AP Physics

Unit 6 - Rotational Motion

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Part (a) – Minimum Coefficient of Friction

Derivation or Formula Reasoning
\[ Mg\sin\theta – f = Ma \] This is Newton’s second law for translation along the incline, where \(Mg\sin\theta\) is the component of gravity down the plane and \(f\) is the friction force.
\[ fR = I\alpha \quad \text{with} \quad a = \alpha R \] The friction force provides the torque needed for rolling without slipping, and the rolling condition relates linear acceleration \(a\) to angular acceleration \(\alpha\).
\[ f = \frac{Ia}{R^2} \] Rearranging the torque equation yields an expression for \(f\) in terms of \(a\).
\[ f = \frac{2}{5}Ma \] Substitute the moment of inertia for a uniform solid sphere \(I = \frac{2}{5}MR^2\) into the previous expression.
\[ Mg\sin\theta – \frac{2}{5}Ma = Ma \] Insert \(f = \frac{2}{5}Ma\) into Newton’s second law and set up the equation for \(a\).
\[ Mg\sin\theta = \left(1+\frac{2}{5}\right)Ma = \frac{7}{5}Ma \] Simplify the equation to combine like terms and isolate \(a\).
\[ a = \frac{5}{7}g\sin\theta \] Solve for the linear acceleration \(a\) of the sphere along the incline.
\[ f = \frac{2}{5}M\left(\frac{5}{7}g\sin\theta\right) = \frac{2}{7}Mg\sin\theta \] Determine the friction force required for rolling by substituting \(a\) back into \(f = \frac{2}{5}Ma\).
\[ \frac{2}{7}Mg\sin\theta = \mu Mg\cos\theta \] For the sphere to roll without slipping, the required friction force must be available, i.e., it must equal the maximum static friction \(\mu Mg\cos\theta\).
\[ \mu = \frac{2}{7}\tan\theta \] Solve for the minimum coefficient of friction \(\mu\) needed to prevent slipping.
\[ \boxed{\mu = \frac{2}{7}\tan\theta} \] This boxed expression is the final answer for part (a).

Part (b) – Speed Comparison with Zero Friction

Derivation or Formula Reasoning
\[ Mgh = \frac{1}{2}Mv_x^2 + \frac{1}{2}I\left(\frac{v_x}{R}\right)^2 \quad \Rightarrow \quad v_x = \sqrt{\frac{10}{7}gh} \] For a rolling sphere, the gravitational potential energy converts into both translational and rotational kinetic energy.
\[ Mgh = \frac{1}{2}Mv_x^2 \quad \Rightarrow \quad v_x = \sqrt{2gh} \] Without friction (\(\mu = 0\)), the sphere slides without rotating, so all potential energy becomes translational kinetic energy.
\[ \sqrt{2gh} > \sqrt{\frac{10}{7}gh} \] Since \(2 > \frac{10}{7}\), the translational speed of a sliding sphere is higher than that of a rolling sphere, where some energy goes into rotation.
\(\text{Speed is greater when } \mu = 0\) Thus, with zero friction the sphere attains a higher speed at the bottom because no energy is diverted to rotational motion.

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\(\mu = \frac{2}{7}\tan\theta\)\n\(\text{Greater}\)

