Vectors

This page defines and describes vectors.

The Main Idea

In mathematics and physics, a vector is a quantity with both a magnitude and a direction in space. The magnitude of a vector is a scalar value which can represent a variety of characteristics, depending on the situation. The magnitude of the vector (and the vector itself) has units corresponding to the characteristic it represents. The direction of a vector is simply an orientation in space giving context to the magnitude. Note that a vector does not necessarily extend from one point in real, physical space to another; unless the magnitude is in units of length, the magnitude of the vector usually represents a property that exists at a single point in real, physical space, or at no position in particular.

A Mathematical Model

Simple Examples of Vector Quantities

To understand what it means for a vector to have both a magnitude and a direction, and to understand why the magnitude and direction together are often considered a single quantity, it can be helpful to consider an example. The Velocity of an object is an example of a vector quantity. The speed of the object, often given in meters per second (m/s), is a scalar value describing how quickly the object is moving. Speed is the magnitude of the velocity vector. However, the object's movement happens in a particular spatial direction, which the speed alone does not tell us. The direction of the object's movement is also a part of the velocity vector. Together, speed and direction comprise the velocity vector and give a complete description of an object's motion at a point in time. Another example of a vector is position; the distance of a point from the origin of a coordinate system can be represented as the magnitude of a vector, and this distance together with a direction describes exactly where a point can be found.

Unit Vectors

A unit vector is a vector whose magnitude is 1 by design.

Some unit vectors are normalized regular vectors. For example, [math]\displaystyle{ \hat{r} }[/math] is the normalized version of some vector [math]\displaystyle{ \vec{r} }[/math]. Normalization is the process of setting a vector's magnitude to 1. This is done to discard information about the vector's magnitude while retaining information about its direction. To normalize a vector, the following formula can be used: [math]\displaystyle{ \hat{a} = \frac{\vec{a}}{|\vec{a}|} }[/math]

Certain letters represent specific unit vectors. For example, [math]\displaystyle{ \hat{i} }[/math], [math]\displaystyle{ \hat{j} }[/math], and [math]\displaystyle{ \hat{k} }[/math] (alternatively, [math]\displaystyle{ \hat{x} }[/math], [math]\displaystyle{ \hat{y} }[/math], and [math]\displaystyle{ \hat{z} }[/math]) are unit vectors pointing in the +x, +y, and +z directions respectively. Non-Cartesian coordinate systems often have their own unit vectors; for example, 2D polar coordinates make use of the [math]\displaystyle{ \hat{r} }[/math] and [math]\displaystyle{ \hat{\theta} }[/math] unit vectors.

Notation

A variable representing a vector is typically written as a letter with an arrow over it: [math]\displaystyle{ \vec{a} }[/math]. The arrow may one-sided to make it easier to write. Alternatively, a vector variable might simply be written as a boldface letter: a. Which letter is used depends on the context; for example, [math]\displaystyle{ \vec{v} }[/math] represents velocity.

Surrounding a vector by | symbols denotes its magnitude: [math]\displaystyle{ |\vec{b}| }[/math].

A specific component of a vector (see the section titled "forms") is denoted by a subscript: c_x. For example, q_y represents the y component of some vector [math]\displaystyle{ \vec{q} }[/math].

A unit vector is denoted by a letter with a ^ symbol (called a "hat") written over it: [math]\displaystyle{ \hat{d} }[/math] (read as "d-hat").

Visually Representing Vectors

Vectors are visually represented by arrows. The length of the arrow represents the magnitude of the vector, while the direction the arrow points in represents the direction of the vector. If a vector exists at a particular point in space, the "tail" of the arrow (the end without the V shape) should be placed at that point.

This example shows a visual representation of the velocity vector of a ball, which is moving to the right at a speed of 5m/s.

Forms

The information necessary to describe a specific vector can be presented in several forms.

