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Complete Solution Manual for Fundamentals of Physics Extended (10th Edition) – Halliday, Resnick, and Walker (Chapters 1–10)

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This exhaustive solution manual provides detailed, step-by-step mathematical and conceptual guidance for the first ten chapters of Fundamentals of Physics Extended, 10th Edition. The resource follows a structured "THINK, EXPRESS, ANALYZE, LEARN" framework to help students master complex problem-solving in calculus-based physics. It covers a wide array of topics, from fundamental measurements to advanced rotational dynamics. Key highlights of this resource include: • Measurement and Units: Exhaustive analysis of unit conversions (e.g., furlongs to chains, picas to points) and geometric calculations for the circumference, surface area, and volume of Earth. • Kinematics (1D, 2D, and 3D): Solutions for average velocity, instantaneous speed, and constant acceleration problems. Includes complex projectile motion scenarios (divers, athletes, and fired projectiles) and relative motion analysis for planes and ships. • Vector Mechanics: Mastery of unit-vector notation, calculating magnitudes/directions, and performing dot and cross products. • Dynamics and Newton’s Laws: Detailed Free-Body Diagrams (FBD) for systems involving tension, normal forces, and multiple blocks. • Friction and Drag Forces: Comprehensive guidance on coefficients of static and kinetic friction, terminal speed, and the physics of banked curves. • Work and Energy: Step-by-step application of the work-kinetic energy theorem, Hooke’s Law for springs, and conservation of mechanical energy in conservative and non-conservative systems. • Momentum and Collisions: Analysis of center of mass, impulse-momentum theorem, and various elastic and inelastic collisions. • Rotational Dynamics: Solutions for angular acceleration, rotational inertia (Parallel-Axis Theorem), torque, and rotational kinetic energy for various rigid bodies like disks, rods, and spheres. This manual is an essential tool for engineering and physics students looking to excel in their coursework and master the principles of classical mechanics.

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1




Soluton_ManualFundamentals_of_Physics_Extended_10th_EVdi
tion


1. THINKVInVthisVproblemVwe’reVgivenVtheVradiusVofVEarth,VandVaskedVtoVcompu
teVitsVcircumference,VsurfaceVareaVandVvolume.


EXPRESSVAssumingVEarthVtoVbeVaVsphereVofVradius



RV =EV(6.37VV106Vm)(10−3Vkm m)V=V6.37VV103V km,



theVcorrespondingVcircumference,VsurfaceVareaVandVvolumeVare:
V4V
CV=V2VRV , AV=V4VR2V, VV =V R3V.
E E E
3
TheVgeometricVformulasVareVgivenVinVAppendixVE.




ANALYZEV(a)VUsingVtheVformulasVgivenVabove,VweVfindVtheVcirc
umferenceVtoVbe

CV=V2VRE =V2V(6.37VV103V km)V=V4.00104V km.


(b) Similarly,VtheVsurfaceVareaVofVEarthVis

AV=V4VE =V4V(6.37VV103V km) =V5.10VV108V km2V,
2V


(c) andVitsVvolumeVi R2
s

,2


(6.37VV103Vkm)
3V
V4V =V1.08VV1012V km3.
VVV4=V R3V =
V E
3 3


LEARNVFromVtheVformulasVgiven,VweVseeVthatV C ,V A R2V,VandV V R3V.VTheVratiosVofVvolume
RE E E

toVsurfaceVarea,VandVsurfaceVareaVtoVcircumferenceVareV VV/VAV=VREV /V3V andV AV/VCV=V2REV .



2. TheVconversionVfactorsVare:V1VgryV=V1/10 V line V,V1Vline V=V1/12 V inch VandV1VpointV=V1/
72Vinch.VTheVfactorsVimplyVthat



1VgryV=V(1/10)(1/12)(72Vpoints)V=V0.60Vpoint.



Thus,V1V gry2V=V(0.60Vpoint)2V =V 0.36Vpoint2,VwhichVmeansVthatV 0.50V gry2V=V 0.18V point 2 V.



3. TheVmetricVprefixesV(micro,Vpico,Vnano,V…)VareVgivenVforVreadyVreferenceVonVtheVinside
VfrontVcoverVofVtheVtextbookV(seeValsoVTableV1–2).




(a) SinceV1VkmV=V1VV103VmVandV1VmV=V1VV106Vm,



1kmV=V103VmV=V(103Vm) Vm m.
m)V=V109
(106

TheVgivenVmeasurementVisV1.0VkmV(twoVsignificantVfigures),VwhichVimpliesVourVresultVshould
VbeVwrittenVasV1.0VV109Vm.




