A Ferris wheel with radius r is rotating at constant angular speed ω . The position of a passenger at the rim of the wheel may be described by a direction angle θ :
θ = 0 ∘ at the right side of the wheel
θ = − 9 0 ∘ at the bottom of the wheel
θ = + 9 0 ∘ at the top of the wheel
Each passengers sits on a level (horizontal) seat. The coefficient of static friction between passenger and seat is μ . However, the seats are so slippery that the friction is not sufficient to keep the passengers in their seats. Between θ = − 5 ∘ and θ = + 2 5 ∘ they must hold on to a bar to stay in their seats.
If r = 2 0 m , how fast is the wheel turning, in rotations per minute?
(For the acceleration due to gravity, use g = 9 . 8 1 m / s 2 .)
Bonus for those who think this still too easy: Calculate the maximum minimum force the passengers need to exert on the bar. ("Minimum" at any given moment, "maximum" over the entire ride.)
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Solution of Bonus question:
Let S be the force exerted on the bar with direction angle ϕ . The equations for the y - and x -components of force become m ω 2 r sin θ = m g − N + S cos ϕ ; m ω 2 r cos θ = μ N + S sin ϕ , assuming of course that static friction is of maximal help in keeping the passenger in place. Eliminate N : m ω 2 r ( cos θ + μ sin θ ) − S ( cos ϕ + μ sin ϕ ) = μ m g , ω 2 r cos ( θ − ζ ) − m S cos ( ϕ − ζ ) = g sin ζ , with tan ζ = μ .
To minimize S we must maximize cos ( ϕ − ζ ) , i.e. the bar must be pushed in direction ϕ = ζ ; the equation becomes m S = ω 2 r cos ( θ − ζ ) − g sin ζ . This is maximal in the situatin θ = ζ , with value m S ) max = ω 2 r − g sin ζ = g sin ζ ( cos Δ 1 − 1 ) . With the given values, m S ) max = 0 . 0 6 0 N / k g .
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At the given angles θ − = − 5 ∘ and θ + = + 2 5 ∘ , the static friction is maximal: f = μ N .
The net force on a passenger is the centripetal force m ω 2 r . This consists of the downward force of gravity m g , the upward normal force N , and a sideways friction force f . For the y - and x -components we have m ω 2 r sin θ = m g − N ; m ω 2 r cos θ = f = μ N . Eliminate N to find m ω 2 r ( cos θ + μ sin θ ) = μ m g . This we write as ω 2 r 1 + μ 2 cos ( θ − ζ ) = μ g , tan ζ = μ . Because cosine is an even function, the solutions θ lie symmetrically around ζ . Thus ζ = 2 θ + + θ − , Δ = θ − ζ = 2 θ + − θ − . From this we can calculate μ = tan − 1 ζ . Note also that μ / 1 + m u 2 = sin ζ . Thus we obtain the equation ω 2 r = 1 + μ 2 cos Δ μ g = g cos Δ sin ζ , ω = r cos 2 1 ( θ + − θ − ) g sin 2 1 ( θ + + θ − ) .
With the given values ω = 2 0 cos 1 5 ∘ 9 . 8 1 sin 1 0 ∘ = 0 . 2 9 6 9 5 rad / s , and multiplication by 6 0 / π gives ω = 2 . 8 3 5 6 6 rpm .