
The Methow Conservancy created the Big Ecology course based on “Big History.” Big History is a unique approach to the evolution of the universe and it is currently being taught in numerous universities around the globe, and over 50 high schools. It provides an excellent framework for how we have arrived, and what our place in the universe is. Instead of breaking down and studying microcosms of the whole picture, big ecology incorporates many disciplines of science and reveals their interdependency through time.
Dana said there were five themes of our evolving universe. The Universe: 1. has a history & a story. 2. has a direction—increasing complexity. 3. is emergent—always new. and developing 4. Is ecological: everything is related and connected, and 5. humans are part of the story.
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The Orion Nebula, a well known star-forming region in Orion's belt |
After the big-bang occurred the universe was made up of nothing but hydrogen, the first element of the periodic table. After a few hundred million years they decided to have a relationship and they formed helium (H2). When two H fuse to He, the H atoms give up about 1% (0.7%) of their mass—which is transformed into energy. All life on earth owes its existence to this 0.7% energy release. With the help of gravity, the rapidly expanding helium and hydrogen began to form stars and galaxies, giving us the second threshold.
The third threshold is the evolution, over time, of the 92 natural elements. Additional heavier elements formed during the creation of stars and they included carbon, nitrogen, oxygen, sodium, and magnesium. It is fun to think that the building blocks for life on earth find their roots in the stars. Stars collapsed into super novas and the energy from those explosions provided us with the remaining heavier elements found on the periodic table. All of the elements necessary to form planets existed at this point and with more help from gravity, the solid cores of planets began forming.
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Our home, taken by NASA |
The sixth threshold occurred when photosynthesis and the production of oxygen began. This opened up the door to plant life on earth. The Biologist Lynn Margulis said, “Photosynthesis is undoubtedly the most important single metabolic innovation in the history of life on the planet.”

The final threshold was the growth of the brain and the emergence of collective learning and symbolic thought. Organisms moved beyond basic survival and reproduction at this point and began creative thought and expression. For Homo sapiens this meant the beginning of artwork and language. One of the most fascinating aspects to the development of the complexity of life on earth is the increasing amount of energy needed at each level of existence. When you compare the energy densities of galaxies to the human brain we discover that the brain is 150,000 times more energy intensive. We think of stars as superheated balls of fire and energy, but because they are so huge, their energy density is only 2 erg/second. As we work our way down in size we find that planets are 75 erg/sec; plants are 900 erg/sec; animals are 20,000 erg/sec; brains are 150,000 erg/sec; and society on earth is 500,000 erg/sec.
A major point Dana made is that the human brain is an emergent phenomenon that is still evolving.
Dana said all of the events that have occurred to get us from one threshold to another are called “Goldilocks” moments. These occur when everything needed for change is in the right place in exactly the right amounts (heat, gravity, etc). These quantum leaps in evolution could not have occurred if any one piece of the puzzle was a fraction of a percent different.

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Many scientists believe we are in a 6th "mass extinction event." |
A clear point in Dana’s talk was that the universe is emergent. New phenomena are always emerging. An emergent universe is never finished, it is always in process. Humans have been formed by the forces at work in the universe. Humans have a place in this story. We are an emergent work in progress.
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One of our ancestor’s hands, from a cave in Altimira, Spain about 17,000 years ago |
See the course syllabus and a fascinating list of resources (readings & films) here
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