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Jetzt kostenlos anmeldenA physical quantity is something that one can measure. When we talk about quantities, we either describe them as a scalar quantity or a vector quantity.

A **scalar quantity **is one that only has magnitude. For example, speed is a scalar quantity as it only describes how quickly something is moving, not the direction in which it moves.

A **vector quantity **has both magnitude and direction. An example is velocity, as here we must give the speed an object is moving at and in which direction (eg 20kph due north).

Now we know what a vector quantity is, how does that relate to maths? Let's first think about how a vector would look in two dimensions. Usually, in two dimensions, we describe things using an x-coordinate and a y-coordinate, as this can describe any point in the xy-plane. By doing this, we describe how far we move in the x direction and then how far we move in the y direction, meaning we have satisfied our need for magnitude and direction.

We can write this vector in a couple of ways. The most common way is as a column vector. In 2D, this looks like , where x corresponds to the x coordinate and y to the y coordinate. We can also write a vector using unit vectors. In 2D, our unit vectors are represented by ** i** and

By definition, we take a positive x value in our vector to mean going to the right of the origin. Conversely, a negative x value represents going to the left of the origin. Again, by definition, we take a positive y value to mean pointing upwards from the origin, and conversely, a negative y value represents going down from the origin.

For example, if I want to show the vector on a coordinate axis, it would be as shown below.

Notice here that to show the vector , I have shown the vector first and then the vector . It is important to note that whenever we are drawing vectors, we must draw on an arrow to show the direction of the vector. Without this, we wouldn't be able to identify the vector from the vector . When we write a vector going from, eg point A to point B, we denote this vector . If it were to go the other way, it would be called . Note that the arrow shows the direction of travel.

We can extend this thinking to three dimensions. In the z-direction, the unit vector is denoted by * k* . This looks like in column vector form. A three-dimensional axis looks like this:

The thing to remember is that all three axes are perpendicular to each other. (If your tabletop were the xy plane, the z-direction would be coming directly out from the table.) If we had a vector of the form **r** = , we could express it as **r** = x ** i** + y

When looking at vectors, we can also directly describe their magnitude and direction. However, it is not obvious how to relate what we see geometrically to the ideas of magnitude and direction. We will explore this further now.

Visually, the magnitude of a vector is its length. We can show the magnitude of vector **a** as | **a** |.

Let's first think about this in two dimensions, and then we can extend these ideas to three dimensions. In 2D, we can draw a right-angled triangle around our vector, using the vector itself as the hypotenuse of the triangle. This Means we can use Pythagoras' Theorem to find the formula for a vector in 2D: .

A sketch of the vector and the triangle are shown below.

We now need to extend this idea to three dimensions. As before, we need to add the z term to the 2D formula, and so the formula in three dimensions is

Find the magnitude of the vector

Using the formula for magnitude, we get

Find the magnitude of the vector .

Using the formula for magnitude, we get

We measure the direction of a vector with respect to another point. In two dimensions, this is usually the x-axis, but we always need to specify. Let's draw a diagram to explain this better.

We give directions in terms of , so this means that in two dimensions, the direction of any vectorwith respect to the x-axis is given as. If we wanted to measure the angle with respect to the y-axis, this would be given as . Notationally, we take anything above the x-axis as a positive value of theta, and anything below the axis will give a negative value of theta.

We can extend this to any axis in three dimensions. Suppose we have a vector , and we want to find the angle with each axis. The formulas are given as follows:

x-axis:

y-axis:

z-axis:

Find the direction of **a ** = 3 ** i** - 2

First, let's work out | **a** | : . Then by the formula, the angle with the x-axis is given by , which gives .

Some calculations require you to add and subtract vectors.

How do we add two vector quantities together? Let's first think of this geometrically. To add two vectors together, we would draw our first vector as usual, starting from the origin. We would then draw the second vector starting at the end of our first vector. We would then draw a line from the origin to the end of the second vector to get the result of adding the two vectors. This new vector is called the **r****esultant vector** . This process is shown below.

Now we know how to do this geometrically. What is the process algebraically? It turns out that we can add two vectors simply by adding the corresponding components. This means that the formula for adding two vectors is given by in two dimensions. The process is exactly the same in three dimensions.

