Comprehensive Two-Dimensional and Three-Dimensional Particle Kinematics

Two-Dimensional Relative Velocity: Airplane Navigation in Wind

  • Galilean Relative Velocity Principle:

    • The velocity of a body relative to a reference frame is given by the vector sum of its velocity relative to an intermediate frame and the velocity of that intermediate frame relative to the primary frame.
    • For an airplane (PP) flying through moving wind/air (WW) over the ground (GG):     v⃗PG=v⃗PW+v⃗WG\vec{v}_{PG} = \vec{v}_{PW} + \vec{v}_{WG}
  • Given Parameters:

    • Plane airspeed relative to the wind: vPW=215 km/hv_{PW} = 215\,km/h
    • Wind velocity relative to the ground: vWG=65 km/hv_{WG} = 65\,km/h
    • Wind direction: 20∘20^\circ East of North
    • Desired ground track: Due East (along the positive xx-axis, requiring vPG,y=0v_{PG, y} = 0

Two-dimensional relative velocity vector addition diagram for airplane, wind, and ground

  • Vector Decomposition:

    • Coordinate axes: +x+x directed due East; +y+y directed due North.
    • Ground velocity components:     vPG,x=vPGv_{PG, x} = v_{PG}vPG,y=0v_{PG, y} = 0
    • Wind velocity components (directed 20∘20^\circ East of North):     vWG,x=vWGsin⁡(20∘)=65sin⁡(20∘)v_{WG, x} = v_{WG} \sin(20^\circ) = 65 \sin(20^\circ)vWG,y=vWGcos⁡(20∘)=65cos⁡(20∘)v_{WG, y} = v_{WG} \cos(20^\circ) = 65 \cos(20^\circ)
    • Plane-to-wind velocity components (heading angle θ\theta South of East):     vPW,x=vPWcos⁡(θ)=215cos⁡(θ)v_{PW, x} = v_{PW} \cos(\theta) = 215 \cos(\theta)vPW,y=−vPWsin⁡(θ)=−215sin⁡(θ)v_{PW, y} = -v_{PW} \sin(\theta) = -215 \sin(\theta)
  • Determination of Heading Angle θ\theta:

    • Balancing the vertical (yy) components:     vPG,y=vPW,y+vWG,yv_{PG, y} = v_{PW, y} + v_{WG, y}0=−215sin⁡(θ)+65cos⁡(20∘)0 = -215 \sin(\theta) + 65 \cos(20^\circ)
    • Solving for sin⁡(θ)\sin(\theta)sin⁡(θ)=65cos⁡(20∘)215=65×0.9397215≈0.2841\sin(\theta) = \frac{65 \cos(20^\circ)}{215} = \frac{65 \times 0.9397}{215} \approx 0.2841
    • Calculating the angle:     θ=arcsin⁡(0.2841)≈16.5∘\theta = \arcsin(0.2841) \approx 16.5^\circ
    • The plane must be directed at an angle of 16.5∘16.5^\circ South of East (or θ=−16.5∘\theta = -16.5^\circ relative to the +x+x-axis).
  • Determination of Ground Speed vPGv_{PG}:

    • Combining the horizontal (xx) components:     vPG=vPW,x+vWG,xv_{PG} = v_{PW, x} + v_{WG, x}vPG=215cos⁡(16.5∘)+65sin⁡(20∘)v_{PG} = 215 \cos(16.5^\circ) + 65 \sin(20^\circ)
    • Evaluating terms:     215cos⁡(16.5∘)≈215×0.9588=206.15 km/h215 \cos(16.5^\circ) \approx 215 \times 0.9588 = 206.15\,km/h65sin⁡(20∘)≈65×0.3420=22.23 km/h65 \sin(20^\circ) \approx 65 \times 0.3420 = 22.23\,km/hvPG=206.15+22.23=228.38 km/h≈228 km/hv_{PG} = 206.15 + 22.23 = 228.38\,km/h \approx 228\,km/h

