(Guest Post) What is Colour?

As often happens on this blog, the comments following an item a few days ago went off in unexpected directions, one of which related to optics and vision. This led to my old friend, and regular commenter on this blog, Anthony Garrett (“Anton”), sending me an essay on the subject of colour perception and some very fine examples of abstract art. There thus appeared a perfect opportunity for another Guest Post, so for the rest of this item I’m handing over to Anton…

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Some years ago I was privileged to get to know, toward the end of her life, a retired teacher from Durham called Olive Chedburn. She made wonderful greeting cards which she sent to her friends, using a technique known as encaustic art. This employs heated beeswax with coloured pigment added, and a hot iron; you can read more about it at Wikipedia.

Here are the three pieces that she sent to me:

Although I am in general not a fan of abstract art, I think these are lovely. One friend said that they resembled underwater coral scenes. To me they look more like the inside of caves or chasms, perhaps with a waterfall. One of their beauties is that they definitely look like something – but you can never quite catch what.

Olive wrote a meditation on light and colour, in nature and in the Christian Bible, which I enjoyed reading very much. The main thing she left out was the science of light and colour, of which she had no knowledge. I wrote and sent her a complementary essay about this. Peter clearly likes her art and my essay, because he kindly offered to reproduce both on his blog, as you see. Olive died two years ago and her art now stands as her memorial. I hope you enjoy it as much as I did.

My essay now follows; if you want to look into the subject in greater depth then I recommend this website, which was designed to inform artists.

Colour perception is often said to be subjective. It is less clear what that means, however. The relevant scientific notion is wavelength. Light is a wave – although, remarkably, no physical medium oscillates (unlike sound waves in air, for instance); in the language of a century ago there is no ‘aether’.

Strictly speaking it would be better to talk about the frequency of light waves, because the wavelength changes with the density of the medium through which the light passes, but the frequency is unchanged. (The product of the wavelength and the frequency is the speed of light, which is a staggering 300,000 kilometers per second in empty space.) But the change in wavelength of light passing from a vacuum into air is so small that it can be ignored for present purposes. The change in wavelength (and in wave speed) is much greater when light passes into glass, or into the transparent fluids inside the eye, is much greater (25% reduction in water), since these media are much denser than air.

Light that consists of a single wavelength is called monochromatic light. Monochromatic light is not divided (further) by a prism, or by anything else that is done to it – a fact discovered by Isaac Newton in the 17th century. (Newton also reassembled the various colours back into white light.) One may superimpose differing amounts (intensities) of light of various wavelengths and look at the result. ‘White light’ is a superposition having roughly the same intensity in each colour band, as we confirm by putting it through a prism. (A prism splits light, because differing wavelengths of light entering the prism are shortened by differing amounts. The same effect creates rainbows as light passes through water droplets in the atmosphere.) In analysing colour, physics deals only the notion of how much light of each wavelength reaches the eye – the ‘spectrum’ (formally, the spectral density function) of the light. The distribution of the light across the retina – the screen at the back of the eye – also counts; a single object may appear to be coloured somewhat differently when viewed against differing backgrounds. Light has further characteristics (such as coherence, which is significant in lasers), but they make no difference to the perception of colour. A property of light known as its polarisation may change upon reflection from – or transmission through – a medium, but polarisation of light is not itself detected by the eye. (This raises the question: Are we interested in the object we are looking upon, or the light entering our eye?)

Wavelength is precisely defined, but colours – such as ‘blue’ – relate to a (fairly narrow) band of wavelengths, such that any monochromatic beam within that band will be perceived as blue. Moreover, if I add a low intensity of white light into blue, the result will still be perceived as blue. And if, in a spectrum that is generally agreed to be white, I make a small change in the amount of one particular wavelength, the result will still generally be agreed to be white. Only black is unambiguous: it is the absence of any light, of any wavelength. (Even then, it is the perceived absence, for light that is below the sensitivity threshold of the eye does not count; we shall consider perception below.)

