Books with author Isaac Newton Stevens

Dragon liver costs 17 sickles per ounce and has 12 magical properties. Do you know what they are!?166 facts you probably don't know about the Magical Wizarding World of Harry Potter! If you want to up your knowledge, feel a bit of nostalgia from your favorite magical world or just need that perfect gift to give to a Harry Potter addict, click 'Add to cart' button Now!Get the Kindle edition FREE when you purchase the paperback book!

Dragon liver costs 17 sickles per ounce and has 12 magical properties. Do you know what they are!?166 facts you probably don't know about the Magical Wizarding World of Harry Potter! If you want to up your knowledge, feel a bit of nostalgia from your favorite magical world or just need that perfect gift to give to a Harry Potter addict, click 'Add to cart' button Now!Get the Kindle edition FREE when you purchase the paperback book!

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Sir Isaac Newton (1642-1727) is without a doubt one of the most well-known and influential scientists in history; he made incalculable contributions to the fields of physics, mathematics, astronomy, philosophy and theology. From 1670 to 1672, Newton lectured on optics while developing his theory of color. This led to his invention of the refracting telescope in 1672, which would correct chromatic aberration in the traditional refracting telescope, and so impressed the Royal Society that they encouraged him to publish his work. "Opticks" was Newton's second major contribution in this field, and offered new insights into the nature of color, light, and the phenomena of diffraction. The book also includes Newton's Queries, which address a wide range of physical phenomena, include the nature and transmission of heat, the possible cause of gravity, electrical phenomena, chemical action, and ethics of both science and human conduct.

A DOCTOR RETURNS FROM INDIA Among the hundreds of people who were awaiting the arrival of the big Cunarder there were two groups, the second of which seemed determined that the first should not get far away. The young men of which this second group was composed represented the various newspapers of New York City, and while a "beat" was evidently impossible, each of them was determined to get a line for his own journal from the returning hero, Dr. John Earl, which he would not share with the Others of the fraternity, and several of them held anxious consultations with their photographers who, by special permit, had been allowed upon the pier. The Other group had moved a number of times to escape the cameras, and a red-haired youth was expatiating upon the glories of American scientific achievement, concluding with a peroration that called forth an exclamation from one of the older men: "Oh, shut up, Bedford; you sound like a Fourth of July oration. Who are the people you are trying to snapshot for your lurid sheet?" he said wearily, as becomes a Chicago newspaper man when in New York. The red-headed one looked at him with cheerful surprise. "Don't you know anybody?" he asked. "The tall, handsome blonde is Mrs. Ramsey, wife of George Ramsey, at whose frown the great gods sit tight and the little ones scuttle to cover. Luckily, he is a kindly disposed arbiter and the Street basks under his smile." The Chicagoan turned and looked at the lady curiously, and the reporter went on: "The fair-haired lady with the wild-rose face is old Gordon Kimball's daughter; born with a diamond teething ring in her mouth, but has never succeeded in getting anything else of value inside her pretty head

Sir Isaac Newton (1642-1727) is without a doubt one of the most well-known and influential scientists in history; he made incalculable contributions to the fields of physics, mathematics, astronomy, philosophy and theology. From 1670 to 1672, Newton lectured on optics while developing his theory of color. This led to his invention of the refracting telescope in 1672, which would correct chromatic aberration in the traditional refracting telescope, and so impressed the Royal Society that they encouraged him to publish his work. "Opticks" was Newton's second major contribution in this field, and offered new insights into the nature of color, light, and the phenomena of diffraction. The book also includes Newton's Queries, which address a wide range of physical phenomena, include the nature and transmission of heat, the possible cause of gravity, electrical phenomena, chemical action, and ethics of both science and human conduct.

Newton's treatise concerning the behaviour of light is published here in full, complete with the original illustrations and tables. In this work, Newton primarily focuses on how light behaves when refracted within a prism or lense. Prior to Newton's examinations, it was assumed that prisms and other refracting instruments simply produced the colors by themselves. However via thorough experimentation and observation, Newton proved that the colors are in fact already present in light, and that the prism simply separates them so as they are visible to the naked eye. Together with his groundbreaking discovery, Opticks examines light as it behaves through a variety of solid mediums. Newton would use many tools, from shaded and colored glass to mirrors to study and record how light behaved under a variety of conditions. Newton eventually manages to organise every color into a circle, which successfully explains how each hue is related to others. Newton's experiments are detailed in full with accompanying images which illustrate the shapes, angles and procedures each entails, while tables record the figures which Newton used. This data allows experimenters to reproduce and verify the results personally. For its thorough use of logic and the scientific method, Opticks has become regarded as one of the finest works of Enlightenment era science. When Newton first presented his discoveries to the Royal Society, they aroused sharp criticisms from his contemporaries both in England and in Europe. Many disputed all or some of his conclusions and methods, with the scientist Robert Hooke giving a particularly withering critique of Newton's Corpuscular theory of light. As a result, the Opticks was not formally published until 1703 following Hooke's death. It received several revisions and additions from Newton until his death in 1726 or 1727 - most notably to the Queries at the end of the book. Many of these deal with completely different scientific subjects, such as the behaviour of chemicals and the nature of gravity. Despite their title, the Queries are purely rhetorical in form, and Newton makes a strident attempt at answering and discussing each.

This scarce antiquarian book is a facsimile reprint of the original. Due to its age, it may contain imperfections such as marks, notations, marginalia and flawed pages. Because we believe this work is culturally important, we have made it available as part of our commitment for protecting, preserving, and promoting the world's literature in affordable, high quality, modern editions that are true to the original work.

This book provides a wide representation of the interests, problems, and diverse philosophic issues that preoccupied the greatest scientific mind of the 17th century. Grouped in sections corresponding to methods, principles, and theological considerations, these selections feature explanatory notes and cross-references to related essays. 1953 edition.

Sir Isaac Newton PRS MP (25 December 1642 – 20 March 1727) was an English physicist and mathematician who is widely regarded as one of the most influential scientists of all time and as a key figure in the scientific revolution. His book Philosophiæ Naturalis Principia Mathematica("Mathematical Principles of Natural Philosophy"), first published in 1687, laid the foundations for most of classical mechanics. Newton also made seminal contributions to optics and shares credit with Gottfried Leibniz for the invention of the infinitesimal calculus. Newton's Principia formulated the laws of motion and universal gravitation that dominated scientists' view of the physical universe for the next three centuries. It also demonstrated that the motion of objects on the Earth and that of celestial bodies could be described by the same principles. By deriving Kepler's laws of planetary motion from his mathematical description of gravity, Newton removed the last doubts about the validity of the heliocentric model of the cosmos. -Wikipedia