Author: Priscila Cheib Duarte

How Earth’s Surface formed, how humans can still watch it happening, and why it is important to set the record straight.

A dynamic fusion of Earth’s solid crust, atmosphere, hydrosphere, and biosphere forms a very, very, very thin layer corresponding to less than 1% of Earth’s total volume – the Surface.

Planet Earth’s Surface is so important that very often, even today, humans refer to it as if they are referring to the whole planet.

Earth’s Surface has an area of around 510,070,000 km²: 361,130,000 km² (70.8%) of water and 148,940,000 km² (29.2%) of land. Its thickness ranges from 105 km to 170 km – 100 km corresponds to the atmosphere, and 5 km to 70 km corresponds to the land. To contextualize, planet Earth’s radius is around 6,371 km.

All of this started to form around 4,500,000,000 years ago (right after the Earth and Moon forming event). At this point, the difference in temperature between Earth’s mantle and the atmosphere started to thicken Earth’s outermost solid layer. The Surface became a relatively cool but hardened shell within a few million years, with most mantle heat escaping via volcanism.

As the heated volcanic material rose to the top, it cooled and deposited at the surface. While the planet’s external layer grew thicker and heavier, it eventually began to slowly sink back to the mantle, where it heated and returned to the surface via volcanism.

This thicker surface created pressure on the heated mantle, which in turn made the shell layer discreetly expand. With tidal interactions, collisions with astronomical bodies, and also under the magnetosphere’s influence, the entire planet’s surface started to crack within just 40,000,000 years. 

Those enormous chunks of cracked material began to move around on top of the mantle. The heated mantle material rose through the cracks, released heat as it approached the surface, and then sank again, setting up convection currents.

Several convection currents moved around Earth in a process called tectonic plates. Because of their proportions, their structure, dynamics, and components are mostly influenced by gravitational interactions with other astronomical bodies, especially the Sun and the Moon.

Since Earth’s formation, astronomical bodies—comets, meteorites, and other objects—have clashed with the planet’s Surface. Those bombardments have decreased throughout the years (there is no significant fabrication of solids after the solar system’s formation), but they still hit Earth quite often.

Because some of those impactors were massive, leaving huge marks on Earth’s solid crust, it is easy to assume that they must significantly influence the surface’s evolution. However, mineral analyses steadily show that the Earth’s Surface structure, dynamics, and components are far more affected by what happens in Earth’s internal layers.

This same engine that has been going on for billions of years is still running today. Recently, some interesting studies have shed light on the ongoing Earth Surface dynamics.

One study focused on a 100 km region of the Southeast Indian Ridge, where an event released around 160 million cubic meters of lava onto the sea floor and shifted two sections of the oceanic crust apart by at least 2 meters in a matter of days. As the existing crust is pulled away from the ridge by the movement of tectonic plates, new crust is produced by magma that wells up from Earth’s core and solidifies.

The other study revealed that eastern Africa is closer to splitting apart than previously thought. The Turkana Rift Zone in Kenya, a critical segment of the East African Rift System, is undergoing a process called “necking” (a stage in continental breakup). High-resolution seismic data show that the crystalline crust beneath the rift has thinned to about 13 km along the rift axis, revealing an active rift undergoing crustal necking. The identification of necking in the East African Rift System indicates that eastern Africa is primed for continental breakup – what was once a molten crack is now a continent in the process of becoming two. 

Curiously, despite all evidence, it is more mainstream science that everything that affects Earth’s Surface—the crust, the atmosphere, and the biosphere—comes from outer space (from the “sky”), with popular narratives often emphasizing asteroid impacts or solar radiation as the primary shapers of Earth’s Surface. 

It is still challenging for humans to recognize that the atmosphere, biosphere, and crust are byproducts of planetary interactions, rather than causes in themselves.

It is important to highlight that what makes planet Earth’s Surface so remarkable is not its thickness, but its thinness. It is not its permanence, but its dynamism. It is not its stability, but its relentlessness.