We perceive some objects because they emit light into our eyes, such as a LED (light-emitting diode). Light of a particular frequency/wavelength/colour is emitted is when a (negatively charged) electron within an atom falls from one orbit around the positively charged atomic nucleus to another orbit around it; quantum theory tells us that only certain orbits are possible. (The difference in energy between the two orbits goes into the light that is emitted when the electron shifts orbit, and is proportional to the frequency of the light.) We see non-emitting objects because they reflect some of the light that falls on them, into our eyes. The colour that we say such an object is depends on the light that passes from the object to our eyes. This depends in turn on two factors: the combination of wavelengths falling on it; and how much of each particular wavelength the object reflects. (All light that is not reflected is absorbed, warming the object in the same way as sunbathing.) Intrinsic to the object is not its ‘colour’ but the proportion of each wavelength hitting it that it reflects. ‘Red paint’ means paint containing pigment that reflects only red light and absorbs all other colours (likewise for blue paint, etc); so that if ‘red paint’ is illuminated by a uniform mixture of light colours (i.e., white light) then only the red bounces back off it, and it looks red. But if the same object is illuminated by blue light, it absorbs the blue light so that (virtually) nothing comes off by way of reflection, and the object is perceived as black. We say that objects ‘are’ a particular colour because we generally view them in daylight or artificial white light, which contains all colours. ‘White paint’ is paint that reflects all colours and absorbs none. It looks whatever colour is shone at it – red in red light, blue in blue light, white in white light, and so on. Black paint absorbs all colours, and (uniquely) looks the same in any light.

A ‘red filter’ is something designed to let only red wavelengths through (and similarly for other filters). Something that lets all wavelengths through – the analogue of ‘white paint’ – is called transparent. (Air is virtually transparent, although it lets slightly more blue light through than other wavelengths – that is why the sky, which is lit by the many wavelengths emitted by the sun, looks blue.) Something that lets no light through – the analogue of black paint – is called a barrier. On its far side from the light source it looks black.

Also important is the texture of a surface. A perfectly reflecting material is colloquially called a white surface if it is rough enough to disperse incoming light in all directions, but if it is smooth on the scale of the incoming wavelengths then it is called a mirror. Texture is also responsible for the difference between matt and gloss paint. As for the scales involved, wavelengths of light visible to humans vary from red, which is around wavelength 0.7 micrometers (a micrometer is one thousandth of a millimetre) to blue/violet, which is about half that wavelength. In contrast, radio waves, which are of the same family and speed as light, have wavelengths of hundreds of metres.

Biological science can translate the physical specification of what lands on the retina into a specific pattern of nerve impulses passing from the eye to the visual cortex. That can in turn be correlated with the person saying “it’s green” or “it’s red” (or whatever). The names of colours are learned by tradition. As a child, each of us shared with an adult the experience of perceiving light of a particular wavelength; the adult named the colour and we learned the name. If children were not taught the names of colours then a consensus would emerge among them of what to call the colours, based on the similarity of their experiences. This consensus arises in turn from the common features of their perceptive systems (eye plus visual cortex).

Every colour to which humans give a name corresponds to a characteristic shape of the spectrum of wavelengths entering the eye. Lodged in the human retina are different types of colour receptor cells, known as cones. Each type of cone contains a different light-sensitive pigment, which absorbs and reacts most strongly to light of a particular wavelength. If you fire monochromatic light at a particular cone cell and then gradually decrease the wavelength (starting from red), the cell will transmit an increasingly strong signal to the brain until its own wavelength of peak sensitivity is reached; after that the signal will fall away on the other side the peak. Humans have three working types of cone cell, having distinct wavelengths of peak sensitivity. (The three sensitivity curves overlap to some extent.) This is why we can reasonably accurately simulate all colours that humans perceive by mixing just three colours, known as the primary colours.

People who are said to be colour-blind may have only two types of working cone, rather than three. They perceive the world differently, although they learn this only by observing that their reactions to certain wavelengths of light differ from the reactions of the majority. A man who was not colour-blind and whose cones of one particular type were suddenly switched off would see the world tinted, but a colour-blind man whose retinal cells had identical firing responses would say that things looked normal – because his brain would have trained itself from birth to regard this as the norm. Some species of animals have sensitivity spectra very different from the normal human one. Some animals see in black-and-white only (like humans at low light levels – see below); others have cone combinations with a less or a more uniform response than humans to light that is equally intense across the visual spectrum.

