Archive for the Art Category

After Piero

Posted in Art, Education, Politics, The Universe and Stuff with tags , , , on October 31, 2010 by telescoper

I don’t often blog about things inspired from TV programmes. I don’t watch that many, and those I do see are rarely inspirational. However, last night, I caught the last of the series Renaissance Revolution, presented by Matthew Collings. It was on the subject of a major obsession of mine, the art of Piero della Francesca, and I thought it was wonderful. I regret having missed the previous programmes in the series, but I’m sure I’ll get a chance to see them sometime.

Collings focused on one particular painting by Piero, The Baptism of Christ, which hangs in the National Gallery in London, and which is illustrated below:

The political and religious backround to this painting are almost as fascinating as its composition, based on the offset superposition of a circle (representing heaven) and a square (representing the Earth). The use of perspective was very new around 1450 when this painting was finished, but that’s not the only geometrical aspect to note. There’s a striking use of symmetry (e.g. in the angles of John the Baptist’s arm and leg), and the central vertical axis defined by the dove, John’s hand and Christ’s hands.

Given the mathematical rigour of his compositional techniques, it should come as no surprise to learn that in his lifetime Piero was just as famous as a mathematician as he was as an artist. In other words he was the archetypal renaissance man. Unfortunately, most of his art doesn’t survive; the vast majority of his works were frescoes in various churches, few of which have withstood the test of time. Regrettably, little also is known about Piero the man, except that he lived into his 80s.

A while ago I mentioned another work by Piero which is the origin of my obsession with his paintings. The Flagellation of Christ is a work that has burrowed so far into my psyche that I quite often dream that I’m in the strange building depicted therein:

In fact I also use this painting in talks about science – I did so in my talk on Wednesday, in fact. The reason I use it in that context is that it is a bit like the standard model of cosmology. On one level it makes sense: the flat Euclidean geometry mapped out by the precise linear perspective allows us to understand the properties of the space extremely well, including the scale (the vanishing point indicates a front-to-back distance of about 250 ft). This is what our standard cosmology says too:- the universe also has a flat geometry. On the other hand, the more you think about the contents, the more confusing the picture gets. The main subject matter of the painting is to the left, in the background, playing an apparently minor part in the whole thing. Who are the characters surrounding the Christ figure? And who are the three figures in the foreground, dominating the whole composition, but seemingly indifferent to what is going on behind? Do they represent dark energy? Do the other characters represent the dark matter?

That’s not meant to be taken seriously, of course, and nobody actually knows what is really going on in this painting. It’s undoubtedly beautiful, but also an enigma, and that combination is what makes it a great work of art. It’s not easy to understand. It makes you wonder.That’s what science is like too. We have our theories, we have data, but there always remains a great deal we don’t understand. And sometimes the more we think about it, the more confused we get. Just as it is with that painting.

As Mark Collings put it brilliantly in the programme last night

When you’re looking at the picture, analysis isn’t exactly what is going on. You’re seeing and you’re getting pleasure from seeing. Partly the picture is telling you how pleasure is constructed, how it’s created, and partly you’re just lost in it. So when you’re lost in the light of Piero, you’re experiencing when you’ve forgotten how to experience. And you’re suddenly curious when you’ve forgotten how to be curious. And what you’re experiencing and being curious about is .. the world.

It doesn’t matter whether you’re a scientist or an artist (or a poet or a philosopher or a historian or whatever). The need to be curious about the world – or some aspect of it – is surely what it’s all about. During the Renaissance it wasn’t unusual for great minds to embrace science, mathematics and art – just think of Leonardo da Vinci. However, over the centuries we’ve become increasingly specialised and compartmentalised and more focused on making money than on making ideas. We’re losing what above all else is what makes us human, our curiosity.

Our society increasingly sees education simply as a means to develop skilled workers, smart enough to do technically complicated jobs, but not clever enough to ask too many questions about the materialistic treadmill they will spend their life upon. The UK government’s plan to withdraw funding for arts and humanities departments in universities is just another step along this path.

