Like father like son

Anybody who did physics at school has almost certainly at some point stumbled across Snell’s Law; this is a law in optics that states that for a light ray travelling from one medium into another the ratio of the sines of the angles of incidence and refraction is constant; that ratio is known as the index of refraction of those two media. We’ll come back to Snell’s Law later but who was Snell? Actually there were two of them, father and son, it’s the son who gave his name to the law and actually the family name only has one ‘l’, it’s Snel not Snell. Rudolph Snel van Royan, the father, and Willebrord Snel van Royan, the son, both played a leading role in the establishment of the mathematical sciences in the then very young Dutch Republic and in what follows I will sketch the role that they played. The English misspelling of the family name comes from a false shortening of the Latinised version of the name, Snellius, used by both as a nom de plume, as was they custom in the Early Modern Period.

Rudolph Snel (1546–1613) was born in the town of Oudewater; he studied Hebrew, mathematics and philosophy at various German universities and taught for some time at the University of Marburg. He acquired a medical doctorate in Italy and settled in the town of his birth in 1575. When the seven United Provinces broke away from the Spanish Netherlands in 1568 they lost their university in Leuven, leaving the Dutch Republic without a university. The University of Leiden was founded in 1575 but didn’t have a mathematics department. In 1579 some students asked Rudolph Snel to hold maths lectures at the university. In 1580 he was given a temporary lectureship, which was converted to a professor extraordinarius in 1581. It would be twenty year before he was finally promoted to professor ordinarius. He was however, viewed historically, the first professor of mathematics of the young Dutch Republic.

Rudolph_Snellius

Rudolf Snell (1546-1613), Hebräist, Mathematiker; aus der Bibliotheca chalcographica von Jean-Jacques Boissard und Theodor de Bay Source: Wikimedia Commons

Rudolph Snel was not in anyway a great mathematician but he was a convinced Ramist i.e. he propagated the pedagogic theories of the French philosopher Pierre de la Ramée (1515–1572), who believed in a simplified, practical, anti-Aristotelian pedagogic. As a result Snel was regarded as modern (not in a positive sense) and controversial. In the history of science Rudolph is by no means as significant as his son but he in notable for two things. Firstly, he acted as an informal tutor in mathematics to the theology student Isaac Beeckman (1588–1637), who went on to have a major influence in the development of the mechanical philosophy. Rudolph Snel was also probably the first person to hold lectures on the newly invented telescope, doing so already in 1609. He was certainly the source of Johann Fabricius’ knowledge of the instrument; Fabricius going on to become one of the first telescopic discoverers of sunspots and the first to publish that discovery. Rudolph Snel also possibly played a role in a Dutch telescope acquired by Simon Marius.

Naturally, Willebrord Snel (1580–1626) was born in Leiden. He originally studied law but also devoted much time to mathematics and in 1600 began to teach mathematics at the university. Shortly afterward he left Leiden to go on a study tour of Europe. He visited Adriaan van Roomen the professor of medicine and mathematics in Würzburg, Tycho Brahe and Kepler in Prague and Michael Maestlin in Tübingen. In 1602 he studied law in Paris from whence he went to Switzerland with his father finally returning to the Dutch Republic in 1604.

Willebrord_Snellius

Willebrord Snel Source: Wikimedia Commons

Back in Leiden he devoted his life to mathematics, translating Simon Stevin’s Wisconstighe Ghedachtenissen into Latin as Hypomnemata Mathematica (this was the collected volume of Stevin’s textbooks on mathematical, engineering and science topics) and working on a reconstruction of Apollonius’s books on plane loci; both works were published in 1608. In the same year Willebrord was awarded his M.A. Over the years he assisted his father at the university lecturing on mathematics and when Rudolph died in 1613, Willebrord succeeded him as professor. Like his Father Willebrord was a Ramist and in 1613 he published Ramus’s Arithmetica with a commentary.

Snel’s main interest was geodesy and he was the first to attempt to determine the length of one degree of meridian arc, and thus the circumference of the Earth, using the method of triangulation first suggested by the Frisian mathematicus Gemma Frisius. He carried out his triangulation using instruments (including a large quadrant) designed and constructed by Willem Janszoon Blaeu.

Museum_Boerhaave_-_Snellius_quadrant

Quadrant built by Willem Janszoon Blaeu for Willebrord Snel Image: Museum Boerhaave, Leiden Source: Wikimedia Commons

Snel mapped the stretch between Alkmaar and Bergen op Zoom, two towns roughly on the same meridian. He published his results in his Eratosthenes batavus in Leiden in 1617. Named for the Alexandrian geographer Eratosthenes, who also determined the size of the Earth, and Batavus the Roman name for the Netherlands. Later he extended his triangulation net over most of the Dutch Republic.

Triangulation_Pays-Bas_Snellius

Snel’s Triangulation of the Dutch Republic from 1615 Source: Wikimedia Commons

Snel also published works on astronomy, navigations (coining the term loxodromes for Pedro Nunez’s so-called rhumb lines), and trigonometry. Using the method devised by Van Ceulen—another Leiden professor some of whose work he translated into Latin—he calculated π to thirty-four decimal places. Willebrord died comparatively young in 1626.