The mixing of primary colours of light to generate any colour known to human experience is a conceptually different problem from mixing paints to do the same. When you mix (‘add’) together light beams of the primary colours (Red, Green, Blue, roughly corresponding to the responses of the differing pigments in the three types of cone cells), you get white light. (Colour monitors and televisions have a multitude of ‘RGB’ dots.) These three are known as the ‘additive primary colours’. If you mix pigments of the three primary colours then the result is black paint, since each primary reflects only one colour, which the other primary pigments in the mixture suppress. Colour printers in fact mix cyan (which is blueish), yellow and magenta (pink-purple) in order to create all the colours known to man when the printer output is viewed in white light. These are the ‘subtractive’ primary colours, so named because if we subtract one of the additive primary colours from white light, leaving a mixture of the other two, we obtain the three subtractive primary colours. Whereas the mixing of light to obtain a desired colour is systematic, the mixing of pigment to do likewise is based on a library of knowledge gained by trial and error. Similarly, prediction of the colour of light that passes through consecutive glass jars of coloured translucent liquid (i.e., filters) is systematic, but the result of mixing the fluids is not.

Photography is conceptually more complicated than painting. What you see depends on further factors: the light that originally hit the photosensitive recorder; the response of the photosensitive recorder; the printing of the photograph (which may compensate for deficiencies in the response); and the light that the photograph is viewed in. Furthermore, negative film followed by printing and viewing; slide film viewing; digital photography viewed onscreen; and viewing a printout of a digital photograph each provide distinct re-creations at the eye of the light coming into the viewfinder.

Human perception of colour is actually more complex than I have stated. There are other cells in the retina called rods. These are more sensitive to light than cones but do not distinguish between colours. They come into their own at low levels of illumination; as a result, human vision under dimly lit conditions is essentially black-and-white. When the light intensity increases, beginning from darkness, the cones ‘kick in’ roughly when the rods become ‘saturated’ and send out no stronger signal as the brightness increases further. The brain also appears to take into account differences between the signals coming from the three types of cone, and differences between these and the rods.

A century after Newton, Goethe wrote on colour in an apparently opposing (and highly critical) way. Although what Newton had said was correct, hindsight makes it clear that Goethe was more concerned with the perception of colour than with the physics of light. We glimpse here two different philosophies: the ‘modern’ view espoused by the Enlightenment (no pun is intended on the name) that a world exists ‘out there’ to be explained (Newton), and the ‘post-modern’ view that our sensory impressions are all we have, and are therefore the most fundamental (Goethe). Goethe took the view that colour arises from the interplay between light and dark. Nowadays we have learned that humans perceive colours when they look at a spinning disc with a particular black-and-white pattern printed on it, for instance – presenting a challenge to theories of colour perception. Although Goethe’s explanations have been superseded, he was an acute observer of colour phenomena more complex than those analysed by Newton. There is still plenty to learn about the perception of colour.

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25 Responses to “(Guest Post) What is Colour?”

  1. Rhodri Evans Says:

    Anton – the sky does not transmit more blue light than other colours. It scatters most strongly in the blue (Rayleigh scattering) and least strongly in the red. As you probably know there is a 1/(wavelength^4) dependence for Rayleigh scattering so red light is scattered roughly 16 times less than blue light. I’m sure this is what you meant to say but I thought I’d better clear up the point. It’s of course why stars, including our Sun, get redder as they get closer to the horizon.

  2. telescoper Says:

    Rhodri,

    Since we’ve got you interested, I wonder if you can offer an opinion on the answer to the vexed question that is troubling all modern astronomers: Why is the Sun not green?

    A monochromatic source with the same wavelength as the peak wavelength of the Sun’s spectrum is most definitely green. Presumably the broadness of the spectrum of solar radiation and the way our eyes perceive it make it appear to have the orange-yellow colour we usually see.

    Interestingly, the green pigment of chlorophyll presumably means that it absorbs green light less efficiently than red or blue, so it isn’t very well optimised for solar radiation….

    Peter

  3. telescoper Says:

    Anton,

    Your comments about red-green-blue (RGB) and cyan-magenta-yellow (CMY) colour models reminded me of some work I did about 10 years ago on the representation of Fourier phase information which resulted in a little Nature paper. I might put together an item on that here sometime, now that you’ve reminded me of it.