The evidence that Earth’s Surface is dynamic, fragile, and constantly changing is not a matter of opinion. Empirical evidence is not a political statement, and it does not need to be believed to be true. It is data. 

And yet, the acknowledgment of these facts (and what they mean for the human relationship with the planet) remains entangled in political debate. 

The question is not whether to believe it. The question is what to do with it.

Whether to act on the evidence, or to protect the Surface that sustains all life, is not a matter of choice – it is a matter of necessity.

The Surface does not care about human politics. It will continue to crack, to spread, to build new crust, to change its atmosphere, to tear continents apart. The only question is whether humans will recognize what is happening in time to respond.

What water reveals about human knowledge – and its limits

Around 4.500.000.000 years ago, 10.000.000 after the Moon-forming event, a day on Earth was about 6 hours long, and the Moon was way closer – 24.000 to 32.000 km away from Earth (today it is 383.000Km). The Sun was a fast-spinning baby star, taking 9 to 10 days per spin (today, it is 24 (equator) and 35 (poles) days). 

The Moon-forming event increased Earth’s and Moon’s temperatures while making them intensely spin and rotate around each other. With such loaded energies, the initial tidal interactions between Earth and Moon were more violent, resulting in energies being dissipated at a faster pace, with both objects considerably slowing their rotation and spin within their first millions of years. At this point, the Sun was way more radioactive despite having lower temperatures (nuclear fusion was just starting). 

A stream of charged particles, the solar wind, was reaching the terrestrial planets, making radioactivity at least 5 times higher than today. The solar wind and the intense tidal interactions between Earth and the Moon created a layer of charged particles early on, a combined magnetosphere around both objects. In turn, the magnetosphere enables a layer of gas to be trapped between the planet’s surface and space – the atmosphere.

Still around 4.500.000.000 years ago (due to gravity, rotation, and tidal interactions), the densest materials (metals like iron and nickel) were sinking to form Earth’s metallic core at the same time that the less dense materials (silica-like) were accumulating in a layer around the core called the mantle. 

Near the mantle surface, the pressure and temperatures caused the mantle minerals to split their chemical compositions, releasing gases and water molecules (roughly 7% of the mantle minerals have 2% of their composition made out of water molecules – which (due to the mantle proportions) is enough to fabricate several oceans like the ones we have at Earth’s surface today). The water molecules from the mantle outgassing could get trapped at the planet’s surface because of the atmosphere, making planet Earth (probably already) with water on its surface.

This is a brief description of HOW and WHEN water appeared on Earth’s surface, according to scientific knowledge based exclusively on empirical evidence.

Believe it or not, scientists are only recently (perhaps) beginning to understand WHAT water actually is.

As commonly known, water behaves differently than any other liquid at Earth’s surface. It gets less dense (expands) at freezing temperatures, which is why ice floats on liquid water. It has a high boiling point compared to other liquids. And it has a high surface tension, creating a membrane-like outer layer that makes it more resistant and cohesive in its liquid form (which explains why insects can walk on water and why water droplets assume a spherical shape). These are just a few of the several “anomalous” features that water, as it is known at the Earth’s surface, presents.

Over the past three decades, advancements in computational modeling have significantly improved the accuracy of molecular simulations. This progress has allowed for detailed studies of the behavior and structure of water molecules, particularly in conditions that cannot be found on the Earth’s surface.

These studies provide evidence that water has two distinct states, that those two states are interconvertible, and that ice has at least 21 different forms – and the list continues to grow. 

Under different pressures and temperatures, water solidifies into distinct crystalline structures, each with its own molecular arrangement and density. The familiar ice from a freezer is Ice Ih, a hexagonal structure found on Earth’s surface. But in the upper atmosphere, Ice Ic—a cubic form—can exist. Under high pressure, dozens of other phases emerge, from Ice II to Ice XXI, each with different properties.

