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Christiaan Huygens

Christiaan Huygens, Lord of Zeelhem, FRS (/ˈhɡənz/ HY-gənz,[4] US: /ˈhɔɪɡənz/ HOY-gənz,[5] Dutch: [ˈkrɪstijaːn ˈɦœyɣə(n)s] (listen); also spelled Huyghens; Latin: Hugenius; 14 April 1629 – 8 July 1695) was a Dutch mathematician, physicist, engineer, astronomer, and inventor who is regarded as a key figure in the Scientific Revolution.[6][7] In physics, Huygens made seminal contributions to optics and mechanics, while as an astronomer he studied the rings of Saturn and discovered its largest moon, Titan. As an engineer and inventor, he improved the design of telescopes and invented the pendulum clock, the most accurate timekeeper for almost 300 years. A talented mathematician and physicist, his works contain the first idealization of a physical problem by a set of mathematical parameters,[8] and the first mathematical and mechanistic explanation of an unobservable physical phenomenon.[9]

Christiaan Huygens

Born(1629-04-14)14 April 1629
Died8 July 1695(1695-07-08) (aged 66)
The Hague, Dutch Republic
Alma mater
Known for
Scientific career
Fields
Institutions
Academic advisorsFrans van Schooten
Influences
Influenced
Signature

Huygens first identified the correct laws of elastic collision in his work De Motu Corporum ex Percussione, completed in 1656 but published posthumously in 1703.[10] In 1659, Huygens derived geometrically the formula in classical mechanics for the centrifugal force in his work De vi Centrifuga, a decade before Newton.[11] In optics, he is best known for his wave theory of light, which he described in his Traité de la Lumière (1690). His theory of light was initially rejected in favour of Newton's corpuscular theory of light, until Augustin-Jean Fresnel adopted Huygens's principle to give a complete explanation of the rectilinear propagation and diffraction effects of light in 1821. Today this principle is known as the Huygens–Fresnel principle.

Huygens invented the pendulum clock in 1657, which he patented the same year. His horological research resulted in an extensive analysis of the pendulum in Horologium Oscillatorium (1673), regarded as one of the most important 17th century works on mechanics.[8] While it contains descriptions of clock designs, most of the book is an analysis of pendular motion and a theory of curves. In 1655, Huygens began grinding lenses with his brother Constantijn to build refracting telescopes. He discovered Saturn's biggest moon, Titan, and was the first to explain Saturn's strange appearance as due to "a thin, flat ring, nowhere touching, and inclined to the ecliptic."[12] In 1662 Huygens developed what is now called the Huygenian eyepiece, a telescope with two lenses to diminish the amount of dispersion.[13]

As a mathematician, Huygens developed the theory of evolutes and wrote on games of chance and the problem of points in Van Rekeningh in Spelen van Gluck, which Frans van Schooten translated and published as De Ratiociniis in Ludo Aleae (1657).[14] The use of expectation values by Huygens and others would later inspire Jacob Bernoulli's work on probability theory.[15][16]

Biography

 
Portrait of Constantijn (centre) and his five children (Christiaan, top right). Mauritshuis, The Hague.

Christiaan Huygens was born on 14 April 1629 in The Hague, into a rich and influential Dutch family,[17][18] the second son of Constantijn Huygens. Christiaan was named after his paternal grandfather.[19][20] His mother, Suzanna van Baerle, died shortly after giving birth to Huygens's sister.[21] The couple had five children: Constantijn (1628), Christiaan (1629), Lodewijk (1631), Philips (1632) and Suzanna (1637).[22]

Constantijn Huygens was a diplomat and advisor to the House of Orange, in addition to being a poet and a musician. He corresponded widely with intellectuals across Europe; his friends included Galileo Galilei, Marin Mersenne, and René Descartes.[23] Christiaan was educated at home until the age of sixteen, and from a young age liked to play with miniatures of mills and other machines. From his father he received a liberal education, studying languages, music, history, geography, mathematics, logic, and rhetoric, alongside dancing, fencing and horse riding.[19][22]

In 1644, Huygens had as his mathematical tutor Jan Jansz Stampioen, who assigned the 15-year-old a demanding reading list on contemporary science.[24] Descartes was later impressed by his skills in geometry, as was Mersenne, who christened him "the new Archimedes."[25][18][26]

Student years

At sixteen years of age, Constantijn sent Huygens to study law and mathematics at Leiden University, where he studied from May 1645 to March 1647.[19] Frans van Schooten was an academic at Leiden from 1646, and became a private tutor to Huygens and his elder brother, Constantijn Jr., replacing Stampioen on the advice of Descartes.[27][28] Van Schooten brought Huygens's mathematical education up to date, introducing him to the work of Viète, Descartes, and Fermat.[29]

After two years, starting in March 1647, Huygens continued his studies at the newly founded Orange College, in Breda, where his father was a curator. Constantijn Huygens was closely involved in the new College, which lasted only to 1669; the rector was André Rivet.[30] Christiaan Huygens lived at the home of the jurist Johann Henryk Dauber while attending college, and had mathematics classes with the English lecturer John Pell. His time in Breda ended around the time when his brother Lodewijk, who was enrolled at the school, duelled with another student.[7][31] Huygens left Breda after completing his studies in August 1649 and had a stint as a diplomat on a mission with Henry, Duke of Nassau.[19] It took him to Bentheim, then Flensburg. He took off for Denmark, visited Copenhagen and Helsingør, and hoped to cross the Øresund to visit Descartes in Stockholm. It was not to be.[32]

Although his father Constantijn had wished his son Christiaan to be a diplomat, circumstances kept him from becoming so. The First Stadtholderless Period that began in 1650 meant that the House of Orange was no longer in power, removing Constantijn's influence. Further, he realized that his son had no interest in such a career.[33]

Early correspondence

 
Picture of a hanging chain (catenary) in a manuscript of Huygens.

Huygens generally wrote in French or Latin.[34] In 1646, while still a college student at Leiden, he began a correspondence with his father's friend, Marin Mersenne, who died soon afterwards in 1648.[19] Mersenne wrote to Constantijn on his son's talent for mathematics, and flatteringly compared him to Archimedes on 3 January 1647.[35]

The letters show Huygens's early interest in mathematics. In October 1646 there is the suspension bridge and the demonstration that a hanging chain is not a parabola, as Galileo thought.[36] Huygens would later label that curve the catenaria (catenary) in 1690 while corresponding with Gottfried Leibniz.[37]

In the next two years (1647-48), Huygens's letters to Mersenne covered various topics, including a mathematical proof of the law of free fall, the claim by Grégoire de Saint-Vincent of circle quadrature, which Huygens showed to be wrong, the rectification of the ellipse, projectiles, and the vibrating string.[38] Some of Mersenne's concerns at the time, such as the cycloid (he sent Huygens Torricelli's treatise on the curve), the centre of oscillation, and the gravitational constant, were matters Huygens only took seriously towards the end of the 17th century.[8] Mersenne had also written on musical theory. Huygens preferred meantone temperament; he innovated in 31 equal temperament (which was not itself a new idea but known to Francisco de Salinas), using logarithms to investigate it further and show its close relation to the meantone system.[39]

In 1654, Huygens returned to his father's house in The Hague, and was able to devote himself entirely to research.[19] The family had another house, not far away at Hofwijck, and he spent time there during the summer. Despite being very active, his scholarly life did not allow him to escape bouts of depression.[40]

Subsequently, Huygens developed a broad range of correspondents, though picking up the threads after 1648 was hampered by the five-year Fronde in France. Visiting Paris in 1655, Huygens called on Ismael Boulliau to introduce himself, who took him to see Claude Mylon.[41] The Parisian group of savants that had gathered around Mersenne held together into the 1650s, and Mylon, who had assumed the secretarial role, took some trouble to keep Huygens in touch.[42] Through Pierre de Carcavi Huygens corresponded in 1656 with Pierre de Fermat, whom he admired greatly, though this side of idolatry. The experience was bittersweet and somewhat puzzling, since it became clear that Fermat had dropped out of the research mainstream, and his priority claims could probably not be made good in some cases. Besides, Huygens was looking by then to apply mathematics to physics, while Fermat's concerns ran to purer topics.[43]

Scientific debut

 
Christiaan Huygens, relief by Jean-Jacques Clérion (c. 1670).

Like some of his contemporaries, Huygens was often slow to commit his results and discoveries to print, preferring to disseminate his work through letters instead.[44] In his early days, his mentor Frans van Schooten provided technical feedback and was cautious for the sake of his reputation.[45]

Between 1651 and 1657, Huygens published a number of works that showed his talent for mathematics and his mastery of classical and analytical geometry, increasing his reach and reputation among mathematicians.[35] Around the same time, Huygens began to question Descartes's laws of collision, which were largely wrong, deriving the correct laws algebraically and later by way of geometry.[46] He showed that, for any system of bodies, the centre of gravity of the system remains the same in velocity and direction, which Huygens called the conservation of "quantity of movement". While others at the time were studying impact, Huygens's theory of collisions was more general.[7] These results were known through correspondence and in a short article in Journal des Sçavans but would remain largely unpublished until the publication of De Motu Corporum ex Percussione (Concerning the motion of colliding bodies) in 1703.[46]

In addition to his work on mechanics, Huygens made important scientific discoveries: he was the first to identify one of Saturn's moons, Titan, in 1655 and invented the pendulum clock in 1657; both these discoveries brought him fame across Europe.[19] On 3 May 1661, Huygens, together with astronomer Thomas Streete and Richard Reeve, observed the planet Mercury transit over the Sun using Reeve's telescope in London.[47] Streete then debated the published record of Hevelius, a controversy mediated by Henry Oldenburg.[48] Huygens passed to Hevelius a manuscript of Jeremiah Horrocks on the transit of Venus in 1639, printed for the first time in 1662.[49]

In that same year, Sir Robert Moray sent Huygens John Graunt's life table, and shortly after Huygens and his brother Lodewijk dabbled on life expectancy.[44][50] Huygens eventually created the first graph of a continuous distribution function under the assumption of a uniform death rate, and used it to solve problems in joint annuities.[51] Contemporaneously, Huygens, who played the harpsichord, took an interest in Simon Stevin's theories on music; however, he showed very little concern to publish his theories on consonance, some of which were lost for centuries.[52][53] For his contributions to science, the Royal Society of London elected Huygens a Fellow in 1665, making him its first foreign member when he was just 36 years old.[54]

France

 
Huygens, right of centre, from L'établissement de l'Académie des Sciences et fondation de l'observatoire, 1666 by Henri Testelin (c. 1675).

The Montmor Academy, started in the mid-1650s, was the form the old Mersenne circle took after his death.[55] Huygens took part in its debates, and supported its "dissident" faction favouring experimental demonstration over amateurish attitudes.[56] During 1663, he made what was his third visit to Paris; when the Montmor Academy closed down the next year, Huygens took the chance to advocate a more Baconian program in science. Two years later, in 1666, he moved to Paris on an invitation to fill a leadership position at King Louis XIV's new French Académie des sciences.[57]

While at the Académie in Paris, Huygens had an important patron and correspondent in Jean-Baptiste Colbert, First Minister to Louis XIV.[58] However, his relationship with the French Académie was not always easy, and in 1670 Huygens, seriously ill, chose Francis Vernon to carry out a donation of his papers to the Royal Society in London, should he die.[59] The aftermath of the Franco-Dutch War (1672–78), and particularly England's role in it, may have damaged his later relationship with the Royal Society.[60] Robert Hooke, as a Royal Society representative, lacked the finesse to handle the situation in 1673.[61]

The physicist and inventor Denis Papin was assistant to Huygens from 1671.[62] One of their projects, which did not bear fruit directly, was the gunpowder engine.[63] Papin moved to England in 1678 to continue work in this area.[64] Also in Paris, Huygens made further astronomical observations using the observatory recently completed in 1672. He introduced Nicolaas Hartsoeker to French scientists such as Nicolas Malebranche and Giovanni Cassini in 1678.[7][65]

Huygens met the young diplomat Leibniz while visiting Paris in 1672 on a vain mission to meet the French Foreign Minister Arnauld de Pomponne. At this time, Leibniz was working on a calculating machine, and he moved on to London in early 1673 with diplomats from Mainz. From March 1673, Leibniz was tutored in mathematics by Huygens, who taught him analytical geometry.[66] An extensive correspondence ensued over the years, in which Huygens showed at first reluctance to accept the advantages of Leibniz's infinitesimal calculus.[67]

Final years

Huygens moved back to The Hague in 1681 after suffering another bout of serious depressive illness. In 1684, he published Astroscopia Compendiaria on his new tubeless aerial telescope. He attempted to return to France in 1685 but the revocation of the Edict of Nantes precluded this move. His father died in 1687, and he inherited Hofwijck, which he made his home the following year.[33]

On his third visit to England, Huygens met Isaac Newton in person on 12 June 1689. They spoke about Iceland spar, and subsequently corresponded about resisted motion.[68]

Huygens returned to mathematical topics in his last years and observed the acoustical phenomenon now known as flanging in 1693.[69] Two years later, on 8 July 1695, Huygens died in The Hague and was buried, like his father before him, in an unmarked grave at the Grote Kerk.[70]

Huygens never married.[71]

Mathematics

Huygens first became internationally known for his work in mathematics, publishing a number of important results that drew the attention of many European geometers.[72] Huygens's preferred method in his published works was that of Archimedes, though he used Descartes's analytic geometry and Fermat's infinitesimal techniques more extensively in his private notebooks.[19]

Published works

Theoremata de Quadratura

 
Huygens's first publication was in the field of quadrature.

