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Physics: Classical Mechanics

Explore Newton's laws of motion, kinematics, and fundamental physics equations with clear mathematical formulations.

Physics: Classical Mechanics

Introduction

Classical mechanics describes the motion of macroscopic objects. From falling apples to orbiting planets, the equations of mechanics govern the physical world around us.


Kinematics: Motion in One Dimension

Position and Displacement

The position of an object is described by x(t)x(t), a function of time. Displacement is:

Δx=xfxi\Delta x = x_f - x_i

Velocity

Average velocity:

vˉ=ΔxΔt\bar{v} = \frac{\Delta x}{\Delta t}

Instantaneous velocity:

v=dxdtv = \frac{dx}{dt}

Acceleration

Average acceleration:

aˉ=ΔvΔt\bar{a} = \frac{\Delta v}{\Delta t}

Instantaneous acceleration:

a=dvdt=d2xdt2a = \frac{dv}{dt} = \frac{d^2x}{dt^2}


Kinematic Equations

For constant acceleration aa, we have the four kinematic equations:

v=v0+atv = v_0 + at

x=x0+v0t+12at2x = x_0 + v_0 t + \frac{1}{2}at^2

v2=v02+2a(xx0)v^2 = v_0^2 + 2a(x - x_0)

x=x0+12(v0+v)tx = x_0 + \frac{1}{2}(v_0 + v)t

where:

  • v0v_0 = initial velocity
  • vv = final velocity
  • aa = acceleration
  • tt = time
  • x0x_0 = initial position
  • xx = final position

Interactive: Projectile Motion

The chart below shows position vs. time for an object dropped from rest (no air resistance, g=9.8m/s2g = 9.8 \, \text{m/s}^2):

Free Fall: Position vs Time

And here is the corresponding velocity vs. time graph (v=gtv = gt):

Free Fall: Velocity vs Time

Newton's Laws of Motion

First Law (Inertia)

An object at rest stays at rest, and an object in motion stays in motion with the same speed and direction, unless acted upon by an unbalanced force.

Second Law (Force and Acceleration)

The net force on an object equals its mass times its acceleration:

F=ma\sum \vec{F} = m\vec{a}

This is the fundamental equation of mechanics. From it, we can derive:

a=Fm\vec{a} = \frac{\sum \vec{F}}{m}

m=Fam = \frac{\sum \vec{F}}{\vec{a}}

Third Law (Action-Reaction)

For every action, there is an equal and opposite reaction:

F12=F21\vec{F}_{12} = -\vec{F}_{21}


Types of Forces

Gravitational Force

Newton's law of universal gravitation:

Fg=Gm1m2r2F_g = G\frac{m_1 m_2}{r^2}

where G=6.674×1011N⋅m2/kg2G = 6.674 \times 10^{-11} \, \text{N·m}^2/\text{kg}^2.

Near Earth's surface:

Fg=mgF_g = mg

where g=9.8m/s2g = 9.8 \, \text{m/s}^2.

Normal Force

The normal force FNF_N acts perpendicular to a surface. For an object on a flat surface:

FN=mgF_N = mg

Friction

Static friction:

fsμsFNf_s \leq \mu_s F_N

Kinetic friction:

fk=μkFNf_k = \mu_k F_N

where μs\mu_s and μk\mu_k are the coefficients of static and kinetic friction.

Spring Force (Hooke's Law)

Fs=kxF_s = -kx

where kk is the spring constant and xx is the displacement from equilibrium.


Work and Energy

Work

Work done by a constant force:

W=FdcosθW = Fd\cos\theta

where θ\theta is the angle between the force and displacement vectors.

Kinetic Energy

KE=12mv2KE = \frac{1}{2}mv^2

Potential Energy

Gravitational potential energy:

PEg=mghPE_g = mgh

Elastic potential energy:

PEs=12kx2PE_s = \frac{1}{2}kx^2

Work-Energy Theorem

Wnet=ΔKE=KEfKEiW_{net} = \Delta KE = KE_f - KE_i

Conservation of Energy

KEi+PEi=KEf+PEfKE_i + PE_i = KE_f + PE_f

12mvi2+mghi=12mvf2+mghf\frac{1}{2}mv_i^2 + mgh_i = \frac{1}{2}mv_f^2 + mgh_f


Momentum and Impulse

Linear Momentum

p=mv\vec{p} = m\vec{v}

Impulse

J=FΔt=Δp\vec{J} = \vec{F}\Delta t = \Delta\vec{p}

Conservation of Momentum

For an isolated system:

m1v1i+m2v2i=m1v1f+m2v2fm_1\vec{v}_{1i} + m_2\vec{v}_{2i} = m_1\vec{v}_{1f} + m_2\vec{v}_{2f}


Interactive Simulation: Forces and Motion

Experiment with the simulation below to see Newton's laws in action. Apply different forces to objects and observe how they accelerate.

Forces and Motion: BasicsOpen fullscreen ↗
Loading simulation...
Simulation by PhET Interactive Simulations, University of Colorado Boulder
💡Tip

Try applying different forces to the objects. Notice how heavier objects accelerate more slowly for the same force — this is Newton's Second Law in action!


3D Molecular Viewer

Explore the 3D structure of Crambin (PDB: 1CRN), a small plant protein with 46 amino acids. Drag to rotate, scroll to zoom, and right-click to pan.

Crambin (1CRN)View on RCSB PDB ↗
Loading molecule...
Structure: 1CRNDrag to rotate · Scroll to zoom · Right-click to pan
ℹ️Note

Molecular structures are loaded from the RCSB Protein Data Bank. You can replace 1CRN with any valid PDB ID (e.g., 4HHB for hemoglobin, 1IGT for an antibody).


Practice Questions

Practice Question

A car accelerates from rest at 2 m/s² for 5 seconds. What is its final velocity?

Practice Question

According to Newton's Second Law, if you double the force on an object, what happens to its acceleration?

Practice Question

A 5 kg object is lifted 3 meters. What is its gravitational potential energy? (g = 10 m/s²)


Interactive Exercises

Drag-and-Drop: Order the Kinematic Steps

Put these steps in the correct order for solving a kinematics problem:

Ordering Question

Order these steps for solving a kinematics problem:

Choose the correct kinematic equation
Plug in values and solve
Identify knowns and unknowns
Check units and reasonableness

Matching: Newton's Laws

Match each law of motion with its correct statement:

Matching Question

Match each law of motion with its statement:

First Law
Drop here
Second Law
Drop here
Third Law
Drop here

Drag answers from here:

F = ma
An object at rest stays at rest unless acted upon
For every action there is an equal and opposite reaction

Fill in the Blanks: Energy Conservation

Fill in the Blanks

Complete the conservation of energy equation:

The total blank energy equals the total blank energy: KE_i + PE_i = KE_f + PE_f. Kinetic energy is blankmv² and gravitational potential energy is blank.

Word Bank — drag words into the blanks above:

final
thermal
½
gh²
mgh
initial
mechanical
mv

Success

Key Takeaways

  • Kinematics equations describe motion with constant acceleration: v=v0+atv = v_0 + at and x=x0+v0t+12at2x = x_0 + v_0 t + \frac{1}{2}at^2
  • Newton's Second Law: F=ma\sum \vec{F} = m\vec{a}
  • Work: W=FdcosθW = Fd\cos\theta; Kinetic Energy: KE=12mv2KE = \frac{1}{2}mv^2
  • Energy is conserved: KEi+PEi=KEf+PEfKE_i + PE_i = KE_f + PE_f
  • Momentum is conserved in isolated systems
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