It shouldn’t be like this. Universities should be about learning for learning’s sake; not about teaching facts or skills, but about teaching people to ask questions and figure out their own answers. In other words, they should be about curiosity.


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Astronomy Photographer of the Year

Posted in Art, The Universe and Stuff with tags , , , on September 10, 2010 by telescoper

Amidst the doom and gloom of spending cuts and Ministerial incompetence we’re sometimes liable to forget what it’s all about. Last night provided us with a reminder, in the form of the Astronomy Photographer of the Year competition held at the National Maritime Museum (site of the Royal Observatory at Greenwich). There’s a varied selection of gorgeous entries on today’s Guardian, but this stunning image by Tom Lowe was the overall winner. Congratulations to him!


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The Sketch Process

Posted in Art, Education, The Universe and Stuff with tags , , , , , , , , , on August 25, 2010 by telescoper

It’s pouring with rain so, rather than set off home and get drenched, I thought I’d spend a few minutes on the blog and hope that the deluge dies down before I leave. Knowing my luck it will probably get worse.

Anyway, I thought I’d put together a short item on the theme of sketching. This is quite a strange subject for me to pick because drawing is something I’m completely useless at, but I hope you’ll bear with me and hopefully it will make some sense in the end.

What  spurred me on to think about it was the exhibit I’ve been involved with for the forthcoming Architecture Biennale in Venice as part of a project called Beyond Entropy organized by the Architectural Association School of Architecture. Unfortunately, although I’d originally planned to attend I can’t be there for the opening Symposium, but I hope it turns out to be as successful event as it promises to be!

Anyway, in the course of this project I came across this image of the Moon as drawn by Galileo

This led to an interesting discussion about the role of drawings like this in science. Of course  the use of sketches for the scientific representation of images has been superseded by photographic techniques, initially using film and more recently by digital techniques. The advantage of these methods is that they are quicker and also more “objective”. However, there are still many amateur astronomers who make drawings of the Moon as well as objects such as Jupiter and Saturn (which Galileo also drew). Moreover there are other fields in which experienced practioners continue to use pencil drawings in preference to photographic techniques. Archaeology provides many good examples, e.g.

The reason sketching still has a role in such fields is not that it can compete with photography for accuracy or objectivity but that there’s something about the process of sketching that engages the sketcher’s brain in a  way that’s very different from taking a photograph. The connection between eye, brain and hand seems to involve a cognitive element that is extremely useful in interpreting notes at a later date. In fact it’s probably their very subjectivity that makes them useful.  A thicker stroke of the pencil, or deliberately enhanced shading, or leaving out seemingly irrelevant detail, can help pick out  features that seem to the observer to be of particular significance. Months later when you’re trying to write up what you saw from your notes, those deliberate interventions against objectivity will take you back to what you  saw with your mind, not just with your eyes.

It doesn’t even matter whether or not you can draw well. The point isn’t so much to explain to other people what you’ve seen, but to record your own interaction with the object you’ve sketched in a way that allows you to preserve something more than a surface recollection.

You might think this is an unscientific thing to do, but I don’t think it is. The scientific process involves an interplay between objective reality and theoretical interpretation and drawing can be a useful part of this discourse. It’s as if the pencil allows the observer to interact with what is observed, forming a closer bond and probably a deeper level of understanding patterns and textures. I’m not saying it replaces a purely passive recording method like photography, but it can definitely help it.

I have not a shred of psychological evidence to back this up, but I’d also assert that sketching is very good for the learning process too.  Nowadays we tend to give out handouts of diagrams involved in physics, whether they relate to the design of apparatus or the geometrical configuration of a physical system. There’s a reason for doing this – they take a long time to draw and there’s a likelihood students will make mistakes copying them down. However, I’ve always  found that the only way to really take in what a diagram is saying is to try to draw it again myself. Even if the level of draftsmanship is worse, the level of understanding is undoubtedly better.Merely looking at someone else’s representation of something won’t give your brain as a good a feeling for what it is trying to say  as you would get if you tried to draw it yourself.

