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| Step | Derivation / Formula | Reasoning |
|---|---|---|
| 1 | \[v_{x}^{2}=v_{i}^{2}+2(-g)\Delta x\] | Use the kinematic relation \(v_{x}^{2}=v_{i}^{2}+2a\Delta x\) with upward positive (so \(a=-g\)). \(v_{x}=14\,\text{m/s}\) at the window, \(\Delta x=18\,\text{m}\). |
| 2 | \[v_{i}^{2}=v_{x}^{2}+2g\Delta x\] | Algebraically solve for \(v_{i}^{2}\). |
| 3 | \[v_{i}^{2}=14^{2}+2(9.8)(18)=196+352.8=548.8\] | Substitute the numerical values. |
| 4 | \[\boxed{v_{i}=23.43\,\text{m/s}}\] | Take the square root to obtain the initial speed. |
| Step | Derivation / Formula | Reasoning |
|---|---|---|
| 1 | \[0=v_{i}^{2}+2(-g)\Delta x_{\text{max}}\] | At the peak, the final velocity is zero, so set \(v_{x}=0\). |
| 2 | \[\Delta x_{\text{max}}=\frac{v_{i}^{2}}{2g}\] | Re-arrange for the upward displacement from the street. |
| 3 | \[\Delta x_{\text{max}}=\frac{548.8}{19.6}=28\,\text{m}\] | Insert \(v_{i}^{2}=548.8\) and \(g=9.8\,\text{m/s}^{2}\). |
| 4 | \[\boxed{28\,\text{m}}\] | The ball rises 28 m above the street. |
| Step | Derivation / Formula | Reasoning |
|---|---|---|
| 1 | \[v_{x}=v_{i}-g t_{1}\] | Use \(v_{x}=v_{i}+at\) with \(a=-g\) to relate velocities and time. |
| 2 | \[t_{1}=\frac{v_{i}-v_{x}}{g}\] | Solve for \(t_{1}\), the interval from the throw to passing the window upward. |
| 3 | \[t_{1}=\frac{23.5-14}{9.8}=0.964\,\text{s}\] | Insert the numerical values. |
| 4 | \[\boxed{0.96\,\text{s}}\] | The ball was thrown roughly one second before being seen at the window. |
| Step | Derivation / Formula | Reasoning |
|---|---|---|
| 1 | \[T_{\text{total}}=\frac{2v_{i}}{g}\] | For motion that starts and ends at the same height, total flight time is twice the time to the peak, \(v_{i}/g\). |
| 2 | \[T_{\text{total}}=\frac{2(23.5)}{9.8}=4.79\,\text{s}\] | Insert \(v_{i}=23.5\,\text{m/s}\) and \(g=9.8\,\text{m/s}^{2}\). |
| 3 | \[t_{\text{after window}}=T_{\text{total}}-t_{1}=4.79-0.96=3.83\,\text{s}\] | Subtract the elapsed time before passing the window to find the interval after it. |
| 4 | \[\boxed{4.8\,\text{s}\;\text{(total from throw)}}\] | The ball returns to the street 4.8 s after being thrown, i.e., about 3.8 s after passing the window. |
Just ask: "Help me solve this problem."
You throw a ball straight upward. It leaves your hand at \( 20 \) \( \text{m/s} \) and slows at a steady rate until it stops at the peak. The ball then comes back down, speeding up steadily until it hits the ground with the same speed it left your hand. Draw the velocity vs. time graph or explain it in terms of functions.
An object’s velocity \(v\) as a function of time \(t\) is given in the graph. Which of the following statements is true about the motion of the object?
Above is the graph of an object’s velocity as a function of time. Which of the following is true about the motion?
An object is thrown upward at \( 65 \, \text{m/s} \) from the top of a \( 800 \, \text{m} \) tall building.
A mine shaft is known to be 57.8 m deep. If you dropped a rock down the shaft, how long would it take for you to hear the sound of the rock hitting the bottom of the shaft knowing that sound travels at a constant velocity of 345 m/s?
\(23.43\,\text{m/s}\)
\(28\,\text{m}\)
\(0.96\,\text{s}\)
\(4.8\,\text{s}\)
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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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