Huygens's first publication was Theoremata de Quadratura Hyperboles, Ellipsis et Circuli (Theorems on the quadrature of the hyperbola, ellipse, and circle), published by the Elzeviers in Leiden in 1651.[44] The first part of the work contained theorems for computing the areas of hyperbolas, ellipses, and circles that paralleled Archimedes's work on conic sections, particularly his Quadrature of the Parabola.[35] The second part included a refutation to Grégoire de Saint-Vincent's claims on circle quadrature, which he had discussed with Mersenne earlier.

Huygens demonstrated that the centre of gravity of a segment of any hyperbola, ellipse, or circle was directly related to the area of that segment. He was then able to show the relationships between triangles inscribed in conic sections and the centre of gravity for those sections. By generalizing these theorems to all conic sections, Huygens extended classical methods to generate new results.[19]

Quadrature was a live issue in the 1650s and, through Mylon, Huygens intervened in the discussion of the mathematics of Thomas Hobbes. Persisting in trying to explain the errors Hobbes had fallen into, he made an international reputation.[73]

De Circuli Magnitudine Inventa

Huygens's next publication was De Circuli Magnitudine Inventa (New findings in the measurement of the circle), published in 1654. In this work, Huygens was able to narrow the gap between the circumscribed and inscribed polygons found in Archimedes's Measurement of the Circle, showing that the ratio of the circumference to its diameter or π must lie in the first third of that interval.[44]

Using a technique equivalent to Richardson extrapolation,[74] Huygens was able to shorten the inequalities used in Archimedes's method; in this case, by using the centre of the gravity of a segment of a parabola, he was able to approximate the centre of gravity of a segment of a circle, resulting in a faster and accurate approximation of the circle quadrature.[75] From these theorems, Huygens obtained two set of values for π: the first between 3.1415926 and 3.1415927, and the second between 3.1415926538 and 3.1415926533.[76]

Huygens also showed that, in the case of the hyperbola, the same approximation with parabolic segments produces a quick and simple method to calculate logarithms.[77] He appended a collection of solutions to classical problems at the end of the work under the title Illustrium Quorundam Problematum Constructiones (Construction of some illustrious problems).[44]

De Ratiociniis in Ludo Aleae

Huygens became interested in games of chance after he visited Paris in 1655 and encountered the work of Fermat, Blaise Pascal and Girard Desargues years earlier.[78] He eventually published what was, at the time, the most coherent presentation of a mathematical approach to games of chance in De Ratiociniis in Ludo Aleae (On reasoning in games of chance).[79][80] Frans van Schooten translated the original Dutch manuscript into Latin and published it in his Exercitationum Mathematicarum (1657).[81][14]

The work contains early game-theoretic ideas and deals in particular with the problem of points.[16][14] Huygens took from Pascal the concepts of a "fair game" and equitable contract (i.e., equal division when the chances are equal), and extended the argument to set up a non-standard theory of expected values.[82] His success in applying algebra to the realm of chance, which hitherto seemed inaccessible to mathematicians, demonstrated the power of combining Euclidean synthetic proofs with the symbolic reasoning found in the works of Viète and Descartes.[83]

Huygens included five challenging problems at the end of the book that became the standard test for anyone wishing to display their mathematical skill in games of chance for the next sixty years.[84] People who worked on these problems included Abraham de Moivre, Jacob Bernoulli, Johannes Hudde, Baruch Spinoza, and Leibniz.

Unpublished work

 
Hofwijck, Huygens's summer home; now a museum.

Huygens had earlier completed a manuscript in the manner of Archimedes's On Floating Bodies entitled De Iis quae Liquido Supernatant (About parts floating above liquids). It was written around 1650 and was made up of three books. Although he sent the completed work to Frans van Schooten for feedback, in the end Huygens chose not to publish it, and at one point suggested it be burned.[35][85] Some of the results found here were not rediscovered until the eighteenth and nineteenth centuries.[10]

Huygens first re-derives Archimedes's results for the stability of the sphere and the paraboloid by a clever application of Torricelli's principle (i.e., that bodies in a system move only if their centre of gravity descends).[86] He then proves the general theorem that, for a floating body in equilibrium, the distance between its centre of gravity and its submerged portion its at a minimum.[10] Huygens uses this theorem to arrive at original solutions for the stability of floating cones, parallelepipeds, and cylinders, in some cases through a full cycle of rotation.[87] His approach was thus equivalent to the principle of virtual work. Huygens was also the first to recognize that, for homogeneous solids, their specific weight and their aspect ratio are the essentials parameters of hydrostatic stability.[88][89]

Natural philosophy

Huygens was the leading European natural philosopher between Descartes and Newton.[19][90] However, unlike many of his contemporaries, Huygens had no taste for grand theoretical or philosophical systems and generally avoided dealing with metaphysical issues (if pressed, he adhered to the Cartesian and mechanical philosophy of his time).[9][35] Instead, Huygens excelled in extending the work of his predecessors, such as Galileo, to derive solutions to unsolved physical problems that were amenable to mathematical analysis. In particular, he sought explanations that relied on contact between bodies and avoided action at a distance.[19][91]

In common with Robert Boyle and Jacques Rohault, Huygens advocated an experimentally oriented, corpuscular-mechanical natural philosophy during his Paris years. This approach was sometimes labelled "Baconian" without being inductivist or identifying with the views of Francis Bacon in a simple-minded way.[92]

After his first visit to England in 1661 and attending a meeting at Gresham College where he learned directly about Boyle's air pump experiments, Huygens spent time in late 1661 and early 1662 replicating the work. It proved a long process that brought to the surface both an experimental issue ("anomalous suspension") and a theoretical issue ("horror vacui"), and which ended in July 1663 as he became a Fellow of the Royal Society. While the replication of results of Boyle's experiments with the air pump trailed off messily, Huygens came to accept Boyle's view of the void against the Cartesian denial of it.[93][94]

Newton's influence on John Locke was mediated by Huygens, who assured Locke that Newton's mathematics was sound, leading to Locke's acceptance of a corpuscular-mechanical physics.[95]

Laws of motion, impact, and gravitation

 
A boating metaphor as a way to think about relative motion, simplifying the theory of colliding bodies, from Huygens's Oeuvres Complètes.

The general approach of the mechanical philosophers was to postulate theories of the kind now called "contact action." Huygens adopted this method, but not without seeing its difficulties and failures.[96] Leibniz, his student in Paris, later abandoned the theory.[97] Seeing the universe this way made the theory of collisions central to physics. Matter in motion made up the universe, and only explanations in those terms could be truly intelligible. While Huygens was influenced by the Cartesian approach, he was less doctrinaire.[98] He studied elastic collisions in the 1650s but delayed publication for over a decade.[29]

Huygens concluded quite early that Descartes's laws for the elastic collision of two bodies must be wrong, and he formulated the correct laws, including the conservation of the product of mass times the square of the speed for hard bodies, and the conservation of quantity of motion in one direction for all bodies.[99] An important step was his recognition of the Galilean invariance of the problems.[100] Huygens had worked out the laws of collision from 1652 to 1656 in a manuscript entitled De Motu Corporum ex Percussione, though his results took many years to be circulated. In 1661, he passed them on in person to William Brouncker and Christopher Wren in London.[101] What Spinoza wrote to Henry Oldenburg about them in 1666, during the Second Anglo-Dutch War, was guarded.[102] The war ended in 1667, and Huygens announced his results to the Royal Society in 1668. He later published them in the Journal des Sçavans in 1669.[29]

In 1659 Huygens found the constant of gravitational acceleration and stated what is now known as the second of Newton's laws of motion in quadratic form.[103] He derived geometrically the now standard formula for the centrifugal force, exerted on an object when viewed in a rotating frame of reference, for instance when driving around a curve. In modern notation:

 

with m the mass of the object, w the angular velocity, and r the radius.[10] Huygens collected his results in a treatise under the title De vi Centrifuga, unpublished until 1703, where the kinematics of free fall were used to produce the first generalized conception of force prior to Newton.[104] The general idea for the centrifugal force, however, was published in 1673 and was a significant step in studying orbits in astronomy. It enabled the transition from Kepler's third law of planetary motion to the inverse square law of gravitation.[105] Yet, the interpretation of Newton's work on gravitation by Huygens differed from that of Newtonians such as Roger Cotes: he did not insist on the a priori attitude of Descartes, but neither would he accept aspects of gravitational attractions that were not attributable in principle to contact between particles.[106]

The approach used by Huygens also missed some central notions of mathematical physics, which were not lost on others. In his work on pendulums Huygens came very close to the theory of simple harmonic motion; the topic, however, was covered fully for the first time by Newton in Book II of the Principia Mathematica (1687).[107] In 1678 Leibniz picked out of Huygens's work on collisions the idea of conservation law that Huygens had left implicit.[108]

Horology

Pendulum clock

 
Spring-driven pendulum clock, designed by Huygens and built by Salomon Coster (1657),[109] with a copy of the Horologium Oscillatorium (1673),[110] at Museum Boerhaave, Leiden.

In 1657, inspired by earlier research into pendulums as regulating mechanisms, Huygens invented the pendulum clock, which was a breakthrough in timekeeping and became the most accurate timekeeper for almost 300 years until the 1930s.[111] The pendulum clock was much more accurate than the existing verge and foliot clocks and was immediately popular, quickly spreading over Europe. He contracted the construction of his clock designs to Salomon Coster in The Hague, who built the clock. However, Huygens did not make much money from his invention. Pierre Séguier refused him any French rights, while Simon Douw in Rotterdam and Ahasuerus Fromanteel in London copied his design in 1658.[112] The oldest known Huygens-style pendulum clock is dated 1657 and can be seen at the Museum Boerhaave in Leiden.[113][114][115][116]

Part of the incentive for inventing the pendulum clock was to create an accurate marine chronometer that could be used to find longitude by celestial navigation during sea voyages. However, the clock proved unsuccessful as a marine timekeeper because the rocking motion of the ship disturbed the motion of the pendulum. In 1660, Lodewijk Huygens made a trial on a voyage to Spain, and reported that heavy weather made the clock useless. Alexander Bruce elbowed into the field in 1662, and Huygens called in Sir Robert Moray and the Royal Society to mediate and preserve some of his rights.[117][113] Trials continued into the 1660s, the best news coming from a Royal Navy captain Robert Holmes operating against the Dutch possessions in 1664.[118] Lisa Jardine doubts that Holmes reported the results of the trial accurately, as Samuel Pepys expressed his doubts at the time.[119]

A trial for the French Academy on an expedition to Cayenne ended badly. Jean Richer suggested correction for the figure of the Earth. By the time of the Dutch East India Company expedition of 1686 to the Cape of Good Hope, Huygens was able to supply the correction retrospectively.[120]

Horologium Oscillatorium

 
Diagram showing the evolute of a curve.

Sixteen years after the invention of the pendulum clock, in 1673, Huygens published his major work on horology entitled Horologium Oscillatorium: Sive de Motu Pendulorum ad Horologia Aptato Demonstrationes Geometricae (The Pendulum Clock: or Geometrical demonstrations concerning the motion of pendula as applied to clocks). It is the first modern work on mechanics where a physical problem is idealized by a set of parameters then analysed mathematically.[8]

Huygens's motivation came from the observation, made by Mersenne and others, that pendulums are not quite isochronous: their period depends on their width of swing, with wide swings taking slightly longer than narrow swings.[121] He tackled this problem by finding the curve down which a mass will slide under the influence of gravity in the same amount of time, regardless of its starting point; the so-called tautochrone problem. By geometrical methods which anticipated the calculus, Huygens showed it to be a cycloid, rather than the circular arc of a pendulum's bob, and therefore that pendulums needed to move on a cycloid path in order to be isochronous. The mathematics necessary to solve this problem led Huygens to develop his theory of evolutes, which he presented in Part III of his Horologium Oscillatorium.[8][122]

He also solved a problem posed by Mersenne earlier: how to calculate the period of a pendulum made of an arbitrarily-shaped swinging rigid body. This involved discovering the centre of oscillation and its reciprocal relationship with the pivot point. In the same work, he analysed the conical pendulum, consisting of a weight on a cord moving in a circle, using the concept of centrifugal force.[8][123]

Huygens was the first to derive the formula for the period of an ideal mathematical pendulum (with mass-less rod or cord and length much longer than its swing), in modern notation:

 

with T the period, l the length of the pendulum and g the gravitational acceleration. By his study of the oscillation period of compound pendulums Huygens made pivotal contributions to the development of the concept of moment of inertia.[124]

Huygens also observed coupled oscillations: two of his pendulum clocks mounted next to each other on the same support often became synchronized, swinging in opposite directions. He reported the results by letter to the Royal Society, and it is referred to as "an odd kind of sympathy" in the Society's minutes.[125] This concept is now known as entrainment.[126]

Balance spring watch

 
Drawing of a balance spring invented by Huygens.

