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Ultimate Guide to Rectilinear Resisted Motion in HSC Mathematics Extension 2

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    Vu Hung
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Introduction

In previous topics, we modelled motion in idealized, frictionless vacuums. However, in the real world, objects moving through a fluid (like a car driving through air or a submarine moving through water) experience drag. Rectilinear Resisted Motion introduces mathematical models for this resistance. In HSC Mathematics Extension 2, you must apply advanced calculus to derive the exact equations for a particle's velocity and displacement when it is slowed down by a resistive force.

Executive Summary

This comprehensive guide covers the core concepts of rectilinear (straight-line) resisted motion:

  • Newton's Laws and Resistance: Establishing the fundamental equation of motion mx¨=R(v)m\ddot{x} = -R(v), where resistance is proportional to a power of speed (R=kvR = kv or R=kv2R = kv^2).
  • Velocity as a Function of Time: Using a=dvdta = \frac{dv}{dt} and integration (often involving logarithms) to find v(t)v(t).
  • Velocity as a Function of Displacement: Using a=vdvdxa = v\frac{dv}{dx} and integration to find v(x)v(x).
  • Displacement as a Function of Time: Integrating the velocity function to find exactly where the particle is at any given moment x(t)x(t).

What is this about?

When you slide a block across a rough table, it eventually stops due to friction. When you coast on a bicycle, air resistance slowly brings you to a halt. In this topic, we model a particle moving horizontally with an initial velocity, but with no driving force pushing it forward. The only force acting on it is a resistive force that directly opposes its motion. Because this resistance changes depending on how fast the object is moving, the acceleration is not constant. You will use the integration techniques learned earlier in Extension 2 (like partial fractions or inverse trig functions) to solve the resulting differential equations.

Main Content

1. Setting up the Equation of Motion

Consider a particle of mass mm projected horizontally along the xx-axis with an initial velocity uu. The only external force acting horizontally is a resistive force RR that opposes the motion. According to the syllabus, the magnitude of this resistance is proportional to a power of the speed, typically R=kvR = kv or R=kv2R = kv^2 (where k>0k > 0).

Using Newton's Second Law (F=maF = ma), and taking the direction of motion as positive: Fnet=RF_{\text{net}} = -R mx¨=kvnm\ddot{x} = -kv^n

From this starting point, we can substitute our different expressions for acceleration to find velocity and displacement.

2. Velocity as a Function of Time, v(t)v(t)

To find how velocity changes over time, we use a=dvdta = \frac{dv}{dt}. mdvdt=kvnm\frac{dv}{dt} = -kv^n

We solve this using the separation of variables: dvvn=kmdt\frac{dv}{v^n} = -\frac{k}{m} dt

Example for R=kvR = kv (n=1n=1): 1vdv=kmdt\int \frac{1}{v} dv = \int -\frac{k}{m} dt ln(v)=kmt+C\ln(v) = -\frac{k}{m}t + C

Using the initial condition (at t=0t=0, v=uv=u): ln(u)=C\ln(u) = C ln(v)ln(u)=kmt\ln(v) - \ln(u) = -\frac{k}{m}t ln(vu)=kmt\ln\left(\frac{v}{u}\right) = -\frac{k}{m}t v=uekmtv = u e^{-\frac{k}{m}t}

This tells us that the velocity decays exponentially over time!

3. Velocity as a Function of Displacement, v(x)v(x)

To find how velocity relates to distance travelled, we use a=vdvdxa = v\frac{dv}{dx}. m(vdvdx)=kvnm \left(v\frac{dv}{dx}\right) = -kv^n

Again, we separate the variables: vvndv=kmdx\frac{v}{v^n} dv = -\frac{k}{m} dx 1vn1dv=kmdx\frac{1}{v^{n-1}} dv = -\frac{k}{m} dx

By integrating both sides and using the initial condition (at x=0x=0, v=uv=u), you can establish the relationship between the particle's speed and how far it has travelled.

4. Displacement as a Function of Time, x(t)x(t)

Once you have established v(t)v(t) in Step 2, you can find x(t)x(t) simply by realizing that v=dxdtv = \frac{dx}{dt} and integrating your expression with respect to time.

