Search over 40,000 articles from the original, classic Encyclopedia Britannica, 11th Edition.
|
See also:SIR See also:ISAAC See also:NEWTON (1642-1727)
, See also:English natural philosopher, was See also:born on the 25th of See also:December 1642 (o.s.), at Woolsthorpe, a See also:hamlet in the See also:parish of Colsterworth, See also:Lincolnshire, about 6 m. from See also:Grantham
.
His See also:father (also See also:Isaac See also:Newton) who farmed a small See also:freehold See also:property of his own, died before his son's See also:birth, a few months after his See also:marriage to Hannah See also:Ayscough, a daughter of See also:
Newton was then in his fifteenth See also:year, and, as his mother in all See also:probability intended him to be a See also:farmer, he was taken away from school
.
He was frequently sent on market days to Grantham with an old and trusty servant, who made all the purchases, while Newton spent his See also:time among the books in Mr Clark's house
.
It soon became apparent to Newton's relatives that they were making a See also:great See also:mistake in attempting to turn him into a farmer, and he was therefore sent back again to school at Grantham
.
His mother's See also:brother, See also:
At such time I found the method of See also:Infinite See also:Series; and in summer 1665, being forced from Cambridge by the See also:plague, I computed the See also:area of the See also:Hyperbola at Boothby, in Lincolnshire, to two and fifty figures by the same method."
That Newton must have begun early to make careful observations of natural phenomena is sufficiently testified by the follow- . See also:ing remarks about halos, which appear in his See also:Optics, book ii. part iv. obs
.
13:
" The like Crowns appear sometimes about the See also:moon; for in the beginning of the Year 1664, See also:February 19th, at See also:night, I saw two such Crowns about her
.
The See also:Diameter of the first or innermost was about three Degrees, and that of the second about five Degrees and an half
.
Next about the moon was a Circle of See also:
He was elected a See also:fellow of his college on the 1st of See also:October 1667
.
There were nine vacancies, one of which was caused by the See also:death of See also:Abraham See also:Cowley in the previous summer, and the nine successful candidates were all of the same academical See also:standing
.
A few See also:weeks after his See also:election to a fellowship Newton went to Lincolnshire, and did not return to Cambridge till the February following, On the 16th of See also:
On the 21st of December 1671 he was proposed as a See also:candidate for See also:admission into the Royal Society by Dr See also:Seth See also: And as that was sensibly better than the first (especially for See also:Day-See also:Objects), so I doubt not, but they will be still brought to a much greater perfection by their endeavours, who, as you inform me, are taking care about it at London." After a remark that microscopes seem as capable of improvement as telescopes, he adds: " I shall now proceed to acquaint you with another more notable difformity in its Rays, wherein the Origin of See also:Colour is unfolded: Concerning which I shall See also:lay down the See also:Doctrine first, and then, for its examination, give you an instance or two of the Experiments, as a specimen of the See also:rest . The Doctrine you will find comprehended and illustrated in the following propositions: " 1 . As the Rays of light differ in degrees of Refrangibility, so they also differ in their disposition to exhibit this or that particular colour . Colours are not Qualifications of Light, derived from Refractions, or Reflections of natural Bodies (as 'tis generally believed), but See also:original and connate properties, which in divers Rays are divers . Some Rays are disposed to exhibit a red colour and no other; some a yellow and no other, some a green and no other, and so of the rest . Nor are there only Rays proper and particular to the more eminent colours, but even to all their intermediate gradations . " 2 . To the same degree of Refrangibility ever belongs the same colour, and to the same colour ever belongs the same degree of Refrangibility . The least Refrangible Rays are all disposed to exhibit a Red colour, and contrarily those Rays, which are disposed to exhibit a Red colour, are all the least Refrangible: So the most refrangible Rays are all disposed to exhibit a deep See also:Violet Colour, and contrarily those which are apt to exhibit such a violet colour are all the most Refrangible . " And so to all the intermediate colours in a continued series belong intermediate degrees of refrangibility . And this See also:Analogy 'twixt colours, and refrangibility is very precise and strict; the Rays always either exactly agreeing in both, or proportionally disagreeing in both . " 3 . The See also:species of colour, and degree of Refrangibility proper to any particular sort of Rays, is not mutable by Refraction, nor by Reflection from natural bodies, nor by any other cause, that I could yet observe . When any one sort of Rave hath been well parted from those of other kinds, it hath afterwards obstinately retained its colour, notwithstanding my utmost endeavours to See also:change it . I have refracted it with Prismes, and reflected it with Bodies, which in Day-light were of other colours; I have intercepted it with the coloured film of See also:Air interceding two compressed plates of glass, transmitted it through coloured Mediums, and through Mediums irradiated with other sorts of Rays, and diversly terminated