How Did The Solar System Form


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The Formation of the Solar System


The Formation of the Solar System

Author: M. M. Woolfson

language: en

Publisher: World Scientific

Release Date: 2007


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This book traces the development of ideas about the origin of the Solar System from ancient times to the present day. A survey of more modern ideas, covering the last 200 years or so, highlights the difficulties experienced by theories and also points the way towards the development of a more successful theory. In particular, the current ?standard model? ? the Solar Nebula Theory ? is examined and discussed in some detail. After more than thirty years of development, this theory has still not settled down into an agreed form, as it experiences both theoretical difficulties and problems with reconciling new observations. By contrast, the Capture Theory, developed over the last forty years by the author, and supported by recent observations provides a complete description of the formation of the Solar System, including an evolutionary hypothesis that explains the detailed structure of the system. Written in an informative yet accessible manner, this book will appeal to both specialist and non-specialist readers alike.

A Question and Answer Guide to Astronomy


A Question and Answer Guide to Astronomy

Author: Pierre-Yves Bely

language: en

Publisher: Cambridge University Press

Release Date: 2010-03-11


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A practical answer guide to humankind's age-old questions on planets, our universe and everything beyond and between.

The Structure of the Sun


The Structure of the Sun

Author: T. Roca Cortes

language: en

Publisher: Cambridge University Press

Release Date: 1996-08-28


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The complex internal structure of the Sun can now be studied in detail through helioseismology and neutrino astronomy. The VI Canary Islands Winter School of Astrophysics was dedicated to examining these powerful new techniques. Based on this meeting, eight specially-written chapters by world-experts are presented in this timely volume. We are shown how the internal composition and dynamical structure of the Sun can be deduced through helioseismology; and how the central temperature can be determined from the flux of solar neutrinos. This volume provides an excellent introduction for graduate students and an up-to-date overview for researchers working on the Sun, neutrino astronomy and helio- and asteroseismology.