Physics for Scientists and Engineers
Physics for Scientists and Engineers
6th Edition
ISBN: 9781429281843
Author: Tipler
Publisher: MAC HIGHER
bartleby

Concept explainers

bartleby

Videos

Question
Book Icon
Chapter 3, Problem 67P

(a)

To determine

The speed and magnitude of the acceleration of a person standing on the equator.

(a)

Expert Solution
Check Mark

Answer to Problem 67P

A person standing on the equator has a speed 463.8 m/s and a centripetal acceleration of magnitude 3.37×102m/s2 which is 0.344% of g .The total acceleration of the person is 99.65%of g .

Explanation of Solution

Given:

Time taken by the Earth to rotate once on its axis, T=24 h

Radius of the Earth, RE=6.378×106m

Formula used:

The speed vE of the person on the equator is determined by the equation

  vE=2πRET.........(1)

The person on the equator experiences a centripetal acceleration arE given by

  arE=vE2RE.........(2)

The total acceleration at the equator is given by,

  aE=garE.........(3)

Calculation:

A person standing on the equator, revolves in a circular path of radius RE , the radius of the Earth as the Earth rotates about its axis. In a time T of 24 h, the earth completes one rotation and in the same time the person completes its circular motion in an orbit of radius RE .

Calculate speed vE of the person on the equator using equation (1).

  vE=2πRET=2π( 6.378× 10 6 m)( 24 h)( 3600 s/h)=463.8 m/s

All particles fixed on the Earth experience a centripetal force directed towards the center of its circular path. Hence it would experience a centripetal acceleration towards the center of its circular path.

Calculate the centripetal acceleration arE of the person using equation (2).

  arE=vE2RE= ( 463.8 m/s )2( 6.378× 10 6 m)=3.37×102m/s2

Express the acceleration as a percentage of g , the acceleration of free fall.

  a rEg×100=3.37× 10 2 m/s29.81  m/s2×100=0.344%

The total acceleration experienced by the person is given by equation (3).

  aE=garE=(1000.344)% of g=99.6% of g

Conclusion:

Thus, a person standing on the equator has a speed 463.8 m/s and a centripetal acceleration of magnitude 3.37×102m/s2 which is 0.344% of g .The total acceleration of the person is 99.65%of g .

(b)

To determine

The direction of the acceleration vector of the person on the equator.

(b)

Expert Solution
Check Mark

Answer to Problem 67P

The acceleration vector of the person is directed towards the center of the Earth.

Explanation of Solution

Introduction:

A person on the surface of the Earth experiences two forces-(i) Gravitational force W directed towards the center of the Earth and (ii) Normal contact force N perpendicular to the surface of the Earth outwards.

An object in order to move in a circular path requires centripetal force. The centripetal force is radial in nature and is directed towards the center of the earth. As the Earth rotates, the difference between W and N should provide the centripetal force FC . This is shown in Figure1.

  WN=FC

  Physics for Scientists and Engineers, Chapter 3, Problem 67P , additional homework tip  1

Figure 1

However, the weight, as felt by the person on the surface of the earth, is equal to the Normal force he experiences.

  N=WFC

Hence, the acceleration aE ,he feels on the surface of Earth on Equator is less than the acceleration of free fall g . But since both g and arE are directed towards the center of the earth, the total acceleration is also directed towards the center of the earth.

Conclusion:

Thus, the acceleration vector of the person on the Equator is directed towards the center of the Earth.

(c)

To determine

The speed and magnitude of the acceleration of a person standing at 35° latitude.

(c)

Expert Solution
Check Mark

Answer to Problem 67P

The speed of the person at 35° latitude is 379.9 m/s and his acceleration is 9.83 m/s2 .

Explanation of Solution

Given:

The latitude where the person was standing, θ=35°

Radius of the earth at equator, RE=6.378×106m

The speed of the person at equator, vE=463.8 m/s

The centripetal acceleration at the equator, arE=3.37×102m/s2

Formula used:

The person at 35° latitude moves in a circle of radius r as the Earth spins around its axis with an angular velocity ω .

The speed of person at 35° latitude is given by,

  vP=rω.........(4)

His speed at equator is given by

  vE=REω.........(5)

From equations (4) and (5),

  vP=rREvE......(6)

The centripetal acceleration at the equator is given by the expression,

  arE=REω2.........(7)

The centripetal acceleration at 35° latitude is given by the expression,

  arP=rω2.........(8)

From equations (4) and (5),

  arP=rREarE.........(9)

The person also experiences acceleration g due to the gravitational force exerted on him by the Earth and this is directed towards the center of Earth.

