*¡Adios, Sapito!*In this iconic cinematic moment from

*Raiders of the Lost Ark*(Lucasfilm, Paramount Pictures, 1981), Indiana Jones outruns a gigantic round boulder. Somehow I don't think the principle of energy conservation was on his mind at the moment, but it ought to have been.

*v*while rotating with an angular speed ω.

*v*and angular speed ω are constrained via the "rolling without slipping" condition

*v*=

*r*·ω, so an object with a radius

*r*that has a slow or fast translational speed must also be rolling with a corresponding slow or fast angular speed. (Note the peculiar nature of the radians unit, where it conveniently disappears on the right-hand side of the equation such that

*v*results in units of meters per second.)

Here two objects with different radii have the same translational speed

*v*, but from the

*v*=

*r*·ω condition, the larger

*r*radius object has a slower ω angular speed as it rolls, while the smaller

*r*radius object has a faster ω angular speed in order to keep up.

*v*and angular speed ω are related, there is a relationship between the mass

*M*and the rotational inertia

*I*of an object. Whereas an object's mass is a measure of how easy or difficult it is to change its translational motion, an object's rotational inertia (also known in more obscure calculus terminology as the "moment of inertia") measures the distribution of mass about its axis that makes it easy or difficult to change its rotational motion. The rotational inertia depends on the mass, size, and configuration of the object, and the appropriate expressions for rotational inertia should be used for each type of rotating object.

*M*swung around in a circle of radius

*R*; its moment of inertia is given by

*I*=

_{point mass}*M*·

*R*

^{2}. (Video link: "2010 Asian Games - Men's Hammer Throw Final.")

*M*and length

*L*that is swung around at one end, its moment of inertia is given by

*I*= (1/3)·

_{rod, at end}*M*·

*R*

^{2}. (The numerical factor of (1/3) for this object comes from calculus, but for the purposes of this course these numerical factors are merely to be looked up for each different type of object as needed.) (Video link: "2013 MLB Home Run Derby Extreme Slow Motion Swings.")

*KE*is the energy of rotational motion. Rotational kinetic energy depends on the rotational inertia

_{rot}*I*and the square of the angular speed ω of the object, and the resulting units of kg·m

^{2}/s

^{2}are also expressed as joules (once the peculiar units of rad

^{2}disappear). A object that is not rotating has no rotational kinetic energy, and the faster an object rotates, the more rotational kinetic energy it has.

Instead of finding out how much rotational kinetic energy

*KE*an object has, often we are more concerned with its initial-to-final change

_{rot}*KE*, which is the final amount of rotational kinetic energy minus the initial amount of rotational kinetic energy. Notice how the common factors of (1/2) and rotational inertia

_{rot}*I*(which is presumed to be constant) are pulled out, leaving a "difference of squares" for the final and initial angular speeds in the parenthesis.

*KE*will be given by (1/2)·(

_{tr}*M*+

_{rider}*m*)·

_{wheel}*v*

^{2}, and the rotational kinetic energy

*KE*will be given by (1/2)·

_{rot}*I*·ω

_{wheel}^{2}. (Video link: "Riding the Solowheel to work - every days obstacle course.")

Note that the two kinetic energy expressions are not unrelated as the Solowheel rolls without slipping, such that the constraint

*v*=

*r*·ω can be used to connect the translational speed

*v*in the translational kinetic energy expression with the angular speed ω in the rotational kinetic energy expression. We'll demonstrate this connection in some examples of objects that roll without slipping during lecture.

As discussed previously, in the idealized case that there are no non-conservative forces (such as friction, drag, or from external sources), then the left-hand size of this equation would be zero. Then the individual energy terms on the right-hand side of this equation can then trade and balance amongst themselves, instead of with the outside world.

So now let's see how this more comprehensive transfer/balance equation can be applied to idealized situations where friction and drag are negligible.

Assuming that there is no friction/drag (such that we can neglect non-conservative work), which energy system experienced a greater amount of change (whether increase or decrease) for this process: translational kinetic energy, rotational kinetic energy, or gravitational potential energy?

Assuming that there is no friction/drag (such that we can neglect non-conservative work), which energy system experienced a greater amount of change (whether increase or decrease) for this process: translational kinetic energy, rotational kinetic energy, or gravitational potential energy?

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