Skin colour is the most obviously visible manifestation and expression of our evolutionary history. This history is carried over the course of hundreds of thousands of generations and tens of thousands of years. What we have to understand is that each one of us—as an individual, a person, a self—has nothing to do with the colour of our skin, the colour of our skin has nothing to do with us, and we have no choice in the matter. What we must also understand is that to be optimally healthy, we have to live and eat in accordance with the colour of our skin and what information it carries about our ancestry. All of this is true for you, and it is true for everyone of every colour in the magnificent spectrum of human skin colours as it exists on the planet today. Let me explain why.
(Photo credit: Pierre David as published in this article of the Guardian)
The Sun, like every other star in the universe, formed from the gravitational collapse of a huge cloud of gas. This happened about 5 billion years ago. All the planets, like every other planet everywhere in the universe, formed from the left over debris that wasn’t needed or used in making the Sun, and that remained orbiting around it in a large, flat accretion disk consisting of 99% hydrogen and helium gas and only 1% of solid dust particles. In a blink of an eye, a million years or so, the disk was replaced by a large number of planetesimals. An additional couple hundred million years or so, and the planets of our Solar system were formed.
Beyond the snow line, the radius from the Sun past which water can only exist as ice and where the temperature is below -120 C, volatiles froze into crystals, and were formed from massive icy cores the gas giants: Jupiter (the king at 320 times the mass of the Earth), Saturn, Uranus and Neptune. Within the snow line were formed the rocky planets: Mercury, Venus, Earth and Mars. About 4.5 billion years ago the Solar system was in place. It was in place but not quite like we know it today. It was fundamentally different in several ways, especially in regards to what concerns us here, which is how the Earth was: a fast-spinning burning inferno of molten rock spewing out of volcanos everywhere and flowing all over the globe, completely devoid of water, oxygen, carbon and other volatiles species.
The Earth formed more or less simultaneously with a very close neighbour about the size of Mars. Inevitably, soon after their formation, they collided. This apocalyptic encounter tilted the Earth off its original axis and destroyed the smaller planet that, in the collision, dumped its iron core into the Earth, and expelled about a third of our planet into the atmosphere. Most of the stuff rained back down, but some of the material lumped into larger and larger lumps that eventually resulted in the moon, our moon. When it formed, the moon was a lot closer—it would have looked twice as large as it does now, and the Earth was spinning approximately five times faster than it does today—a day back then would have lasted only 5 hours. Because of the proximity between them, huge tidal forces would have deformed the liquid Earth on a continuous cycle driven by its super short 5-hour days. This would have heated the Earth tremendously by squeezing its insides from one side and then from the other, and caused massive volcanic activity all over the globe.
But this inelastic gravitational interaction, this drag of the moon on the Earth worked, as it still does, to sap rotational energy from the Earth and transfer it to the smaller and far less rotationally energetic moon. This made, and continues to make, the Earth slow down, the moon speed up and therefore drift out into a progressively larger orbit. The moon’s drag on the Earth continues to make the Earth’s spin slower and the moon’s orbit larger, but at an increasingly slower rate, now of 3.8 cm per year. This will continue until there is no more rotational energy to be transferred from the Earth to the moon, at which point we will be tidally locked in order with the moon, and not only will we always see the same side of the moon as we do today, but the moon will also always see the same side of the Earth. For what it’s worth, this will happen way after the Sun has come to the end of its life, and thus in more than 5 billion years. So, for now, this is definitely not a major issue.
