About F=ma
The AAPT's first-round physics contest on classical mechanics. High scorers may be invited to the USAPhO.
F=ma Exam Format & Focus
25 multiple-choice questions in 75 minutes, focused only on classical mechanics: kinematics, Newton's laws, work and energy, momentum and circular motion.
How Skillzy Young Scholars Prepares Students for F=ma
Skillzy Young Scholars teaches F=ma in live online classes with vetted mentors who have completed 100 hours of training. The curriculum is organised into 7 units, with worksheets, quizzes, timed practice and mock exams. Progress is tracked in the LMS and shared with parents in a monthly report.
What F=ma Covers
- Kinematics and graph analysis
- Newton's laws, free-body diagrams and friction
- Work, energy, power, momentum and collisions
- Circular motion and gravitation
F=ma Curriculum
Classes follow these units. Every student starts with a level check, and the order and pace adapt to your child. Units that go beyond the exam's core topics are stretch material.
- Target Audience
- High school students in Grades 9–12 competing individually.
- Target Exam Format
- The AAPT F = ma Exam is a 75-minute multiple-choice contest containing 25 questions focused strictly on classical mechanics.
- Foundational Focus Areas
- 1. Kinematics: 1D motion, v-t graph analysis, 2D projectile motion.
- 2. Dynamics: Newton's 1st, 2nd, and 3rd Laws, free-body diagrams, friction.
- 3. Work & Energy: Work done by variable forces, potential energy curves, energy conservation.
- 4. Momentum: Impulse, center of mass, 1D/2D collisions.
- 5. Circular Motion & Gravity: Centripetal force, Fg = Gm1m2/r , orbital speed.
- Scoring & Advancement
- High scorers on the F = ma Exam (~top 400 students nationwide) qualify for the prestigious, free-response USAPhO (U.S. Physics Olympiad) Exam.
What the program focuses on
- Targeted Mechanics Foundations (building core intuition and mathematical fluency for the 25-question 75-minute F = ma Exam)
- 1D & 2D Kinematics (motion graphs, calculus/algebraic derivations, and projectile trajectory dynamics)
- Newton's Laws of Motion (free-body diagrams, normal forces, tension, friction, and coupled systems)
- Work, Energy, & Power (work-energy theorem, conservative vs. non-conservative forces, and mechanical energy conservation)
- Linear Momentum & Impulse (impulse-momentum theorem, 1D/2D elastic and inelastic collisions, and center of mass)
- Circular Motion & Universal Gravitation (centripetal acceleration, circular orbits, and Kepler's Laws intuition)
- Interactive, hands-on quantitative problem-solving drills and mock quizzes with continuous progress monitoring
Units
1 1D Kinematics & Graph Analysis
Students will learn to:
- Analyze 1D Motion Variables: Define position (x), displacement (∆x), average vs. instantaneous velocity (v), and average vs. instantaneous acceleration (a).
- Derive Constant Acceleration Equations: Derive and apply the fundamental kinematic equations:
- v = v0 + at 1 2
- x = x0 + v0t + 2 at 2 2
- v = v0 + 2a(x − x0)
- Interpret Motion Graphs: Derive physical quantities from slopes and areas of x-t, v-t, and a-t graphs ( dx dv v = dt , a = dt , ∆x = ∫ vdt, ∆v = ∫ adt).
- Analyze Free-Fall Motion: Solve 1D vertical motion problems under constant gravitational acceleration (g = 9. 8m/s ).
F = ma Alignment - Kinematics Topic. F = ma questions frequently require extracting initial conditions and accelerations directly from non-linear v- t or x-t graphs.
Learning activities:
- Motion graph slope and area derivative workshops
- 1D kinematic equation derivation and variable isolation drills
- Free-fall vertical motion timing speed relays
What this means for your child. Your child will master 1D kinematics, interpreting motion graphs and deriving acceleration equations.
2 2D Kinematics, Vectors, & Projectile Motion
Students will learn to:
- Master Vector Addition & Components: Decompose 2D vectors into orthogonal components ( Ax = A cos θ, Ay = A sin θ) and compute dot/cross products conceptually.
- Analyze 2D Projectile Motion: Treat horizontal (ax = 0) and vertical (ay =− g) motions independently to solve projectile trajectories.
- Derive Projectile Parameters: Calculate time of flight (tflight), maximum height (hmax), and horizontal v0sin2θ range (R = g ) on level and inclined surfaces. → → →
- Understand Relative Motion: Perform 2D relative velocity vector additions (vA/C = vA/B + vB/C) in river-crossing and wind-vector problems.
F = ma Alignment - 2D Kinematics Topic. Questions test projectile motion on inclines, relative velocity frame transformations, and optimal launch angle derivations.
Learning activities:
- 2D vector component decomposition speed relays
- Inclined projectile trajectory calculation workshops
- Relative velocity vector triangle problem-solving labs
What this means for your child. Your child will learn 2D kinematics and vector analysis, solving projectile motion and relative velocity problems.
3 Newton's Laws & Free-Body Diagrams (FBDs)
Students will learn to:
- Apply Newton's First Law: Understand inertia, equilibrium (∑ F = 0), and inertial reference frames. → →
- Apply Newton's Second Law: Formulate ∑ F = ma along component axes for single and multi-body systems. → →
- Apply Newton's Third Law: Identify action-reaction force pairs (FAonB =− FBonA) acting on distinct objects.
- Master Free-Body Diagram (FBD) Construction: Draw complete FBDs isolating all external contact forces (normal force N, tension T, friction f) and field forces (gravity mg).
