<28r>

Cambridge.
December 10th 1672.

Sr

My unwillingness to trouble you in the midst of yor late d|b|uisiness made me suspend writing, though I stood obliged to thank you for the rest of Mr Horrox works wch I received some weeks since. But by yors wch I received two days since I presume the most of that trouble is over. I am heartily glat|d| at the acceptance wch or Reverend friend Dr Barrow's Lectures finds wth forreign Mathematicians, & it pleased me not a little to {illeg}|un|derstand that they are falln into the same method of drawing Tangents wth me. if What I guess their method to be you will apprehend by this example. Suppose CB applyed to AB in any given angle be terminated at any Curve line AC, and calling AB x & BC y let the relation between x & y be expressed by any æquation as ${x}^{3}-2xxy+bxx-bbx+byy-{y}^{3}=0$ whereby the curve is determined. To draw the tangent CD the Rule is this. Multiply the termes of the æquation by any arithmeticall progression according to the dimensions of y suppose thus $\begin{array}{ccccccccccc}{x}^{3}& -& 2xxy& +& bxx& -& bbx& +& byy& -& {y}^{3}\\ 0& & 1& & 0& & 0& & 2& & 3\end{array}$ {illeg}, also according to the dimensions of x suppose thus $\begin{array}{ccccccccccc}{x}^{3}& -& 2xxy& +& bxx& -& bbx& +& byy& -& {y}^{3}\\ 3& & 2& & 2& & 1& & 0& & 0\end{array}$. The first product shall be the Numerator, & the last divided by x the Denominator of a fraction wch expresseth the length of BD to whose end D the tangent CD must be drawn. The length BD therefore is $\frac{-2xxy+2byy-3{y}^{3}}{3xx-4xy+2bx-bb}$.

This Sr is one particular, or rather a Corollary of a Generall Method wch extends it selfe wthout any troublesome calculation, not onely to the drawing tangents to all curve lines whether Geometrick or mechanick or how ever related to streight lines or to other curve lines but also to the resolving other abstruser kinds of Problems about the crookedness, areas, lengths, centers of gravity of curves &c. Nor is it (as Huddens method de maximis et minimis & consequently Slusius his new method of Tangents as I presume) limited to æquations wch are free from surd quantities. This method I have interwoven wth that other of working in æquations by reducing them to infinite series. I remember I once occasionally told Dr Barrow when he was about to publish his Lectures that I had such a meth{illeg}|o|d of drawing Tangents but some divertisment or other hindered me from descr {sic}bing it to him.

Of resolving by Cardans rules Equations that have 3 possible roots there may be examples framed at pleasure, but unlesse b|B|rasser show a direct method of performing it, wch Ferguson doth not, it will not be allowed scientifick. How it is to be done directly I may possibly show upon occasion.

The next disadvantage arising from the distance of the little speculum from the eye-glass being allowed I pass to ye {illeg}|l|ast wch is to this effect, That if to diminish the magnifying virtue of the instrument the little speculum be made of a larger sphære, whose center is infinitely distant (as it is in Mr Gregories designe, a plane being equivalent to a sphære whose center is infinitely distant,) that would cause too many of the best rays to be intercepted. And though in his designe scarce a fourth part of the whole light be intercepted yet those rays seem to me of more value then twice their number next the circumference of ye Tube, because they principally conduce to distinct vision. Their loss will be judged considerable by those that have thought the loss of scarce the fort{illeg} fortieth part of the light in my way worthy of being objected by reason that the{illeg}|y| \were the/ best of the rays.

There are yet other considerations by which Mr Gregory's Tube may perhaps be thought less advantageous, as that unless the speculum F be made so broade as to intercept more then a quarter or perhaps then a third part of the whole light, it will be difficult to inlarge the aperture as is requisite for viewing dull & obscure objects. That the eye-glass if placed at the bottom will scarcely be well defended from the unusefull glareing light wch in the day time comes from objects on all sides the flat speculum, at least not so well as by setting it {illeg}|at| the side. And that an Artificer can scarcely polish the great concave so truly when perforated in the middle. For the metall neare that hole will be apt to weare away too fast as it doth neare the exterior limb. And though the hole may be made after tis polished, yet if the figure happen to be less true, or if afterwards the metall chance to tarnish, it must be polished again.

