Reflection, Refraction, and Diffraction

The history of physics from ancient times to the modern day, focusing on light and matter. Light appeared to be made of atom-like particles since light reflects from a mirror like a ball bouncing off of a surface. In the 1600s, however, Italian natural philosopher Francesco Grimaldi showed that light can bend around corners, like a wave.

Last updated on 5th June 2017 by Dr Helen Klus

1. Reflection

Ancient Greek mathematician Euclid described the law of reflection in about 300 BCE. This states that light travels in straight lines and reflects from a smooth surface at the same angle at which it hit it.

Diagram of reflection.

The angle of incidence (i) equals the angle of reflection (r). Image credit: Helen Klus/CC-NC-SA.

Light is reflected in the same way that a ball would bounce off of a frictionless surface, and so Euclid claimed that light travels in rays that are discrete, like atoms, not continuous, like waves.

This may mean that some of the objects in our visual field will always remain unilluminated, and therefore undetected. Unlike Ancient Greek philosopher Aristotle, Euclid thought that light is emitted in rays from the eye[1].

2. Refraction

Roman astronomer Ptolemy first tried to experimentally derive the law of refraction in the 2nd century CE[2].

Refraction explains how a ray of light changes direction when it travels between different mediums. This is either because it slows down or because it speeds up.

Refraction occurs when light hits the surface of water or travels through the atmosphere, and it's atmospheric refraction that causes the stars to 'twinkle'.

Ptolemy measured the angle that a beam of light hits a boundary, the angle of incidence, and the angle at which it leaves, the angle of refraction, through different mediums.

He discovered that the angle of incidence is proportional to the angle of refraction, but could never derive the full equation. Like Euclid, Ptolemy thought that light is emitted in rays from the eye[3].

Iraqi mathematician Ibn Sahl discovered the full law of refraction in 984. Sahl showed that the angle of incidence is related to the angle of refraction using the law of sines[4].

Ptolemy's law of refraction:
Angle of incidence (i) ∝ Angle of refraction (r),

Ibn Sahl's law of refraction:
Diagram showing that light is refracted when it changes medium. This is because it speeds up or slows down.

Refraction between air and water. Image credit: Helen Klus/CC-NC-SA.

Here V is the velocity of light in each medium, and n is the refractive index of each medium. n=c/V, where c is the speed of light in a vacuum, which is very close to its speed in air.

Sahl couldn't use this method to measure the actual speed of light, however, because he could only determine the ratios.

Dutch mathematician Willebrord Snellius rediscovered the sine law of refraction in 1621. Snellius' theory was not published in his lifetime and, in 1637, French natural philosopher Rene Descartes rediscovered the law again, independently[5].

2.1 The sine function

The sine function shows how the angle inside a triangle changes as the lengths of its sides change.

The sine of angle A equals the ratio of two lengths, the length opposite the angle, and the longest length, the hypotenuse.

Sine(angle) =
Opposite length/Hypotenuse
In the triangle below,
Sine(A) =
Length a/Length c
Diagram of a right-angled triangle. The largest side is labelled ‘c'. The shortest ‘b', and the other side is labelled ‘a'. The angle opposite side ‘a' is labelled ‘A', the angle opposite side ‘b' is labelled ‘B', and the angle opposite side ‘c' is labelled ‘C'. From the perspective of angle ‘A', length 'a' is the opposite length, length ‘c' is the hypotenuse, and length ‘b' is the adjacent length.

Image credit: Helen Klus/Public domain.

The sine of 90° is 1 because the opposite length will also be the longest, the hypotenuse. In the triangle above, Sine(C) would equal Length c/Length c, which equals 1.

Ancient Greek astronomer Hipparchus created the first documented table of sine functions before 125 BCE[6].

Hipparchus' work was referenced by Ptolemy over 250 years later, and so it's not known why he did not derive the sine law of refraction himself[7a]. Some argue that his measurements were not exact enough, and others claim that his theory of perception led him astray[8].

Plot of a sine wave.

Sine wave. Image credit: Helen Klus/Public domain.

The sine wave could not be represented graphically until after the invention of the Cartesian coordinate system by Descartes and French mathematician Pierre de Fermat, in 1637[9].

2.2 Ibn al-Haytham

Iraqi mathematician Ibn al-Haytham (also known as Alhazen) was the first person to correctly describe how perception occurs in about 1021, when he proved that light enters, but is not emitted by, the eye[10].

Al-Haytham stated that light consists of tiny particles of energy that travel in straight lines, and emanate from the Sun at a large but finite velocity. Vision occurs when the Sun's rays are reflected from objects and into our eyes.

Al-Haytham experimented with the laws of reflection and refraction using different shaped mirrors and lenses, and accurately described how the eye functions as an optical instrument. He likened it to a camera obscura, a pinhole camera, and so suggested that images must also be inverted in the eye. This led him to suggest that vision occurs in the brain, rather than the eyes and that it is, therefore, subjective[11].

Science began to progress again in Europe after the Renaissance of the 12th century. This was mainly due to increased contact with the Islamic world[12]. English philosopher Roger Bacon, one of the earliest European advocates of experimental science, reviewed Al-Haytham's The Book of Optics in 1267, and it was translated into Latin shortly after[13].

