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Libreria Antiquaria Giulio Cesare
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Antica nota alla prima bianca, rare annotazioni marginali coeve, microforo marginale di tarlo estinto all'angolo superiore delle prime 50 carte senza alcun interessamento del testo, naturali bruniture dovute alla qualità della carta. L'Autore in quest'opera suddivisa in tre libri (nei primi due espone il moto dei corpi e dei mezzi di contrasto quali aria e acqua e nel terzo descrisse la legge di gravitazione universale) stabilì i fondamenti per la meccanica classica. Nei Principia Newton compie l'unificazione tra la fisica galileiana e l'astronomia di Keplero. Marca calcografica della Compagnie des Libraires di Amsterdam sul frontespizio (Due mani uscenti da nuvole strette davanti a fascio littorio che regge una bilancia con due putti seduti su casse ai lati. In basso cornucopie. In alto motto in cartiglio che cita: Vis Unita Major. Tavola grande ripiegata raffigurante l'orbita della cometa, che secondo la tesi di Newton poteva essere non solo ellittica, ma anche iperbolica e parabolica. Alle prime carte dedica a Carlo II, a seguire un poemetto di E.D. Halley a Newton e due prefazioni di Newton, datate Maii 8, 1686 e Mar. 28, 1713 (28) + 484 + (7) con una tavola grande ripiegata e numerose ill. n.t. p. 260x205 mm.

About The Mathematical Principles of Natural Philosophy

"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.