Perhaps what happens is that simply looking at a diagram only involves the connection between eye and brain. Drawing a copy requires also the connection between brain and hand. Maybe  this additional connection brings in additional levels of brain functionality. Sketching iinvolves your brain in an interaction that is different from merely looking.

The problem with excessive use of handouts – and this applies not only to figures  but also to lecture notes – is that they turn teaching into a very passive process. Taking notes in your own hand, and supplementing them with your own sketches – however scribbly and incomprehensible they may appear to other people – is  a much more active way to learn than collecting a stack of printed notes and meticulously accurate diagrams. And if it was good enough for Galileo, it should good enough for most of us!

Now it’s stopped raining so I’m off home!


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Crater 308

Posted in Art, The Universe and Stuff with tags , , , , , on August 1, 2010 by telescoper

I haven’t got time to post much today – WordPress was down earlier when I had a bit of time and now I’m going to watch the highlights of England’s Test victory against Pakistan in the cricket today, which they achieved by bowling out their opponents for only 80 runs in the second innings.

Nevertheless, as a quick filler, I thought it would be nice to show this wonderful image of the crater Daedalus, formerly known as Crater 308, which is located on the far side of the Moon. Not the dark side, by the way, the far side of the Moon gets just as much sunlight as the near side!
This is one of the images I’ve been working on as part of the project Beyond Entropy for a forthcoming exhibit at the Venice Biennale of Architecture which opens at the end of this month. I won’t say too much about the exhibit I’m involved with, except that it explores the way higher-dimensional information can be recorded in surfaces of lower dimension, like a kind of architectural holographic principle. I was particularly struck by the way the pattern of cratering on the Moon yields information about its formation history, which is why I went looking for dramatic examples. This – taken during the Apollo 11 mission- is my favourite image of all those I’ve looked at. I love the complexy topography, its textural contrasts and the way the shadows play across it.

Daedalus is an impact crater that formed about 3.75 to 3.2 bn years ago. It’s about 93km across. The crater looks relatively fresh; showing sharp-ish-looking rims all around with sequences of wonderfully-preserved terraces down onto a pock-marked, flat floor consisting of numerous craterlets and a central peak divided up into two to three well-defined hills. You can also see the effect of more recent impacts in and around it.

Talking of impact, I wonder if I can get this project into our REF submission?

“The Greatest Picture of the War”

Posted in Art with tags , , , , on July 11, 2010 by telescoper

This remarkable photograph was taken at 8.32am on 6th June 1944 on “Queen Red” beach, a sector in the centre-left of  Sword Area, during the early stages of the D-Day invasion. The precise location is near La Brèche, Hermanville-sur-Mer, Normandy. The shutter clicked just as the beach came under heavy artillery and mortar fire from powerful German divisions inland.

I came across a discussion of this image in today’s Observer and decided to post it here, simply because it’s such a great  composition. As the article describes, it consists of “a series of tableaux that look like quotations from religious art”.  The piece goes on

In the foreground and on the right are sappers of 84 Field Company Royal Engineers. Behind them, heavily laden medical orderlies of 8 Field Ambulance Royal Army Medical Corps (some of whom are treating wounded men) prepare to move off the beach. In the background, men of the 1st Battalion, the Suffolk Regiment and No 4 Army Commando swarm ashore from landing craft.

The sapper in the bottom left, looking directly into the camera, looks terrified, and his expression makes it seem like he’s trying to escape from the photograph; through his eyes we get a glimpse of the shocking reality of armed conflict, which is far from the romantic way it’s portrayed in the movies. His colleague, turning away from the lens, seems to be calling to the men behind, but the image of his head and upper body links with the more distant figures forming a dramatic arc that pulls you into the centre of the picture before veering off to the right. Each element of this  image tells its own story, but apart from one person in the foreground, all the faces are all hidden from view. I’m sure these anonymous figures were all just as frightened as the man in the foreground, but their individual identities are lost as they blend into graphic depiction of the monumental scale of the invasion. It’s a truly wonderful work of art, and a brilliant piece of storytelling, at the same level as an Old Master, but this is made all the more remarkable by the fact that the photographer was risking his life to take this picture.