Under extreme pressures and temperatures, oxygen atoms remain fixed while hydrogen protons flow like a liquid, resulting in superionic ice, which is believed to exist in large amounts deep inside Uranus and Neptune, whose movement of protons generates the unusual magnetic fields observed around these planets.

In addition to these forms, water can also freeze into a glassy, non-crystalline state called amorphous ice. There are at least three types (low-density, high-density, and very high-density amorphous ice), with the amorphous form believed to be the most common ice in the universe.

From all these data, one thing is safe to say – the water molecule H₂O is remarkably adaptable and can assume many different designs, always reacting to temperature and pressure (together or in isolation) to determine its state and, consequently, its molecular structure.

Curiously, like many other things in “science”, researchers often take for granted that what humans experience at Earth’s surface is “normal” or “standard”, only to become disappointed with the results of their experiments.

What happens at Earth’s surface is not universal or common. The acknowledgment that the ice found on Earth’s surface (ice I) is extremely rare in the universe is, somehow, painful because it leads to an inconvenient truth – that humans do not know a lot about everything.

Actually, humans know very little about very little. Things are still not given, controlled, or known. Interestingly, since the dawn of written records, humans have consistently believed they were at the peak of their knowledge, mastering their own time—only to become a laughable footnote to generations to come. In many ways, we are still similar to the ones who lived many years ago.

Perhaps, for the first time in history, humans should acknowledge how little is actually known—about water, about everything—and from that starting point, build what could be a truly new age for human knowledge. At the very least, with such a humble starting point, perhaps striving to “know about everything” can get more interesting.

A billion-year partnership, a frivolous assumption, and what humans risk losing in the new space race.

According to empirical evidence, somewhere between 4.537.000.000 and 4.510.000.000 years ago, as a consequence of the Solar System’s formation, Earth could barely hold itself together; its shape was an ellipsoid, and it no longer had a surface, just a layer of rock gas that gets denser with depth. 

An impact with another astronomical body occurs that makes Earth spin even faster, making it hotter until its equator can no longer remain coupled. Parts of the equator break off, vaporize, and settle into an orbit, forming a disk. The disk rapidly flares into a giant donut-shaped structure whose surroundings settle into the “lunar seed”, growing the Moon with no volatiles. 

After just a few years, the donut-shaped structure shrank to inside the Moon’s orbit, and a newly formed large Moon emerged (the biggest Moon of the solar system, 1% of Earth’s mass), with Earth and Moon sharing the same isotopic profile (same number of neutrons in the atoms of their elements). 

Tidal interactions between the Earth and the Moon act as a gravitational arm against Earth, affecting the orbital inclination and tilt of both (Earth and Moon). It gradually pulls the Earth’s axis tilt to 23.5 degrees while bringing the Moon’s orbit inclination to 5 degrees relative to the ecliptic (Earth plane orbit relative to the Sun) that we can observe today. According to the rock record, this process ended 4.510.000.000 years ago, the last time Earth’s global silicate system had been mixed. Lunar samples also state the same. 

Over the years, the Earth and Moon relationship has become more entangled, intertwined, and sophisticated.  As for today, just one little aspect of it, the Moon’s gravitational pull, creates the ocean tides that in turn drive ocean currents and influence climate patterns across the Earth’s surface. 

A 2018 study elegantly established the statistical correlation between El Niño and the Moon’s 18.6-year tidal cycle. El Niño events tend to occur in specific years relative to the lunar nodal cycle—specifically the 1st, 10th, and 13th years after the peak of the cycle. La Niña events, in contrast, tend to occur in the 3rd, 12th, and 16th years. Despite the resistance to such (lunatic) claims, and much criticism of this study (including a 2025 one), the statistical correlation itself has not been disproven.  

In June 2026, the Japan Aerospace Exploration Agency (JAXA) confirmed the existence of an enormous cavern beneath the Moon’s surface—about 50 kilometers long and 100 meters wide. The cavern could serve as a natural shelter for future astronauts, protecting them from solar radiation and extreme temperatures. Contrary to the study that connects the Moon cycle and climate patterns, the discovery was received with great enthusiasm by the scientific community. 

