The Last Hours of Ancient Sunlight: Revised and Updated Third Edition The Fate of the World and What We Can Do Before It's Too Late

by Hartmann, Thom; Walsch, Neale Donald

• ISBN13: 9781400051571
• ISBN10: 1400051576
• eBook ISBN(s): 9780307422132
• Additional ISBN(s): 9780609805299
• Edition: Revised
• Format: Paperback
• Copyright: 2004-04-27
• Publisher: Harmony
• More Book Details
• Purchase Benefits

Summary

While everything appears to be collapsing around us -- ecodamage, genetic engineering, virulent diseases, the end of cheap oil, water shortages, global famine, wars -- we can still do something about it and create a world that will work for us and for our children's children. The inspiration for Leonardo DiCaprio's web movie Global Warning, The Last Hours of Ancient Sunlight details what is happening to our planet, the reasons for our culture's blind behavior, and how we can fix the problem. Thom Hartmann's comprehensive book, originally published in 1998, has become one of the fundamental handbooks of the environmental activist movement. Now, with fresh, updated material and a focus on political activism and its effect on corporate behavior, The Last Hours of Ancient Sunlight helps us understand--and heal--our relationship to the world, to each other, and to our natural resources. From the Trade Paperback edition.

Author Biography

Thom Hartmann is an award-winning author, international lecturer, teacher, and psychotherapist. His books have been written about in Time magazine, he has been on the front page of the Wall Street Journal, and he has been featured as a guest on numerous radio and TV shows, including NPR's "All Things Considered," CNN, and BBC. A former journalist, editor, and occasional woodsplitter, he lives in Vermont with his wife, Louise.

Table of Contents

Foreword
Introduction
We're running out of ancient sunlight	p. 5
We're made out of sunlight	p. 7
How can things look so good yet be so bad?	p. 20
Slavery and freedom	p. 32
Glimpsing a possible future in Haiti and other hot spots	p. 36
The death of the trees	p. 42
Extinctions : diversity supports survival	p. 51
Climate changes	p. 60
A visit to a country that's planning how to survive : China	p. 84
The last hours of (cheap, clean) water	p. 91
Deforesting, fighting for fuel, and the rise and fall of empires	p. 106
Younger and older cultures : how did we get here?	p. 117
The power of our point of view : older and younger cultures	p. 119
Younger culture drugs of control	p. 124
Younger culture stories about how things are	p. 139
What we need to remember	p. 165
The lives of ancient people	p. 186
Power vs. cooperation in social structure : the city-state vs. tribes	p. 192
The robots take over	p. 215
But what about Darwin? Isn't the victor right?	p. 222
What can we do about it?	p. 229
The new science	p. 233
New stories are necessary to change the world	p. 248
Touching the sacred	p. 253
Learn to create awareness	p. 259
Lessons from a monk	p. 264
Re-empower women	p. 271
The secret of "enough"	p. 273
Respect other cultures and communities	p. 279
Renounce the destruction of life	p. 280
Look into the face of God	p. 289
Change the focus of how we use technology	p. 292
Turn off the TV	p. 300
The modern-day tribe : intentional community	p. 304
Reinventing our daily life and rituals	p. 321
Transforming culture through politics	p. 329
Taking back America	p. 338
Something will save us	p. 344
We have much to learn ... and even more to remember	p. 354
Afterword	p. 357
Notes	p. 359
Recommended reading	p. 366
Acknowledgments	p. 369
Index	p. 371
Table of Contents provided by Blackwell. All Rights Reserved.

Excerpts

We're Running Out of Ancient Sunlight
Where our energy came from, how we're "living beyond our means," and what will happen to our children when we run out

It all starts with sunlight.

Sunlight pours energy on the Earth, and the energy gets converted from one form to another, in an endless cycle of life, death, and renewal. Some of the sunlight got stored underground, which has provided us with a tremendous "savings account" of energy on which we can draw. Our civilization has developed a vast thirst for this energy, as we've built billions and billions of machines large and small that all depend on fuel and electricity.

But our savings are running low, which will most likely make for some very hard times.

In Part I we'll lay out the situation as a foundation for planning our response. Topics in Part I include:


*The history of sunlight in the human story

*How can things look okay yet be so bad?

*The importance of trees--their three vital roles in a renewable environment, and some alarming statistics on what's happening as we cut them down

*The accelerating rate of species extinction as we alter the world and its climate


Let's start at the beginning, with the fuel source that gave life to this planet millions of years ago: sunlight.

We're Made Out of Sunlight

The Sun, the hearth of affection and life, pours burning love on the delighted earth.
--Arthur Rimbaud (1854-1891)

In a very real sense, we're all made out of sunlight.

Sunlight radiating heat, visible light, and ultraviolet light is the source of almost all life on Earth. Everything you see alive around you is there because a plant somewhere was able to capture sunlight and store it. All animals live from these plants, whether directly (as with herbivores) or indirectly (as with carnivores, which eat the herbivores). This is true of mammals, insects, birds, amphibians, reptiles, and bacteria . . . everything living. Every life-form on the surface of this planet is here because a plant was able to gather sunlight and store it, and something else was able to eat that plant and take that sunlight energy in to power its body.