Magnitude and direction form

In this form, the magnitude and the direction of the vector are explicitly stated. The statement describing direction might be a cardinal direction (ex. "north"), a direction on a graph (ex. "the +x direction"), or an angle (ex. "210[math]\displaystyle{ ^\circ }[/math] from the x axis counterclockwise"), depending on the situation. Magnitude and direction form is often used in word problems because it is easy for humans to understand.

Component form

In this form, the vector is divided into components, each representing a different coordinate direction. In 2D space, these are the x and y directions. In 3D space, these are the x, y, and z directions. Each component tells how much the vector extends in that particular direction. Often, the three components are written enclosed by angle brackets and separated by commas. For example, the vector <2,0,-3> describes a vector that extends 2 units in the +x direction, 0 units in the y direction, and 3 units in the -z direction. Most vector operations described below can only be performed if the vectors are in component form, so this form may be necessary to do math for certain problems. Furthermore, programming languages store vectors in component form.

Unit vector form

In this form, the vector is expressed as a sum of unit vectors, each corresponding to a different coordinate direction. The symbols [math]\displaystyle{ \hat{i} }[/math], [math]\displaystyle{ \hat{j} }[/math], and [math]\displaystyle{ \hat{k} }[/math] OR the symbols [math]\displaystyle{ \hat{x} }[/math], [math]\displaystyle{ \hat{y} }[/math], and [math]\displaystyle{ \hat{z} }[/math] are used to represent unit vectors in the x, y, and z directions respectively. Consider the vector <2,0,-3>. It can be expressed in unit vector form as [math]\displaystyle{ 2\hat{i} - 3\hat{k} }[/math], meaning 2 times the x direction unit vector minus 3 times the z direction unit vector (see vector operations). While often considered its own form, unit vector form is very similar to component form, as the information describing the vector is stored in the same values. All references to component form in the rest of this page also apply to unit vector form.

Note that regardless of which form is used, an n-dimensional vector requires n values to mathematically describe. For example, consider a 3-dimensional vector. Describing this vector in component form requires an x value, a y value, and a z value. Describing it in magnitude and direction form requires one value to give the magnitude of the vector and two to give the its direction (the direction of a 3D vector could be described using, say, its polar angle [math]\displaystyle{ \theta }[/math] and its azimuthal angle [math]\displaystyle{ \phi }[/math]). A 1-dimensional vector (such as the velocity of a particle whose movement is constrained to the x axis) can be described using only 1 value whose sign indicates the vector's direction.

Converting between forms

It is possible to convert vectors from one form to another using simple trigonometry.

To find the magnitude of a vector in component form, use the Pythagorean theorem: add the squares of the components and take the square root of the result. For a 2D vector, [math]\displaystyle{ |\vec{a}| = \sqrt{a_x^2 + a_y^2} }[/math].

To find the direction of a vector in component form, use inverse trigonometric functions. For a 2D vector, [math]\displaystyle{ \theta = \tan^{-1}(\frac{a_y}{a_x}) }[/math], where [math]\displaystyle{ \theta }[/math] is the angle vector [math]\displaystyle{ \vec{a} }[/math] makes with the x axis in the counterclockwise direction.

To find the components of a vector in magnitude and direction form, use trigonometric functions. For a 2D vector, [math]\displaystyle{ a_x = |\vec{a}|\cos\theta }[/math] and [math]\displaystyle{ a_y = |\vec{a}|\sin\theta }[/math], where [math]\displaystyle{ \theta }[/math] is the angle vector [math]\displaystyle{ \vec{a} }[/math] makes with the x axis in the counterclockwise direction.

Vector Operations

It is possible to perform a variety of mathematical operations on vectors, both with other vectors and with scalars. These operations appear in a variety of formulas in physics. To make the operations easier to learn, they are defined below assuming all vectors to be 3-dimensional; the more general n-dimensional definitions look more confusing. If necessary, it is easy to guess how to perform each operation with n-dimensional vectors by extrapolating from the 3-dimensional case.

Addition:

[math]\displaystyle{ \vec{a} + \vec{b} = (a_x + b_x)\hat{i} + (a_y + b_y)\hat{j} + (a_z + b_z)\hat{k} }[/math].