Besides this important difference in the Earth’s spin rate and its relationship with the moon, there were a lot of left overs from the Sun’s formation that had clumped up in asteroids and comets whirling around in all sorts of both regular and irregular orbits that had them sweeping across the Solar system from the furthest reaches and most distant places to the inner regions near the Sun and rocky planets. The Heavy Bombardment lasted for a period of approximately 500 million years from about 4.3 to 3.8 billion years ago. During this tumultuous early history of our Solar system, a lot of these asteroids and comets flying past the Earth and the other rocky inner planets were gravitationally captured and pulled in towards the planet to crash on the surface or just swoop down into the atmosphere, leaving behind all or some of their mostly volatile constituents: water and carbon compounds. The Earth would have been regularly bombarded by massive asteroids, and the energy dumped by the impacts would have made it a hellish place covered in flowing lava, obviously without any crust, but rather only molten rock flowing everywhere and volcanos spewing out noxious gases and spilling out more molten rock that merged into the already flowing streams of lava. Very inhospitable.
But with these brutal hundreds of millions of years of bombardment from asteroids and comets, water and carbon compounds were brought to our planet. Given how hot it was, the water was in the atmosphere as vapour, and so were the carbon monoxide and dioxide as well as methane. However, these were now bound to the planet gravitationally and couldn’t escape back into space. Once the bulk of the randomly orbiting solar system debris had been cleared out and incorporated into the various planets onto which they had fallen, the bombardment came to an end, and the Earth started cooling down. It is believed that the last major sterilising impact would have hit the Earth around 3.9 billion years ago.
Cooling during a few thousand years allowed the formation of a thin crust. Further cooling then brought on thousands of years of rain that dumped most of the water vapour from the atmosphere onto the surface. This formed vast planet-spanning oceans. The whole planet was at this point still super hot, but also super wet, and therefore super humid, with the surface practically entirely underwater, lots of active volcanos all over the place but otherwise no mountains. Nevertheless, there would have been some slightly more elevated places, like on the flanks of volcanos, that would have been dry at least some of the time, leaving some spots where water could accumulate in ponds and stagnate. As soon as these conditions were present, around 3.8 billion years ago, the Earth saw its first microbial life emerge.
Claims for the earliest evidence of life at 3.8, 3.7 or 3.5 billion years are still controversial, but it is well established that hydrogen cyanide dissolved in water produces a diversity of essential biological molecules like urea, amino acids and nucleic acid bases; that formaldehyde in slightly alkaline water polymerises to form a range of different sugars; that amino acids, sugars and nucleic acid bases as well as fatty acids have been found in carbonaceous meteorites; and that by 3 billion years ago, prokaryotes (organisms made of cells without a nucleus) were widespread.
There was a major problem, a major impediment to life, that had to be overcome. This was the fact that the entire surface of the Earth was exposed during the day to the Sun’s UV radiation, and UV rays destroy biological structures and DNA. The cleverest of tricks would have been to find a way to absorb these energetic photons and use the energy for something.
Nature is very clever: by 3.5 billion years ago, chlorophylls believed to have developed in order to protect proteins and DNA of early cells appeared, and chlorophyll-containing cyanobacteria—the oldest living organisms and only prokaryotes that can do this—had developed the ability to absorb light, use that energy to split water molecules and use the free electron from the hydrogen atom to sustain their metabolism, spewing out the oxygen in the process. Oxygen accumulated in the crust for a billion years before the latter became saturated with it and unable to absorb any more. Evidence for increasing oxygen levels in the atmosphere is first seen at around 2.5 billion years ago. By 2.2 billion years ago, oxygen concentrations had risen to 1% of what they are today.
Increasing concentrations of reactive and corrosive oxygen was devastating for all forms of life that, at this stage, were all anaerobic: the oxygen was combining with everything it got in contact with creating all sorts of reactive oxygen species (free radicals) that went around causing damage, exactly as they do in our bodies and that of all animals today, and which, in the absence of antioxidants to neutralise them accelerated ageing and death. These were the only card that these simple anaerobic organisms were dealt.
