The period of a pendulum is \(0.24 \mathrm{~s}\) on Earth. The period of the same pendulum is found to be 0.48 s on planet \(X,\) whose mass is equal to that of Earth. (a) Calculate the gravitational acceleration at the surface of planet \(X\). (b) Find the radius of planet \(\mathrm{X}\) in terms of that of Earth.

Short Answer

Expert verified
Based on the given information, the gravitational acceleration on planet X is approximately 2.4525 m/s², and the radius of planet X is approximately 1.996 times the radius of Earth.

Step by step solution

01

Finding the gravitational acceleration on planet X

We can use the formula of the period of a pendulum, which relates the period \(T\), the length of the pendulum \(L\), and the gravitational acceleration \(g\). The formula is given by: \(T = 2\pi \sqrt{\frac{L}{g}}\) We are given the periods on Earth (\(T_1 = 0.24\,s\)) and planet X (\(T_2 = 0.48\,s\)). We can set up the ratio between the two: \(\frac{T_1}{T_2} = \frac{2\pi \sqrt{\frac{L}{g_1}}}{2\pi \sqrt{\frac{L}{g_2}}}\) where \(g_1\) is the gravitational acceleration on Earth and \(g_2\) is the gravitational acceleration on planet X. Now we need to cancel out the common factors and solve for \(g_2\): \(\frac{0.24}{0.48} = \sqrt{\frac{g_2}{g_1}}\) Solving for \(g_2\), we get: \(g_2 = g_1 \left(\frac{0.24}{0.48}\right)^2\) Plug in the known value of \(g_1\) (Earth's gravitational acceleration, which is approximately \(9.81\,\text{m}/\text{s}^2\)), and we solve for \(g_2\): \(g_2 = 9.81\left(\frac{0.24}{0.48}\right)^2 = 2.4525\,\text{m}/\text{s}^2\)
02

Derive the expression for the radius of planet X

We know that gravitational force is given by: \(F = \frac{GMm}{r^2}\) where \(G\) is the gravitational constant, \(M\) is the mass of the planet, \(m\) is the mass of the object (in this case, the pendulum), and \(r\) is the distance between the centers of the masses (approximately equal to the radius of the planet). On the surface of the planets, the gravitational force is also equal to the weight of the object: \(F = mg\) Combining the two equations above, we can express them on both planets: \(\frac{GMm}{r_E^2} = m \cdot 9.81\) \(\frac{GMm}{r_X^2} = m \cdot 2.4525\) Dividing the first equation by the second one: \(\frac{r_X^2}{r_E^2} = \frac{9.81}{2.4525}\) Now solving for the ratio \(r_X/r_E\): \(\frac{r_X}{r_E} = \sqrt{\frac{9.81}{2.4525}} \approx 1.996\) Here, we have found out that the radius of planet X is approximately 1.996 times the radius of Earth.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

A mass \(m=1.00 \mathrm{~kg}\) in a spring-mass system with \(k=\) \(1.00 \mathrm{~N} / \mathrm{m}\) is observed to be moving to the right, past its equi. librium position with a speed of \(1.00 \mathrm{~m} / \mathrm{s}\) at time \(t=0 .\) a) Ignoring all damping, determine the equation of motion. b) Suppose the initial conditions are such that at time \(t=0\), the mass is at \(x=0.500 \mathrm{~m}\) and moving to the right with a speed of \(1.00 \mathrm{~m} / \mathrm{s}\). Determine the new equation of motion. Assume the same spring constant and mass.

A mass, \(M=1.6 \mathrm{~kg}\), is attached to a wall by a spring with \(k=578 \mathrm{~N} / \mathrm{m}\). The mass slides on a frictionless floor. The spring and mass are immersed in a fluid with a damping constant of \(6.4 \mathrm{~kg} / \mathrm{s}\). A horizontal force, \(\mathrm{F}(\mathrm{t})=\mathrm{F}_{\mathrm{d}} \cos \left(\omega_{\mathrm{d}} \mathrm{t}\right)\) where \(F_{d}=52 \mathrm{~N},\) is applied to the mass through a knob, caus. ing the mass to oscillate back and forth. Neglect the mass of the spring and of the knob and rod. At approximately what frequency will the amplitude of the mass's oscillation be greatest, and what is the maximum amplitude? If the driving frequency is reduced slightly (but the driving amplitude remains the same), at what frecuency will the amplitude of the mass's ascillation be half of the maximum amplitude?

In a lab, a student measures the unstretched length of a spring as \(11.2 \mathrm{~cm}\). When a 100.0 - g mass is hung from the spring, its length is \(20.7 \mathrm{~cm}\). The mass-spring system is set into oscillatory motion, and the student obscrves that the amplitude of the oscillation decreases by about a factor of 2 after five complete cycles. a) Calculate the period of oscillation for this system, assuming no damping. b) If the student can measure the period to the nearest \(0.05 \mathrm{~s}\). will she be able to detect the difference between the period with no damping and the period with damping?

A massive object of \(m=5.00 \mathrm{~kg}\) oscillates with simple harmonic motion. Its position as a function of time varies according to the equation \(x(t)=2 \sin ([\pi / 2] t+\pi / 6)\). a) What is the position, velocity, and acceleration of the object at \(t=0 \mathrm{~s}^{2}\) b) What is the kinetic energy of the object as a function of time? c) At which time after \(t=0 \mathrm{~s}\) is the kinetic energy first at a maximum?

The period of oscillation of an object in a frictionless tunnel running through the center of the Moon is \(T=2 \pi / \omega_{0}\) \(=6485 \mathrm{~s}\), as shown in Fxample 142 . What is the period of oscillation of an object in a similar tunnel through the Earth \(\left(R_{\mathrm{I}}=6.37 \cdot 10^{6} \mathrm{~m} ; R_{\mathrm{M}}=1.74 \cdot 10^{6} \mathrm{~m} ; M_{\mathrm{E}}=5.98 \cdot 10^{24} \mathrm{~kg}\right.\) \(\left.M_{u}=7.36 \cdot 10^{22} \mathbf{k g}\right) ?\)

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free