The enthusiasm is understandable—a natural lunar shelter is a remarkable finding. But it also reveals a pattern: the space race celebrates what can be used, while neglecting what is there and is not yet understood.

The 24-hour rotation, gravity, tides, climate stability, and biological rhythms are all byproducts of the Earth and Moon relationship that has been going on for billions of years and that are still poorly understood. 

And yet, curiously, the space race operates as if the Moon is merely a stepping stone. Plans for lunar bases and mining operations proceed as if the Moon is a resource to be extracted – rather than a partner to be understood.

Perhaps there is a lesson here from colonization – The assumption that humans can arrive, take what they need, and move on has a poor track record. A more effective approach might be to start by understanding interactions. 

There is no evidence that humans could reproduce or survive on a planet without a Moon like Earth’s Moon. The Moon is as crucial to human existence as Earth itself. That is why knowing about its origins — and its ongoing influence — matters so much.

Learn first, before destroying. Recognize before the deadline what we actually depend on. Perhaps this time around, we might be able to make what is important not available for exploitation. 

If you enjoy science writing, you can check my publication, Beliefs of a Female Architect. It unfolds what happened from the Big Bang to today’s world, completely grounded in empirical evidence. I’d be delighted to see you there.

A Moon-to-Mars-sized astronomical body once existed in our solar system. It’s gone now—but it left an important call to action.

In 2019, a meteorite was found in the Sahara Desert named Northwest Africa 12774. In 2025, a team of researchers started analyzing it and realized that this meteorite belongs to a rare class of meteorites called angrites. There are fewer than 100 angrites out of the more than 80,000 meteorites discovered on Earth’s surface.

By analyzing Northwest Africa 12774’s chemical fingerprints, scientists found that the number of neutrons in the atoms of its elements (isotopes), specifically oxygen and chromium, matched the composition of astronomical bodies in the solar system.

By measuring the decay of radioactive elements inside Northwest Africa 12774 (which act as natural clocks), scientists determined that it crystallized from molten rock just 4 million years after the first solids formed in the solar system. This dates it to about 4.56 billion years ago, making it one of the oldest known volcanic rocks of the solar system. Only material that formed alongside the Sun and its surrounding disk of gas and dust could be this old.

In addition, by testing Northwest Africa 12774’s mineralogy, scientists observed that the meteorite contains crystals of a mineral called clinopyroxene that are unusually rich in aluminum. To forge these specific crystals, the rock had to be subjected to immense pressure that could only be generated inside a large, differentiated body, not a small, undifferentiated asteroid. Scientists calculated that the “angrite parent body” must have been at least 1,000 km (620 miles) in radius. If the crystals formed at a shallow depth, the body could have been as large as 3,600 km (2,200 miles)—comparable in size to the Moon or even Mars.

Although Northwest Africa 12774 was not seen falling from the sky and its exact path through space cannot be tracked, its classification as an angrite links it to a specific group of meteorites overwhelmingly associated with the main asteroid belt between Mars and Jupiter.

To contextualize where and what the asteroid belt actually is, it might be useful to recap what the solar system consists of today:

• One star: The Sun.
• Orbiting the Sun in different directions: Comets (because they were formed either entirely outside or on the very outskirts of the solar system).
• Orbiting the Sun in the same direction:
  • The terrestrial planets: Mercury, Venus, Earth (with 1 moon), and Mars (with 2 moons).
  • The asteroid belt: Between 1 and 2 million asteroids composed of rocky, refractory materials, where Ceres (a dwarf planet) is the largest object.
  • The giant planets: The gas giants (the number of moons grew exponentially over the last few years) – Jupiter with 95 moons, Saturn with 146 moons; The ice giants – Uranus with 27 moons, Neptune with 16 moons.
  • The Kuiper belt: An icy ring with millions of objects made mostly out of ice and volatile elements, featuring proto-planets and dwarf planets like Pluto (with 5 moons), Eris (with 1 moon), Haumea (with 2 moons), and Makemake (with 1 confirmed moon).

