mass of the oscillating body, k the distance between the centre of gravity and suspension; then the length of the pendulum is r being the radius of the circle, and c the chord, and 7 the length of 613. Generally for n pulleys, let Q, Q..... be their weights; then, the weight sustained is Hence, supposing Q, Q = &c., the inertia arising from the Also the inertia from the descent of Q, Q, &c. is 5 W Let n = 2. Then it is found that the inertia =P+Qx+ Again, let T,, T, . . . . T be the several tensions required, and I, I,.... I, the corresponding inertias; then we have The pressure on each axis is double the tension of the string that goes round it. 614. Let denote the angular distance required, measured from the West, then by the composition of forces, it readily appears that Hence it seems that at sea, when the ship is sailing in a direction oblique to the wind, the position of the vane is no certain criterion as to the quarter from which it blows. It would also appear, at first sight, that the magnet is affected in like manner by the motion of the vessel; but a moment's reflection is sufficient to be convinced of the contrary. The magnet consisting of two equal arms, the action of the ship's motion upon the one is counteracted by its opposite action upon the other. 615. Generally, w being the weight of the cylinder, and the power or weight which puts it in motion, e the radius of the base, and r the distance, then the accelerating force on p is Р P 20, w 133. 6, v = 1, g = 1, r = 10, and it will be found, after substituting and reducing, that t.03214, &c. seconds. 616. Generally, required the length of a pendulum that would oscillate seconds at the distance of n radii of the Earth from its centre. If F be the force which accelerates the pendulum, whose length is L, then the time of an oscillation is got from (see Bridge, vol. II.) Hence, if I be the length of a second's pendulum at the surface of the earth, where g is the accelerating force, we have Within the surface F = gwhence p is easily found. 617. Let a be the distance of the particle dM from the axis of suspension, a the length of the rod, D its density at the lower extremity, L the distance between the point of suspension and centre of oscillation; then L = √x2dM (see Vince, p. 127.) 618. Generally let AC (Fig. 102,) be any curve whatever revolving uniformly round the vertical axis AB, and suppose the body P descending along the curve by the force of gravity; required the velocity of the body at any given epoch t. Let the PM y, AM = x, BC = 6, AB =, and V the known velocity of the point C; then resolving the centrifugal force RP into the tangential and normal ones PQ and RQ, we have PQ PR x cos. RPQ = PR × dy ds Again, the velocity at C being V, that at P is |