Free Christian Curriculum Kindergarten through twelfth grade · free to download

Grade 11 · 15 units · 180 lessons · 1,800 questions

Physics

Algebra-and-trigonometry-based physics in 180 lessons, from kinematics and Newton's laws through circuits, electromagnetism, and modern physics.

About this course

This is a full year of physics on its own, taught with algebra and trigonometry rather than calculus. It opens with SI units, scientific notation, dimensional analysis, measurement uncertainty, and vectors resolved into components, then runs one-dimensional kinematics, projectile motion at an angle, relative motion, circular motion, and simple harmonic motion; Newton's laws with friction, inclined planes, tension and pulleys, torque and static equilibrium, and Atwood machines; work, energy, power, simple machines, and rotational kinetic energy and angular momentum; momentum, impulse, and elastic and inelastic collisions; universal gravitation, Kepler's laws, orbital speed and period, escape velocity, and satellite applications; and fluid mechanics from hydrostatic pressure and Archimedes' principle through Bernoulli, viscosity, surface tension, and hydraulics. The second half covers thermal physics with calorimetry, latent heat, the laws of thermodynamics, PV diagrams, entropy, and heat engines; waves and sound with standing waves, resonance, beats, the Doppler effect, and decibels; light and optics with Snell's law, mirror and thin lens equations, total internal reflection, diffraction, interference, and polarization; electrostatics with Coulomb's law, fields, potential, and capacitors; circuits through Ohm's law, series and parallel networks, Kirchhoff's loop and node analysis, RC circuits, household AC, electrical safety, and multimeters; magnetism through the Lorentz force, motors, Faraday's and Lenz's laws, transformers, and the power grid; and a modern physics unit on the photoelectric effect, wave-particle duality, the Bohr model, fission and fusion, the Standard Model, and special relativity, closing with a lesson that treats natural law as the regular way God governs His creation.

There are 180 lessons in 15 units of 12, about 55 minutes each, one lesson per school day. A lesson states the law and its equations, often with a formula table, works two to four numerical problems in full with the units carried through, and ends with a KJV connection and a ten-question quiz that grades itself. One honest note on the daily rhythm: the lesson plan schedules a practice-problems block and the homework line asks your student to show all work, but most lessons supply worked examples rather than a printed problem set, so if you want daily graded problem work you will need to supply the problems yourself.

The mathematical demand is higher than a science course label usually implies. Trigonometry is in constant use from the first unit onward, in vector components, angled projectiles, banked curves, and Snell's law, and unit 1 includes a trigonometry review that is a refresher rather than a first teaching. A few kinematics lessons in unit 2 use derivative and integral notation directly. Algebra I and geometry should be finished, and your student is best served taking Algebra II or precalculus alongside this course rather than after it. There is also no lab: the listed materials are a pencil, graph paper, a scientific calculator, and a Bible, and although the course teaches experimental design, uncertainty propagation, and lab safety and describes apparatus such as a Van de Graaff generator, breadboards, and multimeters, no equipment is supplied and no experiment is assigned, so documented lab hours for a transcript must be arranged by you and your family. Freedom Homeschool also offers a general eleventh-grade science course covering chemistry, biology, the human body, earth science, astronomy, and environmental science along with a physics strand; that strand overlaps parts of this course, and most families will assign one or the other as the year's science rather than both.

What the course covers

What your student will be able to do

Scope and sequence

All 15 units of Physics for Grade 11, in the order they are taught.

Units in this course, in teaching order
UnitCoversLessonsQuestionsJump to lessons
Unit 1Introduction to Physics and Measurement12120Lessons
Unit 2Kinematics: Motion in One Dimension12120Lessons
Unit 3Kinematics: Motion in Two Dimensions12120Lessons
Unit 4Newton's Laws of Motion12120Lessons
Unit 5Work, Energy, and Power12120Lessons
Unit 6Momentum and Impulse12120Lessons
Unit 7Gravitation and Satellite Motion12120Lessons
Unit 8Fluid Mechanics12120Lessons
Unit 9Thermal Physics and Heat12120Lessons
Unit 10Waves and Sound12120Lessons
Unit 11Light and Optics12120Lessons
Unit 12Electricity and Static Charge12120Lessons
Unit 13Electric Circuits12120Lessons
Unit 14Magnetism and Electromagnetism12120Lessons
Unit 15Modern Physics and Comprehensive Review12120Lessons

Every lesson, by title

All 180 lesson titles are listed here — nothing is withheld until you download. Open a unit to read its contents.

