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| | <math>\Sigma \vec F = m \vec a</math> where | | <math>\Sigma \vec F = m \vec a</math> where |
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| − | * <math>\Sigma \vec F</math> = total force acting on the object | + | * <math>\Sigma \vec F</math> is the net [[force]] acting on the object |
| − | * m = mass of the object | + | * <math>m</math> is the mass of the object |
| − | * <math>\vec a</math> = acceleration of the object | + | * <math>\vec a</math> is the acceleration of the object |
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| | This law also applies to a system of objects. | | This law also applies to a system of objects. |
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| | Newton originally wrote this as | | Newton originally wrote this as |
| | :<math>\Sigma \vec F = \frac{d \vec p}{dt}</math> | | :<math>\Sigma \vec F = \frac{d \vec p}{dt}</math> |
| − | where <math>\vec p</math> is the [[momentum]] of the object. Momentum is defined as mass times velocity, p = m*v. This formulation is more general. It reduces to F = m*a when the object has a constant mass. | + | where <math>\vec p</math> is the [[momentum]] of the object. Momentum is defined as mass times velocity, <math> \vec p = m \vec{v}</math> This formulation is more general. It reduces to <math>\vec F = m \vec{a}</math> when the object has a constant mass. |
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| | '''3. For every action, there is an equal and opposite reaction.''' | | '''3. For every action, there is an equal and opposite reaction.''' |
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| − | If object A exerts a force on object B, object B will exert a force equal in magnitude and opposite in direction on object A. For example, ff the earth pulls you down with a force of 1500 Newtons, you pull up on the earth with a force of 1500 Newtons. (Of course, since F=ma, and the earth's mass is much greater than yours, the earth accelerates much less than you do.) | + | If object A exerts a force on object B, object B will exert a force equal in magnitude and opposite in direction on object A. For example, if the earth pulls you down with a force of 1500 Newtons, you pull up on the earth with a force of 1500 Newtons. (Of course, since <math>\vec F = m \vec{a}</math>, and the earth's mass is much greater than yours, the earth accelerates much less than you do.) |
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| | == Angular Kinematics == | | == Angular Kinematics == |
| | These same basic laws are true with respect to angular motion, that is, for a particle moving in a circle. In this case, the position is described by an angle, and is measured in [[radian]]s. Its first derivative, ω (measured in radians/second), is called angular velocity; its second derivative α is called angular acceleration. The kinematic equations of rotational motion are analogous to those of linear motion: | | These same basic laws are true with respect to angular motion, that is, for a particle moving in a circle. In this case, the position is described by an angle, and is measured in [[radian]]s. Its first derivative, ω (measured in radians/second), is called angular velocity; its second derivative α is called angular acceleration. The kinematic equations of rotational motion are analogous to those of linear motion: |