2.3 Rainbows

German philosopher Theodoric of Freiberg (also known as Dietrich of Freiberg), explained how rainbows form in about 1307. He did this by experimenting with spherical flasks, which he filled with water in order to represent raindrops. Theodoric showed that the light of the Sun is refracted, and then internally reflected, inside each drop[7b].

In order for you to see sunlight that has passed through a raindrop, there needs to be an angle of about 40°-42° between you, the raindrop, and the Sun. The set of all the raindrops that can be seen at this angle at once forms a cone pointing towards the Sun. Coloured light is not visible from any other angle, and so when you move, the rainbow moves with you. This is why you will never be able to reach the end of a rainbow.

In the case of a double rainbow, secondary bows are caused by double reflection inside the raindrop. This causes the colours to be reversed, and produces visible light at about 52°-54°.

Diagram showing how rainbows are created by reflection and refraction inside of raindrops.

Image credit: Mirar abajo/Peo/CC-SA.

3. Diffraction

Italian natural philosopher Francesco Grimaldi discovered and coined the term 'diffraction' in 1660[14]. Grimaldi showed that a single beam of light spreads out, creating an interference pattern, if it's shone through very small slits. Water and sound waves act the same way, and so this was an important finding for those that advocated a wave theory of light.

Diagram of diffraction.

Waves spread out when they move through a slit. Image credit: modified by Helen Klus, original image by John Wetzel, an author at

Before this, people had argued that the sharp boundaries created by shadows meant that light could not bend around corners in the same way that water or sound waves can. Grimaldi's findings were published in 1665, two years after his death[15]. Diffraction is now understood in terms of the superposition principle.

4. References

  1. Lindberg, D. C., 1981, 'Theories of Vision from Al-kindi to Kepler', University of Chicago Press.

  2. Lindberg, D. C., 2010, 'The Beginnings of Western Science: The European Scientific Tradition in Philosophical, Religious, and Institutional Context, Prehistory to A.D. 1450', University of Chicago Press.

  3. Smith, A. M., 1987, 'Descartes's Theory of Light and Refraction: A Discourse on Method', American Philosophical Society.

  4. Wolf, K. B. and Krotzsch, G., 1995, 'Geometry and dynamics in refracting systems', European Journal of Physics, 16, pp.14-20.

  5. Sabra, A. I., 1981, 'Theories of Light: From Descartes to Newton', CUP Archive.

  6. Hosch, W. L., 2010, 'The Britannica Guide to Algebra and Trigonometry', The Rosen Publishing Group.

  7. (a, b) Glick, T. F., Livesey, S., Wallis, F., 2014, 'Medieval Science, Technology, and Medicine: An Encyclopedia', Routledge.

  8. Smith, A. M., 1982, 'Ptolemy's search for a law of refraction: A case-study in the classical methodology of 'saving the appearances' and its limitations', Archive for history of exact sciences, 26, pp.221-240.

  9. Pontrjagin, L. S., 2013, 'Learning Higher Mathematics: Part I: The Method of Coordinates Part II: Analysis of the Infinitely Small', Springer Science & Business Media.

  10. Tbakhi, A. and Amr, S. S., 2007, 'Ibn al-haytham: Father of modern optics', Annals of Saudi medicine, 27, pp.464-467.

  11. Ronchi, V. and Rosen, E., 1991, 'Optics: The Science of Vision', Courier Corporation.

  12. Cloud, R. R., 2007, 'Aristotle's journey to Europe: A synthetic history of the role played by the Islamic Empire in the transmission of Western educational philosophy sources from the fall of Rome through the medieval period', ProQuest.

  13. Grunenberg, J., 2011, 'Computational Spectroscopy: Methods, Experiments and Applications', John Wiley & Sons.

  14. Yurkin, A. V., 2013, 'New view on the diffraction discovered by Grimaldi and Gaussian beams', arXiv preprint arXiv:1302.6287.

  15. Ben-Menahem, A., 2009, 'Historical Encyclopedia of Natural and Mathematical Sciences', Springer Science & Business Media.

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The Star Garden is a science news and science education website run by Dr Helen Klus.

How we came to know the cosmos covers the history of physics focusing on space and time, light and matter, and the mind. It explains the simple discoveries we made in prehistoric times, and how we built on them, little by little, until the conclusions of modern theories seem inevitable. This is shown in a timeline of the universe.

The Star Garden covers the basics for KS3, KS4, and KS5 science revision including SATs, GCSE science, and A-level physics.

Light & Matter

Pre 20th Century theories

1. Atoms and Waves

2. Reflection, Refraction, and Diffraction

3. Newton's theory of Light

4. Measuring the Speed of Light

5. 19th Century Wave Theories

6. 19th Century Particle Theories

7. Spectral Lines and Spectroscopy

Quantum Mechanics

1. Origin of Quantum Mechanics

2. Development of Atomic theory

3. Quantum Mechanical model

4. Sommerfeld's model

5. History of Quantum Spin

6. Superconductivity

7. History of Nuclear Physics

8. De Broglie's Matter Waves

9. Heisenberg's Uncertainty Principle

10. Schrödinger's Wave Equation

11. Quantum Entanglement

12. Schrödinger's Cat

Quantum field theories

1. Field Concept in Physics

2. Electromagnetic Force

3. Strong Nuclear Force

4. Weak Nuclear Force

5. Quantum Gravity