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18.3 Vector Representations, Operations, Magnitude, Direction & Dot Product

Key Takeaways

  • A vector in R2\mathbb{R}^2 is expressed in component form as v=⟨v1,v2⟩=v1i+v2j\mathbf{v} = \langle v_1, v_2 \rangle = v_1 \mathbf{i} + v_2 \mathbf{j}, with magnitude ∥v∥=v12+v22\|\mathbf{v}\| = \sqrt{v_1^2 + v_2^2} and direction angle θ=atan2(v2,v1)\theta = \text{atan2}(v_2, v_1).

  • The unit vector in the direction of any non-zero vector v\mathbf{v} is u=v∥v∥\mathbf{u} = \frac{\mathbf{v}}{\|\mathbf{v}\|}, which has length 1 and shares the identical direction angle.

  • Vector addition u+v=⟨u1+v1,u2+v2⟩\mathbf{u} + \mathbf{v} = \langle u_1 + v_1, u_2 + v_2 \rangle corresponds geometrically to the tip-to-tail method and the parallelogram law, while scalar multiplication scales magnitude by ∣c∣|c| and reverses direction if c<0c < 0.

  • The dot product evaluates algebraically as u⋅v=u1v1+u2v2\mathbf{u} \cdot \mathbf{v} = u_1 v_1 + u_2 v_2 and geometrically as u⋅v=∥u∥∥v∥cos⁡θ\mathbf{u} \cdot \mathbf{v} = \|\mathbf{u}\| \|\mathbf{v}\| \cos \theta; two non-zero vectors are orthogonal if and only if u⋅v=0\mathbf{u} \cdot \mathbf{v} = 0.

  • In navigation, resultant velocity is the vector sum of airspeed and wind velocity (vground=vair+vwind\mathbf{v}_{\text{ground}} = \mathbf{v}_{\text{air}} + \mathbf{v}_{\text{wind}}), with bearings measured clockwise from true North.

Last updated: September 2026

18.3 Vector Representations, Operations, Magnitude, Direction & Dot Product

Vector Fundamentals in the Euclidean Plane (R2\mathbb{R}^2)

A vector in the two-dimensional Euclidean plane is a geometric entity possessing both magnitude (length) and direction. Geometrically, a vector is depicted as a directed line segment with an initial point P(x1,y1)P(x_1, y_1) and a terminal point Q(x2,y2)Q(x_2, y_2). The vector PQ⃗\vec{PQ} is invariant under translation; placing its initial point at the origin (0,0)(0, 0) establishes its standard position as a position vector.

The vector is uniquely characterized by its component form v=⟨v1,v2⟩\mathbf{v} = \langle v_1, v_2 \rangle, where:

v1=x2−x1,v2=y2−y1v_1 = x_2 - x_1, \quad v_2 = y_2 - y_1

The standard unit basis vectors in R2\mathbb{R}^2 are defined along the coordinate axes as i=⟨1,0⟩\mathbf{i} = \langle 1, 0 \rangle and j=⟨0,1⟩\mathbf{j} = \langle 0, 1 \rangle. Any vector v=⟨v1,v2⟩\mathbf{v} = \langle v_1, v_2 \rangle can be written uniquely as a linear combination of these basis vectors:

v=v1i+v2j\mathbf{v} = v_1 \mathbf{i} + v_2 \mathbf{j}

Magnitude, Direction Angle & Normalization

The magnitude (or Euclidean norm) of vector v=⟨v1,v2⟩\mathbf{v} = \langle v_1, v_2 \rangle, denoted ∥v∥\|\mathbf{v}\|, is calculated via the Pythagorean distance formula:

∥v∥=v12+v22\|\mathbf{v}\| = \sqrt{v_1^2 + v_2^2}

The direction angle θ\theta is the counterclockwise angle measured from the positive xx-axis to the vector in standard position (0∘≤θ<360∘0^\circ \le \theta < 360^\circ or 0≤θ<2π0 \le \theta < 2\pi). The components satisfy:

v1=∥v∥cos⁡θ,v2=∥v∥sin⁡θv_1 = \|\mathbf{v}\| \cos \theta, \quad v_2 = \|\mathbf{v}\| \sin \theta

To find θ\theta, compute the reference angle α=arctan⁡∣v2v1∣\alpha = \arctan\left|\frac{v_2}{v_1}\right| for v1≠0v_1 \neq 0 and adjust for the quadrant containing (v1,v2)(v_1, v_2):