Taking our previous result v=uekmtv = u e^{-\frac{k}{m}t}: dxdt=uekmt\frac{dx}{dt} = u e^{-\frac{k}{m}t} dx=uekmtdt\int dx = \int u e^{-\frac{k}{m}t} dt x=mukekmt+Cx = -\frac{mu}{k} e^{-\frac{k}{m}t} + C

Using the initial condition (at t=0t=0, x=0x=0): 0=muk(1)+C    C=muk0 = -\frac{mu}{k}(1) + C \implies C = \frac{mu}{k} x(t)=muk(1ekmt)x(t) = \frac{mu}{k} \left(1 - e^{-\frac{k}{m}t}\right)

Notice something fascinating here: as tt \to \infty, the term ekmt0e^{-\frac{k}{m}t} \to 0. Therefore, xmukx \to \frac{mu}{k}. This means the particle will never travel further than muk\frac{mu}{k} metres, even given an infinite amount of time!

Simple Worked Example

Question: A particle of unit mass (m=1m=1) is projected horizontally with an initial speed of 10 m/s10 \text{ m/s}. It experiences a resistance of magnitude 2v22v^2, where vv is its speed. Find an expression for the particle's velocity vv in terms of its displacement xx.

Solution: Step 1: Set up the equation of motion. F=maF = ma 2v2=1a-2v^2 = 1 \cdot a

Step 2: Choose the correct acceleration formula. Since we want velocity in terms of displacement xx, we use a=vdvdxa = v\frac{dv}{dx}. vdvdx=2v2v\frac{dv}{dx} = -2v^2

Step 3: Separate variables and integrate. Divide both sides by vv (since v0v \ne 0 while it's moving): dvdx=2v\frac{dv}{dx} = -2v 1vdv=2dx\frac{1}{v} dv = -2 dx 1vdv=2dx\int \frac{1}{v} dv = \int -2 \, dx ln(v)=2x+C\ln(v) = -2x + C

Step 4: Find the constant of integration. At x=0x = 0, the initial velocity is v=10v = 10. ln(10)=2(0)+C    C=ln(10)\ln(10) = -2(0) + C \implies C = \ln(10)

Step 5: Write the final expression. ln(v)=2x+ln(10)\ln(v) = -2x + \ln(10) ln(v)ln(10)=2x\ln(v) - \ln(10) = -2x ln(v10)=2x\ln\left(\frac{v}{10}\right) = -2x v10=e2x\frac{v}{10} = e^{-2x} v=10e2xv = 10e^{-2x}

mini-FAQ page

Q: Do I need to memorize the final equations for v(t)v(t) and x(t)x(t)? A: Absolutely not. The HSC syllabus explicitly states you must derive these expressions from Newton's laws. Questions will frequently change the initial conditions, the mass, or the resistance function (kvkv vs kv2kv^2 vs kv3kv^3), which entirely changes the final integrated formula.

Q: Why is the resistance always negative in the initial equation? A: We define the direction of motion as the positive direction. Because resistance acts in the opposite direction to motion, the force vector must be negative.

Common mistakes to avoid

  • Messing up the integration of 1v\frac{1}{v}: Remember that 1vdv=lnv+C\int \frac{1}{v} dv = \ln|v| + C. However, 1v2dvln(v2)\int \frac{1}{v^2} dv \ne \ln(v^2). Instead, use power rules: v2dv=v1+C=1v+C\int v^{-2} dv = -v^{-1} + C = -\frac{1}{v} + C.
  • Forgetting the absolute value in logarithms: While vv is usually positive in rectilinear motion (since it just slows down and doesn't turn around), it's a good habit to recognize lnv\ln|v| just in case the coordinate system is flipped.
  • Skipping the separation of variables: You cannot just integrate vdvdx=kv2v\frac{dv}{dx} = -kv^2 with respect to xx directly on both sides without moving the vv terms to the dvdv side first.

Practice on Vu's Maths Hub

Mastering resisted motion requires absolute confidence in your calculus and integration skills. Prepare for the HSC with our detailed resources:

Further Readings

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