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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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2This rather clumsy formula is a c<strong>on</strong>sequence of following the Babyl<strong>on</strong>ians in defining the unit of angle as1/360 of a full circle. We’d have a much nicer formula if instead we defined our unit of angle as 1/2π ofa full circle!So we define: the radian = 1/2π of a full circle. This works out to be about 57.3°, <strong>and</strong> since thecomplete circumference of a circle is 2πr, the distance around the circle corresp<strong>on</strong>ding to an angle of<strong>on</strong>e radian is <strong>on</strong>e radius. Duh.Angle of <strong>on</strong>e radianthe red solid arc has lengthequal to the radius of the circle.sinθ ≈ θ for θ smallfor r = 1, the arc length is θ,the short black line = sinθ.It’s easy to see that radians are the natural angle unit for trig: look at the sine of a small angle.Our default notati<strong>on</strong> for an angle is θ, measured from the x-axis, with counterclockwise as positive.Angular velocity in radians per sec<strong>on</strong>d will usually be denoted by ω: d/ dt.So if a wheel is rotating at positive angular velocity ω radians per sec<strong>on</strong>d about a fixed axle, a point <strong>on</strong>the wheel at distance r from the axle is moving at speeda formula we’ll be using a lot.vr2 2The st<strong>and</strong>ard notati<strong>on</strong> for angular accelerati<strong>on</strong> is d / dt d / dt .Notice that if we have c<strong>on</strong>stant angular accelerati<strong>on</strong>, formulas for angular velocity <strong>and</strong> angulardisplacement (meaning angle turned through) are just like those for linear moti<strong>on</strong> under c<strong>on</strong>stant force:

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