In 1675, while investigating the oscillating properties of the cycloid, Huygens was able to transform a cycloidal pendulum into a vibrating spring through a combination of geometry and higher mathematics.[127] In the same year, Huygens designed a spiral balance spring and patented a pocket watch. These watches are notable for lacking a fusee for equalizing the mainspring torque. The implication is that Huygens thought his spiral spring would isochronize the balance in the same way that cycloid-shaped suspension curbs on his clocks would isochronize the pendulum.[128]

He later used spiral springs in more conventional watches, made for him by Thuret in Paris. Such springs are essential in modern watches with a detached lever escapement because they can be adjusted for isochronism. Watches in Huygens's time, however, employed the very ineffective verge escapement, which interfered with the isochronal properties of any form of balance spring, spiral or otherwise.[129]

Huygens's design came around the same time as, though independently of, Robert Hooke's. Controversy over the priority of the balance spring persisted for centuries. In February 2006, a long-lost copy of Hooke's handwritten notes from several decades of Royal Society meetings was discovered in a cupboard in Hampshire, England, presumably tipping the evidence in Hooke's favour.[130][131]

Optics

Dioptrics

 
Huygens's aerial telescope from Astroscopia Compendiaria (1684).

Huygens had a long-term interest in the study of light refraction and lenses or dioptrics.[132] From 1652 date the first drafts of a Latin treatise on the theory of dioptrics, known as the Tractatus, which contained a comprehensive and rigorous theory of the telescope. Huygens was one of the few to raise theoretical questions regarding the properties and working of the telescope, and almost the only one to direct his mathematical proficiency towards the actual instruments used in astronomy.[133]

Huygens repeatedly announced its publication to his colleagues but ultimately postponed it in favor of a much more comprehensive treatment, now under the name of the Dioptrica.[25] It consisted of three parts. The first part focused on the general principles of refraction, the second dealt with spherical and chromatic aberration, while the third covered all aspects of the construction of telescopes and microscopes. In contrast to Descartes' dioptrics which treated only ideal (elliptical and hyperbolical) lenses, Huygens dealt exclusively with spherical lenses, which were the only kind that could really be made and incorporated in devices such as microscopes and telescopes.[134]

Huygens also worked out practical ways to minimize the effects of spherical and chromatic aberration, such as long focal distances for the objective of a telescope, internal stops to reduce the aperture, and a new kind of ocular known as the Huygenian eyepiece.[134] The Dioptrica was never published in Huygens’s lifetime and only appeared in press in 1703, when most of its contents were already familiar to the scientific world.

Lenses

Together with his brother Constantijn, Huygens began grinding his own lenses in 1655 in an effort to improve telescopes.[135] He designed in 1662 what is now called the Huygenian eyepiece, a set of two planoconvex lenses used as a telescope ocular.[136][137] Huygens's lenses were known to be of superb quality and polished consistently according to his specifications; however, his telescopes did not produce very sharp images, leading some to speculate that he might have suffered from near-sightedness.[138]

Lenses were also a common interest through which Huygens could meet socially in the 1660s with Spinoza, who ground them professionally. They had rather different outlooks on science, Spinoza being the more committed Cartesian, and some of their discussion survives in correspondence.[139] He encountered the work of Antoni van Leeuwenhoek, another lens grinder, in the field of microscopy which interested his father.[8] Huygens also investigated the use of lenses in projectors. He is credited as the inventor of the magic lantern, described in correspondence of 1659.[140] There are others to whom such a lantern device has been attributed, such as Giambattista della Porta and Cornelis Drebbel, though Huygens's design used lens for better projection (Athanasius Kircher has also been credited for that).[141]

Traité de la Lumière

 
Refraction of a plane wave, explained using Huygens's principle in Traité de la Lumière (1690).

Huygens is especially remembered in optics for his wave theory of light, which he first communicated in 1678 to the Académie des sciences in Paris. Originally a preliminary chapter of his Dioptrica, Huygens's theory was published in 1690 under the title Traité de la Lumière[142] (Treatise on light), and contains the first fully mathematized, mechanistic explanation of an unobservable physical phenomenon (i.e., light propagation).[9][143] Huygens refers to Ignace-Gaston Pardies, whose manuscript on optics helped him on his wave theory.[144]

The challenge at the time was to explain geometrical optics, as most physical optics phenomena (such as diffraction) had not been observed or appreciated as issues. Huygens had experimented in 1672 with double refraction (birefringence) in the Iceland spar (a calcite), a phenomenon discovered in 1669 by Rasmus Bartholin. At first, he could not elucidate what he found but was later able to explain it using his wavefront theory and concept of evolutes.[143] He also developed ideas on caustics.[8] Huygens assumes that the speed of light is finite, based on a report by Ole Christensen Rømer in 1677 but which Huygens is presumed to have already believed.[145] Huygens's theory posits light as radiating wavefronts, with the common notion of light rays depicting propagation normal to those wavefronts. Propagation of the wavefronts is then explained as the result of spherical waves being emitted at every point along the wave front (known today as the Huygens–Fresnel principle).[146] It assumed an omnipresent ether, with transmission through perfectly elastic particles, a revision of the view of Descartes. The nature of light was therefore a longitudinal wave.[145]

His theory of light was not widely accepted, while Newton's rival corpuscular theory of light, as found in his Opticks (1704), gained more support. One strong objection to Huygens's theory was that longitudinal waves have only a single polarization which cannot explain the observed birefringence. However, Thomas Young's interference experiments in 1801, and François Arago's detection of the Poisson spot in 1819, could not be explained through Newton's or any other particle theory, reviving Huygens's ideas and wave models. Fresnel became aware of Huygens's work and in 1821 was able to explain birefringence as a result of light being not a longitudinal (as had been assumed) but actually a transverse wave.[147] The thus-named Huygens–Fresnel principle was the basis for the advancement of physical optics, explaining all aspects of light propagation until Maxwell's electromagnetic theory culminated in the development of quantum mechanics and the discovery of the photon.[134][148]

Astronomy

Systema Saturnium

 
Huygens's explanation for the aspects of Saturn, Systema Saturnium (1659).

In 1655, Huygens discovered the first of Saturn's moons, Titan, and observed and sketched the Orion Nebula using a refracting telescope with a 43x magnification of his own design.[13][12] Huygens succeeded in subdividing the nebula into different stars (the brighter interior now bears the name of the Huygenian region in his honour), and discovered several interstellar nebulae and some double stars.[149] He was also the first to propose that the appearance of Saturn, which have baffled astronomers, was due to "a thin, flat ring, nowhere touching, and inclined to the ecliptic”.[150]

More than three years later, in 1659, Huygens published his theory and findings in Systema Saturnium. It is considered the most important work on telescopic astronomy since Galileo's Sidereus Nuncius fifty years earlier.[151] Much more than a report on Saturn, Huygens provided measurements for the relative distances of the planets from the Sun, introduced the concept of the micrometer, and showed a method to measure angular diameters of planets, which finally allowed the telescope to be used as an instrument to measure (rather than just sighting) astronomical objects.[152] He was also the first to question the authority of Galileo in telescopic matters, a sentiment that was to be common in the years following its publication.

In the same year, Huygens was able to observe Syrtis Major, a volcanic plain on Mars. He used repeated observations of the movement of this feature over the course of a number of days to estimate the length of day on Mars, which he did quite accurately to 24 1/2 hours. This figure is only a few minutes off of the actual length of the Martian day of 24 hours, 37 minutes.[153]

Planetarium

At the instigation of Jean-Baptiste Colbert, Huygens undertook the task of constructing a mechanical planetarium that could display all the planets and their moons then known circling around the Sun. Huygens completed his design in 1680 and had his clockmaker Johannes van Ceulen built it the following year. However, Colbert passed away in the interim and Huygens never got to deliver his planetarium to the French Academy of Sciences as the new minister, François-Michel le Tellier, decided not to renew Huygens's contract.[154][155]

In his design, Huygens made an ingenious use of continued fractions to find the best rational approximations by which he could choose the gears with the correct number of teeth. The ratio between two gears determined the orbital periods of two planets. To move the planets around the Sun, Huygens used a clock-mechanism that could go forwards and backwards in time. Huygens claimed his planetarium was more accurate that a similar device constructed by Ole Rømer around the same time, but his planetarium design was not published until after his death in the Opuscula Posthuma (1703).[154]

Cosmotheoros

 
Relative sizes of the Sun and planets in Cosmotheoros (1698).

Shortly before his death in 1695, Huygens completed his most speculative work entitled Cosmotheoros. At his direction, it was to be published only posthumously by his brother, which Constantijn Jr. did in 1698.[156] In this work, Huygens speculated on the existence of extraterrestrial life, which he imagined similar to that on Earth. Such speculations were not uncommon at the time, justified by Copernicanism or the plenitude principle, but Huygens went into greater detail.[157] However, it did so without the benefit of understanding Newton's laws of gravitation, or the fact that the atmospheres on other planets are composed of different gases.[158] Cosmotheoros, translated into English as The celestial worlds discover’d, has been seen as part of speculative fiction in the tradition of Francis Godwin, John Wilkins, and Cyrano de Bergerac. Huygens's work was fundamentally utopian and owes some inspiration from the cosmography and planetary speculation of Peter Heylin.[159][160]

Huygens wrote that availability of water in liquid form was essential for life and that the properties of water must vary from planet to planet to suit the temperature range. He took his observations of dark and bright spots on the surfaces of Mars and Jupiter to be evidence of water and ice on those planets.[161] He argued that extraterrestrial life is neither confirmed nor denied by the Bible, and questioned why God would create the other planets if they were not to serve a greater purpose than that of being admired from Earth. Huygens postulated that the great distance between the planets signified that God had not intended for beings on one to know about the beings on the others, and had not foreseen how much humans would advance in scientific knowledge.[162]

It was also in this book that Huygens published his estimates for the relative sizes of the solar system and his method for calculating stellar distances.[7] He made a series of smaller holes in a screen facing the Sun, until he estimated the light was of the same intensity as that of the star Sirius. He then calculated that the angle of this hole was 1/27,664th the diameter of the Sun, and thus it was about 30,000 times as far away, on the (incorrect) assumption that Sirius is as luminous as the Sun. The subject of photometry remained in its infancy until the time of Pierre Bouguer and Johann Heinrich Lambert.[163]

Legacy

Huygens has been called the first theoretical physicist and a founder of modern mathematical physics.[164][165] Although his influence was considerable during his lifetime, it began to fade shortly after his death. His skills as a geometer and mechanical insights elicited the admiration of many of his contemporaries, including Newton, Leibniz, l'Hôpital, and the Bernoullis.[44] For his work in physics, Huygens has been deemed one of the greatest scientists in the Scientific Revolution, rivaled only by Newton in both depth of insight and the number of results obtained.[6][166] Huygens also helped develop the institutional frameworks for scientific research on the European continent, making him a leading actor in the establishment of modern science.[167]

Mathematics and physics

 
Portrait of Christiaan Huygens by Bernard Vaillant (1686).

In mathematics, Huygens mastered the methods of ancient Greek geometry, particularly the work of Archimedes, and was an adept user of the analytic geometry and infinitesimal techniques of Descartes, Fermat, and others.[85] His mathematical style can be characterized as geometrical infinitesimal analysis of curves and of motion. Drawing inspiration and imagery from mechanics, it remained pure mathematics in form.[72] Huygens brought this type of geometrical analysis to a close, as more mathematicians turned away from classical geometry to the calculus for handling infinitesimals, limit processes, and motion.[40]

Huygens was moreover able to fully employ mathematics to answer questions of physics. Often this entailed introducing a simple model for describing a complicated situation, then analyzing it starting from simple arguments to their logical consequences, developing the necessary mathematics along the way. As he wrote at the end of a draft of De vi Centrifuga:[35]

Whatever you will have supposed not impossible either concerning gravity or motion or any other matter, if then you prove something concerning the magnitude of a line, surface, or body, it will be true; as for instance, Archimedes on the quadrature of the parabola, where the tendency of heavy objects has been assumed to act through parallel lines.