    Peter

  4. Anton Garrett Says:

    Rhodri,
    Although I obviously accept the lambda^(-4) relation I have never understood why it is supposed to explain the blueness of the sky. Surely it is wavelength-dependent absorption rather than wavelength-dependent scattering that is responsible? (If red is scattered less then more blue light should be scattered back into space, so that your argument actually suggests the sky should be red.) Perhaps I am missing something and should consult a detailed textbook, but can you say more?
    Anton

  5. Anton Garrett Says:

    Peter: More mystifying than why the sun is not green is why the moon is not green, since it is well known to be made of green cheese – Anton

  6. Tim Harries Says:

    I don’t think an essay/discussion on colour and vision should omit Thomas Young (and yet mention Newton). He did after all work on the anatomy of the eye (at the cost of considerable personal discomfort!) and colour vision, as well as the wave nature of light.

    Anton – the scattering effect is optical depth (or air mass) dependent. You do indeed see a red sky at dawn and sunrise occassionally. A lunar eclipse is quite a nice example of the red sky – all the sunsets and sunrises simultaneous viewed in reflected light from the Moon…

  7. telescoper Says:

    That would be Thomas Young, the famous hairdresser – particularly well-known for his fringes….

  8. Anton Garrett Says:

    Tim,
    It’s not a historical essay. But I’ve now grasped the ‘blue sky’ argument and please consider the relevant sentence in my essay deleted – it’s incorrect, and the correct explanation is unrelated to the points I was making.
    Anton

  9. [...] Garrett guest-blogs at In The Dark on the topic of colour and includes some images of very pretty and imaginative art [...]

  10. “A monochromatic source with the same wavelength as the peak wavelength of the Sun’s spectrum is most definitely green. Presumably the broadness of the spectrum of solar radiation and the way our eyes perceive it make it appear to have the orange-yellow colour we usually see.”

    Yes, it’s the broad spectrum. Feynman used this as an example of bad science in a school textbook which mentioned green stars. There are no green stars (there are stars which appear to be green due to effects of contrast with nearby stars right at the limit of colour vision). The idea was to associate the peak of the spectrum with a wavelength, which is fine, but this doesn’t always translate to a perceived colour as the example of the Sun shows. Another bad example was “total temperature”. Star A has temperature X, start Y temperature Z. Add them to get the total temperature. Rubbish, of course. (The idea was to make things less abstract, but the examples were not well chosen.) (Of course, when calculating the average temperature, we have the “total temperature” as an intermediate step.)

  11. Check this out with regard to different primary-colour systems used in 3-D movies:

    http://blog.richmond.edu/physicsbunn/2010/01/20/how-3d-movies-really-work/

  12. Note that Schrödinger was an expert on colour vision before he turned to wave mechanics.

  13. “Interestingly, the green pigment of chlorophyll presumably means that it absorbs green light less efficiently than red or blue, so it isn’t very well optimised for solar radiation….”

    Nature has to use what’s available. Maybe chlorophyll is good for other reasons, despite not being an optimal absorber. Also, it was first used organisms which evolved in water, where the fraction of light of a given colour at a given depth in general differs from that above water.

  14. Originally posted in the wrong thread, to increase this blog’s comedy quotient. :-|

    Just this morning, I was reading that the DNA a) in the rods (not the cones) of b) nocturnal mammals (other classes haven’t yet been tested) has a different DNA structure, with more concentration in the cell nucleus. This leads to a better focusing of dim light, aiding these animals in their night vision. Interestingly, this seems to have been the original model, with non-nocturnal mammals dropping it (in several independent lineages), so it seems to have problems which are only outweighed by the advantages in nocturnal mammals.

  15. Originally posted in the wrong thread, to increase this blog’s comedy quotient. :-|

    Maybe chlorophyll is used because it can take advantage of quantum mechanics:

    http://blogs.discovermagazine.com/cosmicvariance/2010/02/05/quantum-photosynthesis/?utm_source=feedburner&utm_medium=feed&utm_campaign=Feed%3A+CosmicVariance+%28Cosmic+Variance%29

  16. Anton Garrett Says:

    There is the famous Green Flash phenomenon, of course, by which the last of the setting sun appears green for a few seconds. But it seems to require a flat horizon and atmospheric conditions, for it is rarely seen. Presumably it applies also to the rising sun in those conditions, but it is harder to know exactly where on the horizon to look. The phenomenon was once seen for hours from the north pole as the sun orbited the horizon at the time of the equinox. Personnel on US warships in the Pacific ocean during World War 2 became accustomed to seeing it too. But why is it seen so rarely?

