The peoples that embarked and supported the exploration of new trading and colonising routes soon discovered that the free-riding of the technological advantage could be easily perpetuated. Thanks to that, the ones that invested in better and faster understanding of the world, plus the technical innovations that that understanding and implementation represented, contributed to a further control of the world’s connectivity. From that on, there were no major barriers to a hyperconnected world. What they could not control by exchange, they would control by overpowering, as the conquest of Malacca, the Aztecs, the Incas demonstrates. If you kept on expanding your technological and resource allocation dominance over other peoples, your system would be the one to dominate, and that’s exactly what the Western nations did over a period of a few centuries.

New trading routes led to an excess of wealth that could be poured into more navigational sophistication, which in turn would make the trading networks more reliable and affordable, freeing more resources for further improvement. Part of these resources went to the birth of modern science, changing forever the way our understanding of the world was established.

To make a boat sail safely from port to port you would rely less and less on divinity and more on your instruments, navigational skills, the capacity to understand the sky, star positions, read the winds, proper sails, masts, ropes to withstand storms, carrying lemons to stop scurvy, social structures to govern a ship and stop mutinies, etc. Those powers that would put scientific knowledge to good use would have in their hands better control of the high seas and the peoples cruising them. Likewise, those who understood better the fabrication techniques could build better vessels, and equip them with better weapons. On the other hand, the faraway encounters would contribute to the scientific understanding of the world, like sea currents, Volta do mar, steady trade winds, or even catamaran technology from the Pacific and front crawl swimming techniques from North, South America, or South Africa.

In fact, Columbus’s error regarding the radius of the Earth (which he was convinced until he died) was due to the preliminary stages of scientific knowledge attempting to describe the world we lived in. In that case, he was mistaken, but the geographers’ community soon recognised the error and corrected it (or lent more credibility to other estimates circulating at the time). This iterative process helped to better understand the world that was opening up before them as they tried to cartograph the new routes faster than they were explored.

From these explorations and shocks to the perceived worldview, it is not difficult to imagine that the notion of an entire landmass the size of the Americas suddenly appearing on maps (over about 20 years) might have led to the acceptance of rethinking the entire Universe. If the Earth contained a whole part of itself that was unknown to the Old Scriptures, how much more knowledge might be out there—waiting to be found, explored, and understood—not through the lens of the Scriptures, but through the lens of something new? These cartographic shifts might easily have been the seeds for scientific enquiry—the seed of the Scientific Revolution.

In fact, it is interesting to reflect on that word, “revolution.” What does it stand for? It comes from the root “to revolve”, which means to spin around. Why—if an entire continent had been missed, and Jerusalem is not the centre of the Earth—could it not be that the Earth is not the centre of the Universe either? That kind of thought might have helped Copernicus push the heliocentric idea: that the model best suited to describe the Universe is not a geocentric one, with the Earth at the centre, but one with the Sun at the centre of the known cosmos. Copernicus was not the first to propose that idea; the Pythagoreans had already supposed the Earth might move, and Aristarchus of Samos proposed a heliocentric model in the 3rd century BCE. Seleucus of Seleucia said something along the same lines in the 2nd century BCE. About 600 years later, in the 5th century, Martianus Capella, from Roman Carthage, proposed that Mercury and Venus spun around the Sun. At about the same time, Aryabhata in Patna, India, proposed that the Earth spins and that the planets orbit the Sun. In the 12th century, Ibn Rushd (Averroes) and Nur ad-Din al-Bitruji of the Cordoba Caliphate were also critical of the geocentric model and proposed alternatives. Their views spread into European intellectual spheres. However, none of these theories gained much traction at the time they were proposed. One can say that the mindset of the people of those generations was not particularly open to such a shift in worldview, nor was it needed for any practical purpose.

