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Planetary science is a truly multidisciplinary subject. The book deals with the atmospheres, surfaces and interiors of the planets and moons, and with the interplanetary environment of plasma and fields, as well as with asteroids and meteorites. Processes such as accretion, differentiation, thermal evolution, and impact cratering form another category of entries. Remote sensing techniques employed in investigation and exploration, such as magnetometry, photometry, and spectroscopy are described in separate articles. In addition, the Encyclopedia chronicles the history of planetary science, including biographies of pioneering scientists, and detailed descriptions of all major lunar and planetary missions and programs. The Encyclopedia of Planetary Sciences is superbly illustrated throughout with over 450 line drawings, 180 black and white photographs, and 63 color illustrations. It will be a key reference source for planetary scientists, astronomers, and workers in related disciplines such as geophysics, geology, and the atmospheric sciences.
The increase in our knowledge of the solar system during the five years since the author last revised this book (1963) greatly exceeds that in the previous two decades. The program of the U.S. National Aeronautics and Space Administration and the space program of the U.S.S.R. have been prime contributors to this rapid progress, but the impetus has carried over to groundbased studies of the Moon and planets as well. The advances in radio and radar astronomy alone are striking, and are continuing at an accelerating pace. This third edition of Mr. Whipple's popular and authoritative book is thoroughly revised in light of this new knowledge. The most extensive revisions are in the chapters on the Moon, Mars, and Venus--the members of the solar system on which the various space programs have concentrated. The author has included many new and dramatic illustrations in this third edition, among them photographs taken from U.S. and Russian space craft. There are striking photographs of the Moon, with close-up views of its surface texture, pictures of Mars taken from Mariner IV, and radar pictures of Venus that "see through" that planet's obscuring cloud layer. The book is written in nontechnical language and with a lucid, witty style that is readily understandable to the interested layman. Mathematics has been avoided, and scientific methods and processes are described in simple terms. In presenting the latest information about the planets and their moons, Mr. Whipple discusses their origin and evolution, motions, atmospheres, temperatures, surface conditions, the environment essential for life as we know it, and the possibilities of life outside the Earth. He concludes with a discussion of current theories about the origin of the solar system.
This review gathers astronomers, geologists, biologists, and chemists around a common question: how did life emerge on Earth? The ultimate goal is to probe an even more demanding question: is life universal? This not-so linear account highlights problems, gaps, and controversies. Discussion covers the formation of the solar system; the building of a habitable planet; prebiotic chemistry, biochemistry, and the emergence of life; the early Earth environment, and much more.
Since the beginning of civilization, the origins of the Earth and Moon have been the subjects of continuing interest, speculation, and enquiry. These are also among the most challenging of all scientific problems. They are, perhaps to a unique degree, interdisciplinary, having attracted the attention of philosophers, astronomers, mathematicians, geologists, chemists, and physicists. A large and diverse literature has developed, far beyond the capacity of individuals to assimilate adequately. Consequently, most of those who attempt to present review-syntheses in the area tend to reflect the perspectives of their own particular disciplines. The present author's approach is that of a geochemist, strongly influenced by the basic phil osophy of Harold Urey. Whereas most astronomical phenomena are controlled by gravitational and magnetic fields, and by nuclear interactions, Urey (1952) emphasized that the formation of the solar system occurred in a pressure-temperature regime wherein the chemical properties of matter were at least as important as those of gravitational and magnetic fields. This was the principal theme of his 1952 book, "The Planets," which revolutionized our approach to this subject. In many subsequent papers, Urey strongly emphasized the importance of meteorites in providing critical evidence of chemical conditions in the primordial solar nebula, and of the chemical fractionation processes which occurred during formation of the terrestrial planets. This approach has been followed by most subsequent geochemists and cosmochemists.
A detailed overview of Saturn's formation, evolution and structure written by eminent planetary scientists involved in the Cassini Orbiter mission.
A comprehensive and authoritative text on the formation and evolution of planetary atmospheres, for graduate-level students and researchers.