  • Quadrant I (v1>0,v2>0v_1 > 0, v_2 > 0): θ=α=arctan⁡(v2/v1)\theta = \alpha = \arctan(v_2 / v_1)
  • Quadrant II (v1<0,v2>0v_1 < 0, v_2 > 0): θ=180∘−α=180∘+arctan⁡(v2/v1)\theta = 180^\circ - \alpha = 180^\circ + \arctan(v_2 / v_1)
  • Quadrant III (v1<0,v2<0v_1 < 0, v_2 < 0): θ=180∘+α=180∘+arctan⁡(v2/v1)\theta = 180^\circ + \alpha = 180^\circ + \arctan(v_2 / v_1)
  • Quadrant IV (v1>0,v2<0v_1 > 0, v_2 < 0): θ=360∘−α=360∘+arctan⁡(v2/v1)\theta = 360^\circ - \alpha = 360^\circ + \arctan(v_2 / v_1)

A unit vector is any vector with magnitude 1. The process of dividing a non-zero vector by its magnitude to obtain a unit vector in the identical direction is normalization:

u=v∥v∥=⟨v1v12+v22,v2v12+v22⟩\mathbf{u} = \frac{\mathbf{v}}{\|\mathbf{v}\|} = \left\langle \frac{v_1}{\sqrt{v_1^2 + v_2^2}}, \frac{v_2}{\sqrt{v_1^2 + v_2^2}} \right\rangle

Vector Operations: Addition, Subtraction & Scalar Multiplication

Vector algebra in R2\mathbb{R}^2 operates componentwise:

  1. Vector Addition: For u=⟨u1,u2⟩\mathbf{u} = \langle u_1, u_2 \rangle and v=⟨v1,v2⟩\mathbf{v} = \langle v_1, v_2 \rangle: u+v=⟨u1+v1,u2+v2⟩\mathbf{u} + \mathbf{v} = \langle u_1 + v_1, u_2 + v_2 \rangle Geometrically, vector addition corresponds to the tip-to-tail method (translating the tail of v\mathbf{v} to the tip of u\mathbf{u}) and the parallelogram law (the resultant is the directed diagonal of the parallelogram formed by u\mathbf{u} and v\mathbf{v} from a common origin).
  2. Vector Subtraction: u−v=u+(−v)=⟨u1−v1,u2−v2⟩\mathbf{u} - \mathbf{v} = \mathbf{u} + (-\mathbf{v}) = \langle u_1 - v_1, u_2 - v_2 \rangle Geometrically, u−v\mathbf{u} - \mathbf{v} represents the directed segment pointing from the terminal point of v\mathbf{v} to the terminal point of u\mathbf{u}.
  3. Scalar Multiplication: For scalar c∈Rc \in \mathbb{R}: cv=⟨cv1,cv2⟩c\mathbf{v} = \langle c v_1, c v_2 \rangle The magnitude scales to ∥cv∥=∣c∣⋅∥v∥\|c\mathbf{v}\| = |c| \cdot \|\mathbf{v}\|. If c>0c > 0, direction is preserved; if c<0c < 0, direction reverses by 180∘180^\circ; if c=0c = 0, the product is the zero vector 0=⟨0,0⟩\mathbf{0} = \langle 0, 0 \rangle.

The Dot Product & Geometric Angle Determination

The dot product (or Euclidean inner product) is an algebraic operation between two vectors that returns a scalar:

u⋅v=u1v1+u2v2\mathbf{u} \cdot \mathbf{v} = u_1 v_1 + u_2 v_2

The algebraic dot product connects to geometry through the Law of Cosines:

u⋅v=∥u∥∥v∥cos⁡θ\mathbf{u} \cdot \mathbf{v} = \|\mathbf{u}\| \|\mathbf{v}\| \cos \theta

where θ\theta is the angle between u\mathbf{u} and v\mathbf{v} (0∘≤θ≤180∘0^\circ \le \theta \le 180^\circ). Solving for cos⁡θ\cos \theta yields:

cos⁡θ=u⋅v∥u∥∥v∥=u1v1+u2v2u12+u22v12+v22\cos \theta = \frac{\mathbf{u} \cdot \mathbf{v}}{\|\mathbf{u}\| \|\mathbf{v}\|} = \frac{u_1 v_1 + u_2 v_2}{\sqrt{u_1^2 + u_2^2} \sqrt{v_1^2 + v_2^2}}

The sign of the dot product categorizes the angle θ\theta:

  • u⋅v>0  ⟺  0∘≤θ<90∘\mathbf{u} \cdot \mathbf{v} > 0 \iff 0^\circ \le \theta < 90^\circ (acute angle)
  • u⋅v=0  ⟺  θ=90∘\mathbf{u} \cdot \mathbf{v} = 0 \iff \theta = 90^\circ (orthogonal / perpendicular vectors)
  • u⋅v<0  ⟺  90∘<θ≤180∘\mathbf{u} \cdot \mathbf{v} < 0 \iff 90^\circ < \theta \le 180^\circ (obtuse angle)

Thus, two non-zero vectors u\mathbf{u} and v\mathbf{v} are orthogonal if and only if u⋅v=0\mathbf{u} \cdot \mathbf{v} = 0.


