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PROBLEM WORKBOOK - AP-SAT Tutorial

PROBLEMWORKBOOKC over Photo: Lawrence Manning/CORBISC over Design: Jason WilsonCopyright by Holt, Rinehart and WinstonAll rights reserved. No part of this publication may be reproduced or transmittedin any form or by any means, electronic or mechanical, including photocopy,recording, or any information storage and retrieval system, without permission inwriting from the using HOLT PHYSICS may photocopy blackline masters in completepages in sufficient quantities for classroom use only and not for in the United States of AmericaISBN 0-03-057337-81 2 3 4 5 6 095 05 04 03 02 01 Holt PhysicsProblem WorkbookThis WORKBOOK contains additional worked-out samples and practiceproblems for each of the PROBLEM types from the Holt WritersBoris M.

ADDITIONAL PRACTICE 1. One light-year is the distance light travels in one year. This distance is equal to 9.461 × 1015 m. After the sun, the star nearest to Earth is Alpha Centauri, which is about 4.35 light-years from Earth. Express this dis- ... 4 Holt Physics Problem Workbook.

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Transcription of PROBLEM WORKBOOK - AP-SAT Tutorial

1 PROBLEMWORKBOOKC over Photo: Lawrence Manning/CORBISC over Design: Jason WilsonCopyright by Holt, Rinehart and WinstonAll rights reserved. No part of this publication may be reproduced or transmittedin any form or by any means, electronic or mechanical, including photocopy,recording, or any information storage and retrieval system, without permission inwriting from the using HOLT PHYSICS may photocopy blackline masters in completepages in sufficient quantities for classroom use only and not for in the United States of AmericaISBN 0-03-057337-81 2 3 4 5 6 095 05 04 03 02 01 Holt PhysicsProblem WorkbookThis WORKBOOK contains additional worked-out samples and practiceproblems for each of the PROBLEM types from the Holt WritersBoris M.

2 KorsunskyPhysics InstructorScience DepartmentNorthfield Mount Hermon SchoolNorthfield, MAAngela BerensteinScience WriterUrbana, ILJohn StokesScience WriterSocorro, NMCopyright by Holt, Rinehart and Winston. All rights and Practice 1 AMetric Prefixes.. 1 Sample and Practice 2 AAverage Velocity and Displacement.. 3 Sample and Practice 2 BAverage Acceleration.. 5 Sample and Practice 2 CDisplacement with Constant Acceleration.. 7 Sample and Practice 2 DVelocity and Displacement with ConstantAcceleration.. 9 Sample and Practice 2 EFinal Velocity After Any Displacement.. 12 Sample and Practice 2 FFalling Object.. 14 Sample and Practice 3 AFinding Resultant Magnitude and Direction.. 16 Sample and Practice 3 BResolving Vectors.

3 18 Sample and Practice 3 CAdding Vectors Algebraically.. 20 Sample and Practice 3 DProjectiles Launched Horizontally.. 22 Sample and Practice 3 EProjectiles Launched at an Angle.. 24 Sample and Practice 3 FRelative Velocity.. 27 Sample and Practice 4 ANet External Force.. 29 Sample and Practice 4 BNewton s Second Law.. 31 Sample and Practice 4 CCoefficients of Friction.. 35 Sample and Practice 4 DOvercoming Friction.. 37 Sample and Practice 5 AWork.. 39 Sample and Practice 5 BKinetic Energy.. 42 Sample and Practice 5 CWork-Kinetic Energy Theorem.. 44 Sample and Practice 5 DPotential Energy.. 47 Sample and Practice 5 EConservation of Mechanical Energy.. 50 Sample and Practice 5 FPower.. 53 Sample and Practice 6 AMomentum.

4 54 Sample and Practice 6 BForce and Impulse.. 56 Sample and Practice 6 CStopping Distance.. 58 Sample and Practice 6 DConservation of Momentum.. 60 Sample and Practice 6 EPerfectly Inelastic Collision.. 63 Sample and Practice 6 FKinetic Energy in PerfectlyInelastic Collisions.. 66 Sample and Practice 6 GElastic Collisions.. 68 Sample and Practice 7 AAngular Displacement.. 70 Sample and Practice 7 BAngular Speed.. 72 ContentsContentsivSectionTitlePageSample and Practice 7 CAngular Acceleration .. 73 Sample and Practice 7 DAngular Kinematics.. 75 Sample and Practice 7 ETangential Speed.. 77 Sample and Practice 7 FTangential Acceleration .. 79 Sample and Practice 7 GCentripetal Acceleration.. 80 Sample and Practice 7 HForce That Maintains Circular Motion.

