A classical mechanics problem by Abdullah Faysal

An inventor designs a pendulum clock using a bob with mass 200 g at the end of a thin wire of length 23 cm. Instead of swinging back and forth, the bob is to move in a horizontal circle, making a fixed angle 27° with the vertical. This is called a conical pendulum because the suspending wire traces out a cone. Find the period T T of this pendulum.

Note: Use π = 3.1416 \pi = 3.1416 and g = 9.81 g = 9.81 m/s 2 ^2 .

0.908s 1.009s 0.443s 0.777s

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2 solutions

Btari Elizabeth
Dec 3, 2014

T = 2 π L cos θ g = 2 ( 3.14 ) 0.23 cos 2 7 9.81 = 0.908 [s] . T=2π \sqrt{\frac{ L \cos \theta}{g}}=2(3.14) \sqrt{\frac{ 0.23 \cos 27^\circ}{9.81}}=0.908\text{ [s]}.

where is m in this formula?

Deniz SAVAS - 4 years, 5 months ago

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m/k = l/g

Sub into T=2 pi sqrt (m/k)

dhbc bvbbj - 3 years, 6 months ago

In a pendulum m(the mass) doesn't have an effect on the period, essentially because gravity acts the same on all masses.

Mustafa Alsaket - 6 months, 1 week ago

Can someone please explain? Why does Lcosθ work in place of L?

A Former Brilliant Member - 4 years, 5 months ago

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By resolving the forces

Bazmi Farooquee - 4 years, 4 months ago

you have to resolve the length. If you can diagrammatically explain it you'll have no problem

marcy lengar - 2 years ago
Amir Adala
Feb 17, 2019

Let l l be the length of the wire and θ \theta the angle it does with the vertical. The trajectory of the pendulum describes a circle or radius r = l s i n ( θ ) r=lsin(\theta) . We can define e r e_r to be the unit vector directed along the radius and e z e_z the vertical component, perpendicular to e r e_r .

First let's project the forces on the axes. There's T T the tension of the wire and W = m g W=mg the weight of the pendulum. The z z -component of the tension exactly compensates the weight (since the pendulum doesn't move along the z-axis to keep θ \theta constant), so we get T = m g / c o s ( θ ) T= mg/cos(\theta) . Hence, the r r -component of T T is T r = m g t a n ( θ ) T_r= -mgtan(\theta) .

We then apply Newton's second law: m m a = m g t a n ( θ ) mgtan(\theta) e r e_r . Since the speed in polar coordinate is v = r d θ / d t v = r d \theta /dt and r r is constant, a = v 2 / r a = v^2/r . Thus we have v = g r t a n ( θ ) v= \sqrt{grtan(\theta)} . The oscillation period is given by the perimeter of the circle divided by the speed: T = 2 π r / v T=2\pi r/v .

With θ = 27 ° \theta = 27° and l = 0.23 m l = 0.23 m we have T 0.9085 s T \approx 0.9085 s

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