Vector Mechanics for Engineers: Dynamics
Vector Mechanics for Engineers: Dynamics
11th Edition
ISBN: 9780077687342
Author: Ferdinand P. Beer, E. Russell Johnston Jr., Phillip J. Cornwell, Brian Self
Publisher: McGraw-Hill Education
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Chapter 17.3, Problem 17.125P
To determine

(a)

Velocity of the block and angular velocity of the disk immediately after perfectly plastic impact.

Expert Solution
Check Mark

Answer to Problem 17.125P

The velocity of the block and angular velocity of the disk immediately after perfectly plastic impactare m×2gh(12M+m) and m×2gh(12MR+mR) respectively.

Explanation of Solution

Given:

Mass of block is m, mass of the disk is M and Falling distance is h.

Concept used:

Conservation of momentum for perfectly plastic condition is given as follows:

Iω1+mu1R=Iω2+mu2R …… (1)

Here, angular velocity of disk is ω and velocity of the blockis u. 1 and 2 subscripts are for initial and final conditions.

Calculation:

Velocity of the block after the cord becomes taut is calculated by conservation of energy as follows:

mgh=12mu2u=2gh

Substitute 0 for ω1, 2gh for u1, 12MR2 for I and ω2R for u2 in equation (1).

I×0+m×2gh×R=12MR2×ω2+m×ω2R2m×2gh=ω2(12MR+mR)ω2=m×2gh(12MR+mR)

Velocity of the block is calculated as follows:

u2=ω2Ru2=m×2gh(12MR+mR)×Ru2=m×2gh(12M+m)

Thus, the velocity of the block and angular velocity of the disk immediately after perfectly plastic impactare m×2gh(12M+m) and m×2gh(12MR+mR) respectively.

Conclusion:

The velocity of the block and angular velocity of the disk immediately after perfectly plastic impactare m×2gh(12M+m) and m×2gh(12MR+mR) respectively.

To determine

(b)

Velocity of the block and angular velocity of the disk immediately after perfectly elastic impact.

Expert Solution
Check Mark

Answer to Problem 17.125P

The velocity of the block and angular velocity of the disk immediately after perfectly plastic impactare 4m2ghR(2m+M) and 2gh(12M(2m+M)) respectively.

Explanation of Solution

Given:

Mass of block is m, mass of the disk is M and Falling distance is h.

Calculation:

Substitute 0 for ω1, 2gh for u1 and 12MR2 for I in equation (1).

I×0+m×2gh×R=12MR2×ω2+m×u2Ru2=mR2gh12MR2×ω2mRu2=2gh12×MRm×ω2

Apply the conservation of energy for elastic impact as follows:

mgh+12Iω12=12Iω22+12mu22

Substitute 0 for ω1, 2gh12×MRm×ω2 for u2 and 12MR2 for I in above equation.

mgh+12I(0)2=12×12MR2ω22+12m(2gh12×MRm×ω2)2mgh=14MR2ω22+12m(2gh2×2gh×12×MRm×ω2+14×M2R2m2×ω22)mgh=14MR2ω22+(mgh2gh×12×MR×ω2+18×M2R2m×ω22)(14MR2+M2R28m)ω222gh×MR2×ω2+mghmgh=0ω2((14MR2+M2R28m)ω22gh×MR2)=0

On further simplification,

((14MR2+M2R28m)ω22gh×MR2)=0ω2=2gh×MR2(14MR2+M2R28m)ω2=4m2ghR(2m+M)

Velocity of the block is calculated as follows:

u2=2gh12×MRm×4m2ghR(2m+M)u2=2gh(12M(2m+M))

Thus, the velocity of the block and angular velocity of the disk immediately after perfectly elastic impactare 4m2ghR(2m+M) and 2gh(12M(2m+M)) respectively.

Conclusion:

The velocity of the block and angular velocity of the disk immediately after perfectly elastic impactare 4m2ghR(2m+M) and 2gh(12M(2m+M)) respectively.

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Chapter 17 Solutions

Vector Mechanics for Engineers: Dynamics

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