Warning: foreach() argument must be of type array|object, bool given in /var/www/html/web/app/themes/studypress-core-theme/template-parts/header/mobile-offcanvas.php on line 20

Two planets have the same mass, \(M,\) but one of them is much denser than the other. Identical objects of mass \(m\) are placed on the surfaces of the planets. Which object will have the gravitational potential energy of larger magnitude? a) Both objects will have the same gravitational potential energy. b) The object on the surface of the denser planet will have the larger gravitational potential energy. c) The object on the surface of the less dense planet will have the larger gravitational potential energy. d) It is impossible to tell.

Short Answer

Expert verified
Answer: The object on the surface of the denser planet will have the larger gravitational potential energy.

Step by step solution

01

Calculate the radii of the planets

To calculate the potential energy, we need to find the radii of the planets. Let's denote the density of the denser planet as \(\rho_1\) and the less dense planet as \(\rho_2\). The mass of each planet can be expressed as \(M = \rho_1 V_1 = \rho_2 V_2,\) where \(V_1\) and \(V_2\) are the volumes of the planets. For a spherical planet, we have \(V_1 = \frac{4}{3}\pi r_1^3\) and \(V_2 = \frac{4}{3}\pi r_2^3,\) where \(r_1\) and \(r_2\) are the radii of the denser and less dense planets respectively. Thus, using the mass and density, we can determine the radii of the planets: \(r_1 = \sqrt[3]{\frac{3M}{4\pi\rho_1}}\) and \(r_2 = \sqrt[3]{\frac{3M}{4\pi\rho_2}}.\)
02

Calculate the gravitational potential energy for the objects on each planet

Now that we have the radii for both planets, we can calculate the gravitational potential energy for each object using the formula \(U = -\frac{G\M\times m}{r}.\) For the denser planet, we have \(U_1 = -\frac{G(M)(m)}{r_1}\) and for the less dense planet, we have \(U_2 = -\frac{G(M)(m)}{r_2}.\)
03

Compare the gravitational potential energies

To compare the gravitational potential energies \(U_1\) and \(U_2,\) note that the magnitudes of the energies are inversely proportional to the radii of the planets (since the other factors are constants). As the denser planet has a smaller radius (\(r_1 < r_2\)), its gravitational potential energy magnitude will be larger, and the less dense planet's gravitational potential energy magnitude will be smaller. Therefore, the correct answer is: b) The object on the surface of the denser planet will have the larger gravitational potential energy.

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 1000.-kg communications satellite is released from a space shuttle to initially orbit the Earth at a radius of \(7.00 \cdot 10^{6} \mathrm{~m}\). After being deployed, the satellite's rockets are fired to put it into a higher altitude orbit of radius \(5.00 \cdot 10^{7} \mathrm{~m} .\) What is the minimum mechanical energy supplied by the rockets to effect this change in orbit?

A satellite of mass \(m\) is in an elliptical orbit (that satisfies Kepler's laws) about a body of mass \(M,\) with \(m\) negligible compared to \(M\) a) Find the total energy of the satellite as a function of its speed, \(v\), and distance, \(r\), from the body it is orbiting. b) At the maximum and minimum distance between the satellite and the body, and only there, the angular momentum is simply related to the speed and distance. Use this relationship and the result of part (a) to obtain a relationship between the extreme distances and the satellite's energy and angular momentum. c) Solve the result of part (b) for the maximum and minimum radii of the orbit in terms of the energy and angular momentum per unit mass of the satellite. d) Transform the results of part (c) into expressions for the semimajor axis, \(a\), and eccentricity of the orbit, \(e\), in terms of the energy and angular momentum per unit mass of the satellite.

A plumb bob located at latitude \(55.0^{\circ} \mathrm{N}\) hangs motionlessly with respect to the ground beneath it. \(A\) straight line from the string supporting the bob does not go exactly through the Earth's center. Does this line intersect the Earth's axis of rotation south or north of the Earth's center?

Suppose a new extrasolar planet is discovered. Its mass is double the mass of the Earth, but it has the same density and spherical shape as the Earth. How would the weight of an object at the new planet's surface differ from its weight on Earth?

Two identical 20.0 -kg spheres of radius \(10 \mathrm{~cm}\) are \(30.0 \mathrm{~cm}\) apart (center-to-center distance). a) If they are released from rest and allowed to fall toward one another, what is their speed when they first make contact? b) If the spheres are initially at rest and just touching, how much energy is required to separate them to \(1.00 \mathrm{~m}\) apart? Assume that the only force acting on each mass is the gravitational force due to the other mass.

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