Annual review of earth and planetary sciences; v.34, 2006.0824320344 Annual review of earth and planetary sciences planetary science or planetology, study of planets and planetary systems as a whole. Planetary science applies the theories and methods of traditional disciplines such as astronomy, geology, physics, chemistry, and mathematics to the study of ; v.34, 2006. Ed. by Raymond Jeanloz Raymond Jeanloz is a professor of earth and planetary science and of astronomy at the University of California, Berkeley. Educated at the California Institute of Technology, Amherst College and at Deep Springs College, he has contributed research fundamental to understanding of the et al. Annual Reviews 2006 723 pages $205.00 Hardcover QB600 The 2006 entry in this annual series contains 21 papers describing current models of planetary atmospheres, tools for analyzing the composition of the planets and other objects in space, and theories about the processes behind volcanic eruptions volcanic eruptions discharging of fumes, dust and lava from volcanoes. They have damaging potential in addition to those of being physically overpowering by the lava flow or the ash or dust fallout. and water cycling. The contributors review evidence for the presence of water deep inside Earth, the effectiveness of aerogel aerogel, any of a group of extremely light and porous solid materials; the lightest is less than four times as dense as dry air. Aerogels are produced from certain gels (see colloid) by heating the gel under pressure, which causes the liquid in the gel to become in capturing cosmic debris in space, and the use of thermochronometry to document the erosion histories of mountain belts. Other topics include the dynamics of lake eruptions, phanerozoic biodiversity biodiversity: see biological diversity. biodiversity Quantity of plant and animal species found in a given environment. Sometimes habitat diversity (the variety of places where organisms live) and genetic diversity (the variety of traits expressed mass extinctions, the importance of secondary cratering to age constraints on planetary surfaces, and hydrogen isotopic composition of organic matter during thermal maturation. ([c]20062005 Book News, Inc., Portland, OR) |
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