Huygens favoured axiomatic presentations of his results, which require rigorous methods of geometric demonstration: although he allowed levels of uncertainty in the selection of primary axioms and hypotheses, the proofs of theorems derived from these could never be in doubt.[35] Huygens's style of publication exerted an influence in Newton's presentation of his own major works.[168][169]

Besides the application of mathematics to physics and physics to mathematics, Huygens relied on mathematics as methodology, particularly its ability to generate new knowledge about the world.[170] Unlike Galileo, who used mathematics primarily as rhetoric or synthesis, Huygens consistently employed mathematics as a method of discovery and analysis, and insisted that the reduction of the physical to the geometrical satisfy exacting standards of fit between the real and the ideal.[121] In demanding such mathematical tractibility and precision, Huygens set an example for eighteenth-century scientists such as Johann Bernoulli, Jean le Rond d'Alembert, and Charles-Augustin de Coulomb.[164][35]

Although never intended for publication, Huygens made use of algebraic expressions to represent physical entities in a handful of his manuscripts on collisions.[46] This would make him one of the first to employ mathematical formulae to describe relationships in physics, as it is done today.[7] Huygens also came close to the modern idea of limit while working on his Dioptrica, though he never used the notion outside geometrical optics.[171]

Later influence

Huygens's standing as the greatest scientist in Europe was eclipsed by Newton's at the end of the seventeenth century, despite the fact that, as Hugh Aldersey-Williams notes, "Huygens's achievement exceeds that of Newton in some important respects".[172] His very idiosyncratic style and reluctance to publish his work did much to diminish his influence in the aftermath of the Scientific Revolution, as adherents of Leibniz’ calculus and Newton's physics took centre stage.[40][85]

Huygens's analyses of curves that satisfy certain physical properties, such as the cycloid, led to later studies of many other such curves like the caustic, the brachistochrone, the sail curve, and the catenary.[26][37] His application of mathematics to physics, such as in his study of birefringence, would inspire new developments in mathematical physics and rational mechanics in the following centuries (albeit in the new language of the calculus).[9] Additionally, Huygens developed the oscillating timekeeping mechanisms, the pendulum and the balance spring, that have been used ever since in mechanical watches and clocks. These were the first reliable timekeepers fit for scientific use (e.g., it was possible for the first time to make accurate measurements of the inequality of the solar day, which astronomers in the past could not do).[8][121] His work on this area anticipated the union of applied mathematics with mechanical engineering in the centuries that followed.[128]

Portraits

During his lifetime, Huygens and his father had a number of portraits commissioned. These included:

Commemorations

The European Space Agency spacecraft that landed on Titan, Saturn's largest moon, in 2005 was named after him.[175]

A number of monuments to Christiaan Huygens can be found across important cities in the Netherlands, including Rotterdam, Delft, and Leiden.

Works

 
Title page of Oeuvres Complètes I

Source(s):[19]

  • 1650 – De Iis Quae Liquido Supernatant (About parts floating above liquids), unpublished.[176]
  • 1651 – Theoremata de Quadratura Hyperboles, Ellipsis et Circuli, republished in Oeuvres Complètes, Tome XI.[44]
  • 1651 – Epistola, qua diluuntur ea quibus 'Εξέτασις [Exetasis] Cyclometriae Gregori à Sto. Vincentio impugnata fuit, supplement. [177]
  • 1654 – De Circuli Magnitudine Inventa.[35]
  • 1654 – Illustrium Quorundam Problematum Constructiones, supplement. [177]
  • 1655 – Horologium (The clock), short pamphlet on the pendulum clock.[8]
  • 1656 – De Saturni Luna Observatio Nova (About the new observation of the moon of Saturn), describes the discovery of Titan.[178]
  • 1656 – De Motu Corporum ex Percussione, published posthumously in 1703.[179]
  • 1657 – De Ratiociniis in Ludo Aleae (Van reeckening in spelen van geluck), translated into Latin by Frans van Schooten.[14]
  • 1659 – Systema Saturnium (System of Saturn).[177]
  • 1659 – De vi Centrifuga (Concerning the centrifugal force), published posthumously in 1703.[180]
  • 1673 – Horologium Oscillatorium Sive de Motu Pendulorum ad Horologia Aptato Demonstrationes Geometricae, includes a theory of evolutes and designs of pendulum clocks, dedicated to Louis XIV of France.[122]
  • 1684 – Astroscopia Compendiaria Tubi Optici Molimine Liberata (Compound telescopes without a tube).[44]
  • 1685 – Memoriën aengaende het slijpen van glasen tot verrekijckers, dealing with the grinding of lenses.[9]
  • 1686 – Kort onderwijs aengaende het gebruijck der horologiën tot het vinden der lenghten van Oost en West (in Old Dutch), instructions on how to use clocks to establish the longitude at sea.[181]
  • 1690 – Traité de la Lumière, dealing with the nature of light propagation.[25]
  • 1690 – Discours de la Cause de la Pesanteur (Discourse about gravity), supplement.[44]
  • 1691 – Lettre Touchant le Cycle Harmonique, short tract concerning the 31-tone system.[39]
  • 1698 – Cosmotheoros, deals with the solar system, cosmology, and extraterrestrial life.[162]
  • 1703 – Opuscula Posthuma including:[44]
    • De Motu Corporum ex Percussione (Concerning the motions of colliding bodies), contains the first correct laws for collision, dating from 1656.
    • Descriptio Automati Planetarii, provides a description and design of a planetarium.
  • 1724 – Novus Cyclus Harmonicus, a treatise on music published in Leiden after Huygens's death.[39]
  • 1728 – Christiani Hugenii Zuilichemii, dum viveret Zelhemii Toparchae, Opuscula Posthuma (alternate title: Opera Reliqua), includes works in optics and physics.[180]
  • 1888–1950 – Huygens, Christiaan. Oeuvres complètes. Complete works, 22 volumes. Editors D. Bierens de Haan (1–5), J. Bosscha (6–10), D.J. Korteweg (11–15), A.A. Nijland (15), J.A. Vollgraf (16–22). The Hague:[177]
    • Tome I: Correspondance 1638–1656 (1888).
    • Tome II: Correspondance 1657–1659 (1889).
    • Tome III: Correspondance 1660–1661 (1890).
    • Tome IV: Correspondance 1662–1663 (1891).
    • Tome V: Correspondance 1664–1665 (1893).
    • Tome VI: Correspondance 1666–1669 (1895).
    • Tome VII: Correspondance 1670–1675 (1897).
    • Tome VIII: Correspondance 1676–1684 (1899).
    • Tome IX: Correspondance 1685–1690 (1901).
    • Tome X: Correspondance 1691–1695 (1905).
    • Tome XI: Travaux mathématiques 1645–1651 (1908).
    • Tome XII: Travaux mathématiques pures 1652–1656 (1910).
    • Tome XIII, Fasc. I: Dioptrique 1653, 1666 (1916).
    • Tome XIII, Fasc. II: Dioptrique 1685–1692 (1916).
    • Tome XIV: Calcul des probabilités. Travaux de mathématiques pures 1655–1666 (1920).
    • Tome XV: Observations astronomiques. Système de Saturne. Travaux astronomiques 1658–1666 (1925).
    • Tome XVI: Mécanique jusqu’à 1666. Percussion. Question de l'existence et de la perceptibilité du mouvement absolu. Force centrifuge (1929).
    • Tome XVII: L’horloge à pendule de 1651 à 1666. Travaux divers de physique, de mécanique et de technique de 1650 à 1666. Traité des couronnes et des parhélies (1662 ou 1663) (1932).
    • Tome XVIII: L'horloge à pendule ou à balancier de 1666 à 1695. Anecdota (1934).
    • Tome XIX: Mécanique théorique et physique de 1666 à 1695. Huygens à l'Académie royale des sciences (1937).
    • Tome XX: Musique et mathématique. Musique. Mathématiques de 1666 à 1695 (1940).
    • Tome XXI: Cosmologie (1944).
    • Tome XXII: Supplément à la correspondance. Varia. Biographie de Chr. Huygens. Catalogue de la vente des livres de Chr. Huygens (1950).

See also

References

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  180. ^ a b Yoeder, Joella (1991). "Christiaan Huygens' Great Treasure" (PDF). Tractrix. 3: 1–13. (PDF) from the original on 13 April 2018. Retrieved 12 April 2018.
  181. ^ "Christiaan Huygens, Oeuvres complètes. Tome XXII. Supplément à la correspondance" (in Dutch). Digitale Bibliotheek Voor de Nederlandse Lettern. from the original on 13 April 2018. Retrieved 12 April 2018.

Further reading

  • Andriesse, C.D. (2005). Huygens: The Man Behind the Principle. Foreword by Sally Miedema. Cambridge University Press.
  • Bell, A. E. (1947). Christian Huygens and the Development of Science in the Seventeenth Century
  • Boyer, C.B. (1968). A History of Mathematics, New York.
  • Dijksterhuis, E. J. (1961). The Mechanization of the World Picture: Pythagoras to Newton
  • Hooijmaijers, H. (2005). Telling time – Devices for time measurement in Museum Boerhaave – A Descriptive Catalogue, Leiden, Museum Boerhaave.
  • Struik, D.J. (1948). A Concise History of Mathematics
  • Van den Ende, H. et al. (2004). Huygens's Legacy, The golden age of the pendulum clock, Fromanteel Ltd, Castle Town, Isle of Man.
  • Yoder, J G. (2005). "Book on the pendulum clock" in Ivor Grattan-Guinness, ed., Landmark Writings in Western Mathematics. Elsevier: 33–45.

External links

Primary sources, translations

  • Works by Christiaan Huygens at Project Gutenberg:
    • C. Huygens (translated by Silvanus P. Thompson, 1912), Treatise on Light; Errata.
  • Works by or about Christiaan Huygens at Internet Archive
  • Works by Christiaan Huygens at LibriVox (public domain audiobooks)  
  • Clerke, Agnes Mary (1911). "Huygens, Christiaan" . Encyclopædia Britannica. Vol. 14 (11th ed.). pp. 21–22.
  • Correspondence of Christiaan Huygens at Early Modern Letters Online
  • De Ratiociniis in Ludo Aleae or The Value of all Chances in Games of Fortune, 1657 Christiaan Huygens's book on probability theory. An English translation published in 1714. Text pdf file.
  • Horologium oscillatorium (German translation, pub. 1913) or Horologium oscillatorium (English translation by Ian Bruce) on the pendulum clock
  • ΚΟΣΜΟΘΕΩΡΟΣ (Cosmotheoros). (English translation of Latin, pub. 1698; subtitled The celestial worlds discover'd: or, Conjectures concerning the inhabitants, plants and productions of the worlds in the planets.)
  • C. Huygens (translated by Silvanus P. Thompson), Traité de la lumière or Treatise on light, London: Macmillan, 1912, archive.org/details/treatiseonlight031310mbp; New York: Dover, 1962; Project Gutenberg, 2005, gutenberg.org/ebooks/14725; Errata
  • Systema Saturnium 1659 text a digital edition of Smithsonian Libraries
  • On Centrifugal Force (1703)
  • Huygens's work at WorldCat
  • The Correspondence of Christiaan Huygens in EMLO
  • Christiaan Huygens biography and achievements
  • Portraits of Christiaan Huygens
  • Huygens's books, in digital facsimile from the Linda Hall Library:
    • (1659) Systema Saturnium (Latin)
    • (1684) Astroscopia compendiaria (Latin)
    • (1690) Traité de la lumiére (French)
    • (1698) ΚΟΣΜΟΘΕΩΡΟΣ, sive De terris cœlestibus (Latin)

Museums

  • in Voorburg, Netherlands, where Huygens lived and worked.
  • Huygens Clocks exhibition from the Science Museum, London
  • Online exhibition on Huygens in Leiden University Library (in Dutch)

