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Chapter 6 Learning Objectives

Concepts and Skills to Review

  • Gravitational forces (Section 2.5)
  • Newton's second law: force and acceleration (Section 3.4)
  • Falling objects (Section 3.6)
  • Components of vectors in two dimensions (Section 4.2)
  • Circular orbits (Section 5.4)

Summary

  • The principle of conservation of energy states that energy can be converted from one form to another, but the total energy in an isolated system never changes.
  • The work done by a constant force is
      W = FΔr cos θ(6-1)
    where Δr is the displacement of the point of application of the force and θ is the angle between the force and displacement vectors.
  • The kinetic energy of an object of mass m moving with speed v is
     <a onClick="window.open('/olcweb/cgi/pluginpop.cgi?it=gif:: ::/sites/dl/free/0070524076/57989/image6_4.gif','popWin', 'width=NaN,height=NaN,resizable,scrollbars');" href="#"><img valign="absmiddle" height="16" width="16" border="0" src="/olcweb/styles/shared/linkicons/image.gif"> (0.0K)</a> (6-4)
  • Work done during a small displacement (variable forces) is
     ΔW = FxΔx(6-9)
  • The change in potential energy is equal to the negative of the work done by the conservative force that stores the potential energy
     ΔU = -Wc(6-14)
    Why the minus sign? If the force does positive work, it takes energy from its stored potential energy and gives it away in some other form; therefore for a positive Wc , ΔU must be negative.
  • The elastic potential energy of an ideal spring of spring constant k and stretched or compressed a distance x from its relaxed length is
     <a onClick="window.open('/olcweb/cgi/pluginpop.cgi?it=gif:: ::/sites/dl/free/0070524076/57989/image6_11.gif','popWin', 'width=NaN,height=NaN,resizable,scrollbars');" href="#"><img valign="absmiddle" height="16" width="16" border="0" src="/olcweb/styles/shared/linkicons/image.gif"> (0.0K)</a> (6-11)
  • The gravitational potential energy for an object of mass m raised a distance h above some reference level near Earth's surface, where h is small relative to the radius of the Earth, is
     U = mgh(6-12)
    if we choose U = 0 where h = 0.
  • The gravitational potential energy as a function of the distance between the two bodies of masses m1 and m2 whose centers are separated by a distance r is
     <a onClick="window.open('/olcweb/cgi/pluginpop.cgi?it=gif:: ::/sites/dl/free/0070524076/57989/image6_13.gif','popWin', 'width=NaN,height=NaN,resizable,scrollbars');" href="#"><img valign="absmiddle" height="16" width="16" border="0" src="/olcweb/styles/shared/linkicons/image.gif"> (1.0K)</a> (6-13)
    where U = 0 at r = infinity.
  • The work done by a conservative force on an object does not depend on the path taken, but only on the initial and final positions of the object.
  • The principle of conservation of mechanical energy states that for a system on which only conservative forces act, the sum of the kinetic and potential energies is constant.
     E = K + U(6-15a)
     ΔE = ΔK + ΔU = 0(6-15b)
  • The work done on a point particle by nonconservative forces is equal to the change in the mechanical energy:
     Wnc = ΔE =ΔK + ΔU (6-16)
  • Average power is the average rate of energy transfer.
     <a onClick="window.open('/olcweb/cgi/pluginpop.cgi?it=gif:: ::/sites/dl/free/0070524076/57989/image6_17.gif','popWin', 'width=NaN,height=NaN,resizable,scrollbars');" href="#"><img valign="absmiddle" height="16" width="16" border="0" src="/olcweb/styles/shared/linkicons/image.gif"> (0.0K)</a> (6-17)
    The instantaneous rate at which a force does work is the instantaneous power P:
     P = Fv cos θ(6-18)
  • The SI unit of work and energy is the joule. 1 J = 1 N·m.
    The SI unit of power is the watt. 1 W = 1 J/s.







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