Mathematics · IGCSE 0580 · §7.1–7.6

Transformations & Vectors

Two languages for moving a point: one repositions and resizes whole shapes, the other carries them by a fixed step — and a translation shows they are the same idea.

Mathematics · 0580 Extended Topic 10 of 12

Reflection

A reflection turns a shape into its mirror image across a fixed line. Distances and angles are unchanged, so the image is congruent — only its orientation is reversed.

Definition
Reflection, Mirror line
A reflection is a transformation that flips a shape across a fixed mirror line; the image is congruent and reversed. The mirror line is the line every point is reflected across — each point and its image are equidistant from it, on opposite sides.

Describing a reflection

To describe a reflection fully you need just two things: the word reflection and the equation of the mirror line. The mirror line lies exactly halfway between each point and its image, meeting the join at a right angle.

y = x A A′
FIG 7.1 Triangle A reflected in the line y = x; each vertex swaps its coordinates.

Finding the mirror line

Given a shape and its image, join a point to its image and find the perpendicular bisector of that segment — that line is the mirror. One pair of points is enough to fix it; a second pair is a useful check.

Worked example: a triangle has vertices at (1, 4), (1, 2) and (3, 2). Its image has vertices at (4, 1), (2, 1) and (2, 3). Describe the single transformation fully. Step 1: the image is the same size and shape but reversed, so the transformation is a reflection. Step 2: each point’s coordinates have swapped, (1, 4) → (4, 1) — swapping x and y is reflection in y = x. Step 3: the midpoint of (1, 4) and (4, 1) is (2.5, 2.5), which lies on y = x — confirmed.

The four reflections worth memorising: in the x-axis, (x, y) → (x, −y); in the y-axis, (x, y) → (−x, y); in y = x, (x, y) → (y, x); in y = −x, (x, y) → (−y, −x).

Examiner note
To describe a reflection, name it and give the mirror line as an equation (e.g. x = 2), never as a vague direction. No equation, no mark. Two reflections combine into a rotation or translation, covered later in this chapter.
Why this matters
Reflection is the mathematics of mirror symmetry — from optics to the balanced logos designers build around an axis.

Rotation

A rotation turns a shape about a fixed centre. Lengths and angles survive the turn, so the image is congruent — it has simply been swung to a new position.

Definition
Rotation, Centre of rotation
A rotation is a transformation that turns a shape about a fixed point through a given angle; the image is congruent. The centre of rotation is the one point that does not move — every other point stays the same distance from it.

Describing a rotation

A full description gives the centre, the angle and the direction. At exam level the angle is a multiple of 90°; for a 180° turn the direction makes no difference, so it may be omitted. If the centre is not the origin, find it as the point equidistant from each vertex and its image.

O A A′ 90°
FIG 7.2 Triangle A rotated 90° anticlockwise about the origin O onto A′.

About the origin, the three rotations worth memorising: 90° anticlockwise, (x, y) → (−y, x); 90° clockwise, (x, y) → (y, −x); 180°, (x, y) → (−x, −y).

Finding the centre

Join two points to their images and draw the perpendicular bisector of each join. The centre of rotation is where those bisectors cross — the point that keeps its distance to every vertex.

Worked example: the point P(4, 1) is rotated 90° anticlockwise about the origin. Find the coordinates of its image P′. Step 1: for a 90° anticlockwise turn about O, apply (x, y) → (−y, x). Step 2: substitute x = 4, y = 1 to get (−1, 4). Step 3: OP and OP′ are both √17 long — the distance from the centre is preserved, as it must be. P′ = (−1, 4).

Examiner note
State three things: the centre, the angle, and the direction (clockwise or anticlockwise). Tracing paper is allowed — use it to find the centre.
Why this matters
Every gear, clock hand and turbine blade is a rotation about a fixed centre — the angle is what the machine is designed around.

Enlargement

An enlargement changes a shape’s size while keeping its proportions. Angles are unchanged and every length is multiplied by the same scale factor, so object and image are similar.

