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| Step | Derivation / Formula | Reasoning |
|---|---|---|
| 1 | \[m_1 = 4\,\text{kg},\; m_2 = 7\,\text{kg},\; v_i = 10\,\text{m/s}\] | Identify the masses and the initial velocity \(v_i\) of the \(4\,\text{kg}\) mass. The \(7\,\text{kg}\) mass is initially at rest. |
| 2 | \[p_{x,i}=m_1 v_i = 4(10)=40,\; p_{y,i}=0\] | Calculate the initial momentum components. Motion is purely horizontal to the right, so the vertical component is zero. |
| 3 | \[v_{x2}=2\cos22^{\circ},\; v_{y2}=-2\sin22^{\circ}\] | Resolve the \(7\,\text{kg}\) mass’s given final speed (\(2\,\text{m/s}\)) into horizontal and vertical components. The vertical component is negative (below the horizontal). |
| 4 | \[v_{x2}\approx1.854,\; v_{y2}\approx-0.749\] | Numerical evaluation of the trigonometric components. |
| 5 | \[4 v_{x1}+7 v_{x2}=40\] | Apply conservation of momentum in the \(x\)-direction: total initial \(p_x\) equals total final \(p_x\). |
| 6 | \[4 v_{y1}+7 v_{y2}=0\] | Apply conservation of momentum in the \(y\)-direction: initial \(p_y\) is zero, so the final \(p_y\) must also be zero. |
| 7 | \[v_{x1}=\frac{40-7 v_{x2}}{4}\] | Solve the \(x\)-momentum equation for the unknown horizontal component \(v_{x1}\) of the \(4\,\text{kg}\) mass. |
| 8 | \[v_{x1}=\frac{40-7(1.854)}{4}\approx6.755\,\text{m/s}\] | Substitute \(v_{x2}\) and compute \(v_{x1}\). |
| 9 | \[v_{y1}=-\frac{7 v_{y2}}{4}\] | Rearrange the \(y\)-momentum equation to isolate the vertical component \(v_{y1}\) of the \(4\,\text{kg}\) mass. |
| 10 | \[v_{y1}=-\frac{7(-0.749)}{4}\approx1.311\,\text{m/s}\] | Insert \(v_{y2}\) and calculate \(v_{y1}\). The result is positive, meaning the mass moves upward after the collision. |
| 11 | \[v_x=\sqrt{v_{x1}^2+v_{y1}^2}\] | Use the Pythagorean relation to find the magnitude \(v_x\) of the final velocity of the \(4\,\text{kg}\) mass. |
| 12 | \[v_x=\sqrt{(6.755)^2+(1.311)^2}\approx6.88\,\text{m/s}\] | Compute the numerical value of the speed. |
| 13 | \[\theta=\tan^{-1}\!\left(\frac{v_{y1}}{v_{x1}}\right)\] | Determine the direction angle \(\theta\) measured above the horizontal. |
| 14 | \[\theta=\tan^{-1}\!\left(\frac{1.311}{6.755}\right)\approx11^{\circ}\] | Evaluate the inverse tangent to find the angle. |
| 15 | \[\boxed{v_x\approx6.9\,\text{m/s},\;\theta\approx11^{\circ}\,\text{above horizontal}}\] | Present the final boxed answer: the speed and its angle relative to the horizontal. |
Just ask: "Help me solve this problem."
A \(1200 \, \text{kg}\) car moving at \(15.6 \, \text{m/s}\) suddenly collides with a stationary car of mass \(1500 \, \text{kg}\). If the two vehicles lock together, what is their combined velocity immediately after the collision?
A bullet at speed [katex] v_0 [/katex] trikes and embeds itself in a block of wood which is suspended by a string, causing the bullet and block to rise to a maximum height h. Which of the following statements is true?
A \( 1.0 \, \text{kg} \) lump of clay is sliding to the right on a frictionless surface with a speed of \( 2 \, \text{m/s} \). It collides head-on and sticks to a \( 0.5 \, \text{kg} \) metal sphere that is sliding to the left with a speed of \( 4 \, \text{m/s} \). What is the kinetic energy of the combined objects after the collision?
A 3800 kg open railroad car coasts along with a constant speed of 8.60 m/s along a level track. Snow begins to fall vertically and fills the car at rate of 3.50 kg/min. Ignoring friction with the tracks, what is the speed of the car after 90 min?
Car A, mass 1000 kg, is traveling at 40 m/s when it collides with a stationary car B. They stick together and travel at 7 m/s. What is the mass of car B?
\(6.9\,\text{m/s}\)
\(11^{\circ}\text{ above horizontal}\)
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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] | 0.000000000001 |
Nano- | n | [katex]10^{-9}[/katex] | 0.000000001 |
Micro- | µ | [katex]10^{-6}[/katex] | 0.000001 |
Milli- | m | [katex]10^{-3}[/katex] | 0.001 |
Centi- | c | [katex]10^{-2}[/katex] | 0.01 |
Deci- | d | [katex]10^{-1}[/katex] | 0.1 |
(Base unit) | – | [katex]10^{0}[/katex] | 1 |
Deca- or Deka- | da | [katex]10^{1}[/katex] | 10 |
Hecto- | h | [katex]10^{2}[/katex] | 100 |
Kilo- | k | [katex]10^{3}[/katex] | 1,000 |
Mega- | M | [katex]10^{6}[/katex] | 1,000,000 |
Giga- | G | [katex]10^{9}[/katex] | 1,000,000,000 |
Tera- | T | [katex]10^{12}[/katex] | 1,000,000,000,000 |
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