Unit 1: Introduction to Physics and Measurement 12 lessons
  1. 1What Is Physics?10 q
  2. 2SI Units, Measurement, and Scientific Notation10 q
  3. 3Dimensional Analysis and Unit Conversions10 q
  4. 4Vectors and Scalars10 q
  5. 5Vector Addition: Component Method10 q
  6. 6Graphing in Physics and Measurement Uncertainty10 q
  7. 7Trigonometry Review for Physics10 q
  8. 8Scientific Notation and Order-of-Magnitude Estimates10 q
  9. 9Laboratory Skills and Experimental Design10 q
  10. 10Problem-Solving Strategy and Physics Connections10 q
  11. 11Physics in Technology and Daily Life10 q
  12. 12Unit 1 Review: Introduction to Physics10 q
Unit 2: Kinematics: Motion in One Dimension 12 lessons
  1. 1Position, Displacement, and Distance10 q
  2. 2Speed and Velocity10 q
  3. 3Acceleration10 q
  4. 4Kinematic Equations10 q
  5. 5Free Fall and Gravity10 q
  6. 6Motion Graphs and Problem Solving10 q
  7. 7Instantaneous Velocity from Position Functions10 q
  8. 8Reaction Time and Stopping Distance10 q
  9. 9Terminal Velocity and Non-Constant Acceleration10 q
  10. 10Multi-Stage Kinematics Problems10 q
  11. 11Kinematics with Variable Acceleration: Calculus Connections10 q
  12. 12Relative Motion and Unit 2 Review10 q
Unit 3: Kinematics: Motion in Two Dimensions 12 lessons
  1. 1Projectile Motion: Horizontal Launch10 q
  2. 2Projectile Motion: Angled Launch10 q
  3. 3Relative Motion in 2D and River-Crossing Problems10 q
  4. 4Circular Motion and Centripetal Acceleration10 q
  5. 5Parabolic Motion and Range Optimization10 q
  6. 6Circular Motion Applications: Banked Curves and Vertical Circles10 q
  7. 7Non-Uniform Circular Motion and Angular Kinematics10 q
  8. 8Two-Dimensional Collision Problems10 q
  9. 9Springs, Simple Harmonic Motion, and Pendulums10 q
  10. 10Unit 3 Review Extension: 2D Motion Mastery10 q
  11. 11Applications of 2D Motion: Sports, Ballistics, and Engineering10 q
  12. 12Unit 3 Review: 2D Kinematics10 q
Unit 4: Newton's Laws of Motion 12 lessons
  1. 1Newton's First Law: Inertia10 q
  2. 2Newton's Second Law: F = ma10 q
  3. 3Newton's Third Law and Free Body Diagrams10 q
  4. 4Friction, Normal Force, and Inclined Planes10 q
  5. 5Tension, Pulleys, and Newton's Laws Applied10 q
  6. 6Equilibrium: Statics and Torque10 q
  7. 7Apparent Weight and Elevator Problems10 q
  8. 8Newton's Laws on Inclined Planes with Multiple Forces10 q
  9. 9Newton's Laws Review: Complex Applications10 q
  10. 10Static Equilibrium: Torque, Levers, and the Balance of Forces10 q
  11. 11Newton's Laws in Complex Scenarios: Atwood Machines and Linked Systems10 q
  12. 12Circular Motion Forces and Unit 4 Review10 q
Unit 5: Work, Energy, and Power 12 lessons
  1. 1Work10 q
  2. 2Kinetic Energy and the Work-Energy Theorem10 q
  3. 3Potential Energy and Conservation of Energy10 q
  4. 4Power and Simple Machines10 q
  5. 5Energy in Springs and Elastic Systems10 q
  6. 6Power in Real Systems and Energy Efficiency10 q
  7. 7Conservation of Energy: Extended Applications10 q
  8. 8Machines, Mechanical Advantage, and Levers10 q
  9. 9Energy Sources and the Physics of Power Generation10 q
  10. 10Rotational Kinetic Energy and Angular Momentum10 q
  11. 11Energy Conservation in Complex Systems: Roller Coasters and Pendulums10 q
  12. 12Unit 5 Review: Work, Energy, and Power10 q
Unit 6: Momentum and Impulse 12 lessons
  1. 1Linear Momentum and Impulse10 q
  2. 2Conservation of Momentum10 q
