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Fluid Mechanics 9th Edition by Frank White | Complete Solution Manual

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INSTANT PDF DOWNLOAD — This document contains the complete solution manual for Fluid Mechanics, 9th Edition by Frank White. It provides detailed, step-by-step solutions to end-of-chapter problems covering fluid statics, fluid dynamics, control volume analysis, dimensional analysis, pipe flow, boundary layers, and turbomachinery. The material follows the textbook structure and is ideal for homework support, exam preparation, and strengthening conceptual understanding of fluid mechanics principles.

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Institution
Fluid Mechanics ” By
Course
Fluid Mechanics ” by

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ALL 11 CHAPTERS COVERED




SOLUTIONS MANUAL

,TABLE OF CONTENTS

Chapter 1 Introduction
Chapter 2 Pressure Distribution in a Fluid
Chapter 3 Integral Relations for a Control Volume
Chapter 4 Differential Relations for Fluid Flow
Chapter 5 Dimensional Analysis and Similarity
Chapter 6 Viscous Flow in Ducts
Chapter 7 Flow Past Immersed Bodies
Chapter 8 Potential Flow and Computational Fluid Dynamics
Chapter 9 Compressible Flow
Chapter 10 Open-Channel Flow
Chapter 11 Turbomachinery

APPENDIX F

, Chapter 1 • Introduction 1-1




Chapter 1 • Introduction

P1.1 A gas at 20C may be rarefied if it contains less than 1012 molecules per mm3. If
Avogadro’s number is 6.023E23 molecules per mole, what air pressure does this represent?

Solution: The mass of one molecule of air may be computed as
Molecular weight 28.97 mol−1
m= = = 4.81E−23 g
Avogadro’s number 6.023E23 molecules/gmol

Then the density of air containing 1012 molecules per mm3 is, in SI units,

 = 1012 molecules  4.81E−23 
molecule 
g
 3 
mm
  
g = 4.81E−5 kg
= 4.81E−11
mm3 m3
Finally, from the perfect gas law, Eq. (1.13), at 20C = 293 K, we obtain the pressure:
 kg  2 
p =  RT =  4.81E−5 3   287 m (293 K) = 4.0 Pa ns.
 m  s 2
K





Copyright © McGraw-Hill Education. All rights reserved. No reproduction or distribution without the prior written consent of
McGraw-Hill Education.

, Chapter 1 • Introduction 1-2



P1.2 Table A.6 lists the density of the standard atmosphere as a function of altitude. Use
these values to estimate, crudely, say, within a factor of 2, the number of molecules of air in
the entire atmosphere of the earth.

Solution: Make a plot of density  versus altitude z in the atmosphere, from Table A.6:


1.2255 kg/m3
Density in the Atmosphere




0 z 30,000 m

This writer’s approximation: The curve is approximately an exponential,   o exp(-bz), with
b approximately equal to 0.00011 per meter. Integrate this over the entire atmosphere, with the
radius of the earth equal to 6377 km:
m =  d (vol)  
[ e−b z ](4 R2 dz) =
atmosphere  0 o earth

o 4 Rearth
2
(1.2255 kg / m3 )4 (6.377E6 m)2
= =  5.7E18 kg
b 0.00011 / m

Dividing by the mass of one molecule  4.8E−23 g (see Prob. 1.1 above), we obtain
the total number of molecules in the earth’s atmosphere:

N molecules =
m(atmosphere)
=
5.7E21 grams  1.2Ε44 molecules Ans.
m(one molecule) 4.8E−23 gm/molecule

This estimate, though crude, is within 10 per cent of the exact mass of the atmosphere.




Copyright © McGraw-Hill Education. All rights reserved. No reproduction or distribution without the prior written consent of
McGraw-Hill Education.

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