Friends, I still encounter a lot of people who think that Climate Change is not actually happening and consequently they see policies that seek to reduce the impacts of Climate Change as an unjustified imposition. Indeed many people feel extremely indignant and are outraged by policies that can be broadly described as “Net Zero”.
I have no doubt that people with these beliefs are well-intentioned – most people are. But from my point of view, this absolutist denial of reality can make it hard to find a point at which we can begin to engage in a conversation.
I have found that in the face of such an impasse, it can be helpful to re-focus attention onto the early history of humanity’s study of the Earth’s temperature. Considering only work carried out between 1800 and 1900 takes some of the political heat out of the discussion.
Previously on this channel…
I have written previously about several of the pioneering discoveries in the nineteenth Century that laid the foundation for our understanding of Earth’s Climate. Most notable are:
- Arrhenius’s 1896 paper describing his calculation of the warming effect of increasing the concentration of CO2 in Earth’s atmosphere (link).
- Langley’s work in the 1880’s to measure the temperature of the Moon. This involved a breathtaking experimental advance – the invention of the bolometer – that allowed him to measure infrared spectra and hence calculate the absorption of infrared light by the atmosphere (link).
- Tyndall’s truly astonishing discovery in the 1850’s of the absorption of infrared light by vapours and molecular gases (link).
These advances involved a combination of improvements in experimental techniques – notability the ability to measure infrared light – and progress in our understanding of the factors affecting the temperature of the Earth.
Today I would like to revisit the work of an even earlier pioneer: John-Baptiste Joseph Fourier
Fourier: 1827
Fourier (1768 – 1830) was a genius of the first order, and his contribution to our understanding the temperature of the Earth is one of his lesser known claims to fame, possibly because he got it (sort of) wrong!
At the start of his Magnum Opus: the Analytical Theory of Heat (1822) he suggests that he hopes to do for heat what Newton did for mechanics. You can read an English Translation from 1878 here. He writes:
His writings on the temperature of the Earth are based on applying the mathematical principles established in his analytical theory – a theory that has not been replaced in the 200 years since he established it!
He began by addressing the grand problem:

In his analysis, (2004 English translation) Fourier writes that there are three processes occurring simultaneously. In the extract below I have reformatted Fourier’s text with bullet points (Liste à puces).

Let’s look at each of these three processes in turn.
The first process: “The Earth receives the rays of the Sun, which penetrate its mass and are converted there into dark heat” is exactly in line with our modern conception. Fourier uses the phrase dark heat to refer to what we would call infrared light.
He understood that when there is a balance between incoming luminous heat from the Sun and the outgoing dark heat from the Earth, then the Earth’s temperature will be stable.

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The second process: “the Earth also possesses heat of its own which it retains from its origin, and which dissipates continually at the surface” is also exactly in line with our modern conception. Now we know that the interior heat of the Earth is partly primordial, and partly from radioactive decay of minerals within the Earth (Link).

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Fourier notes that the second process can be completely neglected compared with the first. He explains that we can estimate the rate of upwelling heat by measurements of the rise of temperature as we descend below the Earth (about 30 °C/km link).
In modern terms we would say that since the thermal conductivity of rock is about 3 W/m K then the upwelling heat flow is only 0.09 watts for each square metre of surface. In contrast, solar energy reaching the Earth’s surface (averaged over a year and all latitudes ) amounts to around 240 watts for each square metre of surface i.e. thousands of times larger than the rate of upwelling heat.
Fourier did not frame his explanation as I have above, because he lacked access to basic thermophysical data. Instead he said:

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Fourier considered that his analytical theory of heat could be applied in any situation, but the determination of the properties of materials, such as the thermal conductivity of rock or the transparency of the atmosphere was not his job! He considered that such investigations and discoveries were the work of Natural Philosophers.
The third process that Fourier describes is “this planet receives rays of light and heat from the countless stars among which the solar system is located… the influence of the stars, is equivalent to the presence of an immense region closed in all parts, whose constant temperature is little inferior to that which we observe in polar lands.”

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In other words, Fourier reasoned that since the poles receive very little sunlight, and the rate of upwelling heat from the Earth was so small, then their temperature would be established by the temperature of the space just above the poles. Fourier reckoned this was around the temperature at which mercury freezes. This assumes that the atmosphere has no “insulating” properties – and this assumption is quite wrong.
The temperature of space is quite a difficult a concept, but if it means anything at all, then the answer is dramatically colder than -40 °C, more like – 270 °C or just 2.7 °C above absolute zero (an idea with which Fourier was probably not cognisant).
So Fourier scores 2 out of 3, which is not exactly genius level. But his genius emerges from the that fact he knew his ideas were not quite right and he also knew why! He knew it was do with the atmosphere.
The role of the atmosphere
Fourier wrote:

In modern terms we might call Fourier a theoretical physicist and he is pleading for experimental physicists to measure some phenomena against which he could test his theory. We might paraphrase his words, “…if only a Natural Philosopher would discover the properties of the atmosphere, then my analytical theory would be able to calculate the impact of those discoveries…“. And then he praises the work of de Saussure – a brilliant Natural Philosopher (aka experimental physicist) with achievements in many fields. The achievement to which he is referring here is the invention of the heliothermometer – an apparatus to measure the intensity of the Sun’s radiation.
The apparatus consisted of a wooden box covered with several highly transparent glass panes. The bottom of the box was insulated with blackened cork so as to absorb as much sunlight as possible and de Saussure reasoned that the temperature reached would be a measure of the intensity of the Sun’s radiation.

Click on image for a larger version. Left. A modern day re-creation of de Saussure’s Heliothermometer (link). Right: illustration of de Saussure’s experiment in the Alps.
de Saussure made measurements of the intensity of sunlight at different altitudes in the Alps and concluded that in a clear sky, sunlight travelling downwards through the atmosphere was relatively unimpeded.
Fourier would have understood this. But he suspected that the same would not be true of infrared light travelling in the opposite direction. Early experiments of which Fourier might possibly have been aware, had concluded that some substances transparent to visible light were opaque to “dark heat” – most notably water and glass. He wrote:

These sentences confirm that Fourier understood that there had to be some way in which the “transparent body” (the atmosphere) impeded the passage of dark heat (infrared light) from the Earth’s surface to “exterior space”. But as he says clearly – what that mechanism is could not “yet be exactly defined”.
Fourier was exactly correct: there was a missing part of the puzzle. Fourier described the atmosphere as a “transparent body” but he could not have known that as regards infrared light – dark heat – the atmosphere is far from transparent. In fact – like water and glass – it is practically opaque to infrared light.
It would take another 30 years or so until Tyndall found that the atmosphere absorbs infrared radiation. And then to his jaw-dropping astonishment, discovered that the absorption was not due the 99% of the molecules that constitute the bulk of the atmosphere, but due to the trace gases: water vapour and carbon dioxide.
Summary
Friends, I love Fourier’s article. His basic understanding of the mechanism by which the Earth’s temperature is maintained was exactly correct and clearly stated. It is striking to me how he clearly understood the fundamental role of “dark heat” – infrared light – in cooling the Earth.
It would take the invention of a new type of thermal detector – the thermopile – before experiments on the transmission of dark heat through the atmosphere would reveal the astonishing role of trace gases in regulating the temperature of the surface of the Earth.