Chapter One The Past Is Connected to the Now

Nothing exists in isolation. Everything today is a continuation of the past

 

as well as an indication of the future; everything around us is impacted by

distant things, and in turn influences other things in the distance. In order

to answer questions about mankind and human society, one must first

understand humanity and human history itself, as well as the environment in

which humans survive.

Section One: The Pursuit of Truth

In the thousands of years of recorded human civilization, truth is often mistaken

as fallacy, while fallacies are often regarded as sacred and inviolable

truths. The birth of a revolutionary truth must always weather a ruthless and

bloody storm of opposition: that has been the universal law throughout time.

Many scientific conclusions have led to tragic persecution and brutal

combat in the long course of history, but truth always wins out in the end.

Through the endurance of time, fact will always shine through the layers of

absurdity and make its brilliance known universally.

The path to truth is often filled with hardship. Three such examples are

introduced below.

One: The Story of Earth’s Relation to the Universe

Since the beginning of time, humans have been preoccupied with understanding

the earth we live on and the universe surrounding it. Due to the

limitations of the known world, for thousands of years after entering civilized

society, humans could only rely on their intuition and imagination to observe

the sun, moon, stars, earth, and sky and attempt an understanding of the

earth and universe.

Geocentric” was a cosmology ical doctrine established in ancient Europe;

it was first proposed by the third-century BC ancient Greek philosopher

Aristotle. He theorized that the earth was the center of the universe, with

the moon, stars, and all cosmic matter orbiting around it. Aristotle was a

master of ancient Greek philosophy and a teacher to the famous Macedonian

king, Alexander the Great. His lofty status and seemingly reasonable explanation

might have been the reason this wrong theory dominated the Western

world for more than a thousand years. It is often through a series of “developments,”

misinterpretations, and accidental applications that falsehoods gain

and cement their dominance in the world.

The astronomer Ptolemy further developed and improved upon the

geocentric theory. He believed that Earth was located in the center of the

universe, with the moon, Mercury, Venus, the sun, Mars, Jupiter, and Saturn

ranging around it in successive order. According to him, these planets all

orbited the earth within their own trajectory at regular intervals.

All of the above views regarding the earth and its relation to the universe

fall within the realm or normal academia. According to the general

principles of scientific research, as long as there is sufficient basis, a new

correct scientific conclusion can overturn a previous wrong one without

much difficulty; however, once a scientific theory is deliberately exploited by

the dominant religious or political authorities, the situation becomes much

more complicated.

Christian doctrine took up the incorrect geocentric theory. According to

Christianity, God created Earth and the universe. The earth was the center of

the universe, and everything in the universe, including mankind, was created

by God. During the dark medieval times, Christianity firmly imprisoned

people’s belief systems, not allowing any doubt or rebellion against predetermined

Christian ideology. This allowed the geocentric theory to dominate

cosmology virtually unchallenged.

The first person to offer substantive challenge to the geocentric theory was

Copernicus. Nicholas Copernicus was born in Torun, Poland, on February

19, 1473. He studied law, medicine, and theology at university, but his

interests lay in astronomy. In his spare time, Copernicus would observe and

study astronomy. Coupled with his reflections on the universe, he proposed

the heliocentric theory and dedicated his life to completing the astronomical

masterpiece, On the Revolutions of the Heavenly Spheres. This work stated that

Earth was not the center of the universe but just an ordinary planet. The

center of the universe was the sun, followed by Mercury, Venus, Earth, Mars,

Jupiter, and Saturn, in that order.

Today, we can see that Copernicus’ argument is not the ultimate truth

either, but it was a crucial first step on the path to truth and a complete

denial of the geocentric theory. More importantly, the heliocentric theory’s

denial of geocentric theory would move beyond an astronomical debate to

evolve into a challenge of Christian religious theology. The revolutionary

consequences inspired by the heliocentric theory would trigger a chain reaction

across a series of other fields. This was absolutely unacceptable to the

Christian church.