In other words, to add two vectors, simply add their like components to form the new components. The new vector is called the "resultant" of the other two. Visually, if the tail of one vector is placed at the tip of another, their resultant will extend from the tail of the second vector to the tip of the first:

Subtraction:

[math]\displaystyle{ \vec{a} - \vec{b} = (a_x - b_x)\hat{i} + (a_y - b_y)\hat{j} + (a_z - b_z)\hat{k} }[/math].

In other words, to subtract two vectors, simply subtract their like components to form the new components.

Multiplication by scalar:

[math]\displaystyle{ k \vec{a} = ka_x\hat{i} + ka_y\hat{j} + ka_z\hat{k} }[/math].

In other words, multiplying a vector by a scalar multiplies each of that vector's components by that scalar. Multiplying a vector by a scalar multiplies its magnitude by that scalar and does not affect its direction, unless the scalar is negative, in which case the direction of the vector is reversed.

Division by scalar:

[math]\displaystyle{ \frac{\vec{a}}{k} = \frac{a_x}{k}\hat{i} + \frac{a_y}{k}\hat{j} + \frac{a_z}{k}\hat{k} }[/math].

In other words, dividing a vector by a scalar divides each of that vector's components by that scalar. Dividing a vector by a scalar divides its magnitude by that scalar and does not affect its direction, unless the scalar is negative, in which case the direction of the vector is reversed.

Dot product (also called scalar product):

[math]\displaystyle{ \vec{a}\cdot\vec{b} = a_xb_x + a_yb_y + a_zb_z }[/math].

In other words, the dot product of two vectors is the sum of the products of their like components. Note that this is a scalar value.

It is important to note that the dot product of two vectors has a specific value: [math]\displaystyle{ \vec{a}\cdot\vec{b} = |\vec{a}||\vec{b}|\cos\theta }[/math], where [math]\displaystyle{ \theta }[/math] is the angle between the vectors.

Cross product (also called vector product):

[math]\displaystyle{ \vec{a}\times\vec{b} = (a_yb_z - a_zb_y)\hat{i} + (a_zb_x - a_xb_z)\hat{j} + (a_xb_y - a_yb_x)\hat{k} }[/math].

This is equivalent to the following matrix determinant, which may be easier to remember:

[math]\displaystyle{ \begin{vmatrix} \hat{i} & \hat{j} & \hat{k} \\ a_x & a_y & a_z \\ b_x & b_y & b_z \end{vmatrix} }[/math]

Note that this is a vector quantity. It is important to note that the magnitude of the cross product of two vectors has a specific value: [math]\displaystyle{ |\vec{a}\times\vec{b}| = |\vec{a}||\vec{b}|\sin\theta }[/math], where [math]\displaystyle{ \theta }[/math] is the angle between the vectors. The direction of the cross product of two vectors is perpendicular to the plane in which those vectors lie and is given by the Right Hand Rule. 2D vectors do not have cross products. While the other operations listed here are commutative, associative (where the associative property is defined), and distributive over addition; cross product multiplication is not associative and is anticommutative ([math]\displaystyle{ \vec{a}\times\vec{b} = -\vec{b}\times\vec{a} }[/math]), meaning that if the order of the factors is reversed, their cross product will be reversed in direction.

Transformations

A variety of transformations are defined for vectors, including multiplication by matrices and projection onto spaces. These transformations use a combination of the six basic operations above to manipulate vectors in more complex ways. These transformations lie outside of the scope of this page and this course due to their complexity and irrelevance to introductory physics.