  17. telescoper Says:

    I’ve been told that the Green Flash is produced when the Sun has just set below the horizon; some of its rays then reach the observer having travelled through the surface layer of the sea.

    I’ve never seen it myself, however, and I know a number of astronomers who are skeptical of the standard explanation…

  18. Anton Garrett Says:

    Peter,

    That it was visible from the North Pole where there was only snow and ice, rather than water, disproves that hypothesis. A surface wave involving the atmosphere by the interface is not a bad idea, though. A long time ago I read this copy of this book:

    http://depfacoz-newton.lib.cam.ac.uk/vwebv/search?searchArg=green+flash&searchCode=GKEY%5E*&limitTo=none&recCount=25&searchType=1

    Anton

    • telescoper Says:

      I think the reason that the Green Flash is so rarely seen is that sufficiently high quality weed is hard to come by…

  19. Tim Harries Says:

    I have always understood the green flash to be the result of differential atmospheric refraction. I’ve never seen it though, despite many cold vigils on mountaintops around the world. I expect it would be very difficult to catch on camera in any case (but very easy to photoshop in afterwards).

  20. Rhodri Evans Says:

    I too have tried in vain to see the green flash, despite seeing countless sunsets over the sea in West Wales where I grew up. I may have seen it one time whilst on an observing run on the INT at La Palma but I’m not convinced I actually saw it.

    Is Rayleigh scattering isotropic. I will need to check but I seem to remember that it is slightly forward scattering.

  21. [...] in Fourier Space As I threatened promised after Anton’s interesting essay on the perception of colour, a couple of days ago, I thought I’d write a quick item about [...]

  22. I recently started thinking about the concept of colour whilst using scanning probe microscopy where only contrast pictures are given. Plain black and white, since such structures are much smaller than the actual wavelength of light. Since optical light cannot be used to image such small structures, you do begin to wonder what ‘colours’ it would actually be.

    One thing regarding perception of colours I do find interesting are their names. Different languages have perceived the same objects as different colours. This may be due to the language used by people living in certain geographic locations e.g. mountainous regions. I have heard that such people call objects which I would perceive as blue, as grey. This could be due the thinness of air and its effect upon the sunlight.

    Another example of colour naming I’m more sure of is, in Welsh there didn’t used to be a name for green. The colours green and blue where both known as only blue. For example, the Welsh word for grass in ‘glaswellt’ which literally translates to blue-straw.

    Other example are of course general perceptions such as black tea in Welsh being ‘red tea’; ploughed soil is known as ‘red soil’. I’m sure other languages have interesting differences.

  23. telescoper Says:

    Huw,

    I heard the other day on QI (so it must be true) that the Greeks didn’t use the word “blue” for the sky like we do; they called it “bronze”.

    As another random comment, when I first worked in Italy I had a colleague who kept describing himself as “daltonico”. I didn’t understand what it meant until much later. Daltonic – from the name of the famous scientist Dalton – is also an English, though rare, meaning “colour-blind”. Dalton was colour-blind, you see. How did this word become the standard word for colour-blindess in Italy, but not in Dalton’s homeland?

    Peter

  24. Anton Garrett Says:

    Peter,

    “I heard the other day on QI (so it must be true) that the Greeks didn’t use the word “blue” for the sky like we do; they called it “bronze”.”

    By which I take it that you mean they used the same Greek word as for the [colour of the] metal alloy bronze. To see why, recall that bronze weathers quite quickly to blue-green, as shown in this picture:

    http://en.wikipedia.org/wiki/File:Assorted_bronze_castings.JPG

    Homer used to speak of the “wine-dark sea,” incidentally – not blue.

    Translation of colours across languages is not an exact science. As another example, the ‘pale’ or ‘light’ horse that is ridden by the last of the famous four horsemen of the apocalypse, in the book of Revelation which closes the New Testament (Rev 6:8), is *cloron* in the original Greek, meaning pale green – appropriate for putrefaction. From this Greek word comes chlorophyll, our name for the green pigment found in plants.

    Anton

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