Motion in a Straight Line Study Notes

Fundamentals of Mechanics and Reference Frames

  • Mechanics is divided into two primary disciplines:

    • Kinematics: The study of motion without regard to the forces causing it.

    • Dynamics: The study of motion encompassing the forces that induce or alter it.

  • States of Rest and Motion:

    • Rest: An object is at rest when its position remains unchanged relative to its surroundings over time.

    • Motion: An object is in motion when its position changes relative to its surroundings over time.

    • Both states are strictly relative and dependent on the chosen reference point.

  • Frame of Reference: A coordinate system with an origin relative to which the position, displacement, and velocity of an object are observed and measured.

  • Point Object: A body whose physical dimensions are negligibly small compared to the distance it traverses.

Frame of reference showing an observer in an aeroplane coordinate system

Distance and Displacement

  • Scalars versus Vectors:

    • Scalar Quantities: Defined solely by magnitude; governed by ordinary arithmetic and algebra (e.g., distance, speed, mass, time, temperature).

    • Vector Quantities: Defined by both magnitude and direction; governed by vector algebra (e.g., displacement, velocity, acceleration, force).

  • Distance (dd):

    • The total actual path length traversed between initial and final points.

    • Scalar quantity; always positive or zero (d≥0d \ge 0).

    • Dependent on the path taken; never decreases during motion.

  • Displacement (ss):

    • The shortest straight-line vector directed from the initial position to the final position.

    • Vector quantity; can be positive, negative, or zero.

    • Independent of path; its magnitude is always less than or equal to distance (∣s∣≤d|s| \le d).

  • Distance and Displacement Along a Circular Arc:

    • Arc Distance (dd):     d=Rθd = R\theta     (where θ\theta is the subtended angle in radians).

    • Chord Displacement (∣Δs∣|\Delta s|):     ∣Δs∣=2Rsin⁡(θ2)|\Delta s| = 2R\sin\left(\frac{\theta}{2}\right)

Circular arc geometry with radius r and angle theta

Speed and Velocity

  • Speed:

    • The rate of change of distance with respect to time; scalar quantity with SI unit m/s\text{m/s} and dimensional formula [LT−1][LT^{-1}].

    • Average Speed:     vavg=Total DistanceTotal Time Takenv_{\text{avg}} = \frac{\text{Total Distance}}{\text{Total Time Taken}}

    • Instantaneous Speed: The speed of an object at an infinitesimal instant (v=dsdtv = \frac{ds}{dt}; always non-negative).

    • Special Average Speed Conditions:

    • Equal Time Intervals (t1=t2=⋯=tnt_1 = t_2 = \dots = t_n):       vavg=v1+v2+⋯+vnnv_{\text{avg}} = \frac{v_1 + v_2 + \dots + v_n}{n}

    • Equal Distance Halves (x1=x2x_1 = x_2 with speeds v1v_1 and v2v_2):       vavg=2v1v2v1+v2v_{\text{avg}} = \frac{2v_1v_2}{v_1 + v_2}

  • Velocity:

    • The rate of change of displacement with respect to time; vector quantity with SI unit m/s\text{m/s} and dimensional formula [LT−1][LT^{-1}].

    • Can be positive, negative, or zero depending on the direction of displacement.

    • Average Velocity:     v⃗avg=Total DisplacementTotal Time Taken=Δx⃗Δt\vec{v}_{\text{avg}} = \frac{\text{Total Displacement}}{\text{Total Time Taken}} = \frac{\Delta \vec{x}}{\Delta t}

    • Instantaneous Velocity:     v⃗=lim⁡Δt→0Δx⃗Δt=dx⃗dt\vec{v} = \lim_{\Delta t \to 0} \frac{\Delta \vec{x}}{\Delta t} = \frac{d\vec{x}}{dt}

Acceleration and Differential Kinematic Relations

  • Acceleration:

    • The rate of change of velocity with respect to time; vector quantity with SI unit m/s2\text{m/s}^2 and dimensional formula [LT−2][LT^{-2}].

    • Average Acceleration:     a⃗avg=Δv⃗Δt=v⃗2−v⃗1t2−t1\vec{a}_{\text{avg}} = \frac{\Delta \vec{v}}{\Delta t} = \frac{\vec{v}_2 - \vec{v}_1}{t_2 - t_1}

    • Instantaneous Acceleration:     a⃗=dv⃗dt=d2x⃗dt2\vec{a} = \frac{d\vec{v}}{dt} = \frac{d^2\vec{x}}{dt^2}

    • Spatial Form (Chain Rule formulation when velocity depends on position):     a=vdvdxa = v\frac{dv}{dx}

Modes of acceleration: speeding up, slowing down, and changing direction
  • Acceleration Types:

    • Positive Acceleration: Velocity increases over time in the chosen positive direction.

    • Negative Acceleration (Retardation / Deceleration): Velocity decreases over time.