Definition
Enlargement, Scale factor
An enlargement is a transformation that scales a shape from a centre by a scale factor; the image is similar, not congruent. The scale factor is the number every length is multiplied by — it also sets each image point’s distance from the centre.

Centre and scale factor

Measure from the centre of enlargement O. If a point sits at position P, its image P′ lies so that the distance OP′ is the scale factor times OP, along the same ray. The centre is the one point that stays put: OP′ = k × OP, where k > 1 makes the image larger, 0 < k < 1 makes it smaller, and k < 0 puts it on the opposite side of the centre, inverted.

O object image k = 2
FIG 7.3 Enlargement of scale factor 2 from centre O; rays through each vertex fix the image.

Finding centre and factor

The scale factor is any image length divided by the matching object length. To locate the centre, draw a ray through each object point and its image; the rays all meet at the centre.

Worked example: a triangle has a vertex at P(1, 2). It is enlarged by scale factor 3 with centre the origin. Where does P map to? Step 1: with centre the origin, multiply each coordinate by the scale factor, (x, y) → (3x, 3y). Step 2: substitute (1, 2) to get (3 × 1, 3 × 2) = (3, 6). Step 3: P′ sits three times as far from O as P, along the same ray — the shape keeps its proportions. P′ = (3, 6).

Examiner note
State the centre and the scale factor. A negative factor puts the image on the far side of the centre, inverted; a factor between 0 and 1 makes it smaller — still called an enlargement. Enlargement produces similar shapes, using the similarity ratios covered elsewhere in this course.

Translation & Combinations

A translation slides every point of a shape the same distance in the same direction. Nothing turns and nothing resizes, so the image is congruent and the same way up.

Definition
Translation, Column vector
A translation is a slide of a shape with no turn or resize, described by a column vector. A column vector is two stacked numbers: the top is movement right (or left if negative), the bottom is movement up (or down if negative).

Translation by a vector

The slide is captured by a column vector: the top number is the horizontal step, the bottom the vertical step, with left and down counting as negative. Adding the vector to each vertex gives the image — translation by (x⁄y) maps (a, b) to (a + x, b + y).

A A′ (4, 2)
FIG 7.4 Translation by the vector (4, 2): four right and two up, applied to every vertex.

Combining transformations

Apply two transformations in turn and the result can often be described as one. Two reflections in parallel mirrors give a translation; two reflections in mirrors that cross give a rotation about the crossing point. The exam asks for that single equivalent, fully described.

Worked example: a shape is reflected in the y-axis, then the image is reflected in the line x = 3. Describe the single transformation with the same effect. Step 1: the two mirror lines, x = 0 and x = 3, are parallel, so the combined effect is a translation. Step 2: the shift is twice the gap between the mirrors, 2 × 3 = 6 units, toward the second mirror (to the right). Step 3: parallel vertical mirrors give a horizontal slide, so the vertical component is zero. Translation by (6⁄0).

Examiner note
When asked for the single transformation equivalent to two others, you must give one transformation, fully described — writing "reflection then rotation" scores zero. The column vector here is exactly the vector used for vector arithmetic, covered next.

Vector Arithmetic & Magnitude

A vector carries two things at once — how far and which way. In column form, vectors add, subtract and scale one component at a time.

Definition
Vector, Scalar
A vector is a quantity with both size and direction, written as a column or as AB or bold a. A scalar is a plain number with no direction — multiplying a vector by a scalar stretches it and keeps it parallel.

Arithmetic in column form

Add or subtract vectors by combining the top numbers and the bottom numbers separately: (a⁄b) + (c⁄d) = (a+c⁄b+d). A scalar multiplies both components, giving a parallel vector: k(a⁄b) = (ka⁄kb). Geometrically, a + b joins tip-to-tail — the triangle law.

O a b a + b
FIG 7.5 The triangle law: a followed by b reaches the same point as the single vector a + b.