  3. 3Elastic and Inelastic Collisions10 q
  4. 4Center of Mass and System Momentum10 q
  5. 5Impulse in Sports and Safety Engineering10 q
  6. 6Rockets, Explosions, and Recoil Physics10 q
  7. 7Inelastic Collisions and Energy Analysis10 q
  8. 8Two-Dimensional Collisions and Momentum Conservation10 q
  9. 9Angular Momentum and Rotational Collisions10 q
  10. 10Momentum in Astronomy: Stellar Formation and Galaxy Dynamics10 q
  11. 11Momentum Mastery: Multi-Concept Problem Solving10 q
  12. 12Unit 6 Review: Momentum and Impulse10 q
Unit 7: Gravitation and Satellite Motion 12 lessons
  1. 1Kepler's Laws and Universal Gravitation10 q
  2. 2Satellite Orbits and Orbital Mechanics10 q
  3. 3Gravitational Fields and Tides10 q
  4. 4Orbital Speed and Period: Calculating Satellite Orbits10 q
  5. 5Escape Velocity and Gravitational Potential Energy10 q
  6. 6Kepler's Third Law: Comparing Planetary Orbits10 q
  7. 7Weightlessness, Apparent Weight, and Artificial Gravity10 q
  8. 8Satellite Applications: GPS, Weather, and Communication10 q
  9. 9Gravitational Potential Energy and Energy Conservation in Orbits10 q
  10. 10Binary Star Systems and Galactic Structures10 q
  11. 11Gravitational Waves and Modern Astronomy10 q
  12. 12Unit 7 Review: Gravitation10 q
Unit 8: Fluid Mechanics 12 lessons
  1. 1Density, Pressure, and Pascal's Principle10 q
  2. 2Buoyancy and Archimedes' Principle10 q
  3. 3Fluid Flow: Continuity and Bernoulli's Principle10 q
  4. 4Pressure and Depth: Hydrostatic Pressure Applications10 q
  5. 5Archimedes' Principle: Buoyancy Calculations10 q
  6. 6Bernoulli's Principle: Lift, Carburetors, and Venturi10 q
  7. 7Viscosity and Turbulence in Real Fluids10 q
  8. 8Surface Tension and Capillary Action10 q
  9. 9Hydraulic Machines: Brakes, Presses, and Lifts10 q
  10. 10Atmospheric Pressure and Weather Patterns10 q
  11. 11Fluid Dynamics Problem-Solving Mastery10 q
  12. 12Unit 8 Review: Fluid Mechanics10 q
Unit 9: Thermal Physics and Heat 12 lessons
  1. 1Temperature, Thermal Expansion, and Heat10 q
  2. 2Specific Heat and Calorimetry10 q
  3. 3Phase Changes and Latent Heat10 q
  4. 4Heat Transfer: Conduction, Convection, Radiation10 q
  5. 5Laws of Thermodynamics10 q
  6. 6Thermodynamics: Processes and PV Diagrams10 q
  7. 7Entropy, Disorder, and the Arrow of Time10 q
  8. 8Heat Engines and Refrigerators10 q
  9. 9Kinetic Theory of Gases and the Ideal Gas Law10 q
  10. 10Real Gas Behavior and Applications of Thermodynamics10 q
  11. 11Thermal Energy in Earth Systems and Stewardship10 q
  12. 12Unit 9 Review: Thermal Physics10 q
Unit 10: Waves and Sound 12 lessons
  1. 1Wave Properties and Types10 q
  2. 2Sound, Resonance, and the Doppler Effect10 q
  3. 3Wave Behavior: Reflection, Refraction, and Diffraction10 q
  4. 4Superposition, Interference, and Beats10 q
  5. 5Standing Waves and Harmonics10 q
  6. 6Resonance in Musical Instruments10 q
  7. 7The Doppler Effect: Detailed Applications10 q
  8. 8Sound Intensity, Decibels, and Hearing10 q
  9. 9Ultrasound and Infrasound: Technology Applications10 q
  10. 10Seismic Waves and Earthquake Science10 q
  11. 11Waves in Creation: God's Design in Physical Laws10 q
  12. 12Unit 10 Review: Waves and Sound10 q
Unit 11: Light and Optics 12 lessons
  1. 1Nature of Light, Reflection, and Mirrors10 q
  2. 2Refraction, Snell's Law, and Lenses10 q
  3. 3Concave and Convex Mirrors: Ray Diagrams and Image Formation10 q
  4. 4Total Internal Reflection and Fiber Optics10 q