Nevertheless, for another reason entirely, atmospheric oxygen was a blessing because it turned out to be an excellent UV shield. Not only that, but the splitting of oxygen molecules (O2) into oxygen atoms promoted the recombination of these free-floating oxygens into ozone (O3) that turns out to be an even better UV absorbing shield. So, the more photosynthesis was taking place on the surface, the greater the concentration of atmospheric oxygen grew. The more molecular oxygen there was in the atmosphere, the more ozone could be formed. And the more ozone there was to protect and shield the surface from the harsh UV radiation from the Sun, the more complex and delicate structures could develop and grow. Pretty cool for a coincidence, wouldn’t you say?
By 2 billion years ago—within 200 million years—the first eukaryotes appear (organisms made of cells with a nucleus). This makes good sense considering that these simple organisms and independently-living organelles had a great survival advantage by getting together in groups to benefit from one another and protect each other behind a membrane while making sure the precious DNA needed for replication and proliferation was well sheltered inside a resilient nucleus. Note here that these would have been trying to protect themselves both from the damaging UV radiation streaming down from the Sun (it’s estimated that DNA damage from UV exposure would have been about 40 times greater than it is today), as well as from the corrosive oxygen floating in the air (imagine how much more oxidising it is today with concentrations 100 times greater than they were). And in there, within each of these cells, there were chloroplasts—direct descendants from the first UV absorbers and converters, the cyanobacteria—whose job was to convert the photons from the sun into useful energy for the cell.
In all likelihood unrelated to this biological and chemical evolution of the Earth’s biosphere and atmosphere, a long period of glaciation between 750 and 600 million years transformed the planet into an icy snow and slush ball. And with basically all water on the surface of the globe having frozen over, all organisms under a thick layer of ice and snow, photosynthetic activity must have practically or completely ceased. Fortunately, without liquid water in which to dissolve the atmospheric carbon dioxide into the carbonic acid that in turn dissolves the silicates in the rocks over which is streams and carries down to the ocean floor for recycling by the active tectonic plates, all the carbon dioxide sent into the atmosphere by the volcanos just accumulated. It is believed to have reached a level 350 times higher than it is now. This is what saved the planet from runaway glaciation.
Thanks to this powerful greenhouse of CO2, the ice and snow eventually melted back into running streams and rivers, and flowing wave-crested seas and oceans. With water everywhere and incredibly high concentrations of CO2, plant life exploded. And soon after that, some 540 million years ago, complex animals of all kinds—molluscs, arthropods and chordates—also burst into existence in an incredible variety of different body plans (morphological architectures), and specialised appendages and functions. This bursting into life of so many different kinds of complex animals, all of them in the now already salty primordial oceans, is called the Cambrian Explosion. Complex plant life colonised the land by about 500 million years ago, and vertebrate animals crawled out of the sea to set foot on solid ground around 380 million years ago.
Clearly, all plant life descends from cyanobacteria, first to develop the ability to absorb UV radiation, and without complex plant life, it is hard to conceive of a scenario for the evolution of animal life. The key point in this fascinating story of evolution of the solar system, of our Earth and of life on this planet as it pertains to what we are coming to, is that the light and energy coming from the Sun are essential for life while being at the same time dangerous for the countless living organisms that so vitally depend on it. In humans and higher animals this duality is most plainly and clearly exemplified by the relationship between two essential micronutrients without which no animal can develop, survive and procreate. These vital micronutrients are folate and vitamin D.
What makes folate (folic acid or vitamin B9) and vitamin D (cholecalciferol) so important is that they are necessary for proper embryonic development of the skeleton (vitamin D), and for the spine and neural tube as well as for the production of spermatozoa in males (folate). Vitamin D transports calcium into the blood from the intestinal tract making it available to be used in building bones and teeth; folate plays a key role in forming and transcribing DNA in the nucleus of cells, making it crucially important in the development of all embryonic cells and quickly replicating or multiplying cells (like spermatozoa).
Here’s the catch: vitamin D is produced on the surface of the skin (or fur) through the photochemical interaction of the sun’s UV-B rays and the cholesterol in the skin; folate is found in foods, mostly leafy greens (the word comes from the latin folium that means leaf), but it is broken down by sunlight.