Essentially, scientists are able to know all about the size, chemical composition, and age of all these solar system objects through two main sources of evidence.

First: telescopes. By analyzing their images, scientists can infer the size, speed, and rotation of astronomical bodies. By analyzing the light and spectrum of Solar System objects, astronomers can determine their chemical composition.

Second: meteorites. Minerals that either fall to Earth’s surface from space or are sitting at the Earth’s surface waiting to be found carry the chemical signatures of their parent bodies. 

By comparing meteorite compositions with those observed through telescopes, scientists can piece together the solar system’s makeup.

It is important to highlight that understanding how, when, and why the solar system developed the way it did is far more valuable than simply listing and classifying its astronomical bodies. In Science, merely describing something, very often, does not move Science forward. In contrast, understanding something is what propels scientific progress.

To illustrate, consider this timeline:

• 5.103.200.000 years ago — A star cluster that would become the solar system was taking place in the Milky Way
• 4.568.200.000 years ago — The first solar system solids were formed
• 4.518.200.000 years ago — Nuclear fusion ignited the Sun
• 4.510.000.000 years ago — Earth and the Moon formed

Knowing these dates is useful. But they don’t change anything if they are not used to understanding why all those milestones happened the way they did. In this context, we can see the data we have as a starting point rather than as an end in itself.

An effective approach is to look at the Solar System timeline and ask: What are the Solar System milestones that could have happened faster or differently? Are there any shortcuts in terms of planetary system formation that could take place, and does that mean that there might be other planetary systems in the universe, for instance, that could have life for a longer period of time than what happened on Earth?

Anyway, understanding how planets formed—and what their characteristics were at specific points in time—can give a roadmap for what to look for elsewhere in the universe.

Without making a direct association between a planet’s emergence conditions in our own solar system, we are just going to be looking for water out there for a very long time… without ever finding anything.

How little red dots are pushing empirical science to the vanguard of intellectual thought

Recently, the scientific world has been baffled with the new discoveries of the James Webb Space Telescope – JWST

(as the name says, a Space Telescope, launched on December 25, 2021 that sits on the opposite side of the Earth from the Sun, about 1.5 million kilometers (930,000 miles) away from Earth which is nearly four times farther from Earth than the Moon is)

of “Little Red Dots” – LRD that turned out to be black holes that were not just massive but also way older than scientists expect black holes could ever be.

Besides the dichotomy of namegiving (little red dots = massive black holes), the research is extremely elegant. Several dedicated programs

(Cosmic Evolution Early Release Science – CEERS, JWST Advanced Deep Extragalactic Survey – JADES, Next Generation Deep Extragalactic Exploratory Public Survey – NGDEEP, Public Release Imaging for Extragalactic Research – PRIMER, Ultradeep NIRSpec and NIRCam Observations before the Epoch of Reionization –  UNCOVER, and Cosmic Evolution Survey — a project designed to map the evolution of the universe’s large-scale structure – COSMOS-Web)

generated huge amounts of data and images about the universe.

Machine learning algorithms grouped little red objects that were then sorted out through morphology, brightness, and color. By specifically separating some extreme combinations of color cuts, and splitting the object’s light into a rainbow of individual wavelengths through spectrographs, scientists could infer that the light in LRDs was very old coming from very far away, and that hydrogen gas was moving at incredibly high speeds in these objects.

The vast majority of LRDs have been dated between 600 million and 1.5 billion years after the Big Bang, and in about 70% of the analyzed LRDs, hydrogen gas was moving at incredibly high speeds—roughly 1,000 kilometers per second (about 2 million miles per hour) which can only be produced by gas spiraling into a supermassive black hole’s accretion disk. In addition, this discovery was also confirmed with older data from other observatories, together with a comparison with other stellar populations. Beautiful.

But why is everyone talking about it? 

Why black holes matter so much?