On the Revolutions of the Heavenly Spheres was published after Copernicus

had been bedridden by a stroke. With trembling hands, he caressed this masterpiece

for which he’d struggled his whole life, and he died not long after.

It was the genius, atheist, Italian philosopher Giordano Bruno who developed

Copernicus’ theory. Bruno was not an astronomer; he used his own

philosophical speculations to propose the idea of an infinite universe, further

developing the Copernicus theory. Bruno believed that the sun was not static

but constantly moving, and that the sun was not the center of the universe

either. He believed that there were an infinite number of worlds outside the

solar system, and the universe—being unified, material, and infinite—could

not have a center.

Bruno’s ideas infuriated the Catholic Church, and the inquisition held a

seven-year interrogation against him. Bruno was indomitable and insistent

upon the truth, even in prison; he was ultimately sentenced to death by

burning. On February 17, 1600, Bruno was burned at the stake in Rome’s

Campo de’ Fiori.

Brutality, bloodshed, and violence can never stop people’s pursuit of

truth, as evidenced by one of the most outstanding pioneers of modern

science: Galileo. Through astronomical observation, Galileo concurred with

the Copernicus theory and published the book Dialogue Concerning the Two

Chief World Systems in 1632. This book was soon banned by the Roman

Catholic Church. Galileo himself was tried in Rome and sentenced to life

imprisonment in 1633.

The period in which Bruno and Galileo were sentenced by the church was

the darkness before the dawn for Europe. The fourteenth-century Renaissance

movement, originating in Italy, sought to organize ancient Greek and Roman

works as cultural weapons against religious theology. The movement took up

a human-centered humanism ideology to confront the God-centered religious

ideology, opening the way for modern ideological liberation.

It was the dedication in the pursuit of truth and fearless sacrifice for righteousness

demonstrated by men like Copernicus, Bruno, and Galileo that

woke the dawn of the new world. From the seventeenth to the eighteenth

century, the Western Enlightenment movement started in Britain and France

and expanded to Germany, the Netherlands, and many other countries. The

Enlightenment movement used rationalism as an ideological weapon, with

its spearhead directly pointed towards feudal autocratic rule and religious

theology. It opposed religious superstition in favor of promoting the spirit

of science and opposed authoritarian dictatorship in favor of democracy

and freedom. The Enlightenment movement even advocated for a rational

society free from religion—a secularization of human life. It was the effort

of Enlightenment thinkers that uncovered the path to science and reason

for all humanity and removed the shackles of religion from the pursuit of

truth once and for all. And then there was the American Revolution and the

French revolution . . . and so scientific research suddenly saw the light.

It was the power of truth that drove the world to momentous change.

Two: The Story of Earth

The earth is home to man. Our ancestors hunted, gathered, and farmed here

day in, day out. It is Earth—the home our survival depends upon—that

provides a habitat for humanity within the vastness of the universe. And thus

humanity has endured from the beginning of time until today, evolving from

apes to Homo sapiens, from barbarism into civilization.

However, the surface of the earth we live on is far from fixed and eternal;

it consists of separate plates that constantly drift and change. From the formation

of the earth until this day, this surface has undergone much change.

About two hundred million years ago, Earth was one supercontinent encompassing

all lands. What is today the east coast of South America was connected

to the west of Africa; North America was adjoined to the west of the

Eurasian continent; Australian was a peninsula off the east of Antarctica; the

Indian subcontinent was all the way in Antarctic, thousands of miles away

from Southwest China; and China’s Tibet was bordered by vast seas. This was

not the first time a supercontinent existed on Earth. Another supercontinent

had formed about seven hundred million years ago, but the shapes and locations

of the landmasses varied.

The landmasses on Earth have been separating and uniting throughout

time. Just as brothers who must go their separate ways once the time comes,

this supercontinent finally broke apart, the landmasses starting their separate

journeys, two hundred million years ago. The Americas drifted westward,

away from Europe and Africa, while the Indian subcontinent broke off from

the Antarctic continent and traveled north until it bumped into eastwarddrifting

Asia, forming the magnificent Himalayas in the process. Australia

left Antarctica shortly after the Indian subcontinent and traveled north, and

it maintains a northward voyage until this day.

