Class Notes on Rotational Motion - Galileo and Einstein
Class Notes on Rotational Motion - Galileo and Einstein
Class Notes on Rotational Motion - Galileo and Einstein
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5Torque = force × distance of line of force from pivot = 4mgdsin30 = 2mgd2dangle 30°T = 2mg2dsin30Either way, the formula for torque strength is:Fr sin where F is the magnitude of the force, r the distance from the pivot of the point of applicati<strong>on</strong>, <strong>and</strong> θthe angle between the vector r from the pivot point to where the force acts <strong>and</strong> the force F .Rotati<strong>on</strong>al Equivalent of Newt<strong>on</strong>’s First LawBy the time <strong>Galileo</strong> noticed that a smooth ball <strong>on</strong> a flat surface with little fricti<strong>on</strong> would keep the samevelocity a l<strong>on</strong>g time, it was already known that a rotating grindst<strong>on</strong>e, with a well-oiled axle, would keepspinning a l<strong>on</strong>g time too—<strong>and</strong> this, taken to the ideal limit, is Newt<strong>on</strong>’s First Law for rotati<strong>on</strong>: in theabsence of torque, a body will spin at c<strong>on</strong>stant angular velocity indefinitely.It’s worth menti<strong>on</strong>ing that a vertical grindst<strong>on</strong>e must have the axle through the center of gravity. If thisis not the case, gravity will exert a torque, <strong>and</strong> although the wheel might keep spinning, it w<strong>on</strong>’t be atc<strong>on</strong>stant angular velocity.In fact, the torque <strong>on</strong> such an off-center wheel is given by MgrCMsin MgxCM, where r CM is thedistance of the center of mass from the axle, <strong>and</strong> θ the angle between r CM<strong>and</strong> the vertical.To prove this, imagine the wheel to be made up of a large number of glued-together small masses m i atpositi<strong>on</strong>s r i.