Physics Fundamentals
Physics Fundamentals
2nd Edition
ISBN: 9780971313453
Author: Vincent P. Coletta
Publisher: PHYSICS CURRICULUM+INSTRUCT.INC.
bartleby

Concept explainers

bartleby

Videos

Question
Book Icon
Chapter 3, Problem 40P

(a)

To determine

The magnitudes of the velocity and acceleration of the Moon relative to the Earth.

(a)

Expert Solution
Check Mark

Answer to Problem 40P

The velocity of the Moon as it travels in a circular orbit around the Earth is found to be 1.023×103 m/s and its acceleration has a magnitude 2.75×103 m/s2 directed towards the Earth.

Explanation of Solution

Given:

The radius of the Moon’s orbit around the Earth, rM=3.8×105km

The time period of revolution of the moon around the Earth, TM=27 days

Formula used:

The Moon travels a distance equal to the circumference of its orbit in the time equal to its time period. Its velocity vM is given by,

  vM=2πrMTM.....(1)

As it revolves around the Earth, it experiences a centripetal force towards the center of its orbit. Its centripetal acceleration is given by,

  aM=vM2rM.....(2)

Calculation:

Express the radius of the Moon’s orbit around the Earth in meters.

  rM=(3.8× 105km)( 10 3  m 1 km)=3.8×108m

Express the time period of the Moon’s revolution around the Earth.

  TM=(27 days)( 24 h 1 d)( 3600 s 1 h)=2.33×106s

Substitute the values of rM and TM in equation (1) and calculate the magnitude of the Moon’s velocity.

  vM=2πrMTM=2π( 3.8× 10 8 m)( 2.33× 10 6 s)=1.023×103m/s

Substitute the values of vM and TM in equation (2) and calculate the magnitude of the Moon’s acceleration.

  aM=vM2rM= ( 1.023× 10 3 m/s )2( 3.8× 10 8 m)=2.75×103m/s2

Conclusion:

Thus, the velocity of the Moon as it travels in a circular orbit around the Earth is found to be 1.023×103 m/s and its acceleration has a magnitude 2.75×103 m/s2 directed towards the Earth.

(b)

To determine

The magnitudes of the velocity and acceleration of the Earth relative to the Sun

(b)

Expert Solution
Check Mark

Answer to Problem 40P

The velocity of the Earth as it travels in a circular orbit around the sun is found to be 3.0×104 m/s and its acceleration has a magnitude 6.0×103m/s2 directed towards the Sun.

Explanation of Solution

Given:

The radius of the Earth’s orbit around the Sun, rE=1.5×108km

The time period of revolution of the Earth around the Sun, TE=365 days

Formula used:

The Earth travels a distance equal to the circumference of its orbit in the time equal to its time period. Its velocity vE is given by,

  vE=2πrETE.....(3)

As it revolves around the Sun, it experiences a centripetal force towards the center of its orbit. Its centripetal acceleration is given by,

  aE=vE2rE.....(4)

Calculation:

Express the radius of the Earth’s orbit around the sun in meters.

  rE=(1.5× 108km)( 10 3  m 1 km)=1.5×1011m

Express the time period of the Earth’s revolution around the Sun.

  TE=(365 days)( 24 h 1 d)( 3600 s 1 h)=3.15×107s

Substitute the values of rE and TE in equation (3) and calculate the magnitude of the Earth’s velocity.

  vE=2πrETE=2π( 1.5× 10 11 m)( 3.15× 10 7 s)=3.0×104m/s

Substitute the values of vE and TE in equation (4) and calculate the magnitude of the Earth’s acceleration.

  aE=vE2rE= ( 3.0× 10 4 m/s )2( 1.5× 10 11 m)=6.0×103m/s2

Conclusion:

Thus, velocity of the Earth as it travels in a circular orbit around the sun is found to be 3.0×104 m/s and its acceleration has a magnitude 6.0×103m/s2 directed towards the Sun.

(c)

To determine

The value of the maximum acceleration of the Moon relative to Sun and the phase of the Moon this occurs.

(c)

Expert Solution
Check Mark

Answer to Problem 40P

The value of the maximum acceleration of the Moon relative to Sun is found to be 8.75×103m/s2 and this occurs during Full moon.