Today, the Americas continue to drift westward with the Atlantic Ocean,

expanding at a rate of one to four centimeters per year. In fifty million years,

the Atlantic will have widened by more than one thousand kilometers. At the

same time, the Asian continent is drifting eastward and the Indian Ocean

is also enlarging. Under attack on both the east and west side, the Pacific

is becoming narrower; eventually, it will no longer be the largest ocean in

the world.

As the African continent continues to move north, the Mediterranean

will become an inner lake and eventually disappear. The stubborn Indian

continent will remain firmly pressed against Asia, causing the Himalayas to

rise at a rate of one to five centimeters a year. In some tens of thousands

of years, Mount Everest will be more than ten thousand meters in height,

further cementing it as the world’s highest peak.

After swallowing the Mediterranean, the African continent will continue

its “northern expedition,” eventually hitting Europe and creating a tall uplift

along the African-European continental margin. The Alps will gain in height

as well; however, the African continent itself will face large internal divisions.

The Great Rift Valley will rupture completely, East Africa will begin an eastward

drift, and a new ocean will be produced.

This almost fairytale-esque story is the theory of plate tectonics, which

originated from the continental drift theory proposed by German scientist

Alfred Wegener. In 1910, when Wegener was lying in bed sick, he was

inspired by the world map in front of him. He was fascinated by the similarity

of the landmasses on the two sides of the Atlantic, as the protrusion on one

side perfectly fit into the concave of the opposite side. With such consistency

in shape, could it have been possible that these two continents were once

connected? With this idea in mind, Wegener began a series of studies. He

not only conducted comparative studies of the continental strata on the two

sides of the Atlantic, but he also researched the consistency of African and

Brazilian paleontology, eventually producing the theory of continental drift.

Wegener’s theory was almost unanimously opposed by geophysicist everywhere.

People laughed at his “great poetical dream” and regarded him as an

ignorant grandstander lacking basic knowledge of Earth science. Wegener’s

ideas were deemed to be simply ridiculous and completely unjustified.

Wegener was extremely marginalized and shunned in academia; this exclusion

and contempt even affected the small number of people who expressed

recognition or sympathy to his theory. During that time in the United States,

you could not become a university professor if you subscribed to the theory

of continental drift, and you would also face endless irony and disdain. In

such an environment, even those who wholeheartedly supported continental

drift theory could not express it out loud—this was a rare phenomenon in the

United States, where democracy and freedom were such important values.

For a long time, the theory of isostasy held dominance in geology circles.

It theorized that the earth’s crust moved in an equilibrium of alternating

rising and sinking movements that relied mainly on vertical movement and

only minimally on horizontal movements. Therefore, the continental drift

movement was undoubtedly a fundamental negation of isostasy theory,

openly challenging existing geological theories and authorities.

Wegener was alone in his battle; even his famous meteorologist father-inlaw

held continental drift theory to be mere caprice. But Wegener persisted in

his academic beliefs and was committed to proving continental drift theory

in every way possible.

In 1930, the fifty-year-old Wegener met a tragic death in Greenland while

attempting to find further evidence to support his theory. The continental

drift theory faded into obscurity along with its founder.

It was only in the 1950s that breakthroughs in paleomagnetism research

finally validated his theory. When magma goes from hot to cool in its solidification

process, it gains magnetism from the earth’s magnetic fields. Rocks

from different times magnetize in the same direction. Since rocks can be

dated, the magnetization direction of rocks across different time periods can

also be determined; thus, the different locations of different regions at different

times can be determined as well.

In the 1960s, scientists conducted differential research into seabed rocks

and terrestrial rocks in conjunction with research into submarine magnetic

anomalies, eventually finding evidence of subsea expansion. Wegener’s continental

theory finally became recognized as truth instead of “absurd heresy.”

Both Wegener and his theory were vindicated in the academic community.