This photograph, which was taken by Sergeant Jim Mapham of the Army Film and Photography Unit, was described by the US Press as “the greatest picture of the war”.

Jim Mapham was one of seven cameramen of the AFPU who went in on D-Day: Sgt Ian Grant, Sgt Christie, Sgt Norman Clague (killed), Sgt Desmond O’Neill (wounded), Sgt Billie Greenhalgh (wounded) and Sgt George Laws. Their work forms an extraordinary record of the invasion and is still widely used by the media – but rarely credited.

Robert Capa, the famous Hungarian photographer, was also on the beaches that morning, pinned down in the waves by enemy fire. But while he clambered on to a landing craft to get his pictures back to London, Sgt Mapham moved inland with the invasion force…

Jim Mapham survived the D-Day campaign and entered Germany with the army to document the fall of the Third Reich and the horrors of the Belsen concentration camp. He died in 1968. Until today I’d never heard of him. His name should be much more widely celebrated. I understand that the complete set of photographs he took on D-Day can be found in the Imperial War Museum‘s photographic archive.

As a final comment let me add that, contrary to popular myth, the landings at the Sword beaches were by no means a pushover. It’s true that the American forces, especially at Omaha beach, suffered heavier casualties on the actual landings – primarily because they failed to get their tanks and heavy artillery pieces ashore. However, the British troops at Sword were the only ones at any of the five landing areas to encounter strong German Panzer divisions on D-Day. The main assault force at Sword beach was the British 3rd Infantry Division and its primary objective on the day of the invasion was to capture the city of Caen. As it turned out, the fighting was so heavy that they didn’t manage to take Caen until almost a month after D-Day.

European Echoes

Posted in Art, Jazz with tags , , , on July 8, 2010 by telescoper

This is  something I found recently and couldn’t resist sharing. This track from Ornette Coleman has only been on Youtube a month or so and I just found it last night, but I’ve got it on a vinyl LP I bought about 30 years ago. I think the music is completely wonderful on its own, but the idea of accompanying it with examples of the art of Joan Miro was a brilliant one!

European Echoes was recorded live at the Golden Circle club in Stockholm  in 1965, and is part of a famous album that was proclaimed “Record of the Year” the following summer in Downbeat magazine. By the mid-60s Ornette Coleman had already established his reputation as leading light of avant-garde saxophonists and, in his own way, was as great an influence on jazz as Charlie Parker, Sonny Rollins and John Coltrane had been earlier.

The track features a trio of Coleman on alto sax, David Izenzon on bass, and Charles Moffit on bass. It starts in a deceptively simple manner, with Ornette’s little two-note statements over a fast waltzy 3/4 foundation provided by Izenzon and Moffitt. It then eases into  a passage marked by freer improvisations by Ornette, the meter changing at the same time to 4/4. Ornette plays for more than half the track, after which Izenzon and Moffitt take over for all but the final minute, at which point Izenzon drops out and Moffitt plays an intricate percussion solo.

Although most people I know recognize the virtuosity of modern jazz musicians they don’t really like the music very much. I fell in love with this track as soon as I heard it, partly because it begins simply enough for a beginning saxophonist to play along with, but also because it’s highly original without being  at all self-indulgent. In fact, at one level, everything Ornette Coleman  does on this track is quite simple; he plays the saxophone here like he’d just invented the instrument.  In fact, at least in his early years, he didn’t have much of a technique at all in the conventional sense but nevertheless managed to produce amazingly fresh sounds. This a view echoed by the great Charles Mingus in quote I got from another blog about Ornette Coleman

Now aside from the fact that I doubt he can even play a C scale in whole notes—tied whole notes, a couple of bars apiece—in tune, the fact remains that his notes and lines are so fresh. So when [the jazz dj] Symphony Sid played his record, it made everything else he was playing, even my own record that he played, sound terrible.

