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"Carbon is arguably humankind's most important chemical element - indeed, possibly the most important element in the universe. Created in the fiery furnaces of stars, carbon is the chemical backbone of the planets and life as we know it. It is essential to every part of our lives: the bones and tissue which give us all shape, the food we eat, the tools we use, the climate which supports life on this planet. Despite these facts, carbon's importance is often overlooked. In this short, popular-level book, astronomers Theodore Snow and Donald Brownlee consider carbon from a cosmic perspective, explaining the inherent chemical and physical nature of the element as well as the ways in which it is ...
This book was conceived to commemorate the continuing success of the guest observer program for the International Ultraviolet Explorer (IUE) satellite observatory. It is also hoped that this volume will serve as a useful tutorial for those pursuing research in related fields with future space observatories. As the IUE has been the product of the three-way collaboration between the U.S. National Aeronautics and Space Administration (NASA), European Space Agency (ESA) and the British Engineering and Research Council (SERC), so is this book the fruit of the collaboration of the American and European participants in the IUE. As such, it is a testimony to timely international cooperation and sharing of resources that open up new possibilities. The IUE spacecraft was launched on the 26th of January in 1978 into a geosynchronous orbit over the Atlantic Ocean. The scientific operations of the IUE are performed for 16 hours a day from Goddard Space Flight Center in Greenbelt, Maryland, U.S.A, and for 8 hours a day from ESA Villafranca Satellite Tracking Station near Madrid, Spain.
This book is aimed at several distinct audiences: first, the upper division science major who wants an up-to-date appreciation of the present state of the planetary sciences for 'cultural' purposes; second, the first-year graduate student from any of several undergraduate disciplines who intends to take graduate courses in specialized areas of planetary sciences; and third, the practicing Ph. D. scientist with training in physics, chemistry, geology, astronomy, meteorology, biology, etc., who has a highly specialized knowledge of some portion of this material, but has not had the opportunity to study the broad context within which that specialty might be applied to current problems in this field.
Big-Bang? Do you believe it? I don't. Being a career engineering-physicist, I always look for proof. For 50 years I have tried to prove the BB to myself. I have reviewed Slipher's red shift observation, reinterpreted it, and corrected Hubble's declaration, (the universe is not expanding and exploding to its death, instead, it is growing with vim and vigor). Red shift defines velocity, not acceleration or deceleration. So, I developed the New Universe Theory which is believable because it complies with known facts and the Laws of Physics.
IAU Symposium Number 52 on Interstellar Dust and Related Topics was held at Albany, N.Y., on the campus of the State University of New York at Albany from May 29 to June 2, 1972. The members of the Organizing Committee were: Dr A. D. Code, University of Wisconsin, Madison, Wis., U.S.A. Dr B. D. Donn, Goddard Space Flight Center, Greenbelt, Md., U.S.A. Dr A. Elvius, Stockholm Observatory, Saltsjobaden, Sweden. Dr T. Gehrels, Lunar and Planetary Laboratory, University of Arizona, Tucson, Ariz., U.S.A. Dr J. M. Greenberg (Chairman), State University of New York at Albany, Albany, N.Y., U.S.A. Dr H. C. van de Hulst, Sterrewacht, Leiden, Holland. Dr S. B. Pikel'ner, Sternberg Astronomical Institu...
A meeting on "Astrophysics. from Spacelab" was held at the Internatio nal Centre for Theoretical Physics, Trieste, in the Autumn of 1976. Scope of the meeting was to bring to the attention of an increasing number of physi cists and astrophysicists, including scientists from developing countries, the new facil ities made available by the combination of the Shuttle and the Spacelab programmes. This book starts from that meeting and includes, together with reports presented in Trieste, duly updated, a few additional reviews on selected to pi cs. In the first part, D.J. Shapland and G. Giampalmo (liThe Shuttle and the Spacelab") present the design and the programmatic data of these advanced tran...
Physics and Chemistry of the Solar System focuses on planetary physics and chemistry. This book consists of 12 chapters. Chapters I to IV cover the general properties and environment of the planetary system. The solar system beyond Mars is elaborated in Chapters V to VIII, while the inner solar system is considered in Chapters XI to XII. In these chapters, this compilation specifically discusses the limitations on big bang nucleosynthesis; structure and classification of galaxies; and mass and angular momentum distribution. The radio wave propagation in space plasmas; interiors of Jupiter and Saturn; density and composition of icy satellites; and evaporation and non-gravitational forces are also deliberated. This text also explains the physical properties of meteorites; geology of the Moon; geophysical data on Mars; and search for extraterrestrial intelligence. This publication is a good reference for first-year graduate students who intend to take graduate courses in specialized areas of planetary sciences, as well as practicing Ph.D. scientists with training in physics, chemistry, geology, astronomy, meteorology, and biology.