Abstract
The history of the rainbow is as old as that of science. The ancient Greek philosophers tried to describe the rainbow, and Aristotle was the first to fully include it among the phenomena studied by physicists. Sunlight reflected in the clouds, the incidence of light rays, the reason for the rainbow’s circular shape, the optical effect of an infinite depth are aspects that have for centuries intrigued scholars, who studied the rainbow with a mixture science and alchemy, sense and sensibility. In the 17th century the rainbow became a strictly physical phenomenon, the object of rigorous investigations according to the law of reflection and refraction. Here we survey this often forgotten history, from ancient Greeks to modern scientists, the rainbow’s colours belonging to the world of physics but also—as Thomas Young wrote in 1803—to the world of speculation and imagination.
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Notes
In his treatise De iride et de radialibus impressionibus, Theodoric provided a first scientific explanation, still considered phenomenologically valid, of the rainbow, a phenomenon that had already attracted the interest of such scholars as Robert Grosseteste (ca. 1175–1253), Roger Bacon and Witelo (Erazmus Ciolek Witelo, also known as Vitellio, (ca. 1230-post 1280/ante 1314). The German Dominican gave an interpretation of the rainbow as a result of refraction of light in its spectrum of colours, even though he was not actually a scientist, nor in particular an experimentalist, and as a consequence he did not master the experimental method; nevertheless, he showed an attitude to research with a properly scientific object. So the German scholar is a natural interpreter of studies “in the tradition of Albertus Magnus” [see Elisa Chiti, article “Teodorico di Freiberg” in online Manuale di Filosofia Medievale published by the University of Siena, Faculty of Letters and Philosophy]. As regards Theodoric’s work, see his Opera Omnia [44]; it includes the writings De coloribus, De elementis corporum naturalium, De iride et de radialibus impressionibus, De luce et eius origine, De miscibilibus in mixto, De tempore. See also Venturi [45], part III: “Dell’Iride”, pp. 149–246 and Krebs [30].
See, in this regard, Corradi [14].
Kamāl al-Dīn Hasan ibn Ali ibn Hasan al-Fārisī, or Abu Hasan Muhammad ibn Hasan, a mathematician born in Tabriz (Iran), gave important contributions to number theory and to the mathematical theory of light, with interesting insights about colours and rainbows (see Roshdi Rashed, s.v. al-Fārisī, in [48]).
See Gazi Topdemir [23].
See Boyer [7].
See Boyer [8], pp. 127–129.
See Sivin [43], p. 24.
See Albertus Magnus [2], Meteora, Liber III, Meteororum, Trac. IV, Caput X “De causa efficiente et materiali colorum iridis in communi”, pp. 678–679.
See Hackett [27].
See vol. II, pp. 172–201 of Bridges [12]. Moreover, it is necessary to remark that, at the end of 13th century, the Polish philosopher and physicist Witelo, building on Alhazen’s hypoteses, had claimed that the bending of light by refraction was larger the denser the medium through which light had passed. Witelo’s essay, Vitellonis Thuringopoloni opticæ libri decem, is contained in Opticæ Thesaurus by Friedrich Risner (1533-1580), published in Basel in 1572. See also El-Bizri [20].
The writings appearing in this treatise were composed between 1521 and 1552.
See Gedselman [24].
Snell’s law, also known as Snell-Descartes law, describes how a light ray is refracted when passing from a medium to another one with a different refractive index; in general, it is valid only for isotropic substances, such as glass, and shows several similarities to Fermat’s principle (due to Pierre de Fermat, 1601–1665) that “the path taken between two points by a ray of light is the path that can be traversed in the least time”. A first formulation of Snell-Descartes law can be found in a manuscript by the Arab mathematician Abū Sa’d al-‘Alā’ ibn Sahl (X sec.) written in 984; it was later probably guessed in 1602 by Thomas Harriot (1560–1621), an astronomer and a mathematician, who did not publish his work, though. It was rediscovered by Willebrord Snell in 1621, in a form mathematically equivalent, unpublished until his death, and, phinally, republished by Descartes in terms of sine functions in his 1637 Discours de la méthode…, where he used it to solve several problems in optics.
See Brand [10], pp. 30–32.
See Berlin-Kay [4].
“Ex quo clarissime apparet, lumina variorum colorum varia esset refrangibilitate: idque eo ordine, ut color ruber omnium minime refrangibilis sit, reliqui autem colores, aureus, flavus, viridis, cæruleus, indicus, violaceus, gradatim and ex ordine magis magisque refrangibiles”, Newton [40], Propositio II, Experimentum VII.
See Gage [22], p. 140.
“When a ray of light is polarised by reflexion, the reflected ray forms a right angle with the refracted ray”, Brewster [11], p. 132.
For further reading about the controversy Goethe-Newton about colours, see [14].
From Goethe's Maximen und Reflexionen.
For the last two quotations, see [1], p.86.
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Corradi, M. A short history of the rainbow. Lett Mat Int 4, 49–57 (2016). https://doi.org/10.1007/s40329-016-0127-3
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DOI: https://doi.org/10.1007/s40329-016-0127-3