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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
- (\mu_s): Coefficient of static 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
- (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
- (\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
- (\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)
- (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
- (c): Specific heat capacity
- Ideal Gas Law:
[ PV = nRT ]
- (R = 8.314 \, \text{J/(mol} \cdot \text{K)})
- (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.