Note CXXXIII — THE 'LIVES' (continued 7)

] To[1731] make a demonstration of it, telling him the proportion of the gravity to the distance and the curv'd line that was thereby made, to witt that it was an ellipsis in one of the foci of which was the sun and that that gravitation would make the aphelion and perihelion opposite to each other in the same diameter which is the whole celestiall theorie of which Mr. Newton haz made a demonstration.