As for the advantages propounded by Mr Gregory I see not why the first should be recconed for one, viz: That the distance EF groweth almost the one half less & therefore the errors of the concave CD are also diminished upon the plane F by one half. For how much those errors of the concave CD are increased or diminished is to be estimated by the prevarication of the rays not at the plane F but at the Focus of that concave CD. And there the errors in both cases will be alike, provided the speculum F be accurately plane, but if there be any irregularities in the figure of that speculum F they will cause errors so much greater in one case then in the other, as that speculum is remoter from the eye-glass, wch in large Telescopes may be more then 15 or 20 times.

The other advantage, viz: That his Tube will be little more then half the length of mine I should allow to be very considerable, if I thought that wth equall art in the mechanism it {illeg}|c|ould be made to doe the same effect. The greatest difficulty is in forming the great Concave, wch when once well done, perhaps it may be thought most advantageous to make the best use of it though with a longer Tube.

The propounded \supposed/ advantage of Telescopes wth convex or concave speculums in that they may have any desirable charge by altering the distances of the eye-glass & specula, agrees more conveniently to my design of the instrument if that speculum be made use of wch I described in a letter to Mr Oldenburg in answer to Monsr Auzouts considerations on these instruments, wch possibly you may have seen. For instance to double the charge the eye-glass in the other way must be drawn out almost as far behind the great concave as the little speculum is before it, whereby the length of the Tube will be almost doubled whereas in my way it need be drawn out no farther from the side of the Tube then a quarter of the Tubes diameter. The charge may be also conveniently varied by having two or three eye-glasses of severall depths set in a girdle, any of wch may be adjusted to the metall F by sliding that girdle about the Tube or by sliding the ring within the Tube to wch that girdle \metall F/ is fastened.

That Telescopes by convex or concave speculums should be overcharged is not necessary but yet it is not avoydable without running upon one of the other two inconveniences described in the 7th particular of my considerations on M. Cassegrains Tube, as I there intimated.

<29r>

To diminish some of the afforesaid disadvantages there may be other still new variations or additions to these designes. As for instance by using two eye-glasses. Suppose CD represent the great Concave, F the little speculum E the eye-glass & G another double-convex glass between E & F on both sides of wch the rays cross. This way of redoubling these Tubes seems not inferior to the rest. For thus the object appeares erect, the speculum F intercepts less light, & the charge may be varied at pleasure onely by changing the positions of G & F. But yet this is not wthout its imperfections, & particularly the {illeg}(besides those common wth the other Designes) the glass G will intercept many of the best rays in their passage from the concave CD to ye little speculum F, unless it be made less then is consistent wth some other conveniences. And by the iterated decussations of the rays objects will be rendered less distinct, as is manifest in Dioptrick Telescopes where two or three eye-glasses are applyed to erect the object.

As to the attempt in wch Mr Rieve was imployed, I presumed it had been done wth much more accurateness then Mr Gregory now signifys, because Mr Hook, who you know is a curious & accurate experimenter, affirms in his considerations on my letter to Mr Oldenburg concerning refractions & colours published in the Transactions Numb 80, that he made severall experiments wth that Instrument. And though he lays the blame on Mr Rieve's encheiria, yet he says not yt he blamed him then when the Experiment was made. His words are these

" I have made many tryalls both for Telescopes & Microscopes by reflexion wch I have mentioned in my Micrographia, but deserted it as to Telescopes when I con sidered that the focus of a sphericall concave is not a point but a line, & that the rays are less true reflected to a point by a Concave then refracted by a Convex, wch made me seek that by refraction wch I found could not be ex pected from reflexion. Nor indeed could I find any effect of it by one of six foot radius wch about 7 or 8 yeares since Mr Rieve made for Mr Gregory wth wch I made severall tryalls; but it now appeares that it was for want of a good encheiria; From wch cause many good experiments have been lost. Both wch considerations discouraged me from attempting further that way; especially since I found the Parabola much more difficult to describe then the Hyperbola or Ellipsis.

