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Author: A.C. Levasseur-Regourd
Publisher: Springer Science & Business Media
ISBN: 9401136408
Category : Science
Languages : en
Pages : 472
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Book Description
THE THE KYOTO KYOTO COLLOQUIUM COLLOQUIUM It It has has almost almost become become a a tradition tradition to to periodically periodically review review the the progress progress of of our our knowledge knowledge of of interplanetary interplanetary dust dust at at an an interdisciplinary interdisciplinary level. level. After After the the Honolulu Honolulu (1967), (1967), Heidelberg Heidelberg (1975), (1975), Ottawa Ottawa (1979) (1979) and and Marseilles Marseilles (1984) (1984) meetings, meetings, it it was was decided decided to to hold hold a a meeting meeting specially specially devoted devoted to to the the Origin Origin and and Evolution Evolution of of Interplanetary Interplanetary Dust Dust in in Kyoto, Kyoto, Japan Japan on on 27-30 27-30 August August 1990. 1990. This This colloquium colloquium was was certainly certainly appropriate appropriate in in location, location, timing timing and and objective. objective. The The choice choice of of the the location location was was most most appropriate, appropriate, not not only only because because of of the the charm charm of of the the beautiful beautiful city city of of Kyoto, Kyoto, but but also also because because of of the the important important involvement involvement of of our our Japanese Japanese colleagues, colleagues, both both in in observations observations of of interplanetary, interplanetary, cometary, cometary, meteoritic, meteoritic, circumplanetary circumplanetary or or circumstellar circumstellar dust, dust, and and in in physico-chemical physico-chemical analysis analysis or or theoretical theoretical developments. developments.
Author: A.C. Levasseur-Regourd
Publisher: Springer Science & Business Media
ISBN: 9401136408
Category : Science
Languages : en
Pages : 472
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Book Description
THE THE KYOTO KYOTO COLLOQUIUM COLLOQUIUM It It has has almost almost become become a a tradition tradition to to periodically periodically review review the the progress progress of of our our knowledge knowledge of of interplanetary interplanetary dust dust at at an an interdisciplinary interdisciplinary level. level. After After the the Honolulu Honolulu (1967), (1967), Heidelberg Heidelberg (1975), (1975), Ottawa Ottawa (1979) (1979) and and Marseilles Marseilles (1984) (1984) meetings, meetings, it it was was decided decided to to hold hold a a meeting meeting specially specially devoted devoted to to the the Origin Origin and and Evolution Evolution of of Interplanetary Interplanetary Dust Dust in in Kyoto, Kyoto, Japan Japan on on 27-30 27-30 August August 1990. 1990. This This colloquium colloquium was was certainly certainly appropriate appropriate in in location, location, timing timing and and objective. objective. The The choice choice of of the the location location was was most most appropriate, appropriate, not not only only because because of of the the charm charm of of the the beautiful beautiful city city of of Kyoto, Kyoto, but but also also because because of of the the important important involvement involvement of of our our Japanese Japanese colleagues, colleagues, both both in in observations observations of of interplanetary, interplanetary, cometary, cometary, meteoritic, meteoritic, circumplanetary circumplanetary or or circumstellar circumstellar dust, dust, and and in in physico-chemical physico-chemical analysis analysis or or theoretical theoretical developments. developments.
Author: Astronomisches Recheninstitut
Publisher: Springer Science & Business Media
ISBN: 3662123797
Category : Science
Languages : en
Pages : 1456
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Book Description
"Astronomy and Astrophysics Abstracts" appearing twice a year has become oneof the fundamental publications in the fields of astronomy, astrophysics andneighbouring sciences. It is the most important English-language abstracting journal in the mentioned branches. The abstracts are classified under more than a hundred subject categories, thus permitting a quick survey of the whole extended material. The AAA is a valuable and important publication for all students and scientists working in the fields of astronomy and related sciences. As such it represents a necessary ingredient of any astronomical library all over the world.
