Planets Outside the Solar System

. Ed(s): Mariotti, Jean-Marie; Alloin, Danielle M.

ISBN 10: 0792357094 / ISBN 13: 9780792357094

Published by Kluwer Academic Publishers, 1999

About this Item

The observation and understanding of extra-solar planetary systems has become a topic that poses challenges to many fields of human knowledge. This book sets out a synthesis of the advances. It intends to help young students, researchers, engineers involved or about to become involved in quest for extra-solar planets. Editor(s): Mariotti, Jean-Marie; Alloin, Danielle M. Series: NATO Science Series C. Num Pages: 446 pages, index. BIC Classification: PGS; RBX. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly; (UU) Undergraduate. Dimension: 235 x 155. Weight in Grams: 688. . 1999. Paperback. . . . . Books ship from the US and Ireland.

Seller Inventory # V9780792357094

Bibliographic Details

• Title: Planets Outside the Solar System
• Publisher: Kluwer Academic Publishers
• Publication Date: 1999
• Language: English
• ISBN 10: 0792357094
• ISBN 13: 9780792357094
• Binding: Soft cover
• Condition: New

About this title

Synopsis

The question of the existence of other worlds and other living beings has been present in the human quest for knowledge since as far as Epicurus. For centuries this question belonged to the fields of philosophy and theology. The theoretical problem of the formation of the Solar System, and hence of other planetary systems, was tackled only during the 18th century, while the first observational attempts for a detection started less than one hundred years ago. Direct observation of an extra-solar planetary system is an extraordinarily difficult problem: extra-solar planets are at huge distances, are incredibly faint and are overwhelmed by the bright light of their own stars. With virtually no observational insight to test their models, theoreticians have remained for decades in a difficult position to make substantial progress. Yet, the field of stellar formation has provided since the 1980s both the the­ oretical and observational evidences for the formation of discs at the stage of star birth and for debris materials orbiting the very young stellar systems. It was tempting to consider that these left-overs might indeed later agglomerate into planetary systems more or less similar to ours. Then came observational evidences for planets outside the Solar System.