What this translates to is this: too little Sun exposure of the skin leads to vitamin D deficiency, which leads to a deficiency in the available and useable calcium needed to build bones, which in turn leads to a weak, fragile and sometimes malformed skeletal structure—rickets; too much Sun exposure leads to excessive breakdown of folate, which leads to folate deficiency, and which in turn leads to improper development of the quickly replicating embryonic cells of the nervous system and consequent malformation of the neural tube—spina bifida.
The most important thing of all for the survival of a species, is the making and growing of healthy babies and children so that they can make and grow other generations of healthy babies and children. This is true for all living beings, but it is not just true: it is of the highest importance, and it has been—taking evolutionary precedence over everything else—since the dawn of life on Earth. Here is how the biochemistry of the delicate balance between these two essential micronutrients evolved.
Six to seven million years ago, our oldest ape-like ancestors walked out of the forest and into the grassy savannah most probably to look for food. (Isn’t this what also gets you off the couch and into the kitchen?). It is most probably the shift in climate towards hotter and dryer weather and, in response to that, the shrinking of their woodlands, that pushed them to expand their foraging perimeter out into the plains that were growing as the forests were shrinking.
Our first australopith ancestors, these ancestors that we share with modern chimpanzees, would have been in all likelihood covered in hair with pale skin underneath (just as chimps are today), their exposed skin growing darker in time with exposure to sunlight. Having left the forest cover, they were now exposed to the hot scorching Sun most of the day, while walking around looking for food, before going back to the forest’s edges to sleep in the trees.
Natural selection would now favour the development of ways to stay cool and not overheat. This meant more sweat glands to increase cooling by evaporation of water on the surface of the skin. It also meant less hair for the cooling contact of the air with the wet skin to be as effective and efficient as possible. But less hair implied that the skin was now directly exposed to sunlight. To protect itself from burns and DNA damage, but also to protect folate, natural selection pushed towards darker skin: more melanocytes producing more melanin to absorb more photons and avoid burning and DNA damage.
In these circumstances, the problem was never too little sun exposure; it was too much exposure, and thus sunburns and folate deficiency. So these early hominids gradually—and by gradually is meant over tens of thousands of years—became less hairy and darker-skinned. They also became taller and leaner, with narrow hips and long thin limbs: this gave less surface area exposed to the overhead sun but more skin surface area for sweating and cooling down, together with better mechanical efficiency in walking and running across what would appear to us very long distances in the tens of kilometres every day, day after day, in foraging and hunting, always under a blazingly hot sunshine. This process that is described here in a few sentences took place over millions of years, at least 3 or 4 and most probably 5 or 6 million years. The Turkana boy, a 1.6 million years old fossilised skeleton is definitive proof that by that time, hominids were already narrow-hipped and relatively tall.
From an evolutionary standpoint it couldn’t be any other way. While keeping in mind that we are still talking about ancient human ancestors, and not modern homo sapiens, nonetheless, did you, as you were reading these sentences, start to wonder who today would fit such a physical description of being hairless, dark-skinned, tall, lean and narrow hipped? Naturally: savannah dwelling modern hunter-gatherers, and, of course, the world’s best marathon runners. It makes perfect sense, doesn’t it?
Taking all currently available archaeological, paleontological, anthropological, as well as molecular and other scientific evidence as a coherent whole brings us to the most plausible scenario in which all humans on the planet today descend from a single mother who was part of a community of people living somewhere on the western coast of Africa; that it is this group of modern homo sapiens that first developed and used symbolic language to communicate and transmit information and knowledge acquired through their personal and collective experiences; and that it was descendants of these moderns who migrated in small groups, in a number of waves, first into Asia and later into Europe, starting 70 to 100 thousand years ago.
