AP Physics

Unit 2 - Linear Forces

Intermediate

Mathematical

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Step Derivation/Formula Reasoning
1 $$F_{\parallel} = F\cos(\theta)$$ The horizontal force \( F \) is resolved into a component along the inclined plane. The component along the plane is given by \( F\cos(\theta) \).
2 $$F_{g\,\parallel} = mg\sin(\theta)$$ The gravitational force has a component down the incline given by \( mg\sin(\theta) \).
3 $$N = mg\cos(\theta)+ F\sin(\theta)$$ The normal force \( N \) is found by resolving forces perpendicular to the incline. Gravity gives \( mg\cos(\theta) \) and the horizontal force contributes \( F\sin(\theta) \) pushing the block into the plane.
4 $$F_{f} = \mu N = \mu\left(mg\cos(\theta)+ F\sin(\theta)\right)$$ The frictional force is given by the coefficient of friction \( \mu \) times the normal force.
5 $$m\,a = F\cos(\theta)- mg\sin(\theta)- \mu\left(mg\cos(\theta)+ F\sin(\theta)\right)$$ Applying Newton’s second law along the incline, the net force is the sum of the component of \( F \) along the plane minus both the gravitational and frictional forces.
6 $$a = \frac{F\cos(\theta)- mg\sin(\theta)- \mu\left(mg\cos(\theta)+ F\sin(\theta)\right)}{m}$$ This is the final expression for the block’s acceleration \( a \) up the incline in terms of \( m,\,\theta,\,\mu,\,F, \) and \( g \).

 

Step Derivation/Formula Reasoning
1 $$0 = F\cos(\theta)- mg\sin(\theta)- \mu\left(mg\cos(\theta)+ F\sin(\theta)\right)$$ For the block to slide up the plane with constant velocity, the acceleration must be zero. Hence the net force along the incline is zero.
2 $$F\cos(\theta)- \mu F\sin(\theta) = mg\sin(\theta)+ \mu mg\cos(\theta)$$ Rearrange the equation by grouping the terms involving \( F \) on the left and the gravitational terms on the right.
3 $$F \left(\cos(\theta)- \mu \sin(\theta)\right) = mg\left(\sin(\theta)+ \mu\cos(\theta)\right)$$ Factor out \( F \) on the left-hand side and \( mg \) on the right-hand side for clarity.
4 $$F = \frac{mg\left(\sin(\theta)+ \mu\cos(\theta)\right)}{\cos(\theta)- \mu\sin(\theta)}$$ Solve the equation for \( F \) by dividing both sides by \(\cos(\theta)- \mu \sin(\theta)\).
5 $$\cos(\theta)- \mu\sin(\theta)> 0 \quad \Longrightarrow \quad \tan(\theta) < \frac{1}{\mu}$$ For \( F \) to be physically meaningful (i.e., a positive real number), the denominator must be positive. Rearranging the inequality yields the condition \( \tan(\theta) < \frac{1}{\mu} \).
6 $$\boxed{F = \frac{mg\left(\sin(\theta)+ \mu\cos(\theta)\right)}{\cos(\theta)- \mu\sin(\theta)}}$$ This is the final expression for the magnitude of the applied horizontal force required to make the block slide with a constant velocity, including the physical condition on \( \theta \) and \( \mu \).

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a) \( a = \frac{F (\cos \theta – \mu \sin \theta) – mg (\mu \cos \theta + \sin \theta)}{m} \)

b) \( F = \frac{\mu m g \cos \theta + \mu F \sin \theta + m g \sin \theta}{\cos \theta} \)

 

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KinematicsForces
\(\Delta x = v_i t + \frac{1}{2} at^2\)\(F = ma\)
\(v = v_i + at\)\(F_g = \frac{G m_1 m_2}{r^2}\)
\(v^2 = v_i^2 + 2a \Delta x\)\(f = \mu N\)
\(\Delta x = \frac{v_i + v}{2} t\)\(F_s =-kx\)
\(v^2 = v_f^2 \,-\, 2a \Delta x\) 
Circular MotionEnergy
\(F_c = \frac{mv^2}{r}\)\(KE = \frac{1}{2} mv^2\)
\(a_c = \frac{v^2}{r}\)\(PE = mgh\)
\(T = 2\pi \sqrt{\frac{r}{g}}\)\(KE_i + PE_i = KE_f + PE_f\)
 \(W = Fd \cos\theta\)
MomentumTorque 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 MotionFluids
\(F = -kx\)\(P = \frac{F}{A}\)
\(T = 2\pi \sqrt{\frac{l}{g}}\)\(P_{\text{total}} = P_{\text{atm}} + \rho gh\)
\(T = 2\pi \sqrt{\frac{m}{k}}\)\(Q = Av\)
\(x(t) = A \cos(\omega t + \phi)\)\(F_b = \rho V g\)
\(a = -\omega^2 x\)\(A_1v_1 = A_2v_2\)
ConstantDescription
[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
VariableSI 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]
VariableDerived 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. 

  1. Start with the given measurement: [katex]\text{5 km}[/katex]

  2. 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]

  3. 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]

  4. 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]

  1. 1. Some answers may vary by 1% due to rounding.
  2. Gravity values may differ: \(9.81 \, \text{m/s}^2\) or \(10 \, \text{m/s}^2\).
  3. Variables can be written differently. For example, initial velocity (\(v_i\)) may be \(u\), and displacement (\(\Delta x\)) may be \(s\).
  4. Bookmark questions you can’t solve to revisit them later
  5. 5. Seek help if you’re stuck. The sooner you understand, the better your chances on tests.

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