PHYSICS:F/SCI...W/MOD..-UPD(LL)W/ACCES
PHYSICS:F/SCI...W/MOD..-UPD(LL)W/ACCES
9th Edition
ISBN: 9780357001417
Author: SERWAY
Publisher: CENGAGE L
bartleby

Videos

Textbook Question
Book Icon
Chapter 13, Problem 60AP

Two spheres having masses M and 2M and radii R and 3R, respectively, are simultaneously released from rest when the distance between their centers is 12R. Assume the two spheres interact only with each other and we wish to find the speeds with which they collide. (a) What two isolated system models are appropriate for this system? (b) Write an equation from one of the models and solve it for v 1 , the velocity of the sphere of mass M at any time after release in terms of v 2 , the velocity of 2M. (c) Write an equation from the other model and solve it for speed v1 in terms of speed v2 when the spheres collide. (d) Combine the two equations to find the two speeds v1 and v2 when the spheres collide.

(a)

Expert Solution
Check Mark
To determine

To determine: The two isolated system models that are appropriate for this system.

Answer to Problem 60AP

Answer: Conservation of energy and conservation of momentum are the two models that are appropriate for this system.

Explanation of Solution

Explanation:

Given information: The masses of the two spheres are M and 2M respectively, the radius of spheres are R and 3R respectively and the distance between their centers is 12R .

The two isolated system models that are appropriate for this system are conservation of energy and conservation of momentum. In these situations, the energy and momentum is conserved before and after the collision of the bodies. This is also called as the perfect elastic collision.

Conclusion:

Therefore, the conservation of energy and conservation of momentum are the two models that are appropriate for this system.

(b)

Expert Solution
Check Mark
To determine

To determine: The equation from one of the model and estimate the speed v1 .

Answer to Problem 60AP

Answer: The equation from conservation of momentum is Mv1+2Mv2=0 and the expression for speed is v1=2v2 .

Explanation of Solution

Explanation:

Given information: The masses of the two spheres are M and 2M respectively, the radius of spheres are R and 3R respectively and the distance between their centers is 12R .

By the conservation of momentum for elastic collision,

m1u1+m2u2=m1v1+m2v2

m1 is the mass of first sphere.

u1 is the initial velocity of the first sphere.

m2 is the mass of second sphere.

u2 is the initial velocity of second sphere.

v1 is the initial velocity of first sphere.

v2 is the final velocity of second sphere.

Substitute M for m1 , 2M for m2 , 0 for u1 , 0 for u2 in above expression.

M×0+2M×0=Mv1+2Mv2Mv1+2Mv2=0v1=2v2 (I)

Conclusion:

Therefore, the equation from conservation of momentum is Mv1+2Mv2=0 and the expression for speed is v1=2v2 .

(c)

Expert Solution
Check Mark
To determine

To determine: The equation from one of the other model and estimate the speed v1 .

Answer to Problem 60AP

Answer: The equation from conservation of energy is v122+v22=GM3R and the expression for the speed is v1=2(GM3Rv22) .

Explanation of Solution

Explanation:

Given information: The masses of the two spheres are M and 2M respectively, the radius of spheres are R and 3R respectively and the distance between their centers is 12R .

By the conservation of energy is,

KE1+PE1=KE2+PE2 (II)

KE1 is the kinetic energy of the spheres before collide.

KE2 is the final kinetic energy of the spheres after collide.

PE1 is the potential energy of the spheres before collide.

PE2 is final potential energy of the spheres after collide.

Formula to calculate the kinetic energy of the spheres after collide is,

KE2=12m1v12+12m2v22

Formula to calculate the potential energy of the spheres before collide is,

PE1=Gm1m2R1

R1 is the initial distance between the center of first sphere and second sphere.

G is the universal gravitational constant.

Formula to calculate the potential energy of the spheres after collide is,

PE2=Gm1m2R2

R2 is the final distance between the center of first sphere and second sphere.

Substitute Gm1m2R1 for PE1 , Gm1m2R2 for PE2 , 0 for KE1 , and 12m1v12+12m2v22 for KE2 in equation (II).

