| | The second law relates force and [[momentum]]. Mathematically, <math>F = dp/dt = d(m*v)/dt = m*dv/dt + v*dm/dt</math>. Usually <math>dm/dt=0</math>, so the law is simplified to <math>F = m*dv/dt = m*a</math>, or mass times acceleration. A notable exception is [[rocket]] motion, where <math>dm/dt</math> is not 0, and so <math>F = m*a</math> does not apply. Note that the quantities '''F''', '''p''', '''v''', and '''a''' are all [[vector]] quantities--that is, they have an associated direction as well as a magnitude. In general, the second law gives a way to predict the motion of an object by summing all the forces acting on that object. | | The second law relates force and [[momentum]]. Mathematically, <math>F = dp/dt = d(m*v)/dt = m*dv/dt + v*dm/dt</math>. Usually <math>dm/dt=0</math>, so the law is simplified to <math>F = m*dv/dt = m*a</math>, or mass times acceleration. A notable exception is [[rocket]] motion, where <math>dm/dt</math> is not 0, and so <math>F = m*a</math> does not apply. Note that the quantities '''F''', '''p''', '''v''', and '''a''' are all [[vector]] quantities--that is, they have an associated direction as well as a magnitude. In general, the second law gives a way to predict the motion of an object by summing all the forces acting on that object. |
| − | The third law states that momentum is always conserved. If one object imparts a momentum p<sub>0</sub> on another, the first object's momentum will change by -p<sub>0</sub>. This can be viewed as a consequence of [[Noether's Theorem]]; the associated [[symmetry]] is that the laws of physics do not change over small time periods. | + | The third law states that momentum is always conserved. If one object imparts a momentum p<sub>0</sub> on another, the first object's momentum will change by -p<sub>0</sub>. This can be viewed as a consequence of [[Noether's Theorem]]; the associated [[symmetry]] is that the laws of physics do not change under spatial translations (that is, the laws of physics are the same everywhere). |