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How does a resistance proportional to speed change rectilinear motion, and what is the terminal velocity of a body falling under gravity with resistance?

Model rectilinear motion under gravity with a resistive force proportional to velocity or to the square of velocity, and determine terminal velocity

A focused answer to the HSC Maths Extension 2 dot point on resisted motion. Newton's second law with resistance proportional to speed, separating variables for velocity, the concept of terminal velocity, and motion of a rising and falling body, with verified worked examples.

Reviewed by: AI editorial process; not yet individually human-reviewed

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Jump to a section
  1. What this dot point is asking
  2. Setting up Newton's second law
  3. Terminal velocity
  4. Velocity as a function of time
  5. Velocity as a function of position
  6. Up-and-down problems
  7. Choosing the integral form
  8. How exam questions ask about resisted motion

What this dot point is asking

NESA wants you to model a particle moving in a straight line under gravity while a resistive force opposes its motion. The resistance is taken proportional to the speed or to the square of the speed. You set up Newton's second law as a differential equation, separate variables to find velocity as a function of time or position, and identify the terminal velocity where acceleration vanishes.

Setting up Newton's second law

For a particle of mass mm, the net force equals mass times acceleration:

ma=F.m\,a = \sum F.

The forces are gravity, of magnitude mgmg, and resistance, which always opposes the direction of motion. Choosing a positive direction is essential and the sign of the resistance term must oppose velocity. Taking downwards as positive for a falling body with resistance proportional to speed:

mdvdt=mgkv,m\frac{dv}{dt} = mg - kv,

where k>0k > 0 is the resistance constant. For resistance proportional to the square of the speed, replace kvkv by kv2kv^2, again ensuring the sign opposes motion.

The forces and the velocity curve, stage by stage

A falling body with resistance is best understood through the force balance, because the balance is what bends the velocity-time graph into its characteristic shape. The panels below track the forces from release to terminal velocity, then show the curve they produce.

Stage 1, the instant of release. At t=0t = 0 the body is at rest, so v=0v = 0 and the resistance kv=0kv = 0. The only force is gravity mgmg pulling down, so the net force is at its largest and the acceleration is the full gg. The body starts to speed up exactly as it would in free fall.

Stage 1: forces just after releaseA falling body at the instant of release. Only gravity m g acts downward; the resistance is essentially zero because the speed is zero, so the net downward force and the acceleration are large. body mg v = 0, so resistance = 0; net force = mg (largest). 1

Stage 2, falling and speeding up. Once the body moves, the resistance kvkv acts upward, opposing the downward motion. The net downward force is now mgkvmg - kv, smaller than gravity alone, so the acceleration has dropped below gg. The faster the body falls, the larger kvkv becomes and the smaller the acceleration: the body keeps speeding up, but by less and less.

Stage 2: forces while fallingAs the body speeds up, gravity m g still acts downward but a resistance k v now acts upward opposing the motion. The net downward force is gravity minus resistance, smaller than before, so the acceleration is decreasing. body mg kv net force = mg - kv, smaller; acceleration is falling. 2

Stage 3, terminal velocity. Eventually kvkv grows to equal mgmg. Now the two forces cancel, the net force is zero, and the acceleration is zero. The body cannot speed up any further, so its velocity stays fixed at the terminal velocity vT=mgkv_T = \dfrac{mg}{k}. This is the steady state the whole motion is heading towards.

Stage 3: balance at terminal velocityAt terminal velocity the upward resistance k v has grown until it equals gravity m g. The two arrows are equal and opposite, the net force is zero, and the acceleration is zero, so the speed stays constant. body mg resistance kv = mg resistance now equals gravity; net force = 0, a = 0. 3

Stage 4, the velocity-time curve. Putting the three force pictures together gives the velocity-time graph. It starts steep (acceleration near gg), curves over as the resistance builds, and levels off towards the horizontal asymptote v=vTv = v_T. The body gets arbitrarily close to vTv_T but never quite reaches it, which is why terminal velocity is always stated as a limit.

Stage 4: the velocity-time curveStarting from rest, the velocity rises steeply at first and then ever more slowly, leveling off towards a horizontal asymptote at the terminal velocity v T equals m g over k. The curve approaches but never reaches the dashed asymptote. t v terminal velocity vT = mg/k steep: a near g flattening: a near 0 Stage 4: v rises from rest and levels off at vT; the asymptote is never reached. 4

Terminal velocity

As a falling body speeds up, the resistance grows until it balances gravity and the acceleration drops to zero. Setting dvdt=0\dfrac{dv}{dt} = 0 in mdvdt=mgkvm\dfrac{dv}{dt} = mg - kv gives

mgkvT=0vT=mgk.mg - kv_T = 0 \quad\Longrightarrow\quad v_T = \frac{mg}{k}.

