Frontispiece: Astronaut Harrison H. (Jack) Schmitt collecting samples from a boulder at Station 6 (base of the North Massif) on the north side of the Taurus-Littrow Valley, during the Apollo 17 mission. The front portion of the Lunar Roving Vehicle is visible at the left. The directional antenna (umbrella shape) is pointed toward Earth. (NASA Photo.) Lunar Science: A Po st-Apollo View Scientific Results and Insights from the Lunar Samples STUART ROSS TAYLOR Lunar Science Institute Houston, Texas, U.S.A. and Research School of Earth Sciences Australian National University Canberra, Australia PERGAMON PRESS INC. New York · Toronto · Oxford · Sydney · Braunschweig PERGAMON PRESS INC. Maxwell House, Fairview Park, Elmsford, N.Y. 10523 PERGAMON OF CANADA LTD. 207 Queen's Quay West, Toronto 117, Ontario PERGAMON PRESS LTD. Headington Hill Hall, Oxford PERGAMON PRESS (AUST.) PTY. LTD. Rushcutters Bay, Sydney, N.S.W. PERGAMON GmbH Burgplatz 1, Braunschweig Copyright © 1975, Pergamon Press Inc. Library of Congress Cataloging in Publication Data Taylor, Stuart Ross, 1925- Lunar science: a post-Apollo view. Includes bibliographical references. 1. Moon. I. Title. QB592.T38 1975 559.9Ί 74-17227 ISBN 0-08-018274-7 ISBN 0-08-018273-9 (pbk.) All Rights Reserved. No part of this publication may be reproduced, stored in a retrieval system or transmitted in any form, or by any means, electronic, mechanical, photocopying, recording or otherwise, without prior permission of Pergamon Press Inc. Cover picture: Fine detail visible on the lunar surface in this near terminator photo taken during the Apollo 16 mission. View looking south. East is to the left. The large crater with a central peak is Arzachel (97 km diameter) and the larger one in front of it is Alphonsus (116 km diameter). The smooth area to the right (west) is part of Mare Nubium. (NASA.) Back cover: Lick Observatory photo of 4 day old moon. Printed in the United States of America To Noël Susanna, Judith and Helen Preface The Apollo lunar landings represent one of the great triumphs of human imagination and ingenuity. Throughout recorded history the moon has been an object of admiration, longing, and interest. Man long ago realized the connection of the moon with the tides, and in many mystical and religious connotations the moon has had a profound effect on human affairs [1]. The cycle of the lunar month, the disappearance and rebirth of the moon, and the changing phases have been intimately associated with folklore and human intellectual development since our primitive beginnings [2]. We are children of the earth, with a beautiful silver ball, tantalizingly remote, to gaze at and wish for [3]. Now suddenly we have set our feet on the lunar surface and collected the samples; hurriedly at first, in awe of the harsh environment and unknown terrors [4], and then with growing confidence in our ability to survive the vacuum and the high temperatures, in extended missions, complete with vehicles. We have nearly 400 kilograms of rocks, a veritable feast of samples considering that much significant information may be gained from a few milligrams. Scientists have examined and analyzed the rocks and soils with every modern and sophisticated technique and have published the results in more than 30,000 pages of scientific literature. New and often unexpected data have appeared to confound old hypotheses. The resulting clarifica- tion of ideas and problems from the limited number of missions provides fresh support for old adages about the value of small amounts of data in constraining speculation. We now have a reasonably coherent picture of the history of events and processes occurring on the moon for more than xi xii Preface four billion years, a monument indeed to the ability of Homo sapiens to reconstruct the history of past events. Even in the more dimly understood events surrounding the formation of the moon and the earth, we have many more constraints to apply to the theories and a growing confidence that we have opened a new window to the early history of the solar system. Much of this knowledge, less than four years old, is not widely known or available to those outside the lunar investigation teams. A mass of data and the formidable jargon of science, often as impenetrable and baffling as a jungle thicket, surround the precious samples. Yet the observations tell an elegant story. The purpose of this book is to attempt to recount this story and to explain the scientific results and discoveries of the manned lunar missions as they are understood at present. Discussions with many colleagues have