(b) WeVcalculateVtheVnumberVofVmicronsVinV1Vcentimeter.VSinceV1VcmV=V10−2Vm,


1cmV=V10−2VmV=V(10−2m)(106VVm m.
m)V=V104


WeVconcludeVthatVtheVfractionVofVoneVcentimeterVequalVtoV1.0VmVisV1.0VV10−4.

, 3




(c) SinceV1VydV=V(3Vft)(0.3048Vm/ft)V=V0.9144Vm,


1.0VydV=V(0.91m)(106VVm m)V=V9.1VV105V m.

4. (a)VUsingVtheVconversionVfactorsV1VinchV=V2.54VcmVexactlyVandV6VpicasV=V1Vinch,V weVobtai
n V 1VinchV  V6V picasVV
0.80VcmV=V (0.80Vcm V)V  V  V1.9V picas.
2.54V cmV 1VinchV
  
(b)VWithV12VpointsV=V1Vpica,VweVhave

V 1VinchV  V6V picasV V12V pointsVV
0.80VcmV=V (0.80Vcm)VV2.54VcmV V 1VinchV  V V 1Vpica V 23Vpoints.
   


5. THINKVThisVproblemVdealsVwithVconversionVofVfurlongsVtoVrodsVandVchains,VallVofVwhi
chVareV unitsVforVdistance.


EXPRESSV GivenV thatV 1Vfurlo =V 201.168Vm,V1VrodV=V5.029 andV 1VchainV=V20.117V mV,V the
ngVrelevantVconversionVfactorsV 2Vm
are
1Vrod
1.0VfurlongV =V201.168VmV=V(201.168 =V40V rods,
VmV)
5.0292 m

and
1Vchai =10VchainsV.
1.0VfurlongV =V201.168VmV=V(201.168V nm
mV)
20.117

NoteVtheVcancellationVofVmV(meters),VtheVunwantedVunit.



ANALYZEVUsingVtheVaboveVconversionVfactors,VweVfind


40
(a) theVdistanceVdVinVrodsVtoVbeV dV =V 4.0VfurlongsV =(4.0Vfurlongs)V =V160V rods,
Vrods

1Vfurlong
10VchainsV
(b) andVinVchainsVtoV dV =V 4.0V furlongsV =(4.0Vfurlongs) =V 40V chains.
be 1Vfurlong

, 4


LEARNVSinceV4VfurlongsVisVaboutV800Vm,VthisVdistanceVisVapproximatelyVequalVtoV160VrodsV(
1VrodV V 5VmV)VandV40VchainsV(1VchainV V 20VmV).VSoVourVresultsVmakeVsense.



6. WeVmakeVuseVofVTableV1-6.



(a) WeVlookVatVtheVfirstV(“cahiz”)Vcolumn:V1VfanegaVisVequivalentVtoVwhatVamountVofVcahiz
?VWeVnoteVfromVtheValreadyVcompletedVpartVofVtheVtableVthatV1VcahizVequalsVaVdozenVfan
ega.V Thus,V1
fanegaV=V12V1VV cahiz,VorV8.33VV10−2Vcahiz.V Similarly,V“1VcahizV=V48Vcuartilla”V(inVtheValready

=VV1VVcahiz,VorV2.08VV10−2Vcahiz.V ContinuingVinVthis
completedVpart)VimpliesVthatV1VcuartillaV48
Vway,VtheVremainingVentriesVinVtheVfirstVcolumnVareV6.94VV10−3VandV 3.4710− V.
3




(b) InVtheVsecondV(“fanega”)Vcolumn,VweVfindV0.250,V8.33VV10−2,VandV4.17VV10−2VforVt
heVlastVthreeVentries.



(c) InVtheVthirdV(“cuartilla”)Vcolumn,VweVobtainV0.333VandV0.167VforVtheVlastVtwoVentries.



(d) Finally,VinVtheVfourthV(“almude”)Vcolumn,VweVgetV 1V =V0.500VforVtheVlastVentry.
2




(e) SinceVtheVconversionVtableVindicatesVthatV1ValmudeVisVequivalentVtoV2Vmedios,VourVamountVof
7.00ValmudesVmustVbeVequalVtoV14.0Vmedios.



(f) UsingVtheVvalueV(1ValmudeV=V6.94VV10−3Vcahiz)VfoundVinVpartV(a),VweVconcludeVtha
tV7.00ValmudesVisVequivalentVtoV4.86VV10−2Vcahiz.


(g) SinceVeachVdecimeterVisV0.1Vmeter,VthenV55.501VcubicVdecimetersVisVequalVtoV0.055501V
m3VorV55501Vcm3.V Thus,V7.00ValmudesV=V7.00V fanegaV=V7.00V(55501Vcm3)V=V3.24VV104Vcm3.
12 12

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