it; and yet could never produce any new colour out of it . It would by contracting or dilating become more brisk, or faint, and by the loss of many Rays, in some cases very obscure and dark; but I could never see it changed in specie . " Yet seeming transmutations of Colours may be made, where there is any mixture of divers sorts of Rays . For in such mixtures, the component colours appear not, but, by their 'mutual allaying each other constitute a midling colour." Further on, after some remarks on the subject of See also:compound colours, he says: " I might add more instances of this nature, but I shall conclude with this See also:general one, that the Colours of all natural Bodies have no other origin than this, that they are variously qualified to reflect one sort of light in greater plenty then another . And this I have experimented in a dark Room by See also:illuminating those bodies with uncompounded light of divers colours . For by that means any See also:body may be made to appear of any colour . They have there no appropriate colour, but ever appear of the colour of the light See also:cast upon them, but yet with this difference, that they are most brisk and vivid in the light of . their own day-light colour . Minium appeareth there of any colour indifferently, with which 'tis illustrated, but yet most luminous in red, and so Bise appeareth indifferently of any colour with which 'tis illustrated, but yet most luminous in blew . And therefore minium reflecteth Rays of any colour, but most copiously those indeed with red; and consequently when illustrated with day-light, that is with all sorts of Rays promiscuously blended, those qualified with red shall abound most in the reflected See also:binocular See also:vision . He also invented a reflecting See also:sextant for observing. the distance between the moon and the fixed stars,—the same in every essential as the instrument which is still in everyday use at See also:sea under the name of See also:Hadley's quadrant . This discovery was communicated by him to See also:Edmund See also:Halley in 1700, but was not published, or communicated to the Royal Society, till after Newton's death, when a description of it was found among his papers . In March 1673 Newton took a prominent part in a dispute in the university . The public oratorship See also:fell vacant, and a contest arose between the heads of the colleges and the members of the See also:senate as to the mode of electing to the See also:office . The heads claimed the right of nominating two persons, one of whom was to be elected by the senate . The senate insisted that the proper mode was by an open election . The See also:duke of See also:Buckingham, who was the See also:chancellor of the university, endeavoured to effect a See also:compromise which, he says, " I See also:hope may for the See also:present satisfy both sides . I propose that the heads may for this time nominate and the body comply, yet interposing (if they think See also:fit) a protestation concerning their plea that this election may not here-after pass for a decisive precedent in See also:prejudice of their claim," and, " whereas I understand that the whole university has chiefly consideration for Dr Henry Paman of St John's and Mr See also:Craven of Trinity College, I do recommend them both to be nominated." The heads, however, nominated Dr Paman and See also:Ralph Sanderson of St John's, and the next day one See also:hundred and twenty-one members of the senate recorded their votes for Craven and ninety-eight for Paman . On the See also:morning of the election a protest in which Newton's name appeared was read, and entered in the See also:Regent House . But the See also:vice-chancellor admitted Paman the same morning, and so ended the first contest of a non-scientific See also:character in which Newton took part . On the 8th of March 1673 Newton wrote to Oldenburg, the secretary of the Royal Society: " Sir, I desire that you will procure that I may be put out from being any longer Fellow of the Royal Societ : for though I See also:honour that body, yet since I see I shall neither profit them, nor (by See also:reason of this distance) can partake of the See also:advantage of their assemblies, I desire to withdraw." Oldenburg must have replied to this by an offer to apply to the Society to excuse Newton the weekly payments, as in a letter of Newton's to Oldenburg, dated the 23rd of June 1673, he says, " For your proffer about my quarterly payments, I thank you, but I would not have you trouble yourself to get them excused, if you have not done it already." Nothing further seems to have been done in the See also:matter until the 28th of January 1675, when Oldenburg informed " the Society that Mr Newton is now in such circumstances that he desires to be excused from the weekly payments." Upon this " it was agreed to by the See also:council that he be dispensed with, as several others are." On the 18th of February 1675 Newton was formally admitted into the Society . The most probable explanation of the cause why Newton wished to be excused from these payments is to be found in the fact that, as he was not in See also:holy orders, his fellowship at Trinity College would See also:lapse in the autumn of 1675 . It is true that the loss to his income which this would have caused was obviated by a patent from the crown in April 1675, allowing him as Lucasian professor to retain his fellowship without the See also:obligation of taking holy orders . This must have relieved Newton's mind from a great See also:deal of anxiety about pecuniary matters, as we