Scientists established the theory of plate tectonics based on Wegener’s theory,

marking a geological revolution and the advent of a new era in Earth science.

Three: The Story of the Origin of Humanity

When it comes to the origin of humanity, almost every nation has developed

its own interpretation over time. Most of these explanations state that

humans are created by deities and are accompanied by numerous folktales

and legends. When the “God created man” story became a theological doctrine

of the prevalent religious power, however, it became uncontestable, as

any challenge to theological doctrine in a religion-centric world could mean

imprisonment, or even death.

British naturalist Charles Darwin and biologist Alfred Russel Wallace

were both revolutionary figures in the impetus to overthrow the “God created

man” ideology. Darwin in particular cast unprecedented doubt on the creation

theory through his detailed research and rigorous scientific analysis.

In 1831, the British Navy ship Beagle was set to embark on a scientific

investigation of South America. Its main task was to conduct hydrological

mapping of the east and west coast and islands of South America, as well

as record a time for completing an around-the-world voyage. The ship was

missing a naturalist with geophysical knowledge, so Darwin was suggested

due to his interest in botany and geology, even though he was not a geologist.

This voyage took nearly five years, stopping at many places around the

world. While managing geological inspections and collecting data, Darwin

discovered many occurrences that contradicted the creation theory.

On the South American Pampas grasslands, Darwin often observed a

kind of bird that could not fly, called the rhea. These birds lived in environments

similar to that of African ostriches, but although rheas were similar in

body structure to ostriches, they were not identical. If God decided to create

these beings, wouldn’t one be enough? What point was there in repeating

the process?

What struck him as even more odd was his experience while investigating

the Galapagos Islands; each island had their own unique creatures. These

islands were very close to the South American continent, and the islands’

creatures were obviously different yet still clearly genetically related to the

creatures living in South America. Even among the islands, though each

island’s creatures were significantly different from each other, they still shared

obvious genetic traits. This phenomenon made it possible for people to

imagine that such creatures shared the same origin and developed differently

in diverse environments—so species were not necessarily immutable. This

ideology was undoubtedly incompatible with the “God created all things,

and all things are eternal” belief.

Upon arriving in Brazil, Darwin was mesmerized by the variety of plant

life, the beautiful leaves and flowers in the Brazilian forests. All this natural

splendor dazzled Darwin and caused him to question if God had really

created such diverse marvels one by one, all by himself.

After Darwin returned to the Britain, he started thinking in-depth about

his voyage and studying domestic animals, ultimately forming the concept

of evolution and publishing his far-reaching book, On the Origin of Species,

in 1859. In this book, Darwin systematically expounded on his theory of

evolution. He believed that all creatures were capable of evolving; some evolutions

were heritable, and some were not. Evolution was caused by changes

in the living environment and the use of organs; individuals evolved to better

suit the environment had better chances of surviving, and organs used more

were gradually developed. For example, wild ducks have stronger wings than

domesticated ducks because they fly more, while domesticated ducks have

stronger legs because they walk more.

Darwin believed that there was a surplus in nature, and that organisms

reproduced in far greater numbers than necessary for survival. Only those

individuals who evolved to best adapt to the environment survived and

produced offspring, while less suitably evolved individuals were eliminated.

Under natural conditions, evolution is a need for survival and reproduction.

Animals compete for food and mating opportunities, while plants compete

for sunshine and nutrients. They are all evolving through such competitions.

In Darwin’s mind, a primitive ancestor could produce a variety of species

each with their own traits. Different individual hybridizations and isolated

geographical environments all contribute to the formation of new species

and varied traits. All creatures within the same genus share a genetic connection,

just as different foliage on a tree connects to the same trunk.

Shortly after the publication of On the Origin of Species, Darwin’s follower,

Thomas Henry Huxley, published Man’s Place in Nature in 1863. In 1871,

Darwin published The Descent of Man, and Selection in Relation to Sex, in

which he enumerated many facts to scientifically prove that humans were

evolved from animals and shared “kinship” with animals, thus pointing out

man’s position in nature. Darwin’s assertion completely denied the religious

doctrine of “God created the world and man.” These two books once again

caused a sensation. They told people that there was no Creator, that the

world evolved according to its own laws, and that species evolved from other

species from one common ancestor, producing a variety of complex biological

species, including humans.