Author: J. Mayo Greenberg
Publisher: Springer Science & Business Media
ISBN: 9401119368
Category : Science
Languages : en
Pages : 429
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Book Description
This volume contains the lectures presented at the second course of the International School of Space Chemistry held in Erice (Sicily) from October 20 - 30 1991 at the "E. Majorana Centre for Scientific Culture". The course was attended by 58 participants from 13 countries. The Chemistry of Life's Origins is well recognized as one of the most critical subjects of modem chemistry. Much progress has been made since the amazingly perceptive contributions by Oparin some 70 years ago when he first outlined a possible series of steps starting from simple molecules to basic building blocks and ultimate assembly into simple organisms capable of replicating, catalysis and evolution to higher organisms. The pioneering experiments of Stanley Miller demonstrated already forty years ago how easy it could have been to form the amino acids which are critical to living organisms. However we have since learned and are still learning a great deal more about the primitive conditions on earth which has led us to a rethinking of where and how the condition for prebiotic chemical processes occurred. We have also learned a great deal more about the molecular basis for life. For instance, the existence of DNA was just discovered forty years ago.
Author: Sushil K. Atreya
Publisher: University of Arizona Press
ISBN: 0816546541
Category : Science
Languages : en
Pages : 896
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Book Description
An integrated discussion of the similarities and differences between the atmospheres of various bodies of the solar system, including the Earth.
Author: Rainer Schwenn
Publisher: Springer Science & Business Media
ISBN: 3642753647
Category : Science
Languages : en
Pages : 360
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Book Description
Physics of the Inner Heliosphere gives for the first time a comprehensive and complete summary of our knowledge of the inner solar system. Using data collected over more than 11 years by the HELIOS twin solar probes, one of the most successful ventures in unmanned space exploration, the authors have compiled six extensive reviews of the physical processes of the inner heliosphere and their relation to the solar atmosphere. Researchers and advanced students in space and plasma physics, astronomy, and solar physics will be surprised to see just how closely the heliosphere is tied to, and how sensitively it depends on, the sun. Volume 2 deals with particles, waves, and turbulence, with chapters on: - magnetic clouds - interplanetary clouds - the solar wind plasma and MHD turbulence - waves and instabilities - energetic particles in the inner solar system
Author: A.M. Davis
Publisher: Elsevier
ISBN: 0080525350
Category : Science
Languages : en
Pages : 755
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Book Description
Volume 1 provides a broad overview of the chemistry of the solar system. It includes chapters on the origin of the elements and solar system abundances, the solar nebula and planet formation, meteorite classification, the major types of meteorites, important processes in early solar system history, geochemistry of the terrestrial planets, the giant planets and their satellite, comets, and the formation and early differentiation of the Earth. This volume is intended to be the first reference work one would consult to learn about the chemistry of the solar system.Reprinted individual volume from the acclaimed Treatise on Geochemistry (10 Volume Set, ISBN 0-08-043751-6, published in 2003)
Author: Glenn J. MacPherson
Publisher: Walter de Gruyter GmbH & Co KG
ISBN: 1501508504
Category : Science
Languages : en
Pages : 620
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Book Description
Volume 68 of Reviews in Mineralogy and Geochemistry reviews Oxygen in the Solar System, an element that is so critically important in so many ways to planetary science. The book is based on three open workshops: Oxygen in the Terrestrial Planets, held in Santa Fe, NM July 20-23, 2004; Oxygen in Asteroids and Meteorites, held in Flagstaff, AZ June 2-3, 2005; and Oxygen in Earliest Solar System Materials and Processes (and including the outer planets and comets), held in Gatlinburg, TN September 19-22, 2005. As a consequence of the cross-cutting approach, the final book spans a wide range of fields relating to oxygen, from the stellar nucleosynthesis of oxygen, to its occurrence in the interstellar medium, to the oxidation and isotopic record preserved in 4.56 Ga grains formed at the Solar System's birth, to its abundance and speciation in planets large and small, to its role