0+(Gm1m2R1)=12m1v12+12m2v22+(Gm1m2R2)

Substitute M for m1 , 2M for m2 , 0 for u1 , 0 for u2 , 12R for R1 and 4R for R2 in above expression.

0+(G×M×2M12R)=12×M×v12+12×2M×v22+(G×M×2M4R)12×v12+12×2×v22=(G×2M4R)(G×2M12R)v122+v22=2GM(14R112R)v1=2(GM3Rv22) (III)

Conclusion:

Therefore, the equation from one of the other model is v122+v22=GM3R and the speed v1 is v1=2(GM3Rv22) .

(d)

Expert Solution
Check Mark
To determine

To determine: The values of speeds v1 and v2 .

Answer to Problem 60AP

Answer: The value of speed v1 is 2GM9R and value of v2 is GM9R .

Explanation of Solution

Explanation:

Given information: The masses of the two spheres are M and 2M respectively, the radius of spheres are R and 3R respectively and the distance between their centers is 12R .

From equation (III) is,

v1=2(GM3Rv22)

Substitute 2v2 for v1 in above expression.

(2v2)=2(GM3Rv22)(2v2)2=2(GM3Rv22)6v22=2GM3Rv2=GM9R

Substitute GM9R for v2 in equation (I).

v1=2GM9R

Conclusion:

Therefore, the value of speeds v1 is 2GM9R and value of v2 is GM9R .

Want to see more full solutions like this?

Subscribe now to access step-by-step solutions to millions of textbook problems written by subject matter experts!
Students have asked these similar questions
In an experiment, a particle of mass m is shot with speed v0 against a second resting particle of mass 2m After impact, three particles are observed, where the sketched directions and the following masses and velocities are detected during measurements: m1 = m, v1 = 2v0, v2 = v0/2. Determine m2, m3 and v3.
Consider two particles A and B of masses m and 2m at rest in an inertial frame. Each of them are acted upon by net forces of equal magnitude in the positive x direction for equal amounts of time t. Moment of the particles A and B in centre of mass frame respectively are?
Two manned satellites approaching one another at a relative speed of 0.300 m/s intend to dock. The first has a mass of 2.50 ✕ 103 kg, and the second a mass of 7.50 ✕ 103 kg. Assume that the positive direction is directed from the second satellite towards the first satellite. (a) Calculate the final velocity after docking, in the frame of reference in which the first satellite was originally at rest.

