The Great Events by Famous Historians [Volumes 1-14]
- Автор: Gutenberg
- Год: 1905
- Язык: английский
- Жанр: История
Электронная книга - «The Great Events by Famous Historians [Volumes 1-14]». Краткое содержание книги:
The Great Events by Famous Historians, Volume 01
The Great Events by Famous Historians, Volume 02 / (From the Rise of Greece to the Christian Era)
The Great Events by Famous Historians, Volume 03
The Great Events by Famous Historians, Volume 04
The Great Events by Famous Historians, Volume 05 / (From Charlemagne to Frederick Barbarossa)
The Great Events by Famous Historians, Volume 06 / (From Barbarossa to Dante)
The Great Events by Famous Historians, Volume 07
The Great Events by Famous Historians, Volume 08 / The Later Renaissance: from Gutenberg to the Reformation
The Great Events by Famous Historians, Volume 09
The Great Events by Famous Historians, Volume 10
The Great Events by Famous Historians, Volume 11
The Great Events by Famous Historians, Volume 12
The Great Events by Famous Historians, Volume 13
The Great Events by Famous Historians, Volume 14
The Great Events by Famous Historians, Volume 17
The Great Events by Famous Historians, Volume 21 / The Recent Days (1910-1914)
An accident, however, of a very interesting nature induced him to resume his former inquiries, and enabled him to bring them to a close. In June, 1682, when he was attending a meeting of the Royal Society of London, the measurement of a degree of the meridian, executed by M. Picard in 1679, became the subject of conversation. Newton took a memorandum of the result obtained by the French astronomer, and having deduced from it the diameter of the earth, he immediately resumed his calculation of 1665, and began to repeat it with these new data. In the progress of the calculation he saw that the result which he had formerly expected was likely to be produced, and he was thrown into such a state of nervous irritability that he was unable to carry on the calculation. In this state of mind he intrusted it to one of his friends, and he had the high satisfaction of finding his former views amply realized. The force of gravity which regulated the fall of bodies at the earth's surface, when diminished as the square of the moon's distance from the earth, was found to be almost exactly equal to the centrifugal force of the moon as deduced from her observed distance and velocity.
The influence of such a result upon such a mind may be more easily conceived than described. The whole material universe was spread out before him; the sun with all his attending planets; the planets with all their satellites; the comets wheeling in every direction in their eccentric orbits; and the systems of the fixed stars stretching to the remotest limits of space. All the varied and complicated movements of the heavens, in short, must have been at once presented to his mind as the necessary result of that law which he had established in reference to the earth and the moon.
After extending this law to the other bodies of the system, he composed a series of propositions on the motion of the primary planets about the sun, which were sent to London about the end of 1683, and were soon afterward communicated to the Royal Society.
About this period other philosophers had been occupied with the same subject. Sir Christopher Wren had many years before endeavored to explain the planetary motions "by the composition of a descent toward the sun, and an impressed motion; but he at length gave it over, not finding the means of doing it." In January, 1683-1684, Dr. Halley had concluded from Kepler's law of the periods and distances, that the centripetal force decreased in the reciprocal proportion of the squares of the distances, and having one day met Sir Christopher Wren and Dr. Hooke, the latter affirmed that he had demonstrated upon that principle all the laws of the celestial motions. Dr. Halley confessed that his attempts were unsuccessful, and Sir Christopher, in order to encourage the inquiry, offered to present a book of forty shillings value to either of the two philosophers who should, in the space of two months, bring him a convincing demonstration of it. Hooke persisted in the declaration that he possessed the method, but avowed it to be his intention to conceal it for time. He promised, however, to show it to Sir Christopher; but there is every reason to believe that this promise was never fulfilled.
In August, 1684, Dr. Halley went to Cambridge for the express purpose of consulting Newton on this interesting subject. Newton assured him that he had brought this demonstration to perfection, and promised him a copy of it. This copy was received in November by the doctor, who made a second visit to Cambridge, in order to induce its author to have it inserted in the register book of the society. On December 10th Dr. Halley announced to the society that he had seen at Cambridge Newton's treatise De Motu Corporum, which he had promised to send to the society to be entered upon their register, and Dr. Halley was desired to unite with Mr. Paget, master of the mathematical school in Christ's Hospital, in reminding Newton of his promise, "for securing the invention to himself till such time as he can be at leisure to publish it."
On February 25th Mr. Aston, the secretary, communicated a letter from Newton in which he expressed his willingness "to enter in the register his notions about motion, and his intentions to fit them suddenly for the press." The progress of his work was, however, interrupted by a visit of five or six weeks which he made in Lincolnshire; but he proceeded with such diligence on his return that he was able to transmit the manuscript to London before the end of April. This manuscript, entitled Philosophic Naturalis Principia Mathematics and dedicated to the society, was presented by Dr. Vincent on April 28, 1686, when Sir John Hoskins, the vice-president and the particular friend of Dr. Hooke, was in the chair.
Dr. Vincent passed a just encomium on the novelty and dignity of the subject; and another member added that "Mr. Newton had carried the thing so far that there was no more to be added." To these remarks the vice-president replied that the method "was so much the more to be prized as it was both invented and perfected at the same time." Dr. Hooke took offence at these remarks, and blamed Sir John for not having mentioned "what he had discovered to him"; but the vice-president did not seem to recollect any such communication, and the consequence of this discussion was that "these two, who till then were the most inseparable cronies, have since scarcely seen one another, and are utterly fallen out." After the breaking up of the meeting, the society adjourned to the coffee house, where Dr. Hooke stated that he not only had made the same discovery, but had given the first hint of it to Newton.
An account of these proceedings was communicated to Newton through two different channels. In a letter dated May 22d Dr. Halley wrote to him "that Mr. Hooke has some pretensions upon the invention of the rule of the decrease of gravity being reciprocally as the squares of the distances from the centre. He says you had the notion from him, though he owns the demonstration of the curves generated thereby to be wholly your own. How much of this is so you know best, as likewise what you have to do in this matter; only Mr. Hooke seems to expect you would make some mention of him in the preface, which it is possible you may see reason to prefix."
This communication from Dr. Halley induced the author, on June 20th, to address a long letter to him, in which he gives a minute and able refutation of Hooke's claims; but before this letter was despatched another correspondent, who had received his information from one of the members that were present, informed Newton "that Hooke made a great stir, pretending that he had all from him, and desiring they would see that he had justice done him." This fresh charge seems to have ruffled the tranquillity of Newton; and he accordingly added an angry and satirical postscript, in which he treats Hooke with little ceremony, and goes so far as to conjecture that Hooke might have acquired his knowledge of the law from a letter of his own to Huygens, directed to Oldenburg, and dated January 14,1672-1673. "My letter to Hugenius was directed to Mr. Oldenburg, who used to keep the originals. His papers came into Mr. Hooke's possession. Mr. Hooke, knowing my hand, might have the curiosity to look into that letter, and there take the notion of comparing the forces of the planets arising from their circular motion; and so what he wrote to me afterward about the rate of gravity might be nothing but the fruit of my own garden."
In replying to this letter Dr. Halley assured him that Hooke's "manner of claiming the discovery had been represented to him in worse colors than it ought, and that he neither made public application to the society for justice nor pretended that you had all from him." The effect of this assurance was to make Newton regret that he had written the angry postscript to his letter; and in replying to Halley on July 14, 1686, he not only expresses his regret, but recounts the different new ideas which he had acquired from Hooke's correspondence, and suggests it as the best method "of compromising the present dispute" to add a scholium in which Wren, Hooke, and Halley are acknowledged to have independently deduced the law of gravity from the second law of Kepler.