It is very interesting that we also have evidence that moderns had settled areas of the middle east in today’s Israel and Palestine region as early as 200 thousand years ago, and that these moderns shared the land and cohabited with Neanderthals for at least 100 thousand years, using the same rudimentary tools and technologies, without apparently attempting to improve upon the tools they had. Meanwhile, this other group of western African coast moderns had far more sophisticated tools that combined different materials (stone, wood, bone), as well as decorative ornaments and figurines.
Thus, although equal or close to equal in physical structure, appearance, dexterity and skills—a deduction based on fossils and evidence that newer and better tools were immediately adopted and replicated in manufacture by moderns to whom they were introduced by other moderns—it is clear that different and geographically isolated communities of moderns ate differently, lived differently, developed differently and at different rates.
This is not surprising, really. Some children start to speak before they turn one, while other do not until they are two, two and a half or even three. Some children start to walk at 10 or 11 months, while others just crawl on the ground or even drag their bum in a kind of seated-crawl until they are three or more. And this is for children that watch everyone around them walking all day long, and listen to everyone around them speak using complex language also all day long. Now, what do you think would happen if a child grew up without being exposed to speech? Why would they ever, how could they ever start to speak on their own, and to whom would they speak if nobody spoke to them?
Fossil evidence shows that the structures in the ear and throat required for us to be able to make the sounds needed for refined speech and verbal communications were in place (at the very least 200 thousand years ago) tens and even hundreds of thousands of years before the first evidence of symbolic thought (70-50 thousand years ago) and together with it, it is assumed, advanced language.
Symbolic thinking in abstract notions and concepts is the most unique feature of our species. It is the hallmark of humans. And it is the most useful and powerful asset we have in the evolutionary race for survival. Sophistication in symbolic thought can only come with sophistication in language and in the aptitude for language: it is only by developing and acquiring more complex language skills that more complex symbolic thinking can come about, and more sophisticated symbolic thinking naturally leads to developing a more sophisticated and refined language in order to have the means to express it.
It’s surely essential to recognise that this is as true for our ancestors, those that developed that first symbolic language, as it is for you and me today. The difference is that then, the distinction was between those few moderns that used symbolic language and those that didn’t, whereas today, the distinction is more subtle because everyone speaks at least one language to a greater or lesser extent. Nonetheless, anyone can immediately grasp what is described here by listening to Noam Chomsky lecture or even just answer simple questions in the course of an interview.
As they moved northward, settling in different places along the way, staying for thousand or tens of thousands of years, then leaving their settlements behind, either collectively or in smaller groups, and moving on to higher latitudes before settling again somewhere else, these people encountered a wide range of different climates and geographical conditions: usually colder, sometimes dry and sometimes wet, sometimes forested and sometimes open-skyed, sometimes mountainous and sometimes flat. In all cases, they were forced to immediately adapt their living conditions, building suitable dwellings and making adequate clothing. This, we know for sure, because they would have simply not survived otherwise, and it is only those that did survive that are our direct ancestors.
Evolutionary adaptation through natural selection of traits and characteristics arising from small—and, on their own, insignificant and typically unnoticeable—random genetic mutations also took place as it does in every microsecond and in every species of animals and plants. But this, we know to be a slow process that is measured on the timescale of tens of thousands of years (10, 50 even 100). Now, consider the evolutionary pressure—the ultimate evolutionary pressure—of giving birth to healthy and resilient offspring that will grow up to learn from, take care of, and help their parents. The most pressing evolutionary need at these higher latitudes was for the body to more efficiently make and store vitamin D from the incoming UV-B rays that, (and this is an important detail often overlooked or under appreciated), make it to the surface only when the Sun is high in the sky and have less atmosphere to go through. This stringent restriction on the few hours near midday when UV-B can make it to the surface is both constraining and life-saving: it is constraining because only during those hours can the essential vitamin D be made, and it is life-saving because a continual exposure to this energetic, DNA-damaging UV radiation would in time sterilise the surface of the entire planet.