Other

christiaan, huygens, ocean, liner, lord, zeelhem, gənz, ɔɪ, gənz, dutch, ˈkrɪstijaːn, ˈɦœyɣə, listen, also, spelled, huyghens, latin, hugenius, april, 1629, july, 1695, dutch, mathematician, physicist, engineer, astronomer, inventor, regarded, figure, scientif. For the ocean liner see MS Christiaan Huygens Christiaan Huygens Lord of Zeelhem FRS ˈ h aɪ ɡ en z HY genz 4 US ˈ h ɔɪ ɡ en z HOY genz 5 Dutch ˈkrɪstijaːn ˈɦœyɣe n s listen also spelled Huyghens Latin Hugenius 14 April 1629 8 July 1695 was a Dutch mathematician physicist engineer astronomer and inventor who is regarded as a key figure in the Scientific Revolution 6 7 In physics Huygens made seminal contributions to optics and mechanics while as an astronomer he studied the rings of Saturn and discovered its largest moon Titan As an engineer and inventor he improved the design of telescopes and invented the pendulum clock the most accurate timekeeper for almost 300 years A talented mathematician and physicist his works contain the first idealization of a physical problem by a set of mathematical parameters 8 and the first mathematical and mechanistic explanation of an unobservable physical phenomenon 9 Christiaan HuygensFRSHuygens by Caspar Netscher 1671 Museum Boerhaave Leiden 1 Born 1629 04 14 14 April 1629The Hague Dutch RepublicDied8 July 1695 1695 07 08 aged 66 The Hague Dutch RepublicAlma materUniversity of LeidenUniversity of AngersKnown forList Aerial telescopeBalance springBirefringenceCentrifugal forceCentripetal forceCollision formulaeDiscovery of TitanExplanation of Saturn s ringsEvoluteGambler s ruinHuygens s engineHuygenian eyepieceHuygens Fresnel principleHuygens s lemniscateHuygens Steiner theoremHuygens s tritoneInvoluteInjection lockingRepetition pitchMagic lanternPendulum clockProblem of pointsTautochrone curveTractrixWave theory31 equal temperament musical tuningScientific careerFieldsMathematicsPhysicsAstronomyMechanicsHorologyInstitutionsRoyal Society of LondonFrench Academy of SciencesAcademic advisorsFrans van SchootenInfluencesGalileo GalileiRene DescartesInfluencedGottfried Wilhelm LeibnizIsaac Newton 2 3 SignatureHuygens first identified the correct laws of elastic collision in his work De Motu Corporum ex Percussione completed in 1656 but published posthumously in 1703 10 In 1659 Huygens derived geometrically the formula in classical mechanics for the centrifugal force in his work De vi Centrifuga a decade before Newton 11 In optics he is best known for his wave theory of light which he described in his Traite de la Lumiere 1690 His theory of light was initially rejected in favour of Newton s corpuscular theory of light until Augustin Jean Fresnel adopted Huygens s principle to give a complete explanation of the rectilinear propagation and diffraction effects of light in 1821 Today this principle is known as the Huygens Fresnel principle Huygens invented the pendulum clock in 1657 which he patented the same year His horological research resulted in an extensive analysis of the pendulum in Horologium Oscillatorium 1673 regarded as one of the most important 17th century works on mechanics 8 While it contains descriptions of clock designs most of the book is an analysis of pendular motion and a theory of curves In 1655 Huygens began grinding lenses with his brother Constantijn to build refracting telescopes He discovered Saturn s biggest moon Titan and was the first to explain Saturn s strange appearance as due to a thin flat ring nowhere touching and inclined to the ecliptic 12 In 1662 Huygens developed what is now called the Huygenian eyepiece a telescope with two lenses to diminish the amount of dispersion 13 As a mathematician Huygens developed the theory of evolutes and wrote on games of chance and the problem of points in Van Rekeningh in Spelen van Gluck which Frans van Schooten translated and published as De Ratiociniis in Ludo Aleae 1657 14 The use of expectation values by Huygens and others would later inspire Jacob Bernoulli s work on probability theory 15 16 Contents 1 Biography 1 1 Student years 1 2 Early correspondence 1 3 Scientific debut 1 4 France 1 5 Final years 2 Mathematics 2 1 Published works 2 1 1 Theoremata de Quadratura 2 1 2 De Circuli Magnitudine Inventa 2 1 3 De Ratiociniis in Ludo Aleae 2 2 Unpublished work 3 Natural philosophy 3 1 Laws of motion impact and gravitation 3 2 Horology 3 2 1 Pendulum clock 3 2 2 Horologium Oscillatorium 3 2 3 Balance spring watch 3 3 Optics 3 3 1 Dioptrics 3 3 2 Lenses 3 3 3 Traite de la Lumiere 3 4 Astronomy 3 4 1 Systema Saturnium 3 4 2 Planetarium 3 4 3 Cosmotheoros 4 Legacy 4 1 Mathematics and physics 4 1 1 Later influence 4 2 Portraits 4 3 Commemorations 5 Works 6 See also 7 References 7 1 Further reading 8 External links 8 1 Primary sources translations 8 2 Museums 8 3 OtherBiography Edit Portrait of Constantijn centre and his five children Christiaan top right Mauritshuis The Hague Christiaan Huygens was born on 14 April 1629 in The Hague into a rich and influential Dutch family 17 18 the second son of Constantijn Huygens Christiaan was named after his paternal grandfather 19 20 His mother Suzanna van Baerle died shortly after giving birth to Huygens s sister 21 The couple had five children Constantijn 1628 Christiaan 1629 Lodewijk 1631 Philips 1632 and Suzanna 1637 22 Constantijn Huygens was a diplomat and advisor to the House of Orange in addition to being a poet and a musician He corresponded widely with intellectuals across Europe his friends included Galileo Galilei Marin Mersenne and Rene Descartes 23 Christiaan was educated at home until the age of sixteen and from a young age liked to play with miniatures of mills and other machines From his father he received a liberal education studying languages music history geography mathematics logic and rhetoric alongside dancing fencing and horse riding 19 22 In 1644 Huygens had as his mathematical tutor Jan Jansz Stampioen who assigned the 15 year old a demanding reading list on contemporary science 24 Descartes was later impressed by his skills in geometry as was Mersenne who christened him the new Archimedes 25 18 26 Student years Edit At sixteen years of age Constantijn sent Huygens to study law and mathematics at Leiden University where he studied from May 1645 to March 1647 19 Frans van Schooten was an academic at Leiden from 1646 and became a private tutor to Huygens and his elder brother Constantijn Jr replacing Stampioen on the advice of Descartes 27 28 Van Schooten brought Huygens s mathematical education up to date introducing him to the work of Viete Descartes and Fermat 29 After two years starting in March 1647 Huygens continued his studies at the newly founded Orange College in Breda where his father was a curator Constantijn Huygens was closely involved in the new College which lasted only to 1669 the rector was Andre Rivet 30 Christiaan Huygens lived at the home of the jurist Johann Henryk Dauber while attending college and had mathematics classes with the English lecturer John Pell His time in Breda ended around the time when his brother Lodewijk who was enrolled at the school duelled with another student 7 31 Huygens left Breda after completing his studies in August 1649 and had a stint as a diplomat on a mission with Henry Duke of Nassau 19 It took him to Bentheim then Flensburg He took off for Denmark visited Copenhagen and Helsingor and hoped to cross the Oresund to visit Descartes in Stockholm It was not to be 32 Although his father Constantijn had wished his son Christiaan to be a diplomat circumstances kept him from becoming so The First Stadtholderless Period that began in 1650 meant that the House of Orange was no longer in power removing Constantijn s influence Further he realized that his son had no interest in such a career 33 Early correspondence Edit Picture of a hanging chain catenary in a manuscript of Huygens Huygens generally wrote in French or Latin 34 In 1646 while still a college student at Leiden he began a correspondence with his father s friend Marin Mersenne who died soon afterwards in 1648 19 Mersenne wrote to Constantijn on his son s talent for mathematics and flatteringly compared him to Archimedes on 3 January 1647 35 The letters show Huygens s early interest in mathematics In October 1646 there is the suspension bridge and the demonstration that a hanging chain is not a parabola as Galileo thought 36 Huygens would later label that curve the catenaria catenary in 1690 while corresponding with Gottfried Leibniz 37 In the next two years 1647 48 Huygens s letters to Mersenne covered various topics including a mathematical proof of the law of free fall the claim by Gregoire de Saint Vincent of circle quadrature which Huygens showed to be wrong the rectification of the ellipse projectiles and the vibrating string 38 Some of Mersenne s concerns at the time such as the cycloid he sent Huygens Torricelli s treatise on the curve the centre of oscillation and the gravitational constant were matters Huygens only took seriously towards the end of the 17th century 8 Mersenne had also written on musical theory Huygens preferred meantone temperament he innovated in 31 equal temperament which was not itself a new idea but known to Francisco de Salinas using logarithms to investigate it further and show its close relation to the meantone system 39 In 1654 Huygens returned to his father s house in The Hague and was able to devote himself entirely to research 19 The family had another house not far away at Hofwijck and he spent time there during the summer Despite being very active his scholarly life did not allow him to escape bouts of depression 40 Subsequently Huygens developed a broad range of correspondents though picking up the threads after 1648 was hampered by the five year Fronde in France Visiting Paris in 1655 Huygens called on Ismael Boulliau to introduce himself who took him to see Claude Mylon 41 The Parisian group of savants that had gathered around Mersenne held together into the 1650s and Mylon who had assumed the secretarial role took some trouble to keep Huygens in touch 42 Through Pierre de Carcavi Huygens corresponded in 1656 with Pierre de Fermat whom he admired greatly though this side of idolatry The experience was bittersweet and somewhat puzzling since it became clear that Fermat had dropped out of the research mainstream and his priority claims could probably not be made good in some cases Besides Huygens was looking by then to apply mathematics to physics while Fermat s concerns ran to purer topics 43 Scientific debut Edit Christiaan Huygens relief by Jean Jacques Clerion c 1670 Like some of his contemporaries Huygens was often slow to commit his results and discoveries to print preferring to disseminate his work through letters instead 44 In his early days his mentor Frans van Schooten provided technical feedback and was cautious for the sake of his reputation 45 Between 1651 and 1657 Huygens published a number of works that showed his talent for mathematics and his mastery of classical and analytical geometry increasing his reach and reputation among mathematicians 35 Around the same time Huygens began to question Descartes s laws of collision which were largely wrong deriving the correct laws algebraically and later by way of geometry 46 He showed that for any system of bodies the centre of gravity of the system remains the same in velocity and direction which Huygens called the conservation of quantity of movement While others at the time were studying impact Huygens s theory of collisions was more general 7 These results were known through correspondence and in a short article in Journal des Scavans but would remain largely unpublished until the publication of De Motu Corporum ex Percussione Concerning the motion of colliding bodies in 1703 46 In addition to his work on mechanics Huygens made important scientific discoveries he was the first to identify one of Saturn s moons Titan in 1655 and invented the pendulum clock in 1657 both these discoveries brought him fame across Europe 19 On 3 May 1661 Huygens together with astronomer Thomas Streete and Richard Reeve observed the planet Mercury transit over the Sun using Reeve s telescope in London 47 Streete then debated the published record of Hevelius a controversy mediated by Henry Oldenburg 48 Huygens passed to Hevelius a manuscript of Jeremiah Horrocks on the transit of Venus in 1639 printed for the first time in 1662 49 In that same year Sir Robert Moray sent Huygens John Graunt s life table and shortly after Huygens and his brother Lodewijk dabbled on life expectancy 44 50 Huygens eventually created the first graph of a continuous distribution function under the assumption of a uniform death rate and used it to solve problems in joint annuities 51 Contemporaneously Huygens who played the harpsichord took an interest in Simon Stevin s theories on music however he showed very little concern to publish his theories on consonance some of which were lost for centuries 52 53 For his contributions to science the Royal Society of London elected Huygens a Fellow in 1665 making him its first foreign member when he was just 36 years old 54 France Edit Huygens right of centre from L etablissement de l Academie des Sciences et fondation de l observatoire 1666 by Henri Testelin c 1675 The Montmor Academy started in the mid 1650s was the form the old Mersenne circle took after his death 55 Huygens took part in its debates and supported its dissident faction favouring experimental demonstration over amateurish attitudes 56 During 1663 he made what was his third visit to Paris when the Montmor Academy closed down the next year Huygens took the chance to advocate a more Baconian program in science Two years later in 1666 he moved to Paris on an invitation to fill a leadership position at King Louis XIV s new French Academie des sciences 57 While at the Academie in Paris Huygens had an important patron and correspondent in Jean Baptiste Colbert First Minister to Louis XIV 58 However his relationship with the French Academie was not always easy and in 1670 Huygens seriously ill chose Francis Vernon to carry out a donation of his papers to the Royal Society in London should he die 59 The aftermath of the Franco Dutch War 1672 78 and particularly England s role in it may have damaged his later relationship with the Royal Society 60 Robert Hooke as a Royal Society representative lacked the finesse to handle the situation in 1673 61 The physicist and inventor Denis Papin was assistant to Huygens from 1671 62 One of their projects which did not bear fruit directly was the gunpowder engine 63 Papin moved to England in 1678 to continue work in this area 64 Also in Paris Huygens made further astronomical observations using the observatory recently completed in 1672 He introduced Nicolaas Hartsoeker to French scientists such as Nicolas Malebranche and Giovanni Cassini in 1678 7 65 Huygens