Well, first things first. Let us all agree that name-giving is not a strong part of physicists and astronomers – calling something we know so little about a part of a human anatomy we don’t like to talk about is already an indication. 

As weird as it seems, it is through the studies of black holes that science really comes to life. Science, empirical science, is built upon discoveries that are able to move human intelligence and technology further. Black holes are the ultimate test for fundamental physics, general relativity, the quantum gravity quest, galaxy formation, and cosmic expansion. Studying black holes isn’t just about understanding distant, exotic objects. It’s a direct path to unlocking the deepest laws of physics, understanding our cosmic origins, and potentially developing revolutionary future technologies. Black Holes sit the vanguard of intellectual thought. 

The kind of science the study of Black Holes is about, empirical science, does not need consensus to be accurate, and that is the beauty of it. Even if everyone doesn’t like the theory or think it does not make sense, that is when black holes, across the whole universe, shine. 

So Hurrahs to the brave scientists who are moving us to a better place. Let’s celebrate them through an universe timeline.

Around 13.800.000.000 years ago – The Big Bang
According to its latest definition, the Big Bang is the point in history where the observable universe can be verified to have entered into a regime where the laws of physics (as we understand them) can be applied. The Big Bang theory does not explain what was there before the universe, nor why the Big Bang occurred. 

10^-43 seconds after the Big Bang 
temperature and average energies were so high that matter (particles) could not form. The 4 fundamental forces that shape the universe – gravity, electromagnetism, the weak nuclear force, and the strong nuclear force – were combined and formed one fundamental force.

Before 10^-32 seconds after the Big Bang
A phenomenon called inflation occurred – the universe suddenly, very rapidly, and exponentially expanded (from something like half of a DNA molecule in length to 100 trillion kilometers long in a tiny fraction of a second).

About 10⁻³⁰ seconds after the Big Bang
The universe was filled with a radiation/light/field that lasted 380.000 years. This phenomenon, called the cosmic microwave background radiation, has been streaming throughout the universe since. Even though scientists are still figuring out what exactly cosmic microwave background radiation is, the images apparently capture the fundamental building block of nature – the quantum field. 

Around 10^-12 after the Big Bang
The quantum field of gravity, the quantum electrodynamics (electromagnetic force), the gluon field (strong nuclear force), and the W and Z boson field (weak nuclear force) were able to take their present forms. 

1 second after the Big Bang
The quantum fields of matter bedrocks of the universe – the neutrino, the electron, the up quark, and the down quark- were already formed (there are 12 known quantum fields of matter today, of which 8 of them are “heavier” variations of the 4 bedrock ones). 

1 minute after the Big Bang 
The universe had atoms of the lightest and simplest element – hydrogen.

2 minutes after the Big Bang
Pressure and temperature were still too high in the universe, enabling a reaction called nuclear fusion to take place. With nuclear fusion, hydrogen atoms quickly fuse to form helium (the second-lightest element). 

After 20 minutes following the Big Bang
pressure and temperature drop to a point where nuclear fusion ends, leaving the universe with an initial composition of 75% hydrogen and 25% helium (and tiny proportions of other elements). 

No earlier than 150.000.000 years after the Big Bang
ignition of the first stars. 

From 600.000.000 to 1.800,000,000 years after the Big Bang
LRDs – Little Red Dots – Massive black holes

Overcoming a five-century design deadlock to save the reading experience

Perhaps we don’t need more willpower to read more books. By exploring the history and context of book design, we can actually decode the path to enhance the human reading experience.

Books are responsible for a massive part of human development and an active determinant in human history. 

By documenting human knowledge across the most diverse fields, books have been a technology that, for centuries, has shaped minds and civilizations through a silent conversation across time and space, becoming a pivotal human event in cognition and communication.

The 550-Year-Old Blueprint

Books – the paper-printed, page-bounded objects that demand both human hands to hold and are preferably read in a sitting position – started to be manufactured about 550 years ago. 