find him in . See also:November 1676 subscribing £4o towards the See also:building of the new library of Trinity College . It is supposed that it was at Woolsthorpe in the summer of 1666 that Newton's thoughts were directed to the subject of gravity . See also:Voltaire is the authority for the well-known See also:anecdote about the See also:apple . He had his information from Newton's favourite niece Catharine See also:Barton, who married Conduitt, a fellow of the Royal Society, and one of Newton's intimate See also:friends . How much truth there is in what is a plausible and a favourite See also:story can never be known, but it is certain that tradition marked a See also:tree as that from which the apple fell, till 182o, when, owing to decay, the tree was cut down and its See also:wood carefully. preserved . light, and. by their prevalence cause it to appear of that colour . And for the same reason Bise, reflecting blew most copiously, shall appear blew by the excess of those Rays in its reflected Iight; and the like of other bodies . And that this is the intire and adequate cause of their colours, is See also:manifest, because they have no See also:power to change or alter the colours of any sort of Rays incident apart, but put on all colours indifferently, with which they are inlightened . Reviewing what I have written, I see the discourse it self will See also:lead to divers Experiments sufficient for its examination: And therefore I shall not trouble you further, than to describe one of those, which I have already insinuated . " In a darkened Room make a hole in the shut of a window whose diameter may conveniently be about a third part of an See also:inch, to admit a convenient quantity of the Suns light: And there See also:place a clear and colourless Prisme, to refract the mitring light towards the further part of the Room, which, as I said, will thereby be diffused into an oblong coloured See also:Image . Then place a Lens of about three See also:foot See also:radius (suppose a broad Object-glass of a three foot Telescope), at the distance of about four or five foot from thence, through which all those colours may at once be transmitted, and made by its Refraction to convene at a further distance of about ten or twelve feet . If at that distance you intercept this light with a See also:sheet of white paper, you will see the colours converted into whiteness again by being mingled . " But it is requisite, that the Prisme and Lens be placed steddy, and that the paper, on which the colours are cast be moved to and fro; for, by such See also:motion, you will not only find, at what distance the whiteness is most perfect but also see, how the colours gradually convene, and vanish into whiteness, and afterwards having crossed one another in that place where they compound Whiteness, are again dissipated and severed, and in an inverted order retain the same colours, which they had before they entered the composition . You may also see, that, if any of the Colours at the Lens be intercepted, the Whiteness will be changed into the other colours . And therefore, that the composition of whiteness be perfect, care must be taken, that none of the colours fall besides the Lens." He concludes his communication with the words: " This, I conceive, is enough for an Introduction to Experiments of this kind: which if any of the R . Society shall be so curious as to prosecute, I should be very glad to be informed with what success: That, if any thing seem to be defective, or to thwart this relation, I may have an opportunity of giving further direction about it, or of acknowledging my errors, if I have committed any." The publication of these discoveries led to a series of controversies which lasted for several years, in which Newton had to contend with the eminent English natural philosopher See also:Robert See also:Hooke; See also:Lucas, mathematical professor at See also:Liege; See also:Linus, a physician in Liege, and many others . Some of his opponents denied the truth of his experiments, refusing to believe in the existence of the spectrum . Others criticized the experiments, saying that the length of the spectrum was never more than three and a half times the breadth, whereas Newton found it to be five times the breadth . It appears that Newton made the mistake of supposing that all prisms would give a spectrum of exactly the same length; the objections of his opponents led him to measure carefully the lengths of spectra formed by prisms of different angles and of different refractive indices; and it seems See also:strange that he was not led thereby to the discovery of the different dispersive powers of different refractive substances . Newton carried on the discussion with the objectors with great See also:courtesy and See also:patience, but the amount of See also:pain which these perpetual discussions gave to his sensitive mind may be estimated from the fact of his See also:writing on the 18th of November 1676 to Oldenburg: " I promised to send you an See also:answer to Mr Lucas this next Tuesday, but I find I shall scarce finish what I have designed, so as to get a copy taken of it by that time, and therefore I beg your patience a week longer . I see I See also:nave made myself a slave to See also:philosophy, but if I get See also:free of Mr Lucas's business, I will resolutely bid adieu to it eternally, excepting what I do for my private See also:satisfaction, or leave to come out after me; for I see a man must either resolve to put out nothing new, or to become a slave to defend it." It was a fortunate circumstance that these