For the square law mgkv2=0mg - kv^2 = 0 gives vT=mgkv_T = \sqrt{\dfrac{mg}{k}}. The velocity approaches vTv_T but never reaches it in finite time; it is a horizontal asymptote of the velocity-time graph. A useful sense-check: terminal velocity does not depend on how the body started, only on the balance mg=kvTmg = kv_T, so a dropped body and a body thrown downward both tend to the same vTv_T. A body thrown downward faster than vTv_T would actually slow down, because then the resistance exceeds gravity and the net force points up.

Velocity as a function of time

To find v(t)v(t), use a=dvdta = \dfrac{dv}{dt} and separate variables. From mdvdt=mgkvm\dfrac{dv}{dt} = mg - kv,

mdvmgkv=dt.\int \frac{m\,dv}{mg - kv} = \int dt.

The left integral is a logarithm; solving and applying the initial condition (often v=0v = 0 at t=0t = 0 for a dropped body) gives an exponential approach to vTv_T, of the form v=vT(1ekt/m)v = v_T(1 - e^{-kt/m}).

Velocity as a function of position

When the question asks for vv in terms of distance fallen, use a=vdvdxa = v\dfrac{dv}{dx} instead:

mvdvdx=mgkv.mv\frac{dv}{dx} = mg - kv.

Separate as mvdvmgkv=dx\displaystyle\int \frac{mv\,dv}{mg - kv} = \int dx and integrate. The same care with signs and the same use of initial conditions apply. A rising body decelerates under both gravity and resistance, so for upward motion (taking up as positive) the equation is mdvdt=mgkvm\dfrac{dv}{dt} = -mg - kv, with both forces acting downwards.

Up-and-down problems

A projectile thrown upward and then falling back is two separate problems joined at the highest point. On the way up, both gravity and resistance oppose the upward motion, so the deceleration is large and the equation carries mgkv-mg - kv (or mgkv2-mg - kv^2). At the top the velocity is zero. On the way down, gravity drives the motion while resistance opposes it, so the equation becomes mgkvmg - kv (or mgkv2mg - kv^2). Because the resistance always opposes the current direction of travel, the sign of the resistance term flips between the two phases. A consequence worth quoting is that the body returns to its starting level with a speed less than its launch speed, since energy is lost to resistance throughout.

Choosing the integral form

As with all rectilinear motion, the choice between dvdt\frac{dv}{dt} and vdvdxv\frac{dv}{dx} is dictated by what the question asks. If you need velocity as a function of time, or the time to reach a height, use dvdt\frac{dv}{dt}. If you need velocity as a function of distance, or the distance to come to rest, use vdvdxv\frac{dv}{dx}. The resulting integrals are standard: a velocity-only resistance gives a logarithm, while a velocity-squared resistance typically gives a logarithm or an arctangent depending on the sign of the constant term, which is exactly why the inverse-trig and logarithm integrals from the calculus strand are prerequisites here.

How exam questions ask about resisted motion

The wording flags both the model and the tool:

  • "A body falls / is dropped and meets a resistance proportional to its speed (or to the square of its speed)." Write mv˙=mgkvm\dot{v} = mg - kv (or mgkv2mg - kv^2), taking down as positive.
  • "Show that the terminal velocity is ..." Set v˙=0\dot{v} = 0 and solve mg=kvTmg = kv_T (or mg=kvT2mg = kv_T^2). One line, one mark.
  • "Find vv as a function of time" / "how long to reach a given speed." Use dvdt\dfrac{dv}{dt}, separate, integrate to a logarithm (linear law) or use dva2v2\int \frac{dv}{a^2 - v^2} / dva2+v2\int \frac{dv}{a^2 + v^2} (square law). Apply the initial condition.
  • "Find vv as a function of distance fallen" / "the distance to reach a given speed." Use vdvdxv\dfrac{dv}{dx} and separate instead; time never appears.
  • "A body is projected vertically upward against gravity and resistance. Find the time to the top / the greatest height." This is the upward phase: both forces act downward, so v˙=(g+kv2/m)\dot{v} = -(g + kv^2/m) and you integrate, often to an arctangent. The top is where v=0v = 0.
  • "Show the body returns with a smaller speed than it was launched with." An energy or up-then-down argument: resistance removes energy on both legs, so the return speed is below the launch speed (and below terminal velocity).
  • "Two bodies move towards each other in a resisting medium." Subtract the two equations of motion to cancel gravity and reduce to a single first-order equation in the separation, as in the 2024 question above.

Exam-style practice questions

Practice questions written in the style of NESA exam questions on this dot point, with worked answer explainers. The year tag is the paper they imitate, not the source.