The magnitude of the resultant acceleration is determined by using parallelogram law of vectors.

  aP=arP2+g2+2arPgcosθ.....(10)

Calculation:

The motion of the person at 35°latitude is represented in the diagram below:

  Physics for Scientists and Engineers, Chapter 3, Problem 67P , additional homework tip  2

Figure 2

From Figure 2, it can be seen that

  rRE=cosθ.........(11)

Use equation (11) in equation (6).

  vP=rREvE=vEcosθ

Substitute the value of the variables in the above equation.

  vP=vEcosθ=(463.8 m/s)(cos35°)=379.9 m/s

Use equation (11) in equation (9) and substitute the values of the variables to calculate the value of arP .

  arP=rREarE=arEcosθ=(3.37× 10 2 m/s2)(cos35°)=2.76×102m/s2

The vector arP is directed towards the center of its circular path and is at an angle 35° to the direction of the acceleration of free fall g .

Substitute the values of variables in equation (10) and calculate the magnitude of the resultant acceleration aP .

  aP=a rP2+g2+2a rPgcosθ= ( 2.76× 10 2 m/s 2 )2+ ( 9.81 m/s 2 )2+2( 2.76× 10 2 m/s 2 )( 9.81 m/s 2 )( cos35°)=9.83 m/s2

Conclusion:

Thus, the speed of the person at 35° latitude is 379.9 m/s and his acceleration is 9.83 m/s2 .

(d)

To determine

The angle between the direction of the acceleration at 35° latitude and acceleration at equator at the same longitude.

(d)

Expert Solution
Check Mark

Answer to Problem 67P

The angle between the direction of the acceleration at 35° latitude and acceleration at equator at the same longitude is found to be 34.9° .

Explanation of Solution

Given:

The magnitude of centripetal acceleration at 35° latitude, arP=2.76×102m/s2

The value of acceleration of free fall, g=9.81m/s2

The latitude where the person was standing, θ=35°

Formula used:

The direction of the acceleration at the equator is along the horizontal direction parallel to the direction of the centripetal acceleration at 35° latitude.

  aEarP

Hence the angle α between the directions of arP and aP is equal to the angle between aP and aE .

The vector diagram representing the accelerations is shown below:

  Physics for Scientists and Engineers, Chapter 3, Problem 67P , additional homework tip  3

Figure 3

This is given by

  α=tan1(gsinθa rP+gcosθ).........(12)

Calculation:

Substitute the values of the variables in equation (12).

  α=tan1( gsinθ a rP +gcosθ)=tan1[( 9.81 m/s 2 )( sin35°)( 2.76× 10 2 m/s 2 )+( 9.81 m/s 2 )( cos35°)]=34.9°

Conclusion:

Thus, the angle between the direction of the acceleration at 35° latitude and acceleration at equator at the same longitude is found to be 34.9° .

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
You hopefully used g=9.8 m/s2 (or thereabouts).   That is the gravitational acceleration near the earth's surface.  if you rise high above the earth, the gravitational acceleration decreases.  Specifically, the gravitational acceleration is inversely proportional to the square of the distance from the earth's center. Equivalently, if you multiply the acceleration by the distance from the earth's center, you should get the same number for all heights. For this problem, take the radius of the earth as 3,902 miles, and calculate the gravitational acceleration of a satellite in low orbit, 182 miles above the surface.
Kepler's Third Law of planetary motion states that the square of the period T of a planet (the time it takes for the planet to make a complete revolution about the sun) is directly proportional to the cube of its average distance d from the sun. (a) Express Kepler's Third Law as an equation. (Use k for the constant of proportionality.)   (c) The planet Neptune is about 2.79 × 109 mi from the sun. Find the period of Neptune. (Round your answer to the nearest whole number of years.)
Kepler's third law states that for any object in a gravitational orbit,  P2∝a3P2∝a3  where PP  is the orbital period of the object and aa  is the average distance between the object and what it is orbiting. In our Solar System, the natural units are distances measured in astronomical units (A.U.) and orbital periods measured in years. This can be seen for the Earth-Sun system which has an orbital period P=1P=1  year and an average distance  a=1a=1  AU. Using these natural units in the Solar System, the proportionality becomes an equality, so for our Solar System:  (Pyears)2=(aA.U.)3(Pyears)2=(aA.U.)3 . Using your mathematical prowess, determine what the orbital period in years would be for an asteroid that was discovered orbiting the Sun with an average distance of 25 astronomical units.

