Venus II--geology, Geophysics, Atmosphere, and Solar Wind Environment

Venus II--geology, Geophysics, Atmosphere, and Solar Wind Environment
Author :
Publisher : University of Arizona Press
Total Pages : 1384
Release :
ISBN-10 : 0816518300
ISBN-13 : 9780816518302
Rating : 4/5 (302 Downloads)

Book Synopsis Venus II--geology, Geophysics, Atmosphere, and Solar Wind Environment by : Stephen Wesley Bougher

Download or read book Venus II--geology, Geophysics, Atmosphere, and Solar Wind Environment written by Stephen Wesley Bougher and published by University of Arizona Press. This book was released on 1997-12 with total page 1384 pages. Available in PDF, EPUB and Kindle. Book excerpt: The final orbit of Venus by the Magellan spacecraft in October 1994 brought to a close an exciting period of Venus reconnaissance and exploration. The scientific studies resulting from data collected by the Magellan, Galileo, and Pioneer missions are unprecedented in their detail for any planet except Earth. Venus II re-evaluates initial assessments of Venus in light of these and other spacecraft missions and ground-based observations conducted over the past 30 years. More than a hundred contributors summarize our current knowledge of the planet, consider points of disagreement in interpretation, and identify priorities for future research. Topics addressed include geology, surface processes, volcanism, tectonism, impact cratering, geodynamics, upper and lower atmospheres, and solar wind environment. The diversity of the coverage reflects the interdisciplinary nature of Venus science and the breadth of knowledge that has contributed to it. A CD-ROM developed by the Jet Propulsion Laboratory accompanies the book and incorporates text, graphics, video, software, and various digital products from selected contributors to the text. A multimedia interface allows users to navigate the text and the extensive databases included on the disk. Venus II is the most authoritative single volume available on the second planet. Its contents will not only help shape the goals of future Venus missions but will also enhance our understanding of current Mars explorations.


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