met the young diplomat Leibniz while visiting Paris in 1672 on a vain mission to meet the French Foreign Minister Arnauld de Pomponne At this time Leibniz was working on a calculating machine and he moved on to London in early 1673 with diplomats from Mainz From March 1673 Leibniz was tutored in mathematics by Huygens who taught him analytical geometry 66 An extensive correspondence ensued over the years in which Huygens showed at first reluctance to accept the advantages of Leibniz s infinitesimal calculus 67 Final years Edit Huygens moved back to The Hague in 1681 after suffering another bout of serious depressive illness In 1684 he published Astroscopia Compendiaria on his new tubeless aerial telescope He attempted to return to France in 1685 but the revocation of the Edict of Nantes precluded this move His father died in 1687 and he inherited Hofwijck which he made his home the following year 33 On his third visit to England Huygens met Isaac Newton in person on 12 June 1689 They spoke about Iceland spar and subsequently corresponded about resisted motion 68 Huygens returned to mathematical topics in his last years and observed the acoustical phenomenon now known as flanging in 1693 69 Two years later on 8 July 1695 Huygens died in The Hague and was buried like his father before him in an unmarked grave at the Grote Kerk 70 Huygens never married 71 Mathematics EditHuygens first became internationally known for his work in mathematics publishing a number of important results that drew the attention of many European geometers 72 Huygens s preferred method in his published works was that of Archimedes though he used Descartes s analytic geometry and Fermat s infinitesimal techniques more extensively in his private notebooks 19 Published works Edit Theoremata de Quadratura Edit Huygens s first publication was in the field of quadrature Huygens s first publication was Theoremata de Quadratura Hyperboles Ellipsis et Circuli Theorems on the quadrature of the hyperbola ellipse and circle published by the Elzeviers in Leiden in 1651 44 The first part of the work contained theorems for computing the areas of hyperbolas ellipses and circles that paralleled Archimedes s work on conic sections particularly his Quadrature of the Parabola 35 The second part included a refutation to Gregoire de Saint Vincent s claims on circle quadrature which he had discussed with Mersenne earlier Huygens demonstrated that the centre of gravity of a segment of any hyperbola ellipse or circle was directly related to the area of that segment He was then able to show the relationships between triangles inscribed in conic sections and the centre of gravity for those sections By generalizing these theorems to all conic sections Huygens extended classical methods to generate new results 19 Quadrature was a live issue in the 1650s and through Mylon Huygens intervened in the discussion of the mathematics of Thomas Hobbes Persisting in trying to explain the errors Hobbes had fallen into he made an international reputation 73 De Circuli Magnitudine Inventa Edit Huygens s next publication was De Circuli Magnitudine Inventa New findings in the measurement of the circle published in 1654 In this work Huygens was able to narrow the gap between the circumscribed and inscribed polygons found in Archimedes s Measurement of the Circle showing that the ratio of the circumference to its diameter or p must lie in the first third of that interval 44 Using a technique equivalent to Richardson extrapolation 74 Huygens was able to shorten the inequalities used in Archimedes s method in this case by using the centre of the gravity of a segment of a parabola he was able to approximate the centre of gravity of a segment of a circle resulting in a faster and accurate approximation of the circle quadrature 75 From these theorems Huygens obtained two set of values for p the first between 3 1415926 and 3 1415927 and the second between 3 1415926538 and 3 1415926533 76 Huygens also showed that in the case of the hyperbola the same approximation with parabolic segments produces a quick and simple method to calculate logarithms 77 He appended a collection of solutions to classical problems at the end of the work under the title Illustrium Quorundam Problematum Constructiones Construction of some illustrious problems 44 De Ratiociniis in Ludo Aleae Edit Huygens became interested in games of chance after he visited Paris in 1655 and encountered the work of Fermat Blaise Pascal and Girard Desargues years earlier 78 He eventually published what was at the time the most coherent presentation of a mathematical approach to games of chance in De Ratiociniis in Ludo Aleae On reasoning in games of chance 79 80 Frans van Schooten translated the original Dutch manuscript into Latin and published it in his Exercitationum Mathematicarum 1657 81 14 The work contains early game theoretic ideas and deals in particular with the problem of points 16 14 Huygens took from Pascal the concepts of a fair game and equitable contract i e equal division when the chances are equal and extended the argument to set up a non standard theory of expected values 82 His success in applying algebra to the realm of chance which hitherto seemed inaccessible to mathematicians demonstrated the power of combining Euclidean synthetic proofs with the symbolic reasoning found in the works of Viete and Descartes 83 Huygens included five challenging problems at the end of the book that became the standard test for anyone wishing to display their mathematical skill in games of chance for the next sixty years 84 People who worked on these problems included Abraham de Moivre Jacob Bernoulli Johannes Hudde Baruch Spinoza and Leibniz Unpublished work Edit Hofwijck Huygens s summer home now a museum Huygens had earlier completed a manuscript in the manner of Archimedes s On Floating Bodies entitled De Iis quae Liquido Supernatant About parts floating above liquids It was written around 1650 and was made up of three books Although he sent the completed work to Frans van Schooten for feedback in the end Huygens chose not to publish it and at one point suggested it be burned 35 85 Some of the results found here were not rediscovered until the eighteenth and nineteenth centuries 10 Huygens first re derives Archimedes s results for the stability of the sphere and the paraboloid by a clever application of Torricelli s principle i e that bodies in a system move only if their centre of gravity descends 86 He then proves the general theorem that for a floating body in equilibrium the distance between its centre of gravity and its submerged portion its at a minimum 10 Huygens uses this theorem to arrive at original solutions for the stability of floating cones parallelepipeds and cylinders in some cases through a full cycle of rotation 87 His approach was thus equivalent to the principle of virtual work Huygens was also the first to recognize that for homogeneous solids their specific weight and their aspect ratio are the essentials parameters of hydrostatic stability 88 89 Natural philosophy EditHuygens was the leading European natural philosopher between Descartes and Newton 19 90 However unlike many of his contemporaries Huygens had no taste for grand theoretical or philosophical systems and generally avoided dealing with metaphysical issues if pressed he adhered to the Cartesian and mechanical philosophy of his time 9 35 Instead Huygens excelled in extending the work of his predecessors such as Galileo to derive solutions to unsolved physical problems that were amenable to mathematical analysis In particular he sought explanations that relied on contact between bodies and avoided action at a distance 19 91 In common with Robert Boyle and Jacques Rohault Huygens advocated an experimentally oriented corpuscular mechanical natural philosophy during his Paris years This approach was sometimes labelled Baconian without being inductivist or identifying with the views of Francis Bacon in a simple minded way 92 After his first visit to England in 1661 and attending a meeting at Gresham College where he learned directly about Boyle s air pump experiments Huygens spent time in late 1661 and early 1662 replicating the work It proved a long process that brought to the surface both an experimental issue anomalous suspension and a theoretical issue horror vacui and which ended in July 1663 as he became a Fellow of the Royal Society While the replication of results of Boyle s experiments with the air pump trailed off messily Huygens came to accept Boyle s view of the void against the Cartesian denial of it 93 94 Newton s influence on John Locke was mediated by Huygens who assured Locke that Newton s mathematics was sound leading to Locke s acceptance of a corpuscular mechanical physics 95 Laws of motion impact and gravitation Edit A boating metaphor as a way to think about relative motion simplifying the theory of colliding bodies from Huygens s Oeuvres Completes The general approach of the mechanical philosophers was to postulate theories of the kind now called contact action Huygens adopted this method but not without seeing its difficulties and failures 96 Leibniz his student in Paris later abandoned the theory 97 Seeing the universe this way made the theory of collisions central to physics Matter in motion made up the universe and only explanations in those terms could be truly intelligible While Huygens was influenced by the Cartesian approach he was less doctrinaire 98 He studied elastic collisions in the 1650s but delayed publication for over a decade 29 Huygens concluded quite early that Descartes s laws for the elastic collision of two bodies must be wrong and he formulated the correct laws including the conservation of the product of mass times the square of the speed for hard bodies and the conservation of quantity of motion in one direction for all bodies 99 An important step was his recognition of the Galilean invariance of the problems 100 Huygens had worked out the laws of collision from 1652 to 1656 in a manuscript entitled De Motu Corporum ex Percussione though his results took many years to be circulated In 1661 he passed them on in person to William Brouncker and Christopher Wren in London 101 What Spinoza wrote to Henry Oldenburg about them in 1666 during the Second Anglo Dutch War was guarded 102 The war ended in 1667 and Huygens announced his results to the Royal Society in 1668 He later published them in the Journal des Scavans in 1669 29 In 1659 Huygens found the constant of gravitational acceleration and stated what is now known as the second of Newton s laws of motion in quadratic form 103 He derived geometrically the now standard formula for the centrifugal force exerted on an object when viewed in a rotating frame of reference for instance when driving around a curve In modern notation F c m w 2 r displaystyle F c m w 2 r with m the mass of the object w the angular velocity and r the radius 10 Huygens collected his results in a treatise under the title De vi Centrifuga unpublished until 1703 where the kinematics of free fall were used to produce the first generalized conception of force prior to Newton 104 The general idea for the centrifugal force however was published in 1673 and was a significant step in studying orbits in astronomy It enabled the transition from Kepler s third law of planetary motion to the inverse square law of gravitation 105 Yet the interpretation of Newton s work on gravitation by Huygens differed from that of Newtonians such as Roger Cotes he did not insist on the a priori attitude of Descartes but neither would he accept aspects of gravitational attractions that were not attributable in principle to contact between particles 106 The approach used by Huygens also missed some central notions of mathematical physics which were not lost on others In his work on pendulums Huygens came very close to the theory of simple harmonic motion the topic however was covered fully for the first time by Newton in Book II of the Principia Mathematica 1687 107 In 1678 Leibniz picked out of Huygens s work on collisions the idea of conservation law that Huygens had left implicit 108 Horology Edit Pendulum clock Edit Spring driven pendulum clock designed by Huygens and built by Salomon Coster 1657 109 with a copy of the Horologium Oscillatorium 1673 110 at Museum Boerhaave Leiden In 1657 inspired by earlier research into pendulums as regulating mechanisms Huygens invented the pendulum clock which was a breakthrough in timekeeping and became the most accurate timekeeper for almost 300 years until the 1930s 111 The pendulum clock was much more accurate than the existing verge and foliot clocks and was immediately popular quickly spreading over Europe He contracted the construction of his clock designs to Salomon Coster in The Hague who built the clock However Huygens did not make much money from his invention Pierre Seguier refused him any French rights while Simon Douw in Rotterdam and Ahasuerus Fromanteel in London copied his design in 1658 112 The oldest known Huygens style pendulum clock is dated 1657 and can be seen at the Museum Boerhaave in Leiden 113 114 115 116 Part of the incentive for inventing the pendulum clock was to create an accurate marine chronometer that could be used to find longitude by celestial navigation during sea voyages However the clock proved unsuccessful as a marine timekeeper because the rocking motion of the ship disturbed the motion of the pendulum In 1660 Lodewijk Huygens made a trial on a voyage to Spain and reported that heavy weather made the clock useless Alexander Bruce elbowed into the field in 1662 and Huygens called in Sir Robert Moray and the Royal Society to mediate and preserve some of his rights 117 113 Trials continued into the 1660s the best news coming from a Royal Navy captain Robert Holmes operating against the Dutch possessions in 1664 118 Lisa Jardine doubts that Holmes reported the results of the trial accurately as Samuel Pepys expressed his doubts at the time 119 A trial for the French Academy on an expedition to Cayenne ended badly Jean Richer suggested correction for the figure of the Earth By the time of the Dutch East India Company expedition of 1686 to the Cape of Good Hope Huygens was able to supply the correction retrospectively 120 Horologium Oscillatorium Edit Diagram showing the evolute of a curve Sixteen years after the invention of the pendulum clock in 1673 Huygens published his major work on horology entitled Horologium Oscillatorium Sive de Motu Pendulorum ad Horologia Aptato Demonstrationes Geometricae The Pendulum Clock or Geometrical demonstrations concerning the motion of pendula as applied to clocks It is the first modern work on mechanics where a physical problem is idealized by a set of parameters then analysed mathematically 8 Huygens s motivation came from the observation made by Mersenne and