in 1824 by Fraunhofer; its diameter was 23 cm. The sizes of the largest refractors grew linearly with time, culminating in the 102-cm Yerkes telescope (1897) and the 125-cm horizontal refractor with siderostat for the 1900 Universal Exhibition in Paris. This was the end of the giants; however long-focus photographic or visual refractors with diameters 60-70 cm were still being constructed until 1972. In parallel, many short-focus, wide field astrographs were built after 1893. We recall the scientific uses of the large refractors, and discuss why these cumbersome and expensive instruments were not dethroned by the silvered-glass reflecting telescopes until late, in spite of the advantages of the latter.
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Notes
See for an image [1, p. 225]
For a contemporary description (in French, with figure) see [10]
Paul (1848-1905) and Prosper (1849-1903) Henry always worked together.
Fuentès [17], with a picture of the telescope.
Scholl [18], with a photograph.
For details, see [24].
Ritchey [26]; cited by King, op. cit., p. 267.
For the early development of reflecting telescopes in the USA, see [27]
Gascoigne, op. cit., p. 106.
Tobin, op. cit., p. 263.
Mouchez [29]. He was obviously trying to find excuses for the bad quality of the 120-cm reflector of the Observatory, but he is nevertheless right.
Cited by King, op. cit., p. 246.
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Lequeux, J. The great nineteenth century refractors. Exp Astron 25, 43–61 (2009). https://doi.org/10.1007/s10686-009-9154-9
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DOI: https://doi.org/10.1007/s10686-009-9154-9