
Newton’s Second Law states that the net external force acting on an object equals the rate of change of its momentum.
General form:
\(\Sigma{\vec{F}}=\frac{d\vec{p}}{dt}\)
where:
For constant mass:
\(\vec{p}=m\vec{v}\)
Substituting into the momentum form:
\(\Sigma\vec{F}=\frac{d(m/vec{v})}{dt}\)
If mass is constant:
\(\Sigma\vec{F}=m\frac{d(m/vec{v})}{dt}\)
Since
\(\vec{a}=\frac{d\vec{v}}{dt}\)
we obtain the familiar equation:
\(\Sigma\vec{F}=m\vec{a}\)
Newton’s Second Law explains how forces change motion.
Key ideas:
Force and acceleration are vectors.
Thus Newton’s Second Law applies separately along each axis:
\(\SignaF_x=ma_x\)
\(\SignaF_y=ma_y\)
\(\SignaF_z=ma_z\)
SI unit of force:
\(1N=1kg\cdot m/s^2\)
A force of 1 newton produces an acceleration of 1 m/s² on a 1kg object.
To apply Newton’s Second Law, we draw a free-body diagram (FBD).
An FBD shows:
Typical forces include:
A box of mass mmm is pushed with force FFF on a frictionless surface.
Net force:
\(\Sigma{F_x}=F\)
Using Newton’s Second Law:
\(F=ma\)
Acceleration:
\(a=\frac{F}{m}\)
If the net force is zero:
\(\Sigma\vec{F}=0\)
then:
\(\vec{a}=0\)
This corresponds to Newton’s First Law.
The momentum form:
\(\Sigma{\vec{F}}=\frac{d\vec{p}}{dt}\)
is more general and remains valid even when mass changes.
This becomes important in advanced mechanics topics such as rocket motion.
Newton’s Second Law provides the direct connection between:
It explains why:
General form:
\(\Sigma{\vec{F}}=\frac{d\vec{p}}{dt}\)
Constant-mass form:
\(\Sigma\vec{F}=m\vec{a}\)
Key ideas:
Newton’s Second Law is the central mathematical law of classical mechanics and forms the foundation for solving dynamics problems.
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