disputes did not so thoroughly See also:damp Newton's ardour as he at the time See also:felt they would . He subsequently published many papers in the Philosophical Transactions on various parts of the See also:science of optics, and, although some of his views have.been found to be erroneous, and are now almost universally rejected, his investigations led to discoveries which are of permanent value . He succeeded in explaining the colour of thin and of thick plates, and the See also:inflexion of light, and he wrote on See also:double refraction, polarization and Johann See also:Kepler had proved by an elaborate series of measurements that each See also:planet revolves in an elliptical See also:orbit See also:round the See also:sun, whose centre occupies one of the foci of the orbit, that the radius vector of each planet drawn from the sun describes equal areas in equal times, and that the squares of the periodic times of the See also:planets are in the same proportion as the cubes of their mean distances from the sun . The fact that heavy bodies have always a tendency to fall to the See also:earth, no matter at what height they are.placed above the earth's See also:surface, seems to have led Newton to conjecture that it was possible that the same tendency to fall to the earth was the cause by which the moon was retained in its orbit round the earth . Newton, by calculating from Kepler's See also:laws, and supposing the orbits of the planets to be circles round the sun in the centre, had already proved that the force of the sun acting upon the different planets must vary as the inverse square of the distances of the planets from the sun . He therefore was led to inquire whether, if the earth's attraction extended to the moon, the force at that distance would be of the exact magnitude necessary to retain the moon in its orbit . He found that the moon by her motion in her orbit was deflected from the tangent in every See also:minute of time through a space of thirteen feet . But by observing the distance through which a body would fall in one second of time at the earth's surface, and by calculating from that on the supposition of the force diminishing in the ratio of the inverse square of the distance, he found that the earth's attraction at the distance of the moon would draw a body through 15 ft. in r See also:min . Newton regarded the discrepancy between the results as a See also:proof of the inaccuracy of his conjecture, and " laid aside at that time any further thoughts of this matter." But in 1679 a controversy between Hooke and Newton, about the form of the path of a body falling from a height, taking the motion of the earth round its See also:axis into consideration, led Newton again to revert to his former conjectures on the moon . The measure of the earth, which had hitherto been accepted by geographers and navigators, was based on the very rough estimate that the length of a degree of See also:latitude of the earth's surface measured along a See also:meridian was 6o m . More accurate estimates had been made by R . See also:Norwood and W . See also:Snell, and more recently by P . See also:Picard . At a meeting of the Royal Society on the 11th of January 1672, Oldenburg the secretary read a letter from See also:Paris describing the method followed by Picard in measuring a degree, and specifically stating the precise length that he calculated it to be . It is probable that Newton had become acquainted with this measurement of Picard's, and that he, was therefore led to make use of it when his thoughts were redirected to the subject . This estimate of the earth's magnitude, giving 69•r m. to 1°, made the two results, the discrepancy between which Newton had regarded as a disproof of his conjecture, to agree so exactly that he now regarded his conjecture as fully established . In January 1684 Sir See also:Christopher See also:Wren, Halley and Hooke were led to discuss. the See also:law of gravity, and, although probably they all agreed in the truth of the law of the inverse square, yet this truth was not looked upon as established . It appears that Hooke professed to have a See also:solution of the problem of the path of a body moving round a centre of force attracting as the inverse square of the distance; but Halley, finding, after a delay of some months, that Hooke " had not been so See also:good as his word in showing his solution to Wren, started in the month of August 1684 for Cambridge to consult Newton on the subject . Without mentioning the speculations which had been made, he asked Newton what would be the See also:curve described by a planet round the sun on the See also:assumption that the sun's force diminished as the square of the distance . Newton replied promptly, "an See also:ellipse," and on being questioned by Halley as to the reason for his answer he replied, " Why, I have calculated it." He could not, however, put his See also:hand upon his calculation, but he promised to send it to Halley . After the latter had left See also:Cam See also:bridge, Newton set to work to reproduce the calculation . After making a mistake and producing a different result he corrected his work and obtained his former result . In the following November Newton redeemed his promiseto Halley by sending him, by the hand of Mr See also:Paget, one of the fellows of his own college, and at that time mathematical master of See also:Christ's See also:Hospital, a copy of his demonstration; and very soon afterwards Halley paid another visit to Cambridge to confer with Newton about the problem; and on his return to London on the loth of