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Fossil Record

The origin and diversity of life on Earth has been one of humankind's most enduring sources of curiosity. The questions of,“who, how, when, where, and why” are still widely debated. These questions cross the boundaries between science, philosophy, and religion. It is not the intent of this entry to settle this controversy. Rather, it will look at these topics from the standpoint of science based on our current level of knowledge and understanding. This entry is arranged chronologically by era. The time spans discussed are compared to their relative positions from the “recent” end of a 100-meter-long rope to illustrate the quantity of time discussed and its distance from the present. Dates presented herein are primarily from the revised stratigraphic chart of the International Commission on Stratigraphy, 2004. The abbreviation mya means “million years ago.”

One feature of the fossil record is that preserved fossil localities increase in direct proportion to how recently the localities were preserved. In most cases, the preservation is limited to hard body parts, and these parts are often poorly preserved. However, unusually complete and well-preserved assemblages that often include soft-tissue preservation, called lagerstätten, greatly increase the available information for the time when the assemblage was preserved. When interpreting trends in the fossil record, it is easy to infer a gradual increase in diversity through time when, in reality, the increase is merely an artifact of an increased number of fossil localities. Likewise, lagerstätten have nearly always contributed to interpreted “explosions” of diversity. Unfortunately, these glimpses of possibly true representations of biotic diversity are limited to one environment and one instant in time, and these glimpses usually occur tens of millions of years apart. The fossil record thus does not contain enough information to provide any degree of accuracy concerning any but the most basic trends in biotic evolution. For this reason, this report should be considered a tentative representation of our current understanding rather than a definitive statement concerning Earth's evolutionary events.

Earth's Origin–Hadean Era: 4,550–3,800 mya(100 to 83.5 meters)

The Hadean is the most poorly known part of Earth's history. For much of this time, the Earth was in the process of coalescing, cooling, and continent forming. The 4.55-billion-year date for the beginning of the planet was not obtained from Earth's rocks, but rather from meteorites and moon rocks. These sources seem to place the “solidification” of our solar system, including the Earth, at that date. Then, for a period of time, the Earth likely underwent heating, compression, and eventual landmass solidification. The name “Hadean” was actually given to this period of Earth's history because of the tremendous heating and volcanic events that are speculated to have happened during that time. It is thought that a collision of Earth and another planetoid at approximately 4.5 billion years ago produced our moon and significantly remodeled the Earth in the process. This and other collisions kept the Earth very hot. However, it should be noted that this picture of Earth's distant past is highly conjectural. No rock outcrops are known that date to the first half-billion years of Earth's history. Some scientists have postulated the opposite effect, a “snowball Earth,” for Earth's very early history, and still others have postulated an environment rich in oxygen since earliest times. Only the most widely accepted views will be presented here.

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