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Ap Physics One Equation Sheet

Ap Physics One Equation Sheet
Ap Physics One Equation Sheet

AP Physics 1 Equation Sheet

Below is a comprehensive list of essential equations for AP Physics 1, organized by topic. These formulas are critical for solving problems and understanding key concepts in the course.


1. Kinematics

  • Displacement (Δx):
    [ \Delta x = x_f - x_i ]
  • Average Velocity (v_avg):
    [ v_{avg} = \frac{\Delta x}{\Delta t} ]
  • Average Speed:
    [ \text{Average Speed} = \frac{\text{Total Distance}}{\text{Total Time}} ]
  • Constant Acceleration Equations:
    [ v_f = v_i + a \Delta t ]
    [ \Delta x = v_i \Delta t + \frac{1}{2} a (\Delta t)^2 ]
    [ v_f^2 = v_i^2 + 2a \Delta x ]

2. Dynamics

  • Newton’s Second Law:
    [ F = ma ]
  • Weight (Gravitational Force):
    [ F_g = mg ]
  • Normal Force (N):
    [ N = mg \cos(\theta) \quad \text{(on an incline)} ]
  • Frictional Force (f):
    [ f = \mu N ]
    • (\mu_s): Coefficient of static friction
    • (\mu_k): Coefficient of kinetic friction
  • Tension (T):
    Depends on the system; often resolved into components.

3. Work, Energy, and Power

  • Work (W):
    [ W = F \cdot d \cdot \cos(\theta) ]
  • Kinetic Energy (KE):
    [ KE = \frac{1}{2} mv^2 ]
  • Work-Energy Theorem:
    [ W_{net} = \Delta KE ]
  • Potential Energy (PE):
    [ PE_g = mgh ]
  • Power (P):
    [ P = \frac{W}{t} = F \cdot v ]

4. Linear Momentum

  • Momentum (p):
    [ p = mv ]
  • Impulse (J):
    [ J = F \Delta t = \Delta p ]
  • Conservation of Momentum:
    [ m1 v{1i} + m2 v{2i} = m1 v{1f} + m2 v{2f} ]

5. Simple Harmonic Motion (SHM)

  • Period (T):
    [ T = 2\pi \sqrt{\frac{m}{k}} ]
    • (k): Spring constant
  • Frequency (f):
    [ f = \frac{1}{T} ]
  • Displacement in SHM:
    [ x(t) = A \cos\left(\frac{2\pi t}{T}\right) ]

6. Circular Motion

  • Centripetal Force (F_c):
    [ F_c = \frac{mv^2}{r} = mr\omega^2 ]
    • (\omega): Angular velocity
  • Centripetal Acceleration (a_c):
    [ a_c = \frac{v^2}{r} = r\omega^2 ]

7. Rotational Motion

  • Rotational Kinematics:
    [ \theta = \omega t + \frac{1}{2} \alpha t^2 ]
    [ \omega_f^2 = \omega_i^2 + 2\alpha \theta ]
    • (\alpha): Angular acceleration
  • Moment of Inertia (I):
    [ I = \sum m_i r_i^2 ]
  • Torque ((\tau)):
    [ \tau = r \times F = I\alpha ]

8. Gravitation

  • Universal Gravitation (F_g):
    [ F_g = G \frac{m_1 m_2}{r^2} ]
    • (G = 6.674 \times 10^{-11} \, \text{N} \cdot \text{m}^2/\text{kg}^2)
  • Gravitational Potential Energy (PE_g):
    [ PE_g = -\frac{GmM}{r} ]

9. Fluid Mechanics

  • Density ((\rho)):
    [ \rho = \frac{m}{V} ]
  • Pressure (P):
    [ P = \frac{F}{A} ]
  • Buoyant Force (F_B):
    [ FB = \rho{fluid} V_{submerged} g ]
  • Continuity Equation (A1v1 = A2v2):
    [ A_1 v_1 = A_2 v_2 ]

10. Thermodynamics

  • Thermal Energy (Q):
    [ Q = mc\Delta T ]
    • (c): Specific heat capacity
  • Ideal Gas Law:
    [ PV = nRT ]
    • (R = 8.314 \, \text{J/(mol} \cdot \text{K)})
  • First Law of Thermodynamics:
    [ \Delta U = Q - W ]

Key Constants

  • Gravitational Acceleration ((g)): (9.8 \, \text{m/s}^2)
  • Planck’s Constant ((h)): (6.626 \times 10^{-34} \, \text{J} \cdot \text{s})
  • Boltzmann Constant ((k_B)): (1.38 \times 10^{-23} \, \text{J/K})

Key Takeaway: Mastery of these equations, combined with conceptual understanding, is essential for success in AP Physics 1. Practice applying them in various contexts to build problem-solving skills.




What is the most important equation in AP Physics 1?


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Newton’s Second Law ((F = ma)) is foundational, as it connects force, mass, and acceleration, which are central to dynamics.






How do I decide which kinematics equation to use?


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Identify the known and unknown variables in the problem. Choose the equation that includes all knowns and the unknown you’re solving for.






What’s the difference between kinetic and potential energy?


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Kinetic energy ((KE = \frac{1}{2}mv^2)) is energy of motion, while potential energy ((PE = mgh)) is stored energy due to position or condition.





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