Formation, Evolution, and Dynamics of Young Solar Systems
This book's interdisciplinary scope aims at bridging various communities: 1) cosmochemists, who study meteoritic samples from our own solar system, 2) (sub-) millimetre astronomers, who measure the distribution of dust and gas of star-forming regions and
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Martin Pessah Oliver Gressel Editors
Formation, Evolution, and Dynamics of Young Solar Systems
Formation, Evolution, and Dynamics of Young Solar Systems
Astrophysics and Space Science Library EDITORIAL BOARD Chairman W. B. BURTON, National Radio Astronomy Observatory, Charlottesville, Virginia, U.S.A. ([email protected]); University of Leiden, The Netherlands ([email protected]) F. BERTOLA, University of Padua, Italy C. J. CESARSKY, Commission for Atomic Energy, Saclay, France P. EHRENFREUND, Leiden University, The Netherlands O. ENGVOLD, University of Oslo, Norway E. P. J. VAN DEN HEUVEL, University of Amsterdam, The Netherlands V. M. KASPI, McGill University, Montreal, Canada J. M. E. KUIJPERS, University of Nijmegen, The Netherlands H. VAN DER LAAN, University of Utrecht, The Netherlands P. G. MURDIN, Institute of Astronomy, Cambridge, UK B. V. SOMOV, Astronomical Institute, Moscow State University, Russia R. A. SUNYAEV, Max Planck Institute for Astrophysics, Garching, Germany
More information about this series at http://www.springer.com/series/5664
Martin Pessah • Oliver Gressel Editors
Formation, Evolution, and Dynamics of Young Solar Systems
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Editors Martin Pessah Niels Bohr International Academy The Niels Bohr Institute Copenhagen, Denmark
Oliver Gressel Niels Bohr International Academy The Niels Bohr Institute Copenhagen, Denmark
ISSN 0067-0057 ISSN 2214-7985 (electronic) Astrophysics and Space Science Library ISBN 978-3-319-60608-8 ISBN 978-3-319-60609-5 (eBook) DOI 10.1007/978-3-319-60609-5 Library of Congress Control Number: 2017955963 © Springer International Publishing AG 2017 The chapters ‘Chondrules: Ubiquitous Chondritic Solids Tracking the Evolution of the Solar Protoplanetary Disk’, ‘Dust Coagulation with Porosity Evolution’ and ‘The Emerging Paradigm of Pebble Accretion’ are licensed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/). For further details see license information in the chapters. This work is subject to copyright. All rights are reserved by the Publisher, whether the whole or part of the material is concerned, specifically the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfilms or in any other physical way, and transmission or information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed. The use of general descriptive names, registered names, trademarks, service marks, etc. in this publication does not imply, even in the absence of a specific statement, that such names are exempt from the relevant protective laws and regulations and therefore free for general use. The publisher, the authors and the editors are safe to assume that the advice and information in this book are believed to be true and accurate at the date of publication. Neither the publisher nor the authors or the editors give a warranty, express or implied, with respect to the
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