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KinematicsForces
\(\Delta x = v_i t + \frac{1}{2} at^2\)\(F = ma\)
\(v = v_i + at\)\(F_g = \frac{G m_1 m_2}{r^2}\)
\(v^2 = v_i^2 + 2a \Delta x\)\(f = \mu N\)
\(\Delta x = \frac{v_i + v}{2} t\)\(F_s =-kx\)
\(v^2 = v_f^2 \,-\, 2a \Delta x\) 
Circular MotionEnergy
\(F_c = \frac{mv^2}{r}\)\(KE = \frac{1}{2} mv^2\)
\(a_c = \frac{v^2}{r}\)\(PE = mgh\)
\(T = 2\pi \sqrt{\frac{r}{g}}\)\(KE_i + PE_i = KE_f + PE_f\)
 \(W = Fd \cos\theta\)
MomentumTorque and Rotations
\(p = mv\)\(\tau = r \cdot F \cdot \sin(\theta)\)
\(J = \Delta p\)\(I = \sum mr^2\)
\(p_i = p_f\)\(L = I \cdot \omega\)
Simple Harmonic MotionFluids
\(F = -kx\)\(P = \frac{F}{A}\)
\(T = 2\pi \sqrt{\frac{l}{g}}\)\(P_{\text{total}} = P_{\text{atm}} + \rho gh\)
\(T = 2\pi \sqrt{\frac{m}{k}}\)\(Q = Av\)
\(x(t) = A \cos(\omega t + \phi)\)\(F_b = \rho V g\)
\(a = -\omega^2 x\)\(A_1v_1 = A_2v_2\)
ConstantDescription
[katex]g[/katex]Acceleration due to gravity, typically [katex]9.8 , \text{m/s}^2[/katex] on Earth’s surface
[katex]G[/katex]Universal Gravitational Constant, [katex]6.674 \times 10^{-11} , \text{N} \cdot \text{m}^2/\text{kg}^2[/katex]
[katex]\mu_k[/katex] and [katex]\mu_s[/katex]Coefficients of kinetic ([katex]\mu_k[/katex]) and static ([katex]\mu_s[/katex]) friction, dimensionless. Static friction ([katex]\mu_s[/katex]) is usually greater than kinetic friction ([katex]\mu_k[/katex]) as it resists the start of motion.
[katex]k[/katex]Spring constant, in [katex]\text{N/m}[/katex]
[katex] M_E = 5.972 \times 10^{24} , \text{kg} [/katex]Mass of the Earth
[katex] M_M = 7.348 \times 10^{22} , \text{kg} [/katex]Mass of the Moon
[katex] M_M = 1.989 \times 10^{30} , \text{kg} [/katex]Mass of the Sun
VariableSI Unit
[katex]s[/katex] (Displacement)[katex]\text{meters (m)}[/katex]
[katex]v[/katex] (Velocity)[katex]\text{meters per second (m/s)}[/katex]
[katex]a[/katex] (Acceleration)[katex]\text{meters per second squared (m/s}^2\text{)}[/katex]
[katex]t[/katex] (Time)[katex]\text{seconds (s)}[/katex]
[katex]m[/katex] (Mass)[katex]\text{kilograms (kg)}[/katex]
VariableDerived SI Unit
[katex]F[/katex] (Force)[katex]\text{newtons (N)}[/katex]
[katex]E[/katex], [katex]PE[/katex], [katex]KE[/katex] (Energy, Potential Energy, Kinetic Energy)[katex]\text{joules (J)}[/katex]
[katex]P[/katex] (Power)[katex]\text{watts (W)}[/katex]
[katex]p[/katex] (Momentum)[katex]\text{kilogram meters per second (kgm/s)}[/katex]
[katex]\omega[/katex] (Angular Velocity)[katex]\text{radians per second (rad/s)}[/katex]
[katex]\tau[/katex] (Torque)[katex]\text{newton meters (Nm)}[/katex]
[katex]I[/katex] (Moment of Inertia)[katex]\text{kilogram meter squared (kgm}^2\text{)}[/katex]
[katex]f[/katex] (Frequency)[katex]\text{hertz (Hz)}[/katex]

General Metric Conversion Chart

Example of using unit analysis: Convert 5 kilometers to millimeters. 

  1. Start with the given measurement: [katex]\text{5 km}[/katex]

  2. Use the conversion factors for kilometers to meters and meters to millimeters: [katex]\text{5 km} \times \frac{10^3 \, \text{m}}{1 \, \text{km}} \times \frac{10^3 \, \text{mm}}{1 \, \text{m}}[/katex]

  3. Perform the multiplication: [katex]\text{5 km} \times \frac{10^3 \, \text{m}}{1 \, \text{km}} \times \frac{10^3 \, \text{mm}}{1 \, \text{m}} = 5 \times 10^3 \times 10^3 \, \text{mm}[/katex]

  4. Simplify to get the final answer: [katex]\boxed{5 \times 10^6 \, \text{mm}}[/katex]

Prefix

Symbol

Power of Ten

Equivalent

Pico-

p

[katex]10^{-12}[/katex]

Nano-

n

[katex]10^{-9}[/katex]

Micro-

µ

[katex]10^{-6}[/katex]

Milli-

m

[katex]10^{-3}[/katex]

Centi-

c

[katex]10^{-2}[/katex]

Deci-

d

[katex]10^{-1}[/katex]

(Base unit)

[katex]10^{0}[/katex]

Deca- or Deka-

da

[katex]10^{1}[/katex]

Hecto-

h

[katex]10^{2}[/katex]

Kilo-

k

[katex]10^{3}[/katex]

Mega-

M

[katex]10^{6}[/katex]

Giga-

G

[katex]10^{9}[/katex]

Tera-

T

[katex]10^{12}[/katex]

  1. 1. Some answers may vary by 1% due to rounding.
  2. Gravity values may differ: \(9.81 \, \text{m/s}^2\) or \(10 \, \text{m/s}^2\).
  3. Variables can be written differently. For example, initial velocity (\(v_i\)) may be \(u\), and displacement (\(\Delta x\)) may be \(s\).
  4. Bookmark questions you can’t solve to revisit them later
  5. 5. Seek help if you’re stuck. The sooner you understand, the better your chances on tests.

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