HSC 20213 marksAn object of mass 11 kg is projected vertically upwards with an initial velocity of uu m/s. It experiences air resistance of magnitude kv2k v^2 newtons, where vv is the velocity and k>0k > 0 is constant. Acceleration due to gravity is gg m/s2^2. Show that the time to reach maximum height is 1gkarctan ⁣(ukg)\dfrac{1}{\sqrt{gk}}\arctan\!\left(u\sqrt{\tfrac{k}{g}}\right) seconds.
Show worked answer →

Take upwards as positive. While the object rises, both gravity and resistance act downwards, so for unit mass

dvdt=gkv2=(g+kv2)\frac{dv}{dt} = -g - k v^2 = -(g + k v^2).

Separate variables and integrate from launch (t=0t = 0, v=uv = u) to the top (t=Tt = T, v=0v = 0):

dt=dvg+kv2dt = -\frac{dv}{g + k v^2}, so T=0udvg+kv2T = \int_0^u \frac{dv}{g + k v^2}.

Factor out kk: 1g+kv2=1k1gk+v2\frac{1}{g + k v^2} = \frac{1}{k}\cdot\frac{1}{\frac{g}{k} + v^2}. Using dva2+v2=1aarctanva\int \frac{dv}{a^2 + v^2} = \frac{1}{a}\arctan\frac{v}{a} with a=gka = \sqrt{\frac{g}{k}}:

dvg+kv2=1kkgarctan ⁣(vkg)=1gkarctan ⁣(vkg)\int \frac{dv}{g + k v^2} = \frac{1}{k}\cdot\sqrt{\frac{k}{g}}\arctan\!\left(v\sqrt{\tfrac{k}{g}}\right) = \frac{1}{\sqrt{gk}}\arctan\!\left(v\sqrt{\tfrac{k}{g}}\right).

Evaluating from 00 to uu (the arctan is 00 at v=0v = 0):

T=1gkarctan ⁣(ukg)T = \frac{1}{\sqrt{gk}}\arctan\!\left(u\sqrt{\tfrac{k}{g}}\right) seconds, as required.

Mark notes: 1 mark for the equation of motion dvdt=(g+kv2)\frac{dv}{dt} = -(g + k v^2), 1 mark for separating and integrating to an arctan form, 1 mark for applying the limits v=uv = u to v=0v = 0.

HSC 20244 marksTwo particles AA and BB, each of mass 11 kg, move vertically in a medium exerting resistance kvk v, where k>0k > 0. They are simultaneously projected towards each other with the same speed v0v_0 m/s, where 0<v0<gk0 < v_0 < \frac{g}{k}. Particle AA is initially dd metres directly above BB, with d<2v0kd < \frac{2 v_0}{k}. Find the time taken for the particles to meet.
Show worked answer →

Let s=xAxBs = x_A - x_B be the separation (AA above BB). Subtracting the two equations of motion removes gravity, since both particles feel the same g-g.

For each particle, acceleration =gkv= -g - k v. Differencing:

d2sdt2=(gkvA)(gkvB)=k(vAvB)=kdsdt\frac{d^2 s}{dt^2} = (-g - k v_A) - (-g - k v_B) = -k(v_A - v_B) = -k\frac{ds}{dt}.

Let p=dsdtp = \frac{ds}{dt}. Then dpdt=kp\frac{dp}{dt} = -k p, so p=Lektp = L e^{-k t}. Initially AA moves down at v0v_0 and BB moves up at v0v_0, so vAvB=2v0v_A - v_B = -2 v_0 at t=0t = 0, giving L=2v0L = -2 v_0:

dsdt=2v0ekt\frac{ds}{dt} = -2 v_0 e^{-k t}.

Integrate: s=2v0kekt+Cs = \frac{2 v_0}{k} e^{-k t} + C. At t=0t = 0, s=ds = d, so C=d2v0kC = d - \frac{2 v_0}{k}:

s=2v0kekt+d2v0ks = \frac{2 v_0}{k} e^{-k t} + d - \frac{2 v_0}{k}.

The particles meet when s=0s = 0: 2v0kekt=2v0kd\frac{2 v_0}{k} e^{-k t} = \frac{2 v_0}{k} - d, so ekt=2v02v0kde^{k t} = \frac{2 v_0}{2 v_0 - k d}.

Therefore t=1kln ⁣(2v02v0kd)t = \frac{1}{k}\ln\!\left(\frac{2 v_0}{2 v_0 - k d}\right).

(The condition d<2v0kd < \frac{2 v_0}{k} makes 2v0kd>02 v_0 - k d > 0, so the logarithm is defined and t>0t > 0.)

Mark notes: 1 mark for the equations of motion, 1 mark for differencing to dpdt=kp\frac{dp}{dt} = -k p, 1 mark for the separation s(t)s(t) with correct constants, 1 mark for solving s=0s = 0.

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