To be open to other worldviews becomes more likely if a sweeping 30% extra landmass is literally put on the map. The same world that the Scriptures plus Classical Philosophy were so certain they understood. Even though the Catholic Church did not pay much attention to the fact that the world was different than said, surely minds would become more open—even if obtuse. Moreover, those same conceptualisations ended up making navigation more precise. And the required navigational observations and technical means (star and planet positions, astrolabes, compasses, telescopes, clocks…) helped to question the worldview in a more rigorous way—with the newly discovered facts holding more face value than old beliefs. In short, cosmological views came to serve a practical purpose.

Therefore, the landscape was set. After Europeans became aware of a New Continent, Copernicus was able to push his idea (initially as a short leaflet in 1514), and later publish, after his death, his De revolutionibus orbium coelestium. His heliocentric model was not the one we know today. Copernicus’s model was not that innovative, nor significantly simpler than the Ptolemaic one, because he still needed the use of epicycles (small circumferences around the circular orbit of the planets) to accurately describe the rotation of the planets around the Sun. It would be Kepler—about 70 years later—who, after throwing out his own Mysterium theory of planetary movement because Tycho Brahe’s observations did not match, solved the motion of objects in the Solar System with simple elliptical orbits and delivered us pretty much the view that we now have.

The difference with all the previous scholars—after Copernicus’s posthumous publication—proposing that the Earth was not static, was that the public at the time was much more accepting of the revolution of the Earth thought. A thought that would be revolutionary!

Revolution, at the time, had the meaning that Copernicus used in his title: simply the spinning around of the celestial bodies—how they revolved around the Sun. Revolved, revoluted, revolution. It was a physical description, like that of the revolutions or cycles of an engine, or as one famous revolutions podcaster puts it, “coming full circle”, just to come back to the beginning. Revolution did have, on rare occasions, the meaning of change prior to Copernicus’s work. However, the acceptance of heliocentric theory by the public of the time. It was so disruptive to the mindset of the age, overturning millennia of knowledge and worldview—so Earth-shattering (pun intended)—that the first main word of the work itself, revolutionibus, was adapted less than a century later to mean the overthrow of a political system (the Glorious Revolution in Britain). When transferring the physical meaning to the political one, revolution meant “a circular process under which an old system of values is restored to its original position, with England’s supposed ‘ancient constitution’ being reasserted, rather than formed anew”. At that point the use of the word was far form the meaning that it has now, as a radical new direction, or changing of course of what was before. Soon after, however, the word gained the modern concept of revolution, as used for the French one, which probably someone has heard about. Now revolution is more widely understood as the shattering of a previous political, social, technological—or otherwise—system, and the establishment of a new one: the Glorious Revolution, French Revolution, Industrial Revolution, Agrarian Revolution, Sexual Revolution…

It could be that the people at the time—after the Earth had been kicked aside, given rotation, put in orbit around the Sun, and the stars made still—experienced a mental shift so profound that it allowed for a reshuffling of many pre-existing mentalities. Maybe it can be compared to the shattering effect, almost a rite of passage, that many children in the Western world experience when they realise that Santa Claus is not a real being, but a construct created by society to make them believe that the bringer of presents is this exotic figure from faraway lands, and not their parents or families. For the child, it is already a big impact—and if you experienced that, you probably remember the moment, even if it was decades ago. Then imagine if instead of just one child at a time, it were an entire society realising, more or less simultaneously (within a generation), that the reality they had so strongly believed to be true, no longer was. That is what the so-called Copernican Revolution brought to European thought in the 16th century: a collective, mind-shattering effect. We, as humans, have been toying with these moments ever since. But more about that later.

In fact, the public that was more open to these ideas was also in the midst of another revolutionary movement, which at the time was called a protest, for lack of a better word: Protestantism. If the world, the solar system, the Universe, the Cosmos, was not as the Church claimed—with extra continents unaccounted for, the Earth in motion, and stars being other suns, perhaps with other Earths—then the Church became open to protest and reform. And if protest and reform were possible, then the acceptance of truly exotic ideas—like the Earth revolving—became easier in a society already undergoing profound transitions. In fact, different solar system models were readily adopted by Tycho Brahe and Johannes Kepler, Danish and German astronomers sponsored by Protestant-friendly kings. Meanwhile, Latin astronomers such as Galileo Galilei and Giordano Bruno had major conflicts with the Catholic Church in Northern Italy—Galileo famously tried, Bruno burned at the stake. Bruno’s seven-year trial and sentence to be burned alive was not specifically for his belief that the stars in the sky were other distant suns orbited by other planets, but also because of his rejection of most Catholic doctrines.