5 81 Sample and Practice 7 IGravitational Force.. 83 Sample and Practice 8 ATorque.. 85 Sample and Practice 8 BRotational Equilibrium.. 88 Sample and Practice 8 CNewton's Second Law for Rotation.. 91 Sample and Practice 8 DConservation of Angular Momentum.. 94 Sample and Practice 8 EConservation of Mechanical Energy.. 96 Sample and Practice 9 ABuoyant Force.. 98 Sample and Practice 9 BPressure.. 100 Sample and Practice 9 CPressure as a Function of Depth.. 102 Sample and Practice 9 DBernoulli s Equation.. 104 Sample and Practice 9 EGas Laws.. 106 Sample and Practice 10 ATemperature Conversion.. 108 Sample and Practice 10 BConservation of Energy.. 109 Sample and Practice 10 CCalorimetry.. 111 Sample and Practice 10 DHeat of Phase Change.

6 113 Sample and Practice 11 AWork Done on or by a Gas.. 115 Sample and Practice 11 BThe First Law of Thermodynamics.. 116 Sample and Practice 11 CHeat-Engine Efficiency.. 118 Sample and Practice 12 AHooke s Law.. 119 Sample and Practice 12 BSimple Harmonic Motion of a Simple Pendulum.. 121 Sample and Practice 12 CSimple Harmonic Motion of a Mass-Spring System.. 122 Sample and Practice 12 DWave Speed.. 123 Sample and Practice 13 AIntensity of Sound Waves.. 124 Sample and Practice 13 BHarmonics.. 125 Sample and Practice 14 AElectromagnetic Waves.. 126 Sample and Practice 14 BConcave Mirrors.. 127 Sample and Practice 14 CConvex Mirrors.. 129 Copyright by Holt, Rinehart and Winston. All rights and Practice 15 ASnell s Law.

7 131 Sample and Practice 15 BLenses.. 132 Sample and Practice 15 CCritical Angle.. 135 Sample and Practice 16 AInterference.. 136 Sample and Practice 16 BDiffraction Gratings.. 138 Sample and Practice 17 ACoulomb s Law.. 140 Sample and Practice 17 BThe Superposition Principle.. 142 Sample and Practice 17 CEquilibrium.. 145 Sample and Practice 17 DElectric Field Strength.. 148 Sample and Practice 18 AElectrical Potential Energy.. 151 Sample and Practice 18 BPotential Difference.. 153 Sample and Practice 18 CCapacitance.. 156 Sample and Practice 19 ACurrent .. 159 Sample and Practice 19 BResistance.. 160 Sample and Practice 19 CElectric Power.. 161 Sample and Practice 19 DCost of Electrical Energy.. 162 Sample and Practice 20 AResistors in Series.

8 163 Sample and Practice 20 BResistors in Parallel.. 165 Sample and Practice 20 CEquivalent Resistance.. 167 Sample and Practice 20 DCurrent in and Potential DifferenceAcross a Resistor.. 171 Sample and Practice 21 AParticle in a Magnetic Field.. 174 Sample and Practice 21 BForce on a Current-Carrying Conductor.. 176 Sample and Practice 22 AInduced emf and Current.. 178 Sample and Practice 22 BInduction in Generators.. 180 Sample and Practice 22 Crms Currents and Potential Differences.. 182 Sample and Practice 22 DTransformers.. 184 Sample and Practice 23 AQuantum Energy.. 186 Sample and Practice 23 BThe Photoelectric Effect.. 188 Sample and Practice 23 CDe Broglie Waves.. 190 Sample and Practice 25 ABinding Energy.

9 191 Sample and Practice 25 BNuclear Decay.. 193 Sample and Practice 25 CMeasuring Nuclear Decay.. 195 Copyright by Holt, Rinehart and Winston. All rights material copyrighted under notice appearing earlier in this 1A1 NAME _____ DATE _____ CLASS _____Holt PhysicsProblem 1 AMETRIC PREFIXESPROBLEMIn Hindu chronology, the longest time measure is apara. One paraequals 311 040 000 000 000 years. Calculate this value in megahours and innanoseconds. Write your answers in scientific :1 para =311 040 000 000 000 yearsUnknown:1 para =? Mh1 para =? nsExpress the time in years in terms of scientific notation. Then build conversionfactors from the relationships given in Table para = 1014 years 124dahy 1 1M10h6h 124dahy 3610h0s 1 11n0s 9s Convert from years to megahours by multiplying the time by the first para = 1014 years 124dahy 1 1M10h6h =Convert from years to nanoseconds by multiplying the time by the second con-version para = 1014 years 124dahy 3610h0s 1 11n0s 9s = 1012 MhADDITIONAL light-year is the distance light travels in one year.

10 This distance isequal to 1015m. After the sun, the star nearest to Earth is AlphaCentauri, which is about light-years from Earth. Express this dis-tance Physics PROBLEM Workbook2 NAME _____ DATE _____ CLASS _____HRW material copyrighted under notice appearing earlier in this is estimated that the sun will exhaust all of its energy in about ten billion years. By that time, it will have radiated about 1044J (joules)of energy. Express this amount of energy smallest living organism discovered so far is called a is estimated as 10 16g. Express this mass extreme prefixes that are officially recognized are yocto, which in-dicates a fraction equal to 10 24, and yotta,which indicates a factor equalto 1024.


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