Darwin and Huxley’s arguments caused great waves and infuriated the

religious community. One debate on creation versus evolution went down

in history. On June 30, 1860, the British Association for the Advancement

of Science arranged a debate on creation versus evolution theory. Due to

physical discomfort, Darwin did not participate in this debate. Attending

on his behalf was staunch Darwinist and quick-thinker Huxley; on the other

side of the debate was eloquent Oxford Bishop Wilberforce, a man renowned

for his religious attainments. This debate is known in history as the “Oxford

Evolution Debate,” and it took place in the Oxford University Museum. The

sensitive nature of the theme attracted a large volume of listeners; the venue

was packed with over seven hundred attendees.

Wilberforce spoke first. Playing on the religious feelings of the people, he

carried out a deeply provocative attack: “Mr. Darwin would have us believe

that every animal, every reptile, every fish, plant, fly, and fungi descended

from the first living creature that could breathe. This is a blatant denial of the

will of God. Can we allow such betrayal of orthodox religion?” Wilberforce

quickly turned his glance to Huxley and asked, “Mr. Huxley, do you consider

yourself descended from an ape through your grandmother or your grandfather?”

This clearly humiliating provocation caused the audience to burst

into laughter.

After hearing Wilberforce’s speech, Huxley quickly realized that

Wilberforce did not know what evolution was, nor had he seriously read On

the Origin of Species. Huxley calmly stood up after the crowd had quieted and

spoke: “I have come to defend science, and I believe that no prejudice can

take away the prestige of my respected party.” He then plainly explained the

fundamentals of the theory of evolution, pointing out that this was the result

of twenty years of observation on Darwin’s part, not fabrication, and that it

reflected the objective laws of the biological world. Then Huxley said, “On

the question of humans originating from monkeys, it is not as superficial

and literal as the Bishop understands it to be; it just means that humans

are evolved from animals like monkeys.” After further illustrating Darwin’s

views in a more comprehensive manner, Huxley turned his head and started

straight at Wilberforce, replying, “[A] man has no reason to be ashamed of

having an ape for his grandfather. If there were an ancestor whom I should

feel shame in recalling, it would be a MAN, a man of restless and versatile

intellect, who, not content with a success in his own sphere of activity,

plunges into scientific questions with which he has no real acquaintance,

only to obscure them by an aimless rhetoric, and distract the attention of

his hearers from the real point at issue by eloquent digressions, and skilled

appeals to religious prejudice.” The audience responded with warm applause

to Huxley’s brilliant retort.

The Oxford Evolution Debate had great repercussions. It helped people

to clearly understand the absurdity of creationism and the scientific nature of

the Darwinian evolution theory. It was evolution that removed the shackles

of feudal theology from the field of natural science, allowing it to embark

upon a path of independent development. Simultaneously, the theory of

evolution further shook the rule of religion through obscurantism, liberating

people’s minds and defending the dignity of truth.

The pursuit of truth is a demanding process; it requires a certain spirit

and a type of courage. Daring to challenge traditional ideas, daring to contest

authority, daring to face persecution: these are all premises for the birth of a

revolutionary truth.

This book bases its research on the pursuit of truth and the respect for

reality. This author is determined to go forth undeterred, with no regrets or

fears, because he firmly believes that the conclusions of this book are fundamentally

related to the fate and future of humanity.