The higher the latitude, the lower the Sun’s path on the sky throughout the year and especially during the winter months. Therefore, the shorter is the season during which UV-B rays reach the surface and during which it is possible for vitamin D to be produced on the skin or fur of animals. The only solution to this severe evolutionary pressure is as little body hair and as little pigmentation as possible (think of the completely white polar bears, arctic wolves, foxes and rabbits). As an aside, what else do you think as advantageous in the cold? The opposite as what is in the hot sun: more volume for less surface area; a smaller and stockier build that keeps heat better, exactly as we see in the cold-adapted Neanderthal.
Settled in a place that provides what we need to live relatively comfortably, we tend to stay there. This has always been true, and even if it has changed in the last few generations in industrialised western countries, we have witnessed this phenomenon up until very recently on islands like Sardinia, Crete, or Okinawa, remote valleys in the Swiss Alps, the Karakoram, Himalayas or Andes, and in other geographically isolated pockets of people with genetic characteristics homogenous amongst themselves but distinct with respect to other human populations. And thus across the world we find a whole spectrum—a rainbow—of different colours and shades of skin, different colours of hair and eyes, different amounts and textures of body hair, of different physical builds and morphologies, of different metabolic and biochemical sensitivities, all seen on a continuum, all dependent upon the evolutionary history of the subpopulation where particular characteristics are seen to be present or absent to a greater or lesser extent, and all of this driven by the evolutionary pressures to adapt and maximise the survival probability of our offspring, our family, our clan, our species, by optimising the amount of folate and vitamin D through the delicate balance between not enough of the latter from under-exposure to UV-B’s that produce it, and not enough of the former from excessive exposure to the same UV-B’s that destroy it.
What this tells us is that, for one thing, we have absolutely nothing to do with the colour of our skin, eyes and hair, and nothing to do with any of the physical and biochemical characteristics we have inherited. It tells us that this has nothing to do with our parents or grand parents either, really, because these are particularities that have evolved over tens of thousands of years of evolution in a very long line of ancestors that settled in a place, stayed put and lived at a particular latitude in a particular geographical setting with a particular climate. It tells us, in the most obvious manner, that because this is so, discrimination based on colour or physical features is not jut unfounded, but it is simply absurd.
If you’re black, you’re black. If you’re white, you’re white. If you’re chocolate or olive-skinned, then you’re chocolate or olive-skinned. If you are “yellow” or “red” then that’s just how it is. And who cares how you phrase it or not, try to be “political correct” and avoid speaking of it. That’s just silly. All of it is simply just the way it is. In the same way, if you’re short or tall, hairy or not, thin or stocky, it is just the way it is. However you are and whatever features you consider, there is never anything more or less about it, never anything more or less about any of these features: it is an expression of our genetic ancestry going back not just a few but hundreds of thousands of generations.
What this also tells us is that we have to take this information into account in everything we do, especially in regards to what we eat, where we live, and how much or how little we expose ourselves to the Sun’s vitally important UV-B rays. Disregard for these fundamentally important details leads to what we see in the world in this modern era where we all live wherever we want, more or less, and find ourselves with our olive or dark brown skin living in at high northern latitudes, or with our fair or milk-white skin living near the equator with strong overhead sun all year round, and see the consequent high rates of vitamin D deficiency and rickets in our dark-skinned northern dwellers, together with the similarly high rates of folate deficiency and spina bifida in our fair-skinned southern dwellers.
In general, if you are dark-skinned you need to expose your skin to the sun a lot more than if you are fair-skinned, because you will both produce less vitamin D and store less. If you are fair-skinned you need less exposure and will tend to store the vitamin D more efficiently for longer periods of time. As for folate, we all need to eat (or drink) leafy greens (i.e., foliage) and green veggies.