December 1684, he informed the Royal Society " that he had lately seen Mr Newton at Cam-bridge, who had showed him a curious See also:treatise De Motu," which at Halley's desire he promised to send to the Society to be entered upon their See also:register . " Mr Halley was desired to put Mr Newton in mind of his promise for the securing this invention to himself, till such time as he could be at leisure to publish it," and Paget was desired to join with Halley in urging Newton to do so . By the See also:middle of February Newton had sent his paper to See also:Aston, one of the secretaries of the Society, and in a letter to Aston dated the 23rd of February 1685, we find Newton thanking him for " having entered on the register his notions about motion." This treatise De Motu was the germ of the Principia, and was obviously meant to be a See also:short account of what that work was intended to embrace . It occupies twenty-four See also:octavo pages, -and consists of four theorems and seven problems, some of which are identical with some of the most important pro-positions of the second and third sections of' the first book of the Principia . The years 1685 and 1686 will ever be memorable in the See also:history of science . It was in them that Newton composed almost the whole of his great work . During this period Newton had a very extensive See also:correspondence with John See also:Flamsteed, who was then the astronomer-royal . Many of the letters are lost, but it is clear from one of Newton's, dated the 19th of See also:September 1685, that he had received many useful communications from Flamsteed, and especially regarding See also:Saturn, " whose orbit, as defined by Kepler," Newton "found too little for the sesquialterate proportions." In the other letters written in 1685 and 1686 he applies to Flamsteed for information respecting the orbits of the satellites of See also:Jupiter and Saturn, respecting the rise and fall of the spring and See also:neap tides at the solstices and the equinoxes, respecting the flattening of Jupiter at the poles (which, if certain, he says, would conduce much to the stating the reasons of the precession of the equinoxes), and respecting the difference between the observed places of Saturn and those computed from Kepler's tables about the time of his conjunction with Jupiter . On this last point the information supplied by Flamsteed was peculiarly gratifying to Newton; and it is obvious from the See also:language of this part of his letter that he had still doubts of the universal application of the sesquialteral pro-portion . " Your information," he says, " about the errors of Kepler's tables for Jupiter and Saturn has eased me of several scruples . I was apt to suspect there might be some cause or other unknown to me which might disturb the sesquialteral proportions, for the influences of the planets one upon another seemed not great enough, though I imagined Jupiter's See also:influence greater than your See also:numbers determine it . It would add to my satisfaction if you would be pleased to let me know the long diameters of the orbits of Jupiter and Saturn, assigned by yourself and Mr Halley in your new tables, that I may .see how the sesquialteral proportion fills the heavens, together with another small proportion which must be allowed for." Upon Newton's return from Lincolnshire in the beginning of April 1685, he seems to have devoted himself to the preparation of his work . In the spring he had determined the attractions of masses, and thus completed the law of universal See also:gravitation . In the 'summer he had finished-the second book of the Principia, the first book being the treatise De Motu, which he had enlarged and completed . Excepting in the correspondence with Flamsteed we hear nothing more of the preparation of the Principia until the 21st of April 1686, when Halley read to the Royal Society his Discourse concerning Gravity and its Properties, in which he states " that his worthy countryman Mr Isaac Newton has an incomparable treatise of motion almost ready for the See also:press," and that the law of the inverse square " is the principle on which Mr Newton has made out all the phenomena of the See also:celestial motions, so easily and naturally, that its truth is past dispute." At the next meeting of the Society, on the 28th of April, " Dr See also:Vincent presented to the Society a See also:manuscript treatise entitled Philosophiae Naturalis Principia Mathematica, and dedicated to the Society by Mr Isaac Newton." Although this manuscript contained only the first book, yet such was the confidence the Society placed in the author that an order was given " that a letter of thanks be written to Mr Newton; and that the See also:printing of his book be referred to the consideration of the council; and that in the meantime the book be put into the hands of Mr Halley, to make a See also:report thereof to the council." Although there could be no doubt as to the intention of this report, yet no step was taken towards the publication of the work . At the next meeting of the Society, on the loth of May, some dissatisfaction seems to have been expressed at the delay, as it was ordered " that Mr Newton's work should be printed forthwith in See also:quarto, and that a letter should be written to him to signify the Society's resolutions, and to desire his opinion as to the See also:print, See also:volume, cuts and so forth." Three days afterwards Halley communicated the See also:resolution to Newton, and stated to him that the printing was to be at the See also:charge of the Society .