You will note that I’ve said nothing in the above about Snell’s Law, the law of refraction. The law of refraction was discovered independently by at least five different scholars of whom Snel was chronologically the third. Refraction plays an important role in observation astronomy, as the rays of light coming from celestial objects are refracted by the earth’s atmosphere, the amount of refraction, i.e. bending, varying with the altitude of the object under observation. The rays coming from an object on the horizon are bent differently to those of one observed overhead. Ptolemaeus was well aware of this problem but was despite extensive research unable to determine the law governing the relationship between the angle of incidence and the angle of refraction. The problem was also well known to Islamic and Medieval European astronomers.

It would appear that the first to discover the correct ratio was the tenth century Persian mathematician Abū Saʿd al-ʿAlāʾ ibn Sahl. In his optical treatise Ibn Sahl gives a geometrical equivalent to the trigonometrical law of refraction.

A Pioneer in Anaclastics: Ibn Sahl on Burning Mirrors and Lenses

Reproduction of Millī MS 867 fol. 7r, showing Ibn Sahl’s discovery of the law of refraction (from Rashed, 1990). Source: Wikipedia Commons

However his work remained unknown even to his Islamic contemporaries and so played no role in the history of optics. The next to discover the law of refraction was the English polymath Thomas Harriot.

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Portrait often claimed to be Thomas Harriot (1602), which hangs in Oriel College, Oxford. Source: Wikimedia Commons

Interestingly although Harriot discussed the problem extensively in a correspondence with Johannes Kepler he never revealed that he had the correct law and also never published it. So his discovery, like Ibn Sahl’s, remained unknown. Kepler needed the law for his, important in the history of optics, Dioptrice from 1611; not knowing it he used an approximations for his pioneering work on the function of lenses, which proved adequate.

Kepler_dioptrice_titul

Source: Wikimedia Commons

The first to publish the correct law was Descartes in his Dioptrique issued as an appendix to his Discours de la méthode in 1637. In France the law is still referred to as Descartes’ Law.issued as an appendix to his Discours de la méthode in 1637. In France the law is still referred to as Descartes’ Law.

Illustration_des_dioptriques_de_Descartes

Descartes’ explanation of the law of refraction by analogy from his Dioptrique Source: Wikimedia Commons

Christiaan Huygens first discovered that Willebrord Snel had stated the law in an unpublished manuscript from 1621 and falsely accused Descartes of plagiarism. In the end, Ibn Sahl’s and Harriot’s discoveries remaining unknown, Snel’s priority was acknowledged and the law of refraction became Snell’s Law. Strangely, somewhat later than Descartes publication, the Scottish optician James Gregory, unaware of this, rediscovered the law based on his research into Kepler’s work in optics.

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James Gregory Source: Wikimedia Commons

The whole story is a wonderful example for multiple-discovery in the history of science, which are in fact much more common than many people think. It also illustrates that important scientific discoveries can get lost and have to be rediscovered, again a not uncommon occurrence.

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5 Comments

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5 responses to “Like father like son

  1. I’ve often see it called the Descartes-Snell law. (Always with two l’s. What with the recent link to the correct pronunciation of ‘Huygens’, you’re really doing the Netherlanders a good turn.)

    Anyway, two further points. First, as far as improving the accuracy of predictive astronomy, getting the refraction tables right mattered a lot. Curtis Wilson writes:

    Through much of the seventeenth century. an erroneous solar parallax … was one of the principal causes of error in solar theories. the other being mistaken refractions; and from these sources error was propagated
    into the theories of all other planets.

    (Tycho had held that refractions of the stars cease above 20°, and those
    of the Sun above 45° of altitude).

    I believe it was Cassini I who first used the Descartes-Snell law in setting up a table of atmospheric refraction for astronomical use.

    Second, the law has a curious relation to the wave and corpuscular theories of light. You can derive it from *either* theory, and the index of refraction ends up being the ratio of the speeds of light in the two media, but with the fraction flipped between the two theories: light *faster* in glass than in air according to Newton, and *slower* according to the wave theory. So when Foucault measure the speed in both media (or maybe air and water, I forget), that was additional evidence for the wave theory. (Though I don’t know whether, historically speaking, it mattered all that much.)

  2. It isn’t really surprising that Tycho thought that the Sun’s refraction was zero above 45 degrees altitude. At T=283 K and P=760 mm Hg, the atmospheric refraction at 45 degrees altitude is 59 arcsec. For a star at 20 degrees altitude, it is 159 arcsec (Allen, Astrophysical Quantities). I would expect that it would be much harder to read the scales of the quadrant at night.

    • Yup, but in the generation or two after Tycho, this error became an obstacle to further progress. Wilson’s article “Predictive astronomy in the century after Kepler” delves into all the hairy details. One detail that particularly struck me: switching from circles to ellipses was hardly the most important Keplerian improvement, purely from the standpoint of accuracy. Conceptually it looms large, but if all you care about is predictive exactness, other things prove more significant.

  3. Somewhat confusingly the triangulation map uses a map of the modern Netherlands with a French legend instead of one of the Dutch Republic.

  4. Pingback: From decimal fractions to sand yachts – the unbelievably fertile mind of Simon Stevin | The Renaissance Mathematicus

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