From hence I might well infer that ye want of a good encheiria appeared not till now. And that Mr Hook was discouraged from attempting further that way onely by these two \or three/ considerations, That a Convex (as he presumes) refracts more truly then a concave reflects, {illeg} that he found no effect by one of six foot radius, wch {illeg} till now he attributed to some other cause then the want of a good encheiria, as perhaps to the un |namely to the supposedly less| true reflexion of a sphæricall concave, & {illeg} \he supposed apprehended a/ {gr}eater difficulty of describing a Parabola then an Hyperbola or Ellipsis. Nor could I well interpret the cause from {*} |* from wch many {good} experiments have been lost to have been other then the want of a good encheiria wch till afterwards appears not to have been wanting. I contend not that this was Mr Hooks meaning, but onely that his words seemed to import thus much, which gave me occasion to think there was no diligence wanting in making that experiment, especially since he expresseth that he made severall tryalls wth it.|

And that you may not think I strained Mr Gregory's sense where he spake of Hyperbolick & Elliptick Glasses & Speculums attempted in vain; I would ask to what end those Speculums were attempted if not to compose optiqꝫ Instruments wch is all I would infer from those words. For that those instruments if at all attempted were attempted in vain is evident by the want of success.

This Sr I have said not that I desire to discourage the tryall of any practicable way or to contend wth Mr Gregory about so slender a subject \difference/. For I doubt not but when he wrote his Optica promota he could have described more fashions then one of these Telescopes & perhaps have run through all the possible cases of them if he had then thought it worth his paines. Because M. Cassegrain propounded his supposed invention pompously, as if the main buisini|e|ss was in the contrivance of these \instruments/ I thought fit to signify that that was none of his contrivance, nor so advantageous as he imagined. And I have now sent you these further considerations <29v> on Mr Gregory's answer onely to let you see that I chose the most easy & practicable way to make the first tryalls. Others may try other ways. Nor doe I think it materiall wch way these instruments are perfected so they be perfected.

You will pardon this long scribble in wch I have been the more particular because Mr Gregory's discours looks as if intended for the Press. We are here very glad that we shall enjoy Dr Barrow again especially in the circum{illeg}|st|ances of a Master, nor doth any rejoyce at it more then Sr

Yor obliged humble Servant

Newton.

I suppose Slusius his method of Tangnts will shortly appear abroad, when it comes over I'le beg of you the trouble of transmitting a coppy to me if you will give me leave to be accountable to you for it.

< insertion from f 29v >

Scripsi ad te jam sæpius de Regula ducendarum tangentium ad curvas quaslibet geometricas absque omni Calculo quam publico dare decreveram, sed absolvere, quæ animo Conceperam, hactenus non licuit, Ejus enim usum tum in Determinatione Problema tum, tum in pluribus aliis ostendere volebam quorum aliqua ni fallor tibi antehac indicavi, Verum cum nec mihi nunc Otium sit, decrevi si ita videatur Regulam absqꝫ demonstratione et Corollarys (ne moles nimia sit) ad te mittere Transactionibus Philosophicis inserendam quo virorum doctorum censuram Subjre possit, fac igitur me certiorem quid ea de re censeas, ego enim Judicio tuo parebo Libenter, eamqꝫ cum tibi placere indicaveris statim transmittam.

< text from f 29v resumes > < insertion from the right margin >

Mr Newton about Tellescopes with his Method of Tangents

< text from f 29v resumes > < insertion from the right margin >

To Collins. {1{illeg}} Dec. 10. 1{illeg}|6|72.

< text from f 29v resumes >

Professor Rob Iliffe
Director, AHRC Newton Papers Project

Scott Mandelbrote,
Fellow & Perne librarian, Peterhouse, Cambridge

Faculty of History, George Street, Oxford, OX1 2RL - newtonproject@history.ox.ac.uk

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