I did learn to enjoy and admire Ornette Coleman’s more “difficult” music later on, but this was the track that convinced me that Ornette Coleman was a genius.  I hope to get the time over the summer to write a few more posts in appreciation of my favourite jazz artists, but for the time being I’ll just let this piece speak for itself…

All in a day’s work

Posted in Art, Biographical, Education, Science Politics, The Universe and Stuff with tags , , , , , on June 30, 2010 by telescoper

I got back from yesterday’s trip to a very muggy London with a raging sore throat and a brain as sluggish as an England defender on an action replay. Come to think of it, I must be as sick as a parrot. I’m sweating like a pig too, although I don’t know whether that’s a symptom of anything nasty or just because it’s still so warm and humid. Anyway, in view of my likely incoherence I thought I’d keep it brief (again) and just mention a few salient points from the last day or two.

I went to London as part of my duties as External Examiner for the MSc Course in Astrophysics at Queen Mary, University of London. Of course all the proceedings are confidential so I’m not going to comment on anything in detail, except that I spent a bit of time going through the exam scripts before the Examiners’ Meeting in a room that did a very passable impersonation of a heat bath. When I was later joined by the rest of the Exam Board the temperature soared still further. Fortunately the business went relatively smoothly so nobody got too hot under the collar and after concluding the formal business, a few of us cooled off with a beer or two in the Senior Common Room.The students spend the next couple of months writing their dissertations now that the written exams are over, so we have to reconvene in October to determine the final results. I hope it’s a bit cooler by then.

I couldn’t stay long at Queen Mary, however, as I had a working dinner to get to. Regular readers of this blog (both of them) may remember that I’m involved in project called Beyond Entropy which is organized by the Architectural Association School of Architecture. I’ve been working on this occasionally over the months that have passed since I first blogged about it, but deadlines are now looming and we need to accelerate our activity. Last night I met with the ever-enthusiastic Stefano Rabolli Pansera at the house of Eyal Weizman by Victoria Park in the East End, handily close to Queen Mary’s Mile End campus. Assisted by food and wine we managed to crystallise our ideas into something much more tangible than we had managed to do before on our theme of Gravitational Energy. The School has offered us expert practical assistance in making prototypes and  I’m now much more optimistic about our exhibit coming together, not to mention excited at the prospect of seeing it on display at the Venice Architecture Biennale. I won’t say what we’re planning just yet, though. I’d rather wait until it’s done before unveiling it.

Incidentally, here’s a link to a  lecture by Eyal Weizman where he gives some interesting perspectives on architectural history.

Finally, and nothing to do with my trip to the Big Smoke, I noticed today on the Research Fortnight Blog that the Higher Education Funding Council for Wales (HEFCW) is planning to reduce the number of universities in Wales “significantly” from its current level of 12. This is an interesting development and one that I’ve actually argued for here. Quoting Leighton Andrews, Welsh Assembly Minister responsible for higher education, the piece says

“This target does not mean fewer students,” he said in a statement. “But it is likely to mean fewer vice chancellors. We will have significantly fewer HE institutions in Wales but they will be larger and stronger.”

How these reductions will be achieved remains to be seen, but it seems obvious that quite a few  feathers will be ruffled among the management’s plumage in some institutions and it looks like some vice chancellors will be totally plucked!

When Energy Becomes Form

Posted in Art, The Universe and Stuff with tags , , , , , , on February 28, 2010 by telescoper

I’m back in Cardiff, exhausted but, at the same time, rather exhilirated by the past few days in Geneva. Before I crash out I thought I’d update the post I filed a couple of days ago.

