Newtons Principia the Mathematical Principles of Natural Philosophy

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M. The comet in R lay exactly in a line be tween the stars K and C, so as the part CR of the right line CRK was a little greater than CK, and a little less than JCK + jCR, and therefore = iCK + A CR, or if CK.
Wednesday, March 2, S 1 . P. M. The distance of the comet in S from the star C was nearly FC ; the distance of the star F from the right line OS produced was g^FC ; and the distance of the star B from the same right line was five times greater than the distance of the star F ; and the rig
...ht line NS produced passed between the stars H and I five or six times nearer to the star H than to the star I.
Saturday, March 5. LH h . P. M. When the comet was in T, the right line MT was equal to ^ML, and the right line LT produced passed between B and F four or five times nearer to F than to B, cutting off from BF a fifth or sixth part thereof towards F : and MT produced passed on the outside of the space BF towards the star B four times nearer to the star B than to the star F. M was a very small star, scarcely to be seen by the tele scope; but the star L was greater, and of about the eighth magnitude.


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