Add the vectors and .

Using the formula, we get

Add the vectors and

We can add components to get

This is very similar both geometrically and algebraically. Geometrically, when we take away a vector, we reverse its direction and then follow the same process. Algebraically, we take away components, so for two vectors, we get

. Again, the process is exactly the same in three dimensions.

Calculate

Using the given formula, we get

Calculate

Subtraction elementwise gives us

When we talk about multiplying a vector by a scalar, it looks like this: . Geometrically, we can see this as the vector joined to itself over and over a times. This means that for any non-zero a,is parallel to. Algebraically, this means that. Again, we can follow the process for three dimensions.

Calculate

Using the formula, we get this as

Suppose we are given two points in vector form and , and we wish to find the direct distance between these points. We could find a vector connecting these two points by taking one vector away from the other. We have the distance between the points as a vector, so we now need to find the length of the vector. This is given by the magnitude of this vector.

Find the distance between and .

First we need to find the vector connecting and . We do this by taking away one vector from the other . We now need to find the magnitude of this vector. This is given by - which is our answer.

You might be asked about geometric Proof with vectors. This type of question will typically look like a shape annotated with vector lengths. It will ask us to show something - the length of a certain side as a combination of the given lengths, proving two sides are parallel or perpendicular, or proving midpoints. These are best shown through examples.

P is a point on AB such that AP: PB = 1: 3

Show that is

To find we can break this down to .

, and we can break down as .

This means that .

Thus, \[ \vec{OP} = \vec{OA} + \vec{AP} = 3a + \frac{1}{4}(2b - 3a) = \frac{9}{4}a + \frac{1}{2}b = \frac{1}{4}(9a + 2b) \]

C is a point on AO such that AC: CO = 3: 1

M and N are the midpoints of BC and BO respectively

Let us denoteby **a** and by **b.**

Show that MN is parallel to AO.

, so we need to show MN is k **a** for any constant k.

, by breaking it down.

.This means we can write , which satisfies what we needed to show. QED

Now we've seen the mathematical interpretation of vectors, how do we apply these to real life? We've already discussed velocity being a vector quantity. When we describe velocity, we give the magnitude (commonly known as speed in this context) and the direction of travel. Position, velocity and acceleration are all vector quantities related to each other (velocity is the rate of change of position, and acceleration is the rate of change of velocity).

Forces are also a vector quantity, as the direction and magnitude of the force matter. This means that quantities such as thrust, weight and momentum are also vector quantities.

We can apply our knowledge of vectors to other types of questions, too. Examples would include finding the position vector of a missing vertex of a shape or translating a shape by a vector. Let's look at how to calculate these.

Translate the rectangle given by (0,0), (4,7), (4,0), (0,7) by the vector .

Visually, this looks like moving the shape one unit in the positive x direction and four Units in the positive y direction. To find the coordinates of the translated rectangle, we would need to add the vector to each position vector of a corner, which would give us (1, 4), (5, 11), (5, 4 ), (1, 11).

Note: We switch between coordinates and position vectors freely here, as they represent the same thing for our purposes.

A parallelogram has given vertices . Find the missing vertex.

The best place to start here is by plotting points. This gives us

For the completed shape to be a parallelogram, we need the y coordinate to be 4. Then we can find the x coordinate by finding the difference of x between (1, 1) and (8, 1) and adding it to the x value of the top point (shown in black). This gives us 7, meaning that the x coordinate is 10, giving the final point as .

,*i*,**j**are the unit vectors in the x, y and z directions, respectively.**k**A vector has direction and magnitude.

The magnitude of a vector is given by the square root of the sum of the components of the vector squared.

Vector addition, subtraction and scalar multiplication occur elementwise.

To find the magnitude of any vector, calculate the square root of the sum of the squared components.

To find out the magnitude of a vector x, divide the components of the vector by its magnitude.

A vector is a quantity in which we can express both direction and magnitude.

What is the difference between a vector and scalar?

A vector has direction and magnitude, whereas a scalar only has magnitude.

Find the missing vertex of the parallelogram given by (7, 1), (3, 1), (2, 0), (123)

(6, 0)

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