Books

2 vol. in-8 : XXX-752 pp. + Glasgow, Georgis Brookman; Londres, T.T. et J. Tegg, 1833, , 2 vol. in-8 : XXX-752 pp. + 204 pp, Demi-basane maroquin�e long grain rouge, plats de toile verte, dos long, pi�ce de titre noire, �dition �tablie et comment�e par les fr�res minimes fran�ais Thomas Le Sueur (ou Lesueur) et Fran�ois Jacquier, tous deux enseignants de math�matiques. Le premier professait � l'Universit� de la Sapience � Rome, le second au Coll�ge romain. Elle est illustr�e de nombreuses figures dans le texte et dans le monde anglophone, on la surnomme parfois "l'�dition j�suite". Elle est reprise sur l'�dition parue � Gen�ve entre 1739 et 1742. Elle comprend le texte de Newton dans sa troisi�me �dition de 1726, le commentaire des deux eccl�siastiques et les abondantes notes de Jean-Louis Calandrini. Elle fut imprim�e une premi�re fois chez les m�mes �diteurs en 1822. Cette �dition ayant connu un grand succ�s, il s'en fit la pr�senta r�impression. Bien que le texte fut d�j� auparavant publi� et connu, ce sont ces deux �ditions (celle de 1822 et de 1833) qui ont le plus particip� � sa diffusion et son succ�s au XIXe si�cle. Le second volume comprend, ins�r� entre la 24e et la 25e propositions du troisi�me livre, le Trait� sur le flux et reflux de la mer de Bernoulli et De causa physica fluxus et refluxus maris de Mac-Laurin. Gray, G. J. A bibliography of the works of Sir Isaac Newton, pp. 13-14; Petits frottements et �pidermures, dos fonc�s, minuscules taches ou rousseurs �parses. �tiquette et tampons de l'Institut catholique de Paris.

"The Mathematical Principles of Natural Philosophy," commonly known as "Principia," is a monumental scientific work by Sir Isaac Newton, first published in 1687. This magnum opus encompasses Newton's groundbreaking theories on mechanics, motion, and gravity, fundamentally altering scientific paradigms. Newton formulated three laws of motion, elucidating the relationships between force, mass, and acceleration. These laws laid the foundation for classical mechanics, outlining how objects move under the influence of external forces. The first law states that an object remains at rest or moves at a constant velocity unless acted upon by an external force. The second law introduces the concept of force, asserting that force equals mass multiplied by acceleration (F = ma). The third law describes action and reaction, stating that for every action, there is an equal and opposite reaction. However, Newton's most influential contribution was his law of universal gravitation. He proposed that every particle of matter attracts every other particle with a force proportional to their masses and inversely proportional to the square of the distance between their centers. This law explained not only the motion of celestial bodies but also the falling of objects on Earth, unifying celestial and terrestrial mechanics. Newton's Principia revolutionized scientific thought by providing a mathematical framework to describe and predict the motion of objects in the universe. It presented a systematic approach to understanding natural phenomena, marking a departure from earlier qualitative explanations. Newton's work profoundly influenced subsequent scientific inquiry, serving as a cornerstone for further developments in physics and astronomy. Moreover, Principia's impact extended beyond the scientific community, inspiring advancements in various fields. Its emphasis on empirical evidence and mathematical rigor became a model for scientific investigation, fostering a culture of systematic observation and experimentation. The legacy of "The Mathematical Principles of Natural Philosophy" endures as one of the most influential scientific works in history, shaping the foundations of modern physics and serving as a testament to Newton's genius and contribution to humanity's understanding of the natural world.