Chapter 13 Solutions

PHYSICS:F/SCI...W/MOD..-UPD(LL)W/ACCES

Ch. 13 - Prob. 7OQCh. 13 - Prob. 8OQCh. 13 - Prob. 9OQCh. 13 - Prob. 10OQCh. 13 - Prob. 11OQCh. 13 - Prob. 1CQCh. 13 - Prob. 2CQCh. 13 - Prob. 3CQCh. 13 - Prob. 4CQCh. 13 - Prob. 5CQCh. 13 - Prob. 6CQCh. 13 - Prob. 7CQCh. 13 - Prob. 8CQCh. 13 - Prob. 9CQCh. 13 - Prob. 1PCh. 13 - Determine the order of magnitude of the...Ch. 13 - Prob. 3PCh. 13 - During a solar eclipse, the Moon, the Earth, and...Ch. 13 - Prob. 5PCh. 13 - Prob. 6PCh. 13 - Prob. 7PCh. 13 - Prob. 8PCh. 13 - Prob. 9PCh. 13 - Prob. 10PCh. 13 - Prob. 11PCh. 13 - Prob. 12PCh. 13 - Review. Miranda, a satellite of Uranus, is shown...Ch. 13 - (a) Compute the vector gravitational field at a...Ch. 13 - Prob. 15PCh. 13 - A spacecraft in the shape of a long cylinder has a...Ch. 13 - An artificial satellite circles the Earth in a...Ch. 13 - Prob. 18PCh. 13 - Prob. 19PCh. 13 - A particle of mass m moves along a straight line...Ch. 13 - Prob. 21PCh. 13 - Prob. 22PCh. 13 - Prob. 23PCh. 13 - Prob. 24PCh. 13 - Use Keplers third law to determine how many days...Ch. 13 - Prob. 26PCh. 13 - Prob. 27PCh. 13 - (a) Given that the period of the Moons orbit about...Ch. 13 - Suppose the Suns gravity were switched off. The...Ch. 13 - Prob. 30PCh. 13 - Prob. 31PCh. 13 - How much energy is required to move a 1 000-kg...Ch. 13 - Prob. 33PCh. 13 - An object is released from rest at an altitude h...Ch. 13 - A system consists of three particles, each of mass...Ch. 13 - Prob. 36PCh. 13 - A 500-kg satellite is in a circular orbit at an...Ch. 13 - Prob. 38PCh. 13 - Prob. 39PCh. 13 - Prob. 40PCh. 13 - Prob. 41PCh. 13 - Prob. 42PCh. 13 - Prob. 43PCh. 13 - Prob. 44PCh. 13 - Prob. 45PCh. 13 - Prob. 46PCh. 13 - Ganymede is the largest of Jupiters moons....Ch. 13 - Prob. 48PCh. 13 - Prob. 49PCh. 13 - Prob. 50APCh. 13 - Prob. 51APCh. 13 - Voyager 1 and Voyager 2 surveyed the surface of...Ch. 13 - Prob. 53APCh. 13 - Why is the following situation impossible? A...Ch. 13 - Let gM represent the difference in the...Ch. 13 - A sleeping area for a long space voyage consists...Ch. 13 - Prob. 57APCh. 13 - Prob. 58APCh. 13 - Prob. 59APCh. 13 - Two spheres having masses M and 2M and radii R and...Ch. 13 - Prob. 61APCh. 13 - (a) Show that the rate of change of the free-fall...Ch. 13 - Prob. 63APCh. 13 - Prob. 64APCh. 13 - Prob. 65APCh. 13 - A certain quaternary star system consists of three...Ch. 13 - Studies of the relationship of the Sun to our...Ch. 13 - Review. Two identical hard spheres, each of mass m...Ch. 13 - Prob. 69APCh. 13 - Prob. 70APCh. 13 - Prob. 71APCh. 13 - Prob. 72APCh. 13 - Prob. 73APCh. 13 - Two stars of masses M and m, separated by a...Ch. 13 - Prob. 75APCh. 13 - Prob. 76APCh. 13 - As thermonuclear fusion proceeds in its core, the...Ch. 13 - The Solar and Heliospheric Observatory (SOHO)...Ch. 13 - Prob. 79CPCh. 13 - Prob. 80CP
Knowledge Booster
Background pattern image
Physics
Learn more about
Need a deep-dive on the concept behind this application? Look no further. Learn more about this topic, physics and related others by exploring similar questions and additional content below.
Similar questions
Recommended textbooks for you
Text book image
Principles of Physics: A Calculus-Based Text
Physics
ISBN:9781133104261
Author:Raymond A. Serway, John W. Jewett
Publisher:Cengage Learning
Text book image
Classical Dynamics of Particles and Systems
Physics
ISBN:9780534408961
Author:Stephen T. Thornton, Jerry B. Marion
Publisher:Cengage Learning
Text book image
Physics for Scientists and Engineers: Foundations...
Physics
ISBN:9781133939146
Author:Katz, Debora M.
Publisher:Cengage Learning
Text book image
University Physics Volume 3
Physics
ISBN:9781938168185
Author:William Moebs, Jeff Sanny
Publisher:OpenStax
Text book image
The Solar System
Physics
ISBN:9781337672252
Author:The Solar System
Publisher:Cengage
Text book image
Stars and Galaxies (MindTap Course List)
Physics
ISBN:9781337399944
Author:Michael A. Seeds
Publisher:Cengage Learning
Time Dilation - Einstein's Theory Of Relativity Explained!; Author: Science ABC;https://www.youtube.com/watch?v=yuD34tEpRFw;License: Standard YouTube License, CC-BY