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Earth - Life

surface million —the layer

The presence of life on Earth is, as far as we know, unique. Men have walked on the Moon, and it seems certain there is no life on our barren, airless satellite. Unmanned spacecraft have landed on Venus and Mars and have flown close to every other planet in the solar system except Pluto. The most promising possibility, Mars, yielded nothing to the automated experiments performed by the Viking spacecraft that touched down there.

The origin of life on Earth is not understood, but a promising experiment was performed in 1952 that may hold the secret. Stanley Miller and Harold Urey simulated conditions in Earth's early oceans, reproducing the surface and atmospheric conditions thought to have existed more than three billion years ago. A critical element of this experiment was simulated lightning in the form of an electric arc. Miller and Urey found that under these conditions, amino acids, the essential building blocks of life, had formed in their primitive "sludge." Certainly this was a long way from humans—or even an amoeba—but the experiment proved that the early Earth may have been a place where organic compounds, the compounds found in living creatures, could form.

Life has existed on dry land only for the most recent 10% of Earth's history, since about 400 million years ago. Once life got a foothold beyond the oceans, however, it spread rapidly. Within 200 million years forests spread across the continents and the first amphibians evolved into dinosaurs. Mammals became dominant after the demise of the dinosaurs 65 million years ago, and only in the last two million years have humans come onto the scene.

Resources

Books

Beatty, J., and A. Chaikin. The New Solar System. Cambridge: Cambridge University Press, 1991.

Cater, John. Key to the Future: The History of Earth Science. New York: Routledge, 2002.

Hamblin, W. K., and E.H. Christiansen. Earth's Dynamic Systems. 9th ed. Upper Saddle River: Prentice Hall, 2001.

Hancock, P. L. and B. J. Skinner, eds. The Oxford Companion to the Earth. Oxford: Oxford University Press, 2000.

Press, F., and R. Siever. Understanding Earth. 3rd ed. New York: W. H Freeman and Company, 2001.

Periodicals

"The Dynamic Earth." Scientific American 249 (special issue, September 1983): 46–78+.

Haneberg, William C. "Determistic and Probabilistic Approaches to Geologic Hazard Assessment." Environmental & Engineering Geoscience 6, no. 3 (August 2000): 209–226.

Hoehler, T. M., B. M. Bebout, and D. J. Des Marais. "The Role of Microbial Mats in the Production of Reduced Gases on the Early Earth." Nature 412 (July 2001): 324–327.


Jeffrey C. Hall

KEY TERMS

. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

Core

—The innermost layer of Earth's interior. The core is composed of molten iron and nickel, and it is the source of Earth's magnetic field.

Erosion

—One of the two main processes that alter Earth's surface. Erosion, caused by water and wind, tends to wear down surface features such as mountains.

Lithosphere

—The outermost layer of Earth's interior, commonly called the crust. The lithosphere is broken into several large plates that move slowly about. Collisions between the plates produce mountain ranges and volcanism.

Mantle

—The thick layer of Earth's interior between the core and the crust.

Mountain-building

—One of the two main processes that alter Earth's surface. Mountain-building occurs where two crustal plates collide and crumple, resulting in land forms thrust high above the surrounding terrain.

Terrestrial planets

—Planets with Earth-like characteristics relatively close to the Sun. The terrestrial planets are Mercury, Venus, Earth, and Mars.

Troposphere

—The layer of air up to 15 mi (24 km) above the surface of the Earth, also known as the lower atmosphere.

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