0 attempts
0% avg
UBQ Credits
(a) Calculation of the angular frequency (\(\omega\)) of the oscillation:
Step | Derivation/Formula | Reasoning |
---|---|---|
1 | \(\omega = \sqrt{\frac{g}{L}}\) | The angular frequency formula for a simple pendulum, where \(g\) is the acceleration due to gravity \(9.8 \, \text{m/s}^2\) and \(L\) is the length of the pendulum. |
2 | \(\omega = \sqrt{\frac{9.8}{1.2}}\) | Substitute \(g = 9.8 \, \text{m/s}^2\) and \(L = 1.2 \, \text{m}\) into the formula. |
3 | \(\omega = \sqrt{8.17}\) | Calculate the division inside the square root. |
4 | \(\omega \approx 2.86 \, \text{rad/s}\) | Calculate the square root to find the angular frequency. |
(b) Calculation of the period (\(T\)) of oscillation:
Step | Derivation/Formula | Reasoning |
---|---|---|
1 | \(T = \frac{2\pi}{\omega}\) | The period of oscillation is the reciprocal of the angular frequency multiplied by \(2\pi\). |
2 | \(T = \frac{2\pi}{2.86}\) | Substitute the angular frequency value found earlier. |
3 | \(T \approx 2.20 \, \text{s}\) | Calculate the period. |
(c) Calculation of the maximum speed of the pendulum:
Step | Derivation/Formula | Reasoning |
---|---|---|
1 | \(v_{\text{max}} = \omega A\) | Maximum speed is the product of angular frequency and amplitude. |
2 | \(A = 1.2 \cdot \sin(10^\circ)\) | Convert amplitude from degrees to a distance using the pendulum length (1.2 m) and the sine of 10 degrees. |
3 | \(A \approx 0.208\, \text{m}\) | Calculate the amplitude in meters. |
4 | \(v_{\text{max}} = 2.86 \cdot 0.208\) | Substitute the values of \( \omega \) and \( A \) to find maximum velocity. |
5 | \(v_{\text{max}} \approx 0.595 \, \text{m/s}\) | Compute the maximum speed. |
(d) Calculation of the maximum acceleration of the pendulum:
Step | Derivation/Formula | Reasoning |
---|---|---|
1 | \(a_{\text{max}} = \omega^2 A\) | Maximum acceleration is the product of the square of angular frequency and amplitude. |
2 | \(a_{\text{max}} = (2.86)^2 \times 0.208\) | Substitute the values of \( \omega \) and \( A \). |
3 | \(a_{\text{max}} \approx 1.70 \, \text{m/s}^2\) | Calculate the maximum acceleration. |
(e) Determine the acceleration due to gravity on the Exoplanet:
Step | Derivation/Formula | Reasoning |
---|---|---|
1 | \(f = \frac{1}{T}\) | Frequency is the reciprocal of the period. |
2 | \(T = \frac{1}{2.3}\) | Substitute the frequency of oscillation (2.3 Hz). |
3 | \(T \approx 0.435 \, \text{s}\) | Compute the period of oscillation on the Exoplanet. |
4 | \(T = 2\pi \sqrt{\frac{L}{g_{\text{exo}}}}\) | Use the period expression in terms of gravity and pendulum length to solve for gravity on the Exoplanet. |
5 | \(\frac{0.435}{2\pi} = \sqrt{\frac{1.2}{g_{\text{exo}}}}\) | Rearrange to express \(\frac{T}{2\pi}\) in terms of known values. |
6 | \(g_{\text{exo}} = \frac{1.2}{(0.435/(2\pi))^2}\) | Solve for the gravitational acceleration. |
7 | \(g_{\text{exo}} \approx 90 \, \text{m/s}^2\) | Calculate to find the acceleration due to gravity on the Exoplanet. |
Just ask: "Help me solve this problem."
A block with a mass of \( 4 \) \( \text{kg} \) is attached to a spring on the wall that oscillates back and forth with a frequency of \( 4 \) \( \text{Hz} \) and an amplitude of \( 3 \) \( \text{m} \). What would the frequency be if the block were replaced by one with one‑fourth the mass and the amplitude of the block is increased to \( 9 \) \( \text{m} \)?
Three pendulums are set in motion, oscillating through small amplitudes. Each has the same mass. Rank the period of the pendulums from shortest to longest.
A mass is attached to the end of a spring and set into simple harmonic motion with an amplitude \( A \) on a horizontal frictionless surface. Determine the following in terms of only the variable \( A \).
A 0.50-kg mass is attached to a spring constant 20 N/m along a horizontal, frictionless surface. The object oscillates in simple harmonic motion and has a speed of 1.5 m/s at the equilibrium position. What is the total energy of the system?
A 10 meter long pendulum on the earth, is set into motion by releasing it from a maximum angle of less than 10° relative to the vertical. At what time [katex]t[/katex] will the pendulum have fallen to a perfectly vertical orientation?
By continuing you (1) agree to our Terms of Sale and Terms of Use and (2) consent to sharing your IP and browser information used by this site’s security protocols as outlined in our Privacy Policy.
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 |
The most advanced version of Phy. 50% off, for early supporters. Prices increase soon.
per month
Billed Monthly. Cancel Anytime.
Trial –> Phy Pro
Try our free calculator to see what you need to get a 5 on the upcoming AP Physics 1 exam.
A quick explanation
Credits are used to grade your FRQs and GQs. Pro users get unlimited credits.
Submitting counts as 1 attempt.
Viewing answers or explanations count as a failed attempts.
Phy gives partial credit if needed
MCQs and GQs are are 1 point each. FRQs will state points for each part.
Phy customizes problem explanations based on what you struggle with. Just hit the explanation button to see.
Understand you mistakes quicker.
Phy automatically provides feedback so you can improve your responses.
10 Free Credits To Get You Started
By continuing you agree to nerd-notes.com Terms of Service, Privacy Policy, and our usage of user data.
NEW! PHY instantly solves any question
🔥 Elite Members get up to 30% off Physics Tutoring
🧠 Learning Physics this summer? Try our free course.
🎯 Need exam style practice questions? We’ve got over 2000.