A Computational Model

In VPython, vector objects are in component form; each one has an x, y, and z component. Recall that in VPython, using the default camera orientation, the +x axis points to the right, the +y axis points upwards, and the +z axis points out of the plane of the screen towards the viewer. The constructor for a vector object is the word "vec" or "vector," and it takes three arguments, which define its x, y and z components respectively. A line to create a vector called "velocity" might look like this:

velocity = vec(3,-1,2)

To access or modify a specific component of a vector object, its name should be followed by a period and an x, y, or z. For example, to change the x component of the above velocity vector from 3 to 5, the following line might be used:

velocity.x = 5

In VPython, vectors have many uses. The position of each object is defined as a vector; the position vector's tail lies at the origin and its head lies at the center of the object in question. Furthermore, the dimensions of a rectangular prism (a "box" object) are defined as a vector; the x component determines its width, the y component its height, and the z component its thickness.

To graphically represent a vector such as an electric field, "arrow" objects should be used. In addition to taking a position vector (which determines the position of the arrow's tail), arrow objects take an "axis" vector, which determines their size and shape. To represent a vector, simply make it the axis of an arrow object.

Examples

Simple

Vector [math]\displaystyle{ \vec{a} }[/math] is <2,4,2>. Vector [math]\displaystyle{ \vec{b} }[/math] is <-1,1,3>. What is the magnitude of the vector [math]\displaystyle{ \vec{a} - 2\vec{b} }[/math]?

Solution:

[math]\displaystyle{ \vec{a} - 2\vec{b} = \lt 2,4,2\gt - 2 * \lt -1,1,3\gt }[/math]

[math]\displaystyle{ = \lt 2,4,2\gt - \lt -2,2,6\gt }[/math]

[math]\displaystyle{ = \lt 4,2,-4\gt }[/math]

We are asked to find the magnitude of this vector, so let us use the Pythagorean theorem with its components:

[math]\displaystyle{ |\lt 4,2,-4\gt | = \sqrt{4^2 + 2^2 + (-4)^2} }[/math]

[math]\displaystyle{ = \sqrt{16 + 4 + 16} }[/math]

[math]\displaystyle{ = \sqrt{36} }[/math]

[math]\displaystyle{ = 6 }[/math]

Intermediate

An airplane is travelling in still air at 240m/s in the direction 35[math]\displaystyle{ ^\circ }[/math] south of west. A wind begins to blow; the wind has a speed of 80m/s in the direction 15[math]\displaystyle{ ^\circ }[/math] east of north. What should be the new velocity of the plane relative to the air around it to maintain its original trajectory? You may give your answer in component form (+x is east, +y is north).

Solution:

By the Galilean reference frame transformations (or a bit of geometric reasoning), the vector sum of the new velocity of the plane [math]\displaystyle{ \vec{v_{p,1}} }[/math] and the velocity of the wind [math]\displaystyle{ \vec{v_w} }[/math] should equal the original velocity of the plane [math]\displaystyle{ \vec{v_{p,0}} }[/math]:

[math]\displaystyle{ \vec{v_{p,1}} + \vec{v_w} = \vec{v_{p,0}} }[/math]

[math]\displaystyle{ \vec{v_{p,1}} = \vec{v_{p,0}} - \vec{v_w} }[/math]

Let us convert the given vectors to component form for easier subtraction. The +x and +y directions will be east and north respectively.

[math]\displaystyle{ \vec{v_{p,0}} = \lt 240\cos(215^\circ), 240\sin(215^\circ)\gt }[/math]m/s (35[math]\displaystyle{ ^\circ }[/math] south of west is 215[math]\displaystyle{ ^\circ }[/math] above the x axis)

[math]\displaystyle{ \vec{v_{p,0}} = \lt -196.6, -137.7\gt }[/math]m/s

[math]\displaystyle{ \vec{v_w} = \lt 80\cos(75^\circ), 80\sin(75^\circ)\gt }[/math]m/s (15[math]\displaystyle{ ^\circ }[/math] east of north is 75[math]\displaystyle{ ^\circ }[/math] above the x axis)

[math]\displaystyle{ \vec{v_w} = \lt 20.7, 77.3\gt }[/math]m/s

Now let us subtract:

[math]\displaystyle{ \vec{v_{p,1}} = \vec{v_{p,0}} - \vec{v_w} }[/math]

[math]\displaystyle{ \vec{v_{p,1}} = \lt -196.6, -137.7\gt - \lt 20.7, 77.3\gt }[/math]m/s

[math]\displaystyle{ \vec{v_{p,1}} = \lt -217.3, -214.9\gt }[/math]m/s

Difficult

What is the angle between the vectors <2,5,-2> and <3,-4,-1>?

