The Origin and Evolution of Life on Earth


Why do we start the discussion of biology with a discussion of geology? Here are some reasons why one would do this:


The Big Bang theory of the formation of the universe

All material in the universe was created in a huge "explosion," creating and defining matter and space. The sudden cooling of the superheated ejecta facilitated the combination of atomic components into atoms and molecules. These clouds of gasses eventually cooled and formed the principle components of galaxies - including stars and planets.

Other theories have been postulated (i.e. the oscillating universe theory which states that the universe expands and contracts in a cycle every 100 billion years) and these are hotly debated


Location of the Solar System

Our solar system is located on a spiral arm of the Milky Way galaxy. We are approximately 2/3 of the distance from the core to the outer rim of the galaxy. This distance places us in a lower-density region of the galaxy - there are some stars near to ours, but this region is nowhere as congested as the galactic core.


Formation of the solar system

A. The earth formed approximately 4.6 BYA (billion years ago.) Initially, there was a cloud of gasses and dust particles, possibly originating from the ejected particles of a nearby supernova. 

B. The cloud gradually contracted and flattened, concentrating about 99% of its mass in the center with the rest rotating counterclockwise in a flattened disk. 

C. As the disk rotated, turbulence was created, causing condensation of the disk into small, turbular eddies. These gradually accreted together to form protoplanets.

D. These protoplanets further accreted, creating the mature planets of the solar system. 

The sun also accreted, pulling in most of the mass. As these accumulated, the pressure and temperature caused the initiation of thermonuclear fusion. This thermonuclear fusion is what provides the ultimate source of energy for all life on earth.

In the hot accretions of planetesimals, iron-rich elements condensed first, creating the cores (the inner and outer cores). Next, the lower-density silicates began to condense and aggregate, forming the mantle and the crust. Further differentiation of the crust was fueled by the energy output from radioactive decay deep within the earth 


Structure of the earth

There are three clearly defined regions of the earth:
  • Cores (inner (1250 km) and outer (2100 km)) - composed primarily of iron (85%) and nickel. Other heavy elements (such as radioactive elements) are also found here
  • Mantle (2900 km) - a "fluid" region primarily composed of oxygen and silica - derived minerals
  • Crust (5-70 km) - thin film of "crud" which has floated to the surface. We are simply passengers, living on this geologic flotsam.


The Dynamic Earth: Plate Tectonics

The outermost shell of the earth (the lithosphere) is a mosaic of twenty or so large, rigid slabs of rock called tectonic plates
Plate Interactions - Divergent Plate Boundaries
  • The process of adjacent plates moving away from each other is best seen at the oceanic spreading ridges
  • New crust spews out from extensive oceanic ridge systems, like the one seen in the middle of the Atlantic Ocean
    • Smaller scale systems can be seen in rift valleys, such as the African Rift Valley
  • Divergent plate boundaries are the only source of new oceanic floor
Plate Interactions - Convergent Plate Boundaries
  • When two plates meet, a convergent plate boundary forms
  • Usually one plate will slide underneath the other - this will cause some mountain building and lots of volcanic activity
    • The Andes mountains in Chile are a classic example of this
  • Sometimes plates will collide but one will not "smoothly" flow under another - extensive and rapid mountain building will occur
    • The Himalayans are an example of this


The Movement of the Plates

The plates which form the terrestrial land masses have drifted together and apart many times in the history of life on earth

The effects of these movements on life on earth cannot be underestimated.


The origin of the atmosphere and hydrosphere

Volatile gasses were either accreted to the earth during its formation or they were brought here by meteorites. These volatiles were released during the many incidences of heating and melting of the crust. This process is know as outgassing; most outgassing occurred within the first 1 billion years of the earth's history. The primitive atmosphere was rich in CO2, N2, with lesser amounts of CO, H2, HCl, with traces of NH3 and CH4.

What is life?

What is life? Life is everywhere, but it resists a simple one-sentence definition. Some of the properties of life are given below:

The Origin of Life - The Miller-Urey Experiment

How did life on earth first evolve? This question has plagued scientists and philosophers for eons. While we still do not know, experiments have given us some insights to how this may have occurred.

Experiments concerning the origin of life must answer the following questions:

In 1953, Stanley Miller and Harold Urey used an apparatus (basically a still) to recreate what is proposed to be the primitive environment of the earth. A warmed flask of water simulated the primitive oceans. The atmosphere in the Miller-Urey model was composed of H20, H2, CH4 (methane), and NH3 (ammonia). Sparks were discharged in the synthetic atmosphere to mimic lightning. A condenser cooled the atmosphere, raining water and any dissolved compounds back into the miniature sea.

The Miller-Urey Experimental Apparatus

As materials circulated through the apparatus, the solution in the flask changed from clear to murky brown. After one week, Miller and Urey analyzed the contents of the solution and found a variety of organic compounds, including amino acids, nucleic acids, and ATP, providing one scenario in which the first criterion could have been met.

The primitive atmosphere was reducing (electron adding) which facilitated the joining of monomers into polymers. The addition of sand and clays into apparatus similar to the Miller-Urey can generate longer polymers. The clays and sand act as catalysts which facilitate the formation of polymers.

Experiments show protobionts form spontaneously from abiotically formed organic molecules. These protobionts have membranes which are selectively permeable, store energy (voltage difference), etc.

Lastly, simple, self-replicating systems have been created in the lab. These consist of RNA systems. RNA systems can be self-catalyzing and are relatively unstable. This would lead to a rapid evolution.

Much in not known about the origins of life, nor will it probably ever be known. It is a very passionately debated subject. However, this is what makes it interesting and will assure the study of this science for many years to come.


Links to cool related sites

To learn more about the earth or any other planet, visit the nine planets homepage

For a more complete look at plate tectonics, check out The Dynamic Earth, the Story of Plate Tectonics

Extraterrestrial life? Check out the SETI (Search for Extra Terrestrial Intelligence) project or CNN's mars life page




If you have any questions or comments, please feel free to e-mail me.