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exobiology

exobiology or astrobiology, search for extraterrestrial life within the solar system and throughout the universe. Philosophical speculation that there might be other worlds similar to ours dates back to the ancient Chinese and Greeks. However, the achievements of space exploration and molecular biology have turned speculation into experimentation.

Parameters of a Suitable Environment for Life

There are six basic parameters that determine whether an environment is suitable for life as we know it: temperature, pressure, salinity, acidity, water availability, and oxygen content. Advanced life is restricted to a narrow range of these parameters, but primitive microorganisms exist over a much wider range. Data already collected by space probes essentially rule out advanced life on other planets of our solar system; however, given the potential number of planetary systems in the galaxy, there may be as many as 50,000 planets that have earthlike conditions, a fraction of which could have cultures as technologically advanced as our own. Three decades of passive listening with radio telescopes have produced no signals comparable to those radiating from earth, but we do not know if another civilization would produce electromagnetic radiation in detectable amounts.

The Search for Primitive Life

A continuing effort is being made to detect primitive life within our solar system. According to the Russian biologist A. I. Oparin, life can appear as the result of progressive development of organic matter from nonorganic. The principal constituents of organic matter—hydrogen, carbon, nitrogen, and oxygen—are among the most abundant atomic elements in the universe. Oparin assumed that on earth these elements combined to form simple hydrocarbons and that the hydrocarbons combined to form the precursors of life, such as amino and nucleic acids. Once these precursor molecules existed in the earth's primitive seas, they spontaneously interacted to form increasingly complex structures, until self-replicating molecules like deoxyribonucleic acid (DNA) were created, leading the way to protein synthesis.

American chemists Stanley L. Miller and Harold C. Urey provided experimental support for Oparin's theory, by discovering that when a mixture of methane, ammonia, water, and hydrogen is exposed to an electric discharge, amino acids are formed. The composition of this gas mixture is similar to the atmosphere of Jupiter. The same result has been obtained by exposing the gas mixture to ultraviolet radiation, which exists in outer space. Further support for Oparin's theory came with the discovery of organic molecules like ammonia and formaldehyde in the interstellar medium. A labeled-release experiment contained on the Viking landers which analyzed the surface of Mars in 1976 detected what could be organic activity.

Evidence of organic material and, possibly, fossils of microscopic bacteria have been found in certain carbonaceous chondrite meteorites, most notably the Orgeuil meteorite, which fell in France in 1864, the Murchison meteorite, which fell in Australia in 1969, and the Allan Hills Martian meteorite, found in Antarctica in 1984, but other scientists have argued either that such organic traces result from terrestrial contamination or that the data have been misinterpreted. However, an analysis of the Murchison meteorite that extracted material from its core found evidence of 70 amino acids and many other organic compounds. Some scientists believe that the moon, Mars, and Venus have already been contaminated by microorganisms carried on space probes. Conversely, fears that returning Apollo astronauts could introduce destructive alien organisms into earth's biosphere led NASA to quarantine them for as long as two weeks, and lunar rock samples were kept carefully isolated.

Bibliography

See D. Goldsmith, The Hunt for Life on Mars (1997); P. Day, ed., The Search for Extraterrestrial Life: Essays on Science and Technology (1998); S. J. Dick, Life on Other Worlds: The 20th-Century Extraterrestrial Life Debate (1998).

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Exobiology

Exobiology


Exobiology, also known as astrobiology and bioastronomy, is the study of the potential for life beyond Earth and the active search for it. Nobel geneticist Joshua Lederberg coined the term exobiology in 1960, and the field grew significantly with space exploration, especially the Viking landers on Mars. Exobiology draws largely from four disciplines: planetary science, planetary systems science, origins of life studies, and the Search for Extraterrestrial Intelligence (SETI). The field has been invigorated by claims of fossil life in an ancient Mars rock, the discovery of a possible ocean on the Jovian moon Europa, extrasolar planets around sun-like stars, life in extreme environments on Earth, and complex organic molecules in interstellar molecular clouds. Life itself, however, has not yet been found beyond Earth.

See also Extraterrestrial Life

steven j. dick

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exobiology

exobiology Search for life on other planets. Exobiology is concerned with attempts to detect environmental conditions and possible biochemical and evolutionary pathways to life beyond Earth. Examples include the probes sent in 2003 by NASA and the European Space Agency to detect evidence of water on Mars

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exobiology

exobiology The biology of outer space: a study currently limited to the seeking of evidence for the existence of life beyond the Earth, and speculation on the possible alternative forms of such life.

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