Solution:

The dot product between two vectors is equal to the product of their magnitudes times the cosine of the angle between them. Let us use this property to find the angle between the given vectors.

[math]\displaystyle{ \lt 2,5,-2\gt \cdot \lt 3,-4,-1\gt = |\lt 2,5,-2\gt | * |\lt 3,-4,-1\gt | * \cos\theta }[/math]

[math]\displaystyle{ \theta = \cos^{-1}\frac{\lt 2,5,-2\gt \cdot \lt 3,-4,-1\gt }{|\lt 2,5,-2\gt | * |\lt 3,-4,-1\gt |} }[/math]

[math]\displaystyle{ \theta = \cos^{-1}\frac{2(3) + 5(-4) + (-2)(-1)}{\sqrt{2^2 + 5^2 + (-2)^2} * \sqrt{3^2 + (-4)^2 + (-1)^2}} }[/math]

[math]\displaystyle{ \theta = \cos^{-1}\frac{-12}{\sqrt{33 * 26}} }[/math]

[math]\displaystyle{ \theta = 114^\circ }[/math]

Connectedness

Vectors are used in many fields and levels of physics. Kinematics, for example, studies the relationships between the position vector and its time derivatives (velocity, acceleration). Force is also a vector quantity, as are certain system properties such as linear and angular momentum. Vector fields are commonly used in electricity and magnetism, as well as in fluid dynamics.

History

It is unknown who first developed the idea of vectors, but the oldest known reference to vectors is in the work Mechanics by Hero of Alexandria (first century AD), which described their addition. At this point, however, the idea of a vector was little more than a line segment with a specific orientation; they had a length extending from one point in physical space to another but were not used to represent anything else.

In the early 19th century, several mathematicians and physicists (including Caspar Wessel (1745-1818), Jean Robert Argand (1768-1822), Carl Friedrich Gauss (1777-1855)), and William Rowan Hamilton (1805-1865) used 2D vectors to represent complex numbers; one component would represent the real value and another would represent the imaginary value. Hamilton would also become the first to use the word "vector." August Ferdinand Möbius (1790-1868) contributed to vector math in his 1827 book The Barycentric Calculus, in which he developed the convention of labeling vectors with letters and defined the multiplication of a vector by a scalar. Hermann Grassmann (1809-1877) wrote in his 1844 book Ausdehnungslehre (German for "The Calculus of Extension") that vectors could exist in space of any number of dimensions and described much of what would become linear algebra, which makes ample use of vectors.

The modern language and conventions surrounding vectors come largely from notes created by J. Willard Gibbs (1839--1903), a professor at Yale University.

See also

External links

Mathematical Computations on Vectors: [http://ocw.mit.edu/courses/mathematics/18-02sc-multivariable-calculus-fall-2010/1.-vectors-and-matrices/part-a-vectors-determinants-and-planes/session-1-vectors/MIT18_02SC_notes_0.pdf

Computational Work with Vectors: http://vpython.org/contents/docs/vector.html

Basics of Vectors: https://www.physics.uoguelph.ca/tutorials/vectors/vectors.html

Further Reading

Vector Analysis by Josiah Willard Gibbs

Introduction to Matrices and Vectors by Jacob T. Schwartz

References

https://www.mathsisfun.com/algebra/vectors.html

http://ocw.mit.edu/courses/mathematics/18-02sc-multivariable-calculus-fall-2010/1.-vectors-and-matrices/part-a-vectors-determinants-and-planes/session-1-vectors/MIT18_02SC_notes_0.pdf

http://mathinsight.org/vector_introduction

http://www.math.mcgill.ca/labute/courses/133f03/VectorHistory.html