Section Two: The Beginning of the Universe

One: The Universe Started with “the Big Bang”

Nowadays, any ordinary person knows that the sun we rely on to survive is

just another ordinary star in the Milky Way, and that Earth is just another

planet of the sun. Before the 1920s, however, the horizon of astronomers was

confined to the Milky Way, as if the Milky Way was the entire galaxy. The first

person to discover galaxies outside of the Milky Way was American astronomer

Edwin Hubble. In 1925, he discovered the Andromeda Galaxy near the

Milky Way through astronomical observation, marking the first extragalactic

galaxy (i.e., a galaxy outside the Milky Way) observed by humans. In later

observations, Hubble found that there were far more than one or two galaxies

outside the Milky Way. Ten years after the discovery of the first extragalactic

galaxy, the scope of astronomical observation expanded to a range of five

hundred million light-years; that is the distance light travels (300,000 km per

second) in five hundred million years. At the time, this observation distance

seemed to be sufficiently large.

After observing numerous extragalactic galaxies, astronomers discovered

that almost all of them were moving away from us, and the further those galaxies

were, the faster they were moving away. For example, the Virgo Nebula

is moving away from us at a rate of 1,000 kilometers per second; to the

astronomers then, this was simply incredible.

Why are these galaxies moving away from us? Where does our universe

come from, and where is it heading? Many scientists have approached these

questions from different perspectives. In 1927, Belgian astronomer Georges

Lemaître suggested that all material of the universe could be traced back in

time to an originating single point; he called this point the “Cosmic Egg.”

When the Cosmic Egg suddenly exploded, the explosion material formed the

stars. Today, the Big Bang theory of cosmic formation is accepted by most

scientists, and this theory is being constantly perfected.

The universe was formed 13.8 billion years ago; of course, this is only

a rough estimate. Different scientists have varied understanding of this

number, but the differences are not significant. Therefore, it does not prevent

our discussion. This time can be confirmed in at least three ways. The first

method relies on the observation of galaxy retreat speed. If we rewind 13.8

billion years, the universe can be attributed to one originating point. The

second mode focuses on the study of the universe’s oldest stars and the star

clusters they form. Upon further inference, their ages are all close to 13.8

billion years. These are the first generation of stars formed in the universe.

The third approach is centered around the decay of atoms; it uses the law of

the atomic half-life to test the age of the oldest existing atoms.

The most common description humans use to describe cosmic origin

states that the universe began with a primitive atom. This atom was much

smaller than the atoms we refer to today; it had a diameter of only 10-33

centimeters, a high temperature, and large density. In specific numbers, this

atom has a temperature of 1032 K and a density of 1093 grams per cubic

centimeter. This primitive atom suddenly exploded 13.8 billion years ago.

The space it created through that explosion is the universe; the debris it produced

are the galaxies, stars, and various substances in the universe today.

However, the above description is not completely accurate. Our cosmology

today is based on general relativity and quantum mechanics. Based on

today’s scientific theory, we can trace the formation of the universe to 10-43

seconds after the Big Bang. This period is called the Planck time. The abovementioned

figures are the cosmic scale, temperature, and density at this time.

Using this state of time as the origin of the universe is actually very arbitrary;

since there had to have been a “zero-point” and a singularity point before this

time, we are merely unable to describe the universe before Planck time with

existing cosmic theory.

It is not easy to truly understand the description of the universe. It first

demands that we surrender our observation of the things around us and

adopt a completely different way of understanding everything in which we

exist and perceive constantly.

From a geometric point of view, a point is zero-dimensional, a line is onedimensional,

a surface is two-dimensional, and a cube is three-dimensional.

This is something we learn in junior high. We can easily imagine the shape

of a point, a line, a surface, or a cube. But space is four-dimensional; we can

perceive it, but we cannot imagine what it looks like. Of course, there will be

many people who do not agree with this argument. They might ask: Hasn’t

time always flowed naturally? Isn’t the universe the area we see? People have

these doubts because they are confused by their personal experiences.

According to existing understandings of cosmic theory, time and space

came into existence at the moment of the Big Bang 13.8 billion years ago,

and so time has flowed until the present and the universe has been constantly

expanding to this day. Surely someone will ask: Even if there was no matter or

life before the Big Bang, there must have been time . . . right? The answer is

no. Time started with the Big Bang; there was no time before that. If the Big

Bang created the galaxies and matter, surely there was empty space before the

Big Bang—how else did the debris from the Big Bang disperse? The answer

is once again no. Space came into being at the moment of the Big Bang; the

volume of space is determined by the volume of the universe’s expansion.

