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AP Physics

Unit 6 - Rotational Motion

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Mathematical
Intermediate

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To solve this problem, we need to calculate the mass of the sphere given the diameter, torque, number of revolutions, and time. We will use the rotational dynamics principles and formulas.

Step Derivation/Formula Reasoning
1 [katex]I = \frac{2}{5} m r^2[/katex] The moment of inertia (I) for a solid sphere about an axis through its center is [katex]\frac{2}{5} m r^2[/katex], where [katex]m[/katex] is the mass and [katex]r[/katex] is the radius of the sphere.
2 [katex]r = \frac{0.72 \, \text{m}}{2} = 0.36 \, \text{m}[/katex] Convert the diameter of the sphere to radius. This helps in computing the moment of inertia and further calculations.
3 [katex] \tau = I \alpha[/katex] Torque ([katex]\tau[/katex]) is related to the angular acceleration ([katex]\alpha[/katex]) by the formula, where [katex]I[/katex] is the moment of inertia.
4 [katex]\theta = \omega_f t – \frac{1}{2} \alpha t^2[/katex] The angular displacement ([katex] \theta [/katex]) can be expressed in terms of final angular velocity ([katex] \omega_f [/katex]), angular acceleration ([katex] \alpha [/katex]), and time ([katex] t [/katex]). Here, starting from rest simplifies to [katex] \theta = \frac{1}{2} \alpha t^2 [/katex].
5 [katex]\theta = 160 \times 2\pi \text{ rad} = 1005.31 \text{ rad}[/katex] Convert the number of revolutions to radians (since [katex]1[/katex] revolution = [katex]2\pi[/katex] radians).
6 [katex]1005.31 \text{ rad} = \frac{1}{2} \alpha (15.0 \text{ s})^2[/katex] Use the total revolutions in radians and solve for angular acceleration [katex]\alpha[/katex] using the time elapsed.
7 [katex]\alpha = \frac{2 \times 1005.31 \text{ rad}}{(15.0 \text{ s})^2} = 8.937 \text{ rad/s}^2[/katex] Calculate the angular acceleration [katex]\alpha[/katex].
8 [katex]\tau = I \alpha \implies 10.8 \text{ Nm} = \frac{2}{5} m (0.36 \text{ m})^2 \times 8.937 \text{ rad/s}^2[/katex] Plug values of moment of inertia and angular acceleration into the torque equation to solve for mass [katex]m[/katex].
9 [katex]m = \frac{10.8 \text{ Nm}}{\frac{2}{5} \times (0.36 \text{ m})^2 \times 8.937 \text{ rad/s}^2} \approx 23.3 \text{ kg}[/katex] Final step: solve the equation for mass, providing the solution to the problem.

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23.3 kg

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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]

Metric Prefixes

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]

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