in the petrologic and physical evolution of the terrestrial planets. Contents: Introduction Oxygen isotopes in the early Solar System - A historical perspective Abundance, notation, and fractionation of light stable isotopes Nucleosynthesis and chemical evolution of oxygen Oxygen in the interstellar medium Oxygen in the Sun Redox conditions in the solar nebula: observational, experimental, and theoretical constraints Oxygen isotopes of chondritic components Mass-independent oxygen isotope variation in the solar nebula Oxygen and other volatiles in the giant planets and their satellites Oxygen in comets and interplanetary dust particles Oxygen and asteroids Oxygen isotopes in asteroidal materials Oxygen isotopic composition and chemical correlations in meteorites and the terrestrial planets Record of low-temperature alteration in asteroids The oxygen cycle of the terrestrial planets: insights into the processing and history of oxygen in surface environments Redox conditions on small bodies, the Moon and Mars Terrestrial oxygen isotope variations and their implications for planetary lithospheres Basalts as probes of planetary interior redox state Rheological consequences of redox state
Author: John Henry Poynting
Publisher:
ISBN:
Category : Solar radiation
Languages : en
Pages : 18
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Book Description
Author: A. Milani
Publisher: Springer Science & Business Media
ISBN: 9401111480
Category : Science
Languages : en
Pages : 531
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Book Description
THE MEETING The IAU Symposium 160 ASTEROIDS COMETS METEORS 1999 has been held at Villa Carlotta in Belgirate, on the shore of Lago Maggiore (Italy), from June 14 to June 18, 1993. It has been organized by the Astronomical Observatory of Torino and by the Lunar and Planetary Institute of Houston. It has been a very large meeting, with 323 registered participants from 38 countries. The scientific program included 29 invited reviews, 106 oral communications, and 215 posters. The subjects covered included all the aspects of the studies of the minor bodies of the solar system, including asteroids, comets, meteors, meteorites, interplanetary dust, with special focus on the interrelationships between these. The meeting was structured as follows. 5 morning plenary sessions have been devoted to invited reviews on: (1) search programs (2) populations of small bodies (3) dynamics (4) physical observations and modelling (5) origin and evolution. Two afternoon plenary sessions have been devoted to space missions to small bodies and to interrelationships between the different populations. The afternoon parallel sessions have been devoted to: dynamics of comets; Toutatis, Ida, Gaspra; physical processes in cometary comae and tails; meteorites; the cosmogonic message from cometary nuclei; physics of asteroids; the interplanetary dust complex; comet nuclei; meteors; composition and material properties of comets; dynamics of asteroids.
Author: Scott Bolton
Publisher: Springer
ISBN: 9789402415599
Category : Science
Languages : en
Pages : 644
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Book Description
The Juno mission to Jupiter is one of the most ambitious, daring and challenging solar system exploration missions ever conceived. Next to the Sun, Jupiter is the largest object in our solar system. As such, it is both a record and driver of the formation and evolution of the planets -- no other object in our solar system can tell us more about the origin of planetary systems. Understanding the details of giant planet formation, structure, composition and powerful magnetospheric environment required a new perspective close up and over the poles of Jupiter -- an orbit never before attempted. Juno was specifically designed for this challenge, entering into the harshest planetary environment known in the solar system. This volume describes the mission design, scientific strategies and instrument payload that enable Juno to peer deep into Jupiter’s atmosphere and reveal the fundamental process of the formation and early evolution of our solar system. In these papers, the Juno instrument teams describe their investigations, which include gravity radio science, microwave radiometers, magnetometers, an infrared imager auroral mapper, an ultraviolet imager and spectrograph, a visible light imager known as JunoCam, low and high energy particle detectors and plasma wave and radio electromagnetic sensors. The articles also describe a radiation monitoring experiment and the extensive laboratory measurements undertaken to assist with the analysis and interpretation of Juno’s pioneering investigation of Jupiter’s deep atmosphere. Originally published in Space Science Reviews, Volume 213, Issue 1-4, November 2017