  5. 5Converging Lenses: Real Images and the Thin Lens Equation10 q
  6. 6Diverging Lenses and Lens Combinations10 q
  7. 7Dispersion and the Physics of Rainbows10 q
  8. 8Wave Nature of Light: Diffraction and Interference10 q
  9. 9Polarization and Its Applications10 q
  10. 10Optical Instruments: Microscopes, Telescopes, and the Eye10 q
  11. 11Colors, Pigments, and the Physics of Vision10 q
  12. 12Unit 11 Review: Light and Optics10 q
Unit 12: Electricity and Static Charge 12 lessons
  1. 1Electric Charge, Coulomb's Law, and Electric Fields10 q
  2. 2Electric Potential, Voltage, and Capacitance10 q
  3. 3Conductors, Insulators, and Methods of Charging10 q
  4. 4Electric Field Lines: Mapping Invisible Forces10 q
  5. 5Electric Potential Energy and the Electron Volt10 q
  6. 6Capacitors: Charge Storage and Applications10 q
  7. 7Charging and Discharging Capacitors10 q
  8. 8Lightning and Static Electricity in Nature10 q
  9. 9The Van de Graaff Generator and Electrostatics Lab10 q
  10. 10Electrostatics in Technology: Printers, Air Purifiers, and More10 q
  11. 11Electric Fields in the Human Body and Medical Applications10 q
  12. 12Unit 12 Review: Electricity and Charge10 q
Unit 13: Electric Circuits 12 lessons
  1. 1Current, Resistance, and Ohm's Law10 q
  2. 2Series and Parallel Circuits10 q
  3. 3Electric Power and Kirchhoff's Laws10 q
  4. 4Resistor Networks: Series, Parallel, and Mixed Circuits10 q
  5. 5Kirchhoff's Laws: Loop and Node Analysis10 q
  6. 6RC Circuits: Charging and Discharging Dynamics10 q
  7. 7AC versus DC: Household Electrical Systems10 q
  8. 8Electrical Safety: Hazards, Codes, and Protection10 q
  9. 9Practical Electronics: LEDs, Resistors, and Breadboards10 q
  10. 10Multimeters and Circuit Measurement10 q
  11. 11Electric Circuits in Technology, Medicine, and Daily Life10 q
  12. 12Unit 13 Review: Electric Circuits10 q
Unit 14: Magnetism and Electromagnetism 12 lessons
  1. 1Magnetic Fields, Forces, and Electromagnetic Induction10 q
  2. 2Magnetic Fields: Properties and Visualization10 q
  3. 3Magnetic Force on Moving Charges: The Lorentz Force10 q
  4. 4Magnetic Force on Current-Carrying Wires10 q
  5. 5The Electric Motor: Magnetic Force in Action10 q
  6. 6Earth's Magnetic Field and Compass Navigation10 q
  7. 7Electromagnetic Induction: Faraday's Law10 q
  8. 8Lenz's Law and Induced Current Direction10 q
  9. 9Transformers: Stepping Voltage Up and Down10 q
  10. 10AC Power Transmission and the Electrical Grid10 q
  11. 11Applications of Electromagnetism: MRI, Speakers, and Maglev10 q
  12. 12Generators, Transformers, and Unit 14 Review10 q
Unit 15: Modern Physics and Comprehensive Review 12 lessons
  1. 1Review: Mechanics — Kinematics and Newton's Laws10 q
  2. 2Review: Energy, Momentum, and Gravitation10 q
  3. 3Review: Fluids, Waves, Light, and Electricity10 q
  4. 4The Photoelectric Effect and Quantum Theory10 q
  5. 5Nuclear Physics: Radioactivity, Fission, and Fusion10 q
  6. 6Special Relativity and Physics and Faith10 q
  7. 7Wave-Particle Duality and the Double-Slit Experiment10 q
  8. 8Atomic Structure: Bohr Model and Quantum Mechanics10 q
  9. 9Nuclear Reactions: Chain Reactions, Fission Reactors, and Fusion10 q
  10. 10Particle Physics: Quarks, Leptons, and the Standard Model10 q
  11. 11Physics and Faith: The Fine-Tuned Universe and the Creator10 q
  12. 12Comprehensive Physics Review and Reflection10 q

