Hence the side (s) of the octagon being the chord of a, is expressed by =R × √ 2, if instead of being = unity the radius of Re √3, and the distance of the face from the centre, or the 2 altitude of the equal prisms whose bases are the equal faces of the octaedron and common vertex at the centre, is 174. Let b be the radius of the base common to the hemis pheroid (H) and paraboloid (P), and A their height, then 175. Let PQ (Fig. 69,) the transverse axis of the ellipse =2a, and its conjugate (to be determined) = 26, and put ▲ ABC = T, ▲ APQ = T, cone ABC = C, and segment APQ = C', then C: C :: T3 : Tẻ... For since PQ is the axis of the ellipse, its plane is plane ABC which passes through the axis of the cone. Hence pm being the intersection of the O B'C' with the ellipse PQ, and B'C' that with the plane ABC, it is easily shewn that pm2 B'm x m°C. being the perpendiculars let fall from A upon BC and PQ respec and the area of the ellipse is .. expressed by Now it is evident that C' may be decomposed into triangular prisms of the same altitude p', and the limit of the sum of whose C = = P √TT = T√T ..... (1) Again, to find the equation to the surface of the cone, we will suppose the rectangular axes of x, y, z, to originate in its vertex, and the axis of z to be that of the cone itself, as in Fig. 69. Then, L being any point in the surface, let OLA be that position of the generating ▲ in which it passes through L, and draw LN 1 AZ, LL' plane of (x, y,) and L'MAX. Let, therefore, AN=z, AM= x, and L'M=y, and we have Z: NL = AL' = √ x2 + y2 :: OA : OC :: 1 : tan. A being the angle at the vertex of the cone. .. Z x tan. = √x2 + y2 A 2 the equation of the surface of the cone, whose rectangular co-ordinates originate in its vertex, and that of z coincides with its axis, which, in practice, will be found the most commodious way of considering the question. THE RECTIFICATION OF CURVES. 176. This is a particular case of the Theorem of Fagnani, which we will first demonstrate generally. Let 1, and b, be the semi-axes of the ellipse, and e its eccentricity, Then the equation of the curve referred to the centre by rectangular co-ordinates x, y, is y = b √1−x3. Hence, denoting by E, that part of the elliptic arc measured from the extremity of b, whose abscissa is x, we have E1 = √ dx √/1+ dy2 = ƒ dx √2=; and putting dx2 e2 x2 1 - x2 |