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Part A – Explanation of forces on FBD
Step | Derivation/Formula | Reasoning |
---|---|---|
a) | \(B\) | This is the buoyant force acting upward on the balloon, equal to the weight of the displaced air. |
a) | \(W_{\text{balloon}} = (0.0050\,\text{kg})\,g\) | This is the weight of the balloon (including helium) acting downward. |
a) | \(T\) | This is the tension in the string, which transmits the downward pull from the attached \(0.015\,\text{kg}\) object. (Only the balloon is considered here so its forces include the upward buoyant force and the two downward forces: its own weight and the tension from the string.) |
Part B – Buoyant force on the balloon
Step | Derivation/Formula | Reasoning |
---|---|---|
b) 1 | \(B = W_{\text{balloon}} + W_{\text{object}} = (0.0050\,\text{kg} + 0.015\,\text{kg})\,g = 0.0200\,g\) | The balloon is just prevented from rising, so its upward buoyant force exactly balances the combined weight of the balloon and the attached object. (The buoyant force on the object is negligible.) |
b) 2 | \(B = 0.0200 \times 9.8 \; (\text{m/s}^2) = \boxed{0.196\,\text{N}}\) | Substitute \(g \approx 9.8\,\text{m/s}^2\) to calculate the buoyant force in newtons. |
Part C – Volume of the balloon
Step | Derivation/Formula | Reasoning |
---|---|---|
c) 1 | \(B = \rho_{\text{air}} \; g \; V\) | This is Archimedes’ principle stating that the buoyant force is equal to the weight of the displaced air. Here \(\rho_{\text{air}} = 1.29\,\text{kg/m}^3\), and \(g = 9.8\,\text{m/s}^2\). |
c) 2 | \(V = \displaystyle \frac{B}{\rho_{\text{air}} \; g} = \frac{0.196}{1.29 \times 9.8}\) | Rearrange the equation to solve for the volume \(V\) of the balloon. |
c) 3 | \(V \approx \frac{0.196}{12.642} \approx \boxed{0.0155\,\text{m}^3}\) | Calculate the denominator (\(1.29 \times 9.8 \approx 12.642\)) and then evaluate \(V\). The volume of the balloon is approximately \(0.0155\,\text{m}^3\). |
Part D – Position of ballon in the car
Step | Derivation/Formula | Reasoning |
---|---|---|
d) 1 | Effective gravity: \(\vec{g}_{\text{eff}} = \vec{g} – \vec{a}\) | When the car accelerates forward with acceleration \(a\), the effective gravitational field in the car’s frame tilts backward. This is a standard result for non-inertial frames. |
d) 2 | For a mass not affected by buoyancy, the equilibrium direction of the string makes an angle \(\theta\) where \(\tan(\theta)=\frac{a}{g}\). | The heavy \(0.015\,\text{kg}\) object behaves as a normal pendulum, aligning along the effective gravitational field. This causes it to deflect opposite to the car’s acceleration (i.e., towards the rear of the car). |
d) 3 | Result: The \(0.015\,\text{kg}\) object \(\rightarrow\) moves backward relative to the car. | Thus, when the car accelerates forward, the object swings toward the back of the car, while the buoyant balloon (not shown here) would deflect forward. Since the child holds the string midway, the object is pulled into its equilibrium position defined by \(\vec{g}_{\text{eff}}\). |
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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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