Paul G. Falkowski has produced a fascinating little book
titled Life's Engines: How Microbes Made Earth Habitable. He holds the Bennett L. Smith Chair in
Business and Natural Resources at Rutgers University. Falkowski’s intent with this book was to
provide to the non-specialist an explanation of how all forms of life share
common ancestors and how we owe our existence as humans to the efforts of the
tiniest of creatures.
Much of the text is devoted to illustrating the basic set
of molecular engines (nanomachines in Falkowski’s terminology) that were
developed to power cells and manufacture the proteins and other chemicals
necessary for their function. Falkowski
makes clear that many of “life’s engines” that developed in bacteria remain the
engines that drive life in all its current forms. Along the way, he provides an interesting
tale of how microbes played a role in providing the atmosphere that allowed
animals like us to evolve. That will be the
topic here.
By definition microbes are creatures too small to be
visible to the naked eye. Consequently,
they were essentially unknown until the seventeenth century when Hooke and
Leeuwenhoek acquired microscopes of sufficient power to detect them. It was Leeuwenhoek who first identified
bacteria and showed that we are not only surrounded by such creatures, we are
also inhabited by them. Despite the
great significance of these discoveries, Falkowski indicates that it was only
in the middle of the nineteenth century that the study of microbes began as an
active area of science. He attributes to
Ferdinand Julius Cohn the prescience to recognize the potential these little
creatures had to alter the earth’s environment.
“The renaissance of the study of
microbes began only in the middle of the nineteenth century. It was championed by an almost forgotten
hero, Ferdinand Julius Cohn. Cohn was a
Jewish wunderkind who had been born in Breslau, Prussia (today’s Wroclaw,
Poland), in 1828. It is reported that Cohn
learned to read before he was two years old, began high school at seven, and
entered the University of Breslau at fourteen.”
“Cohn was not focused on the
role of microbes in causing human disease.
Although he worked on microbial diseases of plants and animals, and was
far less famous than Pasteur, he had an even broader vision. He saw microbes as organisms that helped
shape the chemistry of the Earth—the planet’s metabolism.”
Little creatures can accomplish great things if there are
enough of them. This source provides us with a way to
visualize the numbers involved.
“There are typically 40 million
bacterial cells in a gram of soil and a million bacterial cells in a millilitre
of fresh water….forming a biomass which exceeds that of all plants and animals.”
“There are approximately ten
times as many bacterial cells in the human flora as there are human cells in
the body, with the largest number of the human flora being in the gut flora,
and a large number on the skin.”
And that neglects the various viruses and other parasites
that inhabit us.
The key requirement for the evolution of complex,
multicellular structures was the availability of free oxygen in the
atmosphere. This source provides a chart
illustrating the history of the atmospheric oxygen abundance.
The red and green lines indicate the highs and lows of
the various estimates of oxygen abundance as a function of time. The x-axis records billions of years in the
past.
The Earth is thought to have been formed about 4.5
billion years ago. There is evidence
that single-celled bacteria existed about 3.5 billion years in the past, but
oxygen as a free molecule doesn’t become available until about a billion years
later. Since life began before free
oxygen was available, the first cellular organisms would have to use other
elements to produce the materials needed for energy, nourishment, and reproduction. For example, bacteria capable of ingesting
hydrogen sulfide and producing sulfur as a waste product (with and without the
utilization of sunlight to drive photosynthesis) predate the photosynthetic
microbes capable of replacing hydrogen sulfide with water and producing
oxygen. These creatures would have
consumed any resident oxygen as they died and their decay produced carbon dioxide. Other sinks for free oxygen molecules
assisted in limiting its concentration.
Oxygen is important for biological evolution because it
reacts readily with many elements and provides considerable energy when it
does. That is exactly the property that
would have rendered it rare as a free molecule in the early atmosphere. It would be readily coupled with the abundant
hydrogen atoms to form water or reacted with other elements to form oxides.
Water is much more difficult to break down than hydrogen
sulfide. It would take a very long time
before the mechanism capable of that feat would be developed. From Falkowski:
“The first photosynthetic
microbes were anoxygenic—that is they were not capable of splitting water. It took several hundred million years before
microbes evolved the ability to split water.
Water is an ideal source of hydrogen on Earth’s surface because it is
far more abundant than any other potential electron donor, but splitting it
takes a lot of energy. The responsible nanomachines
evolved only once among prokaryotes: in the cyanobacteria, or blue-green
algae. When these organisms finally were
able to split water, they produced a new gaseous waste product: oxygen. The biological production of oxygen changed
the evolution of life on Earth forever.”
Producing a source for molecular oxygen does not
immediately produce a ready supply. The
sinks for oxygen would have to be overcome.