On Friday we visited CERN, the highlight of which visit was, for me, seeing the facility where they test the superconducting magnets used in the Large Hadron Collider. We also saw the surface buildings of the ATLAS experiment, but since the LHC was getting ready to rumble again after its winter break we weren’t allowed to see the thing itself, 100 metres below ground. Coincidentally, I learned today that the LHC is now back making collisions once more. Obviously, the practical tips I passed on while I was there did the trick. One likes to help where one can.

The rest of Friday, back in downtown Geneva, was bizarre to say the least. We had the obligatory Swiss dinner of fondue, which is basically a big bowl of melted cheese into which you dip bits of bread repeatedly while hoping that at some point they’re going to bring some proper food. They don’t. To make matters worse we were serenaded by Swiss folk music:  cowbells, alphorns, yodelling – the works. One of the musicians was the spitting image of Dr Evil from the Austin Powers movies but at least there was no sign of Mini-me. I was traumatised by the thought that the world might be brought to a premature end, not by the LHC creating black holes but by excessive yodelling.

After that, as midnight approached, all 24 of us – 8 scientists, 8 artists and 8 architects – gave very short presentations about our work to the others in the hotel lobby area.  I couldn’t do justice to the range of ideas and forms presented there in a short blog like this so I’ll just say it was totally fascinating to listen to these people, see examples of their work, and have the chance to ask questions.

Saturday was the most intense and also the most interesting day. We were housed in a beautiful 19th Century house in the old part of Geneva that used to be the French ambassador’s residence the whole day. Split into various groups we thought, discussed, sketched, scribbled and generally brainstormed our way towards ideas for something to exhibit on our allocated theme. We got together at the end so each group could exchange their ideas with the others. It seemed every group had great fun and there seemed to be some great concepts floating around.

The artist I’m collaborating with is Carlos Garaicoa, who was born in Cuba and who has exhibited his work all over the world. He now shares his time between Havana and Madrid. He showed us examples of his work encompassing a huge range of materials and technologies: video, photography, sculpture – you name it. One of the themes he has been interested in is the idea of documentary matter, meaning objects of various kinds that bear testimony to events or forces acting on them.  Eyal Weizman is the architect Carlos and I will be working with.  He’s a research architect who has, amongst other things, recently completed a long project looking at the construction of the wall that the Israeli government has built in the west bank

And then there was me, like a fish out of water. I had looked at the title of the programme, Beyond Entropy: How Energy Becomes Form and decided that it might be interesting to get across the central idea in general relativity, i.e. that gravitational forces can be described in terms of the curvature of space. In my presentation I took this to an extreme and tried to explain how the large-scale structure of the Universe is shaped by small ripples in space in the early Universe that evolve under the action of gravity to produce the structures we see on scales as large as 100 million light years. It seemed to be a good example of gravitational energy becoming form. I summed it up with a quote from John Archibald Wheeler:

Matter tells space how to curve. Space tells matter how to move

Taking cue from these perspectives we had a wide-ranging conversation that took the idea of gravity as an effect of space, and explored this in more general contexts and from different angles. Space is often understood through its boundaries or through the surfaces constraining it and these edges take on a form that represents a sort of diagram of the forces that have acted on it. On a human scale we thought about walls and how the path they follow is shaped not only by topographical constraints but also by socioeconomic considerations. Walls and buildings generally suffer decay or damage too, including catastrophics events like explosions or earthquakes.

We also talked about the relationship between surfaces and the spaces they enclose or divide. The path of a wall such as the west bank barrier is extremely complicated because of the interplay between such factors. It curves in and out seemingly at random, but its shape makes it a document that contains information about the forces that have shaped it. It is a document in itself, not just because it happens to have things written on it in some places!

This thread of discussion got us interested in the possibility of using material objects to reconstruct the history of the processes that formed them: the Moon’s surface offers an example wherein the sequence of impacts can be inferred from the pattern of overlying and underlying craters. This led on to discussions about the relationship between surfaces and volumes generally, taking in holography as a specific example where  two-dimensional object contains three-dimensional volumes.