emphasized the need for such a work, although the formidable nature of the task is apparent. In an earlier book [5], a summary was given of the advances in knowledge resulting from the first manned landing of Apollo 11 in the Sea of Tranquillity. Now the landing of Apollo 17 (December, 1972) in the Taurus-Littrow valley has marked the close of the first phase of manned lunar landings. Much is known about the lunar samples, and it is appropriate to review and summarize the scientific findings of the Apollo Project. To those readers who may judge this attempt to be premature, I offer the opinions of Poincaré, quoted at the beginning of chapter 7. The previous work gave detailed descriptions of the mineralogy and chemistry of the Apollo 11 samples. It was possible to provide a general interpretation of the data, which in broad outline has changed surprisingly little with subsequent missions. In this book there is less emphasis on sample description and data. The vast amounts of data now available need an independent synthesis. Rather I have stressed the interpretative aspects of the study, with the aim of providing a coherent story of the evolution of the moon and its origin so far as we can judge it at present. The present work is thus a sequel to Moon Rocks and Minerals, not a revised edition. Such a task calls for much selection and evaluation. A vast body of data is already available, but a mere catalogue or data dump must be avoided. At the same time, a condensation of the literature without evaluation is not of much use. It is no service to the reader merely to record the existence of a controversy on a particular topic. The intent is to provide an understanding of the current state of knowledge about the moon as revealed by the lunar samples and the Apollo missions. Such a framework Preface xüi and guide will hopefully enable and encourage interested people to proceed to the more detailed lunar literature. With such a broad canvas, the selection and evaluation of the data necessarily reflect the knowledge, interest, and bias of the author. The approach recalls that of the historian as much as the scientist. As Bertrand Russell has remarked, "a book should be held together by its point of view," [6] and I make no apology for the selection or the interpretations made. These appear to me to be the most reasonable at this date and are offered in the spirit of scientific progress as elucidated by Karl Popper [7]. Many specialists may be chagrined to find that their work is dealt with only briefly or even perhaps omitted from this account. The effort to reduce 30,000 pages of published literature into a book involves a reduction by two orders of magnitude. Thus, each page here represents 100 in the original literature, so that many observations have had to be fitted into less space than that occupied by the typical abstract of a paper. Many questions are posed and discussed throughout the book. The moon (and Mars, as well) has provided many scientific surprises, salutary in reminding us both of the dangers of extrapolating from terrestrial experience and of the empirical and observational basis for science. The broad scope of the work has led me to many unfamiliar fields. I have been sustained in this endeavor both by the many workers [8] who have enlightened me about their specialities and by the observation that those previous writers who took a broad overview of lunar problems seem to have been more often correct than those who took a more circumscribed view [9]. The question of literature citation has proved difficult owing to the bulk of published material. It is impractical in this work to produce a full-scale bibliography, which would amount, in conventional referencing style, to well over 100 printed pages. Fortunately the information is contained at present in a relatively few major sources. Throughout the text, I have attempted to list references to all sources of information, statements of fact, opinion, and interpretation other than my own, so that the interested reader can pursue questions in the original literature. Rather than break up the text with names and dates, I have adopted the method commonly used by historians and some scientific journals of referencing by number. The numbered references are grouped at the end of each chapter. To conserve space, an abbreviated but adequate referencing style is employed [10]. Because of the predilection of the investigators to produce multi-author papers [11], it is not feasible to cite full bibliographic details. Except for two-author papers, first authors only are listed. I