Real-World Applications: Static Equilibrium & Navigation

  1. Resultant Force and Static Equilibrium: Concurrent forces acting on a body sum vectorially to form the resultant force Fnet=∑Fi\mathbf{F}_{\text{net}} = \sum \mathbf{F}_i. A system is in static equilibrium if and only if Fnet=0\mathbf{F}_{\text{net}} = \mathbf{0}. The equilibrant force required to balance a system is Fequilibrant=−Fnet\mathbf{F}_{\text{equilibrant}} = -\mathbf{F}_{\text{net}}.
  2. Aviation & Marine Navigation: Navigation defines direction using bearings measured clockwise from true North (000∘000^\circ). A bearing of ϕ\phi converts to standard Cartesian angle θ\theta via θ=90∘−ϕ\theta = 90^\circ - \phi (mod 360∘360^\circ), with components v=⟨∥v∥sin⁡ϕ,∥v∥cos⁡ϕ⟩\mathbf{v} = \langle \|\mathbf{v}\| \sin \phi, \|\mathbf{v}\| \cos \phi \rangle. The actual ground path (track and ground speed) is the resultant vector sum of the vehicle's airspeed vector and the atmospheric wind vector:
vground=vair+vwind\mathbf{v}_{\text{ground}} = \mathbf{v}_{\text{air}} + \mathbf{v}_{\text{wind}}

2D Vector Operations Summary

OperationAlgebraic FormulaGeometric MeaningScalar or Vector
Component Formv=⟨v1,v2⟩=⟨x2−x1,y2−y1⟩\mathbf{v} = \langle v_1, v_2 \rangle = \langle x_2 - x_1, y_2 - y_1 \rangleDisplacement from initial to terminal pointVector
Magnitude∥v∥=v12+v22\lVert\mathbf{v}\rVert = \sqrt{v_1^2 + v_2^2}Euclidean length of the directed segmentNon-negative Scalar
Unit Vectoru=v∥v∥\mathbf{u} = \frac{\mathbf{v}}{\lVert\mathbf{v}\rVert}Pure direction vector with magnitude 1Vector
Vector Additionu+v=⟨u1+v1,u2+v2⟩\mathbf{u} + \mathbf{v} = \langle u_1 + v_1, u_2 + v_2 \rangleParallelogram diagonal / Tip-to-tail resultantVector
Scalar Productcv=⟨cv1,cv2⟩c\mathbf{v} = \langle c v_1, c v_2 \rangleStretches length by ∣c∣\vert c\vert; reverses if c<0c < 0Vector
Dot Productu⋅v=u1v1+u2v2\mathbf{u} \cdot \mathbf{v} = u_1 v_1 + u_2 v_2∥u∥∥v∥cos⁡θ\lVert\mathbf{u}\rVert \lVert\mathbf{v}\rVert \cos \theta; zero if orthogonalScalar
Angle Betweencos⁡θ=u⋅v∥u∥∥v∥\cos \theta = \frac{\mathbf{u} \cdot \mathbf{v}}{\lVert\mathbf{u}\rVert \lVert\mathbf{v}\rVert}Smallest non-negative angle between vectorsScalar Angle

Worked Exemplar: Resultant Velocity & Course in Navigation

Problem: An airplane flies on a compass heading (bearing) of 060∘060^\circ with an airspeed of 450 mph450\text{ mph}. A crosswind blows toward bearing 045∘045^\circ (northeast) at 60 mph60\text{ mph}.

  1. Express the airspeed and wind velocity vectors in component form.
  2. Determine the airplane's resultant ground velocity vector vg\mathbf{v}_g.
  3. Calculate the aircraft's actual ground speed and ground track heading.