In this way, the abundance or lack of abundance of our human food supply was, until the past few hundred years, largely determined by how much sunlight hit the ground. And for all non-human life- forms on the planet, this is still the case--you can see that many of the areas around the equator that are bathed in sunlight are Wlled with plant and animal life, whereas in the relatively sun-starved polar regions, where sunlight comes in at a thinned-out angle instead of straight-on, there are far fewer living creatures and less diversity among them.

The plant kingdom's method of sunlight storage is quite straightforward. Our atmosphere has billions of tons of carbon in it, most in the form of the gas carbon dioxide, or CO(2). Plants "inhale" this CO(2), and use the energy of sunlight to drive a chemical reaction called photosynthesis in their leaves, which breaks the two atoms of oxygen free from the carbon, producing free carbon (C) and oxygen (O(tm)). The carbon is then used by the plant to manufacture carbohydrates like cellulose and almost all other plant matter--roots, stems, leaves, fruits, and nuts--and the oxygen is "exhaled" as a waste gas by the plant.

Many people I've met believe that plants are made up of soil--that the tree outside your house, for example, is mostly made from the soil in which it grew. That's a common mistake. That tree is mostly made up of one of the gases in our air (carbon dioxide) and water (hydrogen and oxygen). Trees are solidified air and sunlight.

Here's how it works: plant leaves capture sunlight and use that energy to extract carbon as carbon dioxide from the air, combine it with oxygen and hydrogen from water, to form sugars and other complex carbohydrates (carbohydrates are also made of carbon, hydrogen, and oxygen) such as the cellulose that makes up most of the roots, leaves, and trunk.

When you burn wood, the "sunlight energy" is released in the form of light and heat (from the fire). Most of the carbon in the wood reverses the photosynthesis. The small pile of ash you're left with is all the minerals the huge tree had taken from the soil. Everything else was gas from the air: carbon, hydrogen, and oxygen.

Animals, including humans, cannot create tissues directly from sunlight, water, and air, as plants can. Thus the human population of the planet has always been limited by the amount of readily available plant food (and animals-that-eat-plants food). Because of this, from the dawn of humanity (estimated at 200,000 years ago) until about 40,000 years ago, the world probably never held more than about five million human inhabitants. That's fewer people worldwide than live in Detroit today.

I suspect the reason for this low global census is that people in that time ate only wild-growing food. If sunlight fell on a hundred acres of wild lands producing enough food to feed ten people--through edible fruits, vegetables, seeds, and wild animals that ate the plants--then the population density of that forest would stabilize at that level. Studies of all kinds of animal populations show that mammals--including humans--become less fertile and death rates increase when there is not enough food to sustain a local population. This is nature's population control system for every animal species.

Similarly, people's clothing and shelter back then were made out of plants and animal skins which themselves came to life because of "current sunlight," the sunlight that fell on the ground over the few years of their lives. We used the skins of animals and trees to construct clothing and housing.


Extracting more sunlight--from other animals


Something important happened sometime around 40,000 years ago: humans figured out a way to change the patterns of nature so we could get more sunlight/food than other species did. The human food supply was determined by how many deer or rabbits the local forest could support, or the number of edible plants that could be found or grown in good soil. But in areas where the soil was too poor for farming or forest, supporting only scrub brush and grasses, humans discovered that ruminant (grazing) animals like goats, sheep, and cows could eat those plants that we couldn't, and could therefore convert the daily sunlight captured by the scrub and wild plants on that "useless" land into animal flesh, which we could eat. So if we could increase the number of the ruminant animals through herding and domestication, then we could eat more of the recent sunlight they were consuming as grasses and plants. This provided to our ancestors more usable energy, both as work animals and as food animals. And so domestication and herding were born.


Extracting more sunlight--from the land

About this same time in history, we also figured out that we could replace inedible forests with edible crops. Instead of having a plot of land produce only enough food to feed ten people, that same land could now be worked to feed a hundred. The beginning of agriculture is referred to as the Agricultural Revolution, and it began to gather momentum about 10,000 years ago. Because we had discovered and begun to use these two methods (herding and agriculture) to more eficiently convert the sun's energy into human food, our food supply grew. Following the basic laws of nature, because there was more food, there could be more humans, and the human population started growing faster.

Within a few thousand years of that time we also discovered how to extract mineral ores from the Earth, to smelt pure metals from them, and to build tools from these metals. These tools, such as plows and scythes, made us much more productive farmers, so the period from 8,000 b.c. until around the time of Christ saw the human population of the world increase from 5 million people to 250 million people, a number just a bit smaller than the current population of the United States. But we were still only using about one year's worth of sunlight energy per year, and so even though we were eliminating some competing or food species, our impact on the planet remained minimal at worst. We weren't "dipping into our savings" to supply our needs, yet.

Then, as it happened, in the Middle Ages we discovered a new source of sunlight (which had been captured by plants nearly 400 million years ago) that Wt in nicely with our new theory that it was acceptable for humans to destroy our competitors for food, to convert all resources of the planet to the production of food for humans: coal, by replacing forests as a source of heat and thus freeing land for agriculture, could be used to increase our production of food.