One whole lesson, exactly as it comes

This is a real lesson taken from the middle of the course — the teaching text, the practice, the homework, and the first three quiz questions with their answers. It is not a marketing excerpt.

Unit 8: Fluid Mechanics · Lesson 7

Viscosity and Turbulence in Real Fluids

55 minutesPencilGraph paperScientific calculatorBible (KJV)

What this lesson is for

  • Students will understand viscosity and turbulence in real fluids
  • Students will see God's design in physical laws

Viscosity and Turbulence in Real Fluids

Bernoulli's equation applies to ideal fluids — non-viscous and perfectly smooth-flowing. Real fluids, however, have internal friction called viscosity and can transition from orderly (laminar) to chaotic (turbulent) flow. Understanding these effects is essential for engineering blood vessels, pipelines, and aerodynamic surfaces.

Viscosity Defined

Viscosity (η) is a fluid's resistance to flow — its "thickness." It arises from intermolecular attractions between fluid layers moving at different speeds. The SI unit is the Pascal-second (Pa·s) or equivalently N·s/m².

Typical viscosities at room temperature:

  • Water: η ≈ 0.001 Pa·s (1 mPa·s = 1 centipoise)
  • Blood: η ≈ 0.003 Pa·s
  • Motor oil (SAE 30): η ≈ 0.3 Pa·s
  • Honey: η ≈ 10 Pa·s

Honey flows far more slowly than water because its sugar molecules form strong attractions that resist the relative sliding of layers. God designed each fluid with viscosity suited to its purpose — blood thick enough to carry cells but thin enough to flow easily through capillaries.

Poiseuille's Law: Flow in Pipes

For laminar flow of a viscous fluid in a cylindrical pipe:

Q = (π r⁴ ΔP) / (8 η L)

Where:

  • Q = volumetric flow rate (m³/s)
  • r = pipe radius (m)
  • ΔP = pressure difference end-to-end (Pa)
  • η = dynamic viscosity (Pa·s)
  • L = pipe length (m)

The r⁴ dependence is critical: doubling the pipe radius increases flow rate by 16 times. This is why arteries narrowed by even 30% (plaque buildup) dramatically reduce blood flow — a 30% reduction in radius means flow drops to (0.7)⁴ ≈ 24% of normal. Engineers use this law to size water pipes, irrigation lines, and medical catheters.