F = ma Alignment - Dynamics Topic. FBD construction is the single most important skill on the F = ma exam. Questions test force balancing across multi-body contact systems.
Learning activities:
- Multi-body FBD construction speed drills
- Inertial vs. non-inertial frame conceptual workshops
- Action-reaction force pair identification exercises
What this means for your child. Your child will master Newton's Laws of Motion, constructing precise free-body diagrams for complex force systems.
4 Friction, Inclined Planes, & Connected Systems
Students will learn to:
- Model Static & Kinetic Friction: Differentiate static friction (fs ≤ μsN) and kinetic friction (fk = μkN), analyzing the transition point (fs,max).
- Analyze Inclined Plane Dynamics: Decompose weight components along parallel (mg sin θ) and perpendicular (mg cos θ) axes to an incline.
- Solve Connected Atwood Machine Systems: Set up coupled equations of motion for pulleys, strings, and stacked blocks to solve for system acceleration (a) and string tension (T).
- Analyze Drag Force Basics: Understand qualitative terminal velocity mechanics (Fd ∝ v or v ) when drag equals gravitational force.
F = ma Alignment - Advanced Dynamics Topic. Questions test block-on-block friction transitions, ideal pulley systems, and inclines with variable friction coefficients.
Learning activities:
- Block-on-block static vs. kinetic friction transition labs
- Atwood machine system acceleration derivation workshops
- Inclined plane force component resolution speed relays
What this means for your child. Your child will learn complex force dynamics, solving friction problems, inclines, and connected Atwood machines.
5 Work, Energy, & Power
Students will learn to:
- Calculate Work Done by Forces: Apply W = F · d = Fd cos θ for constant forces and W = ∫ F · dr for variable forces (area under F-x graph).
- Apply Work-Energy Theorem: Relate net work done on a system to its change in kinetic energy ( 1 2 1 2 Wnet = ∆K = 2 mvf − 2 mvi ).
- Analyze Potential Energy Functions: Differentiate conservative (gravitational Ug = mgh, elastic 1 2 dU Us = 2 kx ) and non-conservative forces (friction), deriving F =− dx .
- Master Mechanical Energy Conservation: Solve problems using Emech = K + U = constant in closed dW → → systems, and calculate mechanical power (P = dt = F · v).
F = ma Alignment - Work & Energy Topic. Questions test variable spring forces, potential energy curve stability (F =− dU/dx = 0), and energy dissipation via friction.
Learning activities:
- Potential energy function U(x) stability curve analysis labs
- Variable force integration and F-x graph work workshops
- Conservation of mechanical energy setup speed drills
What this means for your child. Your child will master work and energy principles, deriving work-energy theorems and potential energy functions.
6 Linear Momentum, Impulse, & Collisions
Students will learn to:
- Understand Momentum & Impulse: Define linear momentum (p = mv) and relate impulse to → → → momentum change (J = ∫ Fdt = ∆p). → →
- Apply Conservation of Linear Momentum: Apply ∑ pi = ∑ pf in closed systems where external forces → are zero (∑ Fext = 0).
- Differentiate Collision Types: Analyze 1D/2D elastic collisions (conserving momentum and kinetic energy) vs. inelastic/perfectly inelastic collisions (conserving momentum only). → → ∑miri
- Calculate Center of Mass: Compute center of mass position (rcm = M ) and center of mass velocity → → ∑mivi (vcm = M ).
F = ma Alignment - Momentum Topic. Questions test 2D elastic collision velocity vector geometry, center-of-mass frame transformations, and impulse force graphs.
Learning activities:
- 2D elastic collision vector geometry workshops
- Center-of-mass position and velocity calculation labs
- Impulse-momentum F-t graph area analysis drills
What this means for your child. Your child will learn linear momentum and collisions, analyzing elastic/inelastic interactions and center-of-mass systems.
7 Uniform Circular Motion & Gravitation
Students will learn to:
- Analyze Centripetal Acceleration: Derive centripetal acceleration (ac = r = ω r) directed toward the center of circular paths. v
- Apply Centripetal Force: Formulate ∑ Fradial = mac = m r for banked curves, vertical loops, and conical pendulums. m1m2
- Apply Newton's Law of Universal Gravitation: Calculate gravitational force (Fg = G 2 ) and r M gravitational field strength (g = G 2 ). R GM 2 4π 3
- Analyze Circular Orbits & Kepler's Laws: Derive orbital velocity (v = r ), orbital period (T = GM r m1m2 ), and gravitational potential energy (Ug =− G r ).
F = ma Alignment - Gravitation Topic. Questions test banked curve maximum speeds, vertical loop normal force limits, satellite orbital energy ( Mm Etotal =− G 2r ), and Kepler's 3rd Law.
Always check the official exam organizer for the current format, dates and eligibility. We do not guarantee scores or rankings.
Sample F=ma Prep Plan
- Begin with a F=ma diagnostic and check the current official format, scoring rules and eligible level.
- Weeks 3–5: build a topic notebook, practise interpreting evidence and explain answers aloud.
- Weeks 6–8: complete timed sets and review weak concepts.
- Final phase: rehearse pacing, review past-style problems and refine written solutions.
Common F=ma Mistakes We Help Students Avoid
- Preparing for F=ma using a generic or outdated format instead of checking the current official guidance.
- Ignoring the official rules, scoring rubric or allowed materials.
- Leaving timed practice until the final week.
Every student begins with a level check so we can see where the gaps are. Private 1:1 students also get a full diagnostic assessment and a personalized roadmap. We teach the concepts behind each question type, practice under timed conditions, and review every wrong answer. We cannot guarantee specific scores, but progress is tracked in monthly reports.