When ancient sunlight got stored in the Earth


Around 400 million years ago, there was an era that scientists named the Carboniferous Period. Its name derives from the fact that at the beginning of this period there were huge amounts of carbon in the atmosphere in the form of carbon dioxide. Carbon dioxide is a "greenhouse gas," which holds the heat of the Sun against the Earth like the glass of a greenhouse, rather than letting it escape back out into space. During the Carboniferous Period, which lasted 70 million years and extended from 340 to 410 million years ago, there was so much carbon dioxide in the Earth's atmosphere that the temperature of the planet registered much higher than it does today.

The Earth is about 25 percent land and about 75 percent oceans and at that time the entire planet's land mass consisted of one huge continent, which geologists refer to as Pangaea. This continent existed long before the arrival of birds and mammals, even before the dinosaurs, and the only life-forms on the planet were plants, fish, insects, and small reptiles. The high levels of carbon dioxide in the air both trapped sunlight energy as heat and provided copious carbon for the plants to use as raw material, so they grew abundantly. Almost all of Pangaea was covered with a dense mat of vegetation, rising hundreds of feet into the air, creating a thick ground cover of rotting and dead plant matter that became, in some places, hundreds or even thousands of feet deep. The mats of living and dead vegetation became thicker and thicker as this phase continued over 70 million years.

As the plants grew ever more lush, they trapped more and more of the carbon from the atmosphere (converting it into cellulose as leaves, stems, and roots), reducing levels of atmospheric carbon dioxide while retaining that carbon as plant material.

At the same time, the oceans, which cover three-quarters of the Earth's surface, were also home to huge quantities of plant matter, although much of this was of a simpler type, such as single-celled algae and other microscopic plants. These, too, captured the energy of the sun near the surface of the oceans. They used that energy to convert atmospheric carbon dioxide into plant-matter carbon, and then died and settled on the ocean floor.

Approximately 300 million years ago, a massive disaster occurred and created one of the five historical extinctions that have struck our planet. Nobody knows exactly why (a collision with a comet or asteroid is suspected), but a huge explosion of tectonic activity disassembled the continent of Pangaea and irrevocably changed the planetary environment. The Earth's crust was broken open in many places, volcanoes erupted, and continents crumbled and migrated. In those places where the land masses that were once parts of Pangaea collided with other parts of the former single continent, millions of acres of Earth were covered by mountains or other land. The thick vegetation mat sank underground.

Fifty million years later, the dinosaurs appeared, and another period of relative stability reigned on the Earth and what had become its two major continents, which geologists call Laurasia and Gonwanaland. The Triassic, Jurassic, and Cretaceous Periods (known, together, as the Mesozoic) came to an end 65 million years ago when, according to the most widely accepted scientific view, another meteor or asteroid struck the planet and extinguished the dinosaurs. During the Mesozoic Period, the planet moved into another period of geologic upheaval, and the continents of Laurasia and Gonwanaland broke into smaller parts, creating what we now call Asia, North America, South America, Europe, Australia, Africa, and Antarctica. Mountains were created as continents drifted into each other, and some of the plant matter traveled even deeper into the earth, where it was subjected to great pressure.


Using ancient sunlight

About 900 years ago, humans in Europe and Asia discovered coal below the surface of the Earth and began to burn it. This coal was the surface of most of the ancient mats of vegetation--this 300-million-year-old stored sunlight--and by burning it humans were, for the First time, able to use sunlight energy that had been stored in the distant past. Before this, our ancestors had to maintain a certain acreage of forestland because they needed the wood for heat to survive the cold winters in the northern climates. Forests captured the "current sunlight" energy, and they could liberate that captured sunlight in a fireplace or stove to warm a home, cave, or tipi during the long dark days of winter.

The exploitation of coal, however, reduced their reliance on current sunlight, allowing them to cut more forestland and convert it into cropland, since they no longer were absolutely dependent on the trees for heat. By making more croplands available, they were able to produce more food for more humans, and the population of the world went from 500 million people around the year 1000 to the First billion living humans in 1800.

This represents a critical moment in human history, for this is when our ancestors started living off our planet's sunlight savings.

Because our ancestors could consume sunlight that had been stored by plants millions of years ago, they began for the first time to consume more resources--in food, heat, and other materials--than the daily amount of sunlight falling locally on our planet had historically been able to provide. The planet's human population grew beyond the level that the Earth could sustain if humans were using only local "current sunlight" as an energy and food source.

This meant that if our ancestors' supply of coal had run out, they'd have eventually faced the terrible choice of giving up croplands (risking famine) so they could re-grow forests for heat, or having enough to eat but freezing to death in the winters. (Or, of course, they could have abandoned the colder climates, and packed their population closer together nearer the equator. But the historic movement of people had been away from the equator, a trend encouraged by the availability of fuel.)

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Excerpted from The Last Hours of Ancient Sunlight: The Fate of the World and What We Can Do Before It's Too Late by Thom Hartmann
All rights reserved by the original copyright owners. Excerpts are provided for display purposes only and may not be reproduced, reprinted or distributed without the written permission of the publisher.