Step 1: Convert Navigation Bearings to Cartesian Components. For bearing ϕ\phi, components are vx=∥v∥sin⁡ϕv_x = \|\mathbf{v}\| \sin \phi and vy=∥v∥cos⁡ϕv_y = \|\mathbf{v}\| \cos \phi (or using Cartesian angle θ=90∘−ϕ\theta = 90^\circ - \phi):

  • Airspeed Vector (va\mathbf{v}_a): Bearing ϕ=60∘  ⟹  θa=90∘−60∘=30∘\phi = 60^\circ \implies \theta_a = 90^\circ - 60^\circ = 30^\circ. va=⟨450cos⁡30∘,450sin⁡30∘⟩=⟨450(32),450(12)⟩=⟨2253,225⟩≈⟨389.71,225.00⟩\mathbf{v}_a = \langle 450 \cos 30^\circ, 450 \sin 30^\circ \rangle = \left\langle 450 \left(\frac{\sqrt{3}}{2}\right), 450 \left(\frac{1}{2}\right) \right\rangle = \langle 225\sqrt{3}, 225 \rangle \approx \langle 389.71, 225.00 \rangle
  • Wind Vector (vw\mathbf{v}_w): Bearing ϕ=45∘  ⟹  θw=90∘−45∘=45∘\phi = 45^\circ \implies \theta_w = 90^\circ - 45^\circ = 45^\circ. vw=⟨60cos⁡45∘,60sin⁡45∘⟩=⟨60(22),60(22)⟩=⟨302,302⟩≈⟨42.43,42.43⟩\mathbf{v}_w = \langle 60 \cos 45^\circ, 60 \sin 45^\circ \rangle = \left\langle 60 \left(\frac{\sqrt{2}}{2}\right), 60 \left(\frac{\sqrt{2}}{2}\right) \right\rangle = \langle 30\sqrt{2}, 30\sqrt{2} \rangle \approx \langle 42.43, 42.43 \rangle

Step 2: Calculate Resultant Ground Velocity Vector (vg\mathbf{v}_g). Add components algebraically:

vg=va+vw=⟨2253+302,225+302⟩≈⟨389.71+42.43,225.00+42.43⟩=⟨432.14,267.43⟩\mathbf{v}_g = \mathbf{v}_a + \mathbf{v}_w = \langle 225\sqrt{3} + 30\sqrt{2}, 225 + 30\sqrt{2} \rangle \approx \langle 389.71 + 42.43, 225.00 + 42.43 \rangle = \langle 432.14, 267.43 \rangle

Step 3: Calculate Ground Speed & Direction. Compute the magnitude of vg\mathbf{v}_g:

∥vg∥=(432.14)2+(267.43)2=186,745.0+71,519.2=258,264.2≈508.20 mph\|\mathbf{v}_g\| = \sqrt{(432.14)^2 + (267.43)^2} = \sqrt{186,745.0 + 71,519.2} = \sqrt{258,264.2} \approx 508.20\text{ mph}

Compute the standard Cartesian direction angle θg\theta_g:

θg=arctan⁡(267.43432.14)≈arctan⁡(0.61885)≈31.75∘\theta_g = \arctan\left(\frac{267.43}{432.14}\right) \approx \arctan(0.61885) \approx 31.75^\circ

Convert back to navigational bearing ϕg\phi_g:

ϕg=90∘−31.75∘=58.25∘≈058∘\phi_g = 90^\circ - 31.75^\circ = 58.25^\circ \approx 058^\circ

The airplane travels at an actual ground speed of approximately 508.2 mph508.2\text{ mph} along a true course heading of 058.3∘058.3^\circ.

Test Your Knowledge

Find the measure of the angle theta between the vectors u = <3, -4> and v = <5, 12> in the 2D plane.

A

arccos(33 / 65) approx 59.5 deg

B

arccos(-15 / 52) approx 106.8 deg

C

arccos(0) = 90.0 deg

D

arccos(-33 / 65) approx 120.5 deg

Test Your Knowledge

For what real value of the scalar k are the vectors a = <2k - 1, 4> and b = <3, k + 5> orthogonal?

A

k = 1.7

B

k = -1.7

C

k = -2.3

D

k = -8.5

Test Your Knowledge

Which of the following represents the unit vector u that has the same direction as the vector v = <-5, 12>?

A

<-5/13, 12/13>

B

<5/13, -12/13>

C

<-5/7, 12/7>

D

<-65, 156>

Test Your Knowledge

Two forces F_1 = <40, -15> N and F_2 = <-16, 85> N act concurrently on a particle at the origin. What is the magnitude of the resultant force acting on the particle, and what equilibrant force F_3 is required to maintain static equilibrium?

A

Resultant magnitude = 74 N; Equilibrant force F_3 = <24, 70> N

B

Resultant magnitude = 102 N; Equilibrant force F_3 = <-24, -70> N

C

Resultant magnitude = 74 N; Equilibrant force F_3 = <-24, -70> N

D

Resultant magnitude = 56 N; Equilibrant force F_3 = <-24, 70> N

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