Author : Gorden Videen
Publisher : Springer Science & Business Media
Page : 346 pages
File Size : 21,72 MB
Release : 2002
Category : Mathematics
ISBN : 9781402008191
Focuses on the chemical and morphological properties of dust particles, both cosmological and terrestrial, and some of techniques used to gain information. This book treats such areas as observational information, dust morphology and chemistry, light-scattering models, characterisation methodologies, and backscatter polarisation and dynamics.
Author : Gorden Videen
Publisher : Springer Science & Business Media
Page : 333 pages
File Size : 47,10 MB
Release : 2012-12-06
Category : Science
ISBN : 9401006288
Optics of Cosmic Dust describes what we currently know about cosmic dust, how we know it, and the research efforts undertaken to provide that knowledge. Areas treated include observational information, dust morphology and chemistry, light-scattering models, characterisation methodologies, and backscatter polarisation and dynamics. Suitable as an introductory text, the book is also a reference guide for the advanced researcher.
Author : VOSHCHINNIKOV
Publisher :
Page : pages
File Size : 24,66 MB
Release : 2005-01-15
Category :
ISBN : 9780415287791
Author : Eberhard Grün
Publisher : Springer Science & Business Media
Page : 824 pages
File Size : 19,9 MB
Release : 2012-12-06
Category : Science
ISBN : 3642564283
An excellent handbook on the physics of interplanetary dust, a topic of interest not only to astronomers and space scientists but also to engineers. The following topics are covered in the book: historical perspectives; cometary dust; near-Earth environment; meteoroids and meteors; properties of interplanetary dust, information from collected samples; in situ measurements of cosmic dust; numerical modeling of the Zodiacal Cloud structure; synthesis of observations; instrumentation; physical processes; optical properties of interplanetary dust; orbital evolution of interplanetary dust; circumplanetary dust, observations and simple physics; interstellar dust and circumstellar dust disks. No doubt, the text will be regarded as the standard reference on interplanetary dust for many years to come.
Author : Endrik Krugel
Publisher : CRC Press
Page : 416 pages
File Size : 39,82 MB
Release : 2008
Category : Science
ISBN :
A concise reference, this book provides overview of interstellar dust and the interstellar medium. Emphasizing and explaining astronomical formulae, it addresses the absorption and scattering of dust, its creation in old stars, as well as emission, cohesion, and electrical charge. The book offers numerous figures displaying basic properties of dust such as optical constants, specific heat, and absorption and scattering coefficients. It introduces radiative transfer in a dusty medium and describes the use of transfer codes. With strong attention to detail, the author facilitates a complete understanding from which to build a more versatile application and manipulation of the information.
Author : A.M. Davis
Publisher : Elsevier
Page : 755 pages
File Size : 45,11 MB
Release : 2005-11-21
Category : Science
ISBN : 0080525350
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 : N. V. Voshchinnikov
Publisher : Astrophysics & Space Physics R
Page : 196 pages
File Size : 23,27 MB
Release : 2004
Category : Science
ISBN :
The optics of small particles are useful in the interpretation of observational phenomena related to extinction, scattering and emission of radiation by dust grains in space. This review presents three components of dust modelling: Optical constants; Light scattering theories and models. The author aims to show how the general laws of the optics of dust particleswork and to highlight the information about cosmic dust. Part II will be dedicated to the consideration of scattered radiation, dust absorption and emission, radiation pressure and dust properties.
Author : A. G. G. M. Tielens
Publisher : Cambridge University Press
Page : 520 pages
File Size : 49,46 MB
Release : 2005-08-25
Category : Science
ISBN : 9780521826341
Publisher Description
Author : David L. Block
Publisher : Springer Science & Business Media
Page : 890 pages
File Size : 23,95 MB
Release : 2013-04-17
Category : Science
ISBN : 1402028628
THE EDITORS: DAVID L. BLOCK AND KENNETH C. FREEMAN (SOC CO-CHAIRS), IVANIO PUERARI, ROBERT GROESS AND LIZ K. BLOCK 1. Harvard College Observatory, 1958 The past century has truly brought about an explosive period of growth and discovery for the physical sciences as a whole, and for astronomy in particular. Galaxy morphology has reached a renaissance . . The year: 1958. The date: October 1. The venue: Harvard College Observatory. The lecturer: Walter Baade. With amazing foresight, Baade penned these words: "Young stars, supergiants and so on, make a terrific splash - lots of light. The total mass of these can be very small compared to the total mass of the system". Dr Layzer then asked the key question: " . . . the discussion raises the point of what this classification would look like if you were to ignore completely all the Population I, and just focus attention on the Population II . . . " We stand on the shoulders of giants. The great observer E. E. Barnard, in his pioneering efforts to photograph the Milky Way, devoted the major part of his life to identifying and numbering dusty "holes" and dust lanes in our Milky Way. No one could have dreamt that the pervasiveness of these cosmic dust masks (not only in our Galaxy but also in galaxies at high redshift) is so great, that their "penetration" is truly one of the pioneering challenges from both space-borne telescopes and from the ground.
Author : David A Williams
Publisher : Royal Society of Chemistry
Page : 320 pages
File Size : 25,74 MB
Release : 2015-11-18
Category : Science
ISBN : 1782623698
It has been firmly established over the last quarter century that cosmic dust plays important roles in astrochemistry. The consequences of these roles affect the formation of planets, stars and even galaxies. Cosmic dust has been a controversial topic but there is now a considerable measure of agreement as to its nature and roles in astronomy, and its initiation of astrobiology. The subject has stimulated an enormous research effort, with researchers in many countries now involved in laboratory research and in ab initio computations. This is the first book devoted to a study of the chemistry of cosmic dust, presenting current thinking on the subject distilled from many publications in surface and solid-state science, and in astronomy. The authors discuss the nature of dust, its formation and evolution, the chemistry it can promote on its surfaces, and the consequences of these functions. The purpose of this book is to review current understanding and to indicate where future work is required. Mainly intended for researchers in the field of astrochemistry, the book could also be used as the basis of a course for postgraduate students who have an interest in astrochemistry.
