The Heydays of Mechanical Materialism

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The Heydays of Mechanical Materialism A Brief History of Science Part 7: The Heydays of Mechanical Materialism Soumitro Banerjee∗ HE GREAT UPHEAVAL of science in 1865) managed to enrich classical mechan- Tthe 17th century after the millennia of ics substantially beyond the Newtonian for- slumber of the middle ages reached its pin- mulation. nacle in the masterly work of Newton. For a long time Europeans had forgotten to look Measuring the solar system at the nature around them with eyes of cu- riosity, and had directed their interest to After Newton the heliocentric nature of the the divine. The success of Newtonian me- solar system and the laws governing its mo- chanics in explaining the motion around tion were established, but many important us, especially the motion of the heavenly details about the solar system were not yet bodies, caused a resurgence of materialist known. What is the weight of the Earth? outlook. That, in turn, generated interest How big is the solar system? What are the in understanding various aspects of nature, distances to the sun and the moon? What and led to a condition conducive to the de- are the radii of the orbits of the other plan- velopment of various branches of science. ets? The answers to these obvious ques- People in larger numbers were taking part tions were not known in Newton’s time. in scientific enquiry. Using Kepler’s laws, one can measure the However, in the area in which Newton had ratios of the radii of the planetary orbits. maximum contribution, namely mathemat- But unless the true radius of the orbit of ical mechanics, we see relatively few new at least one planet is known, none of the ideas added for a long time. His works radii is known in absolute terms. Thus on mechanics was so exhaustive and com- the measurement of the Earth-to-sun dis- prehensive that scientists in the period fol- tance became a matter of paramount im- lowing Newton’s lifetime found it difficult portance. The distance to the moon could to add anything substantial to this body be measured using the method of parallax of knowledge. It was a period of digestion (the change in the moon’s position in the and assimilation of the ideas he created and background of distant stars when viewed their application in different domains. It from two different locations). But the same was only in the second half of the 18th cen- method cannot be applied to find the dis- tury that Leonhard Euler (1707–1783) and tance to the sun, because when the sun is Joseph-Louis Lagrange (1736–1813) and glowing in the sky, the background stars much later William Rowan Hamilton (1805– are not visible. Newton’s friend Edmond Halley came up ∗ Dr. Banerjee is in the faculty of the Indian Institute with a brilliant idea to measure the dis- of Science Education & Research, Kolkata. He is the newly-elected General Secretary of the Breakthrough tance to the sun. He showed that this can Science Society. be done only when the planet Venus comes Breakthrough, Vol.17, No. 2, November 2014 33 Series Article Figure 1: The Spinning Jenny. between the sun and the Earth, which is ets could be calculated easily using Kepler’s a very rare incident. During a “transit of laws. Cavendish (1731–1810) figured out a Venus,” the planet is seen as a small black way of measuring the weight of the Earth dot passing across the disc of the sun. in 1798 using a sensitive torsional balance. The first recorded observation of a tran- Thus, by the turn of the eighteenth century, sit of Venus was made by the Englishmen most of the important information about Jeremiah Horrocks and William Crabtree in the solar system was known. the year 1639. In a paper published in 1726 Halley showed that, if the path of Venus The Industrial Revolution across the sun’s disc is observed from dis- tant locations on the Earth and the exact In the social sphere, capitalism was com- times of contacts with the sun’s circum- ing out of the initial phase where produc- ference are recorded, one can compute the tion was done in handicraft-oriented man- distance to the sun from that information ufactories controlled by merchants into one (for details, see Breakthrough, Vol.15, No.3, of heavy industry controlled by financial February 2012. The article is available in houses. This transformation resulted from Breakthrough website). the industrial revolution (1760 to about Halley died in 1742, and the next couple 1830) which benefited from the develop- of transits of Venus occurred in 1761 and ment of science, and which, in turn, ben- 1769. In these two years a massive col- efited science. The initial onset of the in- laborative effort was undertaken by scien- dustrial