Mechanics

Essential formulas and concepts in mechanics

Projectile Range (level ground)

\(R = \frac{v_0^2 \sin(2\theta)}{g}\)

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Newton’s Second Law

\(\mathbf{F}_{\text{net}} = m \mathbf{a}\)

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Fundamental law relating force, mass, and acceleration. It implies acceleration is proportional to net force and inversely proportional to mass.

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Weight (Force due to Gravity)

\(W = m g\)

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Weight is the gravitational force exerted on a mass by Earth (or another celestial body). It differs from mass; mass is constant, weight depends on local \(g\).

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Momentum

\(\displaystyle \mathbf{p} = m \mathbf{v}\)

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Impulse

\(\mathbf{J} = \Delta \mathbf{p} = \mathbf{F}_{\text{avg}}\,\Delta t\)

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Momentum is the quantity of motion (mass times velocity). Impulse is the effect of a force acting over time, equal to the change in momentum. These are illustrated by collisions: e.g., a longer impact time reduces force for the same momentum change (crumple zones in cars).

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Work (Constant Force)

\(W = F\,d \,\cos\theta\)

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Power

\(P = \frac{W}{t} = F v \cos\theta\)

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Power is the rate of energy transfer or work done per second (measured in Watts). For example, 1 watt = 1 joule/second. The \(Fv\) form is useful for constant forces (e.g., power required to lift an object at constant speed). Often visualized with mechanical engines or electrical power calculations.

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Newton’s Law of Universal Gravitation

\(F = G \frac{m_1 m_2}{r^2}\)

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Every mass exerts an attractive force on every other mass. This inverse-square law explains planetary orbits, moon’s gravity, etc.

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Gravitational Potential Energy (two masses)

\(U(r) = -\,G \frac{m_1 m_2}{r}\)

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  • \(Same m_1, m_2, r, G as above. The negative sign indicates that the potential energy is zero at infinite separation and becomes more negative as masses come closer (bound state).\)

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Energy associated with two masses in a gravitational field. As \(r\) decreases, \(U\) decreases (becomes more negative), meaning work would be required to separate them. Often visualized as a well or curve approaching 0 at infinity and dipping down as \(r\) decreases.

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Moment of Inertia (for discrete masses)

\(I = \sum m_i r_i^2\)

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  • \(m_i are point masses in the object, r_i is each mass’s distance to the axis of rotation. I depends on the axis chosen.\)

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Moment of inertia is rotational inertia, representing how mass is distributed relative to the axis. It appears in rotational dynamics (\(I\) plays the role of \(m\)). For example, a solid disk vs. a hoop of equal mass have different \(I\) about the center (hoop has more mass at perimeter, larger \(I\)).

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Rotational Dynamics

\(\tau_{\text{net}} = I \alpha\)

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This is the rotational analogue of \(F=ma\). It states that net torque produces angular acceleration proportional to the moment of inertia. For example, it requires more torque to spin up a heavier or more extended object at the same rate.

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Angular Momentum (rotational)

\(L = I \omega\)

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Rotational Kinetic Energy

\(K_{\text{rot}} = \tfrac{1}{2} I \omega^2\)

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