Position and Displacement in Three Dimensions

  • Proton Position Vectors:

    • Initial position vector:     r⃗i=5.0i^−6.0j^+2.0k^ m\vec{r}_i = 5.0\hat{i} - 6.0\hat{j} + 2.0\hat{k}\,\text{m}
    • Final position vector:     r⃗f=−2.0i^+6.0j^+2.0k^ m\vec{r}_f = -2.0\hat{i} + 6.0\hat{j} + 2.0\hat{k}\,\text{m}
  • Displacement Vector Calculation:

    • Displacement definition:     Δr⃗=r⃗f−r⃗i\Delta\vec{r} = \vec{r}_f - \vec{r}_i
    • Evaluating individual cartesian components:     Δx=−2.0 m−5.0 m=−7.0 m\Delta x = -2.0\,\text{m} - 5.0\,\text{m} = -7.0\,\text{m}Δy=6.0 m−(−6.0 m)=12.0 m\Delta y = 6.0\,\text{m} - (-6.0\,\text{m}) = 12.0\,\text{m}Δz=2.0 m−2.0 m=0.0 m\Delta z = 2.0\,\text{m} - 2.0\,\text{m} = 0.0\,\text{m}
    • Result in unit-vector notation:     Δr⃗=−7.0i^+12.0j^+0.0k^ m=−7.0i^+12.0j^ m\Delta\vec{r} = -7.0\hat{i} + 12.0\hat{j} + 0.0\hat{k}\,\text{m} = -7.0\hat{i} + 12.0\hat{j}\,\text{m}
  • Plane Parallel to Displacement:

    • Because the displacement along the zz-axis is zero (Δz=0\Delta z = 0), the displacement has no perpendicular component to the xyxy-plane.
    • Consequently, the displacement vector is parallel to the xyxy-plane.

Parametric Harmonic Motion and Circular Trajectories

  • Parametric Position Vector:

    • Position as a function of time:     r⃗(t)=4cos⁡(πtT)i^−4sin⁡(πtT)j^\vec{r}(t) = 4\cos\left(\frac{\pi t}{T}\right)\hat{i} - 4\sin\left(\frac{\pi t}{T}\right)\hat{j}
    • Baseline position at t=0t = 0:     r⃗(0)=4cos⁡(0)i^−4sin⁡(0)j^=4i^\vec{r}(0) = 4\cos(0)\hat{i} - 4\sin(0)\hat{j} = 4\hat{i}
  • Displacements and Distances from Origin at Specific Times:

