The Multiple‐Mirror Telescope
DOI: 10.1063/1.2995182
In the fall of the year 1609 Galileo Galilei made the first systematic celestial observations that employed a telescope, thus helping to bring the skies from the realm of mythology into that of physics. Since his time, telescopes have increased nearly a hundredfold in size, with each major step providing a widening of our horizons. Galileo himself, however, went to some length to demonstrate how an increase in scale, without a change in design or in materials, must inevitably bring a structure to a size where it will no longer function properly, and eventually, to the point where it will even collapse under its own weight.
This article is only available in PDF format
References
1. Galileo Galilei, The Starry Messenger (Stillman Drake, trans, and ed.) Doubleday, Garden City N.Y. (1957); pages 21–58.
2. Dialogues Concerning Two New Sciences (Stillman Drake, trans.) U. of Wisconsin Press, Madison, Wise. (1974); pages 11–13, 126–129.
3. A. Labeyrie, Nouv. Rev. Opt. 5, 141 (1974); https://doi.org/NVROBC
H. A. McAlister, Sky and Tel. 53, 346 (1977).https://doi.org/SKTEA34. L. G. Jacchia, Sky and Tel. 55, 100 (1978).https://doi.org/SKTEA3
5. A. D. Code, Ann. Rev. Astr. and Astrophys. 11, 239 (1973).https://doi.org/ARAAAJ
6. J. P. Chevillard, P. Connes, M. Cuisenier, J. Friteau, C. Marlot, Appl. Opt. 16, 1817 (1977).https://doi.org/APOPAI
7. J. R. P. Angel, M. T. Adams, T. A. Boroson, R. L. Moore, Ap. J. 218, 776 (1977).
More about the Authors
Nathaniel P. Carleton. Harvard–Smithsonian Center for Astrophysics, Cambridge, Mass..
William F. Hoffmann. University of Arizona, Tucson.