Its design was an engineering revolution in its time, featuring a movable-type system and a press that enabled the mass production of printed goods. Compared to scrolls, books were way better (they were more portable and durable) thanks to their bound pages, which allowed non-linear access via pagination.

Pagination, in turn, allowed books to display their references and sources at their ends, creating an intricate system of small symbols, numbers, and letters for the reader to navigate.

Despite its design choices being pragmatic solutions to the constraints of technology and materials at the time, regarding their purposes,

Books were initially developed with the (almost exclusive) objective of educating human males, targeting their behaviour, concerns, minds, and bodies

Because the very experience of reading a book was a luxury that very few in human societies worldwide could afford, books were assigned, since their birth, with a status of charm, wisdom, and exclusivity – they rapidly became symbols of wealth, knowledge, learning, and intellect. 

Probably because of this initial association with superiority and wisdom, the book as an object—considering both its design and content—has remained largely unquestioned and unchallenged since its initial launch.

The Contemporary Ergonomic Shift

However, the fact that more humans (like females) have been granted the privilege of reading and learning from books, especially over the past 100 years, combined with digital devices that have revolutionized access to knowledge over the past 20 years, makes now the perfect time to rethink the book design so it can suit the minds, bodies, and social concerns of the contemporary human.

Considering that reading experiences are intended to reach all humans, printed publications in general should be lightweight and easy to hold with one hand (like digital devices), with a single-page flip. This format allows immersive reading in any position (lying down, sitting, standing) without any physical discomfort.

The Spatial Landscape of the Page

Today, it is known that while reading a book, humans absorb not only the meaning of the words but also their spatial distribution – a form of spatial memory. This means humans are involuntarily recording the position of the text on a page – whether it is on the right or left side of the book, or at the top, middle, or bottom of the page. 

To address and enhance this human skill, the single-page flip could use a page layout that displays elements for navigation, such as titles, chapters, subtitles, page numbers, and so forth, as well as keywords related to the text, which make use of and reinforce the human spatial memory. 

Furthermore, books today still adopt the confusing and uncomfortable way of displaying references and sources established a long time ago, forcing the reader to navigate a labyrinth of small fonts to access (often trivial) information.

This old system still treats supplementary information as an optional appendage rather than an integral part of the intellectual journey

This way of displaying references and sources is merely an outdated convention, not a scientific method. 

Instead, references and sources should be a valuable asset, displayed comfortably on the same page as the content they relate to, making the reading experience easy and fluid.

Redesigning the Experience

Because reading is (still) one of the most efficient ways humans can learn, reading devices must adapt their purposes and fulfill their functions. 

Perhaps what is needed for humans to read more is not willpower, but simple design adaptation, both in their physical design as objects and in the display of their content.

Reading is not just an act of willpower; it is an experience shaped by design

Quietly decoding written words and being taken by its loud silence is one of the most transformative and fulfilling human experiences. And it can definitely be an even more efficient, comfortable, and pleasant one. 

Contemporary cultures worldwide tend to view farming as one of the pillars of human advancement—a sudden, 10,000-year-old shift in the human evolutionary journey that dragged us from a chaotic, hand-to-mouth existence as “hunter-gatherers” into the enlightened era of modern agricultural industry. It is an appealing, convincing, linear narrative. Yet, empirical evidence tells a different story.

According to contemporary fossil and archaeological records, ancient human populations dating back up to 3,300,000 years ago (yes, more than 3 million years ago) were actively managing and cultivating vast territories. They utilized complex, integrated landscape engineering combined with sophisticated tool manufacturing and use to create subsistence environments, primarily through agroforestry and sustainable land management techniques. 

Furthermore, despite those ancient human populations being way smaller than today, the area they needed to manage in order to reproduce and survive was far larger than the agricultural zones we currently use. 

Alongside this, the physical evidence also suggests that humans have always been settlers. Several archaeological sites feature findings spanning millennia in the exact same location, indicating that multiple generations inhabited the same area for thousands of years.

