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| Step | Derivation / Formula | Reasoning |
|---|---|---|
| 1 | \[p_{\text{before}} = m v_i \] | The clay’s initial momentum equals its mass times its speed. |
| 2 | \[p_{\text{after}} = (m+M) v_x \] | After sticking, the clay + bob move together with speed \(v_x\). |
| 3 | \[m v_i = (m+M) v_x \] | Linear momentum is conserved because the collision is perfectly inelastic and external horizontal forces are negligible. |
| 4 | \[v_x = \frac{m}{m+M} v_i \] | Solve algebraically for the common speed. |
| 5 | \[v_x = \frac{0.020}{0.020+0.500}\,(50) \;=\;1.92\;\text{m/s}\] | Insert \(m = 0.020\,\text{kg}\), \(M = 0.500\,\text{kg}\), and \(v_i = 50\,\text{m/s}\). |
| 6 | \[\boxed{v_x \approx 1.92\,\text{m/s}}\] | Speed of the combined mass just after impact. |
| Step | Derivation / Formula | Reasoning |
|---|---|---|
| 1 | \[\tfrac12 (m+M) v_x^2 = (m+M) g h \] | Kinetic energy right after collision changes into gravitational potential energy at the highest point. |
| 2 | \[h = \frac{v_x^2}{2g} \] | Cancel \((m+M)\) and solve for the height rise \(h\). |
| 3 | \[h = \frac{(1.92)^2}{2(9.81)} = 0.189\,\text{m}\] | Substitute \(v_x\) and \(g = 9.81\,\text{m/s}^2\). |
| 4 | \[h = L(1-\cos\theta)\] | The vertical rise of a pendulum bob is related to its length \(L\) and angular displacement \(\theta\). |
| 5 | \[\cos\theta = 1-\frac{h}{L} = 1-\frac{0.189}{0.800} = 0.764\] | Insert \(h\) and the string length \(L = 0.800\,\text{m}\). |
| 6 | \[\theta = \arccos(0.764) \approx 40.1^{\circ}\] | Take the inverse cosine to find the maximum angle. |
| 7 | \[\boxed{\theta_{\max} \approx 40.1^{\circ}}\] | Maximum angular displacement. |
| Step | Derivation / Formula | Reasoning |
|---|---|---|
| 1 | \[T = 2\pi \sqrt{\frac{L}{g}}\] | For small oscillations, the period of a simple pendulum depends only on its length and \(g\). |
| 2 | \[T = 2\pi \sqrt{\frac{0.800}{9.81}} = 1.79\,\text{s}\] | Insert \(L = 0.800\,\text{m}\) and \(g = 9.81\,\text{m/s}^2\). |
| 3 | \[\boxed{T \approx 1.79\,\text{s}}\] | Period of the clay-bob system. |
| Step | Derivation / Formula | Reasoning |
|---|---|---|
| 1 | \[E = \tfrac12 (m+M) v_x^2\] | Total mechanical energy is the kinetic energy right after the collision (identical to potential energy at the highest point). |
| 2 | \[E = \tfrac12 (0.520) (1.92)^2 = 0.961\,\text{J}\] | Use \(m+M = 0.520\,\text{kg}\) and \(v_x = 1.92\,\text{m/s}\). |
| 3 | \[\boxed{E \approx 0.961\,\text{J}}\] | Total energy of the oscillating system. |
Just ask: "Help me solve this problem."
A \( 0.20 \) \( \text{kg} \) object moves along a straight line. The net force acting on the object varies with the object’s displacement as shown in the graph above. The object starts from rest at displacement \( x = 0 \) and time \( t = 0 \) and is displaced a distance of \( 20 \) \( \text{m} \). Determine each of the following.
A man weighing \( 700 \) \( \text{N} \) and a woman weighing \( 400 \) \( \text{N} \) have the same momentum. What is the ratio of the man’s kinetic energy \( K_m \) to that of the woman \( K_w \)?
A block is attached to a horizontal spring and is initially at rest at the equilibrium position \( x = 0 \), as shown in Figure \( 1 \). The block is then moved to position \( x = -A \), as shown in Figure \( 2 \), and released from rest, undergoing simple harmonic motion. At the instant the block reaches position \( x = +A \), another identical block is dropped onto and sticks to the block, as shown in Figure \( 3 \). The two–block–spring system then continues to undergo simple harmonic motion. Which of the following correctly compares the total mechanical energy \( E_{\text{tot},2} \) of the two–block–spring system after the collision to the total mechanical energy \( E_{\text{tot},1} \) of the one–block–spring system before the collision?
If you want to double the momentum of a gas molecule, by what factor must you increase its kinetic energy?
A rocket of mass \( m \) is launched with kinetic energy \( K_0 \), from the surface of the Earth. How much less kinetic energy does the rocket have at an altitude of two Earth radii? Give your answer in terms of the gravitational constant \( G \), the mass of the Earth \( m_E \), the radius of the Earth \( R_E \), and the mass of the rocket?
\(1.92\,\text{m/s}\)
\(40.1^{\circ}\)
\(1.79\,\text{s}\)
\(0.961\,\text{J}\)
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| Kinematics | Forces |
|---|---|
| \(\Delta x = v_i t + \frac{1}{2} at^2\) | \(F = ma\) |
| \(v = v_i + at\) | \(F_g = \frac{G m_1 m_2}{r^2}\) |
| \(v^2 = v_i^2 + 2a \Delta x\) | \(f = \mu N\) |
| \(\Delta x = \frac{v_i + v}{2} t\) | \(F_s =-kx\) |
| \(v^2 = v_f^2 \,-\, 2a \Delta x\) |
| Circular Motion | Energy |
|---|---|
| \(F_c = \frac{mv^2}{r}\) | \(KE = \frac{1}{2} mv^2\) |
| \(a_c = \frac{v^2}{r}\) | \(PE = mgh\) |
| \(T = 2\pi \sqrt{\frac{r}{g}}\) | \(KE_i + PE_i = KE_f + PE_f\) |
| \(W = Fd \cos\theta\) |
| Momentum | Torque 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 Motion | Fluids |
|---|---|
| \(F = -kx\) | \(P = \frac{F}{A}\) |
| \(T = 2\pi \sqrt{\frac{l}{g}}\) | \(P_{\text{total}} = P_{\text{atm}} + \rho gh\) |
| \(T = 2\pi \sqrt{\frac{m}{k}}\) | \(Q = Av\) |
| \(x(t) = A \cos(\omega t + \phi)\) | \(F_b = \rho V g\) |
| \(a = -\omega^2 x\) | \(A_1v_1 = A_2v_2\) |
| Constant | Description |
|---|---|
| [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 |
| Variable | SI 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] |
| Variable | Derived 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.
Start with the given measurement: [katex]\text{5 km}[/katex]
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]
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]
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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