Magnitude of a vector

The magnitude |a| is the length of the vector, found by Pythagoras on its components: for a = (x⁄y), |a| = √(x² + y²) — always a non-negative number, not a vector.

Worked example: given a = (3⁄4) and b = (−1⁄2), find 2a − b and its magnitude. Step 1: 2a = (6⁄8). Step 2: 2a − b = (6−(−1)⁄8−2) = (7⁄6). Step 3: |2a − b| = √(7² + 6²) = √85 ≈ 9.22.

Examiner note
Keep vectors in column form until the final step — it makes sign slips visible. And |a| is a length: take the square root, and never write it equal to the vector a.
Why this matters
Displacement, velocity and force are all vectors; adding them tip-to-tail is how physics finds a resultant.

Position Vectors

Position vectors pin points to the origin, so a whole diagram can be written in terms of a few vectors. Geometric facts — parallel, collinear, a ratio along a line — then follow from algebra.

Definition
Position vector, Collinear
A position vector is the vector from the origin O to a point — point A has position vector a = OA. Points are collinear if they lie on one straight line: three points are collinear if two vectors along them are parallel and share a point.

From position vectors to displacement

If A and B have position vectors a and b, the journey from A to B is the difference: go back to O, then out to B, giving AB = b − a. Expressing every segment this way lets you combine them like ordinary vectors. The midpoint M of AB has OM = ½(a + b).

O a A b B M
FIG 7.6 In triangle OAB, M is the midpoint of AB and OM = ½(a + b).

Proving a geometric result

Two vectors are parallel when one is a scalar multiple of the other. If they are parallel and pass through a common point, the three endpoints are collinear. Always finish with the conclusion in words.

Worked example: in triangle OAB, OA = a and OB = b. M is the midpoint of AB. Express OM in terms of a and b. Step 1: AB = b − a, so from A the midpoint is half of this, AM = ½(b − a). Step 2: OM = OA + AM = a + ½(b − a). Step 3: tidy to a + ½b − ½a = ½a + ½b — the symmetric average of the two position vectors, as expected.

Examiner note
Build any vector as "finish minus start": AB = b − a. To prove a result, show one vector is a scalar multiple of another, then state in words what that means — parallel, or collinear. Parallel here means the same idea as the equal ratios used for similar shapes.

Exam advice

Common mistakes

Describing a transformation incompletely
A rotation without its centre, or an enlargement without its scale factor, loses a mark for every part left out.
Giving two transformations when one is asked for
"Describe the single transformation" means exactly one — naming a sequence scores zero.
Reading a column vector the wrong way
Top number is horizontal, bottom is vertical; left and down are negative. Swapping them sends the shape the wrong way.
Forgetting the square root in a magnitude
Writing |a| = x² + y² gives the square of the length; the root is worth the final accuracy mark.
Building a vector as start minus finish
AB = b − a, not a − b. The reversed version points the wrong way and derails a proof.

Model answer

Triangle P is mapped onto triangle Q, which is twice the size. Describe fully the single transformation that maps P onto Q.
[3 marks]
B1
Name the transformation — Q is larger and the same way up, so it is not an isometry
Enlargement
B1
State the scale factor — Q is twice the size
Scale factor = 2
B1
State the centre, found where rays through matching vertices meet
e.g. centre (1, 1)

Recall checklist

  • State the four transformations and what each preserves.
  • Describe a reflection by the mirror line’s equation.
  • Describe a rotation by centre, angle and direction.
  • Describe an enlargement by centre and scale factor.
  • Write a translation as a column vector.
  • Add, subtract and scale vectors in column form.
  • Calculate the magnitude of a vector.
  • Apply position vectors to prove points parallel or collinear.

Every Mathematics topic, in one PDF you keep

Print it, write on it, revise with no wifi and no ads. One payment — not a subscription.

Get the Mathematics PDF

Ready to test this topic? Practise with Mathematics past papers and mark schemes →