Chapter 3 Solutions

Physics for Scientists and Engineers

Ch. 3 - Prob. 11PCh. 3 - Prob. 12PCh. 3 - Prob. 13PCh. 3 - Prob. 14PCh. 3 - Prob. 15PCh. 3 - Prob. 16PCh. 3 - Prob. 17PCh. 3 - Prob. 18PCh. 3 - Prob. 19PCh. 3 - Prob. 20PCh. 3 - Prob. 21PCh. 3 - Prob. 22PCh. 3 - Prob. 23PCh. 3 - Prob. 24PCh. 3 - Prob. 25PCh. 3 - Prob. 26PCh. 3 - Prob. 27PCh. 3 - Prob. 28PCh. 3 - Prob. 29PCh. 3 - Prob. 30PCh. 3 - Prob. 31PCh. 3 - Prob. 32PCh. 3 - Prob. 33PCh. 3 - Prob. 34PCh. 3 - Prob. 35PCh. 3 - Prob. 36PCh. 3 - Prob. 37PCh. 3 - Prob. 38PCh. 3 - Prob. 39PCh. 3 - Prob. 40PCh. 3 - Prob. 41PCh. 3 - Prob. 42PCh. 3 - Prob. 43PCh. 3 - Prob. 44PCh. 3 - Prob. 45PCh. 3 - Prob. 46PCh. 3 - Prob. 47PCh. 3 - Prob. 48PCh. 3 - Prob. 49PCh. 3 - Prob. 50PCh. 3 - Prob. 51PCh. 3 - Prob. 52PCh. 3 - Prob. 53PCh. 3 - Prob. 54PCh. 3 - Prob. 55PCh. 3 - Prob. 56PCh. 3 - Prob. 57PCh. 3 - Prob. 58PCh. 3 - Prob. 59PCh. 3 - Prob. 60PCh. 3 - Prob. 61PCh. 3 - Prob. 62PCh. 3 - Prob. 63PCh. 3 - Prob. 64PCh. 3 - Prob. 65PCh. 3 - Prob. 66PCh. 3 - Prob. 67PCh. 3 - Prob. 68PCh. 3 - Prob. 69PCh. 3 - Prob. 70PCh. 3 - Prob. 71PCh. 3 - Prob. 72PCh. 3 - Prob. 73PCh. 3 - Prob. 74PCh. 3 - Prob. 75PCh. 3 - Prob. 76PCh. 3 - Prob. 77PCh. 3 - Prob. 78PCh. 3 - Prob. 79PCh. 3 - Prob. 80PCh. 3 - Prob. 81PCh. 3 - Prob. 82PCh. 3 - Prob. 83PCh. 3 - Prob. 84PCh. 3 - Prob. 85PCh. 3 - Prob. 86PCh. 3 - Prob. 87PCh. 3 - Prob. 88PCh. 3 - Prob. 89PCh. 3 - Prob. 90PCh. 3 - Prob. 91PCh. 3 - Prob. 92PCh. 3 - Prob. 93PCh. 3 - Prob. 94PCh. 3 - Prob. 95PCh. 3 - Prob. 96PCh. 3 - Prob. 97PCh. 3 - Prob. 98PCh. 3 - Prob. 99PCh. 3 - Prob. 100PCh. 3 - Prob. 101PCh. 3 - Prob. 102PCh. 3 - Prob. 103PCh. 3 - Prob. 104PCh. 3 - Prob. 105PCh. 3 - Prob. 106PCh. 3 - Prob. 107PCh. 3 - Prob. 108PCh. 3 - Prob. 109PCh. 3 - Prob. 110PCh. 3 - Prob. 111PCh. 3 - Prob. 112PCh. 3 - Prob. 113PCh. 3 - Prob. 114PCh. 3 - Prob. 115PCh. 3 - Prob. 116PCh. 3 - Prob. 117PCh. 3 - Prob. 118PCh. 3 - Prob. 119PCh. 3 - Prob. 120PCh. 3 - Prob. 121PCh. 3 - Prob. 122P
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
Principles of Physics: A Calculus-Based Text
Physics
ISBN:9781133104261
Author:Raymond A. Serway, John W. Jewett
Publisher:Cengage Learning
Text book image
University Physics Volume 1
Physics
ISBN:9781938168277
Author:William Moebs, Samuel J. Ling, Jeff Sanny
Publisher:OpenStax - Rice University
What Is Circular Motion? | Physics in Motion; Author: GPB Education;https://www.youtube.com/watch?v=1cL6pHmbQ2c;License: Standard YouTube License, CC-BY