John Theophilus Desaguliers. 1683 – 1744 Born in La Rochelle, France Moved to England as a child. Graduated from Christ Church, Oxford University. He was a priest, freemason, engineer and natural philosopher. Popularised Newtonian Sciences.
Desaguliers became experimental assistant to Isaac Newton in 1713 whilst at Oxford.
He soon made a name for himself as apublic experimental lecturer in London.
His popular lectureswere intended to demonstrate Newton propositions to non-academic audiences.
Desaguliers was awarded the Society’s highest honour, the Copley medal, three times in 1734, 1736 and 1741. His most famous achievement was for discoveries of the properties of electricity.
Desagulierswas one of many who tried to provide introductory texts to Newton’s Principa.
Something Newton always refused to provide.
In 1720, Desaguliers translated, Mathematical Elements of Natural Philosophy, Confirmed by experiments: or, An Introduction to Sir Isaac Newton’s Philosophy, into English.
Not only was he able to translate the work of continental Newtonians but also produce translations of his own works, spreading Newtonian philosophy further.
But Newton the unparallel’d, whose Name
No Time will wear out of the Book of Fame,
Caelestial Science has promoted more,
Than all the Sages that have shone before.
Nature compell’d, his piercing Mind, obeys,
And gladly shews him all her secret Ways;
‘GainstMathematicks she has no Defence,
And yield t’experimental Consequence:
His tow’ring Genius, from its certain Cause,
Ev’ry Appearance, a priori draws,
And shewsth’ Almighty Architect’s unalter’d Laws.
Throughout his life, government and Allegorical Poem - 1728Desaguliers helped to publish and write many books about Experimental Philosophy. In 1734 his own book, Course of Experimental Philosophy, was published and became very popular.
Desaguliers’ Planetarium, was an instrument made ‘to shew the motion of the heavenly bodies’. He is credited as the inventor of the planetarium, a model of the solar systemto show the relative motions of the planets.
The water supply in Edinburgh
The ventilation of the houses
The first Westminster bridge
Within the the Royal Society he devised new experiments to defend several of Newton’s claims, such as the shape of the Earth.
At the time, Newton suggested universal gravitation which meant that the Earth’s rotation would cause a slight flattening at the poles, whereas at the time many others believed the poles would be elongated.
Isaac Newton formulated the law of universal gravitation between two objects. The law states that between two objects of masses m1 and m2, with centers of mass a distance d apart, there is an attractive force magnitude.
G is the gravitational constant and in SI units has a value of 6.67x10-11 kg-1 m3 s-1. The force F is called the gravitation force.
The gravitational force of an object on the Earth’s surface is often called the weight of the object.
Find the magnitude of the gravitational force of an object of mass M on the Earth’s surface. Assume that the Earth is a sphere of mass 5.98x1024 kg and a radius 6.37x106 m.
G is the gravitational constant and has a value of 6.67x10-11 kg-1 m3 s-1.
We see that Newton’s universal law of gravitation gives the familiar rule of the force of gravity or the weight of an object of mass M as Mg, where g = 9.8ms-2.
Do you recognise the answer?