revolution, however, did not de- tists, where they launched expeditions to pend on the scientific discoveries. Due to distant lands across the globe, faced un- a short supply of firewood, use of coal in foreseen hurdles, and recorded the event place of firewood as source of heat started scientifically. When the data were brought in the manufactories. Technologies neces- back, the French astronomer Jerome La- sary for the mining and use of coal had lande calculated the distance to the sun to be developed, which paved the way for to be 153 million kilometres. After this path-breaking inventions that changed the success the distances to the other plan- course of history. The initial inventions 34 Breakthrough, Vol.17, No. 2, November 2014 Series Article which steam was introduced through an in- let pipe, which pushed up a piston. When the piston reached the other end of the pis- ton, the steam inlet would be closed and the cylinder would be cooled with a jet of cold water. This would condense the steam into water and the piston would return to the old position. Again steam would be in- troduced and the cycle would be repeated. The cycle was slow, but still the machine managed to replace muscle power in water pumping in mines and some other indus- trial operations. James Watt (1736–1819), the owner of a mechanics shop in Glas- gow, improved the design by replacing the condensation inside the cylinder with con- densation in a separate condenser chamber which was kept cold permanently by circu- lating cold water. At the end of the pushing phase an outlet valve would open, allowing the steam to exit to the condenser. He also devised the means for converting the recip- rocating motion of the piston into the rota- Figure 2: The Newcomen engine. tional motion of a wheel. The first working model was produced in 1765, and after a few refinements was released to the market that multiplied productivity came from the in 1774. working men. In the manufacture of tex- tiles, Hargreaves’ spinning jenny (1764), With the development of the steam en- Arkwright’s water frame (1769), Crompton’s gine, mankind saw a great leap in indus- mule (1779), and Cartwright’s power loom trial productivity. Steam engines could ef- (1785) first increased the productivity of fectively tackle the problem of water accu- hand-operation, and then caused the tran- mulation in mines using steam operated sition from the old hand-operated tech- pumps. This hugely increased the pro- nique to machines that ran on externally duction of coal to provide a cheap source supplied power. In 1709, Darby developed of power. Cotton mills and other facto- the way of making iron from iron ore using ries quickly adopted this source of power. coke obtained from coal (instead of char- Iron and steel making started in a big way. coal), which increased the production of Transportation became much faster with iron many folds. the development of steamers and steam- Finally, with the invention of steam en- ships. Railways powered by steam en- gine made the decisive break with the gines were developed in the early 1800s, old production system. In 1711 a black- which could carry much greater amount of smith called Thomas Newcomen (1664– goods. New industrial towns like Manch- 1729) built the first machine working on ester, Birmingham, Newcastle, and Glas- steam power. It consisted of a cylinder in gow — with favourable political disposition Breakthrough, Vol.17, No. 2, November 2014 35 Series Article Figure 3: Left: The Watt engine in industry. Right: James Watt (1736–1819). and access to water and coal — grew and — the spirit of magnetism. Burning was assumed the centre-stage of industrial ac- thought to be caused by the presence of a tivity. substance called “phlogiston”; when a piece of wood burnt, this substance was believed Science comes out of belief to be coming out to form the flame. The distinction between living matter and non- systems living matter was thought to be due to the presence of a “vital force” in the former. No- We have seen how the development of sci- body bothered to define what the nature ence was impeded for a long time due to of these mysterious spirits was, and how the beliefs in a geocentric picture of the uni- their presence or absence could be tested. verse and Aristotelian ideas in mechanics, One did not know whether these were mate- which were overcome through the work of rial substances which could be isolated, or Copernicus, Galileo, Kepler, and Newton. were particular states of matter. Still these After Newton, the fight with these unscien- ideas persisted even among capable scien- tific notions was gaining victories one after tists and impeded the development of sci- the other.
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