At the next meeting of the council, on the 2nd of June, it was again ordered " that Mr Newton's book be printed," but, instead of sanctioning the resolution of the general meeting to print it at their charge, they added " that Mr Halley undertake the business of looking after it, and printing it at his own charge, which he engaged to do."
In order to explain to Newton the cause of the delay, Halley in his letter of the 22nd of May alleges that it arose from " the See also:president's attendance on the See also:
That what he told me of the duplicate proportion was erroneous, namely, that it reached down from hence to the centre of the earth
.
" That it is not candid to require me now to confess myself, in print, then ignorant of the duplicate proportion in the heavens; for no other reason, but because he had told it me in the case of projectiles, and so upon mistaken grounds, accused me of that ignorance
.
That in my answer to his first letter I refused his correspondence, told him I had laid philosophy aside, sent him only the experiment of projectiles (rather shortly hinted than carefully described), in compliment to sweeten my answer, expected to hear no further from him; could scarce persuade myself to answer his second. letter; did not answer his third, was upon other things; thought no further of philosophical matters than his letters put me upon it, and therefore may be allowed not to have had my thoughts of that kind about me so well at that time
.
That by the same reason he concludes me then ignorant of the rest of the duplicate proportion, he may as well conclude me ignorant of the rest of that theory I had read before in his books
.
That in one of my papers writ (I cannot say in what year, but I am sure some time before I had any correspondence with Mr Oldenburg, and that's above fifteen years ago), the proportion of the forces of the planets from the sun, reciprocally duplicate of their distances from him, is expressed, and the proportion of our gravity to the moon's conatus recedendi a centro terrae is calculated, though not accurately enough
.
That when Hugenius put out his Horol
.
Oscil., a copy being presented to me, in my letter of thanks to him I gave those rules in the end thereof a particular See also:commendation for their usefulness in Philosophy, and added out of my aforesaid paper an instance of their usefulness, in comparing the forces of the moon from the earth, and earth. from the sun; in determining a problem about the moon's phase, and putting a limit to the sun's See also:parallax, which shews that I had then my See also:eye upon comparing the forces of the planets arising from their circular motion, and understood it; so that a while after, when Mr Hooke' propounded the problem solemnly, in the end of his See also:attempt to prove the motion of the earth, if I had not known the duplicate proportion before, I could not but have found it now
.
Between ten and eleven years ago there was an See also:hypothesis of mine registered in your books, wherein I' hinted a cause of gravity towards the earth, sun and planets, with the dependence of the celestial motions thereon; in which the proportion of the decrease of gravity from the superficies of the planet (though for brevity's See also:sake not there expressed) can be no other than reciprocally duplicate of the distance from the centre
.
And I hope I shall not be urged to declare, in print, that' I understood not the obvious mathematical See also:condition of my own hypothesis
.