Explanation of Solution

Given:

The acceleration of the Moon relative to Earth, aM=2.75×103m/s2

The acceleration of the Earth relative to the Sun, aE=6.0×103m/s2

The radius of the Earth’s orbit around the Sun, rE=1.5×108km

The radius of the Moon’s orbit around the Earth, rM=3.8×105km

Calculation:

The Moon revolves around the Earth in a circular orbit and the Earth revolves around the Sun. The Moon experiences accelerations relative to both Earth and the sun.

This is shown in the diagram below:

  Physics Fundamentals, Chapter 3, Problem 40P

At New Moon day, the moon is farthest from the Sun and its acceleration towards the Earth and that towards the Sun point in the same direction. Hence, at this time, the accelerations add up and the Moon’s acceleration relative to the Sun is maximum.

Calculate the distance of the moon from the Sun when it is at its farthest position from the Sun.

  r=rM+rE=(3.8× 108m)+(1.5× 10 11m)=1.5038×1011m1.5×1011m

The Moon’s distance from the Sun is nearly equal to the Earth’s distance from the Sun.

The Moon experiences an acceleration directed towards the Earth due its revolution around the Earth and since it moves around the Sun along with the Earth, it experiences an acceleration towards the Sun. During New moon day, the Moon, Earth and the Sun are in a straight line with the Moon at the farthest from the Sun. In this position, the acceleration of the Moon towards the Earth and towards the Sun are directed along the same straight line, towards the Sun. Hence, they add up.

Since the distance of the Moon from the Sun is nearly equal to that of the Earth’s distance from it, the Moon’s acceleration due its revolution around the Sun can be taken to be equal to that of the Earth’s around the Sun.

The Moon’s maximum acceleration in a direction towards the Sun a is given by,

  a=aM+aE

Substitute the values of the accelerations in the above expression.

  a=aM+aE=(2.75× 10 3 m/s2)+(6.0× 10 3 m/s2)=8.75×103m/s2

Conclusion:

Thus, the value of the maximum acceleration of the Moon relative to Sun is found to be 8.75×103m/s2 and this occurs during Full moon.

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
An object with mass 2.50 kg is moving along a circular path with a radius of 2.20m. At an instant when the speed of the object is equal to 3.50m/s and is changing at a rate of 5.40 m/s^2, calculate the magnitude of the total acceleration (in m/s^2) of the object. Round the answer to 3 decimal places.
Assume that the earth’s orbit around the sun is circular and has a radius of 1.50 x 10 to the 8th power kilometers? (a) What is the magnitude of the orbital velocity of the earth, in meters per second? (b) What is the magnitude of the centripetal acceleration of the earth toward the sun, in meters per second squared?
The earth rotates once per day about an axis passing through the north and south poles, an axis that is perpendicular to the plane of the equator. Assuming the earth is a sphere with a radius of 6.38 x 106 m, determine the speed and centripetal acceleration of a person situated (a) at the equator (b) at a latitude of 76.0 ° north of the equator (All answers need to be in 3 sig figs)
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
SEE MORE QUESTIONS
Recommended textbooks for you
Text book image
College Physics
Physics
ISBN:9781305952300
Author:Raymond A. Serway, Chris Vuille
Publisher:Cengage Learning
Text book image
University Physics (14th Edition)
Physics
ISBN:9780133969290
Author:Hugh D. Young, Roger A. Freedman
Publisher:PEARSON
Text book image
Introduction To Quantum Mechanics
Physics
ISBN:9781107189638
Author:Griffiths, David J., Schroeter, Darrell F.
Publisher:Cambridge University Press
Text book image
Physics for Scientists and Engineers
Physics
ISBN:9781337553278
Author:Raymond A. Serway, John W. Jewett
Publisher:Cengage Learning
Text book image
Lecture- Tutorials for Introductory Astronomy
Physics
ISBN:9780321820464
Author:Edward E. Prather, Tim P. Slater, Jeff P. Adams, Gina Brissenden
Publisher:Addison-Wesley
Text book image
College Physics: A Strategic Approach (4th Editio...
Physics
ISBN:9780134609034
Author:Randall D. Knight (Professor Emeritus), Brian Jones, Stuart Field
Publisher:PEARSON
Kinematics Part 3: Projectile Motion; Author: Professor Dave explains;https://www.youtube.com/watch?v=aY8z2qO44WA;License: Standard YouTube License, CC-BY