others that pendulums are not quite isochronous their period depends on their width of swing with wide swings taking slightly longer than narrow swings 121 He tackled this problem by finding the curve down which a mass will slide under the influence of gravity in the same amount of time regardless of its starting point the so called tautochrone problem By geometrical methods which anticipated the calculus Huygens showed it to be a cycloid rather than the circular arc of a pendulum s bob and therefore that pendulums needed to move on a cycloid path in order to be isochronous The mathematics necessary to solve this problem led Huygens to develop his theory of evolutes which he presented in Part III of his Horologium Oscillatorium 8 122 He also solved a problem posed by Mersenne earlier how to calculate the period of a pendulum made of an arbitrarily shaped swinging rigid body This involved discovering the centre of oscillation and its reciprocal relationship with the pivot point In the same work he analysed the conical pendulum consisting of a weight on a cord moving in a circle using the concept of centrifugal force 8 123 Huygens was the first to derive the formula for the period of an ideal mathematical pendulum with mass less rod or cord and length much longer than its swing in modern notation T 2 p l g displaystyle T 2 pi sqrt frac l g with T the period l the length of the pendulum and g the gravitational acceleration By his study of the oscillation period of compound pendulums Huygens made pivotal contributions to the development of the concept of moment of inertia 124 Huygens also observed coupled oscillations two of his pendulum clocks mounted next to each other on the same support often became synchronized swinging in opposite directions He reported the results by letter to the Royal Society and it is referred to as an odd kind of sympathy in the Society s minutes 125 This concept is now known as entrainment 126 Balance spring watch Edit Drawing of a balance spring invented by Huygens In 1675 while investigating the oscillating properties of the cycloid Huygens was able to transform a cycloidal pendulum into a vibrating spring through a combination of geometry and higher mathematics 127 In the same year Huygens designed a spiral balance spring and patented a pocket watch These watches are notable for lacking a fusee for equalizing the mainspring torque The implication is that Huygens thought his spiral spring would isochronize the balance in the same way that cycloid shaped suspension curbs on his clocks would isochronize the pendulum 128 He later used spiral springs in more conventional watches made for him by Thuret in Paris Such springs are essential in modern watches with a detached lever escapement because they can be adjusted for isochronism Watches in Huygens s time however employed the very ineffective verge escapement which interfered with the isochronal properties of any form of balance spring spiral or otherwise 129 Huygens s design came around the same time as though independently of Robert Hooke s Controversy over the priority of the balance spring persisted for centuries In February 2006 a long lost copy of Hooke s handwritten notes from several decades of Royal Society meetings was discovered in a cupboard in Hampshire England presumably tipping the evidence in Hooke s favour 130 131 Optics Edit Dioptrics Edit Huygens s aerial telescope from Astroscopia Compendiaria 1684 Huygens had a long term interest in the study of light refraction and lenses or dioptrics 132 From 1652 date the first drafts of a Latin treatise on the theory of dioptrics known as the Tractatus which contained a comprehensive and rigorous theory of the telescope Huygens was one of the few to raise theoretical questions regarding the properties and working of the telescope and almost the only one to direct his mathematical proficiency towards the actual instruments used in astronomy 133 Huygens repeatedly announced its publication to his colleagues but ultimately postponed it in favor of a much more comprehensive treatment now under the name of the Dioptrica 25 It consisted of three parts The first part focused on the general principles of refraction the second dealt with spherical and chromatic aberration while the third covered all aspects of the construction of telescopes and microscopes In contrast to Descartes dioptrics which treated only ideal elliptical and hyperbolical lenses Huygens dealt exclusively with spherical lenses which were the only kind that could really be made and incorporated in devices such as microscopes and telescopes 134 Huygens also worked out practical ways to minimize the effects of spherical and chromatic aberration such as long focal distances for the objective of a telescope internal stops to reduce the aperture and a new kind of ocular known as the Huygenian eyepiece 134 The Dioptrica was never published in Huygens s lifetime and only appeared in press in 1703 when most of its contents were already familiar to the scientific world Lenses Edit Together with his brother Constantijn Huygens began grinding his own lenses in 1655 in an effort to improve telescopes 135 He designed in 1662 what is now called the Huygenian eyepiece a set of two planoconvex lenses used as a telescope ocular 136 137 Huygens s lenses were known to be of superb quality and polished consistently according to his specifications however his telescopes did not produce very sharp images leading some to speculate that he might have suffered from near sightedness 138 Lenses were also a common interest through which Huygens could meet socially in the 1660s with Spinoza who ground them professionally They had rather different outlooks on science Spinoza being the more committed Cartesian and some of their discussion survives in correspondence 139 He encountered the work of Antoni van Leeuwenhoek another lens grinder in the field of microscopy which interested his father 8 Huygens also investigated the use of lenses in projectors He is credited as the inventor of the magic lantern described in correspondence of 1659 140 There are others to whom such a lantern device has been attributed such as Giambattista della Porta and Cornelis Drebbel though Huygens s design used lens for better projection Athanasius Kircher has also been credited for that 141 Traite de la Lumiere Edit Refraction of a plane wave explained using Huygens s principle in Traite de la Lumiere 1690 Huygens is especially remembered in optics for his wave theory of light which he first communicated in 1678 to the Academie des sciences in Paris Originally a preliminary chapter of his Dioptrica Huygens s theory was published in 1690 under the title Traite de la Lumiere 142 Treatise on light and contains the first fully mathematized mechanistic explanation of an unobservable physical phenomenon i e light propagation 9 143 Huygens refers to Ignace Gaston Pardies whose manuscript on optics helped him on his wave theory 144 The challenge at the time was to explain geometrical optics as most physical optics phenomena such as diffraction had not been observed or appreciated as issues Huygens had experimented in 1672 with double refraction birefringence in the Iceland spar a calcite a phenomenon discovered in 1669 by Rasmus Bartholin At first he could not elucidate what he found but was later able to explain it using his wavefront theory and concept of evolutes 143 He also developed ideas on caustics 8 Huygens assumes that the speed of light is finite based on a report by Ole Christensen Romer in 1677 but which Huygens is presumed to have already believed 145 Huygens s theory posits light as radiating wavefronts with the common notion of light rays depicting propagation normal to those wavefronts Propagation of the wavefronts is then explained as the result of spherical waves being emitted at every point along the wave front known today as the Huygens Fresnel principle 146 It assumed an omnipresent ether with transmission through perfectly elastic particles a revision of the view of Descartes The nature of light was therefore a longitudinal wave 145 His theory of light was not widely accepted while Newton s rival corpuscular theory of light as found in his Opticks 1704 gained more support One strong objection to Huygens s theory was that longitudinal waves have only a single polarization which cannot explain the observed birefringence However Thomas Young s interference experiments in 1801 and Francois Arago s detection of the Poisson spot in 1819 could not be explained through Newton s or any other particle theory reviving Huygens s ideas and wave models Fresnel became aware of Huygens s work and in 1821 was able to explain birefringence as a result of light being not a longitudinal as had been assumed but actually a transverse wave 147 The thus named Huygens Fresnel principle was the basis for the advancement of physical optics explaining all aspects of light propagation until Maxwell s electromagnetic theory culminated in the development of quantum mechanics and the discovery of the photon 134 148 Astronomy Edit Systema Saturnium Edit Huygens s explanation for the aspects of Saturn Systema Saturnium 1659 In 1655 Huygens discovered the first of Saturn s moons Titan and observed and sketched the Orion Nebula using a refracting telescope with a 43x magnification of his own design 13 12 Huygens succeeded in subdividing the nebula into different stars the brighter interior now bears the name of the Huygenian region in his honour and discovered several interstellar nebulae and some double stars 149 He was also the first to propose that the appearance of Saturn which have baffled astronomers was due to a thin flat ring nowhere touching and inclined to the ecliptic 150 More than three years later in 1659 Huygens published his theory and findings in Systema Saturnium It is considered the most important work on telescopic astronomy since Galileo s Sidereus Nuncius fifty years earlier 151 Much more than a report on Saturn Huygens provided measurements for the relative distances of the planets from the Sun introduced the concept of the micrometer and showed a method to measure angular diameters of planets which finally allowed the telescope to be used as an instrument to measure rather than just sighting astronomical objects 152 He was also the first to question the authority of Galileo in telescopic matters a sentiment that was to be common in the years following its publication In the same year Huygens was able to observe Syrtis Major a volcanic plain on Mars He used repeated observations of the movement of this feature over the course of a number of days to estimate the length of day on Mars which he did quite accurately to 24 1 2 hours This figure is only a few minutes off of the actual length of the Martian day of 24 hours 37 minutes 153 Planetarium Edit At the instigation of Jean Baptiste Colbert Huygens undertook the task of constructing a mechanical planetarium that could display all the planets and their moons then known circling around the Sun Huygens completed his design in 1680 and had his clockmaker Johannes van Ceulen built it the following year However Colbert passed away in the interim and Huygens never got to deliver his planetarium to the French Academy of Sciences as the new minister Francois Michel le Tellier decided not to renew Huygens s contract 154 155 In his design Huygens made an ingenious use of continued fractions to find the best rational approximations by which he could choose the gears with the correct number of teeth The ratio between two gears determined the orbital periods of two planets To move the planets around the Sun Huygens used a clock mechanism that could go forwards and backwards in time Huygens claimed his planetarium was more accurate that a similar device constructed by Ole Romer around the same time but his planetarium design was not published until after his death in the Opuscula Posthuma 1703 154 Cosmotheoros Edit Relative sizes of the Sun and planets in Cosmotheoros 1698 Shortly before his death in 1695 Huygens completed his most speculative work entitled Cosmotheoros At his direction it was to be published only posthumously by his brother which Constantijn Jr did in 1698 156 In this work Huygens speculated on the existence of extraterrestrial life which he imagined similar to that on Earth Such speculations were not uncommon at the time justified by Copernicanism or the plenitude principle but Huygens went into greater detail 157 However it did so without the benefit of understanding Newton s laws of gravitation or the fact that the atmospheres on other planets are composed of different gases 158 Cosmotheoros translated into English as The celestial worlds discover d has been seen as part of speculative fiction in the tradition of Francis Godwin John Wilkins and Cyrano de Bergerac Huygens s work was fundamentally utopian and owes some inspiration from the cosmography and planetary speculation of Peter Heylin 159 160 Huygens wrote that availability of water in liquid form was essential for life and that the properties of water must vary from planet to planet to suit the temperature range He took his observations of dark and bright spots on the surfaces of Mars and Jupiter to be evidence of water and ice on those planets 161 He argued that extraterrestrial life is neither confirmed nor denied by the Bible and questioned why God would create the other planets if they were not to serve a greater purpose than that of being admired from Earth Huygens postulated that the great distance between the planets signified that God had not intended for beings on one to know about the beings on the others and had not foreseen how much humans would advance in scientific knowledge 162 It was also in this book that Huygens published his estimates for the relative sizes of the solar system and his method for calculating stellar distances 7 He made a series of smaller holes in a screen facing the Sun until he estimated the light was of the same intensity as that of the star Sirius He then calculated that the angle of this hole was 1 27 664th the diameter of the Sun and thus it was about 30 000 times as far away on the incorrect assumption that Sirius is as luminous as the Sun The subject of photometry remained in its infancy until the time of Pierre Bouguer and Johann Heinrich Lambert 163 Legacy EditHuygens has been called the first theoretical physicist and a founder of modern mathematical physics 164 165 Although his influence was considerable during his lifetime it began to fade shortly after his death His skills as a geometer and mechanical insights elicited the admiration of many of his contemporaries including Newton Leibniz l Hopital and the Bernoullis 44 For his work in physics Huygens has been deemed one of the greatest scientists in the Scientific Revolution rivaled only by Newton in both depth of