So, if the empirical data states that humans have always been farmers and settlers, what actually happened 10,000 years ago?

Well, the records show that 10,000 years ago wasn’t the sudden start of farming, but rather the peak of a process that had already been underway for at least 40,000 years – domestication. 

Domestication is a phenomenon that deeply alters the biology, lifespan, reproduction, and behavior of all the diverse species involved in it. In the case of humans, it is the force that shifted our behavior away from autonomous environmental integration and regulation toward a rigid compliance with the very species we were managing (and being managed by). 

Especially through mono-culture farming, domestication allowed the human population to grow exponentially, survive, and thrive on the Earth’s surface over the last 10,000 years.

The caveat of domestication is that, evolutionary speaking, it is a process that happens too fast. The biology of the species involved rarely keeps up with the pace; while their reproductive rates scale exponentially, their survival rates and individual longevity often decrease. 

Specifically in humans, domestication has historically taken a heavy toll on overall health and longevity—a trend that only began to reverse over the last 50 years as global life expectancy started to rise.

However, we do not need to wait generations for evolutionary biology to catch up. Given the technology and resources available today, learning from ancient land management offers a fast track to optimizing modern human well-being and longevity. 

By applying farming methods that are inherently more aligned with human biology through automated, high-yield food production right into our cities, we can integrate and optimize our direct biome. Thus, integration with nature becomes a matter of technology and spatial design. 

Furthermore, by utilizing a global digital network to share cultivation data and ecological blueprints, modern communities can increase production and adapt these hyper-localized food systems to their geographical needs.

In order to heal our bond with the ecosystems around us, we don’t need to abandon the future— we just need to design it better. 

We can finally build a sustainable lifestyle that feels entirely native to us—one where we design environments and spaces that don’t just shelter our bodies, but actually support our biology.

For twenty years, the tech industry has told us that digital reading is “liberating.” But as we move between our phones, tablets, and laptops, we’ve ignored a frustrating reality: the digital page is a shape-shifter that sabotages our concentration.

In the traditional publishing world, digital versions (EPUBs) are treated as “liquid” data. They are designed to pour into any screen like water. It sounds convenient, but for the human brain—an organ that evolved to map information spatially—it’s a cognitive disaster.

The Science of “Where”

Cognitive scientists have long known that humans don’t just read words; we map them. We remember an idea because it was “on the top left of the page, near that diagram.” When a digital file “re-flows” the text, it deletes those landmarks; our brain is forced to restart its GPS every time we flip a screen.

The Architecture of the Screen

The structural instability of the “liquid” e-book has created a unique intellectual challenge: how to maintain deep focus in a medium designed to shift?

The solution lies in a return to spatial integrity—treating the digital page not as a fluid bucket of data, but as a fixed architectural environment. This requires a fundamental rethink of the digital interface, focusing on a few key cognitive shifts:

Restoring the Landmark

By anchoring the layout to defined pages, the brain’s natural “spatial GPS” functions again; when a specific keyword or diagram stays at the same coordinate on a phone as on a desktop, the information becomes a landmark rather than a moving target.

The Integrated Horizon

This stability is further reinforced by bringing references out of the “hidden” appendices and onto the active page. It eliminates the disjointed “scavenger hunt” for sources that has plagued book design since the 15th century, allowing the narrative and its evidence to exist on the same visual plane.

The Clickable Verify

Furthermore, the digital medium offers a level of transparency that paper cannot match. By treating every source as a clickable doorway, the narrative becomes a verifiable circuit. The reader is no longer asked to simply “believe” the author; the interface provides the keys to verify the empirical data in real-time.

All these cognitive shifts are the core philosophy behind the Reading Room at Resignify Narratives. By moving away from the industry standard of “reflowable” text, the digital edition ceases to be a secondary backup of the paper book. Instead, it becomes a distinct architectural tool built specifically for the screen.

Digital reading shouldn’t be a “lesser” version of the physical experience.
It should be more precise, more connected, and more memorable.