In fact, the algae that produce oxygen using photosynthesis will respire
carbon dioxide and water when no light is available, thus negating a fraction
of the oxygen production. These same
bacteria will die and decay and thus consume more of the oxygen. For oxygen to build up in the atmosphere,
decaying creatures would have to be stashed somewhere where they would not have
access to oxygen. This is where all that
oil and gas we have been using for so long enters the story.
“By far the most important
storage areas are in shallow seas and along the coasts of continents. But even there, on average less than 1% of
the organic matter produced by phytoplankton reaches the sea floor, and only
about 1% of that is subsequently buried in sediments. This means that less than 0.01% of organic
matter is actually buried, but over millions and millions of years, this very
small fraction becomes significant on a global scale….”
Having these sediments ultimately incorporated into
sedimentary rock still does not necessarily protect the oxygen gas from being
consumed. Yet another mechanism is required
to keep it safe.
“Some of the sedimentary rocks,
which contain the organic matter, are subsequently uplifted onto the continents
to form mountains….Without uplifting the organic matter onto continents, the
organic matter would be subducted into the interior of the Earth by tectonic
processes, heated, and returned to the atmosphere as carbon dioxide from
volcanoes—and little or no oxygen would accumulate.”
Producing an atmosphere containing a significant oxygen
component was no easy matter. For the
planet itself it was revolutionary. As
in most revolutions, death and chaos ensued.
The emergence of oxygen in the atmosphere led to what is known as the
Great Oxygenation Event.
Many species of microbes had evolved in a low oxygen or
oxygen free environment. An excess of
oxygen was poisonous to many. Species
that produced methane were common and methane was a significant component of
the atmosphere. The availability of
oxygen not only harmed the methanogenic microbes it also reacted easily with
methane and removed it from the atmosphere.
Unfortunately methane is a very efficient greenhouse gas and the Earth
needed it to maintain its surface temperature.
As this source puts it:
“Free oxygen is toxic to obligate
anaerobic organisms, and the rising concentrations may have wiped out most of
the Earth's anaerobic inhabitants at the time. Cyanobacteria were therefore
responsible for one of the most significant extinction events in Earth's
history. Additionally, the free oxygen reacted with atmospheric methane, a greenhouse
gas, greatly reducing its concentration and triggering the Huronian glaciation,
possibly the longest snowball Earth episode in the Earth's history.”
Note that after the Great Oxidation Event the oxygen content
of the atmosphere leveled off at just a few percent. Further buildup would require additional
evolution. That would come in the development
of multicelled eukaryotes (made up of cells with nuclei), particularly the phytoplankton. These could be larger and produce more oxygen
and, more importantly, could sink faster and more efficiently hide its decaying
bodies in sediments. This is the
mechanism that generated the rise in oxygen that began about 700 million years
ago in stage 4 on the above chart.
Yet more magic is required to get us to our current
state. At this point in time there are
no land-based plants or animals. As the
oxygen level rises, simple animals that now depend on oxygen can arrange
themselves in more complex configurations without worrying about oxygen
limitations. Stage 5 contains the Cambrian Explosion when nature experimented
with many species, discarded most, and kept the ones that provided the major species
classifications of today. This unique
period occurred around 540 million years ago and lasted a few tens of millions
of years.
Falkowski provides this perspective:
“The evolution of animals seems
to have preceded the evolution of plants on land by approximately 200 million
years….Terrestrial plants are derived from a single group of green algae and
began to colonize land about 450 million years ago.”
The rise of oxygen respiring plants greatly boosted the
oxygen level to higher values than currently exist. The result was that animals began to invade
land from the oceans encouraged by this abundant supply. They would provide a healthy sink for oxygen
as they consumed it and respired carbon dioxide and water. Eventually equilibrium would be established.
What to take away from this story? One thing is that life forms were created
early in the earth’s history, but life as we know it, life based on an oxygen-rich
atmosphere, occurred only through a sequence of not inevitable events. Quite a bit of luck was involved.
“Oxygen is unique to Earth’s
atmosphere. The gas has not been found
in high concentrations on any other planet in our solar system, nor has it been
found in the surrounding neighborhood of stars that have planets. Although it is highly likely that other
planets will be discovered to have oxygen, it does not seem to be a common gas
on terrestrial planets.”
The evolution of life forms may not be that difficult on
other planets; the evolution of life forms like ours might be quite a bit more
unlikely
Another conclusion one might draw is that Earth is a
complicated place and small changes can produce dramatic effects. The pollution we generate and the carbon
dioxide we spew into the air are hardly noticeable to us. However, they are major factors affecting our
oceans. Acidity levels are rising, food
chains are being disrupted, and species populations are being altered. This is risky business. The oceans produced life; they can also
destroy it. Since the Cambrian period
there have been at least five mass extinction events. Our current era
has already been referred to as the sixth.
There is no law of nature that prevents humans from being victims.