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By J. F. Scott (ed.)

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0. 22 21 20 1 0. 18 63 71 72 73 74 75 0. 0. 0. 0, 17 16 15 14 0. 0. 0. 0. 0. 51 49 48 46 44 76 77 78 79 80 0. 0. 0. 0. 0. 12 11 10 43 41 40 38 37 81 82 83 84 85 0. 8 0. 0. 0. 0. 7 66 0. 0. 0. 0. 0. 56 57 58 59 60 0. 0. 0. 0. 0. 36 34 33 32 30 1. 1. 1. 1. 24 21 59 57 66 68 86 87 88 89 90 0. 0. 0. 0. 0. 23 19 13 9 6 5 5 4 3 2 1 0 NOTES (1) (2) (3) (4) 48 4 jiS G. 361, no. 53. The date has been added by Flamsteed. See Letter 477 and the Table of Refractions which accompanied it. See Letter 476. The third synopsis, and the Table of Refractions.

E J ohn F lamsteed I shall write to you againe as soone as I can get another Synopsis transcribed, at present I am very busy about some other papers I am to send to a philo­ sophical! Freind J F : Mr Halley is busy about ye Moon has promised Me his corrections, intends to print something about her Systeme ere long & affirmes the meane Motion different in ye time of Albatani^^^' from what it is now: J : F : To Mr Isaack Newton Fellow of Trinity Golledg in Gambridg there, these present. Gambridge.

He made accurate measurements of the leng^th of a degree along a meridian. La Mesure de la Terre, Paris (1671). I t was at his suggestion that Richer undertook his expedition to Cayenne (note (16) above). He collaborated with Romer in his observations on the satellites of Jupiter which led to the determination of the velocity of light. M. V. pp. 181-2. (17) In 1675 Romer had noted that the eclipse of the outermost satellite of Jupiter (lo) showed an inequahty in the time of its occurrence, and this he ascribed to the time taken by light in its passage across the Earth’s orbit.

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