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Comprehensive AP Physics 1 Review Guide
Apr 27, 2025
AP Physics 1 Review Summary
Introduction
Review of AP Physics 1 curriculum in 30 minutes.
More extensive resources available including detailed video reviews and practice exams.
Unit 1: Kinematics
Vectors and Scalars:
Vectors have magnitude and direction.
Scalars have magnitude only.
Distance vs Displacement:
Distance is the length of the path taken.
Displacement is the straight-line distance between two points, a vector.
Velocity and Acceleration:
Average velocity = displacement / time, a vector.
Average acceleration = change in velocity / time, a vector.
Instantaneous values exist when time intervals are very small.
Uniformly Accelerated Motion (UAM):
Use UAM equations when acceleration is constant.
5 variables, 4 equations; knowing 3 allows finding the other 2.
Graphical Analysis:
Slope of position vs time = velocity.
Slope of velocity vs time = acceleration.
Area under velocity vs time = change in position.
Area under acceleration vs time = change in velocity.
Projectile Motion:
Only gravity acts, use acceleration = 10 m/s².
Use UAM in y-direction, constant velocity in x-direction.
Relative Motion:
Motion changes with observerās frame of reference.
Unit 2: Force and Translational Dynamics
Center of Mass:
Sum of mass-position products divided by total mass.
Forces:
All forces are vectors; interaction between two objects.
Free Body Diagrams illustrate forces.
Newtonās Laws:
1st Law: Object remains at rest or constant velocity without external net force.
2nd Law: Acceleration = net force / mass.
3rd Law: Equal and opposite reaction forces.
Translational equilibrium when net force is zero.
Gravitational and Frictional Forces:
Gravitational force = mass * gravitational field strength.
Friction opposes sliding motion and is parallel to the surface.
Universal Gravitation and Hooke's Law:
Universal gravitation: Force = G * (mass1 * mass2) / distance².
Hookeās Law: Spring force = -k * displacement.
Unit 3: Work, Energy, and Power
Energy Types:
Kinetic, gravitational potential, elastic potential energy.
Work:
Work = force * displacement * cos(theta).
Conservative and Nonconservative Forces:
Conservative: path-independent (e.g., gravity, springs).
Nonconservative: path-dependent (e.g., friction).
Energy Conservation:
Total mechanical energy remains if no net work.
Work-energy principle: Net work = change in kinetic energy.
Power:
Rate of energy change over time.
Power = work / time.
Unit 4: Linear Momentum
Momentum and Impulse:
Momentum = mass * velocity.
Impulse = change in momentum.
Collisions:
Elastic: Kinetic energy conserved.
Inelastic: Kinetic energy not conserved.
Perfectly inelastic: Objects stick together.
Conservation of Momentum:
Momentum remains constant if net external force is zero.*
Unit 5: Torque and Rotational Dynamics
Rotational Motion:
Angular displacement, velocity, acceleration.
All must be in radians.
Torque:
Torque causes angular acceleration; torque = r * F * sin(theta).
Rotational Inertia:
Resists angular acceleration; depends on mass distribution.
Newtonās Laws in Rotation:
1st Law: Constant angular velocity without external torque.
2nd Law: Net torque = rotational inertia * angular acceleration.*
Unit 6: Energy and Momentum of Rotating Systems
Rotational Kinetic Energy:
Rotational kinetic energy = 1/2 * rotational inertia * angular speed².
Angular Momentum:
Angular momentum = rotational inertia * angular velocity.
Rolling Motion:
Combines translational and rotational motion.
Orbits:
Circular: Mechanical energy and angular momentum constant.
Elliptical: Only angular momentum constant.*
Unit 7: Oscillations
Simple Harmonic Motion:
Restoring force proportional to displacement.
Period = time for one cycle; amplitude = max displacement.
Mass-Spring and Pendulum Systems:
Mass-spring: Period = 2Ļā(m/k).
Pendulum: Period = 2Ļā(L/g) for small angles.
Unit 8: Fluids
Density and Pressure:
Density = mass / volume.
Pressure = force / area.
Buoyant Force:
Equals weight of displaced fluid.
Fluid Dynamics:
Continuity equation: Volumetric flow rate is constant.
Bernoulli's equation: Mechanical energy conservation.
Torricelliās Theorem: Fluid exit speed from a small hole.
Conclusion
Extensive additional resources available for more detailed study and practice.
Encouragement and confidence boost for exam preparation.
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