Reynolds Number: Laminar vs Turbulent

The Reynolds number predicts whether flow is smooth (laminar) or chaotic (turbulent):

Re = ρvd / η

Where:

  • ρ = fluid density (kg/m³)
  • v = average velocity (m/s)
  • d = pipe diameter (m)
  • η = dynamic viscosity (Pa·s)

Interpretation:

  • Re < 2300: Laminar flow — smooth, parallel streamlines, Poiseuille's law applies
  • 2300 < Re < 4000: Transitional — unstable, can switch between states
  • Re > 4000: Turbulent flow — chaotic, energy-wasting eddies, greater resistance

Example: Blood Flow in an Artery

A major artery has diameter d = 0.01 m (1 cm), blood velocity v = 0.5 m/s, ρ_blood = 1060 kg/m³, η_blood = 0.003 Pa·s.

Re = ρvd / η = (1060 × 0.5 × 0.01) / 0.003 = 5.3 / 0.003 ≈ 1767

Re < 2300, so blood flow in major arteries is laminar — exactly as designed for efficient, non-destructive flow. During vigorous exercise, increased velocity can push Re toward turbulent levels, which is why doctors can sometimes hear turbulent blood flow as a "bruit" with a stethoscope.

Practical Sizing of Straws and Pipes

The r⁴ dependence explains why:

  • Drinking straws are sized to the minimum radius that allows comfortable sipping (too narrow → very high resistance)
  • Municipal water mains are large (reduces Re and friction losses)
  • Nasal passages use branching architecture to keep Re low in smaller branches

God's Engineering in Blood Vessels

The cardiovascular system — branching from the aorta through arterioles to capillaries — is a masterpiece of fluid engineering. Vessel diameters and branching angles are tuned to minimize the work the heart must do while ensuring every cell receives oxygen. Murray's Law (branching optimization) matches what engineers derive mathematically, yet it was designed by God before any human understood the equations.

Homework

Complete assigned practice problems. Show all work with units.

The first three of this lesson's 10 questions

Viscosity is best defined as:

  1. The rate at which fluid flows through a pipe
  2. A fluid's density relative to water
  3. The pressure a fluid exerts on pipe walls
  4. A fluid's internal resistance to flow due to intermolecular friction
Show the answer

Answer: A fluid's internal resistance to flow due to intermolecular friction

In Poiseuille's Law, if pipe radius doubles while all else stays constant, flow rate changes by a factor of:

  1. 4
  2. 2
  3. 16
  4. 8
Show the answer

Answer: 16

Blood has a viscosity of approximately:

  1. 10 Pa·s
  2. 0.3 Pa·s
  3. 0.003 Pa·s
  4. 0.001 Pa·s
Show the answer

Answer: 0.003 Pa·s

Another 7 questions follow in the lesson itself, each one graded the moment it is answered.

What comes with the download

180 full lessons

Across 15 units, each with objectives, a teaching passage written to be read aloud, guided practice, and homework.

1,800 quiz questions

Graded the instant they are answered, each with the explanation of why that answer is right.

A gradebook that works

Every score kept, a running average maintained, and a breakdown unit by unit — all in the file itself, nothing sent anywhere.

Progress and attendance

Tick lessons off as they are finished, watch the completion bar fill, and mark days present, absent, or excused.

Report card and certificate

Both printable, with your student's name, the grades, and the dates already filled in.

Backup you control

Export every record to a file you keep, and read it back later. A lost browser cache cannot take the year with it.

An answer key

Hidden from the student by default, there for the parent marking the work.

Nothing that phones home

No ads, no affiliate links, no analytics, no fonts fetched from elsewhere. Unplug the network cable and every one of these files still works.

What you will need

Drawn from the materials named across all 180 lessons of this course. Most families already own most of it.

Download Physics — Grade 11

Free, and free of everything else. 17 files, 20.7 MB in total. No account, no email address, no payment. What you download carries no advertising, no affiliate links and no tracking of any kind.