Summary of "Motion in a Plane🔥 | CLASS 11 Physics | Complete Chapter | NCERT Covered | Prashant Kirad"

Overview

This lecture covers the complete Class‑11 NCERT chapter “Motion in a Plane” by Prashant Kirad (Prashant Bhaiya). Topics include: - Vector basics and operations - Kinematics in two dimensions - Projectile motion (derivations and standard results) - Circular motion (kinematics and centripetal quantities) - Relative motion problems (rain/umbrella and boat/river)

The instructor proves core formulas, explains theory visually, and works through many numerical and exam‑style examples.

Key concepts and definitions

Scalar vs vector
- Scalar: magnitude only.
- Vector: magnitude and direction.
Vector representation: arrow with tail & head; components commonly written as a i + b j + c k (i, j, k are unit basis vectors).
Unit vector: û = v / |v| (direction only).
Magnitude of vector v = a i + b j + c k: |v| = sqrt(a^2 + b^2 + c^2).
Resolution of a vector at angle θ: components = v cosθ (adjacent), v sinθ (opposite).
Vector equality: same magnitude, same direction, and same physical quantity (displacement vs velocity are not equal vectors even if numerically same).
Parallel, anti‑parallel, and zero vector concepts.

Vector addition and subtraction

Triangle law: place head of one vector at the tail of the other; resultant is the third side.
Parallelogram law: resultant is the diagonal when two vectors form adjacent sides of a parallelogram.

Resultant for two vectors of magnitudes a and b with included angle θ: - Magnitude: R = sqrt(a^2 + b^2 + 2ab cosθ) - Direction (measured from vector a): tanα = (b sinθ) / (a + b cosθ)

Special cases: - θ = 0° → R_max = a + b - θ = 180° → R_min = |a − b| - θ = 90° → R = sqrt(a^2 + b^2)

Subtraction is handled by taking b → −b in the addition formula (sign change in the 2ab cosθ term).

Motion in a plane (kinematics)

Treat x and y independently:
- Solve x(t) and y(t) separately.
- Velocity = derivative of position (componentwise). Acceleration = derivative of velocity (componentwise).
- Use integration to go from acceleration → velocity → displacement when needed.

Example method: given r(t) = x(t) i + y(t) j, - v(t) = dx/dt i + dy/dt j - a(t) = d^2x/dt^2 i + d^2y/dt^2 j - |v| = sqrt(v_x^2 + v_y^2)

Projectile motion — decomposition and key results

Assume constant downward acceleration g.

Decompose initial speed u: - u_x = u cosθ (horizontal; no horizontal acceleration if air resistance ignored) - u_y = u sinθ (vertical; vertical acceleration = −g)

Important derived results: - Time of flight: T = 2 u sinθ / g - Maximum height: H = (u^2 sin^2θ) / (2 g) - Horizontal range: R = (u^2 sin 2θ) / g — maximum at θ = 45° (max R = u^2 / g) - Complementary angles θ and (90° − θ) give the same range

Equation of trajectory (y as function of x): - y = x tanθ − (g x^2) / (2 u^2 cos^2θ) - Alternative using range R: y = x tanθ (1 − x / R)

Strategy to solve projectile problems: 1. Decompose u into u_x and u_y. 2. Write x(t) and y(t): x = u_x t ; y = u_y t − ½ g t^2. 3. Apply boundary conditions (e.g., at top v_y = 0; at impact y = initial y) to obtain T, H, R or solve for unknowns.

Worked examples typically include numeric computations for T, R, H, finding u from a trajectory, and complementary angle cases.

Circular motion (kinematics)

Uniform circular motion (UCM): - Speed |v| is constant, but velocity direction changes → centripetal acceleration exists. - Centripetal acceleration a_c is directed toward the center and is perpendicular to v: - a_c = v^2 / r = ω^2 r - Centripetal force: F_c = m a_c = m v^2 / r

Non‑uniform circular motion: - Speed changes → tangential acceleration a_t ≠ 0, where a_t = r α (α = angular acceleration). - Total acceleration = vector sum of centripetal (radial) and tangential components (perpendicular).

Linear/angular relations: - Arc length: s = r θ - Linear velocity: v = r ω - Tangential acceleration: a_t = r α - Centripetal acceleration (angular): a_c = ω^2 r

Direction: use right‑hand thumb rule for angular velocity vector.

A geometric triangle Δv/Δt derivation for a_c is explained in the lecture.

Relative motion in two dimensions

Definition: velocity of A relative to B: v_A/B = v_A − v_B.

Common problem types: - Rain and umbrella: - v_rain relative to man = v_rain − v_man. - Tilt umbrella opposite to the relative rain velocity vector; if rain is vertically downward and man moves horizontally, tanθ = v_man / v_rain. - Boat and river: - v_boat/ground = v_boat/river + v_river/ground. - Shortest crossing time: head straight across (perpendicular component used). - To reach a point directly opposite: choose heading so the river drift is canceled by horizontal component of boat velocity (solve using components). - Drift distance = v_river × time.

General approach: draw vectors, resolve into components, equate required components, and use v_rel = v_obj − v_ref.

Practical tips / problem‑solving checklist

Always draw a clear diagram with axes and vectors; mark components and angles.
Represent vectors by components (i, j, k) for algebraic solutions.
Use triangle/parallelogram law visually for additions/subtractions.
For projectiles, split motion into x (constant velocity) and y (constant acceleration −g); use the kinematic equations:
- v = u + at
- s = ut + ½ a t^2
- v^2 − u^2 = 2 a s
For circular motion, note whether it is uniform (only centripetal) or non‑uniform (centripetal + tangential) and convert between angular and linear variables as needed.
For relative motion, compute v_rel = v_object − v_reference and resolve components; find directions with trig.

Formulas / quick reference

|v| = sqrt(v_x^2 + v_y^2)
Unit vector: û = v / |v|
Resultant of two vectors: R = sqrt(a^2 + b^2 + 2ab cosθ)
Direction of resultant: tanα = (b sinθ) / (a + b cosθ)

Projectile: - u_x = u cosθ ; u_y = u sinθ - Time of flight: T = 2 u sinθ / g - Max height: H = u^2 sin^2θ / (2 g) - Range: R = u^2 sin 2θ / g ; max at θ = 45° - Trajectory: y = x tanθ − [g x^2 / (2 u^2 cos^2θ)] or y = x tanθ (1 − x / R)

Circular: - s = r θ ; v = r ω ; a_t = r α - Centripetal acceleration: a_c = v^2 / r = ω^2 r - Centripetal force: F_c = m v^2 / r

Examples & exam context

The instructor demonstrates many exam‑style problems (school exams, NEET/JEE), showing how to apply methods quickly and reliably.
Examples include numeric projectile problems, vector resultant and angle problems, centripetal acceleration examples, and rain/umbrella and boat/river calculations.
Emphasis on diagrams and vector decomposition to avoid errors under time pressure.

Teaching style and highlights

Strong emphasis on visual diagrams and step‑by‑step vector decomposition.
Major results are proved (resultant formula, trajectory, centripetal acceleration) and shortcuts/identities are provided for quick answers.
Repeated encouragement to focus on method rather than memorizing isolated facts.

Speakers / sources

Main instructor: Prashant Bhaiya (Prashant Kirad)
Referenced sources and examples: NCERT textbook, NEET and JEE contexts, Neeraj Chopra (range example), Maxwell’s right‑hand rule, and illustrative examples (e.g., “Chintu Lal”).

If you want, I can: - Condense this into a one‑page printable cheat sheet (formulas + step lists + recommended problem steps). - Produce a short checklist for solving projectile, circular, or relative‑motion problems.