    • Zero Acceleration: Velocity remains constant in magnitude and direction.

  • Calculus Interconversions:

    • Differentiation path: Position x⃗→ddtv⃗→ddta⃗\vec{x} \xrightarrow{\frac{d}{dt}} \vec{v} \xrightarrow{\frac{d}{dt}} \vec{a}.

    • Integration path: Acceleration a⃗→∫dtv⃗→∫dtx⃗\vec{a} \xrightarrow{\int dt} \vec{v} \xrightarrow{\int dt} \vec{x}.

Equations of Uniformly Accelerated Motion

  • Standard Equations for Constant Acceleration (a=constanta = \text{constant}):

    • Velocity-Time Relation:     v=u+atv = u + at

    • Position-Time Relation:     s=ut+12at2s = ut + \frac{1}{2}at^2

    • Velocity-Position Relation:     v2=u2+2asv^2 = u^2 + 2as

    • Mean Velocity Relation:     s=(u+v2)ts = \left(\frac{u + v}{2}\right)t

  • Distance Traversed in the nthn^{\text{th}} Second:

    • Determined by the difference between cumulative displacements: Snth=Sn−Sn−1S_n^{\text{th}} = S_n - S_{n-1}.

    • Direct Formula:     Snth=u+a2(2n−1)S_n^{\text{th}} = u + \frac{a}{2}(2n - 1)

Vertical Free Fall and Motion Under Gravity

  • Governing Parameter: Gravitational acceleration (g=9.8 m/s2g = 9.8\,\text{m/s}^2 or 10 m/s210\,\text{m/s}^2), always directed downward toward the Earth's center.

  • Object Dropped from Rest (u=0u = 0, height hh):

    • Velocity upon Ground Impact:     v=2ghv = \sqrt{2gh}

    • Total Time of Fall:     t=2hgt = \sqrt{\frac{2h}{g}}

  • Object Projected Vertically Upward (Initial speed uu):

    • Maximum Altitude Attained:     Hmax=u22gH_{\text{max}} = \frac{u^2}{2g}

    • Time of Ascent to Crest:     tup=ugt_{\text{up}} = \frac{u}{g}

    • Total Time of Flight (Ascent and Descent):     T=2ugT = \frac{2u}{g}

  • Galileo's Law of Odd Numbers:

    • For an object released from rest under uniform gravitational acceleration, the displacements covered during equal, consecutive time intervals are proportional to consecutive odd integers:     1:3:5:7:9:…1 : 3 : 5 : 7 : 9 : \dots

Graphical Analysis of Motion

  • Geometric Foundations:

    • The gradient of a line or curve represents the instantaneous rate of change:     m=tan⁡(θ)=ΔyΔxm = \tan(\theta) = \frac{\Delta y}{\Delta x}

Linear slope defined by the counter-clockwise tangent angleFour cases of variable slope with concavity variations
  • Graph Interpretations:

    • Position-Time (s–ts\text{--}t) Graph:

    • Slope represents instantaneous velocity (v=dsdtv = \frac{ds}{dt}).

    • A horizontal slope (m=0m = 0) indicates a body at rest.

    • Constant non-zero slope indicates uniform velocity.

    • Upward concavity indicates positive acceleration; downward concavity indicates negative acceleration.

    • Velocity-Time (v–tv\text{--}t) Graph:

    • Slope represents instantaneous acceleration (a=dvdta = \frac{dv}{dt}).

    • Area enclosed between the curve and the time axis equals total displacement (Δx=∫v dt\Delta x = \int v\,dt).

    • Acceleration-Time (a–ta\text{--}t) Graph:

    • Area enclosed between the curve and the time axis yields the net change in velocity (Δv=∫a dt\Delta v = \int a\,dt).

  • Impossible Graph Configurations in Classical Kinematics:

    • Vertical lines or closed loops (a single particle cannot hold multiple positions or velocities simultaneously at the same instant).

    • Decreasing distance or negative values on a distance-time graph.

    • Negative values on a speed-time graph.

Relative Velocity in One Dimension

  • Relative Motion Formulation:

    • The velocity of object AA relative to object BB is defined as:     v⃗AB=v⃗A−v⃗B\vec{v}_{AB} = \vec{v}_A - \vec{v}_B

  • Collinear Motion Regimes:

    • Same Direction: Magnitudes subtract:     vrel=∣vA−vB∣v_{\text{rel}} = |v_A - v_B|

    • Opposite Directions: Magnitudes add:     vrel=vA+vBv_{\text{rel}} = v_A + v_B

  • Crossing of Extended Bodies (e.g., Trains of length L1L_1 and L2L_2 on parallel tracks):

    • Total distance required for complete passage:     Dtotal=L1+L2D_{\text{total}} = L_1 + L_2

    • Time required to clear each other:     t=L1+L2vrelt = \frac{L_1 + L_2}{v_{\text{rel}}}