Someone might ask again: What is outside of the universe? What connects

to the edges of the universe? The answer is that the universe only has size; it

has no edge and does not touch anything. (There are scientists who believe

that there are other universes outside of our universe, but we cannot see them

since space is four-dimensional.)

When we observe the galaxy through a telescope, we discover that the

further away a galaxy is, the faster it is moving away from us—that is not to

say that we are the center of the universe. As a matter of fact, we would reach

the same conclusion observing the universe from any planet in any galaxy.

Just as when we blow balloons we might observe on any point on the balloon

that the further away a point is the faster it is moving away. Observations

made on any fixed point give the illusion that the observer is at the center. In

reality, every point is just an ordinary point.

The explosion 13.8 billion years created the epoch. At the beginning of

the Big Bang, the four natural forces we know today (strong interaction, weak

interaction, electromagnetism, and gravitation) were unified. As the universe

began to cool and expand, these four forces started to separate. At the same

time, the asymmetry between matter and antimatter began to appear; matter

outweighed antimatter by a tiny portion. These were the “Dark Ages” of

the universe; in this dark space, particles and antiparticles annihilated into

photons, producing energy. This annihilation included neutron-antineutron

annihilation, proton-antiproton annihilation, electron-positron annihilation,

and neutrino-antineutrino annihilation. Today, light fills the entire universe

mainly as a product of the early Big Bang period, while the matter that

remains from this large annihilation is our cosmic galaxy.

Three minutes after the Big Bang, the temperature of the universe fell to

one billion K. During this time, protons and neutrons combined to form

nuclei; this process lasted about an hour. When the universe’s temperature

dropped to one hundred million K, the nuclear synthesis ended. According

to theoretical calculations, among the products of the nuclear synthesis,

hydrogen accounts for ¾, helium takes up ¼, while tiny amounts of lithium,

beryllium, and boron account for less than one millionth of the whole. These

theoretical figures have received initial confirmation through astronomical

observations today.

During this time, the universe was full of photons, but it was not transparent

due to the large number of free electrons also existing in the universe.

These electrons blocked the path of photons. About thirty million years later,

the temperature of the universe had dropped to 3,000 K, electron movement

was less intense, and it was possible for hydrogen nuclei to capture one

electron and turn into hydrogen atoms, for helium nuclei to capture two

electrons and form helium atoms, and for lithium nuclei, beryllium nuclei,

and boron nuclei to all capture corresponding electrons and form atoms.

Without the electrons blocking their paths, photons were liberated and lit up

the universe, ending the Dark Age. Concurrently, the universe moved from a

radiation-based era to a matter-based era.

In the 1960s, while debugging the radio astronomical telescope, two

engineers at the Bell Labs—Arno Penzias and Robert Woodrow Wilson—

discovered that a very “cold light” occupied the universe sky. This “light”

encompassed every star and every galaxy, filling every corner of the universe.

It was not visible with optical telescopes but could only be observed through

radio telescopes; its corresponding temperature was 3 K. We know that 0 K

is absolute zero, measuring -273 C. This is the theoretical minimum temperature,

and 3 K is exactly the theoretical calculation of the temperature of

waste heat produced by the Big Bang. That cold light that filled the universe

is the original light remnant of the Big Bang; it is the remains of the photons

from the Dark Age of the universe. Since 13.8 billion years have passed and

the universe has undergone a great expansion, the initial photons are now

scattered throughout the universe and have become very sparse. Only a few

hundred photons exist in every cubic centimeter, which equates to 3 K in

temperature. Evenly spread across the entire universe, this light is called

Cosmic Microwave Background Radiation.” These two engineers’ accidental

discovery proved to be the most powerful proof for the Big Bang Theory, and

the two were awarded the Nobel Prize in Physics in 1978 for that reason.