The difference between Copernicus in the 16th century and all those who proposed alternative cosmological systems before might be that society was more open to new ideas because of empirical slaps in the face—steadily, repeatedly, forcefully. First, sailors and their investors realised that direct observations could actually shift reality—such as the discovery of a continent, accurate measurement of latitudes and longitudes, and the real size of the Earth’s circumference. Second, astronomers and their sponsors (who were often astrologers for European courts—better predictions meant better horoscopes; the zodiac pays for your smartphone, if you think about it) found that when your health or the outcome of a war depends on the conjunction of Saturn and Jupiter, and your astronomer looks through a telescope and tells you that these planets have rings and moons orbiting them, you might predict better when to wage your next war. Third, traders could more precisely calculate profits or invest in new products—like new dyes and pigments (e.g. scarlet), or learning how to plant species such as pepper, potatoes, tomatoes, tobacco, coconuts, sugar cane, among others, across the world. Actual measurements began to overturn established doctrines one after another; these facts reinforced the critiques of the old system and laid the foundation for an alternative system of establishing knowledge. The Scientific Revolution went hand in hand with the development of better instruments and measurements that define the modern world we experience today.

It was equally important that these new ideas travelled and multiplied faster than ever before. On one hand, naval interconnectivity regularly reached all continents and the major inhabited landmasses of the planet. From there, peoples—willingly or unwillingly—became part of a shared system of exchange, a process that continues today, where nearly every human being is regularly connected to the rest of the world in one form or another. Our present hyperconnected world is extending the reach and frequency of connection to ever more remote places. On the other hand, the printing press allowed for the multiplication of ideas at a rate faster than authorities could suppress them. Even if the works of figures like Copernicus or Bruno were censored, confiscated, destroyed, or burned, it was much more likely that one copy would escape, be read, and be copied again. Before the printing press, Protestant ideas—like those of the Hussites in the 15th century—did not spread far beyond their place of origin (e.g. Bohemia). Later, Prague—with its famous astronomical clock—would host Brahe and Kepler. On the other end of the chain, at the point of reception, Spanish missionaries actively protected indigenous languages (while simultaneously suppressing their cultures) in regions such as Mesoamerica, the Andes, and the Philippines, to prevent indigenous peoples from being exposed to “dangerous” Protestant, Enlightenment, or revolutionary ideas. To this day, these regions preserve some of their linguistic diversity and remain heavily Catholic, with the Philippines being the only nation (alongside the Vatican) that does not permit divorce.

Our hyperconnected and idea-copying world is the one that gave birth to the concept of humanity—a “humanity” that can now begin to ask itself what it wants to do, now that we have the means to communicate with one another, and the resources (or energy levels) to invest a fraction of that energy in specific goals. But before asking that question, we first need to understand the mechanisms by which a hyperconnected people is able to pose it: which networks are activated, in which language communication occurs, with whom that exchange is implemented, and what actions can—or cannot—be taken. What is the agency?

Curiously, one of the early adopters of Copernicus’s thesis was Thomas Digges, who removed the need for the sphere of fixed stars. He proposed the existence of distant stars scattered throughout the Universe. This led him to raise the paradox of the dark sky: in an infinite Universe filled with stars, the sky should look like the surface of the Sun, because in every direction there should be at least one star. Since the sky is black, the Universe cannot be infinite. With that in mind, the Copernican Revolution—which displaced us from the centre of the Universe—is still not complete. It is geographical, but not temporal. Heliocentrism kicked the Earth and its peoples out of the centre of space, but the dark sky placed us in a special time—a time when we can still see the horizon of the visible Universe. Now we are in another special time—the time when humanity is conceptualised. The time to ask: what does humanity want?

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