This all took us quite a long way from the initial riff, but I’m glad of that. My main worry about getting involved in this was that we might end up producing something that was merely didactic, just a fancy metaphorical treatment of basic physics. I wanted to avoid that because I think it would be very boring. I think I shouldn’t have worried that we might head in such a dull direction.

Some of the other groups managed to work up concrete ideas for prototypes to be exhibited. We didn’t really get that far. We were much keener to explore as many concepts as possible before settling on one. For myself, I was just really enjoying the discussion! There are no real constraints on what we can make – within reason of course. Sculptures, plans, buildings, installations, videos, photographs, and even books are all possibilities. It’s quite scary having such a blank canvas. We discussed a number of ways we might develop our discussion into material that can be exhibited but they all need a lot of work to develop, so we’ll carry on our collaboration remotely. I’m quite keen to bring some sort of holographic element into it, and promised to investigate the possibility of making some prototypes.

For the meantime, however,  it’s back to reality for me. A lecture to prepare and give, problem sets to get ready and an exercise class to run, an examination paper to finish writing, and a whole afternoon at the School’s research committee. I wonder if what I’ve been doing over the weekend will count as having “impact”?

Beyond Entropy

Posted in Art, The Universe and Stuff with tags , , , , , on February 26, 2010 by telescoper

It’s a cold and rainy morning here in Geneva, but I’m really looking forward to the next few days here. I arrived yesterday evening after a flight that was longer than it should have been. It seems the French air traffic controllers went on some sort of strike so my flight from Heathrow wasn’t allowed to cross French air space. For a flight between London and Geneva that is a bit of a problem. In the end we flew west over Belgium and then down into Switzerland from the North, the whole thing taking about an hour longer than expected. Still, when I did get to where I was going I found the hotel nice and comfortable and, better still, had a very enjoyable dinner at a swish Italian restaurant. It was nice to leave the chaos of French airspace behind.

I’m here as part of an unusual research project called (ironically, in the light of the aforementioned travel problems) Beyond Entropy. Organized by the Architectural Association School of Architecture, this experiment will bring together a group of artists, architects and scientists to investigate the notion of Energy. The way this is being done is by setting up a series of groups (one artist, one architect and one scientist) to look at each of a number of different forms of energy: potential, electric, thermal, mechanical, and so on; my own focus is gravitational energy. Each group will work together over the following few days to generate ideas a collaboration intended to create a work of some sort that gives form to the specific concept of energy they’re looking at. The subtitle of the project is “When Energy becomes Form”.

After we go back home, we’ll continue to work over the following months to produce prototypes of whatever emerges from the collaboration. The results will be exhibited at the Venice Architecture Biennale and the Architectural Association in August 2010. It is hoped that next year these prototypes will be developed into full-scale installations for the Venice Art Biennale in 2011.

I have no idea at this stage how the collaboration will work out or what is going to come out at the other end. The canvas is completely blank. I don’t really know the artist (Carlos Garaicoa) or the architect (Eyal Weizman) that I’ll be working with either. That makes it strangely exciting. At any rate it’s certainly different from the sort of scientific workshop I usually attend.

Anyway, to kick things off we’re going to be spending most of today at CERN, where I’ll be heading by bus just about as soon as I’ve finished this blog post. Later on today I’ll be giving a short presentation about how gravitational energy relates to my own research in the hope that this will stimulate a few ideas for my collaborators. Arts-science collaborations like this have been tried before and they have a chequered history, but we’ll just have to see how it goes. It feels more like research than most research workshops I’ve been to, in fact, because I really haven’t a clue what is going to happen!

P.S. Fellow blogger Andrew Jaffe is here too, but I think I might have beaten him in the competitive blogging stakes.

(Guest Post) What is Colour?

Posted in Art, The Universe and Stuff with tags , , , , , on February 7, 2010 by telescoper

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.