have tried in general to xiv Preface reference the latest relevant and informative paper in the field. This procedure has the advantage of reducing much repetitive referencing since citations of earlier works will be found in the later papers. It is a peculiarity of the lunar literature that references to ideas or data by an author may appear in several places, due to the widespread use of extended abstracts. Thus, much vital information about Apollo 17 first appeared in this form in the Transactions of the American Geophysical Union (EOS, Vol. 54, 580-622). Selection of references therefore be- comes an important consideration. Nearly all the work is of high quality, and citations to many excellent papers have had to be omitted because of space. Most of these can be found by consulting reference lists in the cited papers or the Proceedings of the Lunar Science Conferences. I have tried to avoid references to internal agency reports and other "gray" literature, not always success- fully. Publication deadlines have prevented formal referencing to the Fifth Lunar Science Conference Proceedings (1974), although the data and ideas discussed at that meeting (March, 1974) have been incorporated. References to the volume of extended abstracts (Lunar Science V, 1974) for that meeting are included. The literature coverage extends to April, 1974. Stuart Ross Taylor Houston, Texas April, 1974 REFERENCES AND NOTES 1. Among many curious correlations of lunar phases with biological rhythms, it may be noted that the average duration of human pregnancy is 266 days, close to the length of nine lunar synodical months* (265.8 days) and that the average duration of the human menstrual cycle is 29.5 days, compared with the average lunar synodical month of 29.53 days. Menaker, W., and Menaker, A. (1959) Lunar periodicity in human reproduction, Amer. Jour. Obstetrics Gynecology. 77:905, and Osley, M., et al. (1973) Ibid., 117:413. More sinister correlations, indicating a connection between lunar cycles and psychiat- ric disturbances (recalling the ancient association of the moon and lunacy) are described by Lieber, A. L., and Sherin, C. R. (1972) Amer. Jour. Psychiatry. 129: 69. 2. See, for example, Bedini, S. Α., et al. (1973) Moon, Abrams, N.Y. *A lunar synodical month, or lunation, is the time between successive new moons and is 29 days, 12 hours, and 44 minutes. This contrasts with the sidereal month, which is the average period of revolution of the moon around the earth, as determined by using a fixed star as reference point. The length of a sidereal month is 27 days, 7 hours, and 43 minutes. Preface xv 3. For a discussion on the political aspects of the manned landings, see Logsdon, J. M. (1970) The Decision to go to the Moon : Project Apollo and the National Interest, MIT Press, Cambridge. 4. For example, an often discussed possibility was that the highly reduced samples might ignite in the pure oxygen atmosphere of the landing module. 5. Levinson, Α. Α., and Taylor, S. R. (1971) Moon Rocks and Minerals, Pergamon Press, Elmsford, N.Y. 6. Russell, Bertrand (1967) Autobiography 1914-1944, Atlantic Monthly Press, pp. 340-341. 7. Popper, K. (1968) Conjectures and Refutations: The Growth of Scientific Knowledge, Harper & Row, N.Y. 8. See Acknowledgments. 9. The rationale for this statement will become apparent later in the book. The classic example is the correct interpretation of many lunar surface features by R. B. Baldwin (1949) in The Face of the Moon, University of Chicago Press. 10. See Appendix I. 11. One paper has 30 authors (NASA SP 315, p. 6-1, 1973), and there are many with ten or more. Authors should recall the adage that no committee ever wrote a symphony. The Author Stuart Ross Taylor Ph.D. (Indiana University) is a Professorial Fellow at the Research School of Earth Sciences, the Australian National Univer- sity, Canberra. His research interests have been in trace element geochemistry, analytical chemistry, tektites, continental composition and evolution, island arc volcanic rocks, and lunar studies. Dr. Taylor was a member of the Lunar Sample Preliminary Examination Team (LSPET) for Apollo 11 and 12 missions and carried out the first chemical analysis of a returned lunar sample. He is a Principal Investigator for the lunar sample program. His research publications total over 100 papers and books. He has held visiting posts at the University of California, San Diego, at the Max Planck Institut für Chemie, Mainz and at The Lunar Science Institute, Houston, Texas. He is an Associate Editor of the journal Geochimica et Cosmochimica Acta.