* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
Download Rotational Motion - SFA Physics and Astronomy
Routhian mechanics wikipedia , lookup
Hunting oscillation wikipedia , lookup
Inertial frame of reference wikipedia , lookup
Theoretical and experimental justification for the Schrödinger equation wikipedia , lookup
Jerk (physics) wikipedia , lookup
Tensor operator wikipedia , lookup
Classical mechanics wikipedia , lookup
Coriolis force wikipedia , lookup
Photon polarization wikipedia , lookup
Laplace–Runge–Lenz vector wikipedia , lookup
Accretion disk wikipedia , lookup
Symmetry in quantum mechanics wikipedia , lookup
Moment of inertia wikipedia , lookup
Modified Newtonian dynamics wikipedia , lookup
Fictitious force wikipedia , lookup
Center of mass wikipedia , lookup
Seismometer wikipedia , lookup
Newton's theorem of revolving orbits wikipedia , lookup
Relativistic mechanics wikipedia , lookup
Centrifugal force wikipedia , lookup
Angular momentum operator wikipedia , lookup
Angular momentum wikipedia , lookup
Rotational spectroscopy wikipedia , lookup
Work (physics) wikipedia , lookup
Equations of motion wikipedia , lookup
Classical central-force problem wikipedia , lookup
Relativistic angular momentum wikipedia , lookup
Centripetal force wikipedia , lookup
Rotational Motion In this chapter the motion is constrained to move in a circular path. It is very much like the chapter on linear motion in that the object can only move in one of two directions, clockwise or counterclockwise. We will form motion descriptors like we did for linear motion. Motion Descriptor Distance (x) Speed (v) Acceleration (a) Just as v Units meters m/s m/s2 Rotational Descriptor Angular Distance () Angular Velocity () Angular Acceleration () Units rad rad/s rad/s2 x v , so . Similarly, a becomes . t t t t Angular velocity and acceleration are vectors. To determine the direction of each, curl the fingers of your right hand in the direction of rotation. Your right thumb then points in the direction of or . Basic kinematical equations can be developed for pure rotation as a result of the equivalences in the table above. So we get o o t 1 2 t 2 o t We learned that inertia is a property of matter that resists changes in motion and that inertia is identical to mass. When the motion is pure rotation, the equivalent concept is rotational inertia, the property of an object that resists changes in rotation. We measure rotation inertia with the moment of inertia (I). I depends on the object’s mass and mass distribution, and the axis of rotation. The easiest to compute is the mass on a string. Make the axis of rotation a distance r away from the mass and the moment of inertia is I = mr2. Other shapes and rotational axes require the use of calculus, but all take the form I = f(mr2), where f is a fraction less than one. Remember the basic definition of inertia here and many situations become clear. Torque is the product of force ( F ) and lever arm ( d ). F d Notice that torque is also a vector. The operation is often called the vector (or cross) product. The general rules for finding the lever arm are: 1. Draw in the line of action of the force. This is a line through the force extending in both directions. 2. Locate the axis of rotation (pivot point). 3. The lever arm is the shortest distance from the axis to the line of action. Lever Arm Unbalanced torques produce angular accelerations just as unbalanced forces produce linear accelerations. Newton’s Second Law for the pure rotational case looks like I instead of F ma . Newton showed that all of the mass of an object acts as if it were concentrated in a single point called the center of mass. A useful way of finding the center of mass of an object is to take advantage of the fact that gravity can only point vertically. Suspend the object by a point on the edge. If the center of mass is not along the vertical line through the point of support, then a torque exists and the object rotates. When the center of mass does fall along this line (the line of action for the body’s weight), the lever arm drops to zero and no torque exists. Repeat this test for one or more other suspension points and you can quickly find the center of mass. An object is stable against rotations if the vertical line through the center of mass strikes the base of support. Centripetal force is any force that causes the object to move in a circle. The word literally means “center seeking” and can be provided by many different forces or force combinations. Using Newton’s Second Law, we can write Fc = mac = mv2/r = mr2. “Centrifugal (center fleeing) force” is a fictitious force experienced by an object located in an accelerated reference frame. As viewed from the outside of the system, these “centrifugal forces” can be seen to be simple applications of Newton’s First Law. As an example, while taking a turn in your car, you seem to be push away from the center of the circle through which you are turning. But you are trying to move in a straight line as dictated by the 1st Law and the outer car door is forcing you to turn. As it presses against you, you also press against it, and it feels like a force. Sometimes we can take advantage of the centrifugal force. In the future when we build space habitats that rotate with constant , the occupants experience an outwardly directed “force.” They would feel pressed against the outer rim of the habitat and would experience the sensation of weight due to this force. The centripetal force is proportional to r2 and would be greater the farther from the center the occupant lives. This simulated gravity would, therefore, vary with radius in the habitat, being zero right at the center. Angular momentum is the rotational equivalent to linear momentum. Since p mv , we can write angular momentum as L I . The direction of L is the same as the direction of given by the right hand rule. Recall that an alternate form of Newton’s 2nd p Law is F and that from this we defined impulse as t L and thus p F t . We now realize that in the purely rotational case t rotational impulse is L t . In systems where there are no external torques ( = 0), angular momentum must by conserved (L = 0). Look over the various examples of angular momentum conservation to see this principle in action. For example, the inside of the barrel of a gun has a heliacal groove cut into it called rifling. The purpose of the rifling is to make the bullet rotate. Once the shell is ejected angular momentum is conserved. The vector of angular momentum does not want to change, making the flight truer. Without the rotation the shell would tend to tumble. The same arguments apply to throwing a football. Rotational physics can be approached from the point of view of substitution of variables into the equivalent linear equations. Below is a table of such substitutions