But, See also: Mr Hooke found less of the proportion than Kepler of the ellipsis . " There is so strong an objection against the accurateness of this proportion, that without my demonstrations, to which Mr Hooke is yet a stranger, it cannot be believed by a judicious philosopher to be any where accurate . And so, in stating this business, I do pretend to have done as much for the proportion as for' the ellipsis, and to have as much right to the one from Mr Hooke and all men, as to the other from Kepler; and therefore on this account also he must at least moderate his pretences . The proof you sent me I like very well . I designed the whole to consist of three books; the second was finished last summer being short, and only wants transcribing, and See also:drawing the cuts fair]'' . Some new propositions I have since thought on, which I can as well let alone . The third wants the theory of comets . In autumn last I spent two months in calculations to no purpose for want of a good method, which made me afterwards return to the first book, and enlarge it with divers propositions, some See also:relating to comets, others to other things, found out last winter . The third I now-See also:design td sup-press . ' Philosophy is such an impertinently litigious See also:lady, that a man has as good be engaged in lawsuits, as have to do with her . I found it so formerly, and now I am no sooner come near her again, but she gives me warning . The two first books, without the third, will not so well See also:bear the See also:title of Philosophiae Naturalis Principia Mathematics; and therefore I had altered' it to , this, De . Motu Corporum libri duo . " But, upon second thoughts, I retain the former title . 'See also:Twill help the See also:sale of the book, which I ought not to diminish now 'tis yours . The articles are, with the largest, to be called by that name; if you please you may change the word to sections, though it be not material . In the frst page, I have struck out the words ' uti posthac docebitur,' as referring to the third book; which is all at present, from your affectionate friend, and humble servant, " IS . NEWTON." On the 29th of June 1686 Halley wrote to Newton:—" I am heartily sorry that in this matter, wherein all mankind ought to acknowledge their obligations to you, you should meet with anything that should give you unquiet "; and then, after an account of Hooke's claim to the discovery as made at a meeting of the Royal Society, he concludes: " But I found that they were all of opinion that nothing thereof appearing in print, nor on the books of the Society, you ought to be considered as the inventor . And if in truth he knew it before you, he ought not to blame any but himself for having taken no more care to secure a discovery, which he puts so much value on . What application he has made in private, I know not; but I am sure that the Society have a very great satisfaction, in the honour you do them, by the See also:dedication of so worthy a treatise . Sir, I must now again beg you, not to let your resentments run so high, as to deprive us of your third book, wherein the application of your mathematical doctrine to the theory of comets and several curious experiments, which, as I guess by what you write, ought to compose it, will undoubtedly render it acceptable to those, who will See also:call themselves Philosophers without Mathematics, which are much the greater number . Now you approve of the character and paper, I will push on the edition vigorously . I have sometimes had thoughts of having the cuts neatly done in wood, so as to stand in the page with the demonstrations . It will be more convenient, and not much more charge .
If it please you to have it so, I will try how well it can be done; otherwise I will have them in somewhat a larger See also:size than those you have sent up.—I am, Sir, your most affectionate humble servant, E
.
See also:HAL.LEY."
On the 3oth of June 1686 the president was desired by the council to license Newton's book, entitled Philosophiae Naturalis Principia Mathematica
.
On the 14th of July 1686 Newton wrote to Halley approving of his proposal to introduce woodcuts among the letterpress, stating clearly the different things which he had from Hooke, and adding, " And now having sincerely told you the case between Mr Hooke and me, I hope I shall be free for the future from the prejudice of his letters
.
I have considered how best to compose the present dispute, and I think it may be done by the inclosed scholium to the See also:fourth proposition." This scholium was—" The inverse law of gravity holds in all the celestial motions, as was discovered also independently by my countrymen Wren, Hooke and Halley." After this letter of Newton's the printing of the Principia was begun
.
The second book, though ready for the press in the autumn of 1686, was not sent to the printers until March 1687
.
The third book was presented to the Society on the 6th of April 1687, and the whole work published about midsummer in that year
.
It was dedicated to the Royal Society, and to it was prefixed a set of Latin hexameters addressed by Halley to the author
.
The work, as might have been expected, caused a great deal of excitement throughout See also:Europe, and the whole of the impression was very soon sold
.
In 1691 a copy of the Principia was hardly to be procured
.
While Newton was writing the second and third books of the Principia, a very important event occurred at Cambridge which had the effect of bringing him before the public in a new light
.
James II. had already, in 1686, in open violation of the law, conferred the deanery of Christ See also: |
|
|
[back] SIR CHARLES THOMAS NEWTON (1816-1894) |
[next] NEWTOWN |
There are no comments yet for this article.
Do not copy, download, transfer, or otherwise replicate the site content in whole or in part.
Links to articles and home page are encouraged.