    • Case 1: t=T3t = \frac{T}{3}
    • Position:       r⃗(T3)=4cos⁡(π3)i^−4sin⁡(π3)j^=4(12)i^−4(32)j^=2i^−23j^\vec{r}\left(\frac{T}{3}\right) = 4\cos\left(\frac{\pi}{3}\right)\hat{i} - 4\sin\left(\frac{\pi}{3}\right)\hat{j} = 4\left(\frac{1}{2}\right)\hat{i} - 4\left(\frac{\sqrt{3}}{2}\right)\hat{j} = 2\hat{i} - 2\sqrt{3}\hat{j}
    • Displacement vector:       Δr⃗=r⃗(T3)−r⃗(0)=(2−4)i^−23j^=−2i^−23j^\Delta\vec{r} = \vec{r}\left(\frac{T}{3}\right) - \vec{r}(0) = (2 - 4)\hat{i} - 2\sqrt{3}\hat{j} = -2\hat{i} - 2\sqrt{3}\hat{j}
    • Magnitude of displacement:       ∣Δr⃗∣=(−2)2+(−23)2=4+12=16=4|\Delta\vec{r}| = \sqrt{(-2)^2 + (-2\sqrt{3})^2} = \sqrt{4 + 12} = \sqrt{16} = 4
    • Distance to the origin:       ∣r⃗(T/3)∣=22+(−23)2=4+12=4|\vec{r}(T/3)| = \sqrt{2^2 + (-2\sqrt{3})^2} = \sqrt{4 + 12} = 4
    • Case 2: t=T2t = \frac{T}{2}
    • Position:       r⃗(T2)=4cos⁡(π2)i^−4sin⁡(π2)j^=0i^−4j^=−4j^\vec{r}\left(\frac{T}{2}\right) = 4\cos\left(\frac{\pi}{2}\right)\hat{i} - 4\sin\left(\frac{\pi}{2}\right)\hat{j} = 0\hat{i} - 4\hat{j} = -4\hat{j}
    • Displacement vector:       Δr⃗=r⃗(T2)−r⃗(0)=−4i^−4j^\Delta\vec{r} = \vec{r}\left(\frac{T}{2}\right) - \vec{r}(0) = -4\hat{i} - 4\hat{j}
    • Magnitude of displacement:       ∣Δr⃗∣=(−4)2+(−4)2=32=42≈5.66|\Delta\vec{r}| = \sqrt{(-4)^2 + (-4)^2} = \sqrt{32} = 4\sqrt{2} \approx 5.66
    • Distance to the origin:       ∣r⃗(T/2)∣=02+(−4)2=4|\vec{r}(T/2)| = \sqrt{0^2 + (-4)^2} = 4
    • Case 3: t=2Tt = 2T
    • Position:       r⃗(2T)=4cos⁡(2π)i^−4sin⁡(2π)j^=4i^−0j^=4i^\vec{r}(2T) = 4\cos(2\pi)\hat{i} - 4\sin(2\pi)\hat{j} = 4\hat{i} - 0\hat{j} = 4\hat{i}
    • Displacement vector:       Δr⃗=r⃗(2T)−r⃗(0)=4i^−4i^=0⃗=0i^+0j^\Delta\vec{r} = \vec{r}(2T) - \vec{r}(0) = 4\hat{i} - 4\hat{i} = \vec{0} = 0\hat{i} + 0\hat{j}
    • Magnitude of displacement:       ∣Δr⃗∣=0|\Delta\vec{r}| = 0
    • Distance to the origin:       ∣r⃗(2T)∣=42+02=4|\vec{r}(2T)| = \sqrt{4^2 + 0^2} = 4
    • General Distance to Origin for all tt:     r(t)=x(t)2+y(t)2=16cos⁡2(πtT)+16sin⁡2(πtT)=16=4r(t) = \sqrt{x(t)^2 + y(t)^2} = \sqrt{16\cos^2\left(\frac{\pi t}{T}\right) + 16\sin^2\left(\frac{\pi t}{T}\right)} = \sqrt{16} = 4
    • The particle undergoes uniform circular motion of constant radius R=4R = 4 around the origin.
  • Angle with the Positive xx-Axis for Arbitrary tt:

    • Tangent of the directional angle:     tan⁡(θ)=y(t)x(t)=−4sin⁡(πtT)4cos⁡(πtT)=−tan⁡(πtT)\tan(\theta) = \frac{y(t)}{x(t)} = \frac{-4\sin\left(\frac{\pi t}{T}\right)}{4\cos\left(\frac{\pi t}{T}\right)} = -\tan\left(\frac{\pi t}{T}\right)
    • Evaluating angle:     θ(t)=−πtT\theta(t) = -\frac{\pi t}{T}
    • Measured in radians clockwise from the positive xx-axis, or as standard counterclockwise angle 2π−πtT rad2\pi - \frac{\pi t}{T}\,\text{rad}.