insight and the number of results obtained 6 166 Huygens also helped develop the institutional frameworks for scientific research on the European continent making him a leading actor in the establishment of modern science 167 Mathematics and physics Edit Portrait of Christiaan Huygens by Bernard Vaillant 1686 In mathematics Huygens mastered the methods of ancient Greek geometry particularly the work of Archimedes and was an adept user of the analytic geometry and infinitesimal techniques of Descartes Fermat and others 85 His mathematical style can be characterized as geometrical infinitesimal analysis of curves and of motion Drawing inspiration and imagery from mechanics it remained pure mathematics in form 72 Huygens brought this type of geometrical analysis to a close as more mathematicians turned away from classical geometry to the calculus for handling infinitesimals limit processes and motion 40 Huygens was moreover able to fully employ mathematics to answer questions of physics Often this entailed introducing a simple model for describing a complicated situation then analyzing it starting from simple arguments to their logical consequences developing the necessary mathematics along the way As he wrote at the end of a draft of De vi Centrifuga 35 Whatever you will have supposed not impossible either concerning gravity or motion or any other matter if then you prove something concerning the magnitude of a line surface or body it will be true as for instance Archimedes on the quadrature of the parabola where the tendency of heavy objects has been assumed to act through parallel lines Huygens favoured axiomatic presentations of his results which require rigorous methods of geometric demonstration although he allowed levels of uncertainty in the selection of primary axioms and hypotheses the proofs of theorems derived from these could never be in doubt 35 Huygens s style of publication exerted an influence in Newton s presentation of his own major works 168 169 Besides the application of mathematics to physics and physics to mathematics Huygens relied on mathematics as methodology particularly its ability to generate new knowledge about the world 170 Unlike Galileo who used mathematics primarily as rhetoric or synthesis Huygens consistently employed mathematics as a method of discovery and analysis and insisted that the reduction of the physical to the geometrical satisfy exacting standards of fit between the real and the ideal 121 In demanding such mathematical tractibility and precision Huygens set an example for eighteenth century scientists such as Johann Bernoulli Jean le Rond d Alembert and Charles Augustin de Coulomb 164 35 Although never intended for publication Huygens made use of algebraic expressions to represent physical entities in a handful of his manuscripts on collisions 46 This would make him one of the first to employ mathematical formulae to describe relationships in physics as it is done today 7 Huygens also came close to the modern idea of limit while working on his Dioptrica though he never used the notion outside geometrical optics 171 Later influence Edit Huygens s standing as the greatest scientist in Europe was eclipsed by Newton s at the end of the seventeenth century despite the fact that as Hugh Aldersey Williams notes Huygens s achievement exceeds that of Newton in some important respects 172 His very idiosyncratic style and reluctance to publish his work did much to diminish his influence in the aftermath of the Scientific Revolution as adherents of Leibniz calculus and Newton s physics took centre stage 40 85 Huygens s analyses of curves that satisfy certain physical properties such as the cycloid led to later studies of many other such curves like the caustic the brachistochrone the sail curve and the catenary 26 37 His application of mathematics to physics such as in his study of birefringence would inspire new developments in mathematical physics and rational mechanics in the following centuries albeit in the new language of the calculus 9 Additionally Huygens developed the oscillating timekeeping mechanisms the pendulum and the balance spring that have been used ever since in mechanical watches and clocks These were the first reliable timekeepers fit for scientific use e g it was possible for the first time to make accurate measurements of the inequality of the solar day which astronomers in the past could not do 8 121 His work on this area anticipated the union of applied mathematics with mechanical engineering in the centuries that followed 128 Portraits Edit During his lifetime Huygens and his father had a number of portraits commissioned These included 1639 Constantijn Huygens in the midst of his five children by Adriaen Hanneman painting with medallions Mauritshuis The Hague 173 1671 Portrait by Caspar Netscher Museum Boerhaave Leiden loan from Haags Historisch Museum 173 c 1675 Depiction of Huygens in Etablissement de l Academie des Sciences et fondation de l observatoire 1666 by Henri Testelin Colbert presents the members of the newly founded Academie des Sciences to king Louis XIV of France Musee National du Chateau et des Trianons de Versailles Versailles 174 1679 Medaillon portrait in relief by the French sculptor Jean Jacques Clerion 173 1686 Portrait in pastel by Bernard Vaillant Museum Hofwijck Voorburg 173 1684 to 1687 Engravings by G Edelinck after the painting by Caspar Netscher 173 1688 Portrait by Pierre Bourguignon painter Royal Netherlands Academy of Arts and Sciences Amsterdam 173 Commemorations Edit The European Space Agency spacecraft that landed on Titan Saturn s largest moon in 2005 was named after him 175 A number of monuments to Christiaan Huygens can be found across important cities in the Netherlands including Rotterdam Delft and Leiden Rotterdam Delft Leiden Haarlem VoorburgWorks Edit Title page of Oeuvres Completes ISource s 19 1650 De Iis Quae Liquido Supernatant About parts floating above liquids unpublished 176 1651 Theoremata de Quadratura Hyperboles Ellipsis et Circuli republished in Oeuvres Completes Tome XI 44 1651 Epistola qua diluuntur ea quibus E3etasis Exetasis Cyclometriae Gregori a Sto Vincentio impugnata fuit supplement 177 1654 De Circuli Magnitudine Inventa 35 1654 Illustrium Quorundam Problematum Constructiones supplement 177 1655 Horologium The clock short pamphlet on the pendulum clock 8 1656 De Saturni Luna Observatio Nova About the new observation of the moon of Saturn describes the discovery of Titan 178 1656 De Motu Corporum ex Percussione published posthumously in 1703 179 1657 De Ratiociniis in Ludo Aleae Van reeckening in spelen van geluck translated into Latin by Frans van Schooten 14 1659 Systema Saturnium System of Saturn 177 1659 De vi Centrifuga Concerning the centrifugal force published posthumously in 1703 180 1673 Horologium Oscillatorium Sive de Motu Pendulorum ad Horologia Aptato Demonstrationes Geometricae includes a theory of evolutes and designs of pendulum clocks dedicated to Louis XIV of France 122 1684 Astroscopia Compendiaria Tubi Optici Molimine Liberata Compound telescopes without a tube 44 1685 Memorien aengaende het slijpen van glasen tot verrekijckers dealing with the grinding of lenses 9 1686 Kort onderwijs aengaende het gebruijck der horologien tot het vinden der lenghten van Oost en West in Old Dutch instructions on how to use clocks to establish the longitude at sea 181 1690 Traite de la Lumiere dealing with the nature of light propagation 25 1690 Discours de la Cause de la Pesanteur Discourse about gravity supplement 44 1691 Lettre Touchant le Cycle Harmonique short tract concerning the 31 tone system 39 1698 Cosmotheoros deals with the solar system cosmology and extraterrestrial life 162 1703 Opuscula Posthuma including 44 De Motu Corporum ex Percussione Concerning the motions of colliding bodies contains the first correct laws for collision dating from 1656 Descriptio Automati Planetarii provides a description and design of a planetarium 1724 Novus Cyclus Harmonicus a treatise on music published in Leiden after Huygens s death 39 1728 Christiani Hugenii Zuilichemii dum viveret Zelhemii Toparchae Opuscula Posthuma alternate title Opera Reliqua includes works in optics and physics 180 1888 1950 Huygens Christiaan Oeuvres completes Complete works 22 volumes Editors D Bierens de Haan 1 5 J Bosscha 6 10 D J Korteweg 11 15 A A Nijland 15 J A Vollgraf 16 22 The Hague 177 Tome I Correspondance 1638 1656 1888 Tome II Correspondance 1657 1659 1889 Tome III Correspondance 1660 1661 1890 Tome IV Correspondance 1662 1663 1891 Tome V Correspondance 1664 1665 1893 Tome VI Correspondance 1666 1669 1895 Tome VII Correspondance 1670 1675 1897 Tome VIII Correspondance 1676 1684 1899 Tome IX Correspondance 1685 1690 1901 Tome X Correspondance 1691 1695 1905 Tome XI Travaux mathematiques 1645 1651 1908 Tome XII Travaux mathematiques pures 1652 1656 1910 Tome XIII Fasc I Dioptrique 1653 1666 1916 Tome XIII Fasc II Dioptrique 1685 1692 1916 Tome XIV Calcul des probabilites Travaux de mathematiques pures 1655 1666 1920 Tome XV Observations astronomiques Systeme de Saturne Travaux astronomiques 1658 1666 1925 Tome XVI Mecanique jusqu a 1666 Percussion Question de l existence et de la perceptibilite du mouvement absolu Force centrifuge 1929 Tome XVII L horloge a pendule de 1651 a 1666 Travaux divers de physique de mecanique et de technique de 1650 a 1666 Traite des couronnes et des parhelies 1662 ou 1663 1932 Tome XVIII L horloge a pendule ou a balancier de 1666 a 1695 Anecdota 1934 Tome XIX Mecanique theorique et physique de 1666 a 1695 Huygens a l Academie royale des sciences 1937 Tome XX Musique et mathematique Musique Mathematiques de 1666 a 1695 1940 Tome XXI Cosmologie 1944 Tome XXII Supplement a la correspondance Varia Biographie de Chr Huygens Catalogue de la vente des livres de Chr Huygens 1950 See also EditHistory of the internal combustion engine List of largest optical telescopes historically Fokker Organ Seconds pendulumReferences Edit Wybe Kuitert Japanese Robes Sharawadgi and the landscape discourse of Sir William Temple and Constantijn Huygens Garden History 41 2 2013 pp 157 176 Plates II VI and Garden History 42 1 2014 p 130 ISSN 0307 1243 Online as PDF Archived 9 August 2021 at the 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supernatant Nature 76 1972 381 Bibcode 1907Natur 76 381L doi 10 1038 076381a0 S2CID 4045325 Archived from the original on 28 July 2020 Retrieved 12 September 2019 a b c d Yoder Joella 17 May 2013 A Catalogue of the Manuscripts of Christiaan Huygens including a concordance with his Oeuvres Completes BRILL ISBN 9789004235656 Archived from the original on 16 March 2020 Retrieved 12 April 2018 Audouin Dollfus 2004 Christiaan Huygens as telescope maker and planetary observer In Karen Fletcher ed Titan from discovery to encounter Vol 1278 Noordwijk Netherlands ESA Publications Division pp 115 132 Bibcode 2004ESASP1278 115D ISBN 92 9092 997 9 Huygens Christiaan 1977 Translated by Blackwell Richard J Christiaan Huygens The Motion of Colliding Bodies Isis 68 4 574 597 doi 10 1086 351876 JSTOR 230011 S2CID 144406041 a b Yoeder Joella 1991 Christiaan Huygens Great Treasure PDF Tractrix 3 1 13 Archived PDF from the original on 13 April 2018 Retrieved 12 April 2018 Christiaan Huygens Oeuvres completes Tome XXII Supplement a la correspondance in Dutch Digitale Bibliotheek Voor de Nederlandse Lettern Archived from the original on 13 April 2018 Retrieved 12 April 2018 Further reading Edit Andriesse C D 2005 Huygens The Man Behind the Principle Foreword by Sally Miedema Cambridge University Press Bell A E 1947 Christian Huygens and the Development of Science in the Seventeenth Century Boyer C B 1968 A History of Mathematics New York Dijksterhuis E J 1961 The Mechanization of the World Picture Pythagoras to Newton Hooijmaijers H 2005 Telling time Devices for time measurement in Museum Boerhaave A Descriptive Catalogue Leiden Museum Boerhaave Struik D J 1948 A Concise History of Mathematics Van den Ende H et al 2004 Huygens s Legacy The golden age of the pendulum clock Fromanteel Ltd Castle Town Isle of Man Yoder J G 2005 Book on the pendulum clock in Ivor Grattan Guinness ed Landmark Writings in Western Mathematics Elsevier 33 45 External links Edit Wikimedia Commons has media related to Christiaan Huygens Wikiquote has quotations related to Christiaan Huygens Primary sources translations Edit Works by Christiaan Huygens at Project Gutenberg C Huygens translated by Silvanus P Thompson 1912 Treatise on Light Errata Works by or about Christiaan Huygens at Internet Archive Works by Christiaan Huygens at LibriVox public domain audiobooks Clerke Agnes Mary 1911 Huygens Christiaan Encyclopaedia Britannica Vol 14 11th ed pp 21 22 Correspondence of Christiaan Huygens at Early Modern Letters Online De Ratiociniis in Ludo Aleae or The Value of all Chances in Games of Fortune 1657 Christiaan Huygens s book on probability theory An English translation published in 1714 Text pdf file Horologium oscillatorium German translation pub 1913 or Horologium oscillatorium English translation by Ian Bruce on the pendulum clock KOSMO8EWROS Cosmotheoros English translation of Latin pub 1698 subtitled The celestial worlds discover d or Conjectures concerning the inhabitants plants and productions of the worlds in the planets C Huygens translated by Silvanus P Thompson Traite de la lumiere or Treatise on light London Macmillan 1912 archive org details treatiseonlight031310mbp New York Dover 1962 Project Gutenberg 2005 gutenberg org ebooks 14725 Errata Systema Saturnium 1659 text a digital edition of Smithsonian Libraries On Centrifugal Force 1703 Huygens s work at WorldCat The Correspondence of Christiaan Huygens in EMLO Christiaan Huygens biography and achievements Portraits of Christiaan Huygens Huygens s books in digital facsimile from the Linda Hall Library 1659 Systema Saturnium Latin 1684 Astroscopia compendiaria Latin 1690 Traite de la lumiere French 1698 KOSMO8EWROS sive De terris cœlestibus Latin Museums Edit Huygensmuseum Hofwijck in Voorburg Netherlands where Huygens lived and worked Huygens Clocks exhibition from the Science Museum London Online exhibition on Huygens in Leiden University Library in Dutch Other Edit O Connor John J Robertson Edmund F Christiaan Huygens MacTutor History of Mathematics archive University of St Andrews Huygens and music theory Huygens Fokker Foundation on Huygens s 31 equal temperament and how it has been used Christiaan Huygens on the 25 Dutch Guilder banknote of the 1950s Christiaan Huygens at the Mathematics Genealogy Project How to pronounce Huygens Portals Biography The Netherlands Physics Mathematics Astronomy Stars Outer space Solar System Retrieved from https en wikipedia org w index php title Christiaan Huygens amp oldid 1153994274, wikipedia, wiki, book, books, library,

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