Relative velocity in two dimensions Knowledge-Based Study

Physics · Motion · Physics · Two-Dimensional Motion

Physics topic explanations on Relative velocity in two dimensions.

Study notes

  1. Frames of Reference and Vector Foundations

    Motion is inherently relative; the measured velocity of an object depends entirely on the observer's frame of reference. In one-dimensional motion, relative velocity is handled using simple positive or negative signs along a single line. In two dimensions, velocity must be treated as a full vector possessing both magnitude and direction.

    Consider two moving objects, A and B, observed from a common stationary reference frame G (typically the ground). The velocity of object A relative to object B, denoted as v⃗A/B\vec{v}_{A/B}, describes how object A moves as seen by an observer traveling with object B.

    The fundamental vector relationship is expressed as:

    v⃗A/B=v⃗A−v⃗B\vec{v}_{A/B} = \vec{v}_A - \vec{v}_B

    Equivalently, this relation can be written in terms of vector addition:

    v⃗A=v⃗A/B+v⃗B\vec{v}_A = \vec{v}_{A/B} + \vec{v}_B

    Here, v⃗A\vec{v}_A and v⃗B\vec{v}_B represent the velocities of objects A and B relative to the ground.

    Resolving Vectors into Orthogonal Components

    To analyze two-dimensional relative motion systematically, velocities are resolved into perpendicular components along Cartesian coordinates (usually horizontal xx and vertical yy, or East-West and North-South).

    Given velocity vectors in component form:

    • v⃗A=vAxi^+vAyj^\vec{v}_A = v_{Ax}\hat{i} + v_{Ay}\hat{j}
    • v⃗B=vBxi^+vByj^\vec{v}_B = v_{Bx}\hat{i} + v_{By}\hat{j}

    The relative velocity vector is obtained by subtracting corresponding components:

    v⃗A/B=(vAx−vBx)i^+(vAy−vBy)j^\vec{v}_{A/B} = (v_{Ax} - v_{Bx})\hat{i} + (v_{Ay} - v_{By})\hat{j}

    The magnitude and direction of the relative velocity are calculated as:

    • Magnitude: ∣v⃗A/B∣=(vAx−vBx)2+(vAy−vBy)2|\vec{v}_{A/B}| = \sqrt{(v_{Ax} - v_{Bx})^2 + (v_{Ay} - v_{By})^2}
    • Direction: θ=arctan⁡(vAy−vByvAx−vBx)\theta = \arctan\left(\frac{v_{Ay} - v_{By}}{v_{Ax} - v_{Bx}}\right)

    This component method avoids ambiguities that can arise when constructing scale vector diagrams by hand.

    Motion in a Moving Medium

    A classic application of two-dimensional relative velocity involves an object moving within a moving fluid, such as a boat crossing a flowing river or an aircraft flying through wind.

    Let:

    • v⃗b/w\vec{v}_{b/w} = velocity of the boat relative to the water (the heading and engine speed)
    • v⃗w/g\vec{v}_{w/g} = velocity of the water relative to the ground (river current)
    • v⃗b/g\vec{v}_{b/g} = velocity of the boat relative to the ground (the actual path traversed)

    By vector addition:

    v⃗b/g=v⃗b/w+v⃗w/g\vec{v}_{b/g} = \vec{v}_{b/w} + \vec{v}_{w/g}

    Key Scenarios:

    1. Crossing in Minimum Time: The boat aims perpendicular to the riverbank. The crossing time depends strictly on the river width dd and the perpendicular component of speed: t=dvb/wt = \frac{d}{v_{b/w}} The river current causes downstream drift without altering this crossing time.
    2. Crossing Along the Shortest Path: To travel straight across perpendicular to the banks, the resultant velocity v⃗b/g\vec{v}_{b/g} must point directly across. The boat must steer upstream at an angle α\alpha such that: sin⁡(α)=vw/gvb/w\sin(\alpha) = \frac{v_{w/g}}{v_{b/w}} This is only possible if vb/w>vw/gv_{b/w} > v_{w/g}.

    Apparent Velocity and Apparent Direction

    Another classic two-dimensional problem is determining the apparent direction of falling rain observed by a moving person or vehicle.

    Let v⃗r/g\vec{v}_{r/g} be the velocity of the rain relative to the ground (often directed vertically downward) and v⃗m/g\vec{v}_{m/g} be the velocity of the moving observer relative to the ground (directed horizontally).

    The velocity of the rain relative to the moving observer, v⃗r/m\vec{v}_{r/m}, is:

    v⃗r/m=v⃗r/g−v⃗m/g\vec{v}_{r/m} = \vec{v}_{r/g} - \vec{v}_{m/g}

    If rain falls vertically with speed vrv_r and an observer walks horizontally with speed vmv_m:

    • v⃗r/g=−vrj^\vec{v}_{r/g} = -v_r\hat{j}
    • v⃗m/g=vmi^\vec{v}_{m/g} = v_m\hat{i}
    • v⃗r/m=−vmi^−vrj^\vec{v}_{r/m} = -v_m\hat{i} - v_r\hat{j}

    The apparent rain appears to come from an angle θ\theta relative to the vertical, requiring the observer to tilt an umbrella forward:

    tan⁡(θ)=vmvr\tan(\theta) = \frac{v_m}{v_r}

    As the observer's forward speed increases, the rain strikes at an increasingly tilted angle.

    Structured Problem Analysis

    Example: Car A travels north at 20 m/s relative to the ground. Car B travels east at 15 m/s relative to the ground. Determine the velocity of Car A as observed from Car B.

    Step-by-Step Solution:

    1. Define coordinate axes: Let East be +i^+\hat{i} and North be +j^+\hat{j}.
    2. State given vectors:v⃗A=20j^ m/s\vec{v}_A = 20\hat{j}\text{ m/s}v⃗B=15i^ m/s\vec{v}_B = 15\hat{i}\text{ m/s}
    3. Apply the relative velocity formula:v⃗A/B=v⃗A−v⃗B=−15i^+20j^ m/s\vec{v}_{A/B} = \vec{v}_A - \vec{v}_B = -15\hat{i} + 20\hat{j}\text{ m/s}
    4. Calculate the magnitude:∣v⃗A/B∣=(−15)2+(20)2=225+400=625=25 m/s|\vec{v}_{A/B}| = \sqrt{(-15)^2 + (20)^2} = \sqrt{225 + 400} = \sqrt{625} = 25\text{ m/s}
    5. Determine the direction: The vector points into the second quadrant (west and north). The angle θ\theta north of west is:tan⁡(θ)=2015  ⟹  θ=arctan⁡(43)≈53.1∘ North of West\tan(\theta) = \frac{20}{15} \implies \theta = \arctan\left(\frac{4}{3}\right) \approx 53.1^\circ\text{ North of West}

    Summary:

    Relative velocity in two dimensions requires consistent reference frame labeling and accurate vector subtraction: v⃗A/B=v⃗A−v⃗B\vec{v}_{A/B} = \vec{v}_A - \vec{v}_B. Resolving into components reduces two-dimensional vector problems into two independent one-dimensional calculations.