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Mathematics · Ch 10 — Differential Calculus – Differentiability and Methods of Differentiation

Velocity of Rectilinear motion

10.2.2

Velocity of Rectilinear motion

The same secant-to-tangent limiting idea solves the velocity problem. Suppose an object moves along a straight line with position (signed distance from the origin) s=f(t)s=f(t) at time tt; ff is called the position function. Over the time interval from t0t_0 to t0+Δtt_0+\Delta t, the change in position is f(t0+Δt)−f(t0)f(t_0+\Delta t)-f(t_0), so the average velocity over that interval is

vavg=change in displacementchange in time=f(t0+Δt)−f(t0)Δt=ΔsΔt,v_{\text{avg}} = \frac{\text{change in displacement}}{\text{change in time}} = \frac{f(t_0+\Delta t)-f(t_0)}{\Delta t} = \frac{\Delta s}{\Delta t},

which is exactly the slope of the secant line PQPQ on the position–time graph, where P=(t0,f(t0))P=(t_0,f(t_0)) and Q=(t0+Δt, f(t0+Δt))Q=(t_0+\Delta t,\ f(t_0+\Delta t)).

A subtlety worth flagging: over one fixed time interval Δt\Delta t with one fixed net displacement, the object could in principle have followed any number of genuinely different motions C1,C2,C3,…C_1, C_2, C_3,\ldots between PP and QQ (speeding up then slowing down, pausing, reversing briefly, etc.) — all of them sharing the same average velocity Δs/Δt\Delta s/\Delta t, because average velocity only sees the two endpoints, not the path between them.

To recover the velocity at the single instant t=t0t=t_0, shrink the interval: compute average velocities over shorter and shorter windows [t0,t0+Δt][t_0, t_0+\Delta t], i.e. let Δt→0\Delta t \to 0. The instantaneous velocity is defined as the limit of these average velocities:

v(t0)=lim⁡Δt→0f(t0+Δt)−f(t0)Δt=lim⁡Δt→0ΔsΔt.v(t_0) = \lim_{\Delta t\to 0}\frac{f(t_0+\Delta t)-f(t_0)}{\Delta t} = \lim_{\Delta t\to0}\frac{\Delta s}{\Delta t}.

Geometrically, v(t0)v(t_0) is precisely the slope of the tangent line to the position–time graph at P=(t0,f(t0))P=(t_0,f(t_0)) — the velocity problem and the tangent-line problem are literally the same limit, read two different ways.

Worked illustration — free fall (the book's own example). A body falling freely from rest obeys the law of free fall s=12gt2s=\tfrac12 gt^2 (gg = the gravitational constant, no initial velocity). Then f(t0+Δt)=12g(t02+2t0Δt+(Δt)2)f(t_0+\Delta t)=\tfrac12 g\big(t_0^2+2t_0\Delta t+(\Delta t)^2\big), so

Δs=f(t0+Δt)−f(t0)=12g(2t0Δt+(Δt)2)=gΔt(t0+12Δt),\Delta s = f(t_0+\Delta t)-f(t_0) = \tfrac12 g\big(2t_0\Delta t+(\Delta t)^2\big) = g\Delta t\left(t_0+\tfrac12\Delta t\right), …