Rebuilding the Periodic Debate — Philip Stewart

Rebuilding the Periodic Debate — Philip Stewart

Author: David Bradley

In June 2011, we wrote a feature entitled Periodic Debate that discussed the ongoing evolution, if not revolution, surrounding the periodic table of the chemical elements. It remains the most popular Research Highlight article on and continues to attract comments on the issues raised. In particular, from those who disagree with the standpoint that there could ever be a definitive two-dimensional table and that it is anything more than a tool or mnemonic to help chemists organize their understanding of the world around us.

I interviewed two of the people driving the debate, Philip Stewart and Eric Scerri. In this report, we learn of Stewart’s early life and what has drawn him to the Periodic Table.

60 Years of Interest

Philip Stewart is enjoying his sixth year of fake retirement after thirty years of lecturing in economics to biology students and in human ecology to students in human sciences at Oxford University, UK. This was the unexpected outcome of his having taken degrees in Arabic and in forestry and working for seven years in the Algerian Forest Service.

Through his teaching of both ecology and economics, he came to see them as two parts of a single form of knowledge, and is currently trying to finish a book to explain his ideas. Stewart weighed in on the Periodic Debate article published by ChemistryViews because of an interest instilled in him 60 years ago.

“I conceived a passionate interest in the periodic table when I saw it represented as a huge, colorful spiral in the Science Exhibition of the Festival of Britain, 1951, when I was twelve years old,” he told us. “I had just read Fred Hoyle’s wonderful little book The Nature of the Universe, and I was struck by the resemblance between Longman’s mural and the Andromeda Galaxy.”

Alternative Periodic Table

Stewart was thus very disappointed when he started school chemistry the following year to discover that the periodic table is no galactic spiral but the standard tabular form with which chemists have become familiar over the decades. “I had come to think of the series of elements as continuous,” he says. “The breaks imposed by the tabular form seemed to destroy that insight, especially with the lanthanides taken right out of the sequence.” As a result, Stewart gave up school chemistry two years later, although he never lost his interest in the subject itself.

Stewart was instrumental in getting Longman’s spiral image republished three times in important publications, not least, but most recently in Oliver Sacks’ Uncle Tungsten. This success in disseminating what he considered to be an inspirational form of an infamous icon, gave him the idea of trying to improve it still further. He produced his ‘Chemical Galaxy’ and used colors to indicate the secondary relationships of Mendeleev’s A and B groups as had Longman. He also followed von Antropoff, John Clark and others, in alluding to ‘neutronium’ as element zero.

“I am particularly attached to this latter idea,” Stewart explains, “as I think it helps to lift chemistry above the preoccupation with terrestrial matter; after all, if most of the substance of neutron stars is neutronium, it is probably the third most abundant element in the universe.” Stewart adds that he thinks the esthetics of the periodic table are as important as its functionality. “I tried to make my representation beautiful as well as truthful,” he adds.

There might be other spiral or helical forms of the periodic table yet to be discovered that would offer enlightening, alternative representations of the periodicity in the sequence of elements. He suggests that designers should take greater inspiration from the chemical works of Charles Janet who produced a remarkable range of images.

Oxford-based Stewart has maintained his keen interest in Arab culture and history, in forests, and in ecology and economics, but is currently collecting material for a book on the ten poets who visited or lived on Boars Hill, Oxford, UK, where he lives.



Philip Stewart, Oxford University, UK

Emeritus Professor Philip Stewart was born in London, UK, in 1939. He studied Arabic at Oxford University, UK, taking a second degree in foresty a few years later at the same university. From 1967–1974, he worked as a research officer and lecturer in Forestry and Land Use in Algeria. He became a Lecturer at Oxford University in 1975, teaching Land Use Economics and Human Ecology. He held this position until his retirement in 2006.

Stewart’s on-going interests include the integration of economics into ecology, Islamic culture and history, chemistry, English poetry since 1800, and bicycles.

Selected Publications



See also:




  1. Philip Stewart

    So what do people think? Should the periodic system of the elements be represented in a way that is beautiful as well as scientifically truthful? The relationship between truth and beauty has been debated since the time of Plato. Can the beauty of a graph be a guide to the truth it represents?

  2. Philip Stewart

    I recently came across this, in the Physics Archive Blog: “White dwarf stars are glowing embers, the remains of small stars that have run out of fuel to burn Most white dwarfs are hot lumps of charcoal, gradually radiating their heat into space. But a few are made of helium and it is these that we look at today. Because they generate no heat of their own, white dwarfs will eventually become so cold that they should stop emitting significant amounts of heat and light. But this cooling process takes ages, far longer even than the age of the universe, so no so-called black dwarfs are yet thought to exist. The precise rate at which white dwarfs cool depends on their internal structure. That’s fairly well understood for plain vanilla white dwarfs. But the helium flavour holds some surprises. The conventional view is that helium under high pressure forms a plasma of nuclei in a sea of electrons. When the pressure increases, the nuclei become ordered forming a crystal. The properties of this helium crystal determine how quickly the star cools. Recently, however, astrophysicists have pointed that the helium can also form a Bose-Einstein condensate. The question that Paulo Bedaque at the University of Maryland in College Park and a few pals investigate is how the presence of such a condensate might affect the properties of the star. It turns out that helium condensates have an extraordinary rich behaviour in which various kinds of quasiparticles can form. These quasiparticles are essentially quantised excitations in the condensate and have been well studied for ordinary condensates. Because these quasiparticles transport energy through and out of a condensate, they reduce its specific heat. What Bedaque and co have found is an entirely new quasiparticle that emerges in helium white dwarfs because of the extra constraints on the behaviour of the condensate at the centre of such a dense object. This quasiparticle, they say, reduces the specific heat of the white dwarf core by two orders of magnitude compared to a crystalline core. The consequences aren’t difficult to fathom. The lower specific heat means that helium white dwarfs ought to cool down significantly faster than previously thought. In fact, Bedaque and co suggest this more rapid cooling ought to be detectable. As it turns out, there is a known anomaly in the temperatures of helium white dwarfs. A couple of years ago, astronomers found a group of helium white dwarfs in a globular cluster a few thousand light years from here. Plot the temperature and magnitude of white dwarfs and astronomers usually find that the sequence of stars becomes cooler and less bright until they are no longer visible to whatever telescope they are using. But with these helium white dwarfs, astronomers saw something else: the sequence ended well above the magnitude limit of the observations (which were made with Hubble). For some reason, the dimmest, coolest, oldest stars aren’t where they are supposed to be Nobody knows why but the new quasiparticle and the cooling it causes, raises a possibility. Perhaps helium white dwarfs go through some kind of internal transition as they get older that causes them to suddenly cool much faster than expected. That’s why the oldest coolest stars don’t follow the usual pattern of cooling. For the moment, that’s just a guess. Bedaque and co say that a great deal more modelling is necessary to fully understand how all this might work out. More data on real helium white dwarfs would help too.”


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