Differential Kinematics in Two and Three Dimensions

  • Kinematics of an Electron:

    • Given position vector (tt in seconds, r⃗\vec{r} in meters):     r⃗(t)=3.00ti^−4.00t2j^+2.00k^\vec{r}(t) = 3.00t\hat{i} - 4.00t^2\hat{j} + 2.00\hat{k}
    • Velocity Function by Differentiation:     v⃗(t)=dr⃗dt=ddt(3.00t)i^−ddt(4.00t2)j^+ddt(2.00)k^\vec{v}(t) = \frac{d\vec{r}}{dt} = \frac{d}{dt}(3.00t)\hat{i} - \frac{d}{dt}(4.00t^2)\hat{j} + \frac{d}{dt}(2.00)\hat{k}v⃗(t)=3.00i^−8.00tj^+0k^ m/s\vec{v}(t) = 3.00\hat{i} - 8.00t\hat{j} + 0\hat{k}\,\text{m/s}
    • Unit-Vector Notation at t=2.00 st = 2.00\,\text{s}:     v⃗(2.00)=3.00i^−8.00(2.00)j^=3.00i^−16.0j^ m/s\vec{v}(2.00) = 3.00\hat{i} - 8.00(2.00)\hat{j} = 3.00\hat{i} - 16.0\hat{j}\,\text{m/s}
    • Velocity Magnitude at t=2.00 st = 2.00\,\text{s}:     v=vx2+vy2=(3.00)2+(−16.0)2=9.00+256.0=265.0≈16.3 m/sv = \sqrt{v_x^2 + v_y^2} = \sqrt{(3.00)^2 + (-16.0)^2} = \sqrt{9.00 + 256.0} = \sqrt{265.0} \approx 16.3\,\text{m/s}
    • Orientation Angle Relative to Positive xx-Axis:     θ=arctan⁡(vyvx)=arctan⁡(−16.03.00)≈arctan⁡(−5.333)≈−79.4∘\theta = \arctan\left(\frac{v_y}{v_x}\right) = \arctan\left(\frac{-16.0}{3.00}\right) \approx \arctan(-5.333) \approx -79.4^\circ
    • Corresponds to 79.4∘79.4^\circ below the positive xx-axis (or 280.6∘280.6^\circ standard counterclockwise).
  • Two-Dimensional Kinematics of Polynomial Position:

    • Given position:     r⃗(t)=(2t3−5t)i^+(6−7t4)j^\vec{r}(t) = (2t^3 - 5t)\hat{i} + (6 - 7t^4)\hat{j}
    • Position at t=2.0 st = 2.0\,\text{s}:     x(2.0)=2(2.0)3−5(2.0)=16−10=6 mx(2.0) = 2(2.0)^3 - 5(2.0) = 16 - 10 = 6\,\text{m}y(2.0)=6−7(2.0)4=6−7(16)=6−112=−106 my(2.0) = 6 - 7(2.0)^4 = 6 - 7(16) = 6 - 112 = -106\,\text{m}r⃗(2.0)=6i^−106j^ m\vec{r}(2.0) = 6\hat{i} - 106\hat{j}\,\text{m}
    • Velocity at t=2.0 st = 2.0\,\text{s}:     vx(t)=ddt(2t3−5t)=6t2−5v_x(t) = \frac{d}{dt}(2t^3 - 5t) = 6t^2 - 5vy(t)=ddt(6−7t4)=−28t3v_y(t) = \frac{d}{dt}(6 - 7t^4) = -28t^3vx(2.0)=6(2.0)2−5=24−5=19 m/sv_x(2.0) = 6(2.0)^2 - 5 = 24 - 5 = 19\,\text{m/s}vy(2.0)=−28(2.0)3=−28(8)=−224 m/sv_y(2.0) = -28(2.0)^3 = -28(8) = -224\,\text{m/s}v⃗(2.0)=19i^−224j^ m/s\vec{v}(2.0) = 19\hat{i} - 224\hat{j}\,\text{m/s}
    • Acceleration at t=2.0 st = 2.0\,\text{s}:     ax(t)=ddt(6t2−5)=12ta_x(t) = \frac{d}{dt}(6t^2 - 5) = 12tay(t)=ddt(−28t3)=−84t2a_y(t) = \frac{d}{dt}(-28t^3) = -84t^2ax(2.0)=12(2.0)=24 m/s2a_x(2.0) = 12(2.0) = 24\,\text{m/s}^2ay(2.0)=−84(2.0)2=−84(4)=−336 m/s2a_y(2.0) = -84(2.0)^2 = -84(4) = -336\,\text{m/s}^2a⃗(2.0)=24i^−336j^ m/s2\vec{a}(2.0) = 24\hat{i} - 336\hat{j}\,\text{m/s}^2
    • Orientation of Path Tangent at t=2.0 st = 2.0\,\text{s}:
    • The tangent vector is aligned with the velocity vector v⃗(2.0)\vec{v}(2.0):       θ=arctan⁡(vyvx)=arctan⁡(−22419)≈arctan⁡(−11.789)≈−85.2∘\theta = \arctan\left(\frac{v_y}{v_x}\right) = \arctan\left(\frac{-224}{19}\right) \approx \arctan(-11.789) \approx -85.2^\circ
    • Angle is −85.2∘-85.2^\circ relative to the positive xx-axis (or 274.8∘274.8^\circ counterclockwise).