At the same time the universe was expanding from the massive force of

the Big Bang, atoms were being brought together by gravitational force to

form huge clouds. Two hundred million years after the Big Bang, these atom

clouds had finally been compressed tightly enough so that stars could be

born. At this time, the universal temperature—that is, background radiation—

had dropped to 30 K. The universe’s sky had changed from the earlier

yellow and red to the darkness we see today, with dots of stars twinkling in

the distance. Galaxies began to form as well; 13.8 billion years after the Big

Bang, the universe is still continuing its outward expansion.

Two: The Universe and the Milky Way

There is no question that the Milky Way is also a product of the Big Bang, yet

unlike the cosmic Big Bang theory, there is no consistent view regarding the

formation of the Milky Way. The general belief is that a large cloud of atomic

gas gathered due to gravitational force and formed a relatively enclosed and

independent space shortly after the universe was created. Under gravitational

force, a number of smaller enclosed and independent air masses formed

within this large enclosed air mass; these smaller air masses became more

and more dense, and their internal temperatures rose higher and higher.

About two hundred million years after the universe formed, they ignited

their own hydrogen nuclei one by one, producing enough heat to set the air

masses aflame and form the first generation of stars. That original gas cloud

encompassing hundreds of millions of stars evolved into one giant galaxy: the

Milky Way.

According to research today, the Milky Way is a barred spiral galaxy

comprised of a large number of stars. Some people compare it to the discs

athletes throw, since it is also round, thin, and convex in the center. Along

the diameter of this “disk,” we call the center the Galactic Center, and the

convex part surrounding the center the Galactic Bulge, with the galactic disk

and halo ranging around it.

The Galactic Center of the Milky Way is flat and spherical in shape,

measuring 16,000 light-years in diameter and about 13,000 light-years in

thickness. It is densely populated by stars and is filled with dense interstellar

matter and nebula. According to observation, there is a supermassive black

hole in the nucleus area, supported by the existence of strong cosmic ray

radiation, which is evidence of black hole phagocytosis.

The area around the center is semi-densely populated by stars and called

the galactic disk; it measures 100,000 light-years in diameter, with a thickness

of about 3,000–6,000 light-years. It is thicker near the center and thinner

around the edge. The spherical shape surrounding the galactic disk is called

the halo; it is about 100,000 light-years in diameter and is sparsely populated

with stars, most of which are older and mineral-weak. Within the halo, some

stars have aged to the last period of their star-life, and some of the larger

ones even scatter their heavier elements through supernova explosion. These

scattered elements land on the disk and become the “material” that form new

star systems.

The galactic disk has a spiral arm structure that extends from the inside

out, approximately symmetrical to the Galactic Center. The spiral arm contains

more young, bright, metal-rich stars with denser galaxy dust, and it is

also where stars are born. The Milky Way galactic disk has four spiral arms:

the Norma and Cygnus arm, the Sagittarius arm, the Scutum-Crux arm, and

the Perseus arm. At present, our solar system is located in the Orion arm,

which is a minor spiral arm. The sun is 27,000 light-years away from the

Galactic Center and slants about twenty-six light-years north off the surface

plate; it revolves around the Galactic Center at a rate of 220 kilometers

per second. Even at such high speed, one full rotation around the Galactic

Center takes approximately 250 million years; thus, we call 250 million years

one galactic year.

When we observe the sky with the naked eye, we cannot see the spiral

nebula of the Milky Way, nor the spiral arm structures. In a clear summer

night sky, all we can see is a bright river of stars stretched across the sky. This

is because we are situated in the galactic disk and can only observe a side

view of the Milky Way, so it will always look ribbon-shaped to us. There is a

brighter, denser area near Sagittarius—that is the nucleus of the Milky Way.

In gross estimation, there are about two hundred billion stars in the Milky

Way (some scientists believe the number to be much higher—as much as two

thousand billion galaxies) and around 300 billion galaxies in the universe.

This is an extremely vast number. With so many stars and galaxies out there,

it is hum