However, there is an additional complication that makes matters worse (far worse) That complication is that in this day and age, we all live inside, typically sitting all day facing a computer screen, and sitting all evening eating supper and then watching TV. Not everyone, of course… but most people. Not only that, but most of us all over the world now eat more or less the same things: highly processed packaged foods usually high in processed carbs and low in good, unprocessed fats, high in chemicals of all kinds and low in nutrients, and hardly any leafy and green veggies or nuts and seeds. And boy do we love our Coke, our daily bread, our fries and potatoes, our pizzas and big plates of pasta, and our sweets and desserts! Not everyone, of course… but most people. Consequently, we are all as deficient in folate as we are in vitamin D. We are all as deficient in unprocessed fats and fat-soluble vitamins as we are in all other essential micronutrients. How depressing.
But once we know this, once we have been made aware of this situation, we can correct the problem by switching to a diet of whole foods—of real foods—rich in folic acid and fat-soluble vitamins like A, D, E and K2, (the inuits, for example, get all their vitamin D and the other fat-soluble vitamins from the fat of the whales and seals they eat), and supplementing adequately to maintain optimal levels of both vitamin D (50-80 ng/ml or 125-200 nmol/L) and folate (>5 ng/ml or >11 nmol/l), especially during conception, pregnancy and early childhood, but throughout life and into old age.
There’s one last thing I wanted to mention before closing, and in which you might also be interested: can we ask if one is more important then the other, folate or vitamin D, and do we have a way to answer this question from an evolutionary standpoint? Well, here is something that suggests an answer: in all races of humans on Earth, women are on average about 3% lighter in skin colour than men of the same group. For decades, researchers (mostly old men, of course) were satisfied with the conclusion that this was the result of sexual selection, in the sense that men preferred lighter skinned women and so this is how things evolved over time. Of course, most of you will agree with me now that this just sounds like a cop-out or at best a shot in the dark from a possibly sexist male perspective.
Most of you will surely also agree that considering the question from the perspective of the importance of vitamin D versus folate is clearly more scientific in spirit than claiming sexual selection to explain the difference. And if women are lighter than men no matter where we look on Earth, this strongly suggests that it is either more difficult to build up and maintain good levels of vitamin D to ensure healthy offspring, or that it is more important. In today’s world, it certainly is true that it is far easier to have good levels of folate because even if you stay inside all day, as long as you eat leafy greens or drink green juice, your folate levels will easily be higher than the optimal minimum of 5 ng/ml, and probably much higher, like mine which are five time higher than that at 25 ng/ml.
So, for us today, especially if we eat greens, there is no question that we have to pay much closer attention to our vitamin D levels that tend to be way too low across the board all over the world. We can hypothesise that if we continue evolving over millennia following this indoors lifestyle that we have, humans everywhere will continue to lose both body hair and pigmentation, even those who live in sunny countries, because they don’t expose themselves to the Sun. I would like to encourage you to instead expose your skin to the amount of sunlight that is in accord with your complexion, drink green juice, monitor your vitamin D levels at least once per year, and take supplements to ensure both stay in the optimal range (I recommend taking A-D-K2 together to ensure balance between them, better absorption and physiological action). That alone, even if you don’t do anything else, will be of great benefit to you, and, if you are a soon-to-be or would-like-to-be mother, of even greater benefit to your child or children.
And next time you go out, and each time after that, pay attention, look and appreciate the amazing richness and beauty of all the different skin colours and unique physical features of all the people you see all around. What you will be seeing is the inestimable richness and incalculable pricelessness of our collective human ancestry expressing itself vividly and openly, nothing held back and nothing hidden, for everyone to see and appreciate.
If you are interested in reading more about the topics touched upon in this article, its contents draw from the books Life in the Universe, Rare Earth, Masters of the Planet, The Story of the Human Body and the Scientific American special issue Evolution that features the article, entitled Skin Deep, that prompted me to write this post. And please share this post: we all need to do what we can to help overcome discrimination based on race and appearance.
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