Integral Kinematics: Reconstructing Position from Rates of Change

  • Motion Governed by Time-Varying Velocity:

    • Velocity function:     v⃗(t)=(4+2t2)i^+(−10−4t)j^\vec{v}(t) = (4 + 2t^2)\hat{i} + (-10 - 4t)\hat{j}
    • Boundary condition:     r⃗(0)=0i^+0j^\vec{r}(0) = 0\hat{i} + 0\hat{j}
    • Velocity at t=3 st = 3\,\text{s}:     vx(3)=4+2(3)2=4+18=22 m/sv_x(3) = 4 + 2(3)^2 = 4 + 18 = 22\,\text{m/s}vy(3)=−10−4(3)=−10−12=−22 m/sv_y(3) = -10 - 4(3) = -10 - 12 = -22\,\text{m/s}v⃗(3)=22i^−22j^ m/s\vec{v}(3) = 22\hat{i} - 22\hat{j}\,\text{m/s}
    • Integration for Position:     x(t)=∫0t(4+2τ2) dτ=4t+23t3x(t) = \int_0^t (4 + 2\tau^2)\,d\tau = 4t + \frac{2}{3}t^3y(t)=∫0t(−10−4τ) dτ=−10t−2t2y(t) = \int_0^t (-10 - 4\tau)\,d\tau = -10t - 2t^2
    • Position at t=3 st = 3\,\text{s}:     x(3)=4(3)+23(27)=12+18=30 mx(3) = 4(3) + \frac{2}{3}(27) = 12 + 18 = 30\,\text{m}y(3)=−10(3)−2(9)=−30−18=−48 my(3) = -10(3) - 2(9) = -30 - 18 = -48\,\text{m}r⃗(3)=30i^−48j^ m\vec{r}(3) = 30\hat{i} - 48\hat{j}\,\text{m}
    • Moving Direction with Respect to the xx-Axis:     θ=arctan⁡(vyvx)=arctan⁡(−2222)=arctan⁡(−1)=−45∘\theta = \arctan\left(\frac{v_y}{v_x}\right) = \arctan\left(\frac{-22}{22}\right) = \arctan(-1) = -45^\circ
    • Directed at 45∘45^\circ below the positive xx-axis (or 315∘315^\circ).
  • Motion Governed by Time-Varying Acceleration:

    • Given acceleration and initial states:     a⃗(t)=(2+4t3)i^+(6−3t2)j^\vec{a}(t) = (2 + 4t^3)\hat{i} + (6 - 3t^2)\hat{j}v⃗(0)=10i^ m/s\vec{v}(0) = 10\hat{i}\,\text{m/s}r⃗(0)=0i^+0j^ m\vec{r}(0) = 0\hat{i} + 0\hat{j}\,\text{m}
    • Velocity Vector by Integration:     vx(t)=v0x+∫0t(2+4τ3) dτ=10+2t+t4v_x(t) = v_{0x} + \int_0^t (2 + 4\tau^3)\,d\tau = 10 + 2t + t^4vy(t)=v0y+∫0t(6−3τ2) dτ=0+6t−t3v_y(t) = v_{0y} + \int_0^t (6 - 3\tau^2)\,d\tau = 0 + 6t - t^3v⃗(t)=(10+2t+t4)i^+(6t−t3)j^\vec{v}(t) = (10 + 2t + t^4)\hat{i} + (6t - t^3)\hat{j}
    • Velocity at t=2 st = 2\,\text{s}:     vx(2)=10+2(2)+(2)4=10+4+16=30 m/sv_x(2) = 10 + 2(2) + (2)^4 = 10 + 4 + 16 = 30\,\text{m/s}vy(2)=6(2)−(2)3=12−8=4 m/sv_y(2) = 6(2) - (2)^3 = 12 - 8 = 4\,\text{m/s}v⃗(2)=30i^+4j^ m/s\vec{v}(2) = 30\hat{i} + 4\hat{j}\,\text{m/s}
    • Position Vector by Integration:     x(t)=x0+∫0t(10+2τ+τ4) dτ=10t+t2+t55x(t) = x_0 + \int_0^t (10 + 2\tau + \tau^4)\,d\tau = 10t + t^2 + \frac{t^5}{5}y(t)=y0+∫0t(6τ−τ3) dτ=3t2−t44y(t) = y_0 + \int_0^t (6\tau - \tau^3)\,d\tau = 3t^2 - \frac{t^4}{4}r⃗(t)=(10t+t2+t55)i^+(3t2−t44)j^\vec{r}(t) = \left(10t + t^2 + \frac{t^5}{5}\right)\hat{i} + \left(3t^2 - \frac{t^4}{4}\right)\hat{j}
    • Position at t=2 st = 2\,\text{s}:     x(2)=10(2)+(2)2+(2)55=20+4+6.4=30.4 mx(2) = 10(2) + (2)^2 + \frac{(2)^5}{5} = 20 + 4 + 6.4 = 30.4\,\text{m}y(2)=3(2)2−(2)44=12−4=8.0 my(2) = 3(2)^2 - \frac{(2)^4}{4} = 12 - 4 = 8.0\,\text{m}r⃗(2)=30.4i^+8.0j^ m\vec{r}(2) = 30.4\hat{i} + 8.0\hat{j}\,\text{m}

Projectile Acceleration Components and Launch Optimization

  • Tangential and Radial Acceleration for a Horizontal Projectile:

    • Physical conditions:
    • Initial velocity: v⃗(0)=v0i^\vec{v}(0) = v_0\hat{i}
    • Constant gravitational acceleration: a⃗=−gj^\vec{a} = -g\hat{j}
    • Air resistance: neglected
    • Velocity Components:     vx(t)=v0v_x(t) = v_0vy(t)=−gtv_y(t) = -gtv(t)=v02+g2t2v(t) = \sqrt{v_0^2 + g^2t^2}
    • Derivation of Tangential Acceleration (ata_t):
    • Rate of change of scalar speed:       at=dvdt=ddt(v02+g2t2)=2g2t2v02+g2t2=g2tv02+g2t2a_t = \frac{dv}{dt} = \frac{d}{dt}\left(\sqrt{v_0^2 + g^2t^2}\right) = \frac{2g^2t}{2\sqrt{v_0^2 + g^2t^2}} = \frac{g^2 t}{\sqrt{v_0^2 + g^2t^2}}
    • Equivalent vector projection:       at=a⃗⋅v⃗v=(0)(v0)+(−g)(−gt)v02+g2t2=g2tv02+g2t2a_t = \frac{\vec{a} \cdot \vec{v}}{v} = \frac{(0)(v_0) + (-g)(-gt)}{\sqrt{v_0^2 + g^2t^2}} = \frac{g^2 t}{\sqrt{v_0^2 + g^2t^2}}
    • Derivation of Radial (Normal) Acceleration (ara_r):
    • Orthogonal acceleration relationship:       a2=at2+ar2=g2a^2 = a_t^2 + a_r^2 = g^2
    • Solving for radial component:       ar=g2−at2=g2−g4t2v02+g2t2=g2v02+g4t2−g4t2v02+g2t2=gv0v02+g2t2a_r = \sqrt{g^2 - a_t^2} = \sqrt{g^2 - \frac{g^4 t^2}{v_0^2 + g^2t^2}} = \sqrt{\frac{g^2 v_0^2 + g^4 t^2 - g^4 t^2}{v_0^2 + g^2t^2}} = \frac{g v_0}{\sqrt{v_0^2 + g^2t^2}}
    • Boundary Limits:
    • At launch (t=0t = 0): at=0a_t = 0, ar=ga_r = g
    • At asymptotic limit (t→∞t \rightarrow \infty): at→ga_t \rightarrow g, ar→0a_r \rightarrow 0
  • Launch Angle for Range Equal to Twice Maximum Height:

    • Target condition:     R=2HR = 2H
    • Analytic expressions:
    • Maximum height: H=v02sin⁡2(θ)2gH = \frac{v_0^2 \sin^2(\theta)}{2g}
    • Range on flat ground: R=v02sin⁡(2θ)g=2v02sin⁡(θ)cos⁡(θ)gR = \frac{v_0^2 \sin(2\theta)}{g} = \frac{2v_0^2 \sin(\theta)\cos(\theta)}{g}
    • Algebraic reduction:     2v02sin⁡(θ)cos⁡(θ)g=2(v02sin⁡2(θ)2g)\frac{2v_0^2 \sin(\theta)\cos(\theta)}{g} = 2\left(\frac{v_0^2 \sin^2(\theta)}{2g}\right)2sin⁡(θ)cos⁡(θ)=sin⁡2(θ)2\sin(\theta)\cos(\theta) = \sin^2(\theta)
    • Dividing by sin⁡(θ)cos⁡(θ)\sin(\theta)\cos(\theta) (sin⁡(θ)≠0\sin(\theta) \neq 0, cos⁡(θ)≠0\cos(\theta) \neq 0):     tan⁡(θ)=2\tan(\theta) = 2
    • Angle calculation:     θ=arctan⁡(2)≈63.4∘\theta = \arctan(2) \approx 63.4^\circ

Circular Kinematics: Uniform and Non-Uniform Motion

  • Revolution Period of a Merry-Go-Round:

    • Given values:
    • Distance from axis (radius): r=7.5 mr = 7.5\,\text{m}
    • Centripetal acceleration: ac=3.3 m/s2a_c = 3.3\,\text{m/s}^2
    • Formula relating centripetal acceleration and period TT:     ac=ω2r=(2πT)2r=4π2rT2a_c = \omega^2 r = \left(\frac{2\pi}{T}\right)^2 r = \frac{4\pi^2 r}{T^2}
    • Solving for period TT:     T=2πrac=2π7.53.3≈2π2.2727≈2π×1.5076≈9.47 sT = 2\pi \sqrt{\frac{r}{a_c}} = 2\pi \sqrt{\frac{7.5}{3.3}} \approx 2\pi \sqrt{2.2727} \approx 2\pi \times 1.5076 \approx 9.47\,\text{s}
    • Equivalent linear speed check:     v=acr=3.3×7.5≈4.975 m/sv = \sqrt{a_c r} = \sqrt{3.3 \times 7.5} \approx 4.975\,\text{m/s}T=2πrv=2π(7.5)4.975≈9.47 sT = \frac{2\pi r}{v} = \frac{2\pi (7.5)}{4.975} \approx 9.47\,\text{s}
  • Acceleration of a Decelerating Vehicle on a Circular Track:

    • Given values:
    • Track radius: R=400 mR = 400\,\text{m}
    • Instantaneous speed: v=10 m/sv = 10\,\text{m/s}
    • Tangential acceleration: at=−0.2 m/s2a_t = -0.2\,\text{m/s}^2
    • Radial (Normal) Acceleration:     ar=v2R=(10)2400=100400=0.25 m/s2a_r = \frac{v^2}{R} = \frac{(10)^2}{400} = \frac{100}{400} = 0.25\,\text{m/s}^2
    • Total Acceleration Magnitude:
    • By orthogonality of radial and tangential components:       a=ar2+at2=(0.25)2+(−0.2)2=0.0625+0.0400=0.1025≈0.320 m/s2a = \sqrt{a_r^2 + a_t^2} = \sqrt{(0.25)^2 + (-0.2)^2} = \sqrt{0.0625 + 0.0400} = \sqrt{0.1025} \approx 0.320\,\text{m/s}^2
    • Direction Relative to Inward Radial Direction:     ϕ=arctan⁡(∣at∣ar)=arctan⁡(0.20.25)=arctan⁡(0.8)≈38.7∘\phi = \arctan\left(\frac{|a_t|}{a_r}\right) = \arctan\left(\frac{0.2}{0.25}\right) = \arctan(0.8) \approx 38.7^\circ
    • Total acceleration points inwards and backwards at an angle of 38.7∘38.7^\circ behind the center-pointing normal.

Relative Motion: Observer Reference Frames and Windblown Rain

  • Motion Decomposition and Frame Notation:

    • Subscript notation:
    • RR: Raindrops
    • GG: Stationary Ground observer
    • TT: Moving Train observer
    • Vector addition equation:     v⃗RG=v⃗RT+v⃗TG\vec{v}_{RG} = \vec{v}_{RT} + \vec{v}_{TG}
  • Kinematic Observations and Coordinates:

    • Let horizontal South be +x+x, and vertical downward be +y+y.
    • Train velocity relative to ground:     v⃗TG=30i^ m/s\vec{v}_{TG} = 30\hat{i}\,\text{m/s}
    • Rain path observed on train:
    • Drops fall perfectly vertically, implying no horizontal component relative to the train:       vRT,x=0 m/sv_{RT, x} = 0\,\text{m/s}vRT,y=vyv_{RT, y} = v_y
    • Rain path observed from ground:
    • Vector sum:       vRG,x=vRT,x+vTG,x=0+30 m/s=30 m/sv_{RG, x} = v_{RT, x} + v_{TG, x} = 0 + 30\,\text{m/s} = 30\,\text{m/s}vRG,y=vyv_{RG, y} = v_y
    • Angle with vertical: θ=70∘\theta = 70^\circ
  • Geometric Relationship and Speed Determination:

    • Right triangle formed by components:     sin⁡(70∘)=vRG,xvRG=30vRG\sin(70^\circ) = \frac{v_{RG, x}}{v_{RG}} = \frac{30}{v_{RG}}
    • Solving directly for the raindrop speed relative to the ground (vRGv_{RG}):     vRG=30sin⁡(70∘)=300.9397≈31.9 m/sv_{RG} = \frac{30}{\sin(70^\circ)} = \frac{30}{0.9397} \approx 31.9\,\text{m/s}
    • Vertical Speed Component (vRG,yv_{RG, y}):     vRG,y=vRG,xtan⁡(70∘)=30tan⁡(70∘)=302.7475≈10.9 m/sv_{RG, y} = \frac{v_{RG, x}}{\tan(70^\circ)} = \frac{30}{\tan(70^\circ)} = \frac{30}{2.7475} \approx 10.9\,\text{m/s}
    • Verification via Pythagorean Theorem:     vRG=(30)2+(10.92)2=900+119.2=1019.2≈31.9 m/sv_{RG} = \sqrt{(30)^